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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708.0949 | The Evolution of Galaxies | The evolution of galaxies results from a combination of internal and external
processes. The star formation is an internal process transforming cold and
dense cores of molecular clouds to stars. It may be triggered internally by
expanding shells, or externally, e. g. by galaxy collisions. The gas accretion
and galaxy... | astro-ph | the evolution of galaxies results from a combination of internal and external processes the star formation is an internal process transforming cold and dense cores of molecular clouds to stars it may be triggered internally by expanding shells or externally e g by galaxy collisions the gas accretion and galaxy merging ... | [['the', 'evolution', 'of', 'galaxies', 'results', 'from', 'a', 'combination', 'of', 'internal', 'and', 'external', 'processes', 'the', 'star', 'formation', 'is', 'an', 'internal', 'process', 'transforming', 'cold', 'and', 'dense', 'cores', 'of', 'molecular', 'clouds', 'to', 'stars', 'it', 'may', 'be', 'triggered', 'in... | [-0.13201264139974314, 0.14613588115552856, -0.08130652738705747, 0.08901574031013182, -0.11070713579588694, 0.0356812408729273, -0.00285311506357132, 0.4135708935324132, -0.2077659537198066, -0.3521979912734172, 0.01321309896490324, -0.27574025736901703, -0.013970793135038862, 0.14331508988301878, 0.048454296804495214... |
708.095 | Characteristic Energy of the Coulomb Interactions and the Pileup of
States | Tunneling data on $\mathrm{La_{1.28}Sr_{1.72}Mn_2O_7}$ crystals confirm
Coulomb interaction effects through the $\sqrt{\mathrm{E}}$ dependence of the
density of states. Importantly, the data and analysis at high energy, E, show a
pileup of states: most of the states removed from near the Fermi level are
found between... | cond-mat.str-el cond-mat.mtrl-sci | tunneling data on mathrmla_128sr_172mn_2o_7 crystals confirm coulomb interaction effects through the sqrtmathrme dependence of the density of states importantly the data and analysis at high energy e show a pileup of states most of the states removed from near the fermi level are found between 40 and 130 mev from which... | [['tunneling', 'data', 'on', 'mathrmla_128sr_172mn_2o_7', 'crystals', 'confirm', 'coulomb', 'interaction', 'effects', 'through', 'the', 'sqrtmathrme', 'dependence', 'of', 'the', 'density', 'of', 'states', 'importantly', 'the', 'data', 'and', 'analysis', 'at', 'high', 'energy', 'e', 'show', 'a', 'pileup', 'of', 'states'... | [-0.08755818506968872, 0.12838954246336862, -0.1142582583773349, 0.060457721153008084, 0.03260060803690327, -0.07798639458903511, 0.13661369658740505, 0.3113531581525292, -0.21959049637994862, -0.38859257394714014, 0.00039560550025531226, -0.39835147953459193, -0.08540783681507622, 0.2138618971354195, 0.057228780843849... |
708.0951 | Smooth matter and source size in microlensing simulations of
gravitationally lensed quasars | Several gravitationally lensed quasars are observed with anomalous
magnifications in pairs of images that straddle a critical curve. Simple
theoretical arguments suggest that the magnification of these images should be
approximately equivalent, whereas one image is observed to be significantly
demagnified. Microlensi... | astro-ph | several gravitationally lensed quasars are observed with anomalous magnifications in pairs of images that straddle a critical curve simple theoretical arguments suggest that the magnification of these images should be approximately equivalent whereas one image is observed to be significantly demagnified microlensing pr... | [['several', 'gravitationally', 'lensed', 'quasars', 'are', 'observed', 'with', 'anomalous', 'magnifications', 'in', 'pairs', 'of', 'images', 'that', 'straddle', 'a', 'critical', 'curve', 'simple', 'theoretical', 'arguments', 'suggest', 'that', 'the', 'magnification', 'of', 'these', 'images', 'should', 'be', 'approxima... | [-0.07652324483681766, 0.08124426230250929, -0.06764422872052259, 0.11125192063571795, -0.06617360889840011, -0.1178890619552336, 0.017451671436272312, 0.41376269911415875, -0.16433396361557803, -0.3514134528187032, 0.03947195195248172, -0.2942630982142873, -0.09156260700099385, 0.19820497751621027, -0.0580882448616298... |
708.0952 | Law of Large Numbers Limits for Many Server Queues | This work considers a many-server queueing system in which customers with
i.i.d., generally distributed service times enter service in the order of
arrival. The dynamics of the system is represented in terms of a process that
describes the total number of customers in the system, as well as a
measure-valued process t... | math.PR math.AP | this work considers a manyserver queueing system in which customers with iid generally distributed service times enter service in the order of arrival the dynamics of the system is represented in terms of a process that describes the total number of customers in the system as well as a measurevalued process that keeps ... | [['this', 'work', 'considers', 'a', 'manyserver', 'queueing', 'system', 'in', 'which', 'customers', 'with', 'iid', 'generally', 'distributed', 'service', 'times', 'enter', 'service', 'in', 'the', 'order', 'of', 'arrival', 'the', 'dynamics', 'of', 'the', 'system', 'is', 'represented', 'in', 'terms', 'of', 'a', 'process'... | [-0.17102921475031363, 0.09831925341614375, -0.09538903253545103, 0.04685404179872421, -0.0116278055785714, -0.11909890354022776, 0.07765154128796176, 0.3151763053267802, -0.2918045042352261, -0.29066673140776783, 0.13291042814074133, -0.28522606653063315, -0.08809835148154219, 0.19648042624497689, -0.08387257582753112... |
708.0953 | Chandra View of DA 530: A Sub-Energetic Supernova Remnant with a Pulsar
Wind Nebula? | Based on a Chandra ACIS observation, we report the detection of an extended
X-ray feature close to the center of the remnant DA 530 with 5.3 sigma above
the background within a circle of 20'' radius. This feature, characterized by a
power-law with the photon index gamma=1.6+-0.8 and spatially coinciding with a
nonthe... | astro-ph | based on a chandra acis observation we report the detection of an extended xray feature close to the center of the remnant da 530 with 53 sigma above the background within a circle of 20 radius this feature characterized by a powerlaw with the photon index gamma1608 and spatially coinciding with a nonthermal radiosourc... | [['based', 'on', 'a', 'chandra', 'acis', 'observation', 'we', 'report', 'the', 'detection', 'of', 'an', 'extended', 'xray', 'feature', 'close', 'to', 'the', 'center', 'of', 'the', 'remnant', 'da', '530', 'with', '53', 'sigma', 'above', 'the', 'background', 'within', 'a', 'circle', 'of', '20', 'radius', 'this', 'feature... | [-0.05555737697674582, 0.1359664739401675, -0.0721722295784275, 0.07866426888237281, -0.06598875991403474, -0.0668099943868583, 0.04828051602210811, 0.4194548231898807, -0.16512584199760263, -0.3448534047541519, 0.08203826678679131, -0.32241900062460144, 0.014313517463354705, 0.1983411162994647, -0.020980443063914816, ... |
708.0954 | The HARPS search for southern extra-solar planets XII. A giant planet
orbiting the metal-poor star HD171028 | In this paper we present the detection of a 1.8 M_Jup planet in a 538 day
period trajectory orbiting the metal-poor star HD171028 ([Fe/H]=-0.49). This
planet is the first to be discovered in the context of a HARPS program
searching for planets around metal-poor stars. Interestingly, HD171028 is one
of the least metal... | astro-ph | in this paper we present the detection of a 18 m_jup planet in a 538 day period trajectory orbiting the metalpoor star hd171028 feh049 this planet is the first to be discovered in the context of a harps program searching for planets around metalpoor stars interestingly hd171028 is one of the least metalpoor stars in th... | [['in', 'this', 'paper', 'we', 'present', 'the', 'detection', 'of', 'a', '18', 'm_jup', 'planet', 'in', 'a', '538', 'day', 'period', 'trajectory', 'orbiting', 'the', 'metalpoor', 'star', 'hd171028', 'feh049', 'this', 'planet', 'is', 'the', 'first', 'to', 'be', 'discovered', 'in', 'the', 'context', 'of', 'a', 'harps', '... | [-0.1268549828738388, 0.10752443489359899, -0.0914850838146069, 0.038873366054354444, -0.11894676038840164, -0.02900165972015303, 0.08844959715012617, 0.30465758110707003, -0.1317278341731354, -0.3638939172960818, 0.07912679797057838, -0.2979029308901065, -0.06175484570364157, 0.1582271379754982, -0.12786685317082125, ... |
708.0955 | Formal Maurer-Cartan Structures: from CFT to Classical Field Equations | We show how the well-known classical field equations as Einstein and
Yang-Mills ones, which arise as the conformal invariance conditions of certain
two-dimensional theories, expanded up to the second order in the formal
parameter, can be reformulated as Generalized/formal Maurer-Cartan equations
(GMC), where the diff... | hep-th math-ph math.DG math.MP | we show how the wellknown classical field equations as einstein and yangmills ones which arise as the conformal invariance conditions of certain twodimensional theories expanded up to the second order in the formal parameter can be reformulated as generalizedformal maurercartan equations gmc where the differential is t... | [['we', 'show', 'how', 'the', 'wellknown', 'classical', 'field', 'equations', 'as', 'einstein', 'and', 'yangmills', 'ones', 'which', 'arise', 'as', 'the', 'conformal', 'invariance', 'conditions', 'of', 'certain', 'twodimensional', 'theories', 'expanded', 'up', 'to', 'the', 'second', 'order', 'in', 'the', 'formal', 'par... | [-0.13797200591121192, 0.14704535367048305, -0.1003947670409537, 0.08216509489853785, -0.11661711206872259, -0.08029136961989064, -0.06892141970962731, 0.2643745946115814, -0.2966286140777495, -0.2905844722510032, 0.11396295969936308, -0.2122741860398294, -0.1827810331267993, 0.09137932130176088, -0.04780057935125154, ... |
708.0956 | Quantum estimation via minimum Kullback entropy principle | We address quantum estimation in situations where one has at disposal data
from the measurement of an incomplete set of observables and some a priori
information on the state itself. By expressing the a priori information in
terms of a bias toward a given state the problem may be faced by minimizing the
quantum relat... | quant-ph | we address quantum estimation in situations where one has at disposal data from the measurement of an incomplete set of observables and some a priori information on the state itself by expressing the a priori information in terms of a bias toward a given state the problem may be faced by minimizing the quantum relative... | [['we', 'address', 'quantum', 'estimation', 'in', 'situations', 'where', 'one', 'has', 'at', 'disposal', 'data', 'from', 'the', 'measurement', 'of', 'an', 'incomplete', 'set', 'of', 'observables', 'and', 'some', 'a', 'priori', 'information', 'on', 'the', 'state', 'itself', 'by', 'expressing', 'the', 'a', 'priori', 'inf... | [-0.08880959021034421, 0.08513776970691846, -0.11023642591078628, 0.07194269764653148, -0.018832210516251745, -0.13228828413555108, 0.09171644260068654, 0.2907027834778285, -0.2856905008437204, -0.2955857008336814, 0.14576290340304038, -0.3090309293475002, -0.0750863146452905, 0.19365562161728433, -0.0956622338395749, ... |
708.0957 | Stanilov-Tsankov-Videv Theory | We survey some recent results concerning Stanilov-Tsankov-Videv theory,
conformal Osserman geometry, and Walker geometry which relate algebraic
properties of the curvature operator to the underlying geometry of the
manifold.
| math.DG | we survey some recent results concerning stanilovtsankovvidev theory conformal osserman geometry and walker geometry which relate algebraic properties of the curvature operator to the underlying geometry of the manifold | [['we', 'survey', 'some', 'recent', 'results', 'concerning', 'stanilovtsankovvidev', 'theory', 'conformal', 'osserman', 'geometry', 'and', 'walker', 'geometry', 'which', 'relate', 'algebraic', 'properties', 'of', 'the', 'curvature', 'operator', 'to', 'the', 'underlying', 'geometry', 'of', 'the', 'manifold']] | [-0.15216958571025835, 0.007858807603562517, -0.15298733201676182, 0.09382670711992043, -0.2098968825303018, -0.12598742059032833, -0.05141748633052755, 0.31244977058044504, -0.2878612530018602, -0.23321853910705873, 0.14789591578301042, -0.27352951807967785, -0.28013063448348213, 0.13129437541855232, -0.15588420423279... |
708.0958 | Role models for complex networks | We present a framework for automatically decomposing ("block-modeling") the
functional classes of agents within a complex network. These classes are
represented by the nodes of an image graph ("block model") depicting the main
patterns of connectivity and thus functional roles in the network. Using a
first principles... | physics.soc-ph physics.data-an | we present a framework for automatically decomposing blockmodeling the functional classes of agents within a complex network these classes are represented by the nodes of an image graph block model depicting the main patterns of connectivity and thus functional roles in the network using a first principles approach we ... | [['we', 'present', 'a', 'framework', 'for', 'automatically', 'decomposing', 'blockmodeling', 'the', 'functional', 'classes', 'of', 'agents', 'within', 'a', 'complex', 'network', 'these', 'classes', 'are', 'represented', 'by', 'the', 'nodes', 'of', 'an', 'image', 'graph', 'block', 'model', 'depicting', 'the', 'main', 'p... | [-0.05726129388521341, -0.007465385243289568, -0.08932753993819158, 0.10760808346129841, -0.07201234043547601, -0.13922994409998257, 0.07114649243709265, 0.4082594247478427, -0.2931839298964901, -0.3505765334477253, 0.07859437914536983, -0.2358176861156773, -0.2204809456823789, 0.1509291342501952, -0.07159763807571973,... |
708.0959 | A flexible Bayesian generalized linear model for dichotomous response
data with an application to text categorization | We present a class of sparse generalized linear models that include probit
and logistic regression as special cases and offer some extra flexibility. We
provide an EM algorithm for learning the parameters of these models from data.
