id float64 706 1.8k | title stringlengths 1 343 | abstract stringlengths 6 6.09k | categories stringlengths 5 125 | processed_abstract stringlengths 2 5.96k | tokenized_abstract stringlengths 8 8.74k | centroid stringlengths 2.1k 2.17k |
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1,801.09669 | Super-maximal chaos and instability | An upper bound on Lyapunov exponent of a thermal many body quantum system has
been conjectured recently. In this work, we attempt to achieve a physical
understanding of what prevents a system from violating this bound. To this end,
we propose - super-maximal chaos leads to instability. Our proposal is
supported by fi... | hep-th cond-mat.str-el | an upper bound on lyapunov exponent of a thermal many body quantum system has been conjectured recently in this work we attempt to achieve a physical understanding of what prevents a system from violating this bound to this end we propose supermaximal chaos leads to instability our proposal is supported by findings in ... | [['an', 'upper', 'bound', 'on', 'lyapunov', 'exponent', 'of', 'a', 'thermal', 'many', 'body', 'quantum', 'system', 'has', 'been', 'conjectured', 'recently', 'in', 'this', 'work', 'we', 'attempt', 'to', 'achieve', 'a', 'physical', 'understanding', 'of', 'what', 'prevents', 'a', 'system', 'from', 'violating', 'this', 'bo... | [-0.19178062347938943, 0.22240846303509762, -0.1407629798175158, -0.025748739482521592, -0.054955087746297676, -0.18791821681258974, 0.10684968091908703, 0.3047055415373957, -0.24482378478066247, -0.25578386278248555, 0.060529629940332445, -0.2522948306776305, -0.20440889399707596, 0.17879831512180097, -0.0516140535125... |
1,801.0967 | Kron 3: a fourth intermediate age cluster in the SMC with evidence of
multiple populations | We present the results of a spectroscopic study of the intermediate age
(approximately 6.5 Gyr) massive cluster Kron 3 in the Small Magellanic Cloud.
We measure CN and CH band strengths (at 3839 and 4300 Angstroms respectively)
using VLT FORS2 spectra of 16 cluster members and find a sub-population of 5
stars enriche... | astro-ph.GA | we present the results of a spectroscopic study of the intermediate age approximately 65 gyr massive cluster kron 3 in the small magellanic cloud we measure cn and ch band strengths at 3839 and 4300 angstroms respectively using vlt fors2 spectra of 16 cluster members and find a subpopulation of 5 stars enriched in nitr... | [['we', 'present', 'the', 'results', 'of', 'a', 'spectroscopic', 'study', 'of', 'the', 'intermediate', 'age', 'approximately', '65', 'gyr', 'massive', 'cluster', 'kron', '3', 'in', 'the', 'small', 'magellanic', 'cloud', 'we', 'measure', 'cn', 'and', 'ch', 'band', 'strengths', 'at', '3839', 'and', '4300', 'angstroms', '... | [-0.07099408781962535, 0.13622927916460736, -0.07591928583569825, 0.09183129804192244, -0.020963964361414712, -0.09420109431126288, 0.11403362401927422, 0.440704065713466, -0.16117601391368744, -0.39931506271074924, 0.03337081546404599, -0.2700371624976729, -0.007620673738087395, 0.1493731053546071, -0.0174614420935021... |
1,801.09671 | Reconstructing particle masses in events with displaced vertices | We propose a simple way to extract particle masses given a displaced vertex
signature in event topologies where two long-lived mother particles decay to
visible particles and an invisible daughter. The mother could be either charged
or neutral and the neutral daughter could correspond to a dark matter particle
in dif... | hep-ph hep-ex | we propose a simple way to extract particle masses given a displaced vertex signature in event topologies where two longlived mother particles decay to visible particles and an invisible daughter the mother could be either charged or neutral and the neutral daughter could correspond to a dark matter particle in differe... | [['we', 'propose', 'a', 'simple', 'way', 'to', 'extract', 'particle', 'masses', 'given', 'a', 'displaced', 'vertex', 'signature', 'in', 'event', 'topologies', 'where', 'two', 'longlived', 'mother', 'particles', 'decay', 'to', 'visible', 'particles', 'and', 'an', 'invisible', 'daughter', 'the', 'mother', 'could', 'be', ... | [-0.04142400916246134, 0.2637865952567682, -0.1328654820662773, 0.10897478778497316, -0.07154247570489984, -0.1402364346900985, -0.013650254481622288, 0.31995040200079883, -0.24898189844022836, -0.3215881013011019, 0.018628531124352688, -0.3127793207383929, -0.00683379273358432, 0.10733175939962929, 0.04275468812744704... |
1,801.09672 | Denoising Arterial Spin Labeling Cerebral Blood Flow Images Using Deep
Learning | Arterial spin labeling perfusion MRI is a noninvasive technique for measuring
quantitative cerebral blood flow (CBF), but the measurement is subject to a low
signal-to-noise-ratio(SNR). Various post-processing methods have been proposed
to denoise ASL MRI but only provide moderate improvement. Deep learning (DL) is
a... | cs.CV | arterial spin labeling perfusion mri is a noninvasive technique for measuring quantitative cerebral blood flow cbf but the measurement is subject to a low signaltonoiseratiosnr various postprocessing methods have been proposed to denoise asl mri but only provide moderate improvement deep learning dl is an emerging tech... | [['arterial', 'spin', 'labeling', 'perfusion', 'mri', 'is', 'a', 'noninvasive', 'technique', 'for', 'measuring', 'quantitative', 'cerebral', 'blood', 'flow', 'cbf', 'but', 'the', 'measurement', 'is', 'subject', 'to', 'a', 'low', 'signaltonoiseratiosnr', 'various', 'postprocessing', 'methods', 'have', 'been', 'proposed'... | [-0.0205791187906937, 0.006499654278741218, -0.06513575054620696, 0.09439091436767594, -0.1197529571538627, -0.14333892464541245, -0.004394065942180975, 0.39815667521575265, -0.26222007493958976, -0.3567729987556337, 0.09689650317796367, -0.243637236570481, -0.1484226391028246, 0.2181689840967048, -0.12699260330430853,... |
1,801.09673 | Indistinguishable binomial decision tree of 3-SAT: Proof of class P is a
proper subset of class NP | This paper solves a long standing open problem of whether NP-complete
problems could be solved in polynomial time on a deterministic Turing machine
by showing that the indistinguishable binomial decision tree can be formed in a
3-SAT instance. This paper describes how to construct the decision tree and
explains why 3... | cs.CC math.LO | this paper solves a long standing open problem of whether npcomplete problems could be solved in polynomial time on a deterministic turing machine by showing that the indistinguishable binomial decision tree can be formed in a 3sat instance this paper describes how to construct the decision tree and explains why 3sat h... | [['this', 'paper', 'solves', 'a', 'long', 'standing', 'open', 'problem', 'of', 'whether', 'npcomplete', 'problems', 'could', 'be', 'solved', 'in', 'polynomial', 'time', 'on', 'a', 'deterministic', 'turing', 'machine', 'by', 'showing', 'that', 'the', 'indistinguishable', 'binomial', 'decision', 'tree', 'can', 'be', 'for... | [-0.12797675259377897, 0.181061117318174, -0.07723931529549287, 0.06993159880933471, -0.1162591948783263, -0.19723773399675068, 0.11040094596311509, 0.34831302984558205, -0.3662329818558027, -0.2727457881617816, 0.049984756928368256, -0.2718728182297398, -0.10445924558270564, 0.1684227464336684, -0.08537614600054245, 0... |
1,801.09674 | Modeling of flow generated sound in a constricted duct at low Mach
number flow | Modelling flow and acoustics in a constricted duct at low Mach numbers is
important for investigating many physiological phenomena such as phonation,
generation of arterial murmurs, and pulmonary conditions involving airway
obstruction. The objective of this study is to validate computational fluid
dynamics (CFD) and... | physics.flu-dyn | modelling flow and acoustics in a constricted duct at low mach numbers is important for investigating many physiological phenomena such as phonation generation of arterial murmurs and pulmonary conditions involving airway obstruction the objective of this study is to validate computational fluid dynamics cfd and comput... | [['modelling', 'flow', 'and', 'acoustics', 'in', 'a', 'constricted', 'duct', 'at', 'low', 'mach', 'numbers', 'is', 'important', 'for', 'investigating', 'many', 'physiological', 'phenomena', 'such', 'as', 'phonation', 'generation', 'of', 'arterial', 'murmurs', 'and', 'pulmonary', 'conditions', 'involving', 'airway', 'ob... | [-0.11765842859704907, 0.12728516858585767, -0.09237211322678661, 0.06070563218215582, -0.055517119040659924, -0.10350809861653247, -0.08137905335445937, 0.3259166554973917, -0.2432887550303901, -0.345017051904911, 0.06909296148021137, -0.27012232005565995, -0.09458105493174783, 0.2436969358717216, -0.03601189039535406... |
1,801.09675 | Equation of State Dependence of Nonlinear Mode-tide Coupling in
Coalescing Binary Neutron Stars | Recently, an instability due to the nonlinear coupling of p-modes to g-modes
in tidally deformed neutron stars in coalescing binaries has been studied in
some detail. The result is significant because it could influence the inspiral
and leave an imprint on the gravitational wave signal that depends on the
neutron sta... | astro-ph.HE gr-qc | recently an instability due to the nonlinear coupling of pmodes to gmodes in tidally deformed neutron stars in coalescing binaries has been studied in some detail the result is significant because it could influence the inspiral and leave an imprint on the gravitational wave signal that depends on the neutron star equa... | [['recently', 'an', 'instability', 'due', 'to', 'the', 'nonlinear', 'coupling', 'of', 'pmodes', 'to', 'gmodes', 'in', 'tidally', 'deformed', 'neutron', 'stars', 'in', 'coalescing', 'binaries', 'has', 'been', 'studied', 'in', 'some', 'detail', 'the', 'result', 'is', 'significant', 'because', 'it', 'could', 'influence', ... | [-0.13803881250059288, 0.1842191653719248, -0.11029290886275832, 0.08670019468862875, -0.1448573727993549, -0.040664869285494266, 0.03725395679816456, 0.3308051077255134, -0.1957477528872666, -0.28823931666095187, 0.102148791574073, -0.25857500333158456, -0.10508201812037024, 0.21579353691649003, 0.006544650526151127, ... |
1,801.09676 | Temperature-Dependence of the Solid-Electrolyte Interphase
Overpotential: Part I. Two Parallel Mechanisms, One Phase Transition | It has been shown recently that the overpotential originating from ionic
conduction of alkali-ions through the inner dense solid-electrolyte interphase
(SEI) is strongly non-linear. An empirical equation was proposed to merge the
measured resistances from both galvanostatic cycling (GS) and electrochemical
impedance ... | physics.app-ph cond-mat.mtrl-sci physics.chem-ph | it has been shown recently that the overpotential originating from ionic conduction of alkaliions through the inner dense solidelectrolyte interphase sei is strongly nonlinear an empirical equation was proposed to merge the measured resistances from both galvanostatic cycling gs and electrochemical impedance spectrosco... | [['it', 'has', 'been', 'shown', 'recently', 'that', 'the', 'overpotential', 'originating', 'from', 'ionic', 'conduction', 'of', 'alkaliions', 'through', 'the', 'inner', 'dense', 'solidelectrolyte', 'interphase', 'sei', 'is', 'strongly', 'nonlinear', 'an', 'empirical', 'equation', 'was', 'proposed', 'to', 'merge', 'the'... | [-0.06321385949436645, 0.18614728788027343, 0.016437358892697918, -0.03506795477957648, 0.040642410224068594, -0.213385069366353, 0.09862028391788079, 0.38805147164466436, -0.22806240227203992, -0.30402238316242103, 0.036380460099374255, -0.3344166331454485, -0.049593571893366, 0.22450496710262427, 0.007085896120243488... |
1,801.09677 | Anapole mode excitation in novel perforated all-dielectric metamaterials | In this paper, we concern on nonradiating properties of novel silicon
metamaterials due to multipolar interaction. Destructive interference of
electric dipole moment and the next term of multipolar decomposition - toroidal
dipole moment, leads to nonradiating anapole mode, which is nowadays widely
studying among elec... | physics.app-ph cond-mat.mtrl-sci | in this paper we concern on nonradiating properties of novel silicon metamaterials due to multipolar interaction destructive interference of electric dipole moment and the next term of multipolar decomposition toroidal dipole moment leads to nonradiating anapole mode which is nowadays widely studying among electrodynam... | [['in', 'this', 'paper', 'we', 'concern', 'on', 'nonradiating', 'properties', 'of', 'novel', 'silicon', 'metamaterials', 'due', 'to', 'multipolar', 'interaction', 'destructive', 'interference', 'of', 'electric', 'dipole', 'moment', 'and', 'the', 'next', 'term', 'of', 'multipolar', 'decomposition', 'toroidal', 'dipole',... | [-0.17472294542398073, 0.15243513480886633, -0.013031986645526357, 0.024388820958398512, -0.21685273119788848, -0.15341396620612086, -0.022819981365579604, 0.4220406294190957, -0.24645601518999752, -0.3008207828266385, -0.026545606291979367, -0.24100792527566722, -0.2416804225448473, 0.1949770349641273, -0.061339563034... |
1,801.09678 | Algorithms for the Construction of Incoherent Frames Under Various
Design Constraints | Unit norm finite frames are generalizations of orthonormal bases with many
applications in signal processing. An important property of a frame is its
coherence, a measure of how close any two vectors of the frame are to each
other. Low coherence frames are useful in compressed sensing applications. When
used as measu... | eess.SP cs.IT math.IT | unit norm finite frames are generalizations of orthonormal bases with many applications in signal processing an important property of a frame is its coherence a measure of how close any two vectors of the frame are to each other low coherence frames are useful in compressed sensing applications when used as measurement... | [['unit', 'norm', 'finite', 'frames', 'are', 'generalizations', 'of', 'orthonormal', 'bases', 'with', 'many', 'applications', 'in', 'signal', 'processing', 'an', 'important', 'property', 'of', 'a', 'frame', 'is', 'its', 'coherence', 'a', 'measure', 'of', 'how', 'close', 'any', 'two', 'vectors', 'of', 'the', 'frame', 'a... | [-0.09746110013802536, 0.0812919019875153, -0.017366124970249076, 0.04245660485976259, -0.07988043654768262, -0.16468635231503867, -0.0240499888008344, 0.4284243665810209, -0.3384984691161662, -0.24007586617371998, 0.17014076731356909, -0.2724834960419685, -0.17414464371395297, 0.20480693004792555, -0.09987152292742393... |
1,801.09679 | The Lyapunov dimension, convergency and entropy for a dynamical model of
Chua memristor circuit | For the study of chaotic dynamics and dimension of attractors the concepts of
the Lyapunov exponents was found useful and became widely spread. Such
characteristics of chaotic behavior, as the Lyapunov dimension and the entropy
rate, can be estimated via the Lyapunov exponents. In this work an analytical
approach to ... | math.DS nlin.CD | for the study of chaotic dynamics and dimension of attractors the concepts of the lyapunov exponents was found useful and became widely spread such characteristics of chaotic behavior as the lyapunov dimension and the entropy rate can be estimated via the lyapunov exponents in this work an analytical approach to the st... | [['for', 'the', 'study', 'of', 'chaotic', 'dynamics', 'and', 'dimension', 'of', 'attractors', 'the', 'concepts', 'of', 'the', 'lyapunov', 'exponents', 'was', 'found', 'useful', 'and', 'became', 'widely', 'spread', 'such', 'characteristics', 'of', 'chaotic', 'behavior', 'as', 'the', 'lyapunov', 'dimension', 'and', 'the'... | [-0.1551683906033851, 0.11433745202109845, -0.14056825208599152, 0.09115627099611405, 0.037848201425125204, -0.16742071614809928, 0.0015330320507611918, 0.23115081631956433, -0.2818012980379812, -0.20494111689428487, 0.1393908128881341, -0.2647999342584956, -0.26518988987241965, 0.2699607805841589, -0.03205528334997918... |
1,801.0968 | On the spatial distributions of dense cores in Orion B | We quantify the spatial distributions of dense cores in three spatially
distinct areas of the Orion B star-forming region. For L1622, NGC2068/NGC2071
and NGC2023/NGC2024 we measure the amount of spatial substructure using the
$\mathcal{Q}$-parameter and find all three regions to be spatially
substructured ($\mathcal{... | astro-ph.GA astro-ph.SR | we quantify the spatial distributions of dense cores in three spatially distinct areas of the orion b starforming region for l1622 ngc2068ngc2071 and ngc2023ngc2024 we measure the amount of spatial substructure using the mathcalqparameter and find all three regions to be spatially substructured mathcalq 08 we quantify ... | [['we', 'quantify', 'the', 'spatial', 'distributions', 'of', 'dense', 'cores', 'in', 'three', 'spatially', 'distinct', 'areas', 'of', 'the', 'orion', 'b', 'starforming', 'region', 'for', 'l1622', 'ngc2068ngc2071', 'and', 'ngc2023ngc2024', 'we', 'measure', 'the', 'amount', 'of', 'spatial', 'substructure', 'using', 'the'... | [-0.09839695258530404, 0.1829330020236893, -0.03915051106721331, 0.099759387678472, 0.001420011300604138, -0.038144465807514884, 0.00195926472039546, 0.38068325249320367, -0.14804632898346431, -0.353373420377404, 0.06384929485676948, -0.25862229572303885, -0.04962846685574511, 0.11315946506782261, -0.001765349747167142... |
1,801.09681 | A collapsar model with disk wind: Implications for supernovae associated
with Gamma-Ray Bursts | We construct a simple but self-consistent collapsar model for gamma-ray
bursts (GRBs) and SNe associated with GRBs (GRB-SNe).Our model includes a black
hole, an accretion disk, and the envelope surrounding the central system.The
evolutions of the different components are connected by the transfer of the
