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 |
|---|---|---|---|---|---|---|
708.2749 | The Sloan Digital Sky Survey-II Supernova Survey: Technical Summary | The Sloan Digital Sky Survey-II (SDSS-II) has embarked on a multi-year
project to identify and measure light curves for intermediate-redshift (0.05 <
z < 0.35) Type Ia supernovae (SNe Ia) using repeated five-band (ugriz) imaging
over an area of 300 sq. deg. The survey region is a stripe 2.5 degrees wide
centered on t... | astro-ph | the sloan digital sky surveyii sdssii has embarked on a multiyear project to identify and measure light curves for intermediateredshift 005 z 035 type ia supernovae sne ia using repeated fiveband ugriz imaging over an area of 300 sq deg the survey region is a stripe 25 degrees wide centered on the celestial equator in ... | [['the', 'sloan', 'digital', 'sky', 'surveyii', 'sdssii', 'has', 'embarked', 'on', 'a', 'multiyear', 'project', 'to', 'identify', 'and', 'measure', 'light', 'curves', 'for', 'intermediateredshift', '005', 'z', '035', 'type', 'ia', 'supernovae', 'sne', 'ia', 'using', 'repeated', 'fiveband', 'ugriz', 'imaging', 'over', '... | [-0.08406994758976852, 0.04698695853362644, -0.035195103665927846, 0.059831004756103666, -0.14852348417851466, -0.09946132005116314, 0.09697089402292551, 0.40801319603485114, -0.13663654510176512, -0.3399092099648349, 0.11244979825723746, -0.371481391487225, -0.023040193827390403, 0.25793830878148805, -0.04621363467836... |
708.275 | The Sloan Digital Sky Survey-II Supernova Survey: Search Algorithm and
Follow-up Observations | The Sloan Digital Sky Survey-II Supernova Survey has identified a large
number of new transient sources in a 300 sq. deg. region along the celestial
equator during its first two seasons of a three-season campaign. Multi-band
(ugriz) light curves were measured for most of the sources, which include solar
system object... | astro-ph | the sloan digital sky surveyii supernova survey has identified a large number of new transient sources in a 300 sq deg region along the celestial equator during its first two seasons of a threeseason campaign multiband ugriz light curves were measured for most of the sources which include solar system objects galactic ... | [['the', 'sloan', 'digital', 'sky', 'surveyii', 'supernova', 'survey', 'has', 'identified', 'a', 'large', 'number', 'of', 'new', 'transient', 'sources', 'in', 'a', '300', 'sq', 'deg', 'region', 'along', 'the', 'celestial', 'equator', 'during', 'its', 'first', 'two', 'seasons', 'of', 'a', 'threeseason', 'campaign', 'mul... | [-0.07135445300179223, 0.046101458206281275, -0.032392877570043006, 0.08611225576657389, -0.15102944755926728, -0.09188781276629823, 0.12373420961563372, 0.4187694640292062, -0.1584173065232527, -0.3568927456780026, 0.12808876767392374, -0.3663328886549506, -0.030717734168801043, 0.26473663139363957, -0.032730915478281... |
708.2751 | Scale dependent superconductor-insulator transition | We study the disorder driven superconductor to insulator transition in
amorphous films of high carrier-concentration indium-oxide. Using thin films
with various sizes and aspect ratios we show that the `critical'
sheet-resistance $R_{{\small \square}}$ depends systematically on sample
geometry; superconductivity disa... | cond-mat.dis-nn cond-mat.supr-con | we study the disorder driven superconductor to insulator transition in amorphous films of high carrierconcentration indiumoxide using thin films with various sizes and aspect ratios we show that the critical sheetresistance r_small square depends systematically on sample geometry superconductivity disappears when r_sma... | [['we', 'study', 'the', 'disorder', 'driven', 'superconductor', 'to', 'insulator', 'transition', 'in', 'amorphous', 'films', 'of', 'high', 'carrierconcentration', 'indiumoxide', 'using', 'thin', 'films', 'with', 'various', 'sizes', 'and', 'aspect', 'ratios', 'we', 'show', 'that', 'the', 'critical', 'sheetresistance', '... | [-0.1268672420182961, 0.23840839495673646, 0.0010265670181519684, 0.010906828384064994, -0.020588799454699987, -0.1766008135980402, 0.09083321211517029, 0.40869933358211624, -0.20646596702629294, -0.29044440789041165, 0.07937776401970835, -0.32780602373097134, -0.09130481433594363, 0.19391314500485193, 0.00132989836053... |
708.2752 | Cubic points on cubic curves and the Brauer-Manin obstruction on K3
surfaces | We show that if over some number field there exists a certain diagonal plane
cubic curve that is locally solvable everywhere, but that does not have points
over any cubic galois extension of the number field, then the algebraic part of
the Brauer-Manin obstruction is not the only obstruction to the Hasse principle
fo... | math.NT math.AG | we show that if over some number field there exists a certain diagonal plane cubic curve that is locally solvable everywhere but that does not have points over any cubic galois extension of the number field then the algebraic part of the brauermanin obstruction is not the only obstruction to the hasse principle for k3 ... | [['we', 'show', 'that', 'if', 'over', 'some', 'number', 'field', 'there', 'exists', 'a', 'certain', 'diagonal', 'plane', 'cubic', 'curve', 'that', 'is', 'locally', 'solvable', 'everywhere', 'but', 'that', 'does', 'not', 'have', 'points', 'over', 'any', 'cubic', 'galois', 'extension', 'of', 'the', 'number', 'field', 'th... | [-0.25929631340633413, 0.0767507502044152, -0.12941868184134364, 0.07615086067484558, -0.17544435915936316, -0.1511243820506414, 0.00024228837407593216, 0.3460158899293414, -0.33187774631993044, -0.22009062316335207, 0.11285123434416684, -0.23072231175111874, -0.19742001882072405, 0.22977184281418367, -0.12152804011462... |
708.2753 | Dynamical quantum phase transitions in the dissipative
Lipkin-Meshkov-Glick model and proposed realization in optical cavity QED | We present an optical cavity QED configuration that is described by a
dissipative version of the Lipkin-Meshkov-Glick model of an infinitely
coordinated spin system. This open quantum system exhibits both first- and
second-order non-equilibrium quantum phase transitions as a single, effective
field parameter is varie... | quant-ph cond-mat.other | we present an optical cavity qed configuration that is described by a dissipative version of the lipkinmeshkovglick model of an infinitely coordinated spin system this open quantum system exhibits both first and secondorder nonequilibrium quantum phase transitions as a single effective field parameter is varied light e... | [['we', 'present', 'an', 'optical', 'cavity', 'qed', 'configuration', 'that', 'is', 'described', 'by', 'a', 'dissipative', 'version', 'of', 'the', 'lipkinmeshkovglick', 'model', 'of', 'an', 'infinitely', 'coordinated', 'spin', 'system', 'this', 'open', 'quantum', 'system', 'exhibits', 'both', 'first', 'and', 'secondord... | [-0.2220797575197168, 0.22225397612783127, -0.07718172002702005, -0.0027243474665622686, 0.03127716438076089, -0.19675892317992827, 0.005505460059447657, 0.3446531089998427, -0.23609713081359154, -0.240192140382345, 0.012785114347934723, -0.2891575252075517, -0.14116690674471477, 0.22522833789255292, 0.0424447435264786... |
708.2754 | Convergence of random zeros on complex manifolds | We show that the zeros of random sequences of Gaussian systems of polynomials
of increasing degree almost surely converge to the expected limit distribution
under very general hypotheses. In particular, the normalized distribution of
zeros of systems of m polynomials of degree N, orthonormalized on a regular
compact ... | math.CV math.AG math.PR | we show that the zeros of random sequences of gaussian systems of polynomials of increasing degree almost surely converge to the expected limit distribution under very general hypotheses in particular the normalized distribution of zeros of systems of m polynomials of degree n orthonormalized on a regular compact subse... | [['we', 'show', 'that', 'the', 'zeros', 'of', 'random', 'sequences', 'of', 'gaussian', 'systems', 'of', 'polynomials', 'of', 'increasing', 'degree', 'almost', 'surely', 'converge', 'to', 'the', 'expected', 'limit', 'distribution', 'under', 'very', 'general', 'hypotheses', 'in', 'particular', 'the', 'normalized', 'distr... | [-0.20227526439189472, 0.1254981645684251, -0.1032857058898491, 0.012058354462223017, 0.04106628472971566, -0.1284451377030243, 0.07387432425885516, 0.326583981870071, -0.25355427117799134, -0.20118222473298802, 0.06893666371915434, -0.32481494376107173, -0.11411902849452898, 0.13829874366124653, -0.03005089043119155, ... |
708.2755 | Higgs bosons of the NMSSM with explicit CP violation at the ILC | We study the Higgs sector of the next-to-minimal supersymmetric standard
model (NMSSM) with explicit CP violation at the one-loop level, where the
radiative corrections due to the quarks and squarks of the third generation are
taken into account. We expect that, within a reasonable region of the parameter
space of th... | hep-ph | we study the higgs sector of the nexttominimal supersymmetric standard model nmssm with explicit cp violation at the oneloop level where the radiative corrections due to the quarks and squarks of the third generation are taken into account we expect that within a reasonable region of the parameter space of the present ... | [['we', 'study', 'the', 'higgs', 'sector', 'of', 'the', 'nexttominimal', 'supersymmetric', 'standard', 'model', 'nmssm', 'with', 'explicit', 'cp', 'violation', 'at', 'the', 'oneloop', 'level', 'where', 'the', 'radiative', 'corrections', 'due', 'to', 'the', 'quarks', 'and', 'squarks', 'of', 'the', 'third', 'generation',... | [-0.05832718796811478, 0.23980301085772904, -0.01615158162285509, 0.12763534492773412, -0.013244085720480355, -0.16478537037145607, 0.04640179900533715, 0.3145999907797506, -0.23053065242873894, -0.2665419329612971, 0.02078263536718306, -0.3269896318886949, 0.005758629470175609, 0.12902882597014934, 0.11565760933766331... |
708.2756 | Long-term X-ray changes in the emission from the anomalous X-ray pulsar
4U 0142+61 | We present results obtained from X-ray observations of the anomalous X-ray
pulsar (AXP) 4U 0142+61 taken between 2000-2007 using XMM-Newton, Chandra and
Swift. In observations taken before 2006, the pulse profile is observed to
become more sinusoidal and the pulsed fraction increased with time. These
results confirm ... | astro-ph | we present results obtained from xray observations of the anomalous xray pulsar axp 4u 014261 taken between 20002007 using xmmnewton chandra and swift in observations taken before 2006 the pulse profile is observed to become more sinusoidal and the pulsed fraction increased with time these results confirm those derived... | [['we', 'present', 'results', 'obtained', 'from', 'xray', 'observations', 'of', 'the', 'anomalous', 'xray', 'pulsar', 'axp', '4u', '014261', 'taken', 'between', '20002007', 'using', 'xmmnewton', 'chandra', 'and', 'swift', 'in', 'observations', 'taken', 'before', '2006', 'the', 'pulse', 'profile', 'is', 'observed', 'to'... | [-0.04898012452661836, 0.11413516663069459, -0.06949124929087702, 0.0969248830282595, -0.08953785171712904, -0.0964815617131535, 0.07277470209325353, 0.4877239112121364, -0.17425534220140737, -0.3941650035752294, 0.09503216794497954, -0.3568695268232356, -0.039898632695743196, 0.2726407954634245, -0.02542942331223609, ... |
708.2757 | Twisted automorphisms of Hopf algebras | Twisted homomorphisms of bialgebras are bialgebra homomorphisms from the
first into Drinfeld twistings of the second. They possess a composition
operation extending composition of bialgebra homomorphisms. Gauge
transformations of twists, compatible with adjacent homomorphisms, give rise to
gauge transformation of twi... | math.QA math.CT | twisted homomorphisms of bialgebras are bialgebra homomorphisms from the first into drinfeld twistings of the second they possess a composition operation extending composition of bialgebra homomorphisms gauge transformations of twists compatible with adjacent homomorphisms give rise to gauge transformation of twisted h... | [['twisted', 'homomorphisms', 'of', 'bialgebras', 'are', 'bialgebra', 'homomorphisms', 'from', 'the', 'first', 'into', 'drinfeld', 'twistings', 'of', 'the', 'second', 'they', 'possess', 'a', 'composition', 'operation', 'extending', 'composition', 'of', 'bialgebra', 'homomorphisms', 'gauge', 'transformations', 'of', 'tw... | [-0.23917772678569668, 0.16253117799004985, -0.06842002718310271, 0.08353967241765488, -0.22664028891761387, -0.17993876328580968, -0.06094303056375966, 0.4016528805340862, -0.4652817344204301, -0.2117561210990451, 0.03259362124039659, -0.2033613965336588, -0.13702460347641526, 0.1406864838763362, -0.20245788792436498,... |
708.2758 | Twisted automorphisms of group algebras | We continue the study of twisted automorphisms of Hopf algebras started in
"Twisted automorphisms of Hopf algebras". In this paper we concentrate on the
group algebra case. We describe the group of twisted automorphisms of the group
algebra of a group of order coprime to 6. The description turns out to be very
simila... | math.RT math.QA | we continue the study of twisted automorphisms of hopf algebras started in twisted automorphisms of hopf algebras in this paper we concentrate on the group algebra case we describe the group of twisted automorphisms of the group algebra of a group of order coprime to 6 the description turns out to be very similar to th... | [['we', 'continue', 'the', 'study', 'of', 'twisted', 'automorphisms', 'of', 'hopf', 'algebras', 'started', 'in', 'twisted', 'automorphisms', 'of', 'hopf', 'algebras', 'in', 'this', 'paper', 'we', 'concentrate', 'on', 'the', 'group', 'algebra', 'case', 'we', 'describe', 'the', 'group', 'of', 'twisted', 'automorphisms', ... | [-0.25659493235466274, 0.06990378028780654, -0.09246848291461018, 0.026517117895401905, -0.16629083265644917, -0.07746263695340874, -0.033422325439143766, 0.3476992643613746, -0.39743229266984953, -0.18310733867026324, 0.15836863853610997, -0.21954585298679877, -0.14373726649479807, 0.16375052576641674, -0.178184615623... |
708.2759 | Phase effects on synchronization by dynamical relaying in delay-coupled
systems | Synchronization in an array of mutually coupled systems with a finite
time-delay in coupling is studied using Josephson junction as a model system.
The sum of the transverse Lyapunov exponents is evaluated as a function of the
parameters by linearizing the equation about the synchronization manifold. The
dependence o... | nlin.CD | synchronization in an array of mutually coupled systems with a finite timedelay in coupling is studied using josephson junction as a model system the sum of the transverse lyapunov exponents is evaluated as a function of the parameters by linearizing the equation about the synchronization manifold the dependence of syn... | [['synchronization', 'in', 'an', 'array', 'of', 'mutually', 'coupled', 'systems', 'with', 'a', 'finite', 'timedelay', 'in', 'coupling', 'is', 'studied', 'using', 'josephson', 'junction', 'as', 'a', 'model', 'system', 'the', 'sum', 'of', 'the', 'transverse', 'lyapunov', 'exponents', 'is', 'evaluated', 'as', 'a', 'functi... | [-0.2671724231121071, 0.1440439270179226, -0.0383062723211627, 0.018415463435651855, -0.018521251924771893, -0.15296898887274749, 0.011761515812472777, 0.32025231895200473, -0.2608076128514206, -0.2471399449723515, 0.08657312486258811, -0.23849851224928142, -0.16669560855928253, 0.2208621175241399, 0.031244967018868378... |
708.276 | Theoretic Limits on the Equation of State Parameter of Quintessence | The value of scalar field coupled to gravity should be less than the Planck
scale in the consistent theory of quantum gravity. It provides a theoretic
constraint on the equation of state parameter for the quintessence. In some
cases our theoretic constraints are more stringent than the constraints from
the present ex... | astro-ph hep-ph hep-th | the value of scalar field coupled to gravity should be less than the planck scale in the consistent theory of quantum gravity it provides a theoretic constraint on the equation of state parameter for the quintessence in some cases our theoretic constraints are more stringent than the constraints from the present experi... | [['the', 'value', 'of', 'scalar', 'field', 'coupled', 'to', 'gravity', 'should', 'be', 'less', 'than', 'the', 'planck', 'scale', 'in', 'the', 'consistent', 'theory', 'of', 'quantum', 'gravity', 'it', 'provides', 'a', 'theoretic', 'constraint', 'on', 'the', 'equation', 'of', 'state', 'parameter', 'for', 'the', 'quintess... | [-0.13092042987297575, 0.13258610631769094, -0.14392069643005156, 0.10687270262636818, -0.14400722025535428, -0.17449344758642837, 0.0025741860892874403, 0.22441529894534212, -0.188126638218259, -0.3367404826343633, 0.09680444374232768, -0.3013366821150367, -0.06354854743068035, 0.2542843114441404, -0.01600761376679516... |
708.2761 | Nuclei of categories with tensor products | Following the analogy between algebras (monoids) and monoidal categories the
construction of nucleus for non-associative algebras is simulated on the
categorical level. Nuclei of categories of modules are considered as an
example.
| math.CT | following the analogy between algebras monoids and monoidal categories the construction of nucleus for nonassociative algebras is simulated on the categorical level nuclei of categories of modules are considered as an example | [['following', 'the', 'analogy', 'between', 'algebras', 'monoids', 'and', 'monoidal', 'categories', 'the', 'construction', 'of', 'nucleus', 'for', 'nonassociative', 'algebras', 'is', 'simulated', 'on', 'the', 'categorical', 'level', 'nuclei', 'of', 'categories', 'of', 'modules', 'are', 'considered', 'as', 'an', 'exampl... | [-0.0938785387261305, 0.026289228892437677, -0.031919951434247196, 0.20549258347091381, -0.03925564934615977, -0.12832802921911934, -0.06501933978870511, 0.42143301432952285, -0.38735692854970694, -0.22421064478112385, 0.08307412336580455, -0.2309751873449386, -0.07716372853610665, 0.20502245728857815, -0.1963035316875... |
708.2762 | Digital Frequency Domain Multiplexer for mm-Wavelength Telescopes | An FPGA based digital signal processing (DSP) system for biasing and reading
out multiplexed bolometric detectors for mm-wavelength telescopes is presented.
