Search results for "quantum field"

showing 10 items of 492 documents

Single chain structure in thin polymer films: Corrections to Flory's and Silberberg's hypotheses

2005

Conformational properties of polymer melts confined between two hard structureless walls are investigated by Monte Carlo simulation of the bond-fluctuation model. Parallel and perpendicular components of chain extension, bond-bond correlation function and structure factor are computed and compared with recent theoretical approaches attempting to go beyond Flory's and Silberberg's hypotheses. We demonstrate that for ultrathin films where the thickness, $H$, is smaller than the excluded volume screening length (blob size), $\xi$, the chain size parallel to the walls diverges logarithmically, $R^2/2N \approx b^2 + c \log(N)$ with $c \sim 1/H$. The corresponding bond-bond correlation function d…

FOS: Physical sciences02 engineering and technologyCondensed Matter - Soft Condensed MatterPlateau (mathematics)01 natural sciencesPower lawOmega0103 physical sciencesGeneral Materials Science61.25.Hq 67.70.+n010306 general physicspolymersMonte Carlo simulationPhysicsCondensed matter physicsForm factor (quantum field theory)021001 nanoscience & nanotechnologyCondensed Matter PhysicsCorrelation function (statistical mechanics)thin films[PHYS.COND.CM-GEN]Physics [physics]/Condensed Matter [cond-mat]/Other [cond-mat.other]Excluded volumeExponentSoft Condensed Matter (cond-mat.soft)0210 nano-technologyStructure factor
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Depletion in Bose-Einstein condensates using quantum field theory in curved space

2007

5 pages.-- PACS nrs.: 03.75.Kk; 05.30.Jp; 04.62.+v; 04.70.Dy.-- ISI Article Identifier: 000246074600122.-- ArXiv pre-print available at: http://arxiv.org/abs/cond-mat/0610367

FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Condensed Matter - Soft Condensed MatterBose-Einstein condensationGeneral Relativity and Quantum Cosmologylaw.inventionRenormalizationBOSE EINSTEIN CONDENSATElawQuantum mechanicsAtomSpace-time configurationsQuantum field theoryCurved spacePhysicsCondensed Matter::Quantum GasesTemperaturesQuantum field theory in curved spacetimeCondensed Matter::OtherBlack holesQuantum gravityQUANTUM FIELD THEORY IN CURVED SPACEAtomic and Molecular Physics and OpticsCondensed Matter - Other Condensed MatterQuantum electrodynamicsQuantum gravitySoft Condensed Matter (cond-mat.soft)Bose–Einstein condensateHawking radiationOther Condensed Matter (cond-mat.other)
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Scattering theory for a class of fermionic Pauli–Fierz models

2004

Abstract The scattering theory for a class of fermionic Pauli–Fierz models is considered. We give a proof of the asymptotic completeness of the dynamics in the case of massive fermions. The result applied to the Hamiltonian of a quantized spin- 1 2 Dirac particle interacting with an external field through a cutoff Yukawa interaction and to the Hamiltonian of a system of finitely many confined particles coupled to a fermionic field with a quadratic interaction.

Fermionic fieldHigh Energy Physics::LatticeScattering theoryFermionYukawa interactionQuantum field theorysymbols.namesakePauli exclusion principleQuadratic equationQuantum mechanicssymbolsAsymptotic completenessScattering theoryQuantum field theoryHamiltonian (quantum mechanics)FermionAnalysisMathematical physicsMathematicsJournal of Functional Analysis
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Large-N kinetic theory for highly occupied systems

2018

We consider an effective kinetic description for quantum many-body systems, which is not based on a weak-coupling or diluteness expansion. Instead, it employs an expansion in the number of field components N of the underlying scalar quantum field theory. Extending previous studies, we demonstrate that the large-N kinetic theory at next-to-leading order is able to describe important aspects of highly occupied systems, which are beyond standard perturbative kinetic approaches. We analyze the underlying quasiparticle dynamics by computing the effective scattering matrix elements analytically and solve numerically the large-N kinetic equation for a highly occupied system far from equilibrium. T…