We apply our method in text classification and in simulated data and show that
our met... | stat.ME | we present a class of sparse generalized linear models that include probit and logistic regression as special cases and offer some extra flexibility we provide an em algorithm for learning the parameters of these models from data we apply our method in text classification and in simulated data and show that our method ... | [['we', 'present', 'a', 'class', 'of', 'sparse', 'generalized', 'linear', 'models', 'that', 'include', 'probit', 'and', 'logistic', 'regression', 'as', 'special', 'cases', 'and', 'offer', 'some', 'extra', 'flexibility', 'we', 'provide', 'an', 'em', 'algorithm', 'for', 'learning', 'the', 'parameters', 'of', 'these', 'mo... | [0.01660744839214853, -0.036672907347383446, -0.06708009610218661, 0.0939738687859582, -0.10373228155076504, -0.18526758136493818, 0.06986231521503734, 0.4278280825487205, -0.2792549412231892, -0.27080569975743335, 0.11739463058932285, -0.2612429959732773, -0.25102203421826874, 0.25439088184918673, -0.09864434590563179... |
708.096 | Experimental Demonstration of Decoherence-Free One-Way Information
Transfer | We report the experimental demonstration of a one-way quantum protocol
reliably operating in the presence of decoherence. Information is protected by
designing an appropriate decoherence-free subspace for a cluster state
resource. We demonstrate our scheme in an all-optical setup, encoding the
information into the po... | quant-ph | we report the experimental demonstration of a oneway quantum protocol reliably operating in the presence of decoherence information is protected by designing an appropriate decoherencefree subspace for a cluster state resource we demonstrate our scheme in an alloptical setup encoding the information into the polarizati... | [['we', 'report', 'the', 'experimental', 'demonstration', 'of', 'a', 'oneway', 'quantum', 'protocol', 'reliably', 'operating', 'in', 'the', 'presence', 'of', 'decoherence', 'information', 'is', 'protected', 'by', 'designing', 'an', 'appropriate', 'decoherencefree', 'subspace', 'for', 'a', 'cluster', 'state', 'resource'... | [-0.24615984464685123, 0.16220669762270215, -0.08902244748547673, 0.006870451220311225, 0.016715611728529135, -0.256946168076247, 0.09423753483531376, 0.3987060032288233, -0.2542889055858056, -0.2643763929853837, 0.06679730663386484, -0.23772650763392447, -0.07570821646600961, 0.23823165183266004, -0.08431849071135124,... |
708.0961 | Visualization of Cosmological Particle-Based Datasets | We describe our visualization process for a particle-based simulation of the
formation of the first stars and their impact on cosmic history. The dataset
consists of several hundred time-steps of point simulation data, with each
time-step containing approximately two million point particles. For each
time-step, we in... | astro-ph | we describe our visualization process for a particlebased simulation of the formation of the first stars and their impact on cosmic history the dataset consists of several hundred timesteps of point simulation data with each timestep containing approximately two million point particles for each timestep we interpolate ... | [['we', 'describe', 'our', 'visualization', 'process', 'for', 'a', 'particlebased', 'simulation', 'of', 'the', 'formation', 'of', 'the', 'first', 'stars', 'and', 'their', 'impact', 'on', 'cosmic', 'history', 'the', 'dataset', 'consists', 'of', 'several', 'hundred', 'timesteps', 'of', 'point', 'simulation', 'data', 'wit... | [-0.06923539034634207, 0.1074606654336094, -0.0986893635992116, 0.04532025715536293, -0.07117979617323726, -0.039535407271857066, 0.026518284138292075, 0.3587392233436306, -0.26454578233261905, -0.33919287953525784, 0.09702748087855677, -0.3159906287180881, -0.05698362035560422, 0.18190295742591844, 0.02956346487005551... |
708.0962 | Overconvergence and classicality: the case of curves | Given our set-up of a system of curves and maps between them satisfying
certain assumptions, we prove a classicality criterion for overconvergent
sections of line bundles over these curves. As a result, we prove such criteria
for overconvergent modular forms over various Shimura curves. In particular, we
provide a cl... | math.NT math.AG | given our setup of a system of curves and maps between them satisfying certain assumptions we prove a classicality criterion for overconvergent sections of line bundles over these curves as a result we prove such criteria for overconvergent modular forms over various shimura curves in particular we provide a classicali... | [['given', 'our', 'setup', 'of', 'a', 'system', 'of', 'curves', 'and', 'maps', 'between', 'them', 'satisfying', 'certain', 'assumptions', 'we', 'prove', 'a', 'classicality', 'criterion', 'for', 'overconvergent', 'sections', 'of', 'line', 'bundles', 'over', 'these', 'curves', 'as', 'a', 'result', 'we', 'prove', 'such', ... | [-0.23270966776181012, -0.01619999254352222, -0.21914002801984167, 0.133896099570661, -0.08387496511045939, -0.1416196297878065, 0.03667148753093221, 0.3281424605550292, -0.27500654007188785, -0.2506986145789807, 0.049932315099375464, -0.1741048605300677, -0.18996458183018824, 0.3575707769427353, -0.1557263297518381, 0... |
708.0963 | Search for the rare charmless hadronic decay B+ -> a0+ pi0 | We present a search for B decays to a charged scalar meson a0+ and a pi0
where the a0+ decays to an eta meson and a pi+. The analysis was performed on a
data sample consisting of 383x10-6 BBbar pairs collected with the Babar
detector at the PEP-II asymmetric-energy B Factory at SLAC. We find no
significant signal and... | hep-ex | we present a search for b decays to a charged scalar meson a0 and a pi0 where the a0 decays to an eta meson and a pi the analysis was performed on a data sample consisting of 383x106 bbbar pairs collected with the babar detector at the pepii asymmetricenergy b factory at slac we find no significant signal and set an up... | [['we', 'present', 'a', 'search', 'for', 'b', 'decays', 'to', 'a', 'charged', 'scalar', 'meson', 'a0', 'and', 'a', 'pi0', 'where', 'the', 'a0', 'decays', 'to', 'an', 'eta', 'meson', 'and', 'a', 'pi', 'the', 'analysis', 'was', 'performed', 'on', 'a', 'data', 'sample', 'consisting', 'of', '383x106', 'bbbar', 'pairs', 'co... | [-0.13400092516971154, 0.18674291355605813, -0.07402071248119076, 0.055004462542265285, -0.03152189106553977, -0.16542572374628098, 0.18723983357855936, 0.26735720593758205, -0.13378048109833474, -0.19924592603871852, -0.0542043739826315, -0.47476716459165386, 0.09809623021678424, 0.1492750278018691, 0.1422282219289537... |
708.0964 | Nodally 3-connected planar graphs and convex combination mappings | A convex combination mapping of a planar graph is a plane mapping in which
the external vertices are mapped to the corners of a convex polygon and every
internal vertex is a proper weighted average of its neighbours. If a planar
graph is nodally 3-connected or triangulated then every such mapping is an
embedding (Tut... | cs.CG | a convex combination mapping of a planar graph is a plane mapping in which the external vertices are mapped to the corners of a convex polygon and every internal vertex is a proper weighted average of its neighbours if a planar graph is nodally 3connected or triangulated then every such mapping is an embedding tutte fl... | [['a', 'convex', 'combination', 'mapping', 'of', 'a', 'planar', 'graph', 'is', 'a', 'plane', 'mapping', 'in', 'which', 'the', 'external', 'vertices', 'are', 'mapped', 'to', 'the', 'corners', 'of', 'a', 'convex', 'polygon', 'and', 'every', 'internal', 'vertex', 'is', 'a', 'proper', 'weighted', 'average', 'of', 'its', 'n... | [-0.1528590472829819, 0.06991536955629271, -0.07031003878219053, 0.006105373274476733, -0.17643628879450263, -0.1602596287149936, 0.025127955828793347, 0.4332609220407903, -0.3168330683023669, -0.22515298082726076, 0.09867524150613463, -0.3247014531400055, -0.18427652690152171, 0.09027267420606222, -0.139802641159622, ... |
708.0965 | Dephasing of a particle in a dissipative environment | The motion of a particle in a ring of length L is influenced by a dirty metal
environment whose fluctuations are characterized by a short correlation
distance $\ell << L$. We analyze the induced decoherence process, and compare
the results with those obtained in the opposing Caldeira-Leggett limit ($\ell
>> L$). A pr... | cond-mat.mes-hall | the motion of a particle in a ring of length l is influenced by a dirty metal environment whose fluctuations are characterized by a short correlation distance ell l we analyze the induced decoherence process and compare the results with those obtained in the opposing caldeiraleggett limit ell l a proper definition of t... | [['the', 'motion', 'of', 'a', 'particle', 'in', 'a', 'ring', 'of', 'length', 'l', 'is', 'influenced', 'by', 'a', 'dirty', 'metal', 'environment', 'whose', 'fluctuations', 'are', 'characterized', 'by', 'a', 'short', 'correlation', 'distance', 'ell', 'l', 'we', 'analyze', 'the', 'induced', 'decoherence', 'process', 'and'... | [-0.20217851820018362, 0.19374095602508853, -0.10047499698531978, 0.07521350582976405, -0.03904242819887312, -0.13135567795594824, 0.05151458796634174, 0.36916221818503214, -0.2347868588136728, -0.24495242682888227, 0.038297253240392924, -0.28920778763644833, -0.07287432370597825, 0.1950526446062962, -0.043747075280065... |
708.0966 | The Aspherical Properties of the Energetic Type Ic SN 2002ap as Inferred
from its Nebular Spectra | The nebular spectra of the broad-lined, SN 1998bw-like Type Ic SN 2002ap are
studied by means of synthetic spectra. Two different modelling techniques are
employed. In one technique, the SN ejecta are treated as a single zone, while
in the other a density and abundance distribution in velocity is used from an
explosi... | astro-ph | the nebular spectra of the broadlined sn 1998bwlike type ic sn 2002ap are studied by means of synthetic spectra two different modelling techniques are employed in one technique the sn ejecta are treated as a single zone while in the other a density and abundance distribution in velocity is used from an explosion model ... | [['the', 'nebular', 'spectra', 'of', 'the', 'broadlined', 'sn', '1998bwlike', 'type', 'ic', 'sn', '2002ap', 'are', 'studied', 'by', 'means', 'of', 'synthetic', 'spectra', 'two', 'different', 'modelling', 'techniques', 'are', 'employed', 'in', 'one', 'technique', 'the', 'sn', 'ejecta', 'are', 'treated', 'as', 'a', 'sing... | [-0.009883087208257126, 0.11894848248587286, -0.05060363881946014, 0.1302901782236507, -0.01831750798651609, -0.10174697529630083, -0.014915958026268066, 0.44391151513959387, -0.1797442519125469, -0.33246091090766666, 0.03273742908630245, -0.29743044227912213, 0.0021466871098373796, 0.2411133013195427, -0.0067158268828... |
708.0967 | How to play a disc brake | We consider a gyroscopic system under the action of small dissipative and
non-conservative positional forces, which has its origin in the models of
rotating bodies of revolution being in frictional contact. The spectrum of the
unperturbed gyroscopic system forms a "spectral mesh" in the plane "frequency
-gyroscopic p... | math-ph math.MP nlin.PS physics.class-ph | we consider a gyroscopic system under the action of small dissipative and nonconservative positional forces which has its origin in the models of rotating bodies of revolution being in frictional contact the spectrum of the unperturbed gyroscopic system forms a spectral mesh in the plane frequency gyroscopic parameter ... | [['we', 'consider', 'a', 'gyroscopic', 'system', 'under', 'the', 'action', 'of', 'small', 'dissipative', 'and', 'nonconservative', 'positional', 'forces', 'which', 'has', 'its', 'origin', 'in', 'the', 'models', 'of', 'rotating', 'bodies', 'of', 'revolution', 'being', 'in', 'frictional', 'contact', 'the', 'spectrum', 'o... | [-0.21488965023455733, 0.13478365858696145, -0.10375733570853139, 0.022081716888106794, -0.08855880070242937, -0.10588422847888236, -0.019379272975297568, 0.2923605843689762, -0.27578366034115886, -0.25065718136117365, 0.08876437057463155, -0.2479726667276255, -0.18000874128544844, 0.17584941732626752, -0.0300206826059... |
708.0968 | Estimating the proportion of differentially expressed genes in
comparative DNA microarray experiments | DNA microarray experiments, a well-established experimental technique, aim at
understanding the function of genes in some biological processes. One of the
most common experiments in functional genomics research is to compare two
groups of microarray data to determine which genes are differentially
expressed. In this ... | stat.ME | dna microarray experiments a wellestablished experimental technique aim at understanding the function of genes in some biological processes one of the most common experiments in functional genomics research is to compare two groups of microarray data to determine which genes are differentially expressed in this paper w... | [['dna', 'microarray', 'experiments', 'a', 'wellestablished', 'experimental', 'technique', 'aim', 'at', 'understanding', 'the', 'function', 'of', 'genes', 'in', 'some', 'biological', 'processes', 'one', 'of', 'the', 'most', 'common', 'experiments', 'in', 'functional', 'genomics', 'research', 'is', 'to', 'compare', 'two... | [-0.05798531493588172, 0.011658141181427748, -0.05653659265706355, 0.09130277062587916, -0.03586494696247292, -0.08262951975995476, 0.0547015373211136, 0.37535463626238896, -0.24470251343495392, -0.27592907128657435, 0.04901641752184468, -0.33354640279975817, -0.240677243790297, 0.27835569950811406, -0.0687666342846375... |
708.0969 | One-way quantum computing in a decoherence-free subspace | We introduce a novel scheme for one-way quantum computing (QC) based on the
use of information encoded qubits in an effective cluster state resource. With
the correct encoding structure, we show that it is possible to protect the
entangled resource from phase damping decoherence, where the effective cluster
state can... | quant-ph | we introduce a novel scheme for oneway quantum computing qc based on the use of information encoded qubits in an effective cluster state resource with the correct encoding structure we show that it is possible to protect the entangled resource from phase damping decoherence where the effective cluster state can be desc... | [['we', 'introduce', 'a', 'novel', 'scheme', 'for', 'oneway', 'quantum', 'computing', 'qc', 'based', 'on', 'the', 'use', 'of', 'information', 'encoded', 'qubits', 'in', 'an', 'effective', 'cluster', 'state', 'resource', 'with', 'the', 'correct', 'encoding', 'structure', 'we', 'show', 'that', 'it', 'is', 'possible', 'to... | [-0.13950129431721411, 0.1571044357233883, -0.10099595513913714, 0.029753084776498247, -0.039429229198089034, -0.2609194551651742, 0.0680216846358554, 0.3815180824644733, -0.3023889851021139, -0.2588043422601594, 0.08977780699895352, -0.20141235223089002, -0.15400706770985076, 0.21108540960816308, -0.08381363805056664,... |
708.097 | Supernovae in Three-Dimension: A Link to Gamma-Ray Bursts | Observational consequences of a jet-driven supernova (SN) explosion model are
presented. The results are compared in detail with optical observations of SN
1998bw associated with a Gamma-Ray Burst. It is shown that the jet model is
able to reproduce virtually all the optical observations available for this SN,
althou... | astro-ph | observational consequences of a jetdriven supernova sn explosion model are presented the results are compared in detail with optical observations of sn 1998bw associated with a gammaray burst it is shown that the jet model is able to reproduce virtually all the optical observations available for this sn although a sphe... | [['observational', 'consequences', 'of', 'a', 'jetdriven', 'supernova', 'sn', 'explosion', 'model', 'are', 'presented', 'the', 'results', 'are', 'compared', 'in', 'detail', 'with', 'optical', 'observations', 'of', 'sn', '1998bw', 'associated', 'with', 'a', 'gammaray', 'burst', 'it', 'is', 'shown', 'that', 'the', 'jet',... | [-0.03097377073006808, 0.0887416632268233, -0.023948460179208604, 0.17122424397557215, -0.11270847246999403, -0.14474485639086063, -0.0011783741086859394, 0.46449849226822454, -0.16640021617489834, -0.30020140378770455, 0.06748355332442939, -0.3028930000339945, -0.020621374251412042, 0.2469259761101394, -0.038805753657... |
708.0971 | Ward Identities for the 2PI effective action in QED | We study the issue of symmetries and associated Ward-like identities in the
context of two-particle-irreducible (2PI) functional techniques for abelian
gauge theories. In the 2PI framework, the $n$-point proper vertices of the
theory can be obtained in various different ways which, although equivalent in
the exact th... | hep-th | we study the issue of symmetries and associated wardlike identities in the context of twoparticleirreducible 2pi functional techniques for abelian gauge theories in the 2pi framework the npoint proper vertices of the theory can be obtained in various different ways which although equivalent in the exact theory differ i... | [['we', 'study', 'the', 'issue', 'of', 'symmetries', 'and', 'associated', 'wardlike', 'identities', 'in', 'the', 'context', 'of', 'twoparticleirreducible', '2pi', 'functional', 'techniques', 'for', 'abelian', 'gauge', 'theories', 'in', 'the', '2pi', 'framework', 'the', 'npoint', 'proper', 'vertices', 'of', 'the', 'theo... | [-0.15651289499267781, 0.13918733205031864, -0.10882803167570038, 0.1196270001528319, -0.0755341262362587, -0.10822399773772944, 0.0038053519049383424, 0.32519006195340167, -0.24047438432009788, -0.24869614726399217, 0.06383317578918112, -0.27443108451121523, -0.20738074874410545, 0.13389535777430325, -0.01455129004090... |
708.0972 | Probing the Explosion Mechanism of Supernovae by Radioactive Decay
Gamma- and X-Rays | Gamma- and X-rays resulting from radioactive decays provide a potentially
powerful tool to investigate the explosion physics of supernovae, since the
distribution and the amount of radioactive isotopes are strongly dependent on
properties of the explosion. In this paper, expected features of these high
energy emissio... | astro-ph | gamma and xrays resulting from radioactive decays provide a potentially powerful tool to investigate the explosion physics of supernovae since the distribution and the amount of radioactive isotopes are strongly dependent on properties of the explosion in this paper expected features of these high energy emissions are ... | [['gamma', 'and', 'xrays', 'resulting', 'from', 'radioactive', 'decays', 'provide', 'a', 'potentially', 'powerful', 'tool', 'to', 'investigate', 'the', 'explosion', 'physics', 'of', 'supernovae', 'since', 'the', 'distribution', 'and', 'the', 'amount', 'of', 'radioactive', 'isotopes', 'are', 'strongly', 'dependent', 'on... | [-0.015376303383231128, 0.13191442579651871, -0.03727940645896726, 0.17346246963953255, -0.08955240251358461, -0.12816619139199179, 0.02387985826202634, 0.41093373984201914, -0.2420277139171958, -0.3335152206256882, 0.07085620481531671, -0.3057997604829089, 0.01812168030085525, 0.22784517670947094, 0.002904074377376539... |
708.0973 | Systematic {\it ab initio} study of the magnetic and electronic
properties of all 3d transition metal linear and zigzag nanowires | It is found that all the zigzag chains except the nonmagnetic (NM) Ni and
antiferromagnetic (AF) Fe chains which form a twisted two-legger ladder, look
like a corner-sharing triangle ribbon, and have a lower total energy than the