This readout system is being deployed for balloon-borne and ground based
cosmology experiments with the primary goal of measuring the signature of
inflation with... | physics.ins-det | an fpga based digital signal processing dsp system for biasing and reading out multiplexed bolometric detectors for mmwavelength telescopes is presented this readout system is being deployed for balloonborne and ground based cosmology experiments with the primary goal of measuring the signature of inflation with the co... | [['an', 'fpga', 'based', 'digital', 'signal', 'processing', 'dsp', 'system', 'for', 'biasing', 'and', 'reading', 'out', 'multiplexed', 'bolometric', 'detectors', 'for', 'mmwavelength', 'telescopes', 'is', 'presented', 'this', 'readout', 'system', 'is', 'being', 'deployed', 'for', 'balloonborne', 'and', 'ground', 'based... | [-0.14941466722637414, 0.1168308442066856, -0.01275476126000285, -0.025009486698545514, -0.07371422179442431, -0.19075843964570335, 0.03960307363379148, 0.39364877090257194, -0.22413695980661683, -0.351371986333813, 0.1422750475078023, -0.3088075048024101, -0.050208960409675325, 0.28235695776396563, -0.0353556344791182... |
708.2763 | Diagnosing GRB Prompt Emission Site with Spectral Cut-Off Energy | The site and mechanism of gamma-ray burst (GRB) prompt emission is still
unknown. Although internal shocks have been widely discussed as the emission
site of GRBs, evidence supporting other emission sites have been also suggested
recently, including the closer-in photosphere where the fireball becomes
transparent and... | astro-ph | the site and mechanism of gammaray burst grb prompt emission is still unknown although internal shocks have been widely discussed as the emission site of grbs evidence supporting other emission sites have been also suggested recently including the closerin photosphere where the fireball becomes transparent and furthero... | [['the', 'site', 'and', 'mechanism', 'of', 'gammaray', 'burst', 'grb', 'prompt', 'emission', 'is', 'still', 'unknown', 'although', 'internal', 'shocks', 'have', 'been', 'widely', 'discussed', 'as', 'the', 'emission', 'site', 'of', 'grbs', 'evidence', 'supporting', 'other', 'emission', 'sites', 'have', 'been', 'also', '... | [-0.030459824233100966, 0.1713841935457029, -0.08163258941091883, 0.18246776815533686, -0.13587997843606922, -0.12183455297221932, 0.0044745631957760984, 0.46043076829459423, -0.20118965227335978, -0.3213845166312053, 0.0539136917639273, -0.3005175473443113, 0.03509776137518482, 0.2250182846775995, 0.02899259829129546,... |
708.2764 | Maxima of Moving Sums in a Poisson Random Field | The extremal tail probabilities of moving sums in a marked Poisson random
field is examined here. These sums are computed by adding up the weighted
occurrences of events lying within a scanning set of fixed shape and size.
Change of measure and analysis of local random fields are used to provide tail
probabilities. T... | math.PR | the extremal tail probabilities of moving sums in a marked poisson random field is examined here these sums are computed by adding up the weighted occurrences of events lying within a scanning set of fixed shape and size change of measure and analysis of local random fields are used to provide tail probabilities the as... | [['the', 'extremal', 'tail', 'probabilities', 'of', 'moving', 'sums', 'in', 'a', 'marked', 'poisson', 'random', 'field', 'is', 'examined', 'here', 'these', 'sums', 'are', 'computed', 'by', 'adding', 'up', 'the', 'weighted', 'occurrences', 'of', 'events', 'lying', 'within', 'a', 'scanning', 'set', 'of', 'fixed', 'shape'... | [-0.08668245464567187, 0.12153360262605244, -0.12958526113223223, 0.10306318157512817, -0.096804597470375, -0.13035007670033175, 0.08996760933044497, 0.3972782304082982, -0.26170319934102676, -0.28999448473733225, 0.09813987669061686, -0.25160309033407297, -0.1262046343410296, 0.20143673585090388, -0.06011945832726836,... |
708.2765 | Doublon-Holon Binding Effects on Mott Transitions in Two-Dimensional
Bose Hubbard Model | A mechanism of Mott transitions in a Bose Hubbard model on a square lattice
is studied, using a variational Monte Carlo method. Besides an onsite
correlation factor, we introduce a four-body doublon-holon factor into the
trial state, which considerably improves the variational energy and can
appropriately describe a ... | cond-mat.str-el cond-mat.stat-mech | a mechanism of mott transitions in a bose hubbard model on a square lattice is studied using a variational monte carlo method besides an onsite correlation factor we introduce a fourbody doublonholon factor into the trial state which considerably improves the variational energy and can appropriately describe a superflu... | [['a', 'mechanism', 'of', 'mott', 'transitions', 'in', 'a', 'bose', 'hubbard', 'model', 'on', 'a', 'square', 'lattice', 'is', 'studied', 'using', 'a', 'variational', 'monte', 'carlo', 'method', 'besides', 'an', 'onsite', 'correlation', 'factor', 'we', 'introduce', 'a', 'fourbody', 'doublonholon', 'factor', 'into', 'the... | [-0.12667549674420855, 0.22676009347619688, -0.08139413767115235, 0.09821799144062192, 0.02544028101878804, -0.15779146303011235, 0.11475860542985936, 0.3835259450756576, -0.21998398162446223, -0.2478571939173826, -0.01775967645280193, -0.3137446340974854, -0.11866067128856991, 0.1016010029625884, 0.07304392341621826, ... |
708.2766 | Operator ordering in Two-dimensional N=1 supersymmetry with curved
manifold | We investigate an operator ordering problem in two-dimensional N=1
supersymmetric model which consists of n real superfields. There arises an
operator ordering problem when the target space is curved. We have to fix the
ordering in quantum operator properly to obtain the correct supersymmetry
algebra. We demonstrate ... | hep-th | we investigate an operator ordering problem in twodimensional n1 supersymmetric model which consists of n real superfields there arises an operator ordering problem when the target space is curved we have to fix the ordering in quantum operator properly to obtain the correct supersymmetry algebra we demonstrate that th... | [['we', 'investigate', 'an', 'operator', 'ordering', 'problem', 'in', 'twodimensional', 'n1', 'supersymmetric', 'model', 'which', 'consists', 'of', 'n', 'real', 'superfields', 'there', 'arises', 'an', 'operator', 'ordering', 'problem', 'when', 'the', 'target', 'space', 'is', 'curved', 'we', 'have', 'to', 'fix', 'the', ... | [-0.16760270183407505, 0.15278482425697212, -0.02574576642101919, 0.10316434780194779, -0.14097472248782575, -0.13673091774255458, -0.023599696086562226, 0.3678990197958241, -0.2796427526996589, -0.25358978818944644, 0.0879912982419343, -0.31028911113266794, -0.15422573895849498, 0.001989810015927528, -0.07693294506244... |
708.2767 | Equivalence Principle and the Gauge Hierarchy Problem | We show that the gauge hierarchy problem can be solved in the framework of
scalar-tensor theories of gravity very much in the same way as it is solved in
the Randall-Sundrum scenario. Our solution involves a fine-tuning of the
gravitational sector. However our mechanism does not require the introduction
of extra-dime... | hep-ph hep-th | we show that the gauge hierarchy problem can be solved in the framework of scalartensor theories of gravity very much in the same way as it is solved in the randallsundrum scenario our solution involves a finetuning of the gravitational sector however our mechanism does not require the introduction of extradimensions o... | [['we', 'show', 'that', 'the', 'gauge', 'hierarchy', 'problem', 'can', 'be', 'solved', 'in', 'the', 'framework', 'of', 'scalartensor', 'theories', 'of', 'gravity', 'very', 'much', 'in', 'the', 'same', 'way', 'as', 'it', 'is', 'solved', 'in', 'the', 'randallsundrum', 'scenario', 'our', 'solution', 'involves', 'a', 'fine... | [-0.14549970904419435, 0.1534839363913368, -0.08496391223924397, 0.14441866525652303, -0.13970842718110574, -0.167650773714396, -0.014158020872007874, 0.2682882550995327, -0.268750524962122, -0.3532381571232549, 0.06097727751775274, -0.19900299345586195, -0.11408759760263476, 0.14794064906552362, -0.024930683995407182,... |
708.2768 | A new test of the light dark matter hypothesis | Detection of a surprisingly high flux of positron annihilation radiation from
the inner galaxy has motivated the proposal that dark matter is made of weakly
interacting light particles (possibly as light as the electron). This scenario
is extremely hard to test in current high energy physics experiments. Here,
howeve... | hep-ph | detection of a surprisingly high flux of positron annihilation radiation from the inner galaxy has motivated the proposal that dark matter is made of weakly interacting light particles possibly as light as the electron this scenario is extremely hard to test in current high energy physics experiments here however we de... | [['detection', 'of', 'a', 'surprisingly', 'high', 'flux', 'of', 'positron', 'annihilation', 'radiation', 'from', 'the', 'inner', 'galaxy', 'has', 'motivated', 'the', 'proposal', 'that', 'dark', 'matter', 'is', 'made', 'of', 'weakly', 'interacting', 'light', 'particles', 'possibly', 'as', 'light', 'as', 'the', 'electron... | [-0.08133899026107407, 0.1963772899868739, -0.10549186371698431, 0.1272395781153336, -0.09329107406026707, -0.11860045658356351, 0.00648868820280768, 0.33988354759427103, -0.20173186893438602, -0.3958778152605746, 0.054334568433327284, -0.2697667495188553, -0.02777130181174271, 0.24088011236815918, 0.02154788939373159,... |
708.2769 | Fields with several commuting derivations | For every natural number $m$, the existentially closed models of the theory
of fields with $m$ commuting derivations can be given a first-order geometric
characterization in several ways. In particular, the theory of these
differential fields has a model-companion. The axioms are that certain
differential varieties d... | math.LO | for every natural number m the existentially closed models of the theory of fields with m commuting derivations can be given a firstorder geometric characterization in several ways in particular the theory of these differential fields has a modelcompanion the axioms are that certain differential varieties determined by... | [['for', 'every', 'natural', 'number', 'm', 'the', 'existentially', 'closed', 'models', 'of', 'the', 'theory', 'of', 'fields', 'with', 'm', 'commuting', 'derivations', 'can', 'be', 'given', 'a', 'firstorder', 'geometric', 'characterization', 'in', 'several', 'ways', 'in', 'particular', 'the', 'theory', 'of', 'these', '... | [-0.22052270111453254, 0.13386326565523632, -0.08337089854467195, 0.06962888406451384, -0.08770615825778805, -0.1122498355107382, -0.04894599051112891, 0.307566205970943, -0.3118674964644015, -0.27658450650051236, 0.0808737164370541, -0.24085968188592233, -0.15187663913093274, 0.2368647748771764, -0.12019553751451895, ... |
708.277 | Examples of signature (2,2) manifolds with commuting curvature operators | We exhibit Walker manifolds of signature (2,2) with various commutativity
properties for the Ricci operator, the skew-symmetric curvature operator, and
the Jacobi operator. If the Walker metric is a Riemannian extension of an
underlying affine structure A, these properties are related to the Ricci tensor
of A.
| math.DG | we exhibit walker manifolds of signature 22 with various commutativity properties for the ricci operator the skewsymmetric curvature operator and the jacobi operator if the walker metric is a riemannian extension of an underlying affine structure a these properties are related to the ricci tensor of a | [['we', 'exhibit', 'walker', 'manifolds', 'of', 'signature', '22', 'with', 'various', 'commutativity', 'properties', 'for', 'the', 'ricci', 'operator', 'the', 'skewsymmetric', 'curvature', 'operator', 'and', 'the', 'jacobi', 'operator', 'if', 'the', 'walker', 'metric', 'is', 'a', 'riemannian', 'extension', 'of', 'an', ... | [-0.20677087057698915, 0.1118252242774767, -0.10256542921304068, 0.07286991275341666, -0.1825957484147016, -0.16799917419817537, -0.1298860432778267, 0.3705755354281753, -0.30535617454888975, -0.17153406319545306, 0.16255929752035028, -0.3169165885551496, -0.21724120424465931, 0.07649229683893476, -0.07296626889543172,... |
708.2771 | Approximations to Euler's constant | We study a problem of finding good approximations to Euler's constant
$\gamma=\lim_{n\to\infty}S_n,$ where $S_n=\sum_{k=1}^n\frac{1}{n}-\log(n+1),$
by linear forms in logarithms and harmonic numbers. In 1995, C. Elsner showed
that slow convergence of the sequence $S_n$ can be significantly improved if
$S_n$ is replac... | math.NT | we study a problem of finding good approximations to eulers constant gammalim_ntoinftys_n where s_nsum_k1nfrac1nlogn1 by linear forms in logarithms and harmonic numbers in 1995 c elsner showed that slow convergence of the sequence s_n can be significantly improved if s_n is replaced by linear combinations of s_n with i... | [['we', 'study', 'a', 'problem', 'of', 'finding', 'good', 'approximations', 'to', 'eulers', 'constant', 'gammalim_ntoinftys_n', 'where', 's_nsum_k1nfrac1nlogn1', 'by', 'linear', 'forms', 'in', 'logarithms', 'and', 'harmonic', 'numbers', 'in', '1995', 'c', 'elsner', 'showed', 'that', 'slow', 'convergence', 'of', 'the', ... | [-0.11926753519483926, 0.09988832857367937, -0.09042633034579166, 0.03407849624220814, -0.06925654671965288, -0.12715534584645133, 0.05479720874248048, 0.33850569340896297, -0.2966708223178209, -0.25489604311039693, 0.08431175669395159, -0.2500053707074809, -0.1521986003045912, 0.23096394928341563, -0.11389700699500836... |
708.2772 | On the contact Ozsvath-Szabo invariant | Sarkar and Wang proved that the hat version of Heegaard Floer homology group
of a closed oriented 3-manifold is combinatorial starting from an arbitrary
nice Heegaard diagram and in fact every closed oriented 3-manifold admits such
a Heegaard diagram. Plamenevskaya showed that the contact Ozsvath-Szabo
invariant is c... | math.GT math.SG | sarkar and wang proved that the hat version of heegaard floer homology group of a closed oriented 3manifold is combinatorial starting from an arbitrary nice heegaard diagram and in fact every closed oriented 3manifold admits such a heegaard diagram plamenevskaya showed that the contact ozsvathszabo invariant is combina... | [['sarkar', 'and', 'wang', 'proved', 'that', 'the', 'hat', 'version', 'of', 'heegaard', 'floer', 'homology', 'group', 'of', 'a', 'closed', 'oriented', '3manifold', 'is', 'combinatorial', 'starting', 'from', 'an', 'arbitrary', 'nice', 'heegaard', 'diagram', 'and', 'in', 'fact', 'every', 'closed', 'oriented', '3manifold'... | [-0.21909665790180327, 0.07603147208094348, -0.20458942608737196, 0.096853400596581, -0.12396463146077767, -0.21698059124573496, 0.018893657982676424, 0.36648766955232803, -0.31489723814537623, -0.3186201129165542, 0.04110787735046918, -0.24292393581842192, -0.21468327447366795, 0.15987380985028415, -0.2219102627576421... |
708.2773 | Strongly r-matrix induced tensors, Koszul cohomology, and
arbitrary-dimensional quadratic Poisson cohomology | We introduce the concept of strongly $r$-matrix induced ({\small SRMI})
Poisson structure, report on the relation of this property with the stabilizer
dimension of the considered quadratic Poisson tensor, and classify the Poisson
structures of the Dufour-Haraki classification (DHC) according to their