mass and angu... | astro-ph.HE | we construct a simple but selfconsistent collapsar model for gammaray bursts grbs and sne associated with grbs grbsneour model includes a black hole an accretion disk and the envelope surrounding the central systemthe evolutions of the different components are connected by the transfer of the mass and angular momentumt... | [['we', 'construct', 'a', 'simple', 'but', 'selfconsistent', 'collapsar', 'model', 'for', 'gammaray', 'bursts', 'grbs', 'and', 'sne', 'associated', 'with', 'grbs', 'grbsneour', 'model', 'includes', 'a', 'black', 'hole', 'an', 'accretion', 'disk', 'and', 'the', 'envelope', 'surrounding', 'the', 'central', 'systemthe', '... | [-0.09178853891605493, 0.14187161829894568, -0.06855722813000258, 0.1584005237488989, -0.11363735690593056, -0.0740647351825702, 0.016451721296917722, 0.4074757111046721, -0.23444044267491318, -0.3040865960226643, 0.07109444678385309, -0.2602956785848088, -0.01101393549297337, 0.22408532998570713, -0.022693096255505512... |
1,801.09682 | The impact of baryonic discs on the shapes and profiles of
self-interacting dark matter halos | We employ isolated N-body simulations to study the response of
self-interacting dark matter (SIDM) halos in the presence of the baryonic
potentials. Dark matter self-interactions lead to kinematic thermalization in
the inner halo, resulting in a tight correlation between the dark matter and
baryon distributions. A de... | astro-ph.GA | we employ isolated nbody simulations to study the response of selfinteracting dark matter sidm halos in the presence of the baryonic potentials dark matter selfinteractions lead to kinematic thermalization in the inner halo resulting in a tight correlation between the dark matter and baryon distributions a deep baryoni... | [['we', 'employ', 'isolated', 'nbody', 'simulations', 'to', 'study', 'the', 'response', 'of', 'selfinteracting', 'dark', 'matter', 'sidm', 'halos', 'in', 'the', 'presence', 'of', 'the', 'baryonic', 'potentials', 'dark', 'matter', 'selfinteractions', 'lead', 'to', 'kinematic', 'thermalization', 'in', 'the', 'inner', 'ha... | [-0.08794543342050778, 0.11915991183667467, -0.18356623211338258, 0.14307660750525358, -0.12310704103271876, -0.010475504073918193, -0.04615481961697627, 0.3372697931315218, -0.1892593345082887, -0.37557482870889236, -0.04473749861622659, -0.26565059078959646, -0.03723224409047391, 0.1250028506005797, 0.062693413116094... |
1,801.09683 | High-energy gamma-ray and neutrino production in star-forming galaxies
across cosmic time: Difficulties in explaining the IceCube data | We present a new theoretical modeling to predict luminosity and spectrum of
gamma-ray and neutrino emission of a star-forming galaxy, from star formation
rate ($\psi$), gas mass ($M_{\rm gas}$), stellar mass, and disk size, taking
into account production, propagation and interactions of cosmic rays. The model
reprodu... | astro-ph.HE | we present a new theoretical modeling to predict luminosity and spectrum of gammaray and neutrino emission of a starforming galaxy from star formation rate psi gas mass m_rm gas stellar mass and disk size taking into account production propagation and interactions of cosmic rays the model reproduces the observed gammar... | [['we', 'present', 'a', 'new', 'theoretical', 'modeling', 'to', 'predict', 'luminosity', 'and', 'spectrum', 'of', 'gammaray', 'and', 'neutrino', 'emission', 'of', 'a', 'starforming', 'galaxy', 'from', 'star', 'formation', 'rate', 'psi', 'gas', 'mass', 'm_rm', 'gas', 'stellar', 'mass', 'and', 'disk', 'size', 'taking', '... | [-0.005527866821702024, 0.1362906070795938, -0.04653178807830711, 0.21898990768269158, -0.09494591658003629, -0.0770184991835821, 0.018629037078878866, 0.4232797987940835, -0.0992026683658634, -0.3786159254565108, -0.05201406921203271, -0.31600351366903007, 0.022575685365988713, 0.24226154384384976, 0.04504459039648859... |
1,801.09684 | Latent Space Purification via Neural Density Operators | Machine learning is actively being explored for its potential to design,
validate, and even hybridize with near-term quantum devices. A central question
is whether neural networks can provide a tractable representation of a given
quantum state of interest. When true, stochastic neural networks can be
employed for man... | quant-ph | machine learning is actively being explored for its potential to design validate and even hybridize with nearterm quantum devices a central question is whether neural networks can provide a tractable representation of a given quantum state of interest when true stochastic neural networks can be employed for many unsupe... | [['machine', 'learning', 'is', 'actively', 'being', 'explored', 'for', 'its', 'potential', 'to', 'design', 'validate', 'and', 'even', 'hybridize', 'with', 'nearterm', 'quantum', 'devices', 'a', 'central', 'question', 'is', 'whether', 'neural', 'networks', 'can', 'provide', 'a', 'tractable', 'representation', 'of', 'a',... | [-0.04705383283804164, 0.1373117626111471, -0.07256690419513646, 0.07751010644750826, -0.08296531177737274, -0.23726722178625242, 0.042571779848822884, 0.42688620079109685, -0.286503947339952, -0.2688558492525161, 0.09844544599141983, -0.23167707685039926, -0.15754498781650575, 0.21902821956998633, -0.06692512786257586... |
1,801.09685 | A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). II.
Constraining the quenching time in the stripped galaxy NGC 4330 | The Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a
blind narrow-band H$\alpha$+[NII] imaging survey carried out with MegaCam at
the CFHT. During pilot observations we have observed NGC 4330, an intermediate
mass, edge-on star forming spiral currently falling into the core of the Virgo
cluster.... | astro-ph.GA | the virgo environmental survey tracing ionised gas emission vestige is a blind narrowband halphanii imaging survey carried out with megacam at the cfht during pilot observations we have observed ngc 4330 an intermediate mass edgeon star forming spiral currently falling into the core of the virgo cluster new deep observ... | [['the', 'virgo', 'environmental', 'survey', 'tracing', 'ionised', 'gas', 'emission', 'vestige', 'is', 'a', 'blind', 'narrowband', 'halphanii', 'imaging', 'survey', 'carried', 'out', 'with', 'megacam', 'at', 'the', 'cfht', 'during', 'pilot', 'observations', 'we', 'have', 'observed', 'ngc', '4330', 'an', 'intermediate',... | [-0.05854365648780446, 0.08033526747070986, -0.12214987689524581, 0.0708135178629655, -0.08127743333917917, -0.05159584607532157, 0.009781961220731909, 0.45905804033768743, -0.18334873274471722, -0.33063280868589423, 0.0809880010331383, -0.29064231689443587, -0.022053726568874728, 0.19322088246888205, 0.010099821876596... |
1,801.09686 | Origins of ultra-diffuse galaxies in the Coma cluster - I. Constraints
from velocity phase-space | We use Keck/DEIMOS spectroscopy to confirm the cluster membership of 16
ultra-diffuse galaxies (UDGs) in the Coma cluster, bringing the total number of
spectroscopically con- firmed UDGs to 24. We also identify a new cluster
background UDG. In this pilot study of Coma UDGs in velocity phase-space, we
find evidence th... | astro-ph.GA | we use keckdeimos spectroscopy to confirm the cluster membership of 16 ultradiffuse galaxies udgs in the coma cluster bringing the total number of spectroscopically con firmed udgs to 24 we also identify a new cluster background udg in this pilot study of coma udgs in velocity phasespace we find evidence that most pres... | [['we', 'use', 'keckdeimos', 'spectroscopy', 'to', 'confirm', 'the', 'cluster', 'membership', 'of', '16', 'ultradiffuse', 'galaxies', 'udgs', 'in', 'the', 'coma', 'cluster', 'bringing', 'the', 'total', 'number', 'of', 'spectroscopically', 'con', 'firmed', 'udgs', 'to', '24', 'we', 'also', 'identify', 'a', 'new', 'clust... | [-0.040243489338050345, 0.10633672120538396, -0.1521028598180469, 0.0905408414155939, -0.09845641050603449, 0.005684362293469795, 0.03911501417364578, 0.45419320110115946, -0.1186266909910204, -0.3688139202107924, 0.02251187002616038, -0.2726681053129412, -0.0247805828853331, 0.1637916389262732, -0.056535099377758136, ... |
1,801.09687 | On the Interpretation of Thermal Conductance of the nu=5/2 Edge | Recent experiments [Banerjee et al, arXiv:1710.00492] have measured thermal
conductance of the nu=5/2 edge in a GaAs electron gas and found it to be
quantized as K \approx 5/2 (in appropriate dimensionless units). This result is
unexpected, as prior numerical work predicts that the nu=5/2 state should be
the Anti-Pfa... | cond-mat.mes-hall | recent experiments banerjee et al arxiv171000492 have measured thermal conductance of the nu52 edge in a gaas electron gas and found it to be quantized as k approx 52 in appropriate dimensionless units this result is unexpected as prior numerical work predicts that the nu52 state should be the antipfaffian phase of mat... | [['recent', 'experiments', 'banerjee', 'et', 'al', 'arxiv171000492', 'have', 'measured', 'thermal', 'conductance', 'of', 'the', 'nu52', 'edge', 'in', 'a', 'gaas', 'electron', 'gas', 'and', 'found', 'it', 'to', 'be', 'quantized', 'as', 'k', 'approx', '52', 'in', 'appropriate', 'dimensionless', 'units', 'this', 'result',... | [-0.1239495953622074, 0.21922734348724285, -0.10631347089809806, 0.03463381970313525, -0.07535762086576014, -0.1823831358311796, 0.06733445581732922, 0.32379615689186675, -0.24255760935984813, -0.31589146722271516, 0.06611583011608832, -0.2663002693126991, -0.15317201413333686, 0.12056254525260444, -0.05741615355496801... |
1,801.09688 | UV SEDs of early-type cluster galaxies: A new look at the UV upturn | Using GALEX, UVOT and optical photometry, we explore the prevalence and
strength of the UV-upturn in the spectra of quiescent early type galaxies in
several nearby clusters. Even for galaxies with completely passive optical
colours, there is a large spread in vacuum UV colour consistent with almost all
having some UV... | astro-ph.GA | using galex uvot and optical photometry we explore the prevalence and strength of the uvupturn in the spectra of quiescent early type galaxies in several nearby clusters even for galaxies with completely passive optical colours there is a large spread in vacuum uv colour consistent with almost all having some uv upturn... | [['using', 'galex', 'uvot', 'and', 'optical', 'photometry', 'we', 'explore', 'the', 'prevalence', 'and', 'strength', 'of', 'the', 'uvupturn', 'in', 'the', 'spectra', 'of', 'quiescent', 'early', 'type', 'galaxies', 'in', 'several', 'nearby', 'clusters', 'even', 'for', 'galaxies', 'with', 'completely', 'passive', 'optica... | [-0.02896808257259159, 0.15861782131757052, -0.05841193727711328, 0.11449886041031365, -0.05851055251857094, -0.06899186777489552, 0.06522326016084228, 0.4876677483641898, -0.09276905204716464, -0.365927629604801, 0.02744982827241611, -0.3381724864259422, -0.01649675995249855, 0.18117263664848668, -0.05958825350368777,... |
1,801.09689 | Aluminium abundances in five discrete stellar populations of the
globular cluster NGC 2808 | We observed a sample of 90 red giant branch (RGB) stars in NGC 2808 using
FLAMES/GIRAFFE and the high resolution grating with the set up HR21. These
stars have previous accurate atmospheric parameters and abundances of light
elements. We derived aluminium abundances for them from the strong doublet Al I
8772-8773 Ang... | astro-ph.SR astro-ph.GA | we observed a sample of 90 red giant branch rgb stars in ngc 2808 using flamesgiraffe and the high resolution grating with the set up hr21 these stars have previous accurate atmospheric parameters and abundances of light elements we derived aluminium abundances for them from the strong doublet al i 87728773 angstrom as... | [['we', 'observed', 'a', 'sample', 'of', '90', 'red', 'giant', 'branch', 'rgb', 'stars', 'in', 'ngc', '2808', 'using', 'flamesgiraffe', 'and', 'the', 'high', 'resolution', 'grating', 'with', 'the', 'set', 'up', 'hr21', 'these', 'stars', 'have', 'previous', 'accurate', 'atmospheric', 'parameters', 'and', 'abundances', '... | [-0.0301352916340395, 0.09974008394720575, -0.05594968549791709, 0.054442489091636924, -0.04937485245112137, -0.06804878512414825, 0.07846449629685981, 0.44345945700284417, -0.1392896267460333, -0.3851523365876747, -0.0033898613026996298, -0.3006279137073539, -0.028842146412204075, 0.17277936281280695, -0.0812327600630... |
1,801.0969 | Enhancement of electric and magnetic dipole transition of rare-earth
doped thin films tailored by high-index dielectric nanostructures | We propose a simple experimental technique to separately map the emission
from electric and magnetic dipole transitions close to single dielectric
nanostructures, using a few nanometer thin film of rare-earth ion doped
clusters. Rare-earth ions provide electric and magnetic dipole transitions of
similar magnitude. By... | cond-mat.mes-hall | we propose a simple experimental technique to separately map the emission from electric and magnetic dipole transitions close to single dielectric nanostructures using a few nanometer thin film of rareearth ion doped clusters rareearth ions provide electric and magnetic dipole transitions of similar magnitude by record... | [['we', 'propose', 'a', 'simple', 'experimental', 'technique', 'to', 'separately', 'map', 'the', 'emission', 'from', 'electric', 'and', 'magnetic', 'dipole', 'transitions', 'close', 'to', 'single', 'dielectric', 'nanostructures', 'using', 'a', 'few', 'nanometer', 'thin', 'film', 'of', 'rareearth', 'ion', 'doped', 'clus... | [-0.08509319224646567, 0.14858133950887398, 0.0036172286726886757, -0.027951822512330034, -0.016695977552051378, -0.13290250405820236, 0.06582853420499109, 0.5103798548162386, -0.22865149927501743, -0.3646037186672156, -0.027163632995939838, -0.3001524835724283, -0.08356597723527434, 0.20978108838332715, 0.042176997881... |
1,801.09691 | History and destiny of an emerging early-type galaxy: New IFU insights
on the major-merger remnant NGC7252 | NGC7252, which is one of the nearest major-merger galaxy remnants, is an
ideal laboratory to study the processes inherent to the transformation of disc
galaxies to ellipticals as observed about ~1Gyr after the collision. We
obtained wide-field IFU spectroscopy with the VLT-VIMOS integral-field
spectrograph covering t... | astro-ph.GA | ngc7252 which is one of the nearest majormerger galaxy remnants is an ideal laboratory to study the processes inherent to the transformation of disc galaxies to ellipticals as observed about 1gyr after the collision we obtained widefield ifu spectroscopy with the vltvimos integralfield spectrograph covering the central... | [['ngc7252', 'which', 'is', 'one', 'of', 'the', 'nearest', 'majormerger', 'galaxy', 'remnants', 'is', 'an', 'ideal', 'laboratory', 'to', 'study', 'the', 'processes', 'inherent', 'to', 'the', 'transformation', 'of', 'disc', 'galaxies', 'to', 'ellipticals', 'as', 'observed', 'about', '1gyr', 'after', 'the', 'collision', ... | [-0.060243529782287385, 0.0720852480029479, -0.1065328676580337, 0.096500712599638, -0.09127725696828412, -0.03338513459781544, 0.015872738582976654, 0.42773149411863925, -0.1878551054197535, -0.29953892713580116, 0.07011960568478363, -0.24493577352790324, 0.007339267757835618, 0.16070624636322783, -0.02482595981909661... |
1,801.09692 | Continuum Reverberation Mapping of the Accretion Disks in Two Seyfert 1
Galaxies | We present optical continuum lags for two Seyfert 1 galaxies, MCG+08-11-011
and NGC 2617, using monitoring data from a reverberation mapping campaign
carried out in 2014. Our light curves span the ugriz filters over four months,
with median cadences of 1.0 and 0.6 days for MCG+08-11-011 and NGC\,2617,
respectively, c... | astro-ph.GA | we present optical continuum lags for two seyfert 1 galaxies mcg0811011 and ngc 2617 using monitoring data from a reverberation mapping campaign carried out in 2014 our light curves span the ugriz filters over four months with median cadences of 10 and 06 days for mcg0811011 and ngc2617 respectively combined with rough... | [['we', 'present', 'optical', 'continuum', 'lags', 'for', 'two', 'seyfert', '1', 'galaxies', 'mcg0811011', 'and', 'ngc', '2617', 'using', 'monitoring', 'data', 'from', 'a', 'reverberation', 'mapping', 'campaign', 'carried', 'out', 'in', '2014', 'our', 'light', 'curves', 'span', 'the', 'ugriz', 'filters', 'over', 'four'... | [-0.005264474672940141, 0.10562482922376987, -0.04167856120443094, 0.12806476189191648, -0.032955302934937494, -0.1090356391717953, 0.06993905862048826, 0.48142608786057567, -0.14601008848476776, -0.37110085489819505, 0.12173949521032168, -0.3295841002528358, -0.01742709296181084, 0.2752157147153989, -0.049032618939976... |
1,801.09693 | New synthesis models of consistent extragalactic background light over
cosmic time | We present new synthesis models of the extragalactic background light (EBL)
from far infra-red (FIR) to TeV gamma-rays, with an emphasis on the extreme
ultraviolet (UV) background which is responsible for the observed ionization
and thermal state of the intergalactic medium across the cosmic time. Our
models use upda... | astro-ph.GA astro-ph.CO | we present new synthesis models of the extragalactic background light ebl from far infrared fir to tev gammarays with an emphasis on the extreme ultraviolet uv background which is responsible for the observed ionization and thermal state of the intergalactic medium across the cosmic time our models use updated values o... | [['we', 'present', 'new', 'synthesis', 'models', 'of', 'the', 'extragalactic', 'background', 'light', 'ebl', 'from', 'far', 'infrared', 'fir', 'to', 'tev', 'gammarays', 'with', 'an', 'emphasis', 'on', 'the', 'extreme', 'ultraviolet', 'uv', 'background', 'which', 'is', 'responsible', 'for', 'the', 'observed', 'ionizatio... | [0.05662527500671265, 0.12588829375377297, -0.046590910457271574, 0.12299135416009697, -0.06332728521906594, -0.06547620376604835, 0.035256733031664454, 0.5011038628328871, -0.1597830675165928, -0.3481296600019026, 0.0010028086527812782, -0.32414936101974895, 0.05309486934004376, 0.19925711174815533, 0.0093192134207906... |
1,801.09694 | Strong cosmic censorship in de Sitter space | Recent work indicates that the strong cosmic censorship hypothesis is
violated by nearly extremal Reissner-Nordstrom-de Sitter black holes. It was
argued that perturbations of such a black hole decay sufficiently rapidly that
the perturbed spacetime can be extended across the Cauchy horizon as a weak
solution of the ... | gr-qc hep-th | recent work indicates that the strong cosmic censorship hypothesis is violated by nearly extremal reissnernordstromde sitter black holes it was argued that perturbations of such a black hole decay sufficiently rapidly that the perturbed spacetime can be extended across the cauchy horizon as a weak solution of the equat... | [['recent', 'work', 'indicates', 'that', 'the', 'strong', 'cosmic', 'censorship', 'hypothesis', 'is', 'violated', 'by', 'nearly', 'extremal', 'reissnernordstromde', 'sitter', 'black', 'holes', 'it', 'was', 'argued', 'that', 'perturbations', 'of', 'such', 'a', 'black', 'hole', 'decay', 'sufficiently', 'rapidly', 'that',... | [-0.21393846560011406, 0.14860470987635083, -0.08285585820379823, 0.17501636837622944, -0.07985326538028398, -0.14150668923641638, -0.05285155732475111, 0.24912936882217332, -0.1637209914025325, -0.23641225281586448, 0.12309600114891546, -0.321319630351102, -0.11826141942108032, 0.17636352818053547, -0.0307978949564887... |
1,801.09695 | Origins of ultra-diffuse galaxies in the Coma cluster II. Constraints
from their stellar populations | In this second paper of the series, we study with new Keck/DEIMOS spectra the
stellar populations of seven spectroscopically confirmed ultra-diffuse galaxies
(UDGs) in the Coma cluster. We find intermediate to old ages (~ 7Gyr), low
metallicities ([Z/H] ~ -0.7dex) and mostly super-solar abundance patterns
([Mg/Fe] ~ ... | astro-ph.GA | in this second paper of the series we study with new keckdeimos spectra the stellar populations of seven spectroscopically confirmed ultradiffuse galaxies udgs in the coma cluster we find intermediate to old ages 7gyr low metallicities zh 07dex and mostly supersolar abundance patterns mgfe 013dex these properties are s... | [['in', 'this', 'second', 'paper', 'of', 'the', 'series', 'we', 'study', 'with', 'new', 'keckdeimos', 'spectra', 'the', 'stellar', 'populations', 'of', 'seven', 'spectroscopically', 'confirmed', 'ultradiffuse', 'galaxies', 'udgs', 'in', 'the', 'coma', 'cluster', 'we', 'find', 'intermediate', 'to', 'old', 'ages', '7gyr'... | [-0.06230397173490265, 0.12792563382050154, -0.12028515515871933, 0.10529858780866534, -0.08324720390001082, -0.012043583065757684, 0.05150111880482592, 0.40631983814568357, -0.12113445252008057, -0.35104386617654354, 0.025578388175812407, -0.2657427234085405, -0.06419041073133279, 0.16900296460635264, -0.0946120377492... |
1,801.09696 | Double-Higgs boson production in the high-energy limit: planar master
integrals | We consider the virtual corrections to the process $gg\to HH$ at NLO in the
high energy limit and compute the corresponding planar master integrals in an
expansion for small top quark mass. We provide details on the evaluation of the
boundary conditions and present analytic results expressed in terms of harmonic
poly... | hep-ph | we consider the virtual corrections to the process ggto hh at nlo in the high energy limit and compute the corresponding planar master integrals in an expansion for small top quark mass we provide details on the evaluation of the boundary conditions and present analytic results expressed in terms of harmonic polylogari... | [['we', 'consider', 'the', 'virtual', 'corrections', 'to', 'the', 'process', 'ggto', 'hh', 'at', 'nlo', 'in', 'the', 'high', 'energy', 'limit', 'and', 'compute', 'the', 'corresponding', 'planar', 'master', 'integrals', 'in', 'an', 'expansion', 'for', 'small', 'top', 'quark', 'mass', 'we', 'provide', 'details', 'on', 't... | [-0.12607033597305417, 0.09390685050955373, -0.04117569354219505, 0.09660057697234291, -0.01134104389571943, -0.01870462511858652, 0.05397249738990258, 0.32990670619675744, -0.1919029532895925, -0.22776528318914083, 0.050674913596594706, -0.26477340827337825, -0.06555781198235658, 0.19057104399857613, -0.01071588895641... |
1,801.09697 | Poincar\'e-covariant analysis of heavy-quark baryons | We use a symmetry-preserving truncation of meson and baryon bound-state
equations in quantum field theory in order to develop a unified description of
systems constituted from light- and heavy-quarks. In particular, we compute the
spectrum and leptonic decay constants of ground-state pseudoscalar- and
vector-mesons: ... | nucl-th hep-ph | we use a symmetrypreserving truncation of meson and baryon boundstate equations in quantum field theory in order to develop a unified description of systems constituted from light and heavyquarks in particular we compute the spectrum and leptonic decay constants of groundstate pseudoscalar and vectormesons qprime bar q... | [['we', 'use', 'a', 'symmetrypreserving', 'truncation', 'of', 'meson', 'and', 'baryon', 'boundstate', 'equations', 'in', 'quantum', 'field', 'theory', 'in', 'order', 'to', 'develop', 'a', 'unified', 'description', 'of', 'systems', 'constituted', 'from', 'light', 'and', 'heavyquarks', 'in', 'particular', 'we', 'compute'... | [-0.14557677424884746, 0.24609075196280653, -0.0721049816025503, 0.08889455345251346, -0.05002885943120521, -0.13602075255153784, 0.03768271742917234, 0.3068990102272082, -0.18862124555890666, -0.24746735770044462, -0.03310377120022785, -0.3492539510886484, -0.01515521332709435, 0.05624712377482053, 0.0970604751704249,... |
1,801.09698 | SPECIES I: Spectroscopic Parameters and atmosphEric ChemIstriEs of Stars | The detection and subsequent characterisation of exoplanets are intimately
linked to the characteristics of their host star. Therefore, it is necessary to
study the star in detail in order to understand the formation history and
characteristics of their companion(s). Our aims were to develop a community
tool that all... | astro-ph.SR | the detection and subsequent characterisation of exoplanets are intimately linked to the characteristics of their host star therefore it is necessary to study the star in detail in order to understand the formation history and characteristics of their companions our aims were to develop a community tool that allows the... | [['the', 'detection', 'and', 'subsequent', 'characterisation', 'of', 'exoplanets', 'are', 'intimately', 'linked', 'to', 'the', 'characteristics', 'of', 'their', 'host', 'star', 'therefore', 'it', 'is', 'necessary', 'to', 'study', 'the', 'star', 'in', 'detail', 'in', 'order', 'to', 'understand', 'the', 'formation', 'his... | [-0.02713655655999191, 0.07410455965242294, -0.046961163014874435, 0.0933721427873056, -0.06656414907196867, -0.10948386521627056, 0.06084866645885469, 0.4388481442887946, -0.19543935338648535, -0.3904156455916567, 0.02789997606285124, -0.2901917065969666, -0.052644608573962116, 0.19702815812081909, -0.0369863024911152... |
1,801.09699 | Normal black holes in bulge-less galaxies: the largely quiescent,
merger-free growth of black holes over cosmic time | Understanding the processes that drive the formation of black holes (BHs) is
a key topic in observational cosmology. While the observed
$M_{\mathrm{BH}}$--$M_{\mathrm{Bulge}}$ correlation in bulge-dominated galaxies
is thought to be produced by major mergers, the existence of a
$M_{\mathrm{BH}}$--$M_{\star}$ relation... | astro-ph.GA | understanding the processes that drive the formation of black holes bhs is a key topic in observational cosmology while the observed m_mathrmbhm_mathrmbulge correlation in bulgedominated galaxies is thought to be produced by major mergers the existence of a m_mathrmbhm_star relation across all galaxy morphological type... | [['understanding', 'the', 'processes', 'that', 'drive', 'the', 'formation', 'of', 'black', 'holes', 'bhs', 'is', 'a', 'key', 'topic', 'in', 'observational', 'cosmology', 'while', 'the', 'observed', 'm_mathrmbhm_mathrmbulge', 'correlation', 'in', 'bulgedominated', 'galaxies', 'is', 'thought', 'to', 'be', 'produced', 'by... | [-0.10297940844117383, 0.10930683233989091, -0.06314467667695581, 0.1499135449119848, -0.08836903665284578, -0.03808156082754215, 0.03089715152060943, 0.38833343513915985, -0.16404479052804624, -0.34433156187739666, 0.06761162042000629, -0.27775544460871787, -0.07192884532636717, 0.2293621388500173, -0.0386713083953770... |
1,801.097 | The energetics of AGN radiation pressure-driven outflows | The increasing observational evidence of galactic outflows is considered as a
sign of active galactic nucleus (AGN) feedback in action. However, the physical
mechanism responsible for driving the observed outflows remains unclear, and
whether it is due to momentum, energy, or radiation is still a matter of
debate. Th... | astro-ph.GA astro-ph.HE | the increasing observational evidence of galactic outflows is considered as a sign of active galactic nucleus agn feedback in action however the physical mechanism responsible for driving the observed outflows remains unclear and whether it is due to momentum energy or radiation is still a matter of debate the observed... | [['the', 'increasing', 'observational', 'evidence', 'of', 'galactic', 'outflows', 'is', 'considered', 'as', 'a', 'sign', 'of', 'active', 'galactic', 'nucleus', 'agn', 'feedback', 'in', 'action', 'however', 'the', 'physical', 'mechanism', 'responsible', 'for', 'driving', 'the', 'observed', 'outflows', 'remains', 'unclea... | [-0.09243391504112099, 0.1358739298990085, -0.013686693047306367, 0.16453272765890384, -0.10542079226690389, -0.11022104046174458, 0.027994725427457266, 0.42557462328778844, -0.18479033674534764, -0.3472115731897897, 0.04857090094592422, -0.27488704645740136, 0.0019333308846398722, 0.21344544681653912, 0.00755601274293... |
1,801.09701 | Polarized anisotropic spectral distortions of the CMB: Galactic and
extragalactic constraints on photon-axion conversion | We revisit the cosmological constraints on resonant and non-resonant
conversion of photons to axions in the cosmological magnetic fields. We find
that the constraints on photon-axion coupling and primordial magnetic fields
are much weaker than previously claimed for low mass axion like particles with
masses $m_{\rm a... | astro-ph.CO hep-ph hep-th | we revisit the cosmological constraints on resonant and nonresonant conversion of photons to axions in the cosmological magnetic fields we find that the constraints on photonaxion coupling and primordial magnetic fields are much weaker than previously claimed for low mass axion like particles with masses m_rm a lesssim... | [['we', 'revisit', 'the', 'cosmological', 'constraints', 'on', 'resonant', 'and', 'nonresonant', 'conversion', 'of', 'photons', 'to', 'axions', 'in', 'the', 'cosmological', 'magnetic', 'fields', 'we', 'find', 'that', 'the', 'constraints', 'on', 'photonaxion', 'coupling', 'and', 'primordial', 'magnetic', 'fields', 'are'... | [-0.11464899952288829, 0.230442187363716, 0.006528797428144661, 0.1280169531508678, -0.09740486973984153, -0.06203091286711002, -0.007686322171563157, 0.3768485821941097, -0.21467657509799065, -0.3647811789979416, 0.0308205113364156, -0.29620874098579125, -0.006824912238144841, 0.22893669875338674, 0.07045708231179786,... |
1,801.09702 | Cyclic variations in the periods of RR Lyr stars | We report here on two types of cyclic variations that can be observed in the
periods of RR Lyr stars, i.e., the Blazhko and the light-time effects. The
former has been investigated by studying the amplitude variations recorded in
RR Lyr itself, firstly by Kepler and then by the network of the "Very Tiny
Telescopes" (... | astro-ph.SR | we report here on two types of cyclic variations that can be observed in the periods of rr lyr stars ie the blazhko and the lighttime effects the former has been investigated by studying the amplitude variations recorded in rr lyr itself firstly by kepler and then by the network of the very tiny telescopes vtts the lat... | [['we', 'report', 'here', 'on', 'two', 'types', 'of', 'cyclic', 'variations', 'that', 'can', 'be', 'observed', 'in', 'the', 'periods', 'of', 'rr', 'lyr', 'stars', 'ie', 'the', 'blazhko', 'and', 'the', 'lighttime', 'effects', 'the', 'former', 'has', 'been', 'investigated', 'by', 'studying', 'the', 'amplitude', 'variatio... | [-0.1271647921292692, 0.16734127873574856, -0.09443770812183458, 0.06387530098811933, -0.12419096180187758, -0.09417836370086798, 0.0874670486076064, 0.3238255521983549, -0.182519075066422, -0.3301629874634967, 0.09392953642158298, -0.29779807824837995, -0.16467760037630796, 0.24740997273024293, -0.09689388878177851, -... |
1,801.09703 | Vacuum-like jet fragmentation in a dense QCD medium | We study the fragmentation of a jet propagating in a dense quark-gluon
plasma. Using a leading, double-logarithmic approximation in perturbative QCD,
we compute for the first time the effects of the medium on the vacuum-like
emissions. We show that, due to the scatterings off the plasma, the in-medium
parton showers ... | hep-ph nucl-th | we study the fragmentation of a jet propagating in a dense quarkgluon plasma using a leading doublelogarithmic approximation in perturbative qcd we compute for the first time the effects of the medium on the vacuumlike emissions we show that due to the scatterings off the plasma the inmedium parton showers differ from ... | [['we', 'study', 'the', 'fragmentation', 'of', 'a', 'jet', 'propagating', 'in', 'a', 'dense', 'quarkgluon', 'plasma', 'using', 'a', 'leading', 'doublelogarithmic', 'approximation', 'in', 'perturbative', 'qcd', 'we', 'compute', 'for', 'the', 'first', 'time', 'the', 'effects', 'of', 'the', 'medium', 'on', 'the', 'vacuuml... | [-0.08575692007850323, 0.1992873661782961, -0.1701189612120308, 0.1268395411712885, -0.014267912584837976, 0.025448428195706762, -0.005981310454944333, 0.39172690728126647, -0.19828640823098984, -0.23998808875106847, -0.006506261589762929, -0.32145899923129395, -0.012532745830837515, 0.10857377412657325, 0.072864850788... |
1,801.09704 | What does the matter created in high multiplicity proton-nucleus
collisions teach us about the 3-D structure of the proton? | The study of multiparticle correlations and collectivity in the hot and dense
matter created in collisions of heavy-ions as well as those of smaller systems
such as proton--heavy-ion collisions has progressed to the point where detailed
knowledge of the three-dimensional structure of the proton is needed to
confront ... | hep-ph nucl-ex nucl-th | the study of multiparticle correlations and collectivity in the hot and dense matter created in collisions of heavyions as well as those of smaller systems such as protonheavyion collisions has progressed to the point where detailed knowledge of the threedimensional structure of the proton is needed to confront experim... | [['the', 'study', 'of', 'multiparticle', 'correlations', 'and', 'collectivity', 'in', 'the', 'hot', 'and', 'dense', 'matter', 'created', 'in', 'collisions', 'of', 'heavyions', 'as', 'well', 'as', 'those', 'of', 'smaller', 'systems', 'such', 'as', 'protonheavyion', 'collisions', 'has', 'progressed', 'to', 'the', 'point'... | [-0.05725223521809452, 0.15196241191230142, -0.1410572750475974, 0.10859213491382363, -0.01839162429454378, -0.04757999750122858, -0.03756000331710451, 0.3559955299133435, -0.23208057747867245, -0.31957039762682354, 0.04870868768977324, -0.2966768252528989, -0.06599034485407174, 0.16967269216323844, 0.00283056155044155... |
1,801.09705 | The Morita theory of quantum graph isomorphisms | We classify instances of quantum pseudo-telepathy in the graph isomorphism
game, exploiting the recently discovered connection between quantum information
and the theory of quantum automorphism groups. Specifically, we show that
graphs quantum isomorphic to a given graph are in bijective correspondence with
Morita eq... | quant-ph math.CT math.QA | we classify instances of quantum pseudotelepathy in the graph isomorphism game exploiting the recently discovered connection between quantum information and the theory of quantum automorphism groups specifically we show that graphs quantum isomorphic to a given graph are in bijective correspondence with morita equivale... | [['we', 'classify', 'instances', 'of', 'quantum', 'pseudotelepathy', 'in', 'the', 'graph', 'isomorphism', 'game', 'exploiting', 'the', 'recently', 'discovered', 'connection', 'between', 'quantum', 'information', 'and', 'the', 'theory', 'of', 'quantum', 'automorphism', 'groups', 'specifically', 'we', 'show', 'that', 'gr... | [-0.17157860410437858, 0.0969734379677211, -0.07499409468343471, 0.06790455753849656, -0.12497657498519062, -0.1515489354952952, -0.007636490011075784, 0.4041546481764979, -0.3642637399597126, -0.25471135960314534, 0.08636047775252607, -0.295997043690312, -0.21447182315461644, 0.14286508780974916, -0.17336330361043414,... |
1,801.09706 | No Metallicity Correlation Associated with the Kepler Dichotomy | NASA's Kepler mission has discovered thousands of planetary systems, ~20% of
which are found to host multiple transiting planets. This relative paucity
(compared to the high fraction of single transiting systems) is postulated to
result from a distinction in the architecture between multi-transiting systems
and those... | astro-ph.EP | nasas kepler mission has discovered thousands of planetary systems 20 of which are found to host multiple transiting planets this relative paucity compared to the high fraction of single transiting systems is postulated to result from a distinction in the architecture between multitransiting systems and those hosting a... | [['nasas', 'kepler', 'mission', 'has', 'discovered', 'thousands', 'of', 'planetary', 'systems', '20', 'of', 'which', 'are', 'found', 'to', 'host', 'multiple', 'transiting', 'planets', 'this', 'relative', 'paucity', 'compared', 'to', 'the', 'high', 'fraction', 'of', 'single', 'transiting', 'systems', 'is', 'postulated',... | [-0.11263145847890595, 0.1128013479822444, -0.09260668621655947, 0.07419578857093811, -0.13551860057362697, -0.07616678762393511, 0.11207266139317061, 0.3372094904231589, -0.15836855167962186, -0.4030080280161171, 0.05911856902561177, -0.300281688994993, -0.1240806273398618, 0.22995670922422343, -0.12087964025852309, 0... |
1,801.09707 | Thermal conductivity in 1d: disorder-induced transition from anomalous
to normal scaling | It is well known that the contribution of harmonic phonons to the thermal
conductivity of 1D systems diverges with the harmonic chain length $L$
(explicitly, increases with $L$ as a power-law with a positive power).