corresponding linear chains. All the 3d transition metals in both linear and
zigzag stru... | cond-mat.mtrl-sci | it is found that all the zigzag chains except the nonmagnetic nm ni and antiferromagnetic af fe chains which form a twisted twolegger ladder look like a cornersharing triangle ribbon and have a lower total energy than the corresponding linear chains all the 3d transition metals in both linear and zigzag structures have... | [['it', 'is', 'found', 'that', 'all', 'the', 'zigzag', 'chains', 'except', 'the', 'nonmagnetic', 'nm', 'ni', 'and', 'antiferromagnetic', 'af', 'fe', 'chains', 'which', 'form', 'a', 'twisted', 'twolegger', 'ladder', 'look', 'like', 'a', 'cornersharing', 'triangle', 'ribbon', 'and', 'have', 'a', 'lower', 'total', 'energy... | [-0.18939689665486445, 0.2128834302340044, 0.06697751742806102, 0.0793407130294876, -0.018509083021475962, -0.18537270507918172, 0.026492090546814173, 0.4727915096105916, -0.28937648994690224, -0.2353803282234781, 0.047290507389352386, -0.3557097665610548, -0.024454956605689287, 0.09931321077551324, 0.15273326608158722... |
708.0974 | A representative sampling plan for auditing health insurance claims | A stratified sampling plan to audit health insurance claims is offered. The
stratification is by dollar amount of the claim. The plan is representative in
the sense that with high probability for each stratum, the difference in the
average dollar amount of the claim in the sample and the average dollar amount
in the ... | stat.AP | a stratified sampling plan to audit health insurance claims is offered the stratification is by dollar amount of the claim the plan is representative in the sense that with high probability for each stratum the difference in the average dollar amount of the claim in the sample and the average dollar amount in the popul... | [['a', 'stratified', 'sampling', 'plan', 'to', 'audit', 'health', 'insurance', 'claims', 'is', 'offered', 'the', 'stratification', 'is', 'by', 'dollar', 'amount', 'of', 'the', 'claim', 'the', 'plan', 'is', 'representative', 'in', 'the', 'sense', 'that', 'with', 'high', 'probability', 'for', 'each', 'stratum', 'the', 'd... | [-0.06966219696327361, 0.1113930511995381, -0.06455971347274891, 0.08953316167633502, -0.018909402999069985, -0.04395624998649326, 0.14667417002636768, 0.36217863503373615, -0.23194968690155843, -0.3886487953655353, 0.1211124329652569, -0.3409363137677722, -0.0013623792451695291, 0.18527047740030658, -0.166563487551901... |
708.0975 | Near Optimal Broadcast with Network Coding in Large Sensor Networks | We study efficient broadcasting for wireless sensor networks, with network
coding. We address this issue for homogeneous sensor networks in the plane. Our
results are based on a simple principle (IREN/IRON), which sets the same rate
on most of the nodes (wireless links) of the network. With this rate selection,
we gi... | cs.NI | we study efficient broadcasting for wireless sensor networks with network coding we address this issue for homogeneous sensor networks in the plane our results are based on a simple principle ireniron which sets the same rate on most of the nodes wireless links of the network with this rate selection we give a value of... | [['we', 'study', 'efficient', 'broadcasting', 'for', 'wireless', 'sensor', 'networks', 'with', 'network', 'coding', 'we', 'address', 'this', 'issue', 'for', 'homogeneous', 'sensor', 'networks', 'in', 'the', 'plane', 'our', 'results', 'are', 'based', 'on', 'a', 'simple', 'principle', 'ireniron', 'which', 'sets', 'the', ... | [-0.22475423477590084, -0.019454534038258114, -0.03723123471299521, 0.006427834313798347, -0.05211133053593284, -0.1990258933828889, 0.11554444534871593, 0.3923689011189577, -0.27142283261214256, -0.23997218685439056, 0.12627994774576115, -0.2619067465571566, -0.18449589905576955, 0.19166522201070255, -0.13712761122666... |
708.0976 | Confidence distribution (CD) -- distribution estimator of a parameter | The notion of confidence distribution (CD), an entirely frequentist concept,
is in essence a Neymanian interpretation of Fisher's Fiducial distribution. It
contains information related to every kind of frequentist inference. In this
article, a CD is viewed as a distribution estimator of a parameter. This leads
natura... | math.ST stat.TH | the notion of confidence distribution cd an entirely frequentist concept is in essence a neymanian interpretation of fishers fiducial distribution it contains information related to every kind of frequentist inference in this article a cd is viewed as a distribution estimator of a parameter this leads naturally to cons... | [['the', 'notion', 'of', 'confidence', 'distribution', 'cd', 'an', 'entirely', 'frequentist', 'concept', 'is', 'in', 'essence', 'a', 'neymanian', 'interpretation', 'of', 'fishers', 'fiducial', 'distribution', 'it', 'contains', 'information', 'related', 'to', 'every', 'kind', 'of', 'frequentist', 'inference', 'in', 'thi... | [-0.08800007055922435, -0.02257484410482703, -0.15715450863069969, 0.12014377208727571, -0.09917789041178256, -0.08749944194242722, 0.09006731531997325, 0.34412182098050126, -0.2778905940287542, -0.2704835736715212, 0.09573126781487656, -0.25461220240082716, -0.14780796289716552, 0.14078432439099542, -0.136518251451822... |
708.0977 | From symmetry break to Poisson point process in 2D Voronoi
tessellations: the generic nature of hexagons | We bridge the properties of the regular square and honeycomb Voronoi
tessellations of the plane to those of the Poisson-Voronoi case, thus analyzing
in a common framework symmetry-break processes and the approach to uniformly
random distributions of tessellation-generating points. We consider ensemble
simulations of ... | cond-mat.stat-mech cond-mat.dis-nn cs.CG math-ph math.MP physics.data-an | we bridge the properties of the regular square and honeycomb voronoi tessellations of the plane to those of the poissonvoronoi case thus analyzing in a common framework symmetrybreak processes and the approach to uniformly random distributions of tessellationgenerating points we consider ensemble simulations of tessell... | [['we', 'bridge', 'the', 'properties', 'of', 'the', 'regular', 'square', 'and', 'honeycomb', 'voronoi', 'tessellations', 'of', 'the', 'plane', 'to', 'those', 'of', 'the', 'poissonvoronoi', 'case', 'thus', 'analyzing', 'in', 'a', 'common', 'framework', 'symmetrybreak', 'processes', 'and', 'the', 'approach', 'to', 'unifo... | [-0.1101808119483394, 0.15076605615286098, -0.030027427135792095, 0.0644065946489718, -0.020174784876871854, -0.11205876068379439, 0.0664952147767508, 0.3656366628893011, -0.2665011509911892, -0.2385600681809592, 0.09248853865665296, -0.32495230994027224, -0.14833763387650833, 0.14165789075559587, -0.09750798174172814,... |
708.0978 | Empirical Bayes methods for controlling the false discovery rate with
dependent data | False discovery rate (FDR) has been widely used as an error measure in large
scale multiple testing problems, but most research in the area has been focused
on procedures for controlling the FDR based on independent test statistics or
the properties of such procedures for test statistics with certain types of
stochas... | stat.ME | false discovery rate fdr has been widely used as an error measure in large scale multiple testing problems but most research in the area has been focused on procedures for controlling the fdr based on independent test statistics or the properties of such procedures for test statistics with certain types of stochastic d... | [['false', 'discovery', 'rate', 'fdr', 'has', 'been', 'widely', 'used', 'as', 'an', 'error', 'measure', 'in', 'large', 'scale', 'multiple', 'testing', 'problems', 'but', 'most', 'research', 'in', 'the', 'area', 'has', 'been', 'focused', 'on', 'procedures', 'for', 'controlling', 'the', 'fdr', 'based', 'on', 'independent... | [-0.0374562853703364, -0.01941086729916389, -0.11645395164156244, 0.0572507350960569, -0.06042681862156661, -0.13347935549072212, 0.10659970169376937, 0.37578725789097095, -0.20286459166756166, -0.3259974627622536, 0.13806994839770986, -0.21455643918542636, -0.17721268672363033, 0.3024704927356825, -0.09065216025337577... |
708.0979 | A new doubly discrete analogue of smoke ring flow and the real time
simulation of fluid flow | Modelling incompressible ideal fluids as a finite collection of vortex
filaments is important in physics (super-fluidity, models for the onset of
turbulence) as well as for numerical algorithms used in computer graphics for
the real time simulation of smoke. Here we introduce a time-discrete evolution
equation for ar... | nlin.SI math.DS physics.flu-dyn | modelling incompressible ideal fluids as a finite collection of vortex filaments is important in physics superfluidity models for the onset of turbulence as well as for numerical algorithms used in computer graphics for the real time simulation of smoke here we introduce a timediscrete evolution equation for arbitrary ... | [['modelling', 'incompressible', 'ideal', 'fluids', 'as', 'a', 'finite', 'collection', 'of', 'vortex', 'filaments', 'is', 'important', 'in', 'physics', 'superfluidity', 'models', 'for', 'the', 'onset', 'of', 'turbulence', 'as', 'well', 'as', 'for', 'numerical', 'algorithms', 'used', 'in', 'computer', 'graphics', 'for',... | [-0.1312306720148964, 0.07492581084754664, -0.12955180197454913, 0.07527631918837306, -0.06545952313877258, -0.11669619794282102, -0.031740206649008486, 0.35687478503077913, -0.28960582437281757, -0.2534150666576455, 0.11351742051042539, -0.21270152473265364, -0.14509653360534883, 0.21886810823583724, -0.04925136720358... |
708.098 | A smoothing model for sample disclosure risk estimation | When a sample frequency table is published, disclosure risk arises when some
individuals can be identified on the basis of their values in certain
attributes in the table called key variables, and then their values in other
attributes may be inferred, and their privacy is violated. On the basis of the
sample to be re... | stat.ME | when a sample frequency table is published disclosure risk arises when some individuals can be identified on the basis of their values in certain attributes in the table called key variables and then their values in other attributes may be inferred and their privacy is violated on the basis of the sample to be released... | [['when', 'a', 'sample', 'frequency', 'table', 'is', 'published', 'disclosure', 'risk', 'arises', 'when', 'some', 'individuals', 'can', 'be', 'identified', 'on', 'the', 'basis', 'of', 'their', 'values', 'in', 'certain', 'attributes', 'in', 'the', 'table', 'called', 'key', 'variables', 'and', 'then', 'their', 'values', ... | [-0.0632494278432547, 0.056405137681861485, -0.05313937763710991, 0.05231161732303934, -0.07550102275215446, -0.12336257079485598, 0.12969138863242172, 0.388791370875721, -0.25404053830930007, -0.3204370443073421, 0.1325358645732745, -0.2737152011226519, -0.13150640386796808, 0.20855767315002743, -0.13375749117849442, ... |
708.0981 | A note on the U,V method of estimation | The U,V method of estimation provides unbiased estimators or predictors of
random quantities. The method was introduced by Robbins \citer3 and
subsequently studied in a series of papers by Robbins and Zhang. (See Zhang
\citer5.) Practical applications of the method are featured in these papers. We
demonstrate that fo... | math.ST stat.TH | the uv method of estimation provides unbiased estimators or predictors of random quantities the method was introduced by robbins citer3 and subsequently studied in a series of papers by robbins and zhang see zhang citer5 practical applications of the method are featured in these papers we demonstrate that for one u fun... | [['the', 'uv', 'method', 'of', 'estimation', 'provides', 'unbiased', 'estimators', 'or', 'predictors', 'of', 'random', 'quantities', 'the', 'method', 'was', 'introduced', 'by', 'robbins', 'citer3', 'and', 'subsequently', 'studied', 'in', 'a', 'series', 'of', 'papers', 'by', 'robbins', 'and', 'zhang', 'see', 'zhang', 'c... | [-0.0711714017494625, 0.025382025607456834, -0.06898386698476104, 0.08343526136487463, -0.01558984278939491, -0.15377027672975388, 0.03772897673987372, 0.38096829423637585, -0.24541643292231616, -0.29405180711385814, 0.0872489140304022, -0.2793096393390104, -0.20724667577874348, 0.2459280628597277, -0.11255480987994476... |
708.0982 | Low-power radio galaxy environments in the Subaru/XMM-Newton Deep Field
at z~0.5 | We present multi-object spectroscopy of galaxies in the immediate (Mpc-scale)
environments of four low-power (L_1.4 GHz < 10^25 W/Hz) radio galaxies at
z~0.5, selected from the Subaru/XMM-Newton Deep Field. We use the spectra to
calculate velocity dispersions and central redshifts of the groups the radio
galaxies inh... | astro-ph | we present multiobject spectroscopy of galaxies in the immediate mpcscale environments of four lowpower l_14 ghz 1025 whz radio galaxies at z05 selected from the subaruxmmnewton deep field we use the spectra to calculate velocity dispersions and central redshifts of the groups the radio galaxies inhabit and combined wi... | [['we', 'present', 'multiobject', 'spectroscopy', 'of', 'galaxies', 'in', 'the', 'immediate', 'mpcscale', 'environments', 'of', 'four', 'lowpower', 'l_14', 'ghz', '1025', 'whz', 'radio', 'galaxies', 'at', 'z05', 'selected', 'from', 'the', 'subaruxmmnewton', 'deep', 'field', 'we', 'use', 'the', 'spectra', 'to', 'calcula... | [-0.09741578817976496, 0.08642803448517242, -0.07454971315996368, 0.12765475312391153, -0.10372287074803821, -0.06062370224045755, 0.06444681701856561, 0.4990778175243259, -0.11234098748226799, -0.32729009632572265, 0.05274072124418863, -0.3174264141118716, -0.043461194479240094, 0.22266690558671245, 0.0248534666366059... |
708.0983 | Local polynomial regression on unknown manifolds | We reveal the phenomenon that ``naive'' multivariate local polynomial
regression can adapt to local smooth lower dimensional structure in the sense
that it achieves the optimal convergence rate for nonparametric estimation of
regression functions belonging to a Sobolev space when the predictor variables
live on or cl... | math.ST stat.TH | we reveal the phenomenon that naive multivariate local polynomial regression can adapt to local smooth lower dimensional structure in the sense that it achieves the optimal convergence rate for nonparametric estimation of regression functions belonging to a sobolev space when the predictor variables live on or close to... | [['we', 'reveal', 'the', 'phenomenon', 'that', 'naive', 'multivariate', 'local', 'polynomial', 'regression', 'can', 'adapt', 'to', 'local', 'smooth', 'lower', 'dimensional', 'structure', 'in', 'the', 'sense', 'that', 'it', 'achieves', 'the', 'optimal', 'convergence', 'rate', 'for', 'nonparametric', 'estimation', 'of', ... | [-0.05345239110577565, -0.010107584494667558, -0.11693070721454345, 0.1321058658448657, -0.10194889579613048, -0.17350016622087702, 0.07657174490248927, 0.37895767340579856, -0.31770411094364065, -0.21105212912572405, 0.11404647491648436, -0.20050998281042737, -0.17814420425565913, 0.19379305188956025, -0.1397508050386... |
708.0984 | Microscopic quark study of the eta and eta' masses | We show that it is necessary to go beyond the BCS (rainbow-ladder)
approximation to split the $\eta$ and $\eta'$ masses from the $\pi$ and K
masses. We determine the self-consistent set of one-quark-loop diagrams both
for the Schwinger-Dyson quark mass gap equation and for the Bethe-Salpeter
quark-antiquark boundstat... | hep-ph | we show that it is necessary to go beyond the bcs rainbowladder approximation to split the eta and eta masses from the pi and k masses we determine the selfconsistent set of onequarkloop diagrams both for the schwingerdyson quark mass gap equation and for the bethesalpeter quarkantiquark boundstate equation we identify... | [['we', 'show', 'that', 'it', 'is', 'necessary', 'to', 'go', 'beyond', 'the', 'bcs', 'rainbowladder', 'approximation', 'to', 'split', 'the', 'eta', 'and', 'eta', 'masses', 'from', 'the', 'pi', 'and', 'k', 'masses', 'we', 'determine', 'the', 'selfconsistent', 'set', 'of', 'onequarkloop', 'diagrams', 'both', 'for', 'the'... | [-0.10435269272094157, 0.1522701609211704, -0.08684515012167046, 0.1681384730825166, -0.09392082571078127, -0.11445941537549005, 0.11092014958490139, 0.3418466755859206, -0.20254699654755332, -0.2174667883925488, 0.012563920336140094, -0.31823588649211365, -0.06905787924704986, 0.1465803801351897, 0.08928668047257951, ... |
708.0985 | Formal punctured ribbons and two-dimensional local fields | We investigate formal ribbons on curves. Roughly speaking, formal ribbon is a
family of locally linearly compact vector spaces on a curve. We establish a
one-to-one correspondence between formal ribbons on curves plus some geometric
data and some subspaces of two-dimensional local field.
| math.AG | we investigate formal ribbons on curves roughly speaking formal ribbon is a family of locally linearly compact vector spaces on a curve we establish a onetoone correspondence between formal ribbons on curves plus some geometric data and some subspaces of twodimensional local field | [['we', 'investigate', 'formal', 'ribbons', 'on', 'curves', 'roughly', 'speaking', 'formal', 'ribbon', 'is', 'a', 'family', 'of', 'locally', 'linearly', 'compact', 'vector', 'spaces', 'on', 'a', 'curve', 'we', 'establish', 'a', 'onetoone', 'correspondence', 'between', 'formal', 'ribbons', 'on', 'curves', 'plus', 'some'... | [-0.26256014105625625, 0.07341300167663153, -0.10800110574725062, 0.13214319607860214, -0.11676581293820988, -0.12978850882283824, 0.03636418540723795, 0.4833606938983119, -0.2895909599786581, -0.1896472162307175, 0.0832308141384707, -0.24755220180160778, -0.15610446339083273, 0.2729522672503494, -0.158614102339502, 0.... |
708.0986 | Accurate early positions for Swift GRBS: enhancing X-ray positions with
UVOT astrometry | Here we describe an autonomous way of producing more accurate prompt XRT
positions for Swift-detected GRBs and their afterglows, based on UVOT
astrometry and a detailed mapping between the XRT and UVOT detectors. The
latter significantly reduces the dominant systematic error -- the star-tracker
solution to the World ... | astro-ph | here we describe an autonomous way of producing more accurate prompt xrt positions for swiftdetected grbs and their afterglows based on uvot astrometry and a detailed mapping between the xrt and uvot detectors the latter significantly reduces the dominant systematic error the startracker solution to the world coordinat... | [['here', 'we', 'describe', 'an', 'autonomous', 'way', 'of', 'producing', 'more', 'accurate', 'prompt', 'xrt', 'positions', 'for', 'swiftdetected', 'grbs', 'and', 'their', 'afterglows', 'based', 'on', 'uvot', 'astrometry', 'and', 'a', 'detailed', 'mapping', 'between', 'the', 'xrt', 'and', 'uvot', 'detectors', 'the', 'l... | [-0.037923674325896564, 0.06070942899532383, -0.06945615734404592, 0.10555144084648771, -0.08552779348344723, -0.12049135666535195, 0.10672119641398538, 0.5047023582008126, -0.13563821788654842, -0.3834628454160202, 0.09045469122087416, -0.33500643483182385, -0.02472635926574524, 0.30136087136742756, -0.090960160747027... |
708.0987 | Darwinian Dynamics Implies Developmental Ascendency | A tendency in biological theorizing is to formulate principles above or equal
to Evolution by Variation and Selection of Darwin and Wallace. In this letter I
analyze one such recent proposal which did so for the developmental ascendency.