membership of th... | math.SG | we introduce the concept of strongly rmatrix induced small srmi poisson structure report on the relation of this property with the stabilizer dimension of the considered quadratic poisson tensor and classify the poisson structures of the dufourharaki classification dhc according to their membership of the family of sma... | [['we', 'introduce', 'the', 'concept', 'of', 'strongly', 'rmatrix', 'induced', 'small', 'srmi', 'poisson', 'structure', 'report', 'on', 'the', 'relation', 'of', 'this', 'property', 'with', 'the', 'stabilizer', 'dimension', 'of', 'the', 'considered', 'quadratic', 'poisson', 'tensor', 'and', 'classify', 'the', 'poisson',... | [-0.15779298550296517, 0.010440636450312013, -0.09477133884793147, 0.058543819597252876, -0.10764072679594391, -0.11103506596118677, 0.020861666311975568, 0.3305688278458547, -0.3502732778899372, -0.25925037898414305, 0.07067440428800183, -0.18009538915512166, -0.1957437112250318, 0.14776949661318212, -0.11460571146144... |
708.2774 | The earliest phases of high-mass star formation: a 3 square degree
millimeter continuum mapping of Cygnus X | We have made an extensive 1.2mm continuum mosaicing study of the Cygnus X
molecular cloud complex using the MAMBO cameras at the IRAM 30 m telescope. We
then compared our mm maps with mid-IR images, and have made SiO(2-1) follow-up
observations of the best candidate progenitors of high-mass stars. Our complete
study ... | astro-ph | we have made an extensive 12mm continuum mosaicing study of the cygnus x molecular cloud complex using the mambo cameras at the iram 30 m telescope we then compared our mm maps with midir images and have made sio21 followup observations of the best candidate progenitors of highmass stars our complete study of cygnus x ... | [['we', 'have', 'made', 'an', 'extensive', '12mm', 'continuum', 'mosaicing', 'study', 'of', 'the', 'cygnus', 'x', 'molecular', 'cloud', 'complex', 'using', 'the', 'mambo', 'cameras', 'at', 'the', 'iram', '30', 'm', 'telescope', 'we', 'then', 'compared', 'our', 'mm', 'maps', 'with', 'midir', 'images', 'and', 'have', 'ma... | [-0.09576185145535955, 0.13742640358036426, -0.02312957064111335, 0.09589150348185205, -0.06991461904411504, -0.03698102350298508, 0.074172827363222, 0.42988080742483237, -0.09911567750813595, -0.36145910811406445, 0.06591633759323967, -0.2551895828168112, -0.021019434174188816, 0.14004324393001835, 0.00580668064210920... |
708.2775 | Coupled layered superconductor as a system of 2D Coulomb particles of
two kinds | It is shown that the Josephson subsystem of the Lawrence-Doniach model of
layered superconductors in the London approximation can be presented as a
system with variable number of classical Coulomb particles. This allows us to
consider the vortex system of a coupled layered superconductor as the system of
these partic... | cond-mat.supr-con | it is shown that the josephson subsystem of the lawrencedoniach model of layered superconductors in the london approximation can be presented as a system with variable number of classical coulomb particles this allows us to consider the vortex system of a coupled layered superconductor as the system of these particles ... | [['it', 'is', 'shown', 'that', 'the', 'josephson', 'subsystem', 'of', 'the', 'lawrencedoniach', 'model', 'of', 'layered', 'superconductors', 'in', 'the', 'london', 'approximation', 'can', 'be', 'presented', 'as', 'a', 'system', 'with', 'variable', 'number', 'of', 'classical', 'coulomb', 'particles', 'this', 'allows', '... | [-0.15324284163299856, 0.1422031912055691, -0.10275705182375233, 0.03480311372931894, -0.005733989119972484, -0.1693419472841149, 0.041409054358840965, 0.30666191238513, -0.24514950596590024, -0.29666374422625075, 0.05289047672775895, -0.29981630139988485, -0.13574836067626345, 0.1686008443357423, 0.031282219501425984,... |
708.2776 | Antimagic labelings of regular bipartite graphs: An application of the
Marriage Theorem | A labeling of a graph is a bijection from $E(G)$ to the set $\{1, 2,...,
|E(G)|\}$. A labeling is \textit{antimagic} if for any distinct vertices $u$
and $v$, the sum of the labels on edges incident to $u$ is different from the
sum of the labels on edges incident to $v$. We say a graph is antimagic if it
has an antim... | math.CO | a labeling of a graph is a bijection from eg to the set 1 2 eg a labeling is textitantimagic if for any distinct vertices u and v the sum of the labels on edges incident to u is different from the sum of the labels on edges incident to v we say a graph is antimagic if it has an antimagic labeling in 1990 ringel conject... | [['a', 'labeling', 'of', 'a', 'graph', 'is', 'a', 'bijection', 'from', 'eg', 'to', 'the', 'set', '1', '2', 'eg', 'a', 'labeling', 'is', 'textitantimagic', 'if', 'for', 'any', 'distinct', 'vertices', 'u', 'and', 'v', 'the', 'sum', 'of', 'the', 'labels', 'on', 'edges', 'incident', 'to', 'u', 'is', 'different', 'from', 't... | [-0.1537543700588867, 0.10973527069800185, -0.06697581687243655, -0.020064084782497958, -0.13307204808108508, -0.1619623772194609, 0.06779729869333095, 0.44153245827619686, -0.2816920516639948, -0.30681731000047874, 0.03760083911241963, -0.38546922428533437, -0.14097971135750412, 0.06388732230290771, -0.145404202332720... |
708.2777 | A new metric between distributions of point processes | Most metrics between finite point measures currently used in the literature
have the flaw that they do not treat differing total masses in an adequate
manner for applications. This paper introduces a new metric $\bar{d}_1$ that
combines positional differences of points under a closest match with the
relative differen... | math.PR math.ST stat.TH | most metrics between finite point measures currently used in the literature have the flaw that they do not treat differing total masses in an adequate manner for applications this paper introduces a new metric bard_1 that combines positional differences of points under a closest match with the relative difference in to... | [['most', 'metrics', 'between', 'finite', 'point', 'measures', 'currently', 'used', 'in', 'the', 'literature', 'have', 'the', 'flaw', 'that', 'they', 'do', 'not', 'treat', 'differing', 'total', 'masses', 'in', 'an', 'adequate', 'manner', 'for', 'applications', 'this', 'paper', 'introduces', 'a', 'new', 'metric', 'bard_... | [-0.09764162309467793, 0.05631943086453248, -0.1195010461062193, 0.10318734372282051, -0.04742661347985268, -0.09051442854851484, 0.13279691417794676, 0.3806597234755755, -0.22789230946917086, -0.288403286524117, 0.058598075135611, -0.3085606274306774, -0.1498598261969164, 0.22770061992201954, -0.1051193487867713, 0.06... |
708.2778 | A dense micro-cluster of Class 0 protostars in NGC 2264 D-MM1 | We present sensitive and high angular resolution (~1") 1.3 mm continuum
observations of the dusty core D-MM1 in the Spokes cluster in NGC 2264 using
the Submillimeter Array. A dense micro-cluster of seven Class 0 sources was
detected in a 20" x 20" region with masses between 0.4 to 1.2 solar masses and
deconvolved si... | astro-ph | we present sensitive and high angular resolution 1 13 mm continuum observations of the dusty core dmm1 in the spokes cluster in ngc 2264 using the submillimeter array a dense microcluster of seven class 0 sources was detected in a 20 x 20 region with masses between 04 to 12 solar masses and deconvolved sizes of about 6... | [['we', 'present', 'sensitive', 'and', 'high', 'angular', 'resolution', '1', '13', 'mm', 'continuum', 'observations', 'of', 'the', 'dusty', 'core', 'dmm1', 'in', 'the', 'spokes', 'cluster', 'in', 'ngc', '2264', 'using', 'the', 'submillimeter', 'array', 'a', 'dense', 'microcluster', 'of', 'seven', 'class', '0', 'sources... | [-0.06636658202412284, 0.1407980279889235, 0.013075978287364825, 0.0513649977607006, -0.005436377291960164, -0.045113938237147884, 0.02353986486222995, 0.4281736083390299, -0.18049959718703854, -0.37496328080642566, 0.0894210494156111, -0.2781680035885916, 0.0046857198592552465, 0.13461304807935434, 0.01655836325968146... |
708.2779 | A Survey on the Classical Limit of Quantum Dynamical Entropies | We analyze the behavior of quantum dynamical entropies production from
sequences of quantum approximants approaching their (chaotic) classical limit.
The model of the quantized hyperbolic automorphisms of the 2-torus is examined
in detail and a semi-classical analysis is performed on it using coherent
states, fulfill... | math-ph math.DS math.MP quant-ph | we analyze the behavior of quantum dynamical entropies production from sequences of quantum approximants approaching their chaotic classical limit the model of the quantized hyperbolic automorphisms of the 2torus is examined in detail and a semiclassical analysis is performed on it using coherent states fulfilling an a... | [['we', 'analyze', 'the', 'behavior', 'of', 'quantum', 'dynamical', 'entropies', 'production', 'from', 'sequences', 'of', 'quantum', 'approximants', 'approaching', 'their', 'chaotic', 'classical', 'limit', 'the', 'model', 'of', 'the', 'quantized', 'hyperbolic', 'automorphisms', 'of', 'the', '2torus', 'is', 'examined', ... | [-0.19382442771651162, 0.18945035004213018, -0.1667038386221975, 0.11944792447967403, 0.04042188895659314, -0.14438305701252022, 0.0274318907100274, 0.29787876141361064, -0.2907507942161626, -0.19860989367589355, 0.06999090238079791, -0.31078053410682416, -0.1583462539145128, 0.21468243514795582, -0.060515517226627305,... |
708.278 | Ion dynamics and coherent structure formation following laser pulse
self-channeling | The propagation of a superintense laser pulse in an underdense, inhomogeneous
plasma has been studied numerically by two-dimensional particle-in-cell
simulations on a time scale extending up to several picoseconds. The effects of
the ion dynamics following the charge-displacement self-channeling of the laser
pulse ha... | physics.plasm-ph | the propagation of a superintense laser pulse in an underdense inhomogeneous plasma has been studied numerically by twodimensional particleincell simulations on a time scale extending up to several picoseconds the effects of the ion dynamics following the chargedisplacement selfchanneling of the laser pulse have been a... | [['the', 'propagation', 'of', 'a', 'superintense', 'laser', 'pulse', 'in', 'an', 'underdense', 'inhomogeneous', 'plasma', 'has', 'been', 'studied', 'numerically', 'by', 'twodimensional', 'particleincell', 'simulations', 'on', 'a', 'time', 'scale', 'extending', 'up', 'to', 'several', 'picoseconds', 'the', 'effects', 'of... | [-0.1774981138317401, 0.25034146183112693, -0.0755777438632674, 0.03942019096995192, 0.0029239392931665388, -0.07993378285329102, -0.08462473998991521, 0.4705182710276531, -0.2463717322360288, -0.2995299134101417, 0.06752762174850481, -0.19622125393325077, 0.0026122774291145907, 0.2009828719352414, 0.04958278389630823,... |
708.2781 | Comment on "Entropy production and the arrow of time" | J.M.R. Parrondo at al. in arXiv:0904.1573 continue numerous efforts to unify
the concepts of the arrow of time and entropy production with the concept of
time invariance in physics. This is a wrong way.
| physics.gen-ph | jmr parrondo at al in arxiv09041573 continue numerous efforts to unify the concepts of the arrow of time and entropy production with the concept of time invariance in physics this is a wrong way | [['jmr', 'parrondo', 'at', 'al', 'in', 'arxiv09041573', 'continue', 'numerous', 'efforts', 'to', 'unify', 'the', 'concepts', 'of', 'the', 'arrow', 'of', 'time', 'and', 'entropy', 'production', 'with', 'the', 'concept', 'of', 'time', 'invariance', 'in', 'physics', 'this', 'is', 'a', 'wrong', 'way']] | [-0.07848851125891088, 0.1709182257327484, -0.1656541821284918, 0.03889034467283636, -0.08476463392435107, -0.06689802602340933, 0.07145722978748381, 0.2899397073779255, -0.3111416510946583, -0.3426664316211827, 0.0436900491695269, -0.26847562775947154, -0.09667283319868147, 0.11473156232386827, -0.10490771886543371, 0... |
708.2782 | Anisotropic quasiparticle scattering rates in slightly underdoped to
optimally doped high-temperature \LSCO\ superconductors | An angle-resolved photoemission study of the scattering rate in the
superconducting phase of the high-temperature superconductor \LSCO\ with
$x=0.145$ and $x=0.17$, as a function of binding energy and momentum, is
presented. We observe that the scattering rate scales linearly with binding
energy up to the high-energy... | cond-mat.supr-con | an angleresolved photoemission study of the scattering rate in the superconducting phase of the hightemperature superconductor lsco with x0145 and x017 as a function of binding energy and momentum is presented we observe that the scattering rate scales linearly with binding energy up to the highenergy scale e_1sim04 ev... | [['an', 'angleresolved', 'photoemission', 'study', 'of', 'the', 'scattering', 'rate', 'in', 'the', 'superconducting', 'phase', 'of', 'the', 'hightemperature', 'superconductor', 'lsco', 'with', 'x0145', 'and', 'x017', 'as', 'a', 'function', 'of', 'binding', 'energy', 'and', 'momentum', 'is', 'presented', 'we', 'observe'... | [-0.17574342066008183, 0.23815754403464476, -0.07363337630845813, 0.05086144608180297, -0.0435136820952822, -0.10033695868979622, 0.08601729111655408, 0.39556119690274094, -0.31195841760685045, -0.2594204255082231, -0.008187215550505143, -0.3702954221387497, -0.05944275100935354, 0.1835194815454694, 0.08360194960712558... |
708.2783 | On Energy of the Friedman Universes in Conformally Flat Coordinates | Recently many authors have calculated the energy of the Friedman universes by
using double index energy-momentum complexes in Cartesian comoving coordinates
$(t,x,y,z)$ and concluded that the flat and closed Friedman universes are
energy-free. We show in this paper by using Einstein canonical energy-momentum
complex ... | gr-qc | recently many authors have calculated the energy of the friedman universes by using double index energymomentum complexes in cartesian comoving coordinates txyz and concluded that the flat and closed friedman universes are energyfree we show in this paper by using einstein canonical energymomentum complex and by doing ... | [['recently', 'many', 'authors', 'have', 'calculated', 'the', 'energy', 'of', 'the', 'friedman', 'universes', 'by', 'using', 'double', 'index', 'energymomentum', 'complexes', 'in', 'cartesian', 'comoving', 'coordinates', 'txyz', 'and', 'concluded', 'that', 'the', 'flat', 'and', 'closed', 'friedman', 'universes', 'are',... | [-0.11395917663775275, 0.09203519459731657, -0.08413546723587548, 0.06734115651069099, -0.06648540587219245, -0.06076740493778797, -0.0719012762324008, 0.3791130084763555, -0.17133191311184098, -0.2678269096020171, 0.012035824550206171, -0.24561079440309722, -0.13637709227007103, 0.1515560810043312, -0.0859212394529844... |
708.2784 | On a linear code from a configuration of affine lines | We will show how to obtain a linear code from a configuration of affine lines
in general position and a suitable set of rational points. We will also explain
a new decoding algorithm based on the configuration, which seems to be quite
effective.
| cs.IT cs.DM math.AG math.IT | we will show how to obtain a linear code from a configuration of affine lines in general position and a suitable set of rational points we will also explain a new decoding algorithm based on the configuration which seems to be quite effective | [['we', 'will', 'show', 'how', 'to', 'obtain', 'a', 'linear', 'code', 'from', 'a', 'configuration', 'of', 'affine', 'lines', 'in', 'general', 'position', 'and', 'a', 'suitable', 'set', 'of', 'rational', 'points', 'we', 'will', 'also', 'explain', 'a', 'new', 'decoding', 'algorithm', 'based', 'on', 'the', 'configuration'... | [-0.11531650400612244, 0.040703176975596785, -0.1550262556086446, 0.08955822837387406, -0.11365195528365844, -0.1801449990029945, 0.10428347063878941, 0.39500043237971705, -0.276702735854616, -0.2410728030859731, 0.10123051222966074, -0.17548027517663878, -0.19966869992962064, 0.2322984122086403, -0.11536858845935312, ... |
708.2785 | The uniform order convergence structure on ML(X) | The aim of this paper is to set up appropriate uniform convergence spaces in
which to reformulate and enrich the Order Completion Method for nonlinear PDEs.
