Search results for "Axion"

showing 10 items of 121 documents

D6-brane model building onZ2×Z6: MSSM-like and left–right symmetric models

2015

Abstract We perform a systematic search for globally defined MSSM-like and left–right symmetric models on D6-branes on the T 6 / ( Z 2 × Z 6 × Ω R ) orientifold with discrete torsion. Our search is exhaustive for models that are independent of the value of the one free complex structure modulus. Preliminary investigations suggest that there exists one prototype of visible sector for MSSM-like and another for left–right symmetric models with differences arising from various hidden sector completions to global models. For each prototype, we provide the full matter spectrum, as well as the Yukawa and other three-point couplings needed to render vector-like matter states massive. This provides …

Hidden sectorQuarkPhysicsNuclear and High Energy PhysicsTheoretical physicsParticle physicsOrientifoldHigh Energy Physics::PhenomenologyYukawa potentialBraneAxionLeptonMinimal Supersymmetric Standard ModelNuclear Physics B
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Robustness of cosmological axion mass limits

2015

We present cosmological bounds on the thermal axion mass in an extended cosmological scenario in which the primordial power spectrum of scalar perturbations differs from the usual power-law shape predicted by the simplest inflationary models. The power spectrum is instead modeled by means of a "piecewise cubic Hermite interpolating polynomial" (PCHIP). When using Cosmic Microwave Background measurements combined with other cosmological data sets, the thermal axion mass constraints are degraded only slightly. The addition of the measurements of $\sigma_8$ and $\Omega_m$ from the 2013 Planck cluster catalogue on galaxy number counts relaxes the bounds on the thermal axion mass, mildly favouri…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCosmic microwave backgroundScalar (mathematics)Cosmic background radiationFOS: Physical sciencesFísicaSpectral densityAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologysymbols.namesake13. Climate action0103 physical sciencessymbolsPlanckNeutrino010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaAxionAstrophysics - Cosmology and Nongalactic Astrophysics
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Electronic structure of the ytterbium monohydroxide molecule to search for axionlike particles

2021

Recently, the YbOH molecule has been suggested as a candidate to search for the electron electric dipole moment (eEDM), which violates spatial parity ($P$) and time-reversal ($T$) symmetries [I. Kozyryev and N. R. Hutzler, Phys. Rev. Lett. 119, 133002 (2017)]. In the present paper, we show that the same system can be used to measure coupling constants of the interaction of electrons and nucleus mediated by axionlike particles. The electron-nucleus interaction produced by the axion exchange can contribute to a $T,P$-violating EDM of the whole molecular system. We express the corresponding $T,P$-violating energy shift produced by this effect in terms of the axion mass and product of the axion…

High Energy Physics - TheoryChemical Physics (physics.chem-ph)PhysicsCoupling constantYtterbiumAtomic Physics (physics.atom-ph)High Energy Physics::PhenomenologyFOS: Physical scienceschemistry.chemical_elementParity (physics)ElectronElectronic structure01 natural sciencesElectron electric dipole momentPhysics - Atomic Physics010305 fluids & plasmasHigh Energy Physics - Theory (hep-th)chemistryPhysics - Chemical Physics0103 physical sciencesMoleculeAtomic physics010306 general physicsAxion
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A model for the very early universe

2008

A model with N species of massless fermions interacting via (microscopic) gravitational torsion in de Sitter spacetime is investigated in the limit N->infinity. The U_V(N)*U_A(N) flavor symmetry is broken dynamically irrespective of the (positive) value of the induced four-fermion coupling. This model is equivalent to a theory with free but massive fermions fluctuating about the chiral condensate. When the fermions are integrated out in a way demonstrated long ago by Candelas and Raine, the associated gap equation together with the Friedmann equation predict that the Hubble parameter vanishes. Introducing a matter sector (subject to a finite gauge symmetry) as a source for subsequent cos…

High Energy Physics - TheoryChiral anomalyPhysicsNuclear and High Energy PhysicsHigh Energy Physics::LatticeFriedmann equationsHigh Energy Physics::PhenomenologyFOS: Physical sciencesFermionMassless particleHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum Cosmologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)De Sitter universesymbolsAxionGauge symmetryHubble's lawMathematical physicsJournal of High Energy Physics
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Merger of dark matter axion clumps and resonant photon emission

2020

A portion of light scalar dark matter, especially axions, may organize into gravitationally bound clumps (stars) and be present in large number in the galaxy today. It is therefore of utmost interest to determine if there are novel observational signatures of this scenario. Work has shown that for moderately large axion-photon couplings, such clumps can undergo parametric resonance into photons, for clumps above a critical mass $M^{\star}_c$ determined precisely by some of us in Ref. [1]. In order to obtain a clump above the critical mass in the galaxy today would require mergers. In this work we perform full 3-dimensional simulations of pairs of axion clumps and determine the conditions un…

High Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)astrofysiikkaMilky WayDark matterScalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicskosmologia01 natural sciencesCritical mass (software engineering)General Relativity and Quantum Cosmologyalkeishiukkasetpimeä aineHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesAxionAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsfotonit010308 nuclear & particles physicsAstronomy and AstrophysicsGalaxyHigh Energy Physics - PhenomenologyStarsHigh Energy Physics - Theory (hep-th)Astrophysics - High Energy Astrophysical PhenomenaScalar fieldAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Axionic and nonaxionic electrodynamics in plane and circular geometry

2023

Various aspects of axion electrodynamics in the presence of a homogeneous and isotropic dielectric medium are discussed. 1. We consider first the "antenna-like" property of a planar dielectric surface in axion electrodynamics, elaborating on the treatment given earlier on this topic by Millar {\it et al.} (2017). We calculate the electromagnetic energy transmission coefficient for a dielectric plate, and compare with the conventional expression in ordinary electrodynamics. 2. We consider the situation where the medium exterior to the plate, assumed elastic, is "bent back" and glued together, so that we obtain a circular dielectric string in which the waves can propagate clockwise or counter…

