Search results for " dark"

showing 10 items of 212 documents

Physics beyond colliders at CERN: beyond the Standard Model working group report

2019

The Physics Beyond Colliders initiative is an exploratory study aimed at exploiting the full scientific potential of the CERN's accelerator complex and scientific infrastructures through projects complementary to the LHC and other possible future colliders. These projects will target fundamental physics questions in modern particle physics. This document presents the status of the proposals presented in the framework of the Beyond Standard Model physics working group, and explore their physics reach and the impact that CERN could have in the next 10–20 years on the international landscape.

HIGH-ENERGYHigh energyaxionsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsPhysics beyond the Standard Model01 natural sciencesHigh Energy Physics - Experimentdark matter: couplingHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)photon: coupling[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental Techniquesphysics.ins-detPHOTON VETO DETECTORdark sectorPhysicsLarge Hadron Colliderneutrino: pair productionnew physics: search forlepton: flavor: violationdark matter: pair productionhep-phInstrumentation and Detectors (physics.ins-det)photon: invisible decayNEUTRAL HEAVY-LEPTONSHigh Energy Physics - PhenomenologyLIGHTCERN LHC Collphoton: mixingSystems engineeringParticle Physics - ExperimentNuclear and High Energy PhysicsCERN LabacceleratorPHI-MESON DECAYSExploratory researchFOS: Physical sciences530dark matterStandard ModelELECTRIC-DIPOLE MOMENTacceleratorsVECTOR GAUGE BOSONSEARCH0103 physical sciencesDARK-MATTERddc:530K: semileptonic decay[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]particle physics010306 general physicsvector boson: postulated particleCP CONSERVATIONbeyond standard ModelParticle Physics - Phenomenologylepton: universalityphoton: hidden sectorbeyond standard Model; dark matter; dark sector; axions; particle physics; acceleratorshep-ex010308 nuclear & particles physicscoupling constantCERN SPSlandscapeAccelerators and Storage Ringsdark matter: mediation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Fundamental physicsPhysics::Accelerator Physicsaxion: solarJournal of Physics G: Nuclear and Particle Physics
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Search for gamma-ray spectral lines with the DArk Matter Particle Explorer

2021

The DArk Matter Particle Explorer (DAMPE) is well suitable for searching for monochromatic and sharp $\gamma$-ray structures in the GeV$-$TeV range thanks to its unprecedented high energy resolution. In this work, we search for $\gamma$-ray line structures using five years of DAMPE data. To improve the sensitivity, we develop two types of dedicated data sets (including the BgoOnly data which is the first time to be used in the data analysis for the calorimeter-based gamma-ray observatories) and adopt the signal-to-noise ratio optimized regions of interest (ROIs) for different DM density profiles. No line signals or candidates are found between 10 and 300 GeV in the Galaxy. The constraints o…

High Energy Astrophysical Phenomena (astro-ph.HE)Line-like structureHigh Energy Physics - Experiment (hep-ex)MultidisciplinaryAstrophysics::High Energy Astrophysical PhenomenaDAMPE Dark matter Gamma-ray Line-like structureSettore FIS/01 - Fisica SperimentaleDAMPEDark matterFOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaGamma-rayHigh Energy Physics - ExperimentScience Bulletin
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Dark gamma-ray bursts

2016

Many theories of dark matter (DM) predict that DM particles can be captured by stars via scattering on ordinary matter. They subsequently condense into a DM core close to the center of the star and eventually annihilate. In this work, we trace DM capture and annihilation rates throughout the life of a massive star and show that this evolution culminates in an intense annihilation burst coincident with the death of the star in a core collapse supernova. The reason is that, along with the stellar interior, also its DM core heats up and contracts, so that the DM density increases rapidly during the final stages of stellar evolution. We argue that, counterintuitively, the annihilation burst is …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAnnihilation010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsType II supernova01 natural sciencesHigh Energy Physics - PhenomenologySupernovaHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesGravitational collapseAstrophysics::Solar and Stellar AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burst010303 astronomy & astrophysicsLight dark matterStellar evolutionAstrophysics::Galