Search results for "STANDARD MODEL"

showing 10 items of 1206 documents

Unifying leptogenesis, dark matter and high-energy neutrinos with right-handed neutrino mixing via Higgs portal

2016

We revisit a model in which neutrino masses and mixing are described by a two right-handed (RH) neutrino seesaw scenario, implying a strictly hierarchical light neutrino spectrum. A third decoupled RH neutrino, $N_{\rm DM}$ with mass $M_{\rm DM}$, plays the role of cold dark matter (DM) and is produced by the mixing with a source RH neutrino, $N_{\rm S}$ with mass $M_{\rm S}$, induced by Higgs portal interactions. The same interactions are also responsible for $N_{\rm DM}$ decays. We discuss in detail the constraints coming from DM abundance and stability conditions, showing that in the hierarchical case ($M_{\rm DM} \gg M_{\rm S}$) there is an allowed window on $M_{\rm DM}$, which necessar…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsCold dark matter010308 nuclear & particles physicsPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAstronomy and Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetryNeutrino detector13. Climate actionLeptogenesis0103 physical sciencesInvariant massHigh Energy Physics::ExperimentNeutrino010306 general physicsAstrophysics - High Energy Astrophysical Phenomena
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Updated collider and direct detection constraints on Dark Matter models for the Galactic Center gamma-ray excess

2016

Utilizing an exhaustive set of simplified models, we revisit dark matter scenarios potentially capable of generating the observed Galactic Center gamma-ray excess, updating constraints from the LUX and PandaX-II experiments, as well as from the LHC and other colliders. We identify a variety of pseudoscalar mediated models that remain consistent with all constraints. In contrast, dark matter candidates which annihilate through a spin-1 mediator are ruled out by direct detection constraints unless the mass of the mediator is near an annihilation resonance, or the mediator has a purely vector coupling to the dark matter and a purely axial coupling to Standard Model fermions. All scenarios in w…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Large Hadron ColliderAnnihilation010308 nuclear & particles physicsPhysics beyond the Standard ModelDark matterGalactic CenterFOS: Physical sciencesAstronomy and AstrophysicsFermion01 natural sciencesStandard ModelPseudoscalarHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesAstrophysics - High Energy Astrophysical Phenomena010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Hidden sector dark matter and the Galactic Center gamma-ray excess: a closer look

2017

Stringent constraints from direct detection experiments and the Large Hadron Collider motivate us to consider models in which the dark matter does not directly couple to the Standard Model, but that instead annihilates into hidden sector particles which ultimately decay through small couplings to the Standard Model. We calculate the gamma-ray emission generated within the context of several such hidden sector models, including those in which the hidden sector couples to the Standard Model through the vector portal (kinetic mixing with Standard Model hypercharge), through the Higgs portal (mixing with the Standard Model Higgs boson), or both. In each case, we identify broad regions of parame…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsHyperchargeCosmology and Nongalactic Astrophysics (astro-ph.CO)Large Hadron Collider010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyDark matterFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)01 natural sciencesStandard ModelHidden sectorHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Antiproton0103 physical sciencesHiggs bosonAstrophysics - High Energy Astrophysical Phenomena010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Looking at the axionic dark sector with ANITA

2020

The ANITA experiment has recently observed two anomalous events emerging from well below the horizon. Even though they are consistent with tau cascades, a high energy Standard Model or Beyond the Standard Model explanation is challenging and in tension with other experiments. We study under which conditions the reflection of generic radio pulses can reproduce these signals. We propose that these pulses can be resonantly produced in the ionosphere via axion-photon conversion. This naturally explains the direction and polarization of the events and avoids other experimental bounds.