I show that though the idea of developmental ascendency is brilliant, this is
in... | q-bio.PE q-bio.OT | a tendency in biological theorizing is to formulate principles above or equal to evolution by variation and selection of darwin and wallace in this letter i analyze one such recent proposal which did so for the developmental ascendency i show that though the idea of developmental ascendency is brilliant this is in wron... | [['a', 'tendency', 'in', 'biological', 'theorizing', 'is', 'to', 'formulate', 'principles', 'above', 'or', 'equal', 'to', 'evolution', 'by', 'variation', 'and', 'selection', 'of', 'darwin', 'and', 'wallace', 'in', 'this', 'letter', 'i', 'analyze', 'one', 'such', 'recent', 'proposal', 'which', 'did', 'so', 'for', 'the',... | [-0.034694894833804724, 0.14809601950495468, -0.07076543585288447, 0.11478493692407796, -0.10619926375228089, -0.1297721672718498, 0.002718540851946001, 0.3858712828875362, -0.2651084555046899, -0.3149604467167096, 0.08622827823425026, -0.24084680434316397, -0.262376979782621, 0.13271815050090965, -0.1312763490230329, ... |
708.0988 | The role of the two postulates of special relativity | Students are often mystified by the reasoning that leads from the postulates
of special relativity to the requirement of covariance. This is partly due to
the lack of transparency resulting from the failure to clearly separate the
roles the postulates of the constancy of the speed of light and of relativity
play. The... | physics.ed-ph | students are often mystified by the reasoning that leads from the postulates of special relativity to the requirement of covariance this is partly due to the lack of transparency resulting from the failure to clearly separate the roles the postulates of the constancy of the speed of light and of relativity play their r... | [['students', 'are', 'often', 'mystified', 'by', 'the', 'reasoning', 'that', 'leads', 'from', 'the', 'postulates', 'of', 'special', 'relativity', 'to', 'the', 'requirement', 'of', 'covariance', 'this', 'is', 'partly', 'due', 'to', 'the', 'lack', 'of', 'transparency', 'resulting', 'from', 'the', 'failure', 'to', 'clearl... | [-0.07754414499243303, 0.11348346089765143, -0.10574935503208484, 0.08962482254570112, -0.10027884893441716, -0.07403043306504305, 0.024770783536577932, 0.3292986664037483, -0.2736799551460605, -0.34261733006972533, 0.07542615907135396, -0.2356696462061686, -0.15665733713943225, 0.17382338869934663, -0.1182607067957854... |
708.0989 | Proton Hexality from an Anomalous Flavor U(1) and Neutrino Masses -
Linking to the String Scale | We devise minimalistic gauged U(1)_X Froggatt-Nielsen models which at
low-energy give rise to the recently suggested discrete gauge Z_6 symmetry,
proton hexality, thus stabilizing the proton. Assuming three generations of
right-handed neutrinos, with the proper choice of X-charges, we obtain viable
neutrino masses. F... | hep-ph hep-th | we devise minimalistic gauged u1_x froggattnielsen models which at lowenergy give rise to the recently suggested discrete gauge z_6 symmetry proton hexality thus stabilizing the proton assuming three generations of righthanded neutrinos with the proper choice of xcharges we obtain viable neutrino masses furthermore we ... | [['we', 'devise', 'minimalistic', 'gauged', 'u1_x', 'froggattnielsen', 'models', 'which', 'at', 'lowenergy', 'give', 'rise', 'to', 'the', 'recently', 'suggested', 'discrete', 'gauge', 'z_6', 'symmetry', 'proton', 'hexality', 'thus', 'stabilizing', 'the', 'proton', 'assuming', 'three', 'generations', 'of', 'righthanded'... | [-0.0978554777010638, 0.2787240208616774, -0.03689035912362957, 0.16019610453574723, -0.14310920119628703, -0.1954947277784078, 0.04616739861912241, 0.3457427579713495, -0.19803447256747045, -0.331671557324865, 0.028446581652755605, -0.2094726988245001, -0.06977502409120605, 0.07061813108157367, 0.011844474460782581, -... |
708.099 | Matrice magique associ\'ee \`a un germe de courbe plane et division par
l'id\'eal Jacobien | In the ring of holomorphic functions at the origin of C^2, we consider the
equation uf'_x+vf'_y=wf where f and w are given. We introduce intersection
multiplicities relative to w and f'_y along the branches of f, and we study the
solutions (u,v) using these valuations. As an application, we construct an
explicit func... | math.AG | in the ring of holomorphic functions at the origin of c2 we consider the equation uf_xvf_ywf where f and w are given we introduce intersection multiplicities relative to w and f_y along the branches of f and we study the solutions uv using these valuations as an application we construct an explicit functional equation ... | [['in', 'the', 'ring', 'of', 'holomorphic', 'functions', 'at', 'the', 'origin', 'of', 'c2', 'we', 'consider', 'the', 'equation', 'uf_xvf_ywf', 'where', 'f', 'and', 'w', 'are', 'given', 'we', 'introduce', 'intersection', 'multiplicities', 'relative', 'to', 'w', 'and', 'f_y', 'along', 'the', 'branches', 'of', 'f', 'and',... | [-0.18705654856083648, 0.03603052890529008, -0.056224338203069886, 0.03539398287622524, -0.027571893072620566, -0.10233322270713481, 0.008553030940155233, 0.3591676407626697, -0.31808606957617613, -0.2185681702436081, 0.053571661657770164, -0.29645977758835734, -0.11528284641514931, 0.1676284594058026, -0.0416068036741... |
708.0991 | Full transmission through perfect-conductor subwavelength hole arrays | Light transmission through 2D subwavelength hole arrays in perfect-conductor
films is shown to be complete (100%) at some resonant wavelengths even for
arbitrarily narrow holes. Conversely, the reflection on a 2D planar array of
non-absorbing scatterers is shown to be complete at some wavelengths regardless
how weak ... | cond-mat.other | light transmission through 2d subwavelength hole arrays in perfectconductor films is shown to be complete 100 at some resonant wavelengths even for arbitrarily narrow holes conversely the reflection on a 2d planar array of nonabsorbing scatterers is shown to be complete at some wavelengths regardless how weak the scatt... | [['light', 'transmission', 'through', '2d', 'subwavelength', 'hole', 'arrays', 'in', 'perfectconductor', 'films', 'is', 'shown', 'to', 'be', 'complete', '100', 'at', 'some', 'resonant', 'wavelengths', 'even', 'for', 'arbitrarily', 'narrow', 'holes', 'conversely', 'the', 'reflection', 'on', 'a', '2d', 'planar', 'array',... | [-0.16121212939413873, 0.12129192725898555, -0.046844938931127005, 0.05300071541457258, -0.05912198088704967, -0.1808574891866346, 0.013849135362901367, 0.46592554020193905, -0.21325800132203418, -0.2852563523651602, 0.11994114879724713, -0.3046700227322827, -0.16582182521233335, 0.257018896106344, -0.00041672522526753... |
708.0992 | The transition of equation of state of effective dark energy in the DGP
model with bulk contents | We investigate the effect of the bulk contents in the DGP braneworld on the
evolution of the universe. We find that although the pure DGP model cannot
accommodate the transition of the effective equation of state of dark energy,
once the bulk matter T^5_5 is considered, the modified model can realize the
w_{eff} cros... | hep-th astro-ph gr-qc | we investigate the effect of the bulk contents in the dgp braneworld on the evolution of the universe we find that although the pure dgp model cannot accommodate the transition of the effective equation of state of dark energy once the bulk matter t5_5 is considered the modified model can realize the w_eff crossing 1 h... | [['we', 'investigate', 'the', 'effect', 'of', 'the', 'bulk', 'contents', 'in', 'the', 'dgp', 'braneworld', 'on', 'the', 'evolution', 'of', 'the', 'universe', 'we', 'find', 'that', 'although', 'the', 'pure', 'dgp', 'model', 'can', 'not', 'accommodate', 'the', 'transition', 'of', 'the', 'effective', 'equation', 'of', 'st... | [-0.11567022934385383, 0.1458231609186712, -0.1175879429375312, 0.08241712169469341, -0.0770219913648285, -0.110672464263661, -0.00684313963608148, 0.28620720435758584, -0.2362389243314512, -0.3580640656233744, 0.03903399000054524, -0.2538003245695629, -0.08541851390494418, 0.11850021341424577, 0.015314373507640745, -0... |
708.0993 | A Simple Model for Pulse Profiles from Precessing Pulsars, with Special
Application to Relativistic Binary PSR B1913+16 | We study the observable pulse profiles that can be generated from precessing
pulsars. A novel coordinate system is defined to aid visualization of the
observing geometry. Using this system we explore the different families of
profiles that can be generated by simple, circularly symmetric beam shapes. An
attempt is th... | astro-ph gr-qc | we study the observable pulse profiles that can be generated from precessing pulsars a novel coordinate system is defined to aid visualization of the observing geometry using this system we explore the different families of profiles that can be generated by simple circularly symmetric beam shapes an attempt is then mad... | [['we', 'study', 'the', 'observable', 'pulse', 'profiles', 'that', 'can', 'be', 'generated', 'from', 'precessing', 'pulsars', 'a', 'novel', 'coordinate', 'system', 'is', 'defined', 'to', 'aid', 'visualization', 'of', 'the', 'observing', 'geometry', 'using', 'this', 'system', 'we', 'explore', 'the', 'different', 'famili... | [-0.07942690140890335, 0.08984139129641965, -0.12631450722517532, 0.09472132366594974, -0.1308509832357659, -0.13830976162312758, 0.010080473068371123, 0.42377201293053385, -0.24341538518034164, -0.32207060037363394, 0.0867944939900494, -0.27665782473323974, -0.08405408739824505, 0.25414052995506164, -0.047329759322642... |
708.0994 | Tunneling mechanism of light transmission through metallic films | A mechanism of light transmission through metallic films is proposed,
assisted by tunnelling between resonating buried dielectric inclusions. This is
illustrated by arrays of Si spheres embedded in Ag. Strong transmission peaks
are observed near the Mie resonances of the spheres. The interaction among
various planes ... | cond-mat.other | a mechanism of light transmission through metallic films is proposed assisted by tunnelling between resonating buried dielectric inclusions this is illustrated by arrays of si spheres embedded in ag strong transmission peaks are observed near the mie resonances of the spheres the interaction among various planes of sph... | [['a', 'mechanism', 'of', 'light', 'transmission', 'through', 'metallic', 'films', 'is', 'proposed', 'assisted', 'by', 'tunnelling', 'between', 'resonating', 'buried', 'dielectric', 'inclusions', 'this', 'is', 'illustrated', 'by', 'arrays', 'of', 'si', 'spheres', 'embedded', 'in', 'ag', 'strong', 'transmission', 'peaks... | [-0.16054657979154038, 0.1837479160935844, -0.0345065521248119, 0.02290472028284216, -0.03342668814143817, -0.18915470584648328, 0.053941221003538195, 0.4312442484700564, -0.25578486206896095, -0.31425856860372625, 0.018773774642415923, -0.3186042209277924, -0.16354044505114695, 0.1706596521742063, 0.000529916061866052... |
708.0995 | Fixed-axis polarization states: covariance and comparisons | Addressing the recent criticisms of Kvinikhidze and Miller, we prove that the
spectator wave functions and currents based on ``fixed-axis'' polarization
states (previously introduced by us) are Lorentz covariant, and find an
explicit connection between them and conventional direction-dependent
polarization states. Th... | nucl-th | addressing the recent criticisms of kvinikhidze and miller we prove that the spectator wave functions and currents based on fixedaxis polarization states previously introduced by us are lorentz covariant and find an explicit connection between them and conventional directiondependent polarization states the discussion ... | [['addressing', 'the', 'recent', 'criticisms', 'of', 'kvinikhidze', 'and', 'miller', 'we', 'prove', 'that', 'the', 'spectator', 'wave', 'functions', 'and', 'currents', 'based', 'on', 'fixedaxis', 'polarization', 'states', 'previously', 'introduced', 'by', 'us', 'are', 'lorentz', 'covariant', 'and', 'find', 'an', 'expli... | [-0.10570466357083726, 0.16970348654415698, -0.08847974920977972, 0.10093084161677066, -0.1118794907150524, -0.12477814805710555, 0.04252953187512633, 0.3708818290781762, -0.19086123113187828, -0.2530144109457199, -0.024961084667925855, -0.27725529827876016, -0.17142062517814338, 0.13193723166893637, 0.0105562022488032... |
708.0996 | Formal derivation of an exact series expansion for the Principal Field
Emission Elliptic Function v | An exact series expansion is now known for the Principal Field Emission
Elliptic Function v, in terms of a complementary elliptic variable l' equal to
y*y, where y is the Nordheim parameter. This expansion was originally found by
using the algebraic manipulation package MAPLE. This paper presents a formal
mathematica... | math-ph math.MP | an exact series expansion is now known for the principal field emission elliptic function v in terms of a complementary elliptic variable l equal to yy where y is the nordheim parameter this expansion was originally found by using the algebraic manipulation package maple this paper presents a formal mathematical deriva... | [['an', 'exact', 'series', 'expansion', 'is', 'now', 'known', 'for', 'the', 'principal', 'field', 'emission', 'elliptic', 'function', 'v', 'in', 'terms', 'of', 'a', 'complementary', 'elliptic', 'variable', 'l', 'equal', 'to', 'yy', 'where', 'y', 'is', 'the', 'nordheim', 'parameter', 'this', 'expansion', 'was', 'origina... | [-0.10276017531821537, 0.05776014925282855, -0.12992286442203424, 0.07013153999967925, -0.12185383417000074, -0.16537029885331192, -0.01598861242410659, 0.30990905379736594, -0.2966842202573631, -0.27021354969287126, 0.09591255896592857, -0.25928570227417697, -0.14390210655134156, 0.2121387008225841, -0.053244886298308... |
708.0997 | Spin Pumping of Current in Non-Uniform Conducting Magnets | Using irreversible thermodynamics we show that current-induced spin transfer
torque within a magnetic domain implies spin pumping of current within that
domain. This has experimental implications for samples both with conducting
leads and that are electrically isolated. These results are obtained by
deriving the dyna... | cond-mat.other | using irreversible thermodynamics we show that currentinduced spin transfer torque within a magnetic domain implies spin pumping of current within that domain this has experimental implications for samples both with conducting leads and that are electrically isolated these results are obtained by deriving the dynamical... | [['using', 'irreversible', 'thermodynamics', 'we', 'show', 'that', 'currentinduced', 'spin', 'transfer', 'torque', 'within', 'a', 'magnetic', 'domain', 'implies', 'spin', 'pumping', 'of', 'current', 'within', 'that', 'domain', 'this', 'has', 'experimental', 'implications', 'for', 'samples', 'both', 'with', 'conducting'... | [-0.16996918939249178, 0.23100820480955436, -0.02393128919670833, 0.008446621180137656, -0.04044817619176362, -0.13437040035633424, 0.02872779338983545, 0.375420944167155, -0.27178249266637744, -0.31236939878641246, 0.04509569873506039, -0.23991275438125811, -0.08207828330569993, 0.22825011405089468, 0.0454169554126850... |
708.0998 | Fine-tune your smile: Correction to Hagan et al | In this small note we use results derived in Berestycki et al. to correct the
celebrated formulae of Hagan et al. We derive explicitly the correct zero order
term in the expansion of the implied volatility in time to maturity. The new
term is consistent as $\beta\to 1$. Furthermore, numerical simulations show
that it... | q-fin.CP math.PR q-fin.ST | in this small note we use results derived in berestycki et al to correct the celebrated formulae of hagan et al we derive explicitly the correct zero order term in the expansion of the implied volatility in time to maturity the new term is consistent as betato 1 furthermore numerical simulations show that it reduces or... | [['in', 'this', 'small', 'note', 'we', 'use', 'results', 'derived', 'in', 'berestycki', 'et', 'al', 'to', 'correct', 'the', 'celebrated', 'formulae', 'of', 'hagan', 'et', 'al', 'we', 'derive', 'explicitly', 'the', 'correct', 'zero', 'order', 'term', 'in', 'the', 'expansion', 'of', 'the', 'implied', 'volatility', 'in', ... | [-0.09048780901057105, 0.047225210788794006, -0.05491362650307917, 0.10343420334280498, -0.09870609127345585, -0.06592914969810555, 0.07264848972009795, 0.2869403864136867, -0.23086720996070653, -0.3153693183896042, 0.07259418599818263, -0.26123316946529573, -0.20497505658216053, 0.18855848794262256, -0.168582816908676... |
708.0999 | Plasmon tunability in metallodielectric metamaterials | The dielectric properties of metamaterials consisting of periodically
arranged metallic nanoparticles of spherical shape are calculated by rigorously
solving Maxwell's equations. Effective dielectric functions are obtained by
comparing the reflectivity of planar surfaces limiting these materials with
Fresnel's formul... | cond-mat.mtrl-sci | the dielectric properties of metamaterials consisting of periodically arranged metallic nanoparticles of spherical shape are calculated by rigorously solving maxwells equations effective dielectric functions are obtained by comparing the reflectivity of planar surfaces limiting these materials with fresnels formulas fo... | [['the', 'dielectric', 'properties', 'of', 'metamaterials', 'consisting', 'of', 'periodically', 'arranged', 'metallic', 'nanoparticles', 'of', 'spherical', 'shape', 'are', 'calculated', 'by', 'rigorously', 'solving', 'maxwells', 'equations', 'effective', 'dielectric', 'functions', 'are', 'obtained', 'by', 'comparing', ... | [-0.12198640569020802, 0.19410451223689412, -0.02012780098806298, 0.006094200836886312, -0.026729340136553797, -0.15006667883726693, -0.004515735606204659, 0.45576281708827804, -0.1952743984477979, -0.3017973468092913, -0.001464232344121214, -0.34898379004915203, -0.1471679649359199, 0.17966154712947116, 0.017960876137... |
708.1 | Particle Acceleration and Magnetic Dissipation in Relativistic Current
Sheet of Pair Plasmas | We study linear and nonlinear development of relativistic and
ultrarelativistic current sheets of pair plasmas with antiparallel magnetic
fields. Two types of two-dimensional problems are investigated by
particle-in-cell simulations. First, we present the development of relativistic
magnetic reconnection, whose outfl... | astro-ph | we study linear and nonlinear development of relativistic and ultrarelativistic current sheets of pair plasmas with antiparallel magnetic fields two types of twodimensional problems are investigated by particleincell simulations first we present the development of relativistic magnetic reconnection whose outflow speed ... | [['we', 'study', 'linear', 'and', 'nonlinear', 'development', 'of', 'relativistic', 'and', 'ultrarelativistic', 'current', 'sheets', 'of', 'pair', 'plasmas', 'with', 'antiparallel', 'magnetic', 'fields', 'two', 'types', 'of', 'twodimensional', 'problems', 'are', 'investigated', 'by', 'particleincell', 'simulations', 'f... | [-0.18045694799179512, 0.22444853357093333, -0.019114400357671122, 0.08982068402801054, -0.04555620739958127, -0.08927506429547961, -0.05755754841091745, 0.37790886048929695, -0.26608735601190986, -0.26710145373424, 0.03508322333541567, -0.22303408236091674, -0.05861867872598284, 0.23217494078833062, 0.0556428890724980... |
708.1001 | Fundamental Strings, Holography, and Nonlinear Superconformal Algebras | We discuss aspects of holography in the AdS_3 \times S^p near string geometry
of a collection of straight fundamental heterotic strings. We use anomalies and
symmetries to determine general features of the dual CFT. The symmetries
suggest the appearance of nonlinear superconformal algebras, and we show how
these aris... | hep-th | we discuss aspects of holography in the ads_3 times sp near string geometry of a collection of straight fundamental heterotic strings we use anomalies and symmetries to determine general features of the dual cft the symmetries suggest the appearance of nonlinear superconformal algebras and we show how these arise in th... | [['we', 'discuss', 'aspects', 'of', 'holography', 'in', 'the', 'ads_3', 'times', 'sp', 'near', 'string', 'geometry', 'of', 'a', 'collection', 'of', 'straight', 'fundamental', 'heterotic', 'strings', 'we', 'use', 'anomalies', 'and', 'symmetries', 'to', 'determine', 'general', 'features', 'of', 'the', 'dual', 'cft', 'the... | [-0.14251165265132756, 0.12121847644144013, -0.0776374763161295, 0.12642337935659187, -0.0967116558754986, -0.13559665047902275, -0.035498631036501714, 0.3274141216481274, -0.2084175177680498, -0.21058441881429066, 0.09941925549964335, -0.3177663515152579, -0.19017522652760488, 0.14807175696742805, -0.0970587159542695,... |
708.1002 | On the finiteness of the noncommutative supersymmetric
Maxwell-Chern-Simons theory | Within the superfield approach, we prove the absence of UV/IR mixing in the
three-dimensional noncommutative supersymmetric Maxwell-Chern-Simons theory at
any loop order and demonstrate its finiteness in one, three and higher loop
orders.