Field (physics)Lattice field theoryFOS: Physical sciencesFixed point01 natural sciencesMany-body problemHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencessirontanonperturbative effects in field theoryQuantum field theory010306 general physicsdynamiikkaPhysicsta114010308 nuclear & particles physicsScalar (physics)finite temperature field theoryultracold gasesHigh Energy Physics - PhenomenologyDistribution functionClassical mechanicsQuantum Gases (cond-mat.quant-gas)Kinetic theory of gaseskvanttikenttäteoriaCondensed Matter - Quantum Gasesrelativistic heavy-ion collisions
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Spacetime curvature and Higgs stability after inflation

2015

We investigate the dynamics of the Higgs field at the end of inflation in the minimal scenario consisting of an inflaton field coupled to the Standard Model only through the non-minimal gravitational coupling $\xi$ of the Higgs field. Such a coupling is required by renormalisation of the Standard Model in curved space, and in the current scenario also by vacuum stability during high-scale inflation. We find that for $\xi\gtrsim 1$, rapidly changing spacetime curvature at the end of inflation leads to significant production of Higgs particles, potentially triggering a transition to a negative-energy Planck scale vacuum state and causing an immediate collapse of the Universe.

General PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)spacetime curvaturePhysics MultidisciplinaryVacuum stateFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciences09 Engineeringrenormalizationvacuum stateStandard ModelGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)vacuum stability0103 physical sciencesPARTICLE-PRODUCTIONELECTROWEAK VACUUMHiggs fieldHiggs particles010306 general physics01 Mathematical SciencesPlanck scalePhysicsInflation (cosmology)Science & Technology02 Physical SciencesQuantum field theory in curved spacetimeta114010308 nuclear & particles physicsPhysicsHigh Energy Physics::Phenomenologyhep-phInflatonFIELDSThe Standard ModelCREATIONHiggs fieldHigh Energy Physics - PhenomenologyPhysical Sciencesastro-ph.COHiggs bosonAstrophysics - Cosmology and Nongalactic Astrophysics
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Geometric quantization in the presence of an electromagnetic field

1983

Some aspects of the formalism of geometric quantization are described emphasizing the role played by the symmetry group of the quantum system which, for the free particle, turns out to be a central extensionG(m) of the Galilei groupG. The resulting formalism is then applied to the case of a particle interacting with the electromagnetic field, which appears as a necessary modification of the connection 1-form of the quantum bundle when its invariance group is generalized to alocal extension ofG. Finally, the quantization of the electric charge in the presence of a Dirac monopole is also briefly considered.

Geometric quantizationPhysicsQuantization (physics)Free particleClassical mechanicsPhysics and Astronomy (miscellaneous)Canonical quantizationGeneral MathematicsMagnetic monopoleQuantum field theoryQuantumSecond quantizationInternational Journal of Theoretical Physics
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Limits on neutral Higgs boson production in the forward region in $pp$ collisions at $\sqrt{s} = 7$ TeV

2013

Limits on the cross-section times branching fraction for neutral Higgs bosons, produced in p p collisions at root s = 7 TeV, and decaying to two tau leptons with pseudorapidities between 2.0 and 4.5, are presented. The result is based on a dataset, corresponding to an integrated luminosity of 1.0 fb(-1), collected with the LHCb detector. Candidates are identified by reconstructing final states with two muons, a muon and an electron, a muon and a hadron, or an electron and a hadron. A model independent upper limit at the 95% confidence level is set on a neutral Higgs boson cross-section times branching fraction. It varies from 8.6 pb for a Higgs boson mass of 90 GeV to 0.7 pb for a Higgs bos…

GravitacióSEARCH; MSSM; LHCHadronStandard-model Higgs boson7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Teoria quànticaNuclear ExperimentQCBosonPhysicsHiggs physicsQuantum field theoryHiggs bosonProduction (computer science)Física nuclearLHCHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified leptons photons or other nonhadronic particlesParticle Physics - ExperimentGravitationParticle physicsTeoria quàntica de campsNuclear and High Energy PhysicsFOS: Physical sciencesStandard-model Higgs bosons; Supersymmetric Higgs bosons; Hadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified leptons photons or other nonhadronic particlesHadronsPartícules (Física nuclear)Standard ModelSEARCH0103 physical sciences010306 general physicsLarge Hadron Collider (France and Switzerland)Standard-model Higgs bosonsMuonHadron-Hadron Scattering010308 nuclear & particles physicsBranching fractionComputer Science::Information RetrievalHadron-Hadron Scattering; Higgs physicsHigh Energy Physics::PhenomenologyGran Col·lisionador d'HadronsHiggs physicSupersymmetric Higgs bosonSupersymmetric Higgs bosonsQuantum theoryHadron-Hadron Scattering; Higgs physics; Nuclear and High Energy PhysicsHigh Energy Physics::ExperimentMSSMLepton
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Matter, quantum gravity, and adiabatic phase

