Search results for "SCALAR"

showing 10 items of 1002 documents

Dips in the diffuse supernova neutrino background

2014

Scalar (fermion) dark matter with mass in the MeV range coupled to ordinary neutrinos and another fermion (scalar) is motivated by scenarios that establish a link between radiatively generated neutrino masses and the dark matter relic density. With such a coupling, cosmic supernova neutrinos, on their way to us, could resonantly interact with the background dark matter particles, giving rise to a dip in their redshift-integrated spectra. Current and future neutrino detectors, such as Super-Kamiokande, LENA and Hyper-Kamiokande, could be able to detect this distortion.

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaScalar (mathematics)Dark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and AstrophysicsFermionAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energySpectral lineSupernovaCoupling (physics)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorHigh Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Unravelling cosmic velocity flows: a Helmholtz-Hodge decomposition algorithm for cosmological simulations

2021

In the context of intra-cluster medium turbulence, it is essential to be able to split the turbulent velocity field in a compressive and a solenoidal component. We describe and implement a new method for this aim, i.e., performing a Helmholtz-Hodge decomposition, in multi-grid, multi-resolution descriptions, focusing on (but not being restricted to) the outputs of AMR cosmological simulations. The method is based on solving elliptic equations for a scalar and a vector potential, from which the compressive and the solenoidal velocity fields, respectively, are derived through differentiation. These equations are addressed using a combination of Fourier (for the base grid) and iterative (for t…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Solenoidal vector fieldField (physics)Adaptive mesh refinementMathematical analysisScalar (physics)General Physics and AstronomyFOS: Physical sciencesContext (language use)Astrophysics - Astrophysics of Galaxies01 natural sciences010305 fluids & plasmassymbols.namesakeHardware and ArchitectureHelmholtz free energyAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencessymbolsVector fieldAstrophysics - Instrumentation and Methods for Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics - Cosmology and Nongalactic AstrophysicsVector potential
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Attractive versus repulsive interactions in the Bose-Einstein condensation dynamics of relativistic field theories

2017

We study the impact of attractive self-interactions on the nonequilibrium dynamics of relativistic quantum fields with large occupancies at low momenta. Our primary focus is on Bose-Einstein condensation and nonthermal fixed points in such systems. As a model system we consider O(N)-symmetric scalar field theories. We use classical-statistical real-time simulations, as well as a systematic 1/N expansion of the quantum (2PI) effective action to next-to-leading order. When the mean self-interactions are repulsive, condensation occurs as a consequence of a universal inverse particle cascade to the zero-momentum mode with self-similar scaling behavior. For attractive mean self-interactions the …

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)axionsAnnihilationta114Field (physics)010308 nuclear & particles physicsFOS: Physical sciencesBose-Einstein condensatesCharge (physics)01 natural scienceslaw.inventionHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Q-balllawQuantum electrodynamics0103 physical sciences010306 general physicsScalar fieldQuantumEffective actionBose–Einstein condensateAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Spin-orbit and tensor mean-field effects on spin-orbit splitting including self-consistent core polarizations

2008

A new strategy of fitting the coupling constants of the nuclear energy density functional is proposed, which shifts attention from ground-state bulk to single-particle properties. The latter are analyzed in terms of the bare single-particle energies and mass, shape, and spin core-polarization effects. Fit of the isoscalar spin-orbit and both isoscalar and isovector tensor coupling constants directly to the f5/2-f7/2 spin-orbit splittings in 40Ca, 56Ni, and 48Ca is proposed as a practical realization of this new programme. It is shown that this fit requires drastic changes in the isoscalar spin-orbit strength and the tensor coupling constants as compared to the commonly accepted values but i…

PhysicsCoupling constantNuclear and High Energy PhysicsIsovectorNuclear TheoryBand gapIsoscalarBinding energyNuclear TheoryNuclear structureFOS: Physical sciencesPolarization (waves)Nuclear Theory (nucl-th)Mean field theoryAtomic physics
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Spurious finite-size instabilities in nuclear energy density functionals: Spin channel

2015

Background: It has been recently shown that some Skyrme functionals can lead to nonconverging results in the calculation of some properties of atomic nuclei. A previous study has pointed out a possible link between these convergence problems and the appearance of finite-size instabilities in symmetric nuclear matter (SNM) around saturation density. Purpose: We show that the finite-size instabilities not only affect the ground-state properties of atomic nuclei, but they can also influence the calculations of vibrational excited states in finite nuclei. Method: We perform systematic fully-self consistent random phase approximation (RPA) calculations in spherical doubly magic nuclei. We employ…