In this regard, we consider an appropriate space ML(X) of normal lower
semi-continuous functions. The space ML(X)= appears in the ring theory of C(X),
and its va... | math.GM math.AP math.GN | the aim of this paper is to set up appropriate uniform convergence spaces in which to reformulate and enrich the order completion method for nonlinear pdes in this regard we consider an appropriate space mlx of normal lower semicontinuous functions the space mlx appears in the ring theory of cx and its various extensio... | [['the', 'aim', 'of', 'this', 'paper', 'is', 'to', 'set', 'up', 'appropriate', 'uniform', 'convergence', 'spaces', 'in', 'which', 'to', 'reformulate', 'and', 'enrich', 'the', 'order', 'completion', 'method', 'for', 'nonlinear', 'pdes', 'in', 'this', 'regard', 'we', 'consider', 'an', 'appropriate', 'space', 'mlx', 'of',... | [-0.08943855132339663, 0.06201721195358197, -0.08840791045010767, 0.10501545963272678, -0.08747058636226664, -0.050192659932442686, -0.02245610449410213, 0.3572468138440992, -0.34587873422512505, -0.22139139828857768, 0.14074317602066774, -0.22048727159077922, -0.1641774968328801, 0.1644033142074477, -0.098806239371752... |
708.2786 | Electroweak Contributions to Thermal Gravitino Production | At high temperatures, gravitinos are generated in inelastic scattering
processes with particles that are in thermal equilibrium with the hot
primordial plasma. We consider the regeneration of gravitinos that starts with
completion of reheating after inflation. Following a consistent
finite-temperature approach, we pr... | hep-ph | at high temperatures gravitinos are generated in inelastic scattering processes with particles that are in thermal equilibrium with the hot primordial plasma we consider the regeneration of gravitinos that starts with completion of reheating after inflation following a consistent finitetemperature approach we provide t... | [['at', 'high', 'temperatures', 'gravitinos', 'are', 'generated', 'in', 'inelastic', 'scattering', 'processes', 'with', 'particles', 'that', 'are', 'in', 'thermal', 'equilibrium', 'with', 'the', 'hot', 'primordial', 'plasma', 'we', 'consider', 'the', 'regeneration', 'of', 'gravitinos', 'that', 'starts', 'with', 'comple... | [-0.11666822694607225, 0.30703021717422146, -0.10635300212557994, 0.12110129287283794, -0.04561062170850003, -0.09690361293763214, -0.0008934079167232209, 0.32952806099737975, -0.19953731079951076, -0.2728234649094863, 0.06450525929126431, -0.28416979433420825, 0.04051241449390849, 0.15183827298802927, 0.03930140616299... |
708.2787 | Complete interpolating sequences, the discrete Muckenhoupt condition,
and conformal mapping | We extend the parameterization of sine-type functions in terms of conformal
mappings onto slit domains given by Eremenko and Sodin to the more general case
of generating functions of real complete interpolating sequences. It turns out
that the cuts have to fulfill the discrete Muckenhoupt condition studied
earlier by... | math.CV | we extend the parameterization of sinetype functions in terms of conformal mappings onto slit domains given by eremenko and sodin to the more general case of generating functions of real complete interpolating sequences it turns out that the cuts have to fulfill the discrete muckenhoupt condition studied earlier by lyu... | [['we', 'extend', 'the', 'parameterization', 'of', 'sinetype', 'functions', 'in', 'terms', 'of', 'conformal', 'mappings', 'onto', 'slit', 'domains', 'given', 'by', 'eremenko', 'and', 'sodin', 'to', 'the', 'more', 'general', 'case', 'of', 'generating', 'functions', 'of', 'real', 'complete', 'interpolating', 'sequences',... | [-0.08815108118534017, 0.04997468854372318, -0.08180171287117097, 0.09233321922902878, -0.0805666408000084, -0.10638875135471328, 0.028129872651054308, 0.36366619635373354, -0.2201056698193917, -0.21420270208126077, 0.08658505345542486, -0.23769247345626354, -0.13875379415157324, 0.21295956862517273, -0.087515714829071... |
708.2788 | Integrating users' needs into multimedia information retrieval system | The exponential growth of multimedia information and the development of
various communication media generated new problems at various levels including
the rate of flow of information, problems of storage and management. The
difficulty which arises is no longer the existence of information but rather
the access to thi... | cs.IR | the exponential growth of multimedia information and the development of various communication media generated new problems at various levels including the rate of flow of information problems of storage and management the difficulty which arises is no longer the existence of information but rather the access to this in... | [['the', 'exponential', 'growth', 'of', 'multimedia', 'information', 'and', 'the', 'development', 'of', 'various', 'communication', 'media', 'generated', 'new', 'problems', 'at', 'various', 'levels', 'including', 'the', 'rate', 'of', 'flow', 'of', 'information', 'problems', 'of', 'storage', 'and', 'management', 'the', ... | [-0.12525145962475412, 0.041648948078667064, -0.09403353023226373, 0.07436002661201352, -0.13477676468610297, -0.1458716147695668, 0.05046009782575614, 0.3525684595942342, -0.2859720256538518, -0.3272681460987466, 0.13468598835606826, -0.29916987770896714, -0.15455650665874904, 0.18040343887065927, -0.1007610232452862,... |
708.2789 | Collective excitations of trapped one-dimensional dipolar quantum gases | We calculate the excitation modes of a 1D dipolar quantum gas confined in a
harmonic trap with frequency $\omega_0$ and predict how the frequency of the
breathing n=2 mode characterizes the interaction strength evolving from the
Tonks-Girardeau value $\omega_2=2\omega_0$ to the quasi-ordered, super-strongly
interacti... | cond-mat.other cond-mat.str-el | we calculate the excitation modes of a 1d dipolar quantum gas confined in a harmonic trap with frequency omega_0 and predict how the frequency of the breathing n2 mode characterizes the interaction strength evolving from the tonksgirardeau value omega_22omega_0 to the quasiordered superstrongly interacting value omega_... | [['we', 'calculate', 'the', 'excitation', 'modes', 'of', 'a', '1d', 'dipolar', 'quantum', 'gas', 'confined', 'in', 'a', 'harmonic', 'trap', 'with', 'frequency', 'omega_0', 'and', 'predict', 'how', 'the', 'frequency', 'of', 'the', 'breathing', 'n2', 'mode', 'characterizes', 'the', 'interaction', 'strength', 'evolving', ... | [-0.1234937392976712, 0.21815953724729145, -0.09773452667338131, 0.041717405723556214, 0.014278822957612245, -0.1476589161820248, 0.013005732516428472, 0.36167351727629393, -0.23599764609099488, -0.26065469304083194, 0.0051654588948292415, -0.2778854282692371, -0.07614669710628491, 0.19312057110060632, 0.09665925981089... |
708.279 | Spectral models for solar-scaled and alpha-enhanced stellar populations | We present the first models allowing one to explore in a consistent way the
influence of changes in the alpha-element-to-iron abundance ratio on the
high-resolution spectral properties of evolving stellar populations. The models
cover the wavelength range 300-1340nm at a resolution of FWHM=1AA, for
metallicities in t... | astro-ph | we present the first models allowing one to explore in a consistent way the influence of changes in the alphaelementtoiron abundance ratio on the highresolution spectral properties of evolving stellar populations the models cover the wavelength range 3001340nm at a resolution of fwhm1aa for metallicities in the range 0... | [['we', 'present', 'the', 'first', 'models', 'allowing', 'one', 'to', 'explore', 'in', 'a', 'consistent', 'way', 'the', 'influence', 'of', 'changes', 'in', 'the', 'alphaelementtoiron', 'abundance', 'ratio', 'on', 'the', 'highresolution', 'spectral', 'properties', 'of', 'evolving', 'stellar', 'populations', 'the', 'mode... | [0.007328018144843109, 0.09622070810420923, -0.07321286966020228, 0.1013527022582208, -0.02763584467742579, -0.08937037916662476, 0.030161234359248668, 0.44894564886253774, -0.19393497084908135, -0.4021343857261306, 0.037244204892479676, -0.29221762114547933, -0.05382422996925996, 0.22515633077206296, -0.02534521987384... |
708.2791 | Vector spectropolarimetry of dark-cored penumbral filaments with Hinode | We present spectropolarimetric measurements of dark-cored penumbral filaments
taken with Hinode at a resolution of 0.3". Our observations demonstrate that
dark-cored filaments are more prominent in polarized light than in continuum
intensity. Far from disk center, the Stokes profiles emerging from these
structures ar... | astro-ph | we present spectropolarimetric measurements of darkcored penumbral filaments taken with hinode at a resolution of 03 our observations demonstrate that darkcored filaments are more prominent in polarized light than in continuum intensity far from disk center the stokes profiles emerging from these structures are very as... | [['we', 'present', 'spectropolarimetric', 'measurements', 'of', 'darkcored', 'penumbral', 'filaments', 'taken', 'with', 'hinode', 'at', 'a', 'resolution', 'of', '03', 'our', 'observations', 'demonstrate', 'that', 'darkcored', 'filaments', 'are', 'more', 'prominent', 'in', 'polarized', 'light', 'than', 'in', 'continuum'... | [-0.16295278947344505, 0.14953299688911667, -0.03259398301711658, 0.07034283065338053, -0.10546138564815054, -0.0715110841747764, -0.05820616954852911, 0.4744162143214599, -0.1978080105297007, -0.3171833077693111, 0.06837687480659875, -0.27897979246152865, -0.05050532466412841, 0.1903877485530464, -0.001683729531412774... |
708.2792 | Long nuclear spin decay times controlled by optical pumping in
individual quantum dots | Nuclear polarization dynamics are measured in the nuclear spin bi-stability
regime in a single optically pumped InGaAs/GaAs quantum dot. The controlling
role of nuclear spin diffusion from the dot into the surrounding material is
revealed in pump-probe measurements of the non-linear nuclear spin dynamics. We
measure ... | cond-mat.mes-hall cond-mat.mtrl-sci | nuclear polarization dynamics are measured in the nuclear spin bistability regime in a single optically pumped ingaasgaas quantum dot the controlling role of nuclear spin diffusion from the dot into the surrounding material is revealed in pumpprobe measurements of the nonlinear nuclear spin dynamics we measure nuclear ... | [['nuclear', 'polarization', 'dynamics', 'are', 'measured', 'in', 'the', 'nuclear', 'spin', 'bistability', 'regime', 'in', 'a', 'single', 'optically', 'pumped', 'ingaasgaas', 'quantum', 'dot', 'the', 'controlling', 'role', 'of', 'nuclear', 'spin', 'diffusion', 'from', 'the', 'dot', 'into', 'the', 'surrounding', 'materi... | [-0.12212573669743367, 0.252436833232283, -0.033062433931403436, 0.01244745801467126, 0.05275222797913907, -0.14428864479906714, -0.016764369983530533, 0.4189007953883937, -0.30365465392913815, -0.23121490109210405, 0.06741193336963008, -0.2743007765384391, 0.008126273643798552, 0.22476352646481246, 0.08715014045055096... |
708.2793 | WEBT and XMM-Newton observations of 3C 454.3 during the post-outburst
phase. Detection of the little and big blue bumps | The blazar 3C 454.3 underwent an unprecedented optical outburst in spring
2005. This was first followed by a mm and then by a cm radio outburst, which
peaked in February 2006. We report on follow-up observations by the WEBT to
study the multiwavelength emission in the post-outburst phase. XMM-Newton
observations on J... | astro-ph | the blazar 3c 4543 underwent an unprecedented optical outburst in spring 2005 this was first followed by a mm and then by a cm radio outburst which peaked in february 2006 we report on followup observations by the webt to study the multiwavelength emission in the postoutburst phase xmmnewton observations on july and de... | [['the', 'blazar', '3c', '4543', 'underwent', 'an', 'unprecedented', 'optical', 'outburst', 'in', 'spring', '2005', 'this', 'was', 'first', 'followed', 'by', 'a', 'mm', 'and', 'then', 'by', 'a', 'cm', 'radio', 'outburst', 'which', 'peaked', 'in', 'february', '2006', 'we', 'report', 'on', 'followup', 'observations', 'by... | [-0.04598703834832826, 0.12185748757550638, -0.10202203602192082, 0.05714660760995391, -0.1062725002101938, -0.09928037829963761, 0.06284230042177613, 0.4777121062901232, -0.1634808419696656, -0.3459088082477871, 0.1223736735579047, -0.3187632263044737, -0.06001340065643402, 0.20030165488189536, -0.06600150919151812, -... |
708.2794 | Freezing distributed entanglement in spin chains | We show how to freeze distributed entanglement that has been created from the
natural dynamics of spin chain systems. The technique that we propose simply
requires single-qubit operations and isolates the entanglement in specific
qubits at the ends of branches. Such frozen entanglement provides a useful
resource, for... | quant-ph | we show how to freeze distributed entanglement that has been created from the natural dynamics of spin chain systems the technique that we propose simply requires singlequbit operations and isolates the entanglement in specific qubits at the ends of branches such frozen entanglement provides a useful resource for examp... | [['we', 'show', 'how', 'to', 'freeze', 'distributed', 'entanglement', 'that', 'has', 'been', 'created', 'from', 'the', 'natural', 'dynamics', 'of', 'spin', 'chain', 'systems', 'the', 'technique', 'that', 'we', 'propose', 'simply', 'requires', 'singlequbit', 'operations', 'and', 'isolates', 'the', 'entanglement', 'in', ... | [-0.17332280469808456, 0.21267277966594186, -0.08142906655103149, 0.02248299589789495, 0.03648369722976917, -0.23564680507860897, 0.052146905309111785, 0.39965313318662526, -0.2768064076762374, -0.2684853036956089, 0.060396276729567565, -0.24132173066595342, -0.08056226491405652, 0.24171048374960152, -0.039776692513331... |
708.2795 | Superconductivity and antiferromagnetism in the two-dimensional Hubbard
model: a variational study | A variational ground state of the repulsive Hubbard model on a square lattice
is investigated numerically for an intermediate coupling strength (U = 8t) and
for moderate sizes (from 6 x 6 to 10 x 10). Our ansatz is clearly superior to
other widely used variational wave functions. The results for order parameters
and ... | cond-mat.str-el cond-mat.supr-con | a variational ground state of the repulsive hubbard model on a square lattice is investigated numerically for an intermediate coupling strength u 8t and for moderate sizes from 6 x 6 to 10 x 10 our ansatz is clearly superior to other widely used variational wave functions the results for order parameters and correlatio... | [['a', 'variational', 'ground', 'state', 'of', 'the', 'repulsive', 'hubbard', 'model', 'on', 'a', 'square', 'lattice', 'is', 'investigated', 'numerically', 'for', 'an', 'intermediate', 'coupling', 'strength', 'u', '8t', 'and', 'for', 'moderate', 'sizes', 'from', '6', 'x', '6', 'to', '10', 'x', '10', 'our', 'ansatz', 'i... | [-0.11315797875898007, 0.14281290539600797, -0.0013495442481377185, 0.12109033373268083, -0.025107902594101734, -0.16342634280833104, 0.10896806366956578, 0.38453320499796134, -0.24144401864554638, -0.28804966150439726, 0.10491616308736877, -0.31037035832802456, -0.08377883115257972, 0.19386507221796095, 0.130297498347... |
708.2796 | The spatial clustering of mid-IR selected star forming galaxies at z ~ 1
in the GOODS fields | We present the first spatial clustering measurements of z~1, 24um-selected,
star forming galaxies in the Great Observatories Origins Deep Survey (GOODS).
The sample under investigation includes 495 objects in GOODS-South and 811
objects in GOODS-North selected down to flux densities of f_24>20 uJy and
z_AB<23.5 mag, ... | astro-ph | we present the first spatial clustering measurements of z1 24umselected star forming galaxies in the great observatories origins deep survey goods the sample under investigation includes 495 objects in goodssouth and 811 objects in goodsnorth selected down to flux densities of f_2420 ujy and z_ab235 mag for which spect... | [['we', 'present', 'the', 'first', 'spatial', 'clustering', 'measurements', 'of', 'z1', '24umselected', 'star', 'forming', 'galaxies', 'in', 'the', 'great', 'observatories', 'origins', 'deep', 'survey', 'goods', 'the', 'sample', 'under', 'investigation', 'includes', '495', 'objects', 'in', 'goodssouth', 'and', '811', '... | [-0.05711987492019318, 0.09168047059111353, -0.06630591211659911, 0.14523854489684346, -0.05687350606963662, -0.013703270361602958, 0.030916531359557305, 0.4568833493487732, -0.08858492602806665, -0.36201199257087685, 0.07106144986152578, -0.3338289804784971, 0.016540471066680062, 0.2048662336016982, 0.0034262499313433... |
708.2797 | Investigating the Relationship Between the Hot Gas and the Dark Matter
Components of Galaxy Clusters | Various differences in galaxy cluster properties derived from X-ray and weak
lensing observations have been highlighted in the literature. One such
difference is the observation of mass concentrations in lensing maps which have
no X-ray counterparts (e.g. Jee, White, Ford et al. 2005). We investigate this
issue by id... | astro-ph | various differences in galaxy cluster properties derived from xray and weak lensing observations have been highlighted in the literature one such difference is the observation of mass concentrations in lensing maps which have no xray counterparts eg jee white ford et al 2005 we investigate this issue by identifying sub... | [['various', 'differences', 'in', 'galaxy', 'cluster', 'properties', 'derived', 'from', 'xray', 'and', 'weak', 'lensing', 'observations', 'have', 'been', 'highlighted', 'in', 'the', 'literature', 'one', 'such', 'difference', 'is', 'the', 'observation', 'of', 'mass', 'concentrations', 'in', 'lensing', 'maps', 'which', '... | [-0.04602480768309241, 0.027714363661029244, -0.08266770165729602, 0.12937976970403856, -0.058602346121915616, 0.004698179570758449, 0.01508721693244297, 0.43618426664865445, -0.18209139720836123, -0.38324716560808675, 0.08529265538839224, -0.35121940942813773, -0.11013602892801698, 0.21497111970425717, -0.022098060173... |
708.2798 | Inflection Point Inflation and Time Dependent Potentials in String
Theory | We consider models of inflection point inflation. The main drawback of such
models is that they suffer from the overshoot problem. Namely the initial
condition should be fine tuned to be near the inflection point for the universe
to inflate. We show that stringy realizations of inflection point inflation are
common a... | hep-th astro-ph.CO hep-ph | we consider models of inflection point inflation the main drawback of such models is that they suffer from the overshoot problem namely the initial condition should be fine tuned to be near the inflection point for the universe to inflate we show that stringy realizations of inflection point inflation are common and of... | [['we', 'consider', 'models', 'of', 'inflection', 'point', 'inflation', 'the', 'main', 'drawback', 'of', 'such', 'models', 'is', 'that', 'they', 'suffer', 'from', 'the', 'overshoot', 'problem', 'namely', 'the', 'initial', 'condition', 'should', 'be', 'fine', 'tuned', 'to', 'be', 'near', 'the', 'inflection', 'point', 'f... | [-0.10170416906476021, 0.12722228266453992, -0.13886617856721084, 0.135392818749339, -0.09568070170159142, -0.17292446983822932, 0.029003068959961336, 0.37189403201142945, -0.3411439452941219, -0.27889261251936354, 0.1589725617164125, -0.24665554659441113, -0.1345465324508647, 0.1637242000317201, -0.13326610622461885, ... |
708.2799 | A three-qubit interpretation of BPS and non-BPS STU black holes | Following the recent trend we develop further the black hole analogy between
quantum information theory and the theory of extremal stringy black hole
solutions. We show that the three-qubit interpretation of supersymmetric black
hole solutions in the STU model can be extended also to include
non-supersymmetric ones. ... | hep-th astro-ph quant-ph | following the recent trend we develop further the black hole analogy between quantum information theory and the theory of extremal stringy black hole solutions we show that the threequbit interpretation of supersymmetric black hole solutions in the stu model can be extended also to include nonsupersymmetric ones first ... | [['following', 'the', 'recent', 'trend', 'we', 'develop', 'further', 'the', 'black', 'hole', 'analogy', 'between', 'quantum', 'information', 'theory', 'and', 'the', 'theory', 'of', 'extremal', 'stringy', 'black', 'hole', 'solutions', 'we', 'show', 'that', 'the', 'threequbit', 'interpretation', 'of', 'supersymmetric', '... | [-0.14597842618577966, 0.15813952917976024, -0.05352169767429586, 0.10103327162735361, -0.024358682442260415, -0.17372308804310466, 0.050867057261424826, 0.29052871071586484, -0.22308764616272558, -0.28838830354966616, 0.10470853819830442, -0.3244213986958034, -0.11330367643753753, 0.15612840870836456, -0.1017544291594... |
708.28 | Synchrotron Self-Absorption Process in GRBs and the Isotropic Energy -
Peak Energy Fundamental Relation | The existence of strong correlation between the peak luminosity (and/or
bolometric energetics) of Gamma Ray Bursts (GRB) is one of the most intrigue
problem of GRB physics. This correlation is not yet understood. Here we
demonstrate that this correlation can be explained in framework of synchrotron
self-absorption (S... | astro-ph | the existence of strong correlation between the peak luminosity andor bolometric energetics of gamma ray bursts grb is one of the most intrigue problem of grb physics this correlation is not yet understood here we demonstrate that this correlation can be explained in framework of synchrotron selfabsorption ssa mechanis... | [['the', 'existence', 'of', 'strong', 'correlation', 'between', 'the', 'peak', 'luminosity', 'andor', 'bolometric', 'energetics', 'of', 'gamma', 'ray', 'bursts', 'grb', 'is', 'one', 'of', 'the', 'most', 'intrigue', 'problem', 'of', 'grb', 'physics', 'this', 'correlation', 'is', 'not', 'yet', 'understood', 'here', 'we',... | [-0.08692384096975257, 0.1590673577988387, -0.06296489959244024, 0.22227489593432756, -0.09956348599720892, -0.06850431221476816, 0.02243149048322207, 0.47565226147991496, -0.22026206938362403, -0.2958183642960601, -0.02916119110546764, -0.2860270734247449, 0.003183264057786966, 0.22460774002617903, 0.05929847740169082... |
708.2801 | Simple proof of a useful pointwise estimate for the wave equation | We give a simple proof of a pointwise decay estimate in 3+1 dimensions stated
in two versions, making advantage of a particular simplicity of inverting the
spherically symmetric part of the wave operator and of the comparison theorem.