Furthermore, within various one-dimensional models containing disorder it was
shown that this divergen... | cond-mat.dis-nn cond-mat.stat-mech | it is well known that the contribution of harmonic phonons to the thermal conductivity of 1d systems diverges with the harmonic chain length l explicitly increases with l as a powerlaw with a positive power furthermore within various onedimensional models containing disorder it was shown that this divergence persists w... | [['it', 'is', 'well', 'known', 'that', 'the', 'contribution', 'of', 'harmonic', 'phonons', 'to', 'the', 'thermal', 'conductivity', 'of', '1d', 'systems', 'diverges', 'with', 'the', 'harmonic', 'chain', 'length', 'l', 'explicitly', 'increases', 'with', 'l', 'as', 'a', 'powerlaw', 'with', 'a', 'positive', 'power', 'furth... | [-0.17724349805292958, 0.24146230911719613, -0.05340384123943901, 0.05205489985544571, -0.029740851708791323, -0.22725123875554548, 0.02635471046798759, 0.35943112744199524, -0.2938046032472307, -0.2110211743792105, 0.0644165453389481, -0.35132209562127376, -0.12897296019784538, 0.1882065822913622, 0.029559063041233458... |
1,801.09708 | Comments on $T \bar T$ double trace deformations and boundary conditions | We study the UV dynamics of $\mu T \bar T$ deformed conformal field theories
formulated as a deformation of generating functions. We explore the issue of
non-perturbative completion of the $\mu$ expansion by deriving an integral
expression using the Fourier/Legendre transform technique, and show that it is
more natur... | hep-th | we study the uv dynamics of mu t bar t deformed conformal field theories formulated as a deformation of generating functions we explore the issue of nonperturbative completion of the mu expansion by deriving an integral expression using the fourierlegendre transform technique and show that it is more natural to impose ... | [['we', 'study', 'the', 'uv', 'dynamics', 'of', 'mu', 't', 'bar', 't', 'deformed', 'conformal', 'field', 'theories', 'formulated', 'as', 'a', 'deformation', 'of', 'generating', 'functions', 'we', 'explore', 'the', 'issue', 'of', 'nonperturbative', 'completion', 'of', 'the', 'mu', 'expansion', 'by', 'deriving', 'an', 'i... | [-0.11114356412513024, 0.09747029829041678, -0.12772863890122937, 0.08827794985761529, -0.1134505194264004, -0.13589119189138332, -0.0038156876261963182, 0.33277320958034373, -0.24550432689959206, -0.24609694694707462, 0.09777054850977049, -0.22164534790867782, -0.19774363335805484, 0.1467281829184258, -0.0606056145919... |
1,801.09709 | Temporally-Biased Sampling for Online Model Management | To maintain the accuracy of supervised learning models in the presence of
evolving data streams, we provide temporally-biased sampling schemes that
weight recent data most heavily, with inclusion probabilities for a given data
item decaying exponentially over time. We then periodically retrain the models
on the curre... | cs.DB | to maintain the accuracy of supervised learning models in the presence of evolving data streams we provide temporallybiased sampling schemes that weight recent data most heavily with inclusion probabilities for a given data item decaying exponentially over time we then periodically retrain the models on the current sam... | [['to', 'maintain', 'the', 'accuracy', 'of', 'supervised', 'learning', 'models', 'in', 'the', 'presence', 'of', 'evolving', 'data', 'streams', 'we', 'provide', 'temporallybiased', 'sampling', 'schemes', 'that', 'weight', 'recent', 'data', 'most', 'heavily', 'with', 'inclusion', 'probabilities', 'for', 'a', 'given', 'da... | [-0.08245729030583238, 0.052551994630761566, -0.08462399435534951, 0.04195263039359741, -0.07321644253021137, -0.12623880117498032, 0.12103878973590088, 0.40671462827499527, -0.26126742770095723, -0.33439825471780704, 0.12698365461048644, -0.2549356416476839, -0.07513893492802305, 0.21710604391266883, -0.11031080267132... |
1,801.0971 | tempoGAN: A Temporally Coherent, Volumetric GAN for Super-resolution
Fluid Flow | We propose a temporally coherent generative model addressing the
super-resolution problem for fluid flows. Our work represents a first approach
to synthesize four-dimensional physics fields with neural networks. Based on a
conditional generative adversarial network that is designed for the inference
of three-dimensio... | cs.LG cs.GR | we propose a temporally coherent generative model addressing the superresolution problem for fluid flows our work represents a first approach to synthesize fourdimensional physics fields with neural networks based on a conditional generative adversarial network that is designed for the inference of threedimensional vol... | [['we', 'propose', 'a', 'temporally', 'coherent', 'generative', 'model', 'addressing', 'the', 'superresolution', 'problem', 'for', 'fluid', 'flows', 'our', 'work', 'represents', 'a', 'first', 'approach', 'to', 'synthesize', 'fourdimensional', 'physics', 'fields', 'with', 'neural', 'networks', 'based', 'on', 'a', 'condi... | [-0.02048517719393001, 0.052620276019701526, -0.06977273094105638, 0.05636624980548327, -0.10378297867201683, -0.15365479733219317, 0.013948202795452542, 0.43446776729542763, -0.26342472223720204, -0.3340044798846874, 0.054740474419021565, -0.23122819331215902, -0.19363473733731856, 0.21363591285577666, -0.104383400226... |
1,801.09711 | Nonlinear evolution of the AdS$_4$ black hole bomb | The superradiant instability of rotating black holes with negative
cosmological constant is studied by numerically solving the full
3+1-dimensional Einstein equations. We find evidence for an epoch dominated by
a solution with a single helical Killing vector and a multi-stage process with
distinct superradiant instab... | gr-qc hep-th | the superradiant instability of rotating black holes with negative cosmological constant is studied by numerically solving the full 31dimensional einstein equations we find evidence for an epoch dominated by a solution with a single helical killing vector and a multistage process with distinct superradiant instabilitie... | [['the', 'superradiant', 'instability', 'of', 'rotating', 'black', 'holes', 'with', 'negative', 'cosmological', 'constant', 'is', 'studied', 'by', 'numerically', 'solving', 'the', 'full', '31dimensional', 'einstein', 'equations', 'we', 'find', 'evidence', 'for', 'an', 'epoch', 'dominated', 'by', 'a', 'solution', 'with'... | [-0.20389068126678467, 0.19531935988699034, -0.029281669648157226, 0.06601506699698803, -0.09809835261354843, -0.19518759487610723, -0.059595381220181785, 0.2932911651726398, -0.19060529788128203, -0.22239319504135185, 0.06415019183768891, -0.28224279226528276, -0.1191443572855658, 0.15591811397009425, 0.08122070059180... |
1,801.09712 | Implications of the radio and X-ray emission that followed GW170817 | The radio and X-rays that followed GW170817 increased gradually over
$\sim~100$ days, resembling the radio flare predicted to arise from the
interaction of a binary neutron star merger outflow with the ISM
\citep{nakar2011}. Considering a blast wave moving with a Lorentz factor
$\Gamma$, we show that an off-axis obse... | astro-ph.HE gr-qc | the radio and xrays that followed gw170817 increased gradually over sim100 days resembling the radio flare predicted to arise from the interaction of a binary neutron star merger outflow with the ism citepnakar2011 considering a blast wave moving with a lorentz factor gamma we show that an offaxis observer namely an ob... | [['the', 'radio', 'and', 'xrays', 'that', 'followed', 'gw170817', 'increased', 'gradually', 'over', 'sim100', 'days', 'resembling', 'the', 'radio', 'flare', 'predicted', 'to', 'arise', 'from', 'the', 'interaction', 'of', 'a', 'binary', 'neutron', 'star', 'merger', 'outflow', 'with', 'the', 'ism', 'citepnakar2011', 'con... | [-0.0949454236253956, 0.1853166723892918, -0.10975295372475359, 0.10830328169390839, -0.13329992807315907, -0.1370804371501326, 0.011824311745546484, 0.429878303339999, -0.22833142976129525, -0.30387073541165127, 0.08486384791724692, -0.24753986194176614, -0.03646199173938231, 0.21025774578031683, -0.006340827526900168... |
1,801.09713 | Majorana representations of spin and an alternative solution of the
Kitaev honeycomb model | Based on the Dirac spinor representation of the SO(4) group, we discuss the
relationship between three types of representation of spin in terms of Majorana
fermions, namely the Kitaev representation, the SO(3) representation and the
SO(4) chiral representation. Comparing the three types, we show that the
Hilbert spac... | cond-mat.str-el | based on the dirac spinor representation of the so4 group we discuss the relationship between three types of representation of spin in terms of majorana fermions namely the kitaev representation the so3 representation and the so4 chiral representation comparing the three types we show that the hilbert space of the so3 ... | [['based', 'on', 'the', 'dirac', 'spinor', 'representation', 'of', 'the', 'so4', 'group', 'we', 'discuss', 'the', 'relationship', 'between', 'three', 'types', 'of', 'representation', 'of', 'spin', 'in', 'terms', 'of', 'majorana', 'fermions', 'namely', 'the', 'kitaev', 'representation', 'the', 'so3', 'representation', '... | [-0.15837149590934682, 0.1573188074824319, -0.0926672109741379, 0.06620927795037543, -0.08898089584809812, -0.1293359201711913, 0.008966599724248446, 0.3631297486100459, -0.2126180074234126, -0.25532086710022256, 0.054413439439623755, -0.28024777999345324, -0.19007871890172476, 0.14828555493714343, 0.0289892447181046, ... |
1,801.09714 | Bio-inspired underwater propulsors | Here we present a general overview of bio-inspired propulsion. We identify
the major types of aquatic swimmers (oscillatory, undulatory, pulsatile, and
drag-based) and break down their mechanisms for thrust production (drag-based,
lift-based, added mass, and momentum injection). For each swimmer, we (1)
discuss wake ... | physics.flu-dyn | here we present a general overview of bioinspired propulsion we identify the major types of aquatic swimmers oscillatory undulatory pulsatile and dragbased and break down their mechanisms for thrust production dragbased liftbased added mass and momentum injection for each swimmer we 1 discuss wake characteristics 2 der... | [['here', 'we', 'present', 'a', 'general', 'overview', 'of', 'bioinspired', 'propulsion', 'we', 'identify', 'the', 'major', 'types', 'of', 'aquatic', 'swimmers', 'oscillatory', 'undulatory', 'pulsatile', 'and', 'dragbased', 'and', 'break', 'down', 'their', 'mechanisms', 'for', 'thrust', 'production', 'dragbased', 'lift... | [-0.12857511805128052, 0.18723271099518832, -0.055696452278899, 0.052223278694365126, -0.12565335711744957, -0.14479077082408004, -0.028371879638791443, 0.3639943928342976, -0.2409117628520431, -0.3211715172670067, 0.08878768902042344, -0.2234446136187204, -0.17951137783031348, 0.19319178812422674, -0.11977113434432508... |
1,801.09715 | Contrasting Web Robot and Human Behaviors with Network Models | The web graph is a commonly-used network representation of the hyperlink
structure of a website. A network of similar structure to the web graph, which
we call the session graph has properties that reflect the browsing habits of
the agents in the web server logs. In this paper, we apply session graphs to
compare the ... | cs.SI | the web graph is a commonlyused network representation of the hyperlink structure of a website a network of similar structure to the web graph which we call the session graph has properties that reflect the browsing habits of the agents in the web server logs in this paper we apply session graphs to compare the activit... | [['the', 'web', 'graph', 'is', 'a', 'commonlyused', 'network', 'representation', 'of', 'the', 'hyperlink', 'structure', 'of', 'a', 'website', 'a', 'network', 'of', 'similar', 'structure', 'to', 'the', 'web', 'graph', 'which', 'we', 'call', 'the', 'session', 'graph', 'has', 'properties', 'that', 'reflect', 'the', 'brows... | [-0.12044712601761733, -0.0007095224516732352, -0.09748398938083223, 0.09121476820004838, -0.15440720810887537, -0.1573844046943954, 0.10259494756414954, 0.43467036709189416, -0.2694907022480454, -0.3832986428322537, 0.08154303363125238, -0.2896413074310736, -0.13821912305828715, 0.17753344042359717, -0.116516157907566... |
1,801.09716 | The structure of doubly non-commuting isometries | Suppose that $n\geq 1$ and that, for all $i$ and $j$ with $1\leq i,j\leq n$
and $i\neq j$, $z_{ij}\in{\mathbb T}$ are given such that
$z_{ji}=\overline{z}_{ij}$ for all $i\neq j$. If $V_1,\dotsc, V_n$ are
isometries on a Hilbert space such that $V_i^\ast
V_j^{\phantom{\ast}}\!=\overline{z}_{ij} V_j^{\phantom{\ast}}\!... | math.OA math.FA | suppose that ngeq 1 and that for all i and j with 1leq ijleq n and ineq j z_ijinmathbb t are given such that z_jioverlinez_ij for all ineq j if v_1dotsc v_n are isometries on a hilbert space such that v_iast v_jphantomastoverlinez_ij v_jphantomastv_iast for all ineq j then v_1dotscv_n is called an ntuple of doubly nonc... | [['suppose', 'that', 'ngeq', '1', 'and', 'that', 'for', 'all', 'i', 'and', 'j', 'with', '1leq', 'ijleq', 'n', 'and', 'ineq', 'j', 'z_ijinmathbb', 't', 'are', 'given', 'such', 'that', 'z_jioverlinez_ij', 'for', 'all', 'ineq', 'j', 'if', 'v_1dotsc', 'v_n', 'are', 'isometries', 'on', 'a', 'hilbert', 'space', 'such', 'that... | [-0.157921938922502, 0.1882005693401475, -0.029413362848572433, 0.009302830334086644, -0.055348959890478805, -0.1590611481741588, -0.04874576141446596, 0.38091399183839614, -0.31548102215553325, -0.1746786641047543, 0.09080232475146961, -0.30846943513542, -0.14554106121552954, 0.1486581332800496, -0.1054265724605001, 0... |
1,801.09717 | Compact binary merger and kilonova: outflows from remnant disc | Outflows launched from a remnant disc of compact binary merger may have
essential contribution to the kilonova emission. Numerical calculations are
conducted in this work to study the structure of accretion flows and outflows.
By the incorporation of limited-energy advection in the hyper-accretion discs,
outflows occ... | astro-ph.HE | outflows launched from a remnant disc of compact binary merger may have essential contribution to the kilonova emission numerical calculations are conducted in this work to study the structure of accretion flows and outflows by the incorporation of limitedenergy advection in the hyperaccretion discs outflows occur natu... | [['outflows', 'launched', 'from', 'a', 'remnant', 'disc', 'of', 'compact', 'binary', 'merger', 'may', 'have', 'essential', 'contribution', 'to', 'the', 'kilonova', 'emission', 'numerical', 'calculations', 'are', 'conducted', 'in', 'this', 'work', 'to', 'study', 'the', 'structure', 'of', 'accretion', 'flows', 'and', 'ou... | [-0.10692863366332092, 0.1425002567790844, -0.017589024293216335, 0.13972174742329438, -0.11027912494036363, -0.004515345881713166, -0.014280186120166087, 0.39247551790384994, -0.19541884394925382, -0.332770800418991, 0.0731887475021264, -0.2983798083695148, 0.022749276128229048, 0.23596638154821375, 0.0008213558006468... |
1,801.09718 | Object-based reasoning in VQA | Visual Question Answering (VQA) is a novel problem domain where multi-modal
inputs must be processed in order to solve the task given in the form of a
natural language. As the solutions inherently require to combine visual and
natural language processing with abstract reasoning, the problem is considered
as AI-comple... | cs.CV | visual question answering vqa is a novel problem domain where multimodal inputs must be processed in order to solve the task given in the form of a natural language as the solutions inherently require to combine visual and natural language processing with abstract reasoning the problem is considered as aicomplete recen... | [['visual', 'question', 'answering', 'vqa', 'is', 'a', 'novel', 'problem', 'domain', 'where', 'multimodal', 'inputs', 'must', 'be', 'processed', 'in', 'order', 'to', 'solve', 'the', 'task', 'given', 'in', 'the', 'form', 'of', 'a', 'natural', 'language', 'as', 'the', 'solutions', 'inherently', 'require', 'to', 'combine'... | [-0.06165885124937631, -0.03542805378002903, -0.05003517957475896, 0.06912642030846865, -0.17316682755391902, -0.1414224000674529, 0.01930401666322723, 0.41120859486265826, -0.2981278688261787, -0.3770362933775267, 0.08889309234711198, -0.25907526119576335, -0.1406420304981741, 0.22428796203950277, -0.17415637453534424... |
1,801.09719 | The Epoch of IGM heating by early sources of X-rays | Observations of the 21 cm line from neutral hydrogen indicate that an Epoch
of Heating (EoH) might have preceded the later Epoch of Reionization (EoR).