High Energy Physics - TheoryCp conservationSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciHigh Energy Physics - Theory (hep-th)Casimir energyFOS: Physical sciencesAxion Axion Electrodynamics Dark Matter Relativistic aspects of CosmologySettore FIS/04 - Fisica Nucleare E Subnucleare114 Physical sciencesSettore FIS/03 - Fisica Della Materia
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Implications for dark matter direct detection in the presence of LIGO-motivated primordial black holes

2019

We discuss formation of dark matter (DM) mini-halos around primordial black holes (PBHs) and its implication on DM direct detection experiments, including axion searches. Motivated by LIGO observations, we consider $f_{\textrm{DM}} \simeq 0.01$ as the fraction of DM in PBHs with masses $10 M_{\odot} - 70 M_{\odot}$. In this case, we expect the presence of dressed PBHs after Milky Way halo formation with mini-halo masses peaked around $M_{\textrm{halo}} \sim (50-55) M_{\textrm{PBH}}$. We analyze the effect of tidal forces acting on dressed PBHs within the Milky Way galaxy. In the solar neighborhood, the mini-halos are resistant against tidal disruption from the mean-field potential of the ga…

High Energy Physics - TheoryDISRUPTIONHALO MODELSPrimordial black holeAstrophysicsDark mini-halosdark matter direct detectionkosmologia01 natural sciencesGeneral Relativity and Quantum CosmologyLIMITSHigh Energy Physics - Phenomenology (hep-ph)BulgePhysicsprimordial black holeslcsh:QC1-999High Energy Physics - PhenomenologyBULGEMILKY-WAYLIGO-Virgo collaborationHaloAstrophysics - Cosmology and Nongalactic Astrophysicsaxion dark matterNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Axion dark matterMilky WayDark mattermustat aukotFOS: Physical sciencesPrimordial black holesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsDark matter direct detection114 Physical sciencespimeä ainedark mini-halos0103 physical sciences010306 general physicsAxionCP CONSERVATIONAstrophysics::Galaxy Astrophysics010308 nuclear & particles physicsCONSTRAINTSAstrophysics - Astrophysics of GalaxiesLIGOGalaxyHigh Energy Physics - Theory (hep-th)Astrophysics of Galaxies (astro-ph.GA)lcsh:Physics
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Discrete Abelian gauge symmetries and axions

2015

We combine two popular extensions of beyond the Standard Model physics within the framework of intersecting D6-brane models: discrete Zn symmetries and Peccei-Quinn axions. The underlying natural connection between both extensions is formed by the presence of massive U(1) gauge symmetries in D-brane model building. Global intersecting D6-brane models on toroidal orbifolds of the type T6/Z2N and T6/Z2xZ2M with discrete torsion offer excellent playgrounds for realizing these extensions. A generation-dependent Z2 symmetry is identified in a global Pati-Salam model, while global left-right symmetric models give rise to supersymmetric realizations of the DFSZ axion model. In one class of the lat…

High Energy Physics - TheoryHistoryPhysics beyond the Standard ModelFOS: Physical sciencesD-brane01 natural sciencesEducationTheoretical physicsHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)Non-trivialGauge symmetries0103 physical sciencesAbelian group010306 general physicsAxionPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaCharge (physics)Gauge (firearms)16. Peace & justiceSymmetry (physics)Computer Science ApplicationsStandard Model (mathematical formulation)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Homogeneous spaceStandard model
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Reloading the Axion in a 3-3-1 setup

2020

We generalize the idea of the axion to an extended electroweak gauge symmetry setup. We propose a minimal axion extension of the Singer-Valle-Schechter (SVS) theory, in which the standard model fits in $\mathrm{SU(3)_L\otimes U(1)_X}$, the number of families results from anomaly cancellation, and the Peccei-Quinn (PQ) solution to the strong-CP problem is implemented. Neutrino masses arise from a type-I Dirac seesaw mechanism, suppressed by the ratio of SVS and PQ scales, suggesting the existence of new physics at a moderate SVS scale. Novel features include an enhanced axion coupling to photons when compared to the DFSZ axion, as well as flavour-changing axion couplings to quarks.

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelFOS: Physical sciencesStandard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics::TheoryAxionHigh Energy Physics - Phenomenology (hep-ph)Peccei-Quinn symmetryNeutrinosAxionGauge symmetryPhysicsElectroweak interactionHigh Energy Physics::Phenomenologylcsh:QC1-999High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Theory (hep-th)Anomaly (physics)Neutrinolcsh:Physics
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No chiral light bending by clumps of axion-like particles

2019

We study the propagation of light in the presence of a parity-violating coupling between photons and axion-like particles (ALPs). Naively, this interaction could lead to a split of light rays into two separate beams of different polarization chirality and with different refraction angles. However, by using the eikonal method we explicitly show that this is not the case and that ALP clumps do not produce any spatial birefringence. This happens due to non-trivial variations of the photon's frequency and wavevector, which absorb time-derivatives and gradients of the ALP field. We argue that these variations represent a new way to probe the ALP-photon couping with precision frequency measuremen…

High Energy Physics - TheoryPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)BirefringencePhoton010308 nuclear & particles physicsEikonal equationFOS: Physical sciencesPhysics::OpticsAstronomy and AstrophysicsPolarization (waves)01 natural sciencesMolecular physicsRayPhysics::GeophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Space and Planetary Science0103 physical sciencesWave vectorChirality (chemistry)010303 astronomy & astrophysicsAxionAstrophysics - Cosmology and Nongalactic Astrophysics
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