1990

Based on the observation that particle masses are much smaller than the Planck mass, a framework for the matter-gravity system in which matter follows gravitation adiabatically is examined in a path-integral approach. It is found that the equations that the resulting gravitational wave function satisfies involve, in addition to the expectation value of the matter stress tensor, an adiabatically induced gauge field which can lead to interesting topological structures in superspace. Such a non-trivial geometric contribution modifies the semiclassical quantization condition and can change the conserved quantities associated with the symmetries of the system. © 1990 The American Physical Societ…

GravitationPhysicsQuantization (physics)Classical mechanicsQuantum theoryAdiabatic phaseEinstein field equationsPlanck massSemiclassical physicsQuantum gravityGauge theoryQuantum field theoryGravitationPhysical Review D
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Precision measurement of D meson mass differences

2013

Using three- and four-body decays of D mesons produced in semileptonic b-hadron decays, precision measurements of D meson mass differences are made together with a measurement of the D-0 mass. The measurements are based on a dataset corresponding to an integrated luminosity of 1.0 fb(-1) collected in pp collisions at 7 TeV. Using the decay D-0 -> K+K-K-pi(+), the D-0 mass is measured to be M(D-0) = 1864.75 +/- 0.15 (stat) +/- 0.11 (syst) MeV/c(2). The mass differences M(D+) - M(D-0) = 4.76 +/- 0.12 (stat) +/- 0.07 (syst) MeV/c(2), M(D-s(+)) - M(D+) = 98.68 +/- 0.03 (stat) +/- 0.04 (syst) MeV/c(2) are measured using the D-0 -> K+K-pi(+)pi(-) and D-(s)(+) -> K+K-pi(+) modes.

Hadronic decays of charmed mesonsParticle physicsTeoria quàntica de campsGravitacióNuclear and High Energy PhysicsMesonHigh Energy Physics::LatticeNuclear TheoryFOS: Physical sciencesHadrons01 natural sciencesHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadrons; Leptonic semileptonic and radiative decays of bottom mesons; Charmed mesons (|C|>0 B=0); Hadronic decays of charmed mesonsPartícules (Física nuclear)Settore FIS/04 - Fisica Nucleare e SubnucleareLuminosityHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesD mesonLeptonic semileptonic and radiative decays of bottom meson[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]TOOLTeoria quàntica010306 general physicsHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronsNuclear ExperimentQCHadron-Hadron Scattering; Nuclear and High Energy PhysicsPhysicsHadron-Hadron Scattering010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronRelativity (Physics)DecayRelativitat (Física)Quantum field theoryFIS/01 - FISICA SPERIMENTALEQuantum theoryLeptonic semileptonic and radiative decays of bottom mesonsDECAY; TOOLFísica nuclearHigh Energy Physics::ExperimentCharmed mesons (|C|>0 B=0)DECAYParticle Physics - ExperimentGravitationJournal of High Energy Physics
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Relationship between the comma theory and Witten’s string field theory

1998

The comma representation of interacting string field theory is further elucidated. The proof that Witten's vertex solves the comma overlap equations is established. In this representation, the associativity of the star algebra is seen to hold. The relationship of the symmetry K in the standard formulation of Witten's string field theory to that in the comma theory is discussed.

Heterotic string theoryPhysicsNuclear and High Energy PhysicsCompactification (physics)S-dualityFísicaString field theoryTopological string theoryType I string theoryRelationship between string theory and quantum field theoryHigh Energy Physics::TheoryNon-critical string theoryMathematics::Category TheoryMathematical physicsPhysical Review D
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