Here we study the effects on the ionization state and the thermal history of
the Intergalactic Medium (IGM) during the EoH induced by different assumptions
on ionizin... | astro-ph.CO astro-ph.GA | observations of the 21 cm line from neutral hydrogen indicate that an epoch of heating eoh might have preceded the later epoch of reionization eor here we study the effects on the ionization state and the thermal history of the intergalactic medium igm during the eoh induced by different assumptions on ionizing sources... | [['observations', 'of', 'the', '21', 'cm', 'line', 'from', 'neutral', 'hydrogen', 'indicate', 'that', 'an', 'epoch', 'of', 'heating', 'eoh', 'might', 'have', 'preceded', 'the', 'later', 'epoch', 'of', 'reionization', 'eor', 'here', 'we', 'study', 'the', 'effects', 'on', 'the', 'ionization', 'state', 'and', 'the', 'ther... | [-0.024582279246325407, 0.18146727546634014, -0.022742346442620538, 0.08050537354418859, -0.05119690961873857, -0.05857584832535524, 0.04827108289464377, 0.4347829539578275, -0.1681110089687406, -0.3220268930641136, 0.02727284765153724, -0.3170779130138856, 0.046680656017477826, 0.17106528583462932, 0.05853281254738769... |
1,801.0972 | A Generalized Circuit for the Hamiltonian Dynamics Through the Truncated
Series | In this paper, we present a method for the Hamiltonian simulation in the
context of eigenvalue estimation problems which improves earlier results
dealing with Hamiltonian simulation through the truncated Taylor series. In
particular, we present a fixed-quantum circuit design for the simulation of the
Hamiltonian dyna... | quant-ph cs.DS cs.LG | in this paper we present a method for the hamiltonian simulation in the context of eigenvalue estimation problems which improves earlier results dealing with hamiltonian simulation through the truncated taylor series in particular we present a fixedquantum circuit design for the simulation of the hamiltonian dynamics h... | [['in', 'this', 'paper', 'we', 'present', 'a', 'method', 'for', 'the', 'hamiltonian', 'simulation', 'in', 'the', 'context', 'of', 'eigenvalue', 'estimation', 'problems', 'which', 'improves', 'earlier', 'results', 'dealing', 'with', 'hamiltonian', 'simulation', 'through', 'the', 'truncated', 'taylor', 'series', 'in', 'p... | [-0.13416019636268975, 0.10963979004485525, -0.062131660351437835, -0.009093723791826833, -0.028930194137175253, -0.11300335341705335, 0.04508993499275431, 0.33243612217562346, -0.272931401467477, -0.31913222697659527, 0.0999088985949855, -0.22644479829617548, -0.19031785011308208, 0.21538128303113338, -0.0528242085943... |
1,801.09721 | Pileup mitigation at the LHC: a theorist's view | To maximise the potential for new measurements and discoveries at the LHC,
the machine delivers as high as possible collision rates. As a consequence,
multiple proton-proton collisions occur whenever two bunches cross. Interesting
high-energy (hard) collisions are therefore contaminated by several soft,
zero-bias, on... | hep-ph hep-ex | to maximise the potential for new measurements and discoveries at the lhc the machine delivers as high as possible collision rates as a consequence multiple protonproton collisions occur whenever two bunches cross interesting highenergy hard collisions are therefore contaminated by several soft zerobias ones this effec... | [['to', 'maximise', 'the', 'potential', 'for', 'new', 'measurements', 'and', 'discoveries', 'at', 'the', 'lhc', 'the', 'machine', 'delivers', 'as', 'high', 'as', 'possible', 'collision', 'rates', 'as', 'a', 'consequence', 'multiple', 'protonproton', 'collisions', 'occur', 'whenever', 'two', 'bunches', 'cross', 'interes... | [-0.04422018346748599, 0.07496341330271308, -0.10878828812565189, 0.09422775539678696, -0.07824226377124432, -0.11008538028949665, 0.0268330286457462, 0.3789406083782928, -0.22884932523932852, -0.33166410215684056, 0.12413353097346974, -0.27400176623551586, -0.1024147798856979, 0.23281539858483788, -0.08851633061302916... |
1,801.09722 | Status of Flavour Maximal Non-minimal Universal Extra Dimension | In this paper we consider an $S^{1}/\mathbb{Z}_2$ compactified flat extra
dimensional scenario where all the standard model states can access the bulk
and have generalised brane localised kinetic terms. The flavour structure of
brane kinetic terms for the standard model fermions are dictated by stringent
flavour boun... | hep-ph | in this paper we consider an s1mathbbz_2 compactified flat extra dimensional scenario where all the standard model states can access the bulk and have generalised brane localised kinetic terms the flavour structure of brane kinetic terms for the standard model fermions are dictated by stringent flavour bounds on the fi... | [['in', 'this', 'paper', 'we', 'consider', 'an', 's1mathbbz_2', 'compactified', 'flat', 'extra', 'dimensional', 'scenario', 'where', 'all', 'the', 'standard', 'model', 'states', 'can', 'access', 'the', 'bulk', 'and', 'have', 'generalised', 'brane', 'localised', 'kinetic', 'terms', 'the', 'flavour', 'structure', 'of', '... | [-0.14936384632512256, 0.2036663727861827, -0.025048840782072326, 0.10792295332171593, -0.0967203246698052, -0.1545973550989754, 0.016206142132858502, 0.2690848529754156, -0.2204134891749368, -0.31398928870535076, 0.07296821921812119, -0.23925705644226558, -0.027026849352075038, 0.10794508649531316, 0.01381658438801857... |
1,801.09723 | Unsupervised Classification of Variable Stars | During the last ten years, a considerable amount of effort has been made to
develop algorithms for automatic classification of variable stars. That has
been primarily achieved by applying machine learning methods to photometric
datasets where objects are represented as light curves. Classifiers require
training sets ... | astro-ph.IM | during the last ten years a considerable amount of effort has been made to develop algorithms for automatic classification of variable stars that has been primarily achieved by applying machine learning methods to photometric datasets where objects are represented as light curves classifiers require training sets to le... | [['during', 'the', 'last', 'ten', 'years', 'a', 'considerable', 'amount', 'of', 'effort', 'has', 'been', 'made', 'to', 'develop', 'algorithms', 'for', 'automatic', 'classification', 'of', 'variable', 'stars', 'that', 'has', 'been', 'primarily', 'achieved', 'by', 'applying', 'machine', 'learning', 'methods', 'to', 'phot... | [-0.05071906815782637, 0.053052213918025476, -0.0989177324699214, 0.06317219377500251, -0.14673754300766267, -0.13199636212833898, 0.11352711675319893, 0.444873398337753, -0.22547144409420983, -0.38214917236523377, 0.06712433167477438, -0.2859549653695026, -0.12474144255350715, 0.24581711087975444, -0.13048686641528243... |
1,801.09724 | Denoising Signals in Cognitive Radio Systems Using An Evolutionary
Algorithm Based Adaptive Filter | Noise originating from several sources in a RF environment degrades the
performance of communication systems. In wideband systems, such as cognitive
radios, noise at the receiver can originate from non-linearity present in the
RF front end, time-varying thermal noise within the receiver radio system, and
noise from a... | eess.SP | noise originating from several sources in a rf environment degrades the performance of communication systems in wideband systems such as cognitive radios noise at the receiver can originate from nonlinearity present in the rf front end timevarying thermal noise within the receiver radio system and noise from adjacent n... | [['noise', 'originating', 'from', 'several', 'sources', 'in', 'a', 'rf', 'environment', 'degrades', 'the', 'performance', 'of', 'communication', 'systems', 'in', 'wideband', 'systems', 'such', 'as', 'cognitive', 'radios', 'noise', 'at', 'the', 'receiver', 'can', 'originate', 'from', 'nonlinearity', 'present', 'in', 'th... | [-0.14625978853179084, 0.029830111663538925, -0.04520387617515918, 0.05976487997710494, -0.03535738774484081, -0.24002836261319055, 0.023822929834366114, 0.4691009468677425, -0.2713068520995913, -0.3150319574045536, 0.1652437803358291, -0.2705513794820026, -0.24214174905515842, 0.20070847056832491, -0.11713468257131382... |
1,801.09725 | Noise Cancellation in Cognitive Radio Systems: A Performance Comparison
of Evolutionary Algorithms | Noise cancellation is one of the important signal processing functions of any
communication system, as noise affects data integrity. In existing systems,
traditional filters are used to cancel the noise from the received signals.
These filters use fixed hardware which is capable of filtering specific
frequency or a r... | eess.SP | noise cancellation is one of the important signal processing functions of any communication system as noise affects data integrity in existing systems traditional filters are used to cancel the noise from the received signals these filters use fixed hardware which is capable of filtering specific frequency or a range o... | [['noise', 'cancellation', 'is', 'one', 'of', 'the', 'important', 'signal', 'processing', 'functions', 'of', 'any', 'communication', 'system', 'as', 'noise', 'affects', 'data', 'integrity', 'in', 'existing', 'systems', 'traditional', 'filters', 'are', 'used', 'to', 'cancel', 'the', 'noise', 'from', 'the', 'received', '... | [-0.12995135634665148, 0.019894429106841197, -0.048570990217129746, 0.0864676919795015, -0.06895915084689459, -0.23091708023128085, 0.02326111662019368, 0.4673631832111573, -0.27038483498483035, -0.318768162858461, 0.16865061261299727, -0.2540314420517804, -0.22952682939459287, 0.20570359454413759, -0.11663638409182141... |
1,801.09726 | Adsorption of parahydrogen on graphene | We study the low temperature properties of a single layer of parahydrogen
adsorbed on graphene, by means of Quantum Monte Carlo simulations. The computed
phase diagram is very similar to that of helium on the same substrate,
featuring commensurate solid phases with fillings 1/3 and 7/16, as well as
domain wall phases... | cond-mat.mes-hall cond-mat.other | we study the low temperature properties of a single layer of parahydrogen adsorbed on graphene by means of quantum monte carlo simulations the computed phase diagram is very similar to that of helium on the same substrate featuring commensurate solid phases with fillings 13 and 716 as well as domain wall phases at inte... | [['we', 'study', 'the', 'low', 'temperature', 'properties', 'of', 'a', 'single', 'layer', 'of', 'parahydrogen', 'adsorbed', 'on', 'graphene', 'by', 'means', 'of', 'quantum', 'monte', 'carlo', 'simulations', 'the', 'computed', 'phase', 'diagram', 'is', 'very', 'similar', 'to', 'that', 'of', 'helium', 'on', 'the', 'same'... | [-0.11126438755858949, 0.19215205751194542, -0.033917683316394685, 0.030045656303668188, 0.024745902012930147, -0.13790028758553996, 0.13988388564385887, 0.4093968296940956, -0.24157568520555894, -0.3297193429329329, 0.08660785596714252, -0.3252181474533346, -0.06374516259464953, 0.13144379106039802, 0.0502946724804739... |
1,801.09727 | Coherent buildup of high harmonic radiation: the classical perspective | We present a classical model for high harmonic generation during the
propagation of an intense laser pulse through an atomic gas. Numerical
simulations of the model show excellent quantitative agreement with the
corresponding quantum model for the blueshift and intensity reduction of the
propagating laser pulse over ... | physics.atom-ph nlin.CD | we present a classical model for high harmonic generation during the propagation of an intense laser pulse through an atomic gas numerical simulations of the model show excellent quantitative agreement with the corresponding quantum model for the blueshift and intensity reduction of the propagating laser pulse over exp... | [['we', 'present', 'a', 'classical', 'model', 'for', 'high', 'harmonic', 'generation', 'during', 'the', 'propagation', 'of', 'an', 'intense', 'laser', 'pulse', 'through', 'an', 'atomic', 'gas', 'numerical', 'simulations', 'of', 'the', 'model', 'show', 'excellent', 'quantitative', 'agreement', 'with', 'the', 'correspond... | [-0.09342292667516679, 0.12950603835059538, -0.09525719380594398, 0.07636410930947597, -0.0014911417199886944, -0.06995861804553945, 0.03076050220682335, 0.4387092805026393, -0.26763868591699164, -0.297240511440721, -0.004391138892204158, -0.25935859814604845, -0.12325999591082923, 0.2504276264287335, 0.021637142066059... |
1,801.09728 | Sampling techniques for big data analysis in finite population inference | In analyzing big data for finite population inference, it is critical to
adjust for the selection bias in the big data. In this paper, we propose two
methods of reducing the selection bias associated with the big data sample. The
first method uses a version of inverse sampling by incorporating auxiliary
information f... | stat.ME | in analyzing big data for finite population inference it is critical to adjust for the selection bias in the big data in this paper we propose two methods of reducing the selection bias associated with the big data sample the first method uses a version of inverse sampling by incorporating auxiliary information from ex... | [['in', 'analyzing', 'big', 'data', 'for', 'finite', 'population', 'inference', 'it', 'is', 'critical', 'to', 'adjust', 'for', 'the', 'selection', 'bias', 'in', 'the', 'big', 'data', 'in', 'this', 'paper', 'we', 'propose', 'two', 'methods', 'of', 'reducing', 'the', 'selection', 'bias', 'associated', 'with', 'the', 'big... | [-0.03406378407740877, 0.014398217448615469, -0.07991892503397095, 0.09249038948189645, -0.07970586089594733, -0.11082911412453368, 0.07446064786830296, 0.4024879283848263, -0.2549246632272289, -0.35592487276132617, 0.14986175130941862, -0.2986836274464925, -0.0829009784651654, 0.2188592241766552, -0.0822098270768211, ... |
1,801.09729 | Numerically Modelling Stochastic Lie Transport in Fluid Dynamics | We present a numerical investigation of stochastic transport in ideal fluids.