We briefly explain the role of this estimate in proving decay estimates for
nonline... | math-ph math.MP | we give a simple proof of a pointwise decay estimate in 31 dimensions stated in two versions making advantage of a particular simplicity of inverting the spherically symmetric part of the wave operator and of the comparison theorem we briefly explain the role of this estimate in proving decay estimates for nonlinear wa... | [['we', 'give', 'a', 'simple', 'proof', 'of', 'a', 'pointwise', 'decay', 'estimate', 'in', '31', 'dimensions', 'stated', 'in', 'two', 'versions', 'making', 'advantage', 'of', 'a', 'particular', 'simplicity', 'of', 'inverting', 'the', 'spherically', 'symmetric', 'part', 'of', 'the', 'wave', 'operator', 'and', 'of', 'the... | [-0.11792916790582239, 0.04930218858644366, -0.07703175360026458, 0.11627695809778137, -0.07936799214221538, -0.08465130568947643, -0.01803035258005063, 0.26662260852754116, -0.20707380004848044, -0.22769255588452023, 0.15028140614158475, -0.24032415105029942, -0.1645136281750941, 0.19253707963895675, -0.01018469114787... |
708.2802 | Plasma induced neutrino spin-flip in a supernova and new bounds on the
neutrino magnetic moment | The neutrino chirality-flip process under the conditions of the supernova
core is investigated in detail with the plasma polarization effects in the
photon propagator taken into account in a more complete form than in earlier
publications. It is shown in part that the contribution of the proton fraction
of plasma is ... | hep-ph | the neutrino chiralityflip process under the conditions of the supernova core is investigated in detail with the plasma polarization effects in the photon propagator taken into account in a more complete form than in earlier publications it is shown in part that the contribution of the proton fraction of plasma is esse... | [['the', 'neutrino', 'chiralityflip', 'process', 'under', 'the', 'conditions', 'of', 'the', 'supernova', 'core', 'is', 'investigated', 'in', 'detail', 'with', 'the', 'plasma', 'polarization', 'effects', 'in', 'the', 'photon', 'propagator', 'taken', 'into', 'account', 'in', 'a', 'more', 'complete', 'form', 'than', 'in',... | [-0.05787748371601168, 0.20627990335178298, -0.005748920775472353, 0.14241063611392685, -0.018478829379822325, -0.0076184543819787605, 0.08580537350613497, 0.3348838289419555, -0.14643541686077657, -0.3435503824208027, 0.06483138418203203, -0.3135484803117748, 0.023554100026177544, 0.2247559778774396, 0.064945376052274... |
708.2803 | The Lorentz Integral Transform (LIT) method and its applications to
perturbation induced reactions | The LIT method has allowed ab initio calculations of electroweak cross
sections in light nuclear systems. This review presents a description of the
method from both a general and a more technical point of view, as well as a
summary of the results obtained by its application. The remarkable features of
the LIT approac... | nucl-th | the lit method has allowed ab initio calculations of electroweak cross sections in light nuclear systems this review presents a description of the method from both a general and a more technical point of view as well as a summary of the results obtained by its application the remarkable features of the lit approach whi... | [['the', 'lit', 'method', 'has', 'allowed', 'ab', 'initio', 'calculations', 'of', 'electroweak', 'cross', 'sections', 'in', 'light', 'nuclear', 'systems', 'this', 'review', 'presents', 'a', 'description', 'of', 'the', 'method', 'from', 'both', 'a', 'general', 'and', 'a', 'more', 'technical', 'point', 'of', 'view', 'as'... | [-0.07031805667187048, 0.07294523634724707, -0.1208355039249606, 0.09956326847410917, -0.012306682649068534, -0.10064926189564478, 0.03159224938281113, 0.3563991301925853, -0.19239516938008214, -0.2722220301899749, 0.06632382948252295, -0.274249581474578, -0.14366570408067977, 0.24688695492174398, 0.02809926914051175, ... |
708.2804 | On Fast-Decodable Space-Time Block Codes | We focus on full-rate, fast-decodable space-time block codes (STBCs) for 2x2
and 4x2 multiple-input multiple-output (MIMO) transmission. We first derive
conditions for reduced-complexity maximum-likelihood decoding, and apply them
to a unified analysis of two families of 2x2 STBCs that were recently proposed.
In part... | cs.IT math.IT | we focus on fullrate fastdecodable spacetime block codes stbcs for 2x2 and 4x2 multipleinput multipleoutput mimo transmission we first derive conditions for reducedcomplexity maximumlikelihood decoding and apply them to a unified analysis of two families of 2x2 stbcs that were recently proposed in particular we describ... | [['we', 'focus', 'on', 'fullrate', 'fastdecodable', 'spacetime', 'block', 'codes', 'stbcs', 'for', '2x2', 'and', '4x2', 'multipleinput', 'multipleoutput', 'mimo', 'transmission', 'we', 'first', 'derive', 'conditions', 'for', 'reducedcomplexity', 'maximumlikelihood', 'decoding', 'and', 'apply', 'them', 'to', 'a', 'unifi... | [-0.29003007586212143, -0.03204420454015857, -0.017750253570020982, 0.0661205063868118, -0.032951558505086916, -0.3406273778834331, 0.03341684281507409, 0.4181050330424975, -0.19852244439167216, -0.20243608276053382, 0.1528080348767904, -0.16826630679057225, -0.33278114270222814, 0.17707037948390567, -0.151227019806882... |
708.2805 | The public goods game on homogeneous and heterogeneous networks:
investment strategy according to the pool size | We propose an extended public goods interaction model to study the evolution
of cooperation in heterogeneous population. The investors are arranged on the
well known scale-free type network, the Barab\'{a}si-Albert model. Each
investor is supposed to preferentially distribute capital to pools in its
portfolio based o... | q-fin.GN physics.gen-ph physics.soc-ph q-fin.PM | we propose an extended public goods interaction model to study the evolution of cooperation in heterogeneous population the investors are arranged on the well known scalefree type network the barabasialbert model each investor is supposed to preferentially distribute capital to pools in its portfolio based on the knowl... | [['we', 'propose', 'an', 'extended', 'public', 'goods', 'interaction', 'model', 'to', 'study', 'the', 'evolution', 'of', 'cooperation', 'in', 'heterogeneous', 'population', 'the', 'investors', 'are', 'arranged', 'on', 'the', 'well', 'known', 'scalefree', 'type', 'network', 'the', 'barabasialbert', 'model', 'each', 'inv... | [-0.11244970843934671, 0.12272535466873069, -0.04253171340175519, 0.11911235020944107, -0.08292173882036057, -0.20585113882850437, 0.08333716438067867, 0.43054511106776117, -0.2654850394184932, -0.3078491190112287, 0.05749348987110967, -0.29955792978153867, -0.13116613774441352, 0.09961882563608986, -0.0290620822119841... |
708.2806 | Harmonic nets in metric spaces | We investigate harmonic maps from weighted graphs into metric spaces that
locally admit unique centers of gravity, like Alexandrov spaces with upper
curvature bounds. We prove an existence result by constructing an iterative
geometric process that converges to such maps, called harmonic nets for short.
| math.MG | we investigate harmonic maps from weighted graphs into metric spaces that locally admit unique centers of gravity like alexandrov spaces with upper curvature bounds we prove an existence result by constructing an iterative geometric process that converges to such maps called harmonic nets for short | [['we', 'investigate', 'harmonic', 'maps', 'from', 'weighted', 'graphs', 'into', 'metric', 'spaces', 'that', 'locally', 'admit', 'unique', 'centers', 'of', 'gravity', 'like', 'alexandrov', 'spaces', 'with', 'upper', 'curvature', 'bounds', 'we', 'prove', 'an', 'existence', 'result', 'by', 'constructing', 'an', 'iterativ... | [-0.11196192665956914, 0.1068846548086084, -0.09101357541771399, 0.1481588478991196, -0.085458628502157, -0.13248922967662413, -0.028279209426707693, 0.4295387858110997, -0.3144154705107212, -0.17333336460093657, 0.12973335449350998, -0.2919613880001836, -0.19926114498327177, 0.22462613781293234, -0.15603818921372295, ... |
708.2807 | Energies of B_s meson excited states - a lattice study | This is a follow-up to our earlier work on the energies and radial
distributions of heavy-light mesons. The heavy quark is taken to be static
(infinitely heavy) and the light quark has a mass about that of the strange
quark. We now concentrate on the energies of the excited states with higher
angular momentum and wit... | hep-lat hep-ph | this is a followup to our earlier work on the energies and radial distributions of heavylight mesons the heavy quark is taken to be static infinitely heavy and the light quark has a mass about that of the strange quark we now concentrate on the energies of the excited states with higher angular momentum and with a radi... | [['this', 'is', 'a', 'followup', 'to', 'our', 'earlier', 'work', 'on', 'the', 'energies', 'and', 'radial', 'distributions', 'of', 'heavylight', 'mesons', 'the', 'heavy', 'quark', 'is', 'taken', 'to', 'be', 'static', 'infinitely', 'heavy', 'and', 'the', 'light', 'quark', 'has', 'a', 'mass', 'about', 'that', 'of', 'the',... | [-0.11307650158188254, 0.20940688184224807, -0.1039881880977191, 0.06150727941551142, -0.06805670436264741, -0.10971568610273405, 0.09240830224007368, 0.36789935189816686, -0.1698204909477176, -0.25475264801255737, 0.02908084574737586, -0.3035316234403581, -0.0051488815561040405, 0.12187210370579528, 0.0298925496068679... |
708.2808 | Inclusive Perspectives | I discuss the relation between inclusive and exclusive dynamics suggested by
Bloom-Gilman duality. Duality implies the simultaneous applicability of two
distinct limits, the standard DIS limit of hard inclusive processes taken at
fixed xB and a limit where the hadronic mass is held fixed. I review
experimental eviden... | hep-ph | i discuss the relation between inclusive and exclusive dynamics suggested by bloomgilman duality duality implies the simultaneous applicability of two distinct limits the standard dis limit of hard inclusive processes taken at fixed xb and a limit where the hadronic mass is held fixed i review experimental evidence for... | [['i', 'discuss', 'the', 'relation', 'between', 'inclusive', 'and', 'exclusive', 'dynamics', 'suggested', 'by', 'bloomgilman', 'duality', 'duality', 'implies', 'the', 'simultaneous', 'applicability', 'of', 'two', 'distinct', 'limits', 'the', 'standard', 'dis', 'limit', 'of', 'hard', 'inclusive', 'processes', 'taken', '... | [-0.08541199619260927, 0.22975065579776766, -0.1340896653485272, 0.1618325472043484, -0.0020175636439633215, -0.11099045732254653, 0.10810203196709617, 0.3217950345817627, -0.22548668469269678, -0.17953858649962695, -0.0092792815861717, -0.30723800749534314, 0.006102237409274829, 0.11316724851106603, 0.0545711316170350... |
708.2809 | Quantum enhancement of N-photon phase sensitivity by interferometric
addition of down-converted photon pairs to weak coherent light | It is shown that the addition of down-converted photon pairs to coherent
laser light enhances the N-photon phase sensitivity due to the quantum
interference between components of the same total photon number. Since most of
the photons originate from the coherent laser light, this method of obtaining
non-classical N-p... | quant-ph | it is shown that the addition of downconverted photon pairs to coherent laser light enhances the nphoton phase sensitivity due to the quantum interference between components of the same total photon number since most of the photons originate from the coherent laser light this method of obtaining nonclassical nphoton st... | [['it', 'is', 'shown', 'that', 'the', 'addition', 'of', 'downconverted', 'photon', 'pairs', 'to', 'coherent', 'laser', 'light', 'enhances', 'the', 'nphoton', 'phase', 'sensitivity', 'due', 'to', 'the', 'quantum', 'interference', 'between', 'components', 'of', 'the', 'same', 'total', 'photon', 'number', 'since', 'most',... | [-0.09100499238538583, 0.252389178508627, -0.08682930757047481, 0.0705193591968708, -0.022707099714361637, -0.1443165790117843, 0.09482579051236649, 0.3713174528505617, -0.2416426783881955, -0.3076180327249673, -0.012649912873138358, -0.3173482841586025, -0.04538416136191814, 0.25606592591327515, -0.026036319196296547,... |
708.281 | Is a soft nuclear equation of state extracted from heavy-ion data
incompatible with pulsar data? | We discuss the recent constraints on the nuclear equation of state from
pulsar mass measurements and from subthreshold production of kaons in heavy-ion
collisions. While recent pulsar data points towards a hard equation of state,
the analysis of the heavy-ion data allows only for soft equations of state. We
resolve t... | astro-ph nucl-th | we discuss the recent constraints on the nuclear equation of state from pulsar mass measurements and from subthreshold production of kaons in heavyion collisions while recent pulsar data points towards a hard equation of state the analysis of the heavyion data allows only for soft equations of state we resolve the appa... | [['we', 'discuss', 'the', 'recent', 'constraints', 'on', 'the', 'nuclear', 'equation', 'of', 'state', 'from', 'pulsar', 'mass', 'measurements', 'and', 'from', 'subthreshold', 'production', 'of', 'kaons', 'in', 'heavyion', 'collisions', 'while', 'recent', 'pulsar', 'data', 'points', 'towards', 'a', 'hard', 'equation', '... | [-0.09852848507871385, 0.14844798674621415, -0.1606643754435936, 0.09439982097828761, -0.06983708234911319, -0.07177154996315949, 0.03258553809282603, 0.30895035518333314, -0.23060727202100678, -0.31398496588808483, 0.049815674206183755, -0.34843543634360685, 0.03867689108010382, 0.2210161649156362, 0.03118245578450569... |
708.2811 | Engineering of arbitrary U(N) transformations by quantum Householder
reflections | We propose a simple physical implementation of the quantum Householder
reflection (QHR) M(v)=I-2|v><v| in a quantum system of N degenerate states
(forming a qunit) coupled simultaneously to an ancillary (excited) state by N
resonant or nearly resonant pulsed external fields. We also introduce the
generalized QHR M(v;... | quant-ph | we propose a simple physical implementation of the quantum householder reflection qhr mvi2vv in a quantum system of n degenerate states forming a qunit coupled simultaneously to an ancillary excited state by n resonant or nearly resonant pulsed external fields we also introduce the generalized qhr mvkiexpik1vv which ca... | [['we', 'propose', 'a', 'simple', 'physical', 'implementation', 'of', 'the', 'quantum', 'householder', 'reflection', 'qhr', 'mvi2vv', 'in', 'a', 'quantum', 'system', 'of', 'n', 'degenerate', 'states', 'forming', 'a', 'qunit', 'coupled', 'simultaneously', 'to', 'an', 'ancillary', 'excited', 'state', 'by', 'n', 'resonant... | [-0.13678936527576296, 0.21933179182697132, -0.05446983004512731, 0.03425077387946658, -0.005120942009671126, -0.21780943571357056, 0.024179650640871842, 0.36977071208530105, -0.2380600562217296, -0.2846748937969096, 0.08371274997844011, -0.24015370764536784, -0.1454634143570729, 0.17527421228842285, -0.006600543696549... |
708.2812 | Unparticle effects in Supernovae cooling | Recently H. Georgi suggested that a scale invariant unparticle
${\mathcal{U}}$ sector with an infrared fixed point at high energy can couple
with the SM matter via a higher-dimensional operator suppressed by a high
cut-off scale. Intense phenomenological search of this unparticle sector in the
collider and flavour ph... | hep-ph | recently h georgi suggested that a scale invariant unparticle mathcalu sector with an infrared fixed point at high energy can couple with the sm matter via a higherdimensional operator suppressed by a high cutoff scale intense phenomenological search of this unparticle sector in the collider and flavour physics context... | [['recently', 'h', 'georgi', 'suggested', 'that', 'a', 'scale', 'invariant', 'unparticle', 'mathcalu', 'sector', 'with', 'an', 'infrared', 'fixed', 'point', 'at', 'high', 'energy', 'can', 'couple', 'with', 'the', 'sm', 'matter', 'via', 'a', 'higherdimensional', 'operator', 'suppressed', 'by', 'a', 'high', 'cutoff', 'sc... | [-0.09394063937330717, 0.23353602790754704, -0.10767995941109564, 0.16042036551271419, -0.11156160556711256, -0.14065606784516652, 0.024762736166533277, 0.3222132200277165, -0.24692894343936228, -0.2866399045935587, 0.0458781635793122, -0.27968530569127514, -0.08997437485346668, 0.12540045862429236, 0.04622335706731782... |
708.2813 | Study of nuclear correlation effects via 12C(p,n)12N(g.s.,1+) at 296 MeV | We report measurements of the cross section and a complete set of
polarization observables for the Gamow--Teller ${}^{12}{\rm
C}(\vec{p},\vec{n}){}^{12}{\rm N}({\rm g.s.},1^+)$ reaction at a bombarding
energy of 296 MeV.