PhysicsCoupling constantNuclear and High Energy Physics[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear TheoryIsovector010308 nuclear & particles physicsIsoscalarNuclear TheoryFOS: Physical sciencesFísicaNuclear matter01 natural sciencesNuclear Theory (nucl-th)Nuclear physicsMean-fieldMean field theoryQuantum mechanics0103 physical sciencesAtomic nucleusNuclear force010306 general physicsRandom phase approximation
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Yukawa Alignment in the Two-Higgs-Doublet Model

2009

5 páginas, 1 tabla.-- PACS numbers: 12.60.Fr, 11.30.Hv, 12.15.Mm, 14.80.Cp

PhysicsCouplingNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::LatticeScalar (mathematics)High Energy Physics::PhenomenologyYukawa potentialFOS: Physical sciencesFísicaTwo-Higgs-doublet modelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Homogeneous spaceCP violationHigh Energy Physics::Experiment
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Bounds on Neutrino-Scalar Yukawa Coupling

2015

General neutrino-scalar couplings appear in many extensions of Standard Model. We can probe these neutrino-scalar couplings by leptonic decay of mesons and from heavy neutrino search. Our analysis improves the present limits to $|g_e|^2<1.9\times 10^{-6}$ and $|g_\mu|^2<1.9\times 10^{-7}$ at 90\% C.L. for massless scalars. For massive scalars we found for the first time the constraints for $g^2_{\alpha}$ couplings to be $10^{-6}-10^{-1}$ respectively for scalar masses between below 1 MeV and for 300 MeV.

PhysicsCouplingParticle physicsMeson010308 nuclear & particles physicsPhysics beyond the Standard ModelScalar (mathematics)High Energy Physics::PhenomenologyYukawa potentialFOS: Physical sciences01 natural sciencesMassless particleGeneral Relativity and Quantum CosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentNeutrinoHeavy neutrino010306 general physicsNuclear Experiment
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An extension of two-Higgs-doublet model and the excesses of 750 GeV diphoton, muon g-2 and h → μτ

2016

In this paper we simultaneously explain the excesses of the 750 GeV diphoton, muon g-2 and $h\to \mu\tau$ in an extension of the two-Higgs-doublet model (2HDM) with additional vector-like fermions and a CP-odd scalar singlet ($P$) which is identified as the 750 GeV resonance. This 750 GeV resonance has a mixing with the CP-odd scalar ($A$) in 2HDM, which leads to a coupling between $P$ and the SM particles as well as a coupling between $A$ and the vector-like fermions. Such a mixing and couplings are strongly constrained by $\tau\to\mu\gamma$, muon g-2 and the 750 GeV diphoton data. We scan over the parameter space and find that such an extension can simultaneously account for the observed …

PhysicsCouplingParticle physicsNuclear and High Energy PhysicsMuon010308 nuclear & particles physicsScalar (mathematics)FermionParameter space01 natural sciencesNuclear physicsHigh Energy Physics - PhenomenologyTwo-Higgs-doublet model0103 physical sciencesHigh Energy Physics::ExperimentSinglet state010306 general physicsNuclear ExperimentPhysics Letters B
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Isospin Character of Low-Lying Pygmy Dipole States inPb208via Inelastic Scattering ofO17Ions

2014

The properties of pygmy dipole states in Pb-208 were investigated using the Pb-208(O-17, O-17'gamma) reaction at 340 MeV and measuring the gamma decay with high resolution with the AGATA demonstrator array. Cross sections and angular distributions of the emitted gamma rays and of the scattered particles were measured. The results are compared with (gamma, gamma') and (p, p') data. The data analysis with the distorted wave Born approximation approach gives a good description of the elastic scattering and of the inelastic excitation of the 2(+) and 3(-) states. For the dipole transitions a form factor obtained by folding a microscopically calculated transition density was used for the first t…

PhysicsElastic scatteringDipoleAstrophysics::High Energy Astrophysical PhenomenaIsospinIsoscalarGamma rayGeneral Physics and AstronomyAGATABorn approximationAtomic physicsInelastic scattering7. Clean energyPhysical Review Letters
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ONE-LOOP INTEGRALS REVISITED — THE THREE-POINT FUNCTIONS

1993

This paper presents results concerning a new calculation of the well-known one-loop n- point scalar and tensor functions. In this paper we treat the three-point functions. We give a systematic reduction to a certain class of functions which minimizes the effort for calculating scalar and tensor integrals drastically. We avoid standard techniques such as Feynman parametrization and Wick rotation.

PhysicsFeynman parametrizationNuclear and High Energy PhysicsWick rotationScalar (mathematics)Applied mathematicsAstronomy and AstrophysicsAtomic and Molecular Physics and OpticsInternational Journal of Modern Physics A
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