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsPhysics beyond the Standard ModelFOS: Physical scienceslcsh:AstrophysicsPolarization (waves)01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamicslcsh:QB460-4660103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityIonosphereAstrophysics - High Energy Astrophysical Phenomena010306 general physicsEngineering (miscellaneous)Astronomia ObservacionsThe European Physical Journal C
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Heavy sterile neutrinos in stellar core-collapse

2018

We perform spherically symmetric simulations of the core collapse of a single progenitor star of zero age main sequence mass $M_{\rm ZAMS} = 15 \, M_{\odot}$ with two models of heavy sterile neutrinos in the mass range of hundred MeV$/c^2$. According to both models, these hypothetical particles are copiously produced in the center, stream outwards a subsequently decay releasing energy into final states (including neutrinos) of the Standard Model. We find that they can lead to a successful explosion in otherwise non-exploding progenitors. Depending on their unknown parameters (e.g., mass and coupling constants with matter), we obtain either no explosion or an explosion of one of two types, i…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSterile neutrino010308 nuclear & particles physicsStar (game theory)Astrophysics::High Energy Astrophysical PhenomenaCenter (category theory)FOS: Physical sciencesAstrophysicsType (model theory)01 natural sciences7. Clean energyStandard ModelSupernovaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics - Solar and Stellar Astrophysics0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsNeutrinoAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Energy (signal processing)Astrophysics::Galaxy Astrophysics
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On unification and nucleon decay in supersymmetric grand unified theories based on SU(5)

2006

9 pages, 4 figures.-- ISI Article Identifier: 000247170700016.-- ArXiv pre-print available at: http://arxiv.org/abs/hep-ph/0610034

High Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaHigh Energy Physics::ExperimentSupergravity Unification (SU)GUT; Beyond Standard Model; Nucleon decay.Proton-decayFlipped SU(5)High Energy Physics - Experiment
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Scalar contributions to b→c(u)τν transitions

2017

Abstract We perform a comprehensive analysis of scalar contributions in b → c τ ν transitions including the latest measurements of R ( D ( ⁎ ) ) , the q 2 differential distributions in B → D ( ⁎ ) τ ν , the τ polarization asymmetry for B → D ⁎ τ ν , and the bound derived from the total width of the B c meson. We find that scalar contributions with the simultaneous presence of both left- and right-handed couplings to quarks can explain the available data, specifically R ( D ( ⁎ ) ) together with the measured differential distributions. However, the constraints from the total B c width present a slight tension with the current data on B → D ⁎ τ ν in this scenario, preferring smaller values fo…

High Energy Physics - Phenomenology; High Energy Physics - Phenomenology; High Energy Physics - Experiment; Nuclear and High Energy PhysicsQuarkPhysicsNuclear and High Energy PhysicsParticle physicsMeson010308 nuclear & particles physicsPhysics beyond the Standard Modelmedia_common.quotation_subjectObservablePolarization (waves)01 natural sciences7. Clean energyAsymmetrylcsh:QC1-999High Energy Physics - ExperimentBaryonHigh Energy Physics - Phenomenology0103 physical sciencesCurrent vector010306 general physicslcsh:Physicsmedia_commonPhysics Letters B
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QCD and Strongly Coupled Gauge Theories: Challenges and Perspectives

2014

We dedicate this document to the memory of Mikhail Polikarpov, who passed away in July 2013. Misha worked with us for decades as a convener of the “Confinement” section of the Quark Confinement and Hadron Spectrum Series. He guided and expanded the scientific discussion of that topic, inspiring and under taking new research avenues. From its initial conception, he supported the enterprise of this document and organized Sect. 8, writing the part on confinement himself. He attracted the XIth Conference on Quark Confinement and the Hadron Spectrum to St. Petersburg (September 8-12, 2014; see http://phys.spbu.ru/confxi.html). His warm and kind personality, his high sense of humor, his ideas in …