The data are compared with distorted wave impulse approximation calculations
employing transiti... | nucl-ex | we report measurements of the cross section and a complete set of polarization observables for the gamowteller 12rm cvecpvecn12rm nrm gs1 reaction at a bombarding energy of 296 mev the data are compared with distorted wave impulse approximation calculations employing transition form factors normalized to reproduce the ... | [['we', 'report', 'measurements', 'of', 'the', 'cross', 'section', 'and', 'a', 'complete', 'set', 'of', 'polarization', 'observables', 'for', 'the', 'gamowteller', '12rm', 'cvecpvecn12rm', 'nrm', 'gs1', 'reaction', 'at', 'a', 'bombarding', 'energy', 'of', '296', 'mev', 'the', 'data', 'are', 'compared', 'with', 'distort... | [-0.08441833936795592, 0.17852730049192905, -0.04727874610037543, 0.12520725207962097, 0.04719165067444556, -0.05015884714759886, 0.041502587627619505, 0.37311236263811587, -0.19914016000926493, -0.3182760902494192, -0.04923751960508525, -0.35382866361737253, 0.018709628675307614, 0.14704450157145038, 0.099071894437074... |
708.2814 | Polarizability of molecular chains: does one need exact exchange? | Standard density functional approximations greatly over-estimate the static
polarizability of longchain polymers, but Hartree-Fock or exact exchange
calculations do not. Simple self-interaction corrected (SIC) approximations can
be even better than exact exchange, while their computational cost can scale
only linearl... | physics.atm-clus cond-mat.mtrl-sci physics.comp-ph | standard density functional approximations greatly overestimate the static polarizability of longchain polymers but hartreefock or exact exchange calculations do not simple selfinteraction corrected sic approximations can be even better than exact exchange while their computational cost can scale only linearly with the... | [['standard', 'density', 'functional', 'approximations', 'greatly', 'overestimate', 'the', 'static', 'polarizability', 'of', 'longchain', 'polymers', 'but', 'hartreefock', 'or', 'exact', 'exchange', 'calculations', 'do', 'not', 'simple', 'selfinteraction', 'corrected', 'sic', 'approximations', 'can', 'be', 'even', 'bet... | [-0.1202431058096092, 0.13542325883779838, -0.04630139494395774, 0.156568700791863, -0.04512249693557944, -0.20747536514460554, 0.09237337069909858, 0.3942082301085896, -0.2307946544505008, -0.3552059828526462, -0.012758962364624376, -0.31626184681511443, -0.06329861159294682, 0.06613259251563526, 0.04197099276453904, ... |
708.2815 | Driven degenerate three-level cascade laser | We analyze a degenerate three-level cascade laser coupled to an external
coherent light via one of the coupler mirrors and vacuum reservoir in the
other, employing the stochastic differential equation associated with the
normal ordering. We study the squeezing properties and also calculate the mean
photon number of t... | quant-ph | we analyze a degenerate threelevel cascade laser coupled to an external coherent light via one of the coupler mirrors and vacuum reservoir in the other employing the stochastic differential equation associated with the normal ordering we study the squeezing properties and also calculate the mean photon number of the ca... | [['we', 'analyze', 'a', 'degenerate', 'threelevel', 'cascade', 'laser', 'coupled', 'to', 'an', 'external', 'coherent', 'light', 'via', 'one', 'of', 'the', 'coupler', 'mirrors', 'and', 'vacuum', 'reservoir', 'in', 'the', 'other', 'employing', 'the', 'stochastic', 'differential', 'equation', 'associated', 'with', 'the', ... | [-0.14353578705049586, 0.22964625364303565, -0.09500394360033429, 0.050508664046771755, -0.008442357267735392, -0.13997276883206464, 0.003938502940789996, 0.3729357610074138, -0.27693183234493646, -0.2880305923588042, 0.05592396267768761, -0.26953800054798194, -0.0858366726440311, 0.25696884286922533, -0.02826728949107... |
708.2816 | Testing Isotropy of Cosmic Microwave Background Radiation | We introduce new symmetry-based methods to test for isotropy in cosmic
microwave background radiation. Each angular multipole is factored into unique
products of power eigenvectors, related multipoles and singular values that
provide 2 new rotationally invariant measures mode by mode. The power entropy
and directiona... | astro-ph | we introduce new symmetrybased methods to test for isotropy in cosmic microwave background radiation each angular multipole is factored into unique products of power eigenvectors related multipoles and singular values that provide 2 new rotationally invariant measures mode by mode the power entropy and directional entr... | [['we', 'introduce', 'new', 'symmetrybased', 'methods', 'to', 'test', 'for', 'isotropy', 'in', 'cosmic', 'microwave', 'background', 'radiation', 'each', 'angular', 'multipole', 'is', 'factored', 'into', 'unique', 'products', 'of', 'power', 'eigenvectors', 'related', 'multipoles', 'and', 'singular', 'values', 'that', 'p... | [-0.1109723651822766, 0.14200863983723513, -0.04215571886914618, 0.07795204521663597, -0.09880015105146038, -0.14563817452940653, -0.008250396208399359, 0.36680959695402315, -0.25536861860686366, -0.28250732941224294, 0.061520227774470936, -0.3106548322145553, -0.022593946371446638, 0.22128233279731563, 0.0120550023787... |
708.2817 | Thermal expansion of the magnetically ordering intermetallics RTMg (R =
Eu, Gd and T = Ag, Au) | We report measurements of the thermal expansion for two Eu$^{+2}$- and two
Gd$^{+3}$-based intermetallics which exhibit ferro- or antiferromagnetic phase
transitions. These materials show sharp positive (EuAgMg and GdAuMg) and
negative (EuAuMg and GdAgMg) peaks in the temperature dependence of the thermal
expansion c... | cond-mat.mtrl-sci cond-mat.other | we report measurements of the thermal expansion for two eu2 and two gd3based intermetallics which exhibit ferro or antiferromagnetic phase transitions these materials show sharp positive euagmg and gdaumg and negative euaumg and gdagmg peaks in the temperature dependence of the thermal expansion coefficient alpha which... | [['we', 'report', 'measurements', 'of', 'the', 'thermal', 'expansion', 'for', 'two', 'eu2', 'and', 'two', 'gd3based', 'intermetallics', 'which', 'exhibit', 'ferro', 'or', 'antiferromagnetic', 'phase', 'transitions', 'these', 'materials', 'show', 'sharp', 'positive', 'euagmg', 'and', 'gdaumg', 'and', 'negative', 'euaumg... | [-0.16807315349624066, 0.27775809049136707, -0.05588269806964305, -0.0008204956765024407, -0.038521989768606074, -0.15372691493372895, 0.09465962266594678, 0.3959749039009358, -0.26559876748225064, -0.30510708602886755, 0.055930662687158086, -0.33094424099742786, -0.05961535200114968, 0.13979463764687874, 0.12098724294... |
708.2818 | Baryon-charge Chemical Potential in AdS/CFT | We present a closed framework of AdS/CFT with finite U(1)B-charge chemical
potential. We show how the gauge-invariant identification of the chemical
potential with the bulk gauge field emerges from the standard AdS/CFT
dictionary. Physical importance and necessity of the Minkowski embeddings
within the present framew... | hep-th hep-ph nucl-th | we present a closed framework of adscft with finite u1bcharge chemical potential we show how the gaugeinvariant identification of the chemical potential with the bulk gauge field emerges from the standard adscft dictionary physical importance and necessity of the minkowski embeddings within the present framework is als... | [['we', 'present', 'a', 'closed', 'framework', 'of', 'adscft', 'with', 'finite', 'u1bcharge', 'chemical', 'potential', 'we', 'show', 'how', 'the', 'gaugeinvariant', 'identification', 'of', 'the', 'chemical', 'potential', 'with', 'the', 'bulk', 'gauge', 'field', 'emerges', 'from', 'the', 'standard', 'adscft', 'dictionar... | [-0.08609647025318387, 0.10961813618336896, -0.1265180998706965, 0.07500432223813343, -0.056427337167845974, -0.094890147739264, 0.044657218080668984, 0.365256427449512, -0.21183364731924875, -0.23959584259888628, 0.04715147481688841, -0.2596182399889925, -0.19822236053021317, 0.13108949964753464, -0.035750138836882106... |
708.2819 | On the cyclic subgroup separability of free products of two groups with
amalgamated subgroup | Let $G$ be a free product of two groups with amalgamated subgroup, $\pi$ be
either the set of all prime numbers or the one-element set \{$p$\} for some
prime number $p$. Denote by $\Sigma$ the family of all cyclic subgroups of
group $G$, which are separable in the class of all finite $\pi$-groups.
Obviously, cyclic s... | math.GR | let g be a free product of two groups with amalgamated subgroup pi be either the set of all prime numbers or the oneelement set p for some prime number p denote by sigma the family of all cyclic subgroups of group g which are separable in the class of all finite pigroups obviously cyclic subgroups of the free factors w... | [['let', 'g', 'be', 'a', 'free', 'product', 'of', 'two', 'groups', 'with', 'amalgamated', 'subgroup', 'pi', 'be', 'either', 'the', 'set', 'of', 'all', 'prime', 'numbers', 'or', 'the', 'oneelement', 'set', 'p', 'for', 'some', 'prime', 'number', 'p', 'denote', 'by', 'sigma', 'the', 'family', 'of', 'all', 'cyclic', 'subgr... | [-0.20108262292381857, 0.22295452612547242, -0.06213143886364743, 0.003345725212886068, -0.09084626605740564, -0.14173344212273756, -0.005288951355507787, 0.3789179349178765, -0.3499347049438832, -0.24073982027162905, 0.10046981081531263, -0.2724867768040827, -0.03490778768029647, 0.22172137937464176, -0.10522642762077... |
708.282 | Associated Charm Production in Neutrino-Nucleus Interactions | In this paper a search for associated charm production both in neutral and
charged current $\nu$-nucleus interactions is presented. The improvement of
automatic scanning systems in the {CHORUS} experiment allows an efficient
search to be performed in emulsion for short-lived particles. Hence a search
for rare process... | hep-ex | in this paper a search for associated charm production both in neutral and charged current nunucleus interactions is presented the improvement of automatic scanning systems in the chorus experiment allows an efficient search to be performed in emulsion for shortlived particles hence a search for rare processes like the... | [['in', 'this', 'paper', 'a', 'search', 'for', 'associated', 'charm', 'production', 'both', 'in', 'neutral', 'and', 'charged', 'current', 'nunucleus', 'interactions', 'is', 'presented', 'the', 'improvement', 'of', 'automatic', 'scanning', 'systems', 'in', 'the', 'chorus', 'experiment', 'allows', 'an', 'efficient', 'sea... | [-0.07385645611812511, 0.21852844528085927, -0.048267964319130705, 0.13319997678721143, 0.012617849438421189, -0.1101651863780834, 0.04205486023002454, 0.337707858801549, -0.18015138183630283, -0.3091288190214865, 0.01834716117535267, -0.4043695835713034, 0.030482301843022145, 0.15765739187087502, 0.08683888618458784, ... |
708.2821 | Collective flow in heavy ion collisions at intermediate energies | We present results of a flow analysis for the set of reactions of 124,129Xe
projectiles and 112,124Sn targets at incident energies 100 and 150 A MeV
studied with the INDRA detector at GSI. The dependence on centrality and on p_t
of the directed and elliptic flow are determined for isotopically selected
reaction produ... | nucl-ex | we present results of a flow analysis for the set of reactions of 124129xe projectiles and 112124sn targets at incident energies 100 and 150 a mev studied with the indra detector at gsi the dependence on centrality and on p_t of the directed and elliptic flow are determined for isotopically selected reaction products w... | [['we', 'present', 'results', 'of', 'a', 'flow', 'analysis', 'for', 'the', 'set', 'of', 'reactions', 'of', '124129xe', 'projectiles', 'and', '112124sn', 'targets', 'at', 'incident', 'energies', '100', 'and', '150', 'a', 'mev', 'studied', 'with', 'the', 'indra', 'detector', 'at', 'gsi', 'the', 'dependence', 'on', 'centr... | [-0.06548855966927174, 0.24974786893128315, -0.08710638730594332, 0.04396286472264263, 0.03822017640332989, -0.11317809277938472, -0.016674313290018797, 0.4041007755634685, -0.21242805287733468, -0.3347018566499982, -0.020482961788527772, -0.42789796988169354, 0.06905187529304789, 0.19305153756674068, 0.080663682957593... |
708.2822 | The high mass end of the Tully-Fisher relation | We study the location of massive disk galaxies on the Tully-Fisher relation.