| hep-th | within the superfield approach we prove the absence of uvir mixing in the threedimensional noncommutative supersymmetric maxwellchernsimons theory at any loop order and demonstrate its finiteness in one three and higher loop orders | [['within', 'the', 'superfield', 'approach', 'we', 'prove', 'the', 'absence', 'of', 'uvir', 'mixing', 'in', 'the', 'threedimensional', 'noncommutative', 'supersymmetric', 'maxwellchernsimons', 'theory', 'at', 'any', 'loop', 'order', 'and', 'demonstrate', 'its', 'finiteness', 'in', 'one', 'three', 'and', 'higher', 'loop... | [-0.13938040047827543, 0.1889143522095048, -0.013062745798379183, 0.1237540979248782, -0.002171936868266626, -0.10059903684834187, -0.029932757123429892, 0.31641347452320834, -0.20324124441002356, -0.2851166970054196, 0.08731002680900873, -0.24130890941755337, -0.1814047611798301, 0.10082077607512474, -0.05098510226658... |
708.1003 | How Magnetic Field Enters Heat Current: Application to Fluctuation
Nernst Effect | A problem of the definition of the heat transported in thermomagnetic
phenomena has been well realized in the late sixties, but not solved up to
date. Ignoring this problem, numerous recent theories grossly overestimate the
thermomagnetic coefficients in strongly interacting systems. Here we develop a
gauge-invariant... | cond-mat.supr-con cond-mat.str-el | a problem of the definition of the heat transported in thermomagnetic phenomena has been well realized in the late sixties but not solved up to date ignoring this problem numerous recent theories grossly overestimate the thermomagnetic coefficients in strongly interacting systems here we develop a gaugeinvariant micros... | [['a', 'problem', 'of', 'the', 'definition', 'of', 'the', 'heat', 'transported', 'in', 'thermomagnetic', 'phenomena', 'has', 'been', 'well', 'realized', 'in', 'the', 'late', 'sixties', 'but', 'not', 'solved', 'up', 'to', 'date', 'ignoring', 'this', 'problem', 'numerous', 'recent', 'theories', 'grossly', 'overestimate',... | [-0.14262291616727402, 0.2011502191201377, -0.08868137383374425, 0.08423302218918098, -0.06896826046400927, -0.10505736254247457, 0.03242601690941792, 0.3183640403620584, -0.28727072067427595, -0.2989265220108586, 0.02343050629707237, -0.2838682753401218, -0.15533834883392278, 0.19292417573201484, 0.0021317334760400193... |
708.1004 | Cluster Formation in Contracting Molecular Clouds | We explore, through a simplified, semi-analytic model, the formation of dense
clusters containing massive stars. The parent cloud spawning the cluster is
represented as an isothermal sphere. This sphere is in near force balance
between self-gravity and turbulent pressure. Self-gravity, mediated by
turbulent dissipati... | astro-ph | we explore through a simplified semianalytic model the formation of dense clusters containing massive stars the parent cloud spawning the cluster is represented as an isothermal sphere this sphere is in near force balance between selfgravity and turbulent pressure selfgravity mediated by turbulent dissipation drives sl... | [['we', 'explore', 'through', 'a', 'simplified', 'semianalytic', 'model', 'the', 'formation', 'of', 'dense', 'clusters', 'containing', 'massive', 'stars', 'the', 'parent', 'cloud', 'spawning', 'the', 'cluster', 'is', 'represented', 'as', 'an', 'isothermal', 'sphere', 'this', 'sphere', 'is', 'in', 'near', 'force', 'bala... | [-0.11031206338040052, 0.146953501885829, -0.10362101864745045, 0.069366001332048, -0.06311836490429372, -0.018568809340947595, 0.08754295442928696, 0.33857344862139016, -0.2174193131851784, -0.32448661876964924, 0.02250465961603437, -0.233477106503053, -0.047258655571833875, 0.14673181265532664, -0.02262219355839212, ... |
708.1005 | Langevin Dynamics of the vortex matter two-stage melting transition in
Bi_2Sr_2CaCu_2O$_{8+\delta}$ in the presence of straight and of tilted
columnar defects | In this paper we use London Langevin molecular dynamics simulations to
investigate the vortex matter melting transition in the highly anisotropic
high-temperature superconductor material Bi_2Sr_2CaCu_2O$_{8+\delta}$ in the
presence of low concentration of columnar defects (CDs). We reproduce with
further details our ... | cond-mat.supr-con cond-mat.dis-nn | in this paper we use london langevin molecular dynamics simulations to investigate the vortex matter melting transition in the highly anisotropic hightemperature superconductor material bi_2sr_2cacu_2o_8delta in the presence of low concentration of columnar defects cds we reproduce with further details our previous res... | [['in', 'this', 'paper', 'we', 'use', 'london', 'langevin', 'molecular', 'dynamics', 'simulations', 'to', 'investigate', 'the', 'vortex', 'matter', 'melting', 'transition', 'in', 'the', 'highly', 'anisotropic', 'hightemperature', 'superconductor', 'material', 'bi_2sr_2cacu_2o_8delta', 'in', 'the', 'presence', 'of', 'lo... | [-0.1183623369237881, 0.1852850336913976, -0.049303822043240846, 0.004851524247015812, -0.013855919214158555, -0.08892079841537362, 0.05133003558193869, 0.4230013122309212, -0.25868764888842644, -0.2639524950265855, 0.06639043450743982, -0.2831423365139436, -0.10433420233315834, 0.14847747211638895, 0.00969730005864961... |
708.1006 | Electromagnetic forces and torques in nanoparticles irradiated by a
plane wave | Optical tweezers and optical lattices are making it possible to control small
particles by means of electromagnetic forces and torques. In this context, a
method is presented in this work to calculate electromagnetic forces and
torques for arbitrarily-shaped objects in the presence of other objects
illuminated by a p... | cond-mat.other | optical tweezers and optical lattices are making it possible to control small particles by means of electromagnetic forces and torques in this context a method is presented in this work to calculate electromagnetic forces and torques for arbitrarilyshaped objects in the presence of other objects illuminated by a plane ... | [['optical', 'tweezers', 'and', 'optical', 'lattices', 'are', 'making', 'it', 'possible', 'to', 'control', 'small', 'particles', 'by', 'means', 'of', 'electromagnetic', 'forces', 'and', 'torques', 'in', 'this', 'context', 'a', 'method', 'is', 'presented', 'in', 'this', 'work', 'to', 'calculate', 'electromagnetic', 'for... | [-0.13803864797425808, 0.12895636752519635, -0.06784146685985107, 0.0013810452582423114, -0.08763153650300595, -0.049979073574169745, -0.0255501821537692, 0.4124872151002722, -0.2270406693405499, -0.3073878662965319, 0.057874877275944266, -0.25647827527300426, -0.16159403246366283, 0.2468906764361501, 0.004401113380772... |
708.1007 | On-Chip Matching Networks for Radio-Frequency
Single-Electron-Transistors | In this letter, we describe operation of a radio-frequency superconducting
single electron transistor (RF-SSET) with an on-chip superconducting LC
matching network consisting of a spiral inductor L and its capacitance to
ground. The superconducting network has a lower parasitic capacitance and gives
a better matching... | cond-mat.mes-hall | in this letter we describe operation of a radiofrequency superconducting single electron transistor rfsset with an onchip superconducting lc matching network consisting of a spiral inductor l and its capacitance to ground the superconducting network has a lower parasitic capacitance and gives a better matching for the ... | [['in', 'this', 'letter', 'we', 'describe', 'operation', 'of', 'a', 'radiofrequency', 'superconducting', 'single', 'electron', 'transistor', 'rfsset', 'with', 'an', 'onchip', 'superconducting', 'lc', 'matching', 'network', 'consisting', 'of', 'a', 'spiral', 'inductor', 'l', 'and', 'its', 'capacitance', 'to', 'ground', ... | [-0.21039314765483141, 0.10521584618036287, -0.012717836727388203, -0.03659157938323915, -0.03027381539810449, -0.17288379076402635, 0.09521590857766568, 0.35781612518243494, -0.16462499984540047, -0.326890671281144, -0.004828524628974265, -0.307619094485417, -0.08562677715905011, 0.21629673086106777, -0.06970126599801... |
708.1008 | An Isotropic Metric | An isotropic metric for a black hole and a better vacuum condition \nabla^2
V_G =0 are presented which yield distinct terms for the energy densities of
ordinary matter and gravitational fields in the Einstein tensor (G^44 =-g^2
(2\nabla^2 V_G +(\nabla V_G)^2)) This model resolves an inconsistency between
electromagne... | physics.gen-ph | an isotropic metric for a black hole and a better vacuum condition nabla2 v_g 0 are presented which yield distinct terms for the energy densities of ordinary matter and gravitational fields in the einstein tensor g44 g2 2nabla2 v_g nabla v_g2 this model resolves an inconsistency between electromagnetism and gravity in ... | [['an', 'isotropic', 'metric', 'for', 'a', 'black', 'hole', 'and', 'a', 'better', 'vacuum', 'condition', 'nabla2', 'v_g', '0', 'are', 'presented', 'which', 'yield', 'distinct', 'terms', 'for', 'the', 'energy', 'densities', 'of', 'ordinary', 'matter', 'and', 'gravitational', 'fields', 'in', 'the', 'einstein', 'tensor', ... | [-0.19588726252051336, 0.09867624539723953, -0.09425535472109914, 0.10466913219341742, -0.0893195395757045, -0.12879086736190531, -0.08294230904430151, 0.2896758347350572, -0.20558256464345115, -0.3537281477025577, -0.015472027044078069, -0.286478401986616, -0.06959847395441361, 0.12106811790394463, -0.0572212189569004... |
708.1009 | An SU(5)$\otimes$Z_{13} Grand Unification Model | We propose an SU(5) grand unified model with an invisible axion and the
unification of the three coupling constants which is in agreement with the
values, at $M_Z$, of $\alpha$, $\alpha_s$, and $\sin^2\theta_W$. A discrete,
anomalous, $Z_{13}$ symmetry implies that the Peccei-Quinn symmetry is an
automatic symmetry o... | hep-ph | we propose an su5 grand unified model with an invisible axion and the unification of the three coupling constants which is in agreement with the values at m_z of alpha alpha_s and sin2theta_w a discrete anomalous z_13 symmetry implies that the pecceiquinn symmetry is an automatic symmetry of the classical lagrangian pr... | [['we', 'propose', 'an', 'su5', 'grand', 'unified', 'model', 'with', 'an', 'invisible', 'axion', 'and', 'the', 'unification', 'of', 'the', 'three', 'coupling', 'constants', 'which', 'is', 'in', 'agreement', 'with', 'the', 'values', 'at', 'm_z', 'of', 'alpha', 'alpha_s', 'and', 'sin2theta_w', 'a', 'discrete', 'anomalous... | [-0.1594605374403975, 0.24288084229218923, -0.06394828935153782, 0.1376346566841345, -0.09824368479576978, -0.13652094961726108, 0.0025560857558792286, 0.31110599308528686, -0.23963510586287487, -0.32331907920200714, 0.09296422568044033, -0.20185865079137413, -0.06444665181704543, 0.08146136618346314, 0.007873490681363... |
708.101 | Search for a pentaquark decaying to Cascade- pi- | We present a search for a pentaquark decaying strongly to $\Xi^-\pi^-$ in
$\gamma N$ collisions at a center-of-mass energy up to 25 GeV/c^2. Finding no
evidence for such a state in the mass range of 1480 MeV/c^2 to 2400 MeV/c^2, we
set limits on the yield and on the cross section times branching ratio relative
to $\X... | hep-ex | we present a search for a pentaquark decaying strongly to xipi in gamma n collisions at a centerofmass energy up to 25 gevc2 finding no evidence for such a state in the mass range of 1480 mevc2 to 2400 mevc2 we set limits on the yield and on the cross section times branching ratio relative to xi15300 | [['we', 'present', 'a', 'search', 'for', 'a', 'pentaquark', 'decaying', 'strongly', 'to', 'xipi', 'in', 'gamma', 'n', 'collisions', 'at', 'a', 'centerofmass', 'energy', 'up', 'to', '25', 'gevc2', 'finding', 'no', 'evidence', 'for', 'such', 'a', 'state', 'in', 'the', 'mass', 'range', 'of', '1480', 'mevc2', 'to', '2400',... | [-0.10874143045236308, 0.18792086177946707, -0.054672922546926295, 0.08272918436284128, 0.005068668883228511, -0.055625273290564096, 0.12126352126187269, 0.35694197148672846, -0.12774708608916976, -0.36503807827830315, -0.041897989870784316, -0.3505214587213439, 0.11648907218732986, 0.18963415456298544, 0.0961786816468... |
708.1011 | Resonance scattering in the X-ray emission line profiles of Zeta Puppis | We present XMM-Newton Reflection Grating Spectrometer observations of pairs
of X-ray emission line profiles from the O star Zeta Pup that originate from
the same He-like ion. The two profiles in each pair have different shapes and
cannot both be consistently fit by models assuming the same wind parameters. We
show th... | astro-ph | we present xmmnewton reflection grating spectrometer observations of pairs of xray emission line profiles from the o star zeta pup that originate from the same helike ion the two profiles in each pair have different shapes and cannot both be consistently fit by models assuming the same wind parameters we show that the ... | [['we', 'present', 'xmmnewton', 'reflection', 'grating', 'spectrometer', 'observations', 'of', 'pairs', 'of', 'xray', 'emission', 'line', 'profiles', 'from', 'the', 'o', 'star', 'zeta', 'pup', 'that', 'originate', 'from', 'the', 'same', 'helike', 'ion', 'the', 'two', 'profiles', 'in', 'each', 'pair', 'have', 'different... | [-0.047023311996187166, 0.10812358357246936, -0.08497195015478087, 0.10707706643550796, -0.0843281525931519, -0.15841845541415134, 0.012211423380095072, 0.47275489140448607, -0.22344856993771914, -0.31934836688708135, 0.039153519785031676, -0.29837924535349597, -0.05928851500168208, 0.18420341465160192, 0.0149236528466... |
708.1012 | Spin-exchange relaxation free magnetometry with Cs vapor | We describe a Cs atomic magnetometer operating in the spin-exchange
relaxation-free (SERF) regime. With a vapor cell temperature of
$103^\circ\rm{C}$ we achieve intrinsic magnetic resonance widths $\Delta B=17
{\rm \mu G}$ corresponding to an electron spin-relaxation rate of $300 {\rm
s^{-1}}$ when the spin-exchange ... | physics.atom-ph | we describe a cs atomic magnetometer operating in the spinexchange relaxationfree serf regime with a vapor cell temperature of 103circrmc we achieve intrinsic magnetic resonance widths delta b17 rm mu g corresponding to an electron spinrelaxation rate of 300 rm s1 when the spinexchange rate is gamma_se14000 rm s1 we al... | [['we', 'describe', 'a', 'cs', 'atomic', 'magnetometer', 'operating', 'in', 'the', 'spinexchange', 'relaxationfree', 'serf', 'regime', 'with', 'a', 'vapor', 'cell', 'temperature', 'of', '103circrmc', 'we', 'achieve', 'intrinsic', 'magnetic', 'resonance', 'widths', 'delta', 'b17', 'rm', 'mu', 'g', 'corresponding', 'to',... | [-0.13676253947847355, 0.18783792056345866, 0.029472523456894037, 0.007191932451265945, 0.021987959062387274, -0.13305758477800972, 0.07484123845746023, 0.42684403941856597, -0.20271353306996776, -0.2893056275367033, 0.0590438428403641, -0.2907669479577384, 0.0014393211917137713, 0.22773332353571327, -0.003576409266014... |
708.1013 | Noise-induced energy excitation by a general environment | We analyze the effects that general environments, namely ohmic and non-ohmic,
at zero and high temperature induce over a quantum Brownian particle. We state
that the evolution of the system can be summarized in terms of two main
environmental induced physical phenomena: decoherence and energy activation. In
this arti... | quant-ph cond-mat.other hep-ph hep-th | we analyze the effects that general environments namely ohmic and nonohmic at zero and high temperature induce over a quantum brownian particle we state that the evolution of the system can be summarized in terms of two main environmental induced physical phenomena decoherence and energy activation in this article we s... | [['we', 'analyze', 'the', 'effects', 'that', 'general', 'environments', 'namely', 'ohmic', 'and', 'nonohmic', 'at', 'zero', 'and', 'high', 'temperature', 'induce', 'over', 'a', 'quantum', 'brownian', 'particle', 'we', 'state', 'that', 'the', 'evolution', 'of', 'the', 'system', 'can', 'be', 'summarized', 'in', 'terms', ... | [-0.14807792605620018, 0.2292091465760332, -0.10805071803411068, 0.09081574761146356, 0.003716306348295906, -0.10284351692476039, 0.021343809125143328, 0.35971361042672323, -0.2814595672903182, -0.25838278363682804, 0.06264356122045672, -0.2518050890427696, -0.15502103270750633, 0.19999919720053014, -0.0151235380245349... |