High Energy Physics - TheoryEFFECTIVE-FIELD-THEORYNuclear TheoryPhysics and Astronomy (miscellaneous)Physics beyond the Standard ModelReviewHEAVY-ION COLLISIONSnucl-ex7. Clean energyCosmologyHigh Energy Physics - ExperimentQUARK-GLUON PLASMADEEP-INELASTIC SCATTERINGHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Gauge theoryNuclear Experiment (nucl-ex)Nuclear ExperimentQuantum chromodynamicsPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thHigh Energy Physics - Lattice (hep-lat)hep-phddc:High Energy Physics - PhenomenologyYANG-MILLS THEORYastro-ph.COAstrophysics - Cosmology and Nongalactic AstrophysicsPB-PB COLLISIONSParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)nucl-th[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]530 PhysicsStrong interactionComplex systemFOS: Physical scienceshep-lat[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]CHIRAL PERTURBATION-THEORY114 Physical sciencesELECTRIC-DIPOLE MOMENTNuclear Theory (nucl-th)Theoretical physicsHigh Energy Physics - Latticeddc:530Engineering (miscellaneous)Particle Physics - Phenomenologyhep-ex[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat]NUCLEUS-NUCLEUS COLLISIONSPerspective (graphical)FísicaRADIATIVE ENERGY-LOSSFlow (mathematics)High Energy Physics - Theory (hep-th)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]European Physical Journal C
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Ricci-Based Gravity theories and their impact on Maxwell and nonlinear electromagnetic models

2019

Abstract We extend the correspondence between metric-affine Ricci-Based Gravity the- ories and General Relativity (GR) to the case in which the matter sector is represented by linear and nonlinear electromagnetic fields. This complements previous studies focused on fluids and scalar fields. We establish the general algorithm that relates the matter fields in the GR and RBG frames and consider some applications. In particular, we find that the so-called Eddington-inspired Born-Infeld gravity theory coupled to Maxwell electromag- netism is in direct correspondence with GR coupled to Born-Infeld electromagnetism. We comment on the potential phenomenological implications of this relation.

High Energy Physics - TheoryElectromagnetic fieldPhysicsNuclear and High Energy PhysicsGravity (chemistry)010308 nuclear & particles physicsGeneral relativityScalar (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyNonlinear systemTheoretical physicsHigh Energy Physics - Theory (hep-th)Electromagnetism0103 physical sciencesBeyond Standard Modellcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityElectromagnetic model010306 general physicsClassical Theories of GravityGeneral algorithmJournal of High Energy Physics
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Einstein, Planck and Vera Rubin: Relevant Encounters Between the Cosmological and the Quantum Worlds

2021

In Cosmology and in Fundamental Physics there is a crucial question like: where the elusive substance that we call Dark Matter is hidden in the Universe and what is it made of? that, even after 40 years from the Vera Rubin seminal discovery [1] does not have a proper answer. Actually, the more we have investigated, the more this issue has become strongly entangled with aspects that go beyond the established Quantum Physics, the Standard Model of Elementary particles and the General Relativity and related to processes like the Inflation, the accelerated expansion of the Universe and High Energy Phenomena around compact objects. Even Quantum Gravity and very exotic Dark Matter particle candid…

High Energy Physics - TheoryGeneral Physics and AstronomyNature of dark matter01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyClassical vs quantum cosmologyHigh Energy Physics - Phenomenology (hep-ph)010303 astronomy & astrophysicsQuantumMathematical PhysicsQuantum gravity and cosmologyPhysicsModification of general relativityChaplygin Gaslcsh:QC1-999CosmologyHigh Energy Physics - PhenomenologyExpansion of the UniversesymbolsGeneral RelativityGeneral relativityMaterials Science (miscellaneous)BiophysicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Metric expansion of spacesymbols.namesakeTheory of relativitySettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesDark matterddc:530Cosmological ModelsPhysical and Theoretical ChemistryPlanckEinsteindark matter; galaxies; nature of dark matter; beyond standard model; modification of general relativity; quantum gravity and cosmology; expansion of the Universe010308 nuclear & particles physicsFísicaGalaxiesAstrophysics - Astrophysics of GalaxiesCosmosEpistemologyHigh Energy Physics - Theory (hep-th)quantum gravityAstrophysics of Galaxies (astro-ph.GA)Quantum gravityBeyond standard modellcsh:Physics
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