Search results for "Field Theory"

showing 10 items of 1188 documents

Primordial dark matter from curvature induced symmetry breaking

2020

We demonstrate that adiabatic dark matter can be generated by gravity induced symmetry breaking during inflation. We study a $Z_2$ symmetric scalar singlet that couples to other fields only through gravity and for which the symmetry is broken by the spacetime curvature during inflation when the non-minimal coupling $\xi$ is negative. We find that the symmetry breaking leads to the formation of adiabatic dark matter with the observed abundance for the singlet mass $m\sim{\rm MeV}$ and $|\xi|\sim 1$.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterScalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCurvature01 natural sciences114 Physical sciencessymmetry breakingGeneral Relativity and Quantum Cosmologypimeä aineGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesprimordial dark matterSymmetry breakinginflationAdiabatic processMathematical physicsPhysicsInflation (cosmology)symmetriadark matter theory010308 nuclear & particles physicsAstronomy and AstrophysicsCoupling (probability)Symmetry (physics)quantum field theory on curved spaceHigh Energy Physics - PhenomenologyAstrophysics - Cosmology and Nongalactic Astrophysics
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Do metric fluctuations affect the Higgs dynamics during inflation?

2017

We show that the dynamics of the Higgs field during inflation is not affected by metric fluctuations if the Higgs is an energetically subdominant light spectator. For Standard Model parameters we find that couplings between Higgs and metric fluctuations are suppressed by $\mathcal{O}(10^{-7})$. They are negligible compared to both pure Higgs terms in the effective potential and the unavoidable non-minimal Higgs coupling to background scalar curvature. The question of the electroweak vacuum instability during high energy scale inflation can therefore be studied consistently using the Jordan frame action in a Friedmann--Lema\^itre--Robertson--Walker metric, where the Higgs-curvature coupling …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcSTANDARD MODELFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGeneral Relativity and Quantum Cosmology0202 Atomic Molecular Nuclear Particle And Plasma PhysicsHigh Energy Physics - Phenomenology (hep-ph)EINSTEIN FRAMESELECTROWEAK VACUUMFIELDquantumfield theory on curved spaceScience & TechnologyPhysicsHigh Energy Physics::Phenomenologyhep-phNuclear & Particles PhysicsJORDANHigh Energy Physics - Phenomenology0201 Astronomical And Space SciencesMETASTABILITYparticle physics - cosmology connectionPhysical Sciencesastro-ph.COHigh Energy Physics::ExperimentEQUIVALENCEAstrophysics - Cosmology and Nongalactic Astrophysics
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Despicable dark relics: generated by gravity with unconstrained masses

2019

We demonstrate the existence of a generic, efficient and purely gravitational channel producing a significant abundance of dark relics during reheating after the end of inflation. The mechanism is present for any inert scalar with the non-minimal curvature coupling $\xi R\chi^2$ and the relic production is efficient for natural values $\xi = {\cal O}(1)$. The observed dark matter abundance can be reached for a broad range of relic masses extending from $m \sim 1 {\rm k eV}$ to $m \sim 10^{8} {\rm GeV}$, depending on the scale of inflation and the dark sector couplings. Frustratingly, such relics escape direct, indirect and collider searches since no non-gravitational couplings to visible ma…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)inationScalar (mathematics)Dark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCurvature01 natural sciencesGeneral Relativity and Quantum Cosmologylaw.inventionpimeä aineGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)law0103 physical sciencesinflationColliderkosminen inflaatioPhysicsInflation (cosmology)Couplingdark matter theory010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsSCALAR-FIELD115 Astronomy Space science16. Peace & justicequantum field theory on curved spaceHigh Energy Physics - PhenomenologyProduction (computer science)kvanttikenttäteoriaMATTERAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Electromagnetic mass difference of pions at low temperature

1999

We compute low temperature corrections to the electromagnetic mass difference of pions in the chiral limit. The computation is done in a model independent way in the framework of chiral perturbation theory, using the background field method and the hard thermal loop approximation. We also generalize at low temperature the sum rule of Das et al. We find that the mass difference between the charged and neutral pions decreases at low temperature $T$ with respect to the T=0 value. This is so in spite of the fact that charged particles always get a thermal correction to their masses of order $\sim eT$, where $e$ is the gauge coupling constant. Our result can be understood as a consequence of the…

Coupling constantChiral anomalyPhysicsNuclear and High Energy PhysicsChiral perturbation theoryNuclear TheoryThermal quantum field theoryHigh Energy Physics::LatticeFOS: Physical sciencesFísicaNuclear Theory (nucl-th)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)PionQuantum mechanicsQuantum electrodynamicsSum rule in quantum mechanicsElectromagnetic massChiral symmetry breaking
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Contribution of the $a_1$ meson to the axial nucleon-to-$\Delta$ transition form factors