Using a combination of K-band photometry and high-quality rotation curves, we
show that in traditional formulations of the TF relation (using the width of
the global HI profile or the maximum rotation velocity), galaxies with rotation
veloci... | astro-ph | we study the location of massive disk galaxies on the tullyfisher relation using a combination of kband photometry and highquality rotation curves we show that in traditional formulations of the tf relation using the width of the global hi profile or the maximum rotation velocity galaxies with rotation velocities large... | [['we', 'study', 'the', 'location', 'of', 'massive', 'disk', 'galaxies', 'on', 'the', 'tullyfisher', 'relation', 'using', 'a', 'combination', 'of', 'kband', 'photometry', 'and', 'highquality', 'rotation', 'curves', 'we', 'show', 'that', 'in', 'traditional', 'formulations', 'of', 'the', 'tf', 'relation', 'using', 'the',... | [-0.07435303794322073, 0.11073004433785157, -0.09569030888532558, 0.11391774799159059, -0.11112761750340092, -0.043862290870906276, 0.036751890832111854, 0.3924775599571299, -0.1829530080195424, -0.3498182735994674, 0.04645626170874365, -0.28385825922581837, -0.062021690489116224, 0.22165948198049923, -0.02768752431835... |
708.2823 | Bedforms in a turbulent stream.Part 1: Turbulent flow over topography | In the context of subaqueous ripple and dune formation, we present here a
Reynolds averaged calculation of the turbulent flow over a topography. We
perform a weakly non-linear expansion of the velocity field, sufficiently
accurate to recover the separation of streamlines and the formation of a
recirculation bubble ab... | cond-mat.soft | in the context of subaqueous ripple and dune formation we present here a reynolds averaged calculation of the turbulent flow over a topography we perform a weakly nonlinear expansion of the velocity field sufficiently accurate to recover the separation of streamlines and the formation of a recirculation bubble above so... | [['in', 'the', 'context', 'of', 'subaqueous', 'ripple', 'and', 'dune', 'formation', 'we', 'present', 'here', 'a', 'reynolds', 'averaged', 'calculation', 'of', 'the', 'turbulent', 'flow', 'over', 'a', 'topography', 'we', 'perform', 'a', 'weakly', 'nonlinear', 'expansion', 'of', 'the', 'velocity', 'field', 'sufficiently'... | [-0.13923840912343083, 0.1744320617160973, -0.06334264618897084, 0.011205110186710953, -0.028632195007008643, -0.04008786080630054, -0.01408769060478751, 0.3287744643719141, -0.31220216588551275, -0.2702831962718076, 0.0785156935552072, -0.24418374979079274, -0.12717549919655893, 0.17800073026584745, -0.010543955087472... |
708.2824 | Cosmology with Galaxy Correlations | In this review, I outline the use of galaxy correlations to constrain
cosmological parameters. As with the Cosmic Microwave Background (CMB), the
density of dark and baryonic matter imprints important scales on the
fluctuations of matter and thus the clustering of galaxies, e.g., the particle
horizon at matter--radia... | astro-ph | in this review i outline the use of galaxy correlations to constrain cosmological parameters as with the cosmic microwave background cmb the density of dark and baryonic matter imprints important scales on the fluctuations of matter and thus the clustering of galaxies eg the particle horizon at matterradiation equality... | [['in', 'this', 'review', 'i', 'outline', 'the', 'use', 'of', 'galaxy', 'correlations', 'to', 'constrain', 'cosmological', 'parameters', 'as', 'with', 'the', 'cosmic', 'microwave', 'background', 'cmb', 'the', 'density', 'of', 'dark', 'and', 'baryonic', 'matter', 'imprints', 'important', 'scales', 'on', 'the', 'fluctuat... | [-0.06986583250721819, 0.09780364465037374, -0.12453847232666847, 0.12148448581880841, -0.14932920684253698, -0.044954653663291155, -0.04610785637050867, 0.30756996083808574, -0.22438221544909634, -0.3347183234223753, 0.048155822841401554, -0.33454875769093634, -0.009186308674122158, 0.21026825067820026, 0.081746782352... |
708.2825 | Apollo asteroids (1566) Icarus and 2007 MK6: Icarus family members? | Although it is more complicated to search for near-Earth object (NEO)
families than main belt asteroid (MBA) families, since differential orbital
evolution within a NEO family can cause current orbital elements to drastically
differ from each other, we have found that Apollo asteroids (1566) Icarus and
the newly disc... | astro-ph | although it is more complicated to search for nearearth object neo families than main belt asteroid mba families since differential orbital evolution within a neo family can cause current orbital elements to drastically differ from each other we have found that apollo asteroids 1566 icarus and the newly discovered 2007... | [['although', 'it', 'is', 'more', 'complicated', 'to', 'search', 'for', 'nearearth', 'object', 'neo', 'families', 'than', 'main', 'belt', 'asteroid', 'mba', 'families', 'since', 'differential', 'orbital', 'evolution', 'within', 'a', 'neo', 'family', 'can', 'cause', 'current', 'orbital', 'elements', 'to', 'drastically',... | [-0.08742825589165344, 0.15745432346110408, -0.113142897646187, 0.06568540553607553, -0.09462678773798844, -0.048744523663806175, 0.02217134084095907, 0.37479015262526216, -0.1941160457073123, -0.4024954242812632, 0.06123090138912056, -0.29320034055599886, -0.14403125482783155, 0.2231353976497047, -0.15522416591309735,... |
708.2826 | Magnetic and transport properties of the one-dimensional ferromagnetic
Kondo lattice model with an impurity | We have studied the ferromagnetic Kondo lattice model (FKLM) with an Anderson
impurity on finite chains with numerical techniques. We are particularly
interested in the metallic ferromagnetic phase of the FKLM. This model could
describe either a quantum dot coupled to one-dimensional ferromagnetic leads
made with man... | cond-mat.str-el | we have studied the ferromagnetic kondo lattice model fklm with an anderson impurity on finite chains with numerical techniques we are particularly interested in the metallic ferromagnetic phase of the fklm this model could describe either a quantum dot coupled to onedimensional ferromagnetic leads made with manganites... | [['we', 'have', 'studied', 'the', 'ferromagnetic', 'kondo', 'lattice', 'model', 'fklm', 'with', 'an', 'anderson', 'impurity', 'on', 'finite', 'chains', 'with', 'numerical', 'techniques', 'we', 'are', 'particularly', 'interested', 'in', 'the', 'metallic', 'ferromagnetic', 'phase', 'of', 'the', 'fklm', 'this', 'model', '... | [-0.12272925168001039, 0.22659077540895872, 0.0017041830064425635, 0.07920353839290328, 0.007105304602381968, -0.23545350375866822, 0.07920709025956756, 0.4088429748527381, -0.23694547641613564, -0.267690633835141, 0.028153227223218745, -0.33377631673816766, -0.09212815187814602, 0.13694363389554065, 0.0472430012411868... |
708.2827 | Brown dwarf formation by gravitational fragmentation of massive,
extended protostellar discs | We suggest that low-mass hydrogen-burning stars like the Sun should sometimes
form with massive extended discs; and we show, by means of radiation
hydrodynamic simulations, that the outer parts of such discs (R>100 AU) are
likely to fragment on a dynamical timescale (10^3 to $10^4 yr), forming
low-mass companions: pr... | astro-ph | we suggest that lowmass hydrogenburning stars like the sun should sometimes form with massive extended discs and we show by means of radiation hydrodynamic simulations that the outer parts of such discs r100 au are likely to fragment on a dynamical timescale 103 to 104 yr forming lowmass companions principally brown dw... | [['we', 'suggest', 'that', 'lowmass', 'hydrogenburning', 'stars', 'like', 'the', 'sun', 'should', 'sometimes', 'form', 'with', 'massive', 'extended', 'discs', 'and', 'we', 'show', 'by', 'means', 'of', 'radiation', 'hydrodynamic', 'simulations', 'that', 'the', 'outer', 'parts', 'of', 'such', 'discs', 'r100', 'au', 'are'... | [-0.1283204653197523, 0.2144084858024405, -0.06769374874986855, 0.14939946674150667, -0.11991020294413818, -0.07090383765920662, 0.05248279925045407, 0.3610440628090037, -0.18274350808780015, -0.36315504036018414, 0.05469091375034949, -0.24728955029549, -0.05535653002318246, 0.16831488011008922, -0.08491896441928529, -... |
708.2828 | Characterizations of Hankel multipliers | We give characterizations of radial Fourier multipliers as acting on radial
L^p-functions, 1<p<2d/(d+1), in terms of Lebesgue space norms for Fourier
localized pieces of the convolution kernel. This is a special case of
corresponding results for general Hankel multipliers. Besides L^p-L^q bounds we
also characterize ... | math.CA | we give characterizations of radial fourier multipliers as acting on radial lpfunctions 1p2dd1 in terms of lebesgue space norms for fourier localized pieces of the convolution kernel this is a special case of corresponding results for general hankel multipliers besides lplq bounds we also characterize weak type inequal... | [['we', 'give', 'characterizations', 'of', 'radial', 'fourier', 'multipliers', 'as', 'acting', 'on', 'radial', 'lpfunctions', '1p2dd1', 'in', 'terms', 'of', 'lebesgue', 'space', 'norms', 'for', 'fourier', 'localized', 'pieces', 'of', 'the', 'convolution', 'kernel', 'this', 'is', 'a', 'special', 'case', 'of', 'correspon... | [-0.09527656243594944, 0.07808816732770046, -0.056874945859012545, 0.1583872560839184, -0.12017962668610156, -0.09229425442420312, -0.03301672219512526, 0.3751556598505036, -0.28474432735352734, -0.12388864038970138, 0.1866355771408798, -0.25456404764220486, -0.12770300563119474, 0.31692267702434396, -0.109418776115310... |
708.2829 | Effective action for the field equations of charged black holes | In this article, we consistently reduce the equations of motion for the
bosonic N = 2 supergravity action, using a multi-centered black hole ansatz for
the metric. This reduction is done in a general, non-supersymmetric setup, in
which we extend concepts of BPS black hole technology. First of all we obtain a
more gen... | hep-th | in this article we consistently reduce the equations of motion for the bosonic n 2 supergravity action using a multicentered black hole ansatz for the metric this reduction is done in a general nonsupersymmetric setup in which we extend concepts of bps black hole technology first of all we obtain a more general form of... | [['in', 'this', 'article', 'we', 'consistently', 'reduce', 'the', 'equations', 'of', 'motion', 'for', 'the', 'bosonic', 'n', '2', 'supergravity', 'action', 'using', 'a', 'multicentered', 'black', 'hole', 'ansatz', 'for', 'the', 'metric', 'this', 'reduction', 'is', 'done', 'in', 'a', 'general', 'nonsupersymmetric', 'set... | [-0.11289066532952026, 0.06361174863270529, -0.05413248373181833, 0.10644157880126252, -0.055044223694815576, -0.12007174692981233, 0.00830008128147764, 0.3105945788693669, -0.16109888030298272, -0.2911703964996645, 0.09939276266617098, -0.27874989103635445, -0.1907625199511291, 0.1721311102840392, -0.08210878395338488... |
708.283 | Symmetry Energy as a Function of Density and Mass | Energy in nuclear matter is, in practice, completely characterized at
different densities and asymmetries, when the density dependencies of symmetry
energy and of energy of symmetric matter are specified. The density dependence
of the symmetry energy at subnormal densities produces mass dependence of
nuclear symmetry... | nucl-th | energy in nuclear matter is in practice completely characterized at different densities and asymmetries when the density dependencies of symmetry energy and of energy of symmetric matter are specified the density dependence of the symmetry energy at subnormal densities produces mass dependence of nuclear symmetry coeff... | [['energy', 'in', 'nuclear', 'matter', 'is', 'in', 'practice', 'completely', 'characterized', 'at', 'different', 'densities', 'and', 'asymmetries', 'when', 'the', 'density', 'dependencies', 'of', 'symmetry', 'energy', 'and', 'of', 'energy', 'of', 'symmetric', 'matter', 'are', 'specified', 'the', 'density', 'dependence'... | [-0.09508404785320779, 0.2522367258625459, -0.06281551538219998, 0.07721707176163116, -0.030243952163064098, -0.06454103180661427, 0.014874340412168464, 0.3524923094121108, -0.22810520133588555, -0.3702472879605229, 0.0348679431115685, -0.26196997268664196, 0.004894143478436904, 0.1353722157587936, 0.07396063909765856,... |
708.2831 | The rotational broadening of V395 Car - implications on compact object's
mass | CONTEXT: The masses previously obtained for the X-ray binary 2S0921-630
inferred a compact object that was either a high-mass neutron star or low-mass
black-hole, but used a previously published value for the rotational broadening
(vsini) with large uncertainties. AIMS: We aim to determine an accurate mass
for the co... | astro-ph | context the masses previously obtained for the xray binary 2s0921630 inferred a compact object that was either a highmass neutron star or lowmass blackhole but used a previously published value for the rotational broadening vsini with large uncertainties aims we aim to determine an accurate mass for the compact object ... | [['context', 'the', 'masses', 'previously', 'obtained', 'for', 'the', 'xray', 'binary', '2s0921630', 'inferred', 'a', 'compact', 'object', 'that', 'was', 'either', 'a', 'highmass', 'neutron', 'star', 'or', 'lowmass', 'blackhole', 'but', 'used', 'a', 'previously', 'published', 'value', 'for', 'the', 'rotational', 'broad... | [-0.04924851204309244, 0.0760381534483438, -0.09050619602925325, 0.06800812270263094, -0.12645174890337874, -0.11712487617168257, 0.08062806928732483, 0.44229389630373594, -0.15961716210021992, -0.37319705877164305, 0.05130937100476549, -0.25499179185817766, -0.010231975257548308, 0.2250765811150186, -0.086095117751776... |
708.2832 | On Reedy Model Categories | The sole purpose of this note is to introduce some elementary results on the
structure and functoriality of Reedy model categories. In particular, I give a
very useful little criterion to determine whether composition with a morphism
of Reedy categories determines a left or right Quillen functor. I then give a
number... | math.AT math.CT | the sole purpose of this note is to introduce some elementary results on the structure and functoriality of reedy model categories in particular i give a very useful little criterion to determine whether composition with a morphism of reedy categories determines a left or right quillen functor i then give a number of u... | [['the', 'sole', 'purpose', 'of', 'this', 'note', 'is', 'to', 'introduce', 'some', 'elementary', 'results', 'on', 'the', 'structure', 'and', 'functoriality', 'of', 'reedy', 'model', 'categories', 'in', 'particular', 'i', 'give', 'a', 'very', 'useful', 'little', 'criterion', 'to', 'determine', 'whether', 'composition', ... | [-0.10737292705120385, 0.013912782929505088, -0.11556804303212889, 0.15391271546416516, -0.15912287323070423, -0.2108461925028158, 0.020636223472787867, 0.37363773833827246, -0.3750581650861672, -0.22439407156447747, 0.05726162933569867, -0.1407549463172992, -0.14634060349635547, 0.10994287974400711, -0.197649404606116... |
708.2833 | Fully Unintegrated Parton Correlation Functions and Factorization in
Lowest Order Hard Scattering | Motivated by the need to correct the potentially large kinematic errors in
approximations used in the standard formulation of perturbative QCD, we
reformulate deeply inelastic lepton-proton scattering in terms of gauge
invariant, universal parton correlation functions which depend on all
components of parton four-mom... | hep-ph | motivated by the need to correct the potentially large kinematic errors in approximations used in the standard formulation of perturbative qcd we reformulate deeply inelastic leptonproton scattering in terms of gauge invariant universal parton correlation functions which depend on all components of parton fourmomentum ... | [['motivated', 'by', 'the', 'need', 'to', 'correct', 'the', 'potentially', 'large', 'kinematic', 'errors', 'in', 'approximations', 'used', 'in', 'the', 'standard', 'formulation', 'of', 'perturbative', 'qcd', 'we', 'reformulate', 'deeply', 'inelastic', 'leptonproton', 'scattering', 'in', 'terms', 'of', 'gauge', 'invaria... | [-0.06966270092371638, 0.15411340372487045, -0.14873180799614424, 0.14880635216096202, -0.10110037037085784, -0.07316440171776233, 0.03400704652424259, 0.3648738457189723, -0.21466106426334758, -0.26189829096005396, 0.0048529844029924305, -0.23095249141641389, -0.1054965327600895, 0.1251898403413294, -0.025435040378407... |
708.2834 | Negative differential resistance of Styrene on an ideal Si[111] surface:
dependence of the I-V characteristics on geometry, surface doping and shape
of the STM-tip | We study the electron transport properties through a supported organic
molecule styrene (C8H8) on an ideal silicon surface Si[111] and probed by a
STM-tip. The I-V characteristics and the differential conductance of the
molecule are calculated using a self consistent approach based on non
equilibrium Green's function... | cond-mat.mtrl-sci | we study the electron transport properties through a supported organic molecule styrene c8h8 on an ideal silicon surface si111 and probed by a stmtip the iv characteristics and the differential conductance of the molecule are calculated using a self consistent approach based on non equilibrium greens functions two diff... | [['we', 'study', 'the', 'electron', 'transport', 'properties', 'through', 'a', 'supported', 'organic', 'molecule', 'styrene', 'c8h8', 'on', 'an', 'ideal', 'silicon', 'surface', 'si111', 'and', 'probed', 'by', 'a', 'stmtip', 'the', 'iv', 'characteristics', 'and', 'the', 'differential', 'conductance', 'of', 'the', 'molec... | [-0.14114067862182855, 0.0989216293200152, -0.0695655214805156, 0.044722909320145846, 0.01844467356428504, -0.1383776979409158, 0.08611903997231275, 0.37918915165029465, -0.24607641102746128, -0.29217146326601506, 0.03410878738202155, -0.30088194377720356, -0.1195209389552474, 0.20838919995725155, 0.0063164516966789964... |
708.2835 | Unraveling unparticles through violation of atomic parity and rare
beauty | We put constraints on unparticle physics, specifically on the scale
$\Lambda_\U$ and the scale dimension $d_\U$ of unparticle operators, using (i)
measurements of atomic parity violation as well as (ii) branching ratio and CP
asymmetry measurements in some rare non-leptonic B decay channels.