708.1014 | Evolution of Gravitational Perturbations in Non-Commutative Inflation | We consider the non-commutative inflation model of [3] in which it is the
unconventional dispersion relation for regular radiation which drives the
accelerated expansion of space. In this model, we study the evolution of linear
cosmological perturbations through the transition between the phase of
accelerated expansi... | hep-th astro-ph gr-qc hep-ph | we consider the noncommutative inflation model of 3 in which it is the unconventional dispersion relation for regular radiation which drives the accelerated expansion of space in this model we study the evolution of linear cosmological perturbations through the transition between the phase of accelerated expansion and ... | [['we', 'consider', 'the', 'noncommutative', 'inflation', 'model', 'of', '3', 'in', 'which', 'it', 'is', 'the', 'unconventional', 'dispersion', 'relation', 'for', 'regular', 'radiation', 'which', 'drives', 'the', 'accelerated', 'expansion', 'of', 'space', 'in', 'this', 'model', 'we', 'study', 'the', 'evolution', 'of', ... | [-0.17721484303807042, 0.23788838448576377, -0.112271151009846, 0.06674186214113834, -0.07384527618945627, -0.11157169314561882, -0.04941800380494077, 0.2889598623112581, -0.2798264782010977, -0.2639124758214086, 0.10262378489990094, -0.24751816734487375, -0.14135292553148426, 0.16385157511359758, 0.02456551279033442, ... |
708.1015 | Prime numbers with Beatty sequences | A study of certain Hamiltonian systems has lead Y. Long to conjecture the
existence of infinitely many primes of the form $p=2[\alpha n]+1$, where
$1<\alpha<2$ is a fixed irrational number. An argument of P. Ribenboim coupled
with classical results about the distribution of fractional parts of irrational
multiples of... | math.NT | a study of certain hamiltonian systems has lead y long to conjecture the existence of infinitely many primes of the form p2alpha n1 where 1alpha2 is a fixed irrational number an argument of p ribenboim coupled with classical results about the distribution of fractional parts of irrational multiples of primes in an arit... | [['a', 'study', 'of', 'certain', 'hamiltonian', 'systems', 'has', 'lead', 'y', 'long', 'to', 'conjecture', 'the', 'existence', 'of', 'infinitely', 'many', 'primes', 'of', 'the', 'form', 'p2alpha', 'n1', 'where', '1alpha2', 'is', 'a', 'fixed', 'irrational', 'number', 'an', 'argument', 'of', 'p', 'ribenboim', 'coupled', ... | [-0.2286549968532873, 0.1690866422420152, -0.09685007811144546, 0.06201224475840313, -0.01798630659414576, -0.21005507861436518, 0.014561393501719942, 0.27803334013593417, -0.22965770311032732, -0.2556741592319061, 0.04783244657899356, -0.2999865462348141, -0.1374073568041678, 0.23065333420203793, -0.06938444220081523,... |
708.1016 | Rotating Black Holes on Codimension-2 Branes | It has recently been demonstrated that certain types of non-tensional
stress-energy can live on tensional codimension-2 branes, including
gravitational shockwaves and small Schwarzschild black holes. In this note we
generalize the earlier Schwarzschild results, and construct the exact
gravitational fields of small ro... | hep-th astro-ph gr-qc hep-ph | it has recently been demonstrated that certain types of nontensional stressenergy can live on tensional codimension2 branes including gravitational shockwaves and small schwarzschild black holes in this note we generalize the earlier schwarzschild results and construct the exact gravitational fields of small rotating b... | [['it', 'has', 'recently', 'been', 'demonstrated', 'that', 'certain', 'types', 'of', 'nontensional', 'stressenergy', 'can', 'live', 'on', 'tensional', 'codimension2', 'branes', 'including', 'gravitational', 'shockwaves', 'and', 'small', 'schwarzschild', 'black', 'holes', 'in', 'this', 'note', 'we', 'generalize', 'the',... | [-0.17140636105950063, 0.14740916290775097, -0.08868343635467735, 0.12929778039102724, -0.12397720550390831, -0.1346935212816051, -0.05218571111747235, 0.30434427781102175, -0.1298476734733176, -0.279095203285078, 0.08077317403048034, -0.3043707717312865, -0.08217705149870344, 0.19852474221915622, -0.0685674683604191, ... |
708.1017 | On the injectivity of the X-ray transform for Anosov thermostats | We consider Anosov thermostats on a closed surface and the X-ray transform on
functions which are up to degree two in the velocities. We show that the
subspace where the X-ray transform fails to be s-injective is finite
dimensional. Furthermore, if the surface is negatively curved and the
thermostat is pure Gaussian ... | math.DS | we consider anosov thermostats on a closed surface and the xray transform on functions which are up to degree two in the velocities we show that the subspace where the xray transform fails to be sinjective is finite dimensional furthermore if the surface is negatively curved and the thermostat is pure gaussian ie no ma... | [['we', 'consider', 'anosov', 'thermostats', 'on', 'a', 'closed', 'surface', 'and', 'the', 'xray', 'transform', 'on', 'functions', 'which', 'are', 'up', 'to', 'degree', 'two', 'in', 'the', 'velocities', 'we', 'show', 'that', 'the', 'subspace', 'where', 'the', 'xray', 'transform', 'fails', 'to', 'be', 'sinjective', 'is'... | [-0.08104785156225966, 0.20533498266952172, -0.1053049327024529, 0.07679499361491311, -0.07700338224399715, -0.12432679890715066, -0.034036628680393824, 0.4615092522674991, -0.28440846631964367, -0.1856000147789957, 0.11130443780735556, -0.3106414435371276, -0.14325770757521591, 0.23133294201726395, -0.068116751978279,... |
708.1018 | Normal State Nernst Effect in Electron-doped Pr2-xCexCuO4:
Superconducting Fluctuations and Two-band Transport | We report a systematic study of normal state Nernst effect in the
electron-doped cuprates Pr$_{2-x}$Ce$_x$CuO$_{4-\delta}$ over a wide range of
doping (0.05$\leq x \leq$0.21) and temperature. At low temperatures, we
observed a notable vortex Nernst signal above T$_c$ in the underdoped films,
but no such normal state ... | cond-mat.supr-con cond-mat.str-el | we report a systematic study of normal state nernst effect in the electrondoped cuprates pr_2xce_xcuo_4delta over a wide range of doping 005leq x leq021 and temperature at low temperatures we observed a notable vortex nernst signal above t_c in the underdoped films but no such normal state vortex nernst signal is found... | [['we', 'report', 'a', 'systematic', 'study', 'of', 'normal', 'state', 'nernst', 'effect', 'in', 'the', 'electrondoped', 'cuprates', 'pr_2xce_xcuo_4delta', 'over', 'a', 'wide', 'range', 'of', 'doping', '005leq', 'x', 'leq021', 'and', 'temperature', 'at', 'low', 'temperatures', 'we', 'observed', 'a', 'notable', 'vortex'... | [-0.1843223385820987, 0.24373630593832143, -0.03757258325554978, 0.037277617098024005, -0.08988877321655095, -0.1837506914641434, 0.12256976335843586, 0.3364658646614236, -0.2376116389696108, -0.21700432495323613, -0.03696092762402259, -0.4205425857936087, -0.07619161998873632, 0.2481713176085203, -0.022569933927169425... |
708.1019 | 1/Nc Expansion in QCD: Double-Line Counting Rules and the Undeservingly
Discarded U(1) Ghost | The 1/Nc expansion is one of the very few methods we have for generating a
systematic expansion of QCD at the energy scale relevant to hadron structure.
The present formulation of this theory relies on the double-line notation for
calculating the leading order of a diagram in the 1/Nc expansion, where the
local SU(Nc... | hep-ph hep-th nucl-th | the 1nc expansion is one of the very few methods we have for generating a systematic expansion of qcd at the energy scale relevant to hadron structure the present formulation of this theory relies on the doubleline notation for calculating the leading order of a diagram in the 1nc expansion where the local sunc gauge s... | [['the', '1nc', 'expansion', 'is', 'one', 'of', 'the', 'very', 'few', 'methods', 'we', 'have', 'for', 'generating', 'a', 'systematic', 'expansion', 'of', 'qcd', 'at', 'the', 'energy', 'scale', 'relevant', 'to', 'hadron', 'structure', 'the', 'present', 'formulation', 'of', 'this', 'theory', 'relies', 'on', 'the', 'doubl... | [-0.12874581532501536, 0.16195855317321622, -0.10356934244000358, 0.09586040716780098, -0.09458242140915561, -0.051244141211362275, 0.038144973269466434, 0.3271726795424849, -0.17245264148726364, -0.24665749016202101, 0.06880019809379857, -0.24945102904339211, -0.11832365247626174, 0.11423602452604258, 0.03215961088031... |
708.102 | Evidence for a Population of High-Redshift Submillimeter Galaxies from
Interferometric Imaging | We have used the Submillimeter Array to image a flux limited sample of seven
submillimeter galaxies, selected by the AzTEC camera on the JCMT at 1.1 mm, in
the COSMOS field at 890um with 2" resolution. All of the sources - two
radio-bright and five radio-dim - are detected as single point-sources at high
significance... | astro-ph | we have used the submillimeter array to image a flux limited sample of seven submillimeter galaxies selected by the aztec camera on the jcmt at 11 mm in the cosmos field at 890um with 2 resolution all of the sources two radiobright and five radiodim are detected as single pointsources at high significance 6sigma with p... | [['we', 'have', 'used', 'the', 'submillimeter', 'array', 'to', 'image', 'a', 'flux', 'limited', 'sample', 'of', 'seven', 'submillimeter', 'galaxies', 'selected', 'by', 'the', 'aztec', 'camera', 'on', 'the', 'jcmt', 'at', '11', 'mm', 'in', 'the', 'cosmos', 'field', 'at', '890um', 'with', '2', 'resolution', 'all', 'of', ... | [-0.037600898832777105, 0.07001757453901475, -0.033257310942763234, 0.08074889995003416, -0.049871133013298465, -0.10506253918500606, 0.019810989603797007, 0.5090745924228042, -0.07082066026973653, -0.4133917994345345, 0.11557238022920803, -0.3497563654435633, 0.014999572826913122, 0.1859239143079709, 0.009884938999966... |
708.1021 | Codeword Stabilized Quantum Codes | We present a unifying approach to quantum error correcting code design that
encompasses additive (stabilizer) codes, as well as all known examples of
nonadditive codes with good parameters. We use this framework to generate new
codes with superior parameters to any previously known. In particular, we find
((10,18,3))... | quant-ph | we present a unifying approach to quantum error correcting code design that encompasses additive stabilizer codes as well as all known examples of nonadditive codes with good parameters we use this framework to generate new codes with superior parameters to any previously known in particular we find 10183 and 10203 cod... | [['we', 'present', 'a', 'unifying', 'approach', 'to', 'quantum', 'error', 'correcting', 'code', 'design', 'that', 'encompasses', 'additive', 'stabilizer', 'codes', 'as', 'well', 'as', 'all', 'known', 'examples', 'of', 'nonadditive', 'codes', 'with', 'good', 'parameters', 'we', 'use', 'this', 'framework', 'to', 'generat... | [-0.06299670868768142, 0.019741869108894698, -0.04026483421643766, 0.13076655434695286, -0.008286913627615342, -0.24817682194451873, 0.03136726156450235, 0.4142255566011255, -0.28523134577732817, -0.31707833363191007, 0.06074598188547847, -0.2113174345344305, -0.23746317791251037, 0.2763139765261887, -0.150660816640951... |
708.1022 | The Detectability of Neon Fluorescence and Measurement of the Solar
Photospheric Neon Abundance | Monte Carlo calculations of the Ne K$\alpha$ line fluoresced by coronal
x-rays and emitted near the temperature minimum region of the solar atmosphere
have been employed to investigate the use of this feature to measure directly
the solar photospheric Ne abundance. Though very weak, comparison with spectral
line data... | astro-ph | monte carlo calculations of the ne kalpha line fluoresced by coronal xrays and emitted near the temperature minimum region of the solar atmosphere have been employed to investigate the use of this feature to measure directly the solar photospheric ne abundance though very weak comparison with spectral line databases in... | [['monte', 'carlo', 'calculations', 'of', 'the', 'ne', 'kalpha', 'line', 'fluoresced', 'by', 'coronal', 'xrays', 'and', 'emitted', 'near', 'the', 'temperature', 'minimum', 'region', 'of', 'the', 'solar', 'atmosphere', 'have', 'been', 'employed', 'to', 'investigate', 'the', 'use', 'of', 'this', 'feature', 'to', 'measure... | [-0.047111712187166234, 0.17837185391386415, 0.06209425637354073, 0.09444821099693802, 0.026943419049003797, -0.11357687004750833, 0.04411681012348517, 0.4599991891501625, -0.1622892782316172, -0.3976247119997397, 0.008084887722717192, -0.3150889550972926, 0.046119668669788574, 0.15345084282947719, 0.015171909818375007... |
708.1023 | Quaternionic Kahler Manifolds, Constrained Instantons and the Magic
Square: I | The classification of homogeneous quaternionic manifolds has been done by
Alekseevskii, Wolf et al using transitive solvable group of isometries. These
manifolds are not generically symmetric, but there is a subset of quaternionic
manifolds that are symmetric and Einstein. A further subset of these manifolds
are the ... | hep-th math-ph math.MP | the classification of homogeneous quaternionic manifolds has been done by alekseevskii wolf et al using transitive solvable group of isometries these manifolds are not generically symmetric but there is a subset of quaternionic manifolds that are symmetric and einstein a further subset of these manifolds are the magic ... | [['the', 'classification', 'of', 'homogeneous', 'quaternionic', 'manifolds', 'has', 'been', 'done', 'by', 'alekseevskii', 'wolf', 'et', 'al', 'using', 'transitive', 'solvable', 'group', 'of', 'isometries', 'these', 'manifolds', 'are', 'not', 'generically', 'symmetric', 'but', 'there', 'is', 'a', 'subset', 'of', 'quater... | [-0.15915792602838083, 0.1508642946234437, -0.04878224995562652, 0.13975298056856486, -0.08365783112636725, -0.1644499688379609, -0.022404218445514226, 0.41373335220109503, -0.22628402951392967, -0.26326859707997485, 0.1720830718282266, -0.2595718246617704, -0.20769043535047513, 0.17354364443428008, -0.1092937474693675... |
708.1024 | Neutron star magnetospheres: the binary pulsar, Crab and magnetars | A number of disparate observational and theoretical pieces of evidence
indicate that, contrary to the conventional wisdom, neutron stars' closed field
lines are populated by dense, hot plasma and may be responsible for producing
some radio and high energy emission. This conclusion is based on eclipse
modeling of the ... | astro-ph | a number of disparate observational and theoretical pieces of evidence indicate that contrary to the conventional wisdom neutron stars closed field lines are populated by dense hot plasma and may be responsible for producing some radio and high energy emission this conclusion is based on eclipse modeling of the binary ... | [['a', 'number', 'of', 'disparate', 'observational', 'and', 'theoretical', 'pieces', 'of', 'evidence', 'indicate', 'that', 'contrary', 'to', 'the', 'conventional', 'wisdom', 'neutron', 'stars', 'closed', 'field', 'lines', 'are', 'populated', 'by', 'dense', 'hot', 'plasma', 'and', 'may', 'be', 'responsible', 'for', 'pro... | [-0.14513974591594536, 0.2430996318005519, -0.04386459894377334, 0.1082497210885645, -0.11905103416675814, -0.08871167247093854, 0.05751838607093634, 0.393635414024613, -0.20275799464714905, -0.3416646329169891, 0.040090921716427946, -0.24942494544526, -0.04013484746711441, 0.2708015974683979, -0.0623169957852294, -0.0... |
708.1025 | Entanglement Distribution in Pure-State Quantum Networks | We investigate entanglement distribution in pure-state quantum networks. We
consider the case when non-maximally entangled two-qubit pure states are shared
by neighboring nodes of the network. For a given pair of nodes, we investigate
how to generate the maximal entanglement between them by performing local