2018

We analyze the low-$Q^2$ behavior of the axial form factor $G_A(Q^2)$, the induced pseudoscalar form factor $G_P(Q^2)$, and the axial nucleon-to-$\Delta$ transition form factors $C^A_5(Q^2)$ and $C^A_6(Q^2)$. Building on the results of chiral perturbation theory, we first discuss $G_A(Q^2)$ in a chiral effective-Lagrangian model including the $a_1$ meson and determine the relevant coupling parameters from a fit to experimental data. With this information, the form factor $G_P(Q^2)$ can be predicted. For the determination of the transition form factor $C^A_5(Q^2)$ we make use of an SU(6) spin-flavor quark-model relation to fix two coupling constants such that only one free parameter is left.…

Coupling constantPhysicsChiral perturbation theoryMesonNuclear Theory010308 nuclear & particles physicsHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyForm factor (quantum field theory)Coupling (probability)01 natural sciencesHigh Energy Physics - ExperimentPseudoscalarHigh Energy Physics - Phenomenology0103 physical sciencesSU(6)010306 general physicsNucleonNuclear ExperimentMathematical physics
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Path integral quantization for massive vector bosons

2010

A parity-conserving and Lorentz-invariant effective field theory of self-interacting massive vector fields is considered. For the interaction terms with dimensionless coupling constants the canonical quantization is performed. It is shown that the self-consistency condition of this system with the second-class constraints in combination with the perturbative renormalizability leads to an SU(2) Yang-Mills theory with an additional mass term.

Coupling constantPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsCanonical quantizationFOS: Physical sciencesAstronomy and AstrophysicsYang–Mills existence and mass gapAtomic and Molecular Physics and OpticsRenormalizationQuantization (physics)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Path integral formulationEffective field theoryVector fieldMathematical physics
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A finite size scaling study of the five-dimensional Ising model

1994

For systems above the marginal dimension d*, where mean field theory starts to become valid, such as Ising models in d = 5 for which d* = 4, hyperscaling is invalid and hence it was suggested that finite size scaling is not ruled by the correlation length ξ (∝ |t| −1/2 in Landau theory, t being the distance from the critical point) but by a “thermodynamic length” l (∝ |t| −2/d). Early simulation work by Binder et al. using nearest neighbor hypercubic L5 lattices with L ⩽ 7 yielded some evidence for this prediction, but the renormalized coupling constant gL = −3 + 〈M4〉/〈M2〉2 at Tc was gL ≈ −1.0 instead of the prediction of Brezin and Zinn-Justin, gL(Tc) = −3 + Γ4(1/4)/(8 π2) ≈ −0.812. In the…

Coupling constantPhysicsMean field theoryCondensed matter physicsCritical point (thermodynamics)General Physics and AstronomyIsing modelCoupling (probability)ScalingLandau theoryk-nearest neighbors algorithmAnnalen der Physik
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Effective-field-theory predictions of the muon-deuteron capture rate

2018

We quantify the theoretical uncertainties of chiral effective-field-theory predictions of the muon-deuteron capture rate. Theoretical error estimates of this low-energy process is important for a reliable interpretation of forthcoming experimental results by the MuSun collaboration. Specifically, we estimate the three dominant sources of uncertainties that impact theoretical calculations of this rate: those resulting from uncertainties in the pool of fit data used to constrain the coupling constants in the nuclear interaction, those due to the truncation of the effective field theory, and those due to uncertainties in the axial radius of the nucleon. For the capture rate into the ${}^1S_0$ …

Coupling constantPhysicsMuonNuclear Theory010308 nuclear & particles physicsFOS: Physical sciencesRadius01 natural sciencesComputational physicsInterpretation (model theory)Nuclear Theory (nucl-th)0103 physical sciencesEffective field theoryTruncation (statistics)Nuclear Experiment (nucl-ex)010306 general physicsNucleonNuclear ExperimentCommunication channel
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Muon capture revisited

1990

Abstract The problem of inclusive muon capture in nuclei is studied by calculating the capture rate in asymmetric infinite nuclear matter and using the local density approximation to evaluate the capture rates in nuclei. It is shown that the method is rather reliable and allows one to improve on approximations used in the past. The need for a strong nuclear renormalization is shown, reducing the capture rates by about a factor two in medium and heavy nuclei. By using standard effective interactions in the spin-isospin channel one can account for this renormalization and one finds a remarkable overall agreement with the measured capture rates for a large list of nuclei through the periodic t…

Coupling constantPhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryForm factor (quantum field theory)Nuclear matterMuon captureNuclear physicsRenormalizationBibliographyLocal-density approximationNuclear ExperimentCommunication channelNuclear Physics A
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Proposal for a running coupling JIMWLK equation

2014

In the CGC framework the initial stages of a heavy ion collision at high energy are described as "glasma" field configurations. The initial condition for these evolving fields depends, in the CGC effective theory, on a probability distribution for color charges. The energy dependence of this distribution can be calculated from the JIMWLK renormalization group equation. We discuss recent work on a practical implementation of the running coupling constant in the Langevin method of solving the JIMWLK equation.

Coupling constantPhysicsNuclear and High Energy Physicsta114Field (physics)010308 nuclear & particles physicsFOS: Physical sciencesRenormalization group01 natural sciencesLangevin equationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamics0103 physical sciencesEffective field theoryInitial value problemProbability distributionBoundary value problem010306 general physicsNuclear Physics A
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