Search results for "SCALAR"

showing 10 items of 1002 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
researchProduct

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
researchProduct

Karplus-Type Dependence of Vicinal119Sn-13C and119Sn-1H Spin-Spin Couplings in Organotin(IV) Derivatives: A DFT Study

2009

The empirical Karplus-type dependence of (3)J((119)Sn,(13)C) and (3)J((119)Sn,(1)H) couplings in organotin(IV) derivatives has been computationally validated by DFT methods both at the nonrelativistic and scalar ZORA relativistic level. A preliminary calibration of the computational protocols, by comparing experimental and calculated couplings for a Set Of Suitable rigid molecules, revealed their high predictive power: in particular, relativistic results for (3)J((119)Sn,(13)C) have a mean absolute error of just above 2 Hz, over a range of values up to about 70 Hz. The latter protocol has then been used to study in detail the influence of substituents and multiple paths connecting the coupl…

Coupling constantChemistryKarplus equationOrganic ChemistryCarbon-13Scalar (mathematics)Relativistic effectsNuclear magnetic resonance spectroscopyRelativistic effects DFT NMR spectroscopy tinMolecular physicsDensity functional calculations; NMR spectroscopy; Relativistic effects; TinDensity functional calculationsNMR spectroscopyNuclear magnetic resonanceTinMoleculePhysical and Theoretical ChemistryRelativistic quantum chemistryorganotinVicinalSpin-½European Journal of Organic Chemistry
researchProduct

Scaling behaviour of non-hyperbolic coupled map lattices

2006

Coupled map lattices of non-hyperbolic local maps arise naturally in many physical situations described by discretised reaction diffusion equations or discretised scalar field theories. As a prototype for these types of lattice dynamical systems we study diffusively coupled Tchebyscheff maps of N-th order which exhibit strongest possible chaotic behaviour for small coupling constants a. We prove that the expectations of arbitrary observables scale with \sqrt{a} in the low-coupling limit, contrasting the hyperbolic case which is known to scale with a. Moreover we prove that there are log-periodic oscillations of period \log N^2 modulating the \sqrt{a}-dependence of a given expectation value.…

Coupling constantDynamical systems theoryPhase spaceMathematical analysisReaction–diffusion systemFOS: Physical sciencesObservableExpectation valueChaotic Dynamics (nlin.CD)Nonlinear Sciences - Chaotic DynamicsScalar fieldScalingMathematics
researchProduct

Radiative muon capture and the value of gP in nuclei

1990

Abstract Radiative muon capture by nuclei is analyzed by means of sum rule techniques, providing a total photon yield calculated with RPA precision. The measured yields relative to the ordinary muon capture rate are well reproduced for the nuclei 12C, 16O and 40Ca using a value of the pseudoscalar weak coupling constant gP enhanced by only 25% with respect to its canonical value. Therefore, the large renormalization of gP claimed up to now must be reconsidered.

Coupling constantNuclear physicsRenormalizationPseudoscalarPhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryRadiative transferValue (computer science)Sum rule in quantum mechanicsPhoton yieldMuon capturePhysics Letters B
researchProduct

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
researchProduct

Dynamical formation and stability of fermion-boson stars

2020

Gravitationally bound structures composed by fermions and scalar particles known as fermion-boson stars are regular and static configurations obtained by solving the coupled Einstein-Klein-Gordon-Euler (EKGE) system. In this work, we discuss one possible scenario through which these fermion-boson stars may form by solving numerically the EKGE system under the simplifying assumption of spherical symmetry. Our initial configurations assume an already existing neutron star surrounded by an accreting cloud of a massive and complex scalar field. The results of our simulations show that once part of the initial scalar field is expelled via gravitational cooling the system gradually oscillates aro…

Coupling constantPhysicsCondensed Matter::Quantum Gases010308 nuclear & particles physicsScalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationTheoretical physicsNeutron starStars0103 physical sciencesCircular symmetry010306 general physicsScalar fieldAstrophysics::Galaxy AstrophysicsBoson
researchProduct

New constraints on axion-mediated P , T -violating interaction from electric dipole moments of diamagnetic atoms

2018

The exchange of an axionlike particle between atomic electrons and the nucleus may induce electric dipole moments (EDMs) of atoms and molecules. This interaction is described by a parity- and time-reversal-invariance-violating potential which depends on the product of a scalar ${g}^{s}$ and a pseudoscalar ${g}^{p}$ coupling constant. We consider the interaction with the specific combination of these constants, ${g}_{e}^{s}{g}_{N}^{p}$, which gives significant contributions to the EDMs of diamagnetic atoms. In this paper, we calculate these contributions to the EDMs of $^{199}\mathrm{Hg}$, $^{129}\mathrm{Xe}$, $^{211}\mathrm{Rn}$, and $^{225}\mathrm{Ra}$ for a wide range of axion masses. Com…

Coupling constantPhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAtoms in moleculesParity (physics)Electron01 natural sciencesPseudoscalarDipole0103 physical sciencesAtomPhysics::Atomic Physics010306 general physicsAxionPhysical Review D
researchProduct

Probing long-range leptonic forces with solar and reactor neutrinos

2006

In this work we study the phenomenological consequences of the existence of long-range forces coupled to lepton flavour numbers in solar neutrino oscillations. We study electronic forces mediated by scalar, vector or tensor neutral bosons and analyze their effect on the propagation of solar neutrinos as a function of the force strength and range. Under the assumption of one mass scale dominance, we perform a global analysis of solar and KamLAND neutrino data which depends on the two standard oscillation parameters, \Delta m^2_{21} and \tan^2\theta_{12}, the force coupling constant, its range and, for the case of scalar-mediated interactions, on the neutrino mass scale as well. We find that,…

Coupling constantPhysicsParticle physics010308 nuclear & particles physicsOscillationSolar neutrinoHigh Energy Physics::PhenomenologyScalar (mathematics)FOS: Physical sciencesAstronomy and Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentTensorNeutrino010306 general physicsLeptonBosonJournal of Cosmology and Astroparticle Physics
researchProduct

Global nuclear structure aspects of tensor interaction

2008

A direct fit of the isoscalar spin-orbit and both isoscalar and isovector tensor coupling constants to the f5/2-f7/2 SO splittings in 40Ca, 56Ni, and 48Ca requires: (i) a significant reduction of the standard isoscalar spin-orbit strength and (ii) strong attractive tensor coupling constants. The aim of this paper is to address the consequences of these strong attractive tensor and weak spin-orbit fields on total binding energies, two-neutron separation energies and nuclear deformability.

Coupling constantReductPhysicsNuclear and High Energy PhysicsIsovectorNuclear TheoryIsoscalarNuclear TheoryNuclear structureGeneral Physics and AstronomyFOS: Physical sciencesNuclear Theory (nucl-th)Quantum electrodynamicsTensorNuclear theory
researchProduct