measureme... | quant-ph | we investigate entanglement distribution in purestate quantum networks we consider the case when nonmaximally entangled twoqubit pure states are shared by neighboring nodes of the network for a given pair of nodes we investigate how to generate the maximal entanglement between them by performing local measurements assi... | [['we', 'investigate', 'entanglement', 'distribution', 'in', 'purestate', 'quantum', 'networks', 'we', 'consider', 'the', 'case', 'when', 'nonmaximally', 'entangled', 'twoqubit', 'pure', 'states', 'are', 'shared', 'by', 'neighboring', 'nodes', 'of', 'the', 'network', 'for', 'a', 'given', 'pair', 'of', 'nodes', 'we', 'i... | [-0.17119036105577834, 0.1551091237080982, -0.016490727919153868, 0.07166666496559629, 0.01974724292922474, -0.2477364884049166, 0.08886540048115421, 0.41450255615636705, -0.2704729152913842, -0.25990467172232457, 0.052151387276535385, -0.2756291843339568, -0.1637405305991706, 0.16144147096783854, -0.059386714374704754... |
708.1026 | The Radio Evolution of SN 2001gd | We present the results of observations of the radio emission from Supernova
2001gd in NGC 5033 from 2002 February 8 through 2006 September 25. The data
were obtained using the Very Large Array at wavelengths of 1.3 cm (22.4 GHz), 2
cm (14.9 GHz), 3.6 cm (8.4 GHz), 6 cm (4.9 GHz), and 20 cm (1.5 GHz), with one
upper l... | astro-ph | we present the results of observations of the radio emission from supernova 2001gd in ngc 5033 from 2002 february 8 through 2006 september 25 the data were obtained using the very large array at wavelengths of 13 cm 224 ghz 2 cm 149 ghz 36 cm 84 ghz 6 cm 49 ghz and 20 cm 15 ghz with one upper limit at 90 cm 03 ghz in a... | [['we', 'present', 'the', 'results', 'of', 'observations', 'of', 'the', 'radio', 'emission', 'from', 'supernova', '2001gd', 'in', 'ngc', '5033', 'from', '2002', 'february', '8', 'through', '2006', 'september', '25', 'the', 'data', 'were', 'obtained', 'using', 'the', 'very', 'large', 'array', 'at', 'wavelengths', 'of', ... | [-0.0430799932991459, 0.0885003088132623, -0.04001434345618458, 0.0531359944236614, -0.07755067698561992, -0.14927804319020838, 0.05464122990050759, 0.4350429603155368, -0.15576695399921356, -0.3531931689343391, 0.14202305072327503, -0.30039898701458395, -0.0333874570138645, 0.20270788322504346, 0.011560166573848946, -... |
708.1027 | Unusual oxygen isotope effects in cuprates -- importance of doping | A recent angle resolved photoelectron spectroscopy (ARPES) study by Douglas
et al. \cite {dessau-comment} on oxygen isotope exchanged
Bi_2Sr_2CaCu_2O$_{8+\delta}$ superconductors reported an absence of isotope
effect at optimal doping, questioning the previous work by us \cite
{gweon-nature}. Here, we report a new re... | cond-mat.supr-con cond-mat.str-el | a recent angle resolved photoelectron spectroscopy arpes study by douglas et al cite dessaucomment on oxygen isotope exchanged bi_2sr_2cacu_2o_8delta superconductors reported an absence of isotope effect at optimal doping questioning the previous work by us cite gweonnature here we report a new result that sheds light ... | [['a', 'recent', 'angle', 'resolved', 'photoelectron', 'spectroscopy', 'arpes', 'study', 'by', 'douglas', 'et', 'al', 'cite', 'dessaucomment', 'on', 'oxygen', 'isotope', 'exchanged', 'bi_2sr_2cacu_2o_8delta', 'superconductors', 'reported', 'an', 'absence', 'of', 'isotope', 'effect', 'at', 'optimal', 'doping', 'question... | [-0.0887085705753108, 0.1701751329623642, -0.03951699317486818, 0.06586753629332731, -0.06872974124050138, -0.136490022563491, 0.19077388035549112, 0.36014119498739555, -0.23326000996888424, -0.31709940220452537, -0.023253411552022128, -0.35680810429833154, -0.13367731693731852, 0.19571346846026222, -0.0857393078521386... |
708.1028 | MTGEN : Mass scale measurements in pair-production at colliders | We introduce a new kinematic event variable MTGEN which can provide
information relating to the mass scales of particles pair-produced at hadronic
and leptonic colliders. The variable is of particular use in events with a
large number of particles in the final state when some of those particles are
massive and not de... | hep-ph | we introduce a new kinematic event variable mtgen which can provide information relating to the mass scales of particles pairproduced at hadronic and leptonic colliders the variable is of particular use in events with a large number of particles in the final state when some of those particles are massive and not detect... | [['we', 'introduce', 'a', 'new', 'kinematic', 'event', 'variable', 'mtgen', 'which', 'can', 'provide', 'information', 'relating', 'to', 'the', 'mass', 'scales', 'of', 'particles', 'pairproduced', 'at', 'hadronic', 'and', 'leptonic', 'colliders', 'the', 'variable', 'is', 'of', 'particular', 'use', 'in', 'events', 'with'... | [-0.09487651965691377, 0.28342967311520195, -0.06963880480882728, 0.137560564908199, -0.09434464790116427, -0.12480181476922106, -0.0189569499432425, 0.31371492658883837, -0.2151710659470725, -0.34209065638103725, 0.09519117999766653, -0.29192535276130094, -0.012481628017405332, 0.12973265324608754, -0.0139625871127818... |
708.1029 | Study of Cabibbo Suppressed Decays of the Ds Charmed-Strange Meson
involving a KS | We study the decay of Ds meson into final states involving a Ks and report
the discovery of Cabibbo suppressed decay modes Ds -> Kspi-pi+pi+ (179 +/- 36
events) and Ds -> Kspi+ (113 +/-26 events). The branching ratios for the new
modes are Gamma(Ds -> Kspi-pi+pi+)/Gamma(Ds -> KsK-pi+pi+) = 0.18 +/- 0.04 +/-
0.05 and ... | hep-ex | we study the decay of ds meson into final states involving a ks and report the discovery of cabibbo suppressed decay modes ds kspipipi 179 36 events and ds kspi 113 26 events the branching ratios for the new modes are gammads kspipipigammads kskpipi 018 004 005 and gammads kspigammads ksk 0104 0024 0013 | [['we', 'study', 'the', 'decay', 'of', 'ds', 'meson', 'into', 'final', 'states', 'involving', 'a', 'ks', 'and', 'report', 'the', 'discovery', 'of', 'cabibbo', 'suppressed', 'decay', 'modes', 'ds', 'kspipipi', '179', '36', 'events', 'and', 'ds', 'kspi', '113', '26', 'events', 'the', 'branching', 'ratios', 'for', 'the', ... | [-0.12528580953585333, 0.2829824881046079, -0.044358234580916665, 0.09600747784134, -0.005654151629035671, -0.12067519146755028, 0.18845816334942356, 0.21739540146275735, -0.12959479632748602, -0.3073659870618333, 0.07136230781907216, -0.42411394518179196, 0.05709741924268504, 0.0875352931713375, 0.04450196254765615, 0... |
708.103 | Discovery of a New Dusty B[e] Star in the Small Magellanic Cloud | We present new optical spectroscopic and archival Spitzer IRAC photometric
observations of a B-type star in the SMC cluster NGC 346, NGC 346:KWBBe 200. We
detect numerous Fe II, [O I], and [Fe II] lines, as well as strong P-Cygni
profile H I emission lines in its optical spectrum. The star's near-IR color
and optical... | astro-ph | we present new optical spectroscopic and archival spitzer irac photometric observations of a btype star in the smc cluster ngc 346 ngc 346kwbbe 200 we detect numerous fe ii o i and fe ii lines as well as strong pcygni profile h i emission lines in its optical spectrum the stars nearir color and optical to ir sed clearl... | [['we', 'present', 'new', 'optical', 'spectroscopic', 'and', 'archival', 'spitzer', 'irac', 'photometric', 'observations', 'of', 'a', 'btype', 'star', 'in', 'the', 'smc', 'cluster', 'ngc', '346', 'ngc', '346kwbbe', '200', 'we', 'detect', 'numerous', 'fe', 'ii', 'o', 'i', 'and', 'fe', 'ii', 'lines', 'as', 'well', 'as', ... | [-0.01388021238895957, 0.04575201846724108, -0.06768636401885977, 0.06363404182126173, -0.13583230334692276, -0.10004860406669859, 0.06105255124051697, 0.517136461688922, -0.14722781537387233, -0.32535900465714246, 0.0488579957289263, -0.31758925872496685, -0.013057369930902497, 0.14028401065152138, -0.0461190838116006... |
708.1031 | Perturbation theory for anisotropic dielectric interfaces, and
application to sub-pixel smoothing of discretized numerical methods | We derive a correct first-order perturbation theory in electromagnetism for
cases where an interface between two anisotropic dielectric materials is
slightly shifted. Most previous perturbative methods give incorrect results for
this case, even to lowest order, because of the complicated discontinuous
boundary condit... | physics.optics physics.comp-ph | we derive a correct firstorder perturbation theory in electromagnetism for cases where an interface between two anisotropic dielectric materials is slightly shifted most previous perturbative methods give incorrect results for this case even to lowest order because of the complicated discontinuous boundary conditions o... | [['we', 'derive', 'a', 'correct', 'firstorder', 'perturbation', 'theory', 'in', 'electromagnetism', 'for', 'cases', 'where', 'an', 'interface', 'between', 'two', 'anisotropic', 'dielectric', 'materials', 'is', 'slightly', 'shifted', 'most', 'previous', 'perturbative', 'methods', 'give', 'incorrect', 'results', 'for', '... | [-0.1253190059982542, 0.07199014159685592, -0.10682601385775048, 0.04323628537004461, -0.09309009082388837, -0.1274097602764094, 0.0047371690495040366, 0.3794213760316976, -0.2710273701590612, -0.2775130547683787, 0.11726944669326012, -0.24065994772858718, -0.1792958150919829, 0.21737101618829813, -0.06448321442144948,... |
708.1032 | Generalized Kaehler Potentials from Supergravity | We consider supersymmetric N=2 solutions with non-vanishing NS three-form.
Building on worldsheet results, we reduce the problem to a single generalized
Monge-Ampere equation on the generalized Kaehler potential K recently
interpreted geometrically by Lindstrom, Rocek, Von Unge and Zabzine. One input
in the procedure... | hep-th | we consider supersymmetric n2 solutions with nonvanishing ns threeform building on worldsheet results we reduce the problem to a single generalized mongeampere equation on the generalized kaehler potential k recently interpreted geometrically by lindstrom rocek von unge and zabzine one input in the procedure is a holom... | [['we', 'consider', 'supersymmetric', 'n2', 'solutions', 'with', 'nonvanishing', 'ns', 'threeform', 'building', 'on', 'worldsheet', 'results', 'we', 'reduce', 'the', 'problem', 'to', 'a', 'single', 'generalized', 'mongeampere', 'equation', 'on', 'the', 'generalized', 'kaehler', 'potential', 'k', 'recently', 'interprete... | [-0.11975325020864817, 0.13326054028200232, -0.06805401827858866, 0.12068821387233669, -0.12553707289208552, -0.20524871028643452, -0.031860296517821414, 0.278039626346655, -0.20490879876503967, -0.2479325716102601, 0.09650370413942684, -0.2503532638492168, -0.18257221674441165, 0.15115291413956516, -0.1019939224385076... |
708.1033 | Double Beta Decay, Majorana Neutrinos, and Neutrino Mass | The theoretical and experimental issues relevant to neutrinoless double-beta
decay are reviewed. The impact that a direct observation of this exotic process
would have on elementary particle physics, nuclear physics, astrophysics and
cosmology is profound. Now that neutrinos are known to have mass and
experiments are... | nucl-ex hep-ph nucl-th | the theoretical and experimental issues relevant to neutrinoless doublebeta decay are reviewed the impact that a direct observation of this exotic process would have on elementary particle physics nuclear physics astrophysics and cosmology is profound now that neutrinos are known to have mass and experiments are becomi... | [['the', 'theoretical', 'and', 'experimental', 'issues', 'relevant', 'to', 'neutrinoless', 'doublebeta', 'decay', 'are', 'reviewed', 'the', 'impact', 'that', 'a', 'direct', 'observation', 'of', 'this', 'exotic', 'process', 'would', 'have', 'on', 'elementary', 'particle', 'physics', 'nuclear', 'physics', 'astrophysics',... | [-0.01843527250457555, 0.23336328666472267, -0.05165800731629133, 0.13787806601811498, -0.0959311437046697, -0.12886221411948404, -0.0016664130380377173, 0.3430483701460539, -0.2167208818718791, -0.3017097829233406, 0.12024018038163319, -0.31515176084341734, -0.11566932879740055, 0.2412757906709395, 0.03388196494800191... |
708.1034 | On deciding stability of multiclass queueing networks under buffer
priority scheduling policies | One of the basic properties of a queueing network is stability. Roughly
speaking, it is the property that the total number of jobs in the network
remains bounded as a function of time. One of the key questions related to the
stability issue is how to determine the exact conditions under which a given
queueing network... | math.PR math.OC | one of the basic properties of a queueing network is stability roughly speaking it is the property that the total number of jobs in the network remains bounded as a function of time one of the key questions related to the stability issue is how to determine the exact conditions under which a given queueing network oper... | [['one', 'of', 'the', 'basic', 'properties', 'of', 'a', 'queueing', 'network', 'is', 'stability', 'roughly', 'speaking', 'it', 'is', 'the', 'property', 'that', 'the', 'total', 'number', 'of', 'jobs', 'in', 'the', 'network', 'remains', 'bounded', 'as', 'a', 'function', 'of', 'time', 'one', 'of', 'the', 'key', 'questions... | [-0.18152377795576005, 0.08385943546230257, -0.05966209002474549, 0.0706864389776966, -0.03722350620642896, -0.1848357412920586, 0.11880711932660072, 0.37450352753294963, -0.26369867658962837, -0.2845239541319277, 0.13639235786471307, -0.21795699762062945, -0.14057683974839572, 0.18965016765450346, -0.15745509721808762... |
708.1035 | Neutrino flavor ratios as diagnostic of solar WIMP annihilation | We consider the neutrino (and antineutrino) flavors arriving at Earth for
neutrinos produced in the annihilation of weakly interacting massive particles
(WIMPs) in the Sun's core. Solar-matter effects on the flavor propagation of
the resulting $\agt$ GeV neutrinos are studied analytically within a
density-matrix form... | hep-ph astro-ph | we consider the neutrino and antineutrino flavors arriving at earth for neutrinos produced in the annihilation of weakly interacting massive particles wimps in the suns core solarmatter effects on the flavor propagation of the resulting agt gev neutrinos are studied analytically within a densitymatrix formalism matter ... | [['we', 'consider', 'the', 'neutrino', 'and', 'antineutrino', 'flavors', 'arriving', 'at', 'earth', 'for', 'neutrinos', 'produced', 'in', 'the', 'annihilation', 'of', 'weakly', 'interacting', 'massive', 'particles', 'wimps', 'in', 'the', 'suns', 'core', 'solarmatter', 'effects', 'on', 'the', 'flavor', 'propagation', 'o... | [-0.0802569221411651, 0.314876882824545, -0.02102415658059883, 0.17170322154486023, -0.04936153660147001, -0.11744862986559948, 0.05133341938249189, 0.32991489572129373, -0.20026475737465482, -0.32319950367372224, -0.008957443779920516, -0.30082240140473004, -0.017680912667981767, 0.16401874146962153, 0.035518401057523... |
708.1036 | Kaehler-Ricci Flow, Morse Theory, and Vacuum Structure Deformation of
N=1 Supersymmetry in Four Dimensions | We address some aspects of four dimensional chiral N=1 supersymmetric
theories on which the scalar manifold is described by K\"ahler geometry and can
further be viewed as K\"ahler-Ricci soliton generating a one-parameter family
of K\"ahler geometries. All couplings and solutions, namely the BPS domain
walls and their... | hep-th math-ph math.DG math.DS math.MP | we address some aspects of four dimensional chiral n1 supersymmetric theories on which the scalar manifold is described by kahler geometry and can further be viewed as kahlerricci soliton generating a oneparameter family of kahler geometries all couplings and solutions namely the bps domain walls and their supersymmetr... | [['we', 'address', 'some', 'aspects', 'of', 'four', 'dimensional', 'chiral', 'n1', 'supersymmetric', 'theories', 'on', 'which', 'the', 'scalar', 'manifold', 'is', 'described', 'by', 'kahler', 'geometry', 'and', 'can', 'further', 'be', 'viewed', 'as', 'kahlerricci', 'soliton', 'generating', 'a', 'oneparameter', 'family'... | [-0.15447827637595332, 0.1164740174419388, -0.10715562668543939, 0.10265811286190499, -0.06838474361561919, -0.16097496325983646, -0.03603472919936917, 0.3465272323462313, -0.2053656136855211, -0.2226517597358508, 0.10889912656397818, -0.26768440433743845, -0.18106632305045514, 0.11603210009017866, -0.08709721760114668... |
708.1037 | A Formulation of the Channel Capacity of Multiple-Access Channel | The necessary and sufficient condition of the channel capacity is rigorously
formulated for the N-user discrete memoryless multiple-access channel (MAC).