| hep-ph | we put constraints on unparticle physics specifically on the scale lambda_u and the scale dimension d_u of unparticle operators using i measurements of atomic parity violation as well as ii branching ratio and cp asymmetry measurements in some rare nonleptonic b decay channels | [['we', 'put', 'constraints', 'on', 'unparticle', 'physics', 'specifically', 'on', 'the', 'scale', 'lambda_u', 'and', 'the', 'scale', 'dimension', 'd_u', 'of', 'unparticle', 'operators', 'using', 'i', 'measurements', 'of', 'atomic', 'parity', 'violation', 'as', 'well', 'as', 'ii', 'branching', 'ratio', 'and', 'cp', 'as... | [-0.1345868410588632, 0.26317386786171865, 0.002927806071373959, 0.16109560248117114, -0.09904308066443475, -0.23739388326269595, 0.11645544844484607, 0.21712720385471054, -0.25531946750747603, -0.26937512117762896, 0.07196022265016773, -0.32402264886687315, -0.04231435239185081, 0.0755279952400299, 0.13777209129617657... |
708.2836 | Free-Floating HI Clouds in the M 81 Group | Recent VLA observations pointed at dwarf spheroidal (dSph) galaxies in the M
81 group reveal a hitherto hidden population of extremely low mass (~1e5 Msol)
HI clouds with no obvious optical counterparts. We have searched 10 fields in
the M81 group totalling 2.2 square degree, both targeting known dwarf
spheroidal gal... | astro-ph | recent vla observations pointed at dwarf spheroidal dsph galaxies in the m 81 group reveal a hitherto hidden population of extremely low mass 1e5 msol hi clouds with no obvious optical counterparts we have searched 10 fields in the m81 group totalling 22 square degree both targeting known dwarf spheroidal galaxies and ... | [['recent', 'vla', 'observations', 'pointed', 'at', 'dwarf', 'spheroidal', 'dsph', 'galaxies', 'in', 'the', 'm', '81', 'group', 'reveal', 'a', 'hitherto', 'hidden', 'population', 'of', 'extremely', 'low', 'mass', '1e5', 'msol', 'hi', 'clouds', 'with', 'no', 'obvious', 'optical', 'counterparts', 'we', 'have', 'searched'... | [-0.11943633604373428, 0.07907886118517213, -0.06474610851035409, 0.11563673398701385, -0.1137273551943335, -0.07289623485190705, 0.06210865857013102, 0.42957676485890434, -0.11405328073583189, -0.3743922883295454, 0.04050996242273998, -0.2946110988213193, -0.04304277875746179, 0.15183911555297008, -0.01141089023457468... |
708.2837 | The Physics of Information | We review of the interface between (theoretical) physics and information for
non-experts. The origin of information as related to the notion of entropy is
described, first in the context of thermodynamics then in the context of
statistical mechanics. A close examination of the foundations of statistical
mechanics and... | physics.class-ph cond-mat.stat-mech gr-qc physics.gen-ph quant-ph | we review of the interface between theoretical physics and information for nonexperts the origin of information as related to the notion of entropy is described first in the context of thermodynamics then in the context of statistical mechanics a close examination of the foundations of statistical mechanics and the nee... | [['we', 'review', 'of', 'the', 'interface', 'between', 'theoretical', 'physics', 'and', 'information', 'for', 'nonexperts', 'the', 'origin', 'of', 'information', 'as', 'related', 'to', 'the', 'notion', 'of', 'entropy', 'is', 'described', 'first', 'in', 'the', 'context', 'of', 'thermodynamics', 'then', 'in', 'the', 'con... | [-0.06700574723269664, 0.12145689650060376, -0.11620111700336812, 0.12178128972793613, -0.09908487800295639, -0.15384688428642576, 0.05625964627429543, 0.2929913284888706, -0.2943467533381624, -0.3008799579456228, 0.11075519524333147, -0.2779539608232819, -0.16805411467597015, 0.18979217558783495, -0.11420275769144655,... |
708.2838 | CW type of inverse limits and function spaces | Given CW complexes X and Y, let map(X,Y) denote the space of continuous
functions from X to Y with the compact open topology. The space map(X,Y) need
not have the homotopy type of a CW complex. Here the results of an extensive
investigation of various necessary and various sufficient conditions for
map(X,Y) to have t... | math.AT | given cw complexes x and y let mapxy denote the space of continuous functions from x to y with the compact open topology the space mapxy need not have the homotopy type of a cw complex here the results of an extensive investigation of various necessary and various sufficient conditions for mapxy to have the homotopy ty... | [['given', 'cw', 'complexes', 'x', 'and', 'y', 'let', 'mapxy', 'denote', 'the', 'space', 'of', 'continuous', 'functions', 'from', 'x', 'to', 'y', 'with', 'the', 'compact', 'open', 'topology', 'the', 'space', 'mapxy', 'need', 'not', 'have', 'the', 'homotopy', 'type', 'of', 'a', 'cw', 'complex', 'here', 'the', 'results',... | [-0.15375868403827725, 0.08582934304637156, -0.05790732781731742, 0.10795035158673218, -0.09205164603885513, -0.14582650823546434, 0.020139664218677626, 0.3894450667578338, -0.3146491546684237, -0.23337631553077876, 0.1387795443531932, -0.20215053717716971, -0.15587669261615372, 0.2513152377920883, -0.13955085235532022... |
708.2839 | Quark mass and condensate in HQCD | We extend the Sakai-Sugimoto holographic model of QCD (HQCD) by including the
scalar bi-fundamental "tachyon" field in the 8-brane-anti-8-brane probe theory.
We show that this field is responsible both for the spontaneous breaking of the
chiral symmetry, and for the generation of (current algebra) quark masses, from
... | hep-th hep-ph | we extend the sakaisugimoto holographic model of qcd hqcd by including the scalar bifundamental tachyon field in the 8braneanti8brane probe theory we show that this field is responsible both for the spontaneous breaking of the chiral symmetry and for the generation of current algebra quark masses from the point of view... | [['we', 'extend', 'the', 'sakaisugimoto', 'holographic', 'model', 'of', 'qcd', 'hqcd', 'by', 'including', 'the', 'scalar', 'bifundamental', 'tachyon', 'field', 'in', 'the', '8braneanti8brane', 'probe', 'theory', 'we', 'show', 'that', 'this', 'field', 'is', 'responsible', 'both', 'for', 'the', 'spontaneous', 'breaking',... | [-0.09818000104278327, 0.2102336498110422, -0.10024371773802808, 0.09909507301469733, -0.06983678407434907, -0.05143739519241665, 0.03583459918487019, 0.29290599888190627, -0.2041167533823422, -0.2507651944644749, 0.0356096137165358, -0.23811911647873266, -0.14423605961658592, 0.10036985645004148, 0.017725526980523553,... |
708.284 | CO-activator model for reconstructing Pt(100) surfaces: local
microstructures and chemical turbulence | We present the results of the modelling of CO adsorption and catalytic CO
oxidation on inhomogeneous Pt(100) surfaces which contain structurally
different areas. These areas are formed during the CO-induced transition from a
reconstructed phase with hexagonal geometry of the overlayer to a bulk-like
(1x1) phase with ... | cond-mat.stat-mech cond-mat.mtrl-sci | we present the results of the modelling of co adsorption and catalytic co oxidation on inhomogeneous pt100 surfaces which contain structurally different areas these areas are formed during the coinduced transition from a reconstructed phase with hexagonal geometry of the overlayer to a bulklike 1x1 phase with square at... | [['we', 'present', 'the', 'results', 'of', 'the', 'modelling', 'of', 'co', 'adsorption', 'and', 'catalytic', 'co', 'oxidation', 'on', 'inhomogeneous', 'pt100', 'surfaces', 'which', 'contain', 'structurally', 'different', 'areas', 'these', 'areas', 'are', 'formed', 'during', 'the', 'coinduced', 'transition', 'from', 'a'... | [-0.15345764488810834, 0.20291275699283776, -0.059949333420174056, -0.006073646565005614, 0.02732407241505221, -0.10156000261006586, 0.07542952720205047, 0.37273678553931283, -0.25111436544556837, -0.28375430667848256, 0.07153126722264959, -0.2878209460483638, -0.1506166479609519, 0.13923381738407764, 0.013217602391973... |
708.2841 | Geodesics and Geodesic Deviation in static Charged Black Holes | The radial motion along null geodesics in static charged black hole
space-times, in particular, the Reissner-Nordstr\"om and stringy charged black
holes are studied. We analyzed the properties of the effective potential. The
circular photon orbits in these space-times are investigated. We found that the
radius of cir... | math-ph math.MP | the radial motion along null geodesics in static charged black hole spacetimes in particular the reissnernordstrom and stringy charged black holes are studied we analyzed the properties of the effective potential the circular photon orbits in these spacetimes are investigated we found that the radius of circular photon... | [['the', 'radial', 'motion', 'along', 'null', 'geodesics', 'in', 'static', 'charged', 'black', 'hole', 'spacetimes', 'in', 'particular', 'the', 'reissnernordstrom', 'and', 'stringy', 'charged', 'black', 'holes', 'are', 'studied', 'we', 'analyzed', 'the', 'properties', 'of', 'the', 'effective', 'potential', 'the', 'circ... | [-0.1716442094919713, 0.14318934013870985, -0.038317666673346566, 0.1740140494645426, -0.014756870367809346, -0.1512851740674753, -0.08370558929286505, 0.340467326205812, -0.08856489663257411, -0.2827566497027874, 0.015974827410996352, -0.38068257062450833, -0.05451384552901513, 0.1916573773285276, -0.05926147241537508... |
708.2842 | The Structural Parameters of Bulges, Bars and Discs in the Local
Universe | Image decomposition of galaxies is now routinely used to estimate the
structural parameters of galactic components. In this work, I address questions
on the reliability of this technique. In particular, do bars and AGN need to be
taken into account to obtain the structural parameters of bulges and discs? And
to what ... | astro-ph | image decomposition of galaxies is now routinely used to estimate the structural parameters of galactic components in this work i address questions on the reliability of this technique in particular do bars and agn need to be taken into account to obtain the structural parameters of bulges and discs and to what extent ... | [['image', 'decomposition', 'of', 'galaxies', 'is', 'now', 'routinely', 'used', 'to', 'estimate', 'the', 'structural', 'parameters', 'of', 'galactic', 'components', 'in', 'this', 'work', 'i', 'address', 'questions', 'on', 'the', 'reliability', 'of', 'this', 'technique', 'in', 'particular', 'do', 'bars', 'and', 'agn', '... | [-0.03995278256430322, 0.07426495525701823, -0.08494465612861628, 0.10804665696331679, -0.08342633367085955, -0.08714102819893446, 0.042479747539323015, 0.41650020228540996, -0.2296153725562933, -0.35324112332220803, 0.10486226427611516, -0.26711653459864526, -0.0663618535758884, 0.1714673184289526, -0.1053742067769990... |
708.2843 | The Impossibility Of Secure Two-Party Classical Computation | We present attacks that show that unconditionally secure two-party classical
computation is impossible for many classes of function. Our analysis applies to
both quantum and relativistic protocols. We illustrate our results by showing
the impossibility of oblivious transfer.
| quant-ph cs.CR | we present attacks that show that unconditionally secure twoparty classical computation is impossible for many classes of function our analysis applies to both quantum and relativistic protocols we illustrate our results by showing the impossibility of oblivious transfer | [['we', 'present', 'attacks', 'that', 'show', 'that', 'unconditionally', 'secure', 'twoparty', 'classical', 'computation', 'is', 'impossible', 'for', 'many', 'classes', 'of', 'function', 'our', 'analysis', 'applies', 'to', 'both', 'quantum', 'and', 'relativistic', 'protocols', 'we', 'illustrate', 'our', 'results', 'by'... | [-0.1833381248748322, 0.01278032345305148, -0.11640381185632002, 0.12182583318300251, 0.022470585805805104, -0.2462745316718754, 0.09415898495353758, 0.3706258542615136, -0.24750401099261485, -0.27345565632966, 0.0650700236774834, -0.205887625729175, -0.20941549853274696, 0.3286310099065304, -0.11999356850758072, 0.160... |
708.2844 | Dynamics of Femtosecond Electron Bunches | In the laser wakefield accelerator (LWFA) a short intense laser pulse, with a
duration of the order of a plasma wave period, excites an unusually strong
plasma wake wave (laser wakefield). Recent experiments on laser wakefield
acceleration [Nature (London) 431, p.535, p.538, p.541 (2004)] demonstrated
generation of u... | physics.plasm-ph physics.acc-ph | in the laser wakefield accelerator lwfa a short intense laser pulse with a duration of the order of a plasma wave period excites an unusually strong plasma wake wave laser wakefield recent experiments on laser wakefield acceleration nature london 431 p535 p538 p541 2004 demonstrated generation of ultrashort with a dura... | [['in', 'the', 'laser', 'wakefield', 'accelerator', 'lwfa', 'a', 'short', 'intense', 'laser', 'pulse', 'with', 'a', 'duration', 'of', 'the', 'order', 'of', 'a', 'plasma', 'wave', 'period', 'excites', 'an', 'unusually', 'strong', 'plasma', 'wake', 'wave', 'laser', 'wakefield', 'recent', 'experiments', 'on', 'laser', 'wa... | [-0.1448545073399513, 0.29105624621282766, -0.06003611679000761, 0.10083823904778451, 0.04965980248784439, -0.13153478630225768, -0.05361985887172679, 0.5094191231905962, -0.22238248886394718, -0.2903134030186468, -0.0005182235424096385, -0.23231144513666743, 0.07559194494123486, 0.30250150304654555, -0.028384914116068... |
708.2845 | Transport of a quantum degenerate heteronuclear Bose-Fermi mixture in a
harmonic trap | We report on the transport of mixed quantum degenerate gases of bosonic 87Rb
and fermionic 40K in a harmonic potential provided by a modified QUIC trap. The
samples are transported over a distance of 6 mm to the geometric center of the
anti-Helmholtz coils of the QUIC trap. This transport mechanism was implemented
by... | cond-mat.other | we report on the transport of mixed quantum degenerate gases of bosonic 87rb and fermionic 40k in a harmonic potential provided by a modified quic trap the samples are transported over a distance of 6 mm to the geometric center of the antihelmholtz coils of the quic trap this transport mechanism was implemented by a sm... | [['we', 'report', 'on', 'the', 'transport', 'of', 'mixed', 'quantum', 'degenerate', 'gases', 'of', 'bosonic', '87rb', 'and', 'fermionic', '40k', 'in', 'a', 'harmonic', 'potential', 'provided', 'by', 'a', 'modified', 'quic', 'trap', 'the', 'samples', 'are', 'transported', 'over', 'a', 'distance', 'of', '6', 'mm', 'to', ... | [-0.10802024220517738, 0.21474544931869438, -0.02372304093645416, -0.01590375723109043, 0.0046549024840256545, -0.1659842347385498, 0.06275676079548714, 0.38542441704227187, -0.24442781544313197, -0.2717159853384989, 0.06383744762203376, -0.2745026467251828, -0.03331177554479459, 0.24384890990407487, -0.007587914885120... |
708.2846 | On the origin of families of quarks and leptons - predictions for four
families | The approach unifying all the internal degrees of freedom--proposed by one of
us--is offering a new way of understanding families of quarks and leptons: A
part of the starting Lagrange density in d(=1+13), which includes two kinds of
spin connection fields--the gauge fields of two types of Clifford algebra
objects--t... | hep-ph | the approach unifying all the internal degrees of freedomproposed by one of usis offering a new way of understanding families of quarks and leptons a part of the starting lagrange density in d113 which includes two kinds of spin connection fieldsthe gauge fields of two types of clifford algebra objectstransforms the ri... | [['the', 'approach', 'unifying', 'all', 'the', 'internal', 'degrees', 'of', 'freedomproposed', 'by', 'one', 'of', 'usis', 'offering', 'a', 'new', 'way', 'of', 'understanding', 'families', 'of', 'quarks', 'and', 'leptons', 'a', 'part', 'of', 'the', 'starting', 'lagrange', 'density', 'in', 'd113', 'which', 'includes', 't... | [-0.1340185665541281, 0.2618694834813665, -0.0320257249848633, 0.09879879544141813, -0.06990301215003039, -0.12155312808798784, 0.018135783858439426, 0.29117605453199247, -0.2577368737695644, -0.3102479796477799, 0.024341143085621297, -0.27823691410643947, -0.02839023822186499, 0.11047757095045616, 0.07915212414464202,... |
708.2847 | Physical Properties of Red Supergiants | Red supergiants (RSGs) are an evolved stage in the life of intermediate
massive stars (<25Mo). For many years their location in the H-R diagram was at
variance with the evolutionary models. Using the MARCS stellar atmosphere
models, we have determined new effective temperatures and bolometric
luminosities for RSGs in... | astro-ph | red supergiants rsgs are an evolved stage in the life of intermediate massive stars 25mo for many years their location in the hr diagram was at variance with the evolutionary models using the marcs stellar atmosphere models we have determined new effective temperatures and bolometric luminosities for rsgs in the milky ... | [['red', 'supergiants', 'rsgs', 'are', 'an', 'evolved', 'stage', 'in', 'the', 'life', 'of', 'intermediate', 'massive', 'stars', '25mo', 'for', 'many', 'years', 'their', 'location', 'in', 'the', 'hr', 'diagram', 'was', 'at', 'variance', 'with', 'the', 'evolutionary', 'models', 'using', 'the', 'marcs', 'stellar', 'atmosp... | [0.0020822312669932013, 0.1032793857974765, -0.09758751538659756, 0.10720173755025068, -0.08071965023150875, -0.021255930067531556, 0.07816921032159978, 0.4943551559052948, -0.1135937502905209, -0.35544870835858294, 0.023818093936521716, -0.27655747743685627, -0.02189567137328494, 0.1794584738268491, -0.104177061846712... |
708.2848 | PKS1932-46: a radio source in an interacting group? | We present the results of a multiwavelength study of the z=0.23 radio source
PKS1932-46. VIMOS IFU spectroscopy is used to study the morphology, kinematics
and ionisation state of the EELR surrounding this source, and also a companion
galaxy at a similar redshift. Near- and far-IR imaging observations obtained
using ... | astro-ph | we present the results of a multiwavelength study of the z023 radio source pks193246 vimos ifu spectroscopy is used to study the morphology kinematics and ionisation state of the eelr surrounding this source and also a companion galaxy at a similar redshift near and farir imaging observations obtained using the ntt and... | [['we', 'present', 'the', 'results', 'of', 'a', 'multiwavelength', 'study', 'of', 'the', 'z023', 'radio', 'source', 'pks193246', 'vimos', 'ifu', 'spectroscopy', 'is', 'used', 'to', 'study', 'the', 'morphology', 'kinematics', 'and', 'ionisation', 'state', 'of', 'the', 'eelr', 'surrounding', 'this', 'source', 'and', 'als... | [-0.047486520415231596, 0.06297699636370863, -0.08651234162679332, 0.09030313843701705, -0.13533692093965657, -0.04995852831435296, 0.015501190768877064, 0.4733096989948032, -0.1352285488269366, -0.30346141904785867, 0.0900491774295679, -0.3013142314175576, -0.053268480726927005, 0.19828818124831704, -0.024550393637459... |
Subsets and Splits
No community queries yet
The top public SQL queries from the community will appear here once available.