According to Holm (Proc Roy Soc, 2015) and Cotter et al. (2017), the principles
of transformation theory and multi-time homogenisation, respectively, imply a
physically meaningful, data-driven approach for decomposing the fluid transport
ve... | physics.flu-dyn | we present a numerical investigation of stochastic transport in ideal fluids according to holm proc roy soc 2015 and cotter et al 2017 the principles of transformation theory and multitime homogenisation respectively imply a physically meaningful datadriven approach for decomposing the fluid transport velocity into its... | [['we', 'present', 'a', 'numerical', 'investigation', 'of', 'stochastic', 'transport', 'in', 'ideal', 'fluids', 'according', 'to', 'holm', 'proc', 'roy', 'soc', '2015', 'and', 'cotter', 'et', 'al', '2017', 'the', 'principles', 'of', 'transformation', 'theory', 'and', 'multitime', 'homogenisation', 'respectively', 'impl... | [-0.1090845767534432, 0.03765264601738314, -0.1056439783800431, 0.013589724237475582, -0.08961169913674545, -0.092960998133728, -0.020939212662845173, 0.268987687572724, -0.3079384233322785, -0.2848702536124473, 0.09241677507537069, -0.2236331016450857, -0.14472754835739093, 0.18717254826597954, -0.06401620230065998, 0... |
1,801.0973 | Anomaly mediated SUSY breaking model retrofitted for naturalness | Anomaly-mediated supersymmetry breaking (AMSB) models seem to have become
increasingly implausible due to 1. difficulty in generating a Higgs mass
m(h)~125 GeV, 2. typically unnatural superparticle spectra characterized by a
large superpotential mu term and 3. the possibility of a wino-like lightest
SUSY particle (LS... | hep-ph | anomalymediated supersymmetry breaking amsb models seem to have become increasingly implausible due to 1 difficulty in generating a higgs mass mh125 gev 2 typically unnatural superparticle spectra characterized by a large superpotential mu term and 3 the possibility of a winolike lightest susy particle lsp as dark matt... | [['anomalymediated', 'supersymmetry', 'breaking', 'amsb', 'models', 'seem', 'to', 'have', 'become', 'increasingly', 'implausible', 'due', 'to', '1', 'difficulty', 'in', 'generating', 'a', 'higgs', 'mass', 'mh125', 'gev', '2', 'typically', 'unnatural', 'superparticle', 'spectra', 'characterized', 'by', 'a', 'large', 'su... | [-0.07500500636428363, 0.3036844998963243, -0.04450558059918592, 0.24525298806992543, -0.1545043709320693, -0.2564889582536606, 0.011232653832255907, 0.32067928456348505, -0.20788760433826875, -0.37354101396128864, 0.018237123978201153, -0.27321467049715276, 0.04731769170735179, 0.1182556215869591, 0.02001284289744063,... |
1,801.09731 | Broadband radio spectro-polarimetric observations of high Faraday
rotation measure AGN | We present broadband polarimetric observations of a sample of high Faraday
rotation measure (RM) AGN using the VLA telescope from 1 to 2 GHz, and 4 to 12
GHz. The sample (14 sources) consists of compact sources (linear resolution
smaller than ~ 5 kpc) that are unpolarized at 1.4 GHz in the NVSS. Total
intensity data ... | astro-ph.GA | we present broadband polarimetric observations of a sample of high faraday rotation measure rm agn using the vla telescope from 1 to 2 ghz and 4 to 12 ghz the sample 14 sources consists of compact sources linear resolution smaller than 5 kpc that are unpolarized at 14 ghz in the nvss total intensity data have been mode... | [['we', 'present', 'broadband', 'polarimetric', 'observations', 'of', 'a', 'sample', 'of', 'high', 'faraday', 'rotation', 'measure', 'rm', 'agn', 'using', 'the', 'vla', 'telescope', 'from', '1', 'to', '2', 'ghz', 'and', '4', 'to', '12', 'ghz', 'the', 'sample', '14', 'sources', 'consists', 'of', 'compact', 'sources', 'l... | [-0.09517203350571499, 0.11986979171357735, -0.049381546578209465, 0.0801900520907017, -0.094721371426793, -0.07689634587069781, 0.013488683087654926, 0.46809632943878915, -0.2353597880296955, -0.3550622645637085, 0.08845714612518726, -0.2618008782894447, -0.027514301242852778, 0.21266099779850578, 0.0172385158932543, ... |
1,801.09732 | Uncertain classification of Variable Stars: handling observational GAPS
and noise | Automatic classification methods applied to sky surveys have revolutionized
the astronomical target selection process. Most surveys generate a vast amount
of time series, or \quotes{lightcurves}, that represent the brightness
variability of stellar objects in time. Unfortunately, lightcurves'
observations take severa... | astro-ph.IM | automatic classification methods applied to sky surveys have revolutionized the astronomical target selection process most surveys generate a vast amount of time series or quoteslightcurves that represent the brightness variability of stellar objects in time unfortunately lightcurves observations take several years to ... | [['automatic', 'classification', 'methods', 'applied', 'to', 'sky', 'surveys', 'have', 'revolutionized', 'the', 'astronomical', 'target', 'selection', 'process', 'most', 'surveys', 'generate', 'a', 'vast', 'amount', 'of', 'time', 'series', 'or', 'quoteslightcurves', 'that', 'represent', 'the', 'brightness', 'variabilit... | [-0.037419164021638966, 0.06036983528661095, -0.10789690830420537, 0.06053542924102938, -0.10806610455231266, -0.08401652564848905, 0.08904114548778652, 0.412688638183556, -0.2278627730997445, -0.349189892488528, 0.11525713633943861, -0.293424541254147, -0.1357735667192954, 0.25253387017605394, -0.09415492080698763, 0.... |
1,801.09733 | Semi-Fredholm and semi-Browder spectrums for the ${\alpha}$-times
integrated semigroups | In this paper, we describe the different spectrums of the {\alpha}-times
integrated semigroups by the spectrums of their generators. Specially,
essential ascent and descent, upper and lower semi-Fredholm and semi-Browder
spectrums.
| math.FA math.SP | in this paper we describe the different spectrums of the alphatimes integrated semigroups by the spectrums of their generators specially essential ascent and descent upper and lower semifredholm and semibrowder spectrums | [['in', 'this', 'paper', 'we', 'describe', 'the', 'different', 'spectrums', 'of', 'the', 'alphatimes', 'integrated', 'semigroups', 'by', 'the', 'spectrums', 'of', 'their', 'generators', 'specially', 'essential', 'ascent', 'and', 'descent', 'upper', 'and', 'lower', 'semifredholm', 'and', 'semibrowder', 'spectrums']] | [-0.08695666810437556, 0.15666588299697445, -0.05542667671256969, 0.1674132434643745, -0.005576172753447487, -0.051437496703358426, -0.001277893507522681, 0.3990127168175194, -0.26436852705815145, -0.283667593593559, 0.14713603948738666, -0.2912238796031283, -0.14279563059549658, 0.2205898843465313, -0.0668053529675929... |
1,801.09734 | HFF-DeepSpace Photometric Catalogs of the Twelve Hubble Frontier Fields,
Clusters and Parallels: Photometry, Photometric Redshifts, and Stellar Masses | We present Hubble multi-wavelength photometric catalogs, including (up to) 17
filters with the Advanced Camera for Surveys and Wide Field Camera 3 from the
ultra-violet to near-infrared for the Hubble Frontier Fields and associated
parallels. We have constructed homogeneous photometric catalogs for all six
clusters a... | astro-ph.GA | we present hubble multiwavelength photometric catalogs including up to 17 filters with the advanced camera for surveys and wide field camera 3 from the ultraviolet to nearinfrared for the hubble frontier fields and associated parallels we have constructed homogeneous photometric catalogs for all six clusters and their ... | [['we', 'present', 'hubble', 'multiwavelength', 'photometric', 'catalogs', 'including', 'up', 'to', '17', 'filters', 'with', 'the', 'advanced', 'camera', 'for', 'surveys', 'and', 'wide', 'field', 'camera', '3', 'from', 'the', 'ultraviolet', 'to', 'nearinfrared', 'for', 'the', 'hubble', 'frontier', 'fields', 'and', 'ass... | [-0.013198605239926744, 0.07119092074566218, -0.09568583586174044, 0.09196495892940021, -0.15728301394576213, -0.057670365176295584, 0.0393397833589702, 0.48466110351657576, -0.180757576603959, -0.3862725568026576, 0.12454053700872346, -0.33964800214025415, -0.06762740345387097, 0.26905681243871415, -0.0449338871420093... |
1,801.09735 | On Bott-Morse Foliations and their Poisson Structures in Dimension 3 | We show that a Bott-Morse foliation in dimension 3 admits a linear, singular,
Poisson structure of rank 2 with Bott-Morse singularities. We provide the
Poisson bivectors for each type of singular component, and compute the
symplectic forms of the characteristic distribution.
| math.SG math.DG math.GT | we show that a bottmorse foliation in dimension 3 admits a linear singular poisson structure of rank 2 with bottmorse singularities we provide the poisson bivectors for each type of singular component and compute the symplectic forms of the characteristic distribution | [['we', 'show', 'that', 'a', 'bottmorse', 'foliation', 'in', 'dimension', '3', 'admits', 'a', 'linear', 'singular', 'poisson', 'structure', 'of', 'rank', '2', 'with', 'bottmorse', 'singularities', 'we', 'provide', 'the', 'poisson', 'bivectors', 'for', 'each', 'type', 'of', 'singular', 'component', 'and', 'compute', 'th... | [-0.20386979156514493, 0.017638821807894403, -0.12812924943864346, 0.07077795471541765, -0.10023938830396752, -0.16407776630778864, -0.0814201684396078, 0.31683017013639936, -0.3127449332940869, -0.12520026624566172, 0.07521749785022311, -0.25179763429048585, -0.21359743273294554, 0.12399212720735771, -0.05331918524532... |
1,801.09736 | Boundary elements with mesh refinements for the wave equation | The solution of the wave equation in a polyhedral domain in $\mathbb{R}^3$
admits an asymptotic singular expansion in a neighborhood of the corners and
edges. In this article we formulate boundary and screen problems for the wave
equation as equivalent boundary integral equations in time domain, study the
regularity ... | math.NA math.AP | the solution of the wave equation in a polyhedral domain in mathbbr3 admits an asymptotic singular expansion in a neighborhood of the corners and edges in this article we formulate boundary and screen problems for the wave equation as equivalent boundary integral equations in time domain study the regularity properties... | [['the', 'solution', 'of', 'the', 'wave', 'equation', 'in', 'a', 'polyhedral', 'domain', 'in', 'mathbbr3', 'admits', 'an', 'asymptotic', 'singular', 'expansion', 'in', 'a', 'neighborhood', 'of', 'the', 'corners', 'and', 'edges', 'in', 'this', 'article', 'we', 'formulate', 'boundary', 'and', 'screen', 'problems', 'for',... | [-0.12393831985323357, -0.00321354205523075, -0.08176416809106707, 0.0711326786101189, -0.11459079637713389, -0.08554899794211902, -0.023714123218995305, 0.324924331173352, -0.3265408442073732, -0.21196636434969143, 0.1827971868733918, -0.3165015730528383, -0.16563757609815224, 0.17983251133369743, -0.07101933734166786... |
1,801.09737 | Automatic Survey-Invariant Variable Star Classification | Machine learning techniques have been successfully used to classify variable
stars on widely-studied astronomical surveys. These datasets have been
available to astronomers long enough, thus allowing them to perform deep
analysis over several variable sources and generating useful catalogs with
identified variable st... | astro-ph.IM | machine learning techniques have been successfully used to classify variable stars on widelystudied astronomical surveys these datasets have been available to astronomers long enough thus allowing them to perform deep analysis over several variable sources and generating useful catalogs with identified variable stars t... | [['machine', 'learning', 'techniques', 'have', 'been', 'successfully', 'used', 'to', 'classify', 'variable', 'stars', 'on', 'widelystudied', 'astronomical', 'surveys', 'these', 'datasets', 'have', 'been', 'available', 'to', 'astronomers', 'long', 'enough', 'thus', 'allowing', 'them', 'to', 'perform', 'deep', 'analysis'... | [-0.010051062642615514, 0.0342764328738207, -0.09261418532519809, 0.08572238234299714, -0.18175351286970592, -0.15262617834048112, 0.0923116336565329, 0.4473490394380411, -0.2641144470247602, -0.3660958429067, 0.1406935412820376, -0.3109002273901755, -0.07018176410893952, 0.22089130163422752, -0.05745100938273888, 0.05... |
1,801.09738 | Photoevaporation Does Not Create a Pileup of Giant Planets at 1 AU | The semimajor axis distribution of giant exoplanets appears to have a pileup
near 1 AU. Photoevaporation opens a gap in the inner few AU of gaseous disks
before dissipating them. Here we investigate whether photoevaporation can
significantly affect the final distribution of giant planets by modifying gas
surface dens... | astro-ph.EP | the semimajor axis distribution of giant exoplanets appears to have a pileup near 1 au photoevaporation opens a gap in the inner few au of gaseous disks before dissipating them here we investigate whether photoevaporation can significantly affect the final distribution of giant planets by modifying gas surface density ... | [['the', 'semimajor', 'axis', 'distribution', 'of', 'giant', 'exoplanets', 'appears', 'to', 'have', 'a', 'pileup', 'near', '1', 'au', 'photoevaporation', 'opens', 'a', 'gap', 'in', 'the', 'inner', 'few', 'au', 'of', 'gaseous', 'disks', 'before', 'dissipating', 'them', 'here', 'we', 'investigate', 'whether', 'photoevapo... | [-0.1325916716261488, 0.16125890923788264, -0.07264977472424868, 0.05564092219906189, -0.07229591293062493, -0.05747864406177963, 0.06150064401773979, 0.3970425989971483, -0.22760028403155633, -0.3320284135378717, 0.057074878146592976, -0.22235579992720975, -0.07832573694435672, 0.14147777622678107, -0.0651239262025461... |
1,801.09739 | Model selection in sparse high-dimensional vine copula models with
application to portfolio risk | Vine copulas allow to build flexible dependence models for an arbitrary
number of variables using only bivariate building blocks. The number of
parameters in a vine copula model increases quadratically with the dimension,
which poses new challenges in high-dimensional applications. To alleviate the
computational burd... | stat.ME stat.CO | vine copulas allow to build flexible dependence models for an arbitrary number of variables using only bivariate building blocks the number of parameters in a vine copula model increases quadratically with the dimension which poses new challenges in highdimensional applications to alleviate the computational burden and... | [['vine', 'copulas', 'allow', 'to', 'build', 'flexible', 'dependence', 'models', 'for', 'an', 'arbitrary', 'number', 'of', 'variables', 'using', 'only', 'bivariate', 'building', 'blocks', 'the', 'number', 'of', 'parameters', 'in', 'a', 'vine', 'copula', 'model', 'increases', 'quadratically', 'with', 'the', 'dimension',... | [-0.012497658492928302, 0.011389783224741998, -0.1136828013419829, 0.16189309764239523, -0.16084430585270404, -0.22482608172145707, 0.06389473798141504, 0.38025758645359287, -0.2756365326129728, -0.30892266134765967, 0.10481520759942078, -0.1993264744506666, -0.1667578330229002, 0.16820607550821645, -0.1143050521094766... |
1,801.0974 | When does a disaster become a systemic event? Estimating indirect
economic losses from natural disasters | Reliable estimates of indirect economic losses arising from natural disasters
are currently out of scientific reach. To address this problem, we propose a
novel approach that combines a probabilistic physical damage catastrophe model
with a new generation of macroeconomic agent-based models (ABMs). The ABM moves
beyo... | q-fin.EC | reliable estimates of indirect economic losses arising from natural disasters are currently out of scientific reach to address this problem we propose a novel approach that combines a probabilistic physical damage catastrophe model with a new generation of macroeconomic agentbased models abms the abm moves beyond the s... | [['reliable', 'estimates', 'of', 'indirect', 'economic', 'losses', 'arising', 'from', 'natural', 'disasters', 'are', 'currently', 'out', 'of', 'scientific', 'reach', 'to', 'address', 'this', 'problem', 'we', 'propose', 'a', 'novel', 'approach', 'that', 'combines', 'a', 'probabilistic', 'physical', 'damage', 'catastroph... | [-0.09017387923318892, 0.09298087989963824, -0.06080573621322401, 0.15800513106118888, -0.0959707636386156, -0.10567918955534697, 0.09888250930886716, 0.33308077497780325, -0.26559713066741825, -0.3224600231591612, 0.12700963543122634, -0.30552566345850934, -0.15491333872452379, 0.17609013533685355, -0.1278906244114041... |
1,801.09741 | An Optimized Information-Preserving Relational Database Watermarking
Scheme for Ownership Protection of Medical Data | Recently, a significant amount of interest has been developed in motivating
physicians to use e-health technology (especially Electronic Medical Records
(EMR) systems). An important utility of such EMR systems is: a next generation
of Clinical Decision Support Systems (CDSS) will extract knowledge from these
electron... | cs.MM cs.CR | recently a significant amount of interest has been developed in motivating physicians to use ehealth technology especially electronic medical records emr systems an important utility of such emr systems is a next generation of clinical decision support systems cdss will extract knowledge from these electronic medical r... | [['recently', 'a', 'significant', 'amount', 'of', 'interest', 'has', 'been', 'developed', 'in', 'motivating', 'physicians', 'to', 'use', 'ehealth', 'technology', 'especially', 'electronic', 'medical', 'records', 'emr', 'systems', 'an', 'important', 'utility', 'of', 'such', 'emr', 'systems', 'is', 'a', 'next', 'generati... | [-0.09526270298159671, 0.014831583605672388, -0.06307819664140242, 0.09453450591480568, -0.08338956834890902, -0.17715715843143465, 0.0750827201500409, 0.4093825093576572, -0.24572270944568717, -0.31419844252763324, 0.16365956852553923, -0.2890542058416665, -0.16616160355282955, 0.23315106565728277, -0.1827436547139758... |
1,801.09742 | Microtransformers: controlled microscale navigation with flexible robots | Artificial microswimmers are a new technology with promising microfluidics
and biomedical applications, such as directed cargo transport, microscale
assembly, and targeted drug delivery. A fundamental barrier to realising this
potential is the ability to control the trajectories of multiple individuals
within a large... | physics.flu-dyn | artificial microswimmers are a new technology with promising microfluidics and biomedical applications such as directed cargo transport microscale assembly and targeted drug delivery a fundamental barrier to realising this potential is the ability to control the trajectories of multiple individuals within a large group... | [['artificial', 'microswimmers', 'are', 'a', 'new', 'technology', 'with', 'promising', 'microfluidics', 'and', 'biomedical', 'applications', 'such', 'as', 'directed', 'cargo', 'transport', 'microscale', 'assembly', 'and', 'targeted', 'drug', 'delivery', 'a', 'fundamental', 'barrier', 'to', 'realising', 'this', 'potenti... | [-0.12671123252382122, 0.2086578416246591, -0.05161674938420147, -0.011270714036716494, -0.13510777269679625, -0.19248539705933854, 0.013895619455601327, 0.42501509235759755, -0.2861386747305504, -0.33127810852190037, 0.05057818139748714, -0.21258463825107413, -0.22934857155278787, 0.21219660846961547, -0.1087850582944... |
1,801.09743 | Quasi-Fredholm, Saphar Spectra for Integrated Semigroup | In this paper, we show a spectral inclusion of integrated semigroups for
Saphar, essentially Saphar and quasi-Fredholm spectra.