The essence of the formulation is to invoke an {\em elementary} MAC where sizes
of input alphabets are not greater than the size of output alphabet. The main
object... | cs.IT math.IT | the necessary and sufficient condition of the channel capacity is rigorously formulated for the nuser discrete memoryless multipleaccess channel mac the essence of the formulation is to invoke an em elementary mac where sizes of input alphabets are not greater than the size of output alphabet the main objective is to d... | [['the', 'necessary', 'and', 'sufficient', 'condition', 'of', 'the', 'channel', 'capacity', 'is', 'rigorously', 'formulated', 'for', 'the', 'nuser', 'discrete', 'memoryless', 'multipleaccess', 'channel', 'mac', 'the', 'essence', 'of', 'the', 'formulation', 'is', 'to', 'invoke', 'an', 'em', 'elementary', 'mac', 'where',... | [-0.200533453254577, 0.09083894354955513, -0.09274845159996081, 0.054213355997960795, -0.055474667768815863, -0.2101117968066212, 0.08919475011746673, 0.3504927223219591, -0.2965453839039101, -0.22744364554288468, 0.11842204450650196, -0.16589073433321627, -0.10825112399316447, 0.16644712659694694, -0.13001378620152965... |
708.1038 | Crossing the phantom divide in brane cosmology with curvature
corrections and brane-bulk energy transfer | We consider the Randall-Sundrum brane-world model with bulk-brane energy
transfer where the Einstein-Hilbert action is modified by curvature correction
terms: a four-dimensional scalar curvature from induced gravity on the brane,
and a five-dimensional Gauss-Bonnet curvature term. It is remarkable that these
curvatur... | astro-ph | we consider the randallsundrum braneworld model with bulkbrane energy transfer where the einsteinhilbert action is modified by curvature correction terms a fourdimensional scalar curvature from induced gravity on the brane and a fivedimensional gaussbonnet curvature term it is remarkable that these curvature terms will... | [['we', 'consider', 'the', 'randallsundrum', 'braneworld', 'model', 'with', 'bulkbrane', 'energy', 'transfer', 'where', 'the', 'einsteinhilbert', 'action', 'is', 'modified', 'by', 'curvature', 'correction', 'terms', 'a', 'fourdimensional', 'scalar', 'curvature', 'from', 'induced', 'gravity', 'on', 'the', 'brane', 'and'... | [-0.10209068195527476, 0.09599026288011704, -0.08630411585397793, 0.11444439420786996, -0.16239168909660567, -0.1491191866186758, -0.014287441110972202, 0.2851648066700859, -0.1923038424535965, -0.3483284762862957, 0.02720409257083454, -0.3264796773366856, -0.05787129717540335, 0.15852811792300958, -0.01778858807220152... |
708.1039 | Ammonia Imaging of the Disks in the NGC 1333 IRAS 4A Protobinary System | The NGC 1333 IRAS 4A protobinary was observed in the ammonia (2, 2) and (3,
3) lines and in the 1.3 cm continuum with a high resolution (about 1.0 arcsec).
The ammonia maps show two compact sources, one for each protostar, and they are
probably protostellar accretion disks. The disk associated with IRAS 4A2 is
seen n... | astro-ph | the ngc 1333 iras 4a protobinary was observed in the ammonia 2 2 and 3 3 lines and in the 13 cm continuum with a high resolution about 10 arcsec the ammonia maps show two compact sources one for each protostar and they are probably protostellar accretion disks the disk associated with iras 4a2 is seen nearly edgeon and... | [['the', 'ngc', '1333', 'iras', '4a', 'protobinary', 'was', 'observed', 'in', 'the', 'ammonia', '2', '2', 'and', '3', '3', 'lines', 'and', 'in', 'the', '13', 'cm', 'continuum', 'with', 'a', 'high', 'resolution', 'about', '10', 'arcsec', 'the', 'ammonia', 'maps', 'show', 'two', 'compact', 'sources', 'one', 'for', 'each'... | [-0.10106686311800414, 0.09922828917718686, -0.030731649341760203, 0.047067849538445276, -0.04079737272960218, -0.11393506326897875, -0.007261294120160694, 0.4663806948069991, -0.1781448460739987, -0.30557861422527244, 0.09986310055947714, -0.2750010399983942, -0.022926092916432852, 0.13037717785217948, -0.036666669993... |
708.104 | The Properties and Evolution of a K-band Selected Sample of Massive
Galaxies at z~0.4 - 2 in the Palomar/DEEP2 Survey | We present the results of a study on the properties and evolution of massive
(M_* > 10^11 M_0) galaxies at z~0.4 - 2 utilising Keck spectroscopy,
near-Infrared Palomar imaging, and Hubble, Chandra, and Spitzer data covering
fields targeted by the DEEP2 galaxy spectroscopic survey. Our sample is K band
selected based ... | astro-ph | we present the results of a study on the properties and evolution of massive m_ 1011 m_0 galaxies at z04 2 utilising keck spectroscopy nearinfrared palomar imaging and hubble chandra and spitzer data covering fields targeted by the deep2 galaxy spectroscopic survey our sample is k band selected based on widearea nir im... | [['we', 'present', 'the', 'results', 'of', 'a', 'study', 'on', 'the', 'properties', 'and', 'evolution', 'of', 'massive', 'm_', '1011', 'm_0', 'galaxies', 'at', 'z04', '2', 'utilising', 'keck', 'spectroscopy', 'nearinfrared', 'palomar', 'imaging', 'and', 'hubble', 'chandra', 'and', 'spitzer', 'data', 'covering', 'fields... | [-0.08933234148108485, 0.1640572232939954, -0.01538695585816265, 0.09967331953836814, -0.05543329324280205, -0.009990370841338657, 0.06078880411243861, 0.46258526541605277, -0.0625679414097376, -0.4032957510863125, 0.04555137295087057, -0.3392532270896685, -0.020470474063503472, 0.22526977487540173, 0.03291159784225942... |
708.1041 | Single-Molecule Device Prototypes for Protein-Based Nanoelectronics:
Negative Differential Resistance and Current Rectification in Oligopeptides | We investigate electrical conduction through individual oligopeptide
molecules thiol-bonded between gold nanocontacts using ab initio and
semi-empirical techniques. Our theory explains for the first time these
molecules' experimentally observed current-voltage characteristics, including
both the magnitude and rectifi... | cond-mat.mes-hall | we investigate electrical conduction through individual oligopeptide molecules thiolbonded between gold nanocontacts using ab initio and semiempirical techniques our theory explains for the first time these molecules experimentally observed currentvoltage characteristics including both the magnitude and rectification o... | [['we', 'investigate', 'electrical', 'conduction', 'through', 'individual', 'oligopeptide', 'molecules', 'thiolbonded', 'between', 'gold', 'nanocontacts', 'using', 'ab', 'initio', 'and', 'semiempirical', 'techniques', 'our', 'theory', 'explains', 'for', 'the', 'first', 'time', 'these', 'molecules', 'experimentally', 'o... | [-0.1289301044779205, 0.08334748343493836, -0.027852297695707295, 0.02666557632103751, -0.038586172110200684, -0.15644048783881, 0.10777674224433972, 0.4318917908859027, -0.2725330045847576, -0.3536062713806765, -0.026010945900579136, -0.29792964849856834, -0.1967654719807302, 0.2553144411620083, 0.018503957486982588, ... |
708.1042 | Exotic Superconducting Properties in the Electron-Hole Compensated Heavy
Fermion `Semimetal' URu2Si2 | We show that the charge and thermal transport measurements on ultraclean
crystals of URu2Si2 reveal a number of unprecedented superconducting
properties. The uniqueness is best highlighted by the peculiar field dependence
of thermal conductivity including the first order transition at Hc2 with a
reduction of entropy ... | cond-mat.supr-con cond-mat.str-el | we show that the charge and thermal transport measurements on ultraclean crystals of uru2si2 reveal a number of unprecedented superconducting properties the uniqueness is best highlighted by the peculiar field dependence of thermal conductivity including the first order transition at hc2 with a reduction of entropy flo... | [['we', 'show', 'that', 'the', 'charge', 'and', 'thermal', 'transport', 'measurements', 'on', 'ultraclean', 'crystals', 'of', 'uru2si2', 'reveal', 'a', 'number', 'of', 'unprecedented', 'superconducting', 'properties', 'the', 'uniqueness', 'is', 'best', 'highlighted', 'by', 'the', 'peculiar', 'field', 'dependence', 'of'... | [-0.21462043505162, 0.165248769324492, -0.07130244057077695, -0.003148782625794411, -0.07563043017597759, -0.09769611569011913, 0.10386575908564469, 0.3297628083937418, -0.2624369575696833, -0.30746774469118787, 0.034089745182598774, -0.3442576711668688, -0.10970214244306964, 0.15802413672208787, 0.03934821908307426, 0... |
708.1043 | Form factors and correlation functions of an interacting spinless
fermion model | Introducing the fermionic R-operator and solutions of the inverse scattering
problem for local fermion operators, we derive a multiple integral
representation for zero-temperature correlation functions of a one-dimensional
interacting spinless fermion model. Correlation functions particularly
considered are the one-p... | cond-mat.stat-mech math-ph math.MP nlin.SI | introducing the fermionic roperator and solutions of the inverse scattering problem for local fermion operators we derive a multiple integral representation for zerotemperature correlation functions of a onedimensional interacting spinless fermion model correlation functions particularly considered are the oneparticle ... | [['introducing', 'the', 'fermionic', 'roperator', 'and', 'solutions', 'of', 'the', 'inverse', 'scattering', 'problem', 'for', 'local', 'fermion', 'operators', 'we', 'derive', 'a', 'multiple', 'integral', 'representation', 'for', 'zerotemperature', 'correlation', 'functions', 'of', 'a', 'onedimensional', 'interacting', ... | [-0.14218403283416867, 0.18357111458256012, -0.07804740896358726, 0.19270751598369645, -0.016103458781558347, -0.15507818034188037, -0.0038430777978690632, 0.3368041952062084, -0.20045917449485376, -0.23321881542453565, 0.0011273785648553308, -0.32417328999635864, -0.15208040574449466, 0.1416975368552067, 0.15449755698... |
708.1044 | Aharonov-Bohm Oscillations in Photoluminescence from Charged Exciton in
Quantum Tubes | The oscillation of photoluminescence peak energies is observed in InAs
quantum tubes depending on the magnetic flux through the tube. The oscillation
is shown to be due to the Aharonov-Bohm effect of a charged exciton in a
quantum tube. No quadratic shift in photoluminescence peak energies is
observed, which is a cha... | cond-mat.mes-hall | the oscillation of photoluminescence peak energies is observed in inas quantum tubes depending on the magnetic flux through the tube the oscillation is shown to be due to the aharonovbohm effect of a charged exciton in a quantum tube no quadratic shift in photoluminescence peak energies is observed which is a character... | [['the', 'oscillation', 'of', 'photoluminescence', 'peak', 'energies', 'is', 'observed', 'in', 'inas', 'quantum', 'tubes', 'depending', 'on', 'the', 'magnetic', 'flux', 'through', 'the', 'tube', 'the', 'oscillation', 'is', 'shown', 'to', 'be', 'due', 'to', 'the', 'aharonovbohm', 'effect', 'of', 'a', 'charged', 'exciton... | [-0.14938983226201727, 0.23912720366522833, -0.04958397268817045, 0.05100473868019501, -0.010713839005894852, -0.1212782591405878, 0.013161693703032273, 0.4316713346195394, -0.2111666415669564, -0.2951036550482546, 0.003770734995023172, -0.2717754681041275, -0.0571387117067217, 0.22807680016410523, 0.02006068257479996,... |
708.1045 | HCN to HCO^+ Millimeter Line Diagnostics of AGN Molecular Torus I :
Radiative Transfer Modeling | We explore millimeter line diagnostics of an obscuring molecular torus
modeled by a hydrodynamic simulation with three-dimensional nonLTE radiative
transfer calculations. Based on the results of high-resolution hydrodynamic
simulation of the molecular torus around an AGN, we calculate intensities of
HCN and HCO^{+} r... | astro-ph | we explore millimeter line diagnostics of an obscuring molecular torus modeled by a hydrodynamic simulation with threedimensional nonlte radiative transfer calculations based on the results of highresolution hydrodynamic simulation of the molecular torus around an agn we calculate intensities of hcn and hco rotational ... | [['we', 'explore', 'millimeter', 'line', 'diagnostics', 'of', 'an', 'obscuring', 'molecular', 'torus', 'modeled', 'by', 'a', 'hydrodynamic', 'simulation', 'with', 'threedimensional', 'nonlte', 'radiative', 'transfer', 'calculations', 'based', 'on', 'the', 'results', 'of', 'highresolution', 'hydrodynamic', 'simulation',... | [-0.09265068868040352, 0.06902046489152494, -0.022040364999128016, 0.08039058151434322, -0.021659671147599032, -0.0759808406907771, 0.001604815611713811, 0.46510959017139514, -0.16858665456407165, -0.299770676257628, 0.05073652532821717, -0.2213235713958152, -0.0507984370152515, 0.1628419631369118, 0.0790068146184479, ... |
708.1046 | Probe of dark galaxies via disturbed/ lopsided isolated galaxies | Searching for lopsided/interacting objects among ~1500 isolated galaxies
yields only eight strongly disturbed galaxies which may be explained as a
result of their interaction with massive dark objects. We present results of
spectral and photometric observations of these galaxies performed with the 6-m
telescope that ... | astro-ph | searching for lopsidedinteracting objects among 1500 isolated galaxies yields only eight strongly disturbed galaxies which may be explained as a result of their interaction with massive dark objects we present results of spectral and photometric observations of these galaxies performed with the 6m telescope that lead t... | [['searching', 'for', 'lopsidedinteracting', 'objects', 'among', '1500', 'isolated', 'galaxies', 'yields', 'only', 'eight', 'strongly', 'disturbed', 'galaxies', 'which', 'may', 'be', 'explained', 'as', 'a', 'result', 'of', 'their', 'interaction', 'with', 'massive', 'dark', 'objects', 'we', 'present', 'results', 'of', '... | [-0.11451815668907431, 0.10052540390407322, -0.11320286254502004, 0.0983721130286102, -0.13227395895497734, -0.08001697460982811, 0.008719018751030995, 0.4331195080583846, -0.05903038603288156, -0.43781999926324244, 0.03638063156459895, -0.2757139157296883, -0.03671677320919655, 0.23063443461433053, -0.0031693491187912... |
708.1047 | Special K\"ahler-Ricci potentials and Ricci solitons | On a manifold of dimension at least six, let $(g,\tau)$ be a pair consisting
of a K\"ahler metric g which is locally K\"ahler irreducible, and a nonconstant
smooth function $\tau$. Off the zero set of $\tau$, if the metric
$\hat{g}=g/\tau^2$ is a gradient Ricci soliton which has soliton function
$1/\tau$, we show tha... | math.DG | on a manifold of dimension at least six let gtau be a pair consisting of a kahler metric g which is locally kahler irreducible and a nonconstant smooth function tau off the zero set of tau if the metric hatggtau2 is a gradient ricci soliton which has soliton function 1tau we show that hatg is kahler with respect to ano... | [['on', 'a', 'manifold', 'of', 'dimension', 'at', 'least', 'six', 'let', 'gtau', 'be', 'a', 'pair', 'consisting', 'of', 'a', 'kahler', 'metric', 'g', 'which', 'is', 'locally', 'kahler', 'irreducible', 'and', 'a', 'nonconstant', 'smooth', 'function', 'tau', 'off', 'the', 'zero', 'set', 'of', 'tau', 'if', 'the', 'metric'... | [-0.1995608350972979, 0.0899555912909617, -0.12882279923526954, 0.043930510227845714, -0.11342743283869941, -0.18020326091076128, -0.01978932334046157, 0.3402536008933573, -0.2655239964742924, -0.18175778062951942, 0.08625993065585788, -0.26895887054367884, -0.15322741411114468, 0.17339286924062566, -0.0676516386971787... |
708.1048 | Singular and tangent slit solutions to the Loewner equation | We consider the Loewner differential equation generating univalent maps of
the unit disk (or of the upper half-plane) onto itself minus a single slit. We
prove that the circular slits, tangent to the real axis are generated by
H\"older continuous driving terms with exponent 1/3 in the Loewner equation.
Singular solut... | math.CV | we consider the loewner differential equation generating univalent maps of the unit disk or of the upper halfplane onto itself minus a single slit we prove that the circular slits tangent to the real axis are generated by holder continuous driving terms with exponent 13 in the loewner equation singular solutions are de... | [['we', 'consider', 'the', 'loewner', 'differential', 'equation', 'generating', 'univalent', 'maps', 'of', 'the', 'unit', 'disk', 'or', 'of', 'the', 'upper', 'halfplane', 'onto', 'itself', 'minus', 'a', 'single', 'slit', 'we', 'prove', 'that', 'the', 'circular', 'slits', 'tangent', 'to', 'the', 'real', 'axis', 'are', '... | [-0.18006999958568895, 0.07093984598267666, -0.0251442176051287, 0.03461819016341854, -0.08815666617789555, -0.11227421075249956, -0.0405623409241228, 0.3566550790450313, -0.3468699595353133, -0.1624733474840161, 0.12101618932153453, -0.2993104040727649, -0.0883044968851068, 0.24921749306278645, -0.049655443791982154, ... |
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