| math.FA math.SP | in this paper we show a spectral inclusion of integrated semigroups for saphar essentially saphar and quasifredholm spectra | [['in', 'this', 'paper', 'we', 'show', 'a', 'spectral', 'inclusion', 'of', 'integrated', 'semigroups', 'for', 'saphar', 'essentially', 'saphar', 'and', 'quasifredholm', 'spectra']] | [-0.025252479335500136, 0.05177279760957592, -0.08376806722016125, 0.08233103339120539, 0.0235257050436404, -0.010238229271231426, -0.02996803710832157, 0.42298617131180233, -0.2626810347040494, -0.23920583455926842, 0.09225200830001591, -0.3199712426091234, -0.12167348278065522, 0.2061831145029929, -0.0936986795212659... |
1,801.09744 | Compressive Sensing: Performance Comparison Of Sparse Recovery
Algorithms | Spectrum sensing is an important process in cognitive radio. A number of
sensing techniques that have been proposed suffer from high processing time,
hardware cost and computational complexity. To address these problems,
compressive sensing has been proposed to decrease the processing time and
expedite the scanning p... | eess.SP | spectrum sensing is an important process in cognitive radio a number of sensing techniques that have been proposed suffer from high processing time hardware cost and computational complexity to address these problems compressive sensing has been proposed to decrease the processing time and expedite the scanning process... | [['spectrum', 'sensing', 'is', 'an', 'important', 'process', 'in', 'cognitive', 'radio', 'a', 'number', 'of', 'sensing', 'techniques', 'that', 'have', 'been', 'proposed', 'suffer', 'from', 'high', 'processing', 'time', 'hardware', 'cost', 'and', 'computational', 'complexity', 'to', 'address', 'these', 'problems', 'comp... | [-0.09996889177209779, -0.0011985355489277875, -0.08134698197901899, 0.050482241590879426, -0.06287565546097772, -0.16881434006253945, 0.03397602293462236, 0.46864452585577965, -0.30789765795605295, -0.3114761274007943, 0.18843808424059028, -0.20295646144139687, -0.1931669508675801, 0.19131976072895246, -0.146709629725... |
1,801.09745 | The spectrum of the Schr\"{o}dinger Hamiltonian for trapped particles in
a cylinder with a topological defect perturbed by two attractive delta
interactions | In this paper we exploit the technique used in \cite{A}-\cite{5b} to deal
with delta interactions in a rigorous way in a curved spacetime represented by
a cosmic string along the $z$ axis. This mathematical machinery is applied in
order to study the discrete spectrum of a point-mass particle confined in an
infinitely... | math-ph hep-th math.MP | in this paper we exploit the technique used in citeacite5b to deal with delta interactions in a rigorous way in a curved spacetime represented by a cosmic string along the z axis this mathematical machinery is applied in order to study the discrete spectrum of a pointmass particle confined in an infinitely long cylinde... | [['in', 'this', 'paper', 'we', 'exploit', 'the', 'technique', 'used', 'in', 'citeacite5b', 'to', 'deal', 'with', 'delta', 'interactions', 'in', 'a', 'rigorous', 'way', 'in', 'a', 'curved', 'spacetime', 'represented', 'by', 'a', 'cosmic', 'string', 'along', 'the', 'z', 'axis', 'this', 'mathematical', 'machinery', 'is', ... | [-0.14894693736558812, 0.14730475321649514, -0.055847614037287586, 0.04484659380212083, -0.006007154860223333, -0.12781502155325652, 0.03891653551315693, 0.3359490096070722, -0.26146690248360593, -0.29748512641628877, 0.04328514786953874, -0.28889418523881194, -0.11930199626275632, 0.1443586577227331, -0.00826636197151... |
1,801.09746 | A Corpus for Modeling Word Importance in Spoken Dialogue Transcripts | Motivated by a project to create a system for people who are deaf or
hard-of-hearing that would use automatic speech recognition (ASR) to produce
real-time text captions of spoken English during in-person meetings with
hearing individuals, we have augmented a transcript of the Switchboard
conversational dialogue corp... | cs.CL | motivated by a project to create a system for people who are deaf or hardofhearing that would use automatic speech recognition asr to produce realtime text captions of spoken english during inperson meetings with hearing individuals we have augmented a transcript of the switchboard conversational dialogue corpus with a... | [['motivated', 'by', 'a', 'project', 'to', 'create', 'a', 'system', 'for', 'people', 'who', 'are', 'deaf', 'or', 'hardofhearing', 'that', 'would', 'use', 'automatic', 'speech', 'recognition', 'asr', 'to', 'produce', 'realtime', 'text', 'captions', 'of', 'spoken', 'english', 'during', 'inperson', 'meetings', 'with', 'he... | [-0.0753482352096277, -0.0037978154035711973, -0.023591782671088975, 0.06835756922839209, -0.15115842676372268, -0.1789445923237751, 0.1031123226787895, 0.4676102777260045, -0.19582830674946308, -0.3409565557683042, -0.008262780371587723, -0.35147458987155306, -0.13983999103036088, 0.22181467356315504, -0.1892658603012... |
1,801.09747 | Distributed Model Construction in Radio Interferometric Calibration | Calibration of a typical radio interferometric array yields thousands of
parameters as solutions. These solutions contain valuable information about the
systematic errors in the data (ionosphere and beam shape). This information
could be reused in calibration to improve the accuracy and also can be fed into
imaging t... | astro-ph.IM cs.DC | calibration of a typical radio interferometric array yields thousands of parameters as solutions these solutions contain valuable information about the systematic errors in the data ionosphere and beam shape this information could be reused in calibration to improve the accuracy and also can be fed into imaging to impr... | [['calibration', 'of', 'a', 'typical', 'radio', 'interferometric', 'array', 'yields', 'thousands', 'of', 'parameters', 'as', 'solutions', 'these', 'solutions', 'contain', 'valuable', 'information', 'about', 'the', 'systematic', 'errors', 'in', 'the', 'data', 'ionosphere', 'and', 'beam', 'shape', 'this', 'information', ... | [-0.10240034647115054, -0.014213183410802147, -0.09917225868979451, 0.056308790893986, -0.09475589159090038, -0.1237324787081655, 0.04352468374364693, 0.4234697277392816, -0.32405145326202067, -0.36107175370011857, 0.1528198488597083, -0.23249352132952814, -0.10333758958299226, 0.22098889464828606, -0.10438602158816856... |
1,801.09748 | Stability of Periodic Travelling Flexural-Gravity Waves in Two
Dimensions | In this work, we solve the Euler's equations for periodic waves travelling
under a sheet of ice using a reformulation introduced in Ablowitz et al.
(2006). These waves are referred to as flexural-gravity waves. We compare and
contrast two models for the effect of the ice: a linear model and a nonlinear
model. The ben... | math.AP | in this work we solve the eulers equations for periodic waves travelling under a sheet of ice using a reformulation introduced in ablowitz et al 2006 these waves are referred to as flexuralgravity waves we compare and contrast two models for the effect of the ice a linear model and a nonlinear model the benefit of this... | [['in', 'this', 'work', 'we', 'solve', 'the', 'eulers', 'equations', 'for', 'periodic', 'waves', 'travelling', 'under', 'a', 'sheet', 'of', 'ice', 'using', 'a', 'reformulation', 'introduced', 'in', 'ablowitz', 'et', 'al', '2006', 'these', 'waves', 'are', 'referred', 'to', 'as', 'flexuralgravity', 'waves', 'we', 'compar... | [-0.13133165627071747, 0.09353511313572019, -0.08835131116211414, 0.07688409952149049, -0.07133421836560275, -0.0856871964777408, -0.0036574618314348514, 0.31429382251436205, -0.2685817307246165, -0.25899073598133465, 0.12334078279415742, -0.2619283015801742, -0.22391125446400878, 0.21105024081553478, -0.00718614104545... |
1,801.09749 | Deep Learning based Retinal OCT Segmentation | Our objective is to evaluate the efficacy of methods that use deep learning
(DL) for the automatic fine-grained segmentation of optical coherence
tomography (OCT) images of the retina. OCT images from 10 patients with mild
non-proliferative diabetic retinopathy were used from a public (U. of Miami)
dataset. For each ... | cs.CV | our objective is to evaluate the efficacy of methods that use deep learning dl for the automatic finegrained segmentation of optical coherence tomography oct images of the retina oct images from 10 patients with mild nonproliferative diabetic retinopathy were used from a public u of miami dataset for each patient five ... | [['our', 'objective', 'is', 'to', 'evaluate', 'the', 'efficacy', 'of', 'methods', 'that', 'use', 'deep', 'learning', 'dl', 'for', 'the', 'automatic', 'finegrained', 'segmentation', 'of', 'optical', 'coherence', 'tomography', 'oct', 'images', 'of', 'the', 'retina', 'oct', 'images', 'from', '10', 'patients', 'with', 'mil... | [0.008976682673646468, -0.027895406801474423, -0.01708591355677149, 0.0695222328583473, -0.04984489373592181, -0.15720353945500765, 0.019389830826019697, 0.4536905844692185, -0.21014302834986226, -0.3505187111155759, 0.10289419160487698, -0.31451371929832833, -0.14587575504501082, 0.2116668534395193, -0.167800778820797... |
1,801.0975 | Nucleon Resonance Structure from Exclusive Meson Electroproduction with
CLAS | Studies of the nucleon resonance electroexcitation amplitudes in a wide range
of photon virtualities offer unique information on many facets of strong QCD
behind the generation of all prominent excited nucleon states. Advances in the
evaluation of resonance electroexcitation amplitudes from the data measured
with the... | nucl-ex hep-ph | studies of the nucleon resonance electroexcitation amplitudes in a wide range of photon virtualities offer unique information on many facets of strong qcd behind the generation of all prominent excited nucleon states advances in the evaluation of resonance electroexcitation amplitudes from the data measured with the cl... | [['studies', 'of', 'the', 'nucleon', 'resonance', 'electroexcitation', 'amplitudes', 'in', 'a', 'wide', 'range', 'of', 'photon', 'virtualities', 'offer', 'unique', 'information', 'on', 'many', 'facets', 'of', 'strong', 'qcd', 'behind', 'the', 'generation', 'of', 'all', 'prominent', 'excited', 'nucleon', 'states', 'adva... | [-0.09464547646699423, 0.22169709319964728, -0.09500652693976659, 0.08104307920552413, -0.05258528508811262, -0.07243375813815894, 0.05128624510375152, 0.34117007789705744, -0.168178926393252, -0.28449752788034044, -0.02782944446417833, -0.32458135550877926, -0.022395248455086048, 0.16006637893432338, 0.114767555522475... |
1,801.09751 | Neutrino conversion in a neutrino flux: Towards an effective theory of
collective oscillations | Collective oscillations of supernova neutrinos above the neutrino sphere can
be completely described by the propagation of individual neutrinos in external
potentials and are in this sense a linear phenomenon. An effective theory of
collective oscillations can be developed based on certain assumptions about
time depe... | hep-ph astro-ph.HE | collective oscillations of supernova neutrinos above the neutrino sphere can be completely described by the propagation of individual neutrinos in external potentials and are in this sense a linear phenomenon an effective theory of collective oscillations can be developed based on certain assumptions about time depende... | [['collective', 'oscillations', 'of', 'supernova', 'neutrinos', 'above', 'the', 'neutrino', 'sphere', 'can', 'be', 'completely', 'described', 'by', 'the', 'propagation', 'of', 'individual', 'neutrinos', 'in', 'external', 'potentials', 'and', 'are', 'in', 'this', 'sense', 'a', 'linear', 'phenomenon', 'an', 'effective', ... | [-0.1521444036149414, 0.26328336082791703, -0.047584913965715854, 0.1702975614066675, -0.04923137770116376, -0.11177954559782578, 0.023752835414477817, 0.3753091902149923, -0.2633218828137706, -0.2767619002001278, 0.04891103579525092, -0.2680702757840074, -0.11925713106720422, 0.17561616187142032, 0.025674355520907813,... |
1,801.09752 | Problem of Descent Spectrum Equality | Let $\mathcal{B}(X)$ be the algebra of all bounded operators acting on an
infinite dimensional complex Banach space $X$. We say that an operator $T \in
\mathcal{B}(X)$ satisfies the problem of descent spectrum equality, if the
descent spectrum of $T$ as an operator coincides with the descent spectrum of
$T$ as an ele... | math.SP | let mathcalbx be the algebra of all bounded operators acting on an infinite dimensional complex banach space x we say that an operator t in mathcalbx satisfies the problem of descent spectrum equality if the descent spectrum of t as an operator coincides with the descent spectrum of t as an element of the algebra of al... | [['let', 'mathcalbx', 'be', 'the', 'algebra', 'of', 'all', 'bounded', 'operators', 'acting', 'on', 'an', 'infinite', 'dimensional', 'complex', 'banach', 'space', 'x', 'we', 'say', 'that', 'an', 'operator', 't', 'in', 'mathcalbx', 'satisfies', 'the', 'problem', 'of', 'descent', 'spectrum', 'equality', 'if', 'the', 'desc... | [-0.15217604060821674, 0.13558191625577143, -0.054195021018933726, 0.0007051884689751794, -0.056388431361091194, -0.1439351971973391, -0.04146916921337263, 0.3542696219553952, -0.3834246311008054, -0.15353635226589782, 0.12672548256723173, -0.3266236763904054, -0.09124586740326063, 0.17452501267304316, -0.1345887848258... |
1,801.09753 | Resource Allocation for Containing Epidemics from Temporal Network Data | We study the problem of containing epidemic spreading processes in temporal
networks. We specifically focus on the problem of finding a resource allocation
to suppress epidemic infection, provided that an empirical time-series data of
connectivities between nodes is available. Although this problem is of
practical re... | cs.SI physics.soc-ph | we study the problem of containing epidemic spreading processes in temporal networks we specifically focus on the problem of finding a resource allocation to suppress epidemic infection provided that an empirical timeseries data of connectivities between nodes is available although this problem is of practical relevanc... | [['we', 'study', 'the', 'problem', 'of', 'containing', 'epidemic', 'spreading', 'processes', 'in', 'temporal', 'networks', 'we', 'specifically', 'focus', 'on', 'the', 'problem', 'of', 'finding', 'a', 'resource', 'allocation', 'to', 'suppress', 'epidemic', 'infection', 'provided', 'that', 'an', 'empirical', 'timeseries'... | [-0.132070051359811, -0.0005772818160559317, -0.11138406536275787, 0.06428327061917766, -0.10795983468747831, -0.14694910465872713, 0.1057057274023204, 0.4098261322052817, -0.26938543135578846, -0.29160748154057986, 0.10577058206378881, -0.25534805387235665, -0.1913277271802404, 0.18997579752467572, -0.1123262239337366... |
1,801.09754 | Total density profile of massive early-type galaxies in Horizon-AGN
simulation: impact of AGN feedback and comparison with observations | Using the two large cosmological hydrodynamical simulations, Horizon-AGN
(H-AGN) and Horizon-noAGN (H-noAGN, no AGN feedback), we investigate how a
typical sub-grid model for AGN feedback affects the evolution of the total
density profiles (dark matter + stars) at the effective radius of massive
early-type galaxies (... | astro-ph.GA | using the two large cosmological hydrodynamical simulations horizonagn hagn and horizonnoagn hnoagn no agn feedback we investigate how a typical subgrid model for agn feedback affects the evolution of the total density profiles dark matter stars at the effective radius of massive earlytype galaxies m1011 msun we have s... | [['using', 'the', 'two', 'large', 'cosmological', 'hydrodynamical', 'simulations', 'horizonagn', 'hagn', 'and', 'horizonnoagn', 'hnoagn', 'no', 'agn', 'feedback', 'we', 'investigate', 'how', 'a', 'typical', 'subgrid', 'model', 'for', 'agn', 'feedback', 'affects', 'the', 'evolution', 'of', 'the', 'total', 'density', 'pr... | [-0.05595653777043173, 0.10694825154525316, -0.09801488433181499, 0.17919876502099358, -0.08201897114547739, -0.06766829574109977, 0.030640773390030573, 0.4188284228616093, -0.08635446188776795, -0.38572611737143786, 0.02788957583356593, -0.31851042587940226, -0.01894561095112258, 0.18433054910152594, 0.011527702794989... |
1,801.09755 | Optonanofluidics: Modelling fluid flow through surfactant-modified
liquid tethers by laser beams | When a surfactant-stabilised oil droplet with an ultralow interfacial tension
is trapped in the focus of two laser beams and pulled apart (by moving the
laser beams) a configuration of two droplets connected by a thin tether of oil
results. The tether radius depends on the ratio of the bending modulus to the
renormal... | cond-mat.soft | when a surfactantstabilised oil droplet with an ultralow interfacial tension is trapped in the focus of two laser beams and pulled apart by moving the laser beams a configuration of two droplets connected by a thin tether of oil results the tether radius depends on the ratio of the bending modulus to the renormalized i... | [['when', 'a', 'surfactantstabilised', 'oil', 'droplet', 'with', 'an', 'ultralow', 'interfacial', 'tension', 'is', 'trapped', 'in', 'the', 'focus', 'of', 'two', 'laser', 'beams', 'and', 'pulled', 'apart', 'by', 'moving', 'the', 'laser', 'beams', 'a', 'configuration', 'of', 'two', 'droplets', 'connected', 'by', 'a', 'th... | [-0.15782843432086416, 0.23315151757782537, -0.10056851356971024, -0.06946092152304012, -0.014570512608395297, -0.12293251526788411, 0.010150033138946092, 0.37705139554786443, -0.29800858783155615, -0.2762835511716914, 0.08702938253740726, -0.27581113345520114, -0.050175319024833596, 0.21130109218266613, -0.03986491105... |
1,801.09756 | Counterexamples in Calculus of Variations in $L^\infty$ through the
vectorial Eikonal equation | We show that for any regular bounded domain $\Omega\subseteq \mathbb R^n$,
$n=2,3$, there exist infinitely many global diffeomorphisms equal to the
identity on $\partial \Omega$ which solve the Eikonal equation. We also provide
explicit examples of such maps on annular domains. This implies that the
$\infty$-Laplace ... | math.AP | we show that for any regular bounded domain omegasubseteq mathbb rn n23 there exist infinitely many global diffeomorphisms equal to the identity on partial omega which solve the eikonal equation we also provide explicit examples of such maps on annular domains this implies that the inftylaplace system arising in vector... | [['we', 'show', 'that', 'for', 'any', 'regular', 'bounded', 'domain', 'omegasubseteq', 'mathbb', 'rn', 'n23', 'there', 'exist', 'infinitely', 'many', 'global', 'diffeomorphisms', 'equal', 'to', 'the', 'identity', 'on', 'partial', 'omega', 'which', 'solve', 'the', 'eikonal', 'equation', 'we', 'also', 'provide', 'explici... | [-0.15444254831067825, 0.0351167630257183, -0.02743776091129372, 0.09272740645744641, -0.09023441778691976, -0.13117573461740425, -0.02677296381443739, 0.3551971418292899, -0.3182972034341411, -0.16130865179002285, 0.15394157352765384, -0.31684947097796556, -0.12735379996133575, 0.169760705690255, -0.12271212426774007,... |
1,801.09757 | Cloud Atlas: Rotational Modulations in the L/T Transition Brown Dwarf
Companion HN Peg B | Time-resolved observations of brown dwarfs' rotational modulations provide
powerful insights into the properties of condensate clouds in ultra-cool
atmospheres. Multi-wavelength light curves reveal cloud vertical structures,
condensate particle sizes, and cloud morphology, which directly constrain
condensate cloud an... | astro-ph.EP astro-ph.SR | timeresolved observations of brown dwarfs rotational modulations provide powerful insights into the properties of condensate clouds in ultracool atmospheres multiwavelength light curves reveal cloud vertical structures condensate particle sizes and cloud morphology which directly constrain condensate cloud and atmosphe... | [['timeresolved', 'observations', 'of', 'brown', 'dwarfs', 'rotational', 'modulations', 'provide', 'powerful', 'insights', 'into', 'the', 'properties', 'of', 'condensate', 'clouds', 'in', 'ultracool', 'atmospheres', 'multiwavelength', 'light', 'curves', 'reveal', 'cloud', 'vertical', 'structures', 'condensate', 'partic... | [-0.1095851186852418, 0.14400522248624012, -0.12595183993835235, 0.08536376349895197, -0.13987953263197347, -0.138021760255056, 0.0724202356650494, 0.43249107199318876, -0.18122524363893303, -0.33376285593311134, 0.05316423649029192, -0.2627067960407162, -0.08692660894964567, 0.20084712096749255, -0.0638824211041951, -... |
1,801.09758 | Design principles and optimal performance for molecular motors under
realistic constraints | The performance of a molecular motor, characterized by its power output and
energy efficiency, is investigated in the motor design space spanned by the
stepping rate function and the motor-track interaction potential. Analytic
results and simulations show that a gating mechanism that restricts forward
stepping in a n... | cond-mat.soft physics.bio-ph q-bio.SC | the performance of a molecular motor characterized by its power output and energy efficiency is investigated in the motor design space spanned by the stepping rate function and the motortrack interaction potential analytic results and simulations show that a gating mechanism that restricts forward stepping in a narrow ... | [['the', 'performance', 'of', 'a', 'molecular', 'motor', 'characterized', 'by', 'its', 'power', 'output', 'and', 'energy', 'efficiency', 'is', 'investigated', 'in', 'the', 'motor', 'design', 'space', 'spanned', 'by', 'the', 'stepping', 'rate', 'function', 'and', 'the', 'motortrack', 'interaction', 'potential', 'analyti... | [-0.1410710262710747, 0.1193026393687517, -0.04456694234677437, 0.052327458193458465, -0.05525219781305065, -0.15103767369873822, 0.10546721406545029, 0.36905767941924256, -0.2584821343369129, -0.3128142720616432, 0.04943649799169339, -0.24964640931389534, -0.12578395970907427, 0.2319966713062574, -0.04317788160994131,... |
1,801.09759 | Radio-frequency capacitive gate-based sensing | Developing fast, accurate and scalable techniques for quantum state readout
is an active area in semiconductor-based quantum computing. Here, we present
results on dispersive sensing of silicon corner state quantum dots coupled to
lumped-element electrical resonators via the gate. The gate capacitance of the
quantum ... | physics.app-ph quant-ph | developing fast accurate and scalable techniques for quantum state readout is an active area in semiconductorbased quantum computing here we present results on dispersive sensing of silicon corner state quantum dots coupled to lumpedelement electrical resonators via the gate the gate capacitance of the quantum device i... | [['developing', 'fast', 'accurate', 'and', 'scalable', 'techniques', 'for', 'quantum', 'state', 'readout', 'is', 'an', 'active', 'area', 'in', 'semiconductorbased', 'quantum', 'computing', 'here', 'we', 'present', 'results', 'on', 'dispersive', 'sensing', 'of', 'silicon', 'corner', 'state', 'quantum', 'dots', 'coupled'... | [-0.16597136342563004, 0.11569746032036027, 0.0178854795769125, -0.09745803347239337, -0.012388526328015242, -0.2541936210477256, 0.10434717871918739, 0.43926233072637866, -0.1625224628348386, -0.3085970862654688, 0.0638588270098775, -0.28195663479243893, -0.07112842105059355, 0.3101192273186158, -0.003780919602040282,... |
1,801.0976 | Laboratory and On-Sky Validation of the Shaped Pupil Coronagraph's
Sensitivity to Low-Order Aberrations With Active Wavefront Control | We present early laboratory simulations and extensive on-sky tests validating
of the performance of a shaped pupil coronagraph (SPC) behind an extreme-AO
corrected beam of the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO)
system. In tests with the SCExAO internal source/wavefront error simulator, the
normaliz... | astro-ph.IM astro-ph.EP | we present early laboratory simulations and extensive onsky tests validating of the performance of a shaped pupil coronagraph spc behind an extremeao corrected beam of the subaru coronagraphic extreme adaptive optics scexao system in tests with the scexao internal sourcewavefront error simulator the normalized intensit... | [['we', 'present', 'early', 'laboratory', 'simulations', 'and', 'extensive', 'onsky', 'tests', 'validating', 'of', 'the', 'performance', 'of', 'a', 'shaped', 'pupil', 'coronagraph', 'spc', 'behind', 'an', 'extremeao', 'corrected', 'beam', 'of', 'the', 'subaru', 'coronagraphic', 'extreme', 'adaptive', 'optics', 'scexao'... | [-0.09509111422448768, 0.08799688464153275, -0.04938088602419677, 0.03985702624631813, -0.06998198164593694, -0.17420982214950656, 0.012426030980922015, 0.4255290345155767, -0.15157615978137723, -0.36028622278245165, 0.15394187102210707, -0.25679638044509506, -0.11873113646818508, 0.25458957399906856, -0.13907716434748... |
1,801.09761 | Degradation Kinetics of Inverted Perovskite Solar Cells | We explore the degradation behaviour under continuous illumination and direct
oxygen exposure of inverted unencapsulated
formamidinium(FA)0.83Cs0.17Pb(I0.8Br0.2)3, CH3NH3PbI3, and CH3NH3PbI3-xClx
perovskite solar cells. We continuously test the devices in-situ and
in-operando with current-voltage sweeps, transient ph... | physics.app-ph cond-mat.mtrl-sci | we explore the degradation behaviour under continuous illumination and direct oxygen exposure of inverted unencapsulated formamidiniumfa083cs017pbi08br023 ch3nh3pbi3 and ch3nh3pbi3xclx perovskite solar cells we continuously test the devices insitu and inoperando with currentvoltage sweeps transient photocurrent and tra... | [['we', 'explore', 'the', 'degradation', 'behaviour', 'under', 'continuous', 'illumination', 'and', 'direct', 'oxygen', 'exposure', 'of', 'inverted', 'unencapsulated', 'formamidiniumfa083cs017pbi08br023', 'ch3nh3pbi3', 'and', 'ch3nh3pbi3xclx', 'perovskite', 'solar', 'cells', 'we', 'continuously', 'test', 'the', 'device... | [-0.09432490751476444, 0.1967987362817251, 0.04648500788105844, 0.012450984578804466, 0.025671272875805354, -0.12831104464893198, 0.15011773717485305, 0.458062247726424, -0.24097053232956037, -0.30406379392611443, 0.05512516577989023, -0.28343369362972165, -0.16304427100514093, 0.2515996968100682, -0.13255734951034637,... |
1,801.09762 | The Kinetics of Dissolution of an Amorphous Solid | The kinetics of dissolution of an amorphous solid is studied using a simple
model of a glass that captures with reasonable accuracy the dynamic
heterogeneities associated with the relaxation of an amorphous material at low
temperatures. The intrinsic dissolution rate is shown to be proportional to the
concentration o... | cond-mat.soft | the kinetics of dissolution of an amorphous solid is studied using a simple model of a glass that captures with reasonable accuracy the dynamic heterogeneities associated with the relaxation of an amorphous material at low temperatures the intrinsic dissolution rate is shown to be proportional to the concentration of s... | [['the', 'kinetics', 'of', 'dissolution', 'of', 'an', 'amorphous', 'solid', 'is', 'studied', 'using', 'a', 'simple', 'model', 'of', 'a', 'glass', 'that', 'captures', 'with', 'reasonable', 'accuracy', 'the', 'dynamic', 'heterogeneities', 'associated', 'with', 'the', 'relaxation', 'of', 'an', 'amorphous', 'material', 'at... | [-0.05838881013784139, 0.2110045834505287, -0.1188461989677103, -0.01432917724897185, -0.00865300245886522, -0.09641340765264932, 0.005426995194611255, 0.3824137967456593, -0.28816231749323984, -0.29062797855376526, 0.0764032012646955, -0.2563215282777052, -0.10168742668668457, 0.10496437598250052, -0.03424591584696194... |
1,801.09763 | Battery-like Supercapacitors from Vertically Aligned Carbon Nanofibers
Coated Diamond: Design and Demonstrator | Battery-like supercapacitors feature high power and energy densities as well
as long-term capacitance retention. The utilized capacitor electrodes are thus
better to have large surface areas, high conductivity, high stability, and
importantly be of binder free. Herein, vertically aligned carbon nanofibers
(CNFs) coat... | physics.app-ph cond-mat.mtrl-sci | batterylike supercapacitors feature high power and energy densities as well as longterm capacitance retention the utilized capacitor electrodes are thus better to have large surface areas high conductivity high stability and importantly be of binder free herein vertically aligned carbon nanofibers cnfs coated borondope... | [['batterylike', 'supercapacitors', 'feature', 'high', 'power', 'and', 'energy', 'densities', 'as', 'well', 'as', 'longterm', 'capacitance', 'retention', 'the', 'utilized', 'capacitor', 'electrodes', 'are', 'thus', 'better', 'to', 'have', 'large', 'surface', 'areas', 'high', 'conductivity', 'high', 'stability', 'and', ... | [-0.10886181247638757, 0.1486593013595756, 0.05462014986630026, -0.06040932004773142, 0.013088430672347008, -0.23742932775519318, 0.07737702928244362, 0.43944958338161577, -0.2022416068236805, -0.3762159197557684, 0.07169179878090634, -0.33126991550094104, -0.012787165649881301, 0.20216283553462425, -0.0626782258817305... |
1,801.09764 | Essential Descent Spectrum Equality | A bounded operator $T$ in a Banach space $X$ is said to satisfy the essential
descent spectrum equality, if the descent spectrum of $T$ as an operator on $X$
coincides with the essential descent spectrum of $T$. In this note, we give
some conditions under which the equality $\sigma_{desc}(T) =
\sigma^e_{desc}(T)$ hol... | math.SP | a bounded operator t in a banach space x is said to satisfy the essential descent spectrum equality if the descent spectrum of t as an operator on x coincides with the essential descent spectrum of t in this note we give some conditions under which the equality sigma_desct sigmae_desct holds for a single operator t | [['a', 'bounded', 'operator', 't', 'in', 'a', 'banach', 'space', 'x', 'is', 'said', 'to', 'satisfy', 'the', 'essential', 'descent', 'spectrum', 'equality', 'if', 'the', 'descent', 'spectrum', 'of', 't', 'as', 'an', 'operator', 'on', 'x', 'coincides', 'with', 'the', 'essential', 'descent', 'spectrum', 'of', 't', 'in', '... | [-0.17139534384909053, 0.12519306545733275, -0.11741814962415784, 0.07780131263037522, -0.034459217222993846, -0.18465219135396183, -0.01011691459765037, 0.3674303625054933, -0.35259447574477504, -0.1584328870392508, 0.09524197017998193, -0.27035591649581436, -0.0883564784846924, 0.17721096709094666, -0.118884964518387... |
1,801.09765 | Enhancing silicon solar cells with singlet fission: the case for
Foerster resonant energy transfer using a quantum dot intermediate | One way for solar cell efficiencies to overcome the Shockley-Queisser limit
is downconversion of high-energy photons using singlet fission (SF) in
polyacenes like tetracene (Tc). SF enables generation of multiple excitons from
the high-energy photons which can be harvested in combination with Si. In this
work we inve... | physics.app-ph cond-mat.mtrl-sci physics.optics | one way for solar cell efficiencies to overcome the shockleyqueisser limit is downconversion of highenergy photons using singlet fission sf in polyacenes like tetracene tc sf enables generation of multiple excitons from the highenergy photons which can be harvested in combination with si in this work we investigate the... | [['one', 'way', 'for', 'solar', 'cell', 'efficiencies', 'to', 'overcome', 'the', 'shockleyqueisser', 'limit', 'is', 'downconversion', 'of', 'highenergy', 'photons', 'using', 'singlet', 'fission', 'sf', 'in', 'polyacenes', 'like', 'tetracene', 'tc', 'sf', 'enables', 'generation', 'of', 'multiple', 'excitons', 'from', 't... | [-0.04297098108297027, 0.14970254620202833, -0.0136226637996195, 0.057903798737307034, 0.029101274204417014, -0.2012791216523204, 0.0793286369020709, 0.4385245696702345, -0.28231039585314, -0.33280325402042377, -0.044210801663897445, -0.3012808506534553, -0.08565697994787508, 0.2147237490558407, -0.013229809544662284, ... |
1,801.09766 | Couniversal spaces which are equivariant commutative ring spectra | The note identifies which which couniversal spaces have suspension spectra
equivalent to commutative orthogonal ring G-spectra for a compact Lie group G.
These are precisely those whose cofamily is closed under passage to finite
index subgroups. Equivalently these are the couniversal spaces admitting an
action of an ... | math.AT | the note identifies which which couniversal spaces have suspension spectra equivalent to commutative orthogonal ring gspectra for a compact lie group g these are precisely those whose cofamily is closed under passage to finite index subgroups equivalently these are the couniversal spaces admitting an action of an equiv... | [['the', 'note', 'identifies', 'which', 'which', 'couniversal', 'spaces', 'have', 'suspension', 'spectra', 'equivalent', 'to', 'commutative', 'orthogonal', 'ring', 'gspectra', 'for', 'a', 'compact', 'lie', 'group', 'g', 'these', 'are', 'precisely', 'those', 'whose', 'cofamily', 'is', 'closed', 'under', 'passage', 'to',... | [-0.18744382679462432, 0.13596180727297905, -0.1292485449463129, 0.06773902480723336, -0.1344848014973104, -0.14664887904189527, -0.09183057880727574, 0.4597067092731595, -0.3691811902821064, -0.16264188916422426, 0.12761952763423323, -0.23010347853414714, -0.07823657239787281, 0.18318711832165718, -0.2050087714381516,... |
1,801.09767 | What Is the Fractional Laplacian? | The fractional Laplacian in R^d has multiple equivalent characterizations.
Moreover, in bounded domains, boundary conditions must be incorporated in these
characterizations in mathematically distinct ways, and there is currently no
consensus in the literature as to which definition of the fractional Laplacian
in boun... | math.NA cs.NA | the fractional laplacian in rd has multiple equivalent characterizations moreover in bounded domains boundary conditions must be incorporated in these characterizations in mathematically distinct ways and there is currently no consensus in the literature as to which definition of the fractional laplacian in bounded dom... | [['the', 'fractional', 'laplacian', 'in', 'rd', 'has', 'multiple', 'equivalent', 'characterizations', 'moreover', 'in', 'bounded', 'domains', 'boundary', 'conditions', 'must', 'be', 'incorporated', 'in', 'these', 'characterizations', 'in', 'mathematically', 'distinct', 'ways', 'and', 'there', 'is', 'currently', 'no', '... | [-0.08625322893833903, 0.03432979198598017, -0.07751033296872767, 0.08352952040860238, -0.14413734342569237, -0.11044735563038958, 0.0027699913026574324, 0.3663286969659659, -0.2895557073955094, -0.30006375521106105, 0.1388250429331743, -0.2724210110467338, -0.17369141801550075, 0.18684579642474886, -0.1190043653244167... |
1,801.09768 | Contextuality, Witness of Quantum Weirdness | The notion of contextuality, which emerges from a theorem established by
Simon Kochen and Ernst Specker (1960-1967) and by John Bell (1964-1966), is
certainly one of the most fundamental aspects of quantum weirdness. If it is a
questioning on scholastic philosophy and a study of contrafactual logic that
led Specker t... | quant-ph | the notion of contextuality which emerges from a theorem established by simon kochen and ernst specker 19601967 and by john bell 19641966 is certainly one of the most fundamental aspects of quantum weirdness if it is a questioning on scholastic philosophy and a study of contrafactual logic that led specker to his demon... | [['the', 'notion', 'of', 'contextuality', 'which', 'emerges', 'from', 'a', 'theorem', 'established', 'by', 'simon', 'kochen', 'and', 'ernst', 'specker', '19601967', 'and', 'by', 'john', 'bell', '19641966', 'is', 'certainly', 'one', 'of', 'the', 'most', 'fundamental', 'aspects', 'of', 'quantum', 'weirdness', 'if', 'it',... | [-0.08126848072691249, 0.06270459855274525, -0.14881741805452425, 0.06912332500950069, -0.12418469956619933, -0.1645778234427174, 0.07380087664322123, 0.223139343304184, -0.24123733347767357, -0.3194271531358453, 0.0620462680743325, -0.25136690459562916, -0.16939341695787608, 0.22336928532583403, -0.16265956109242108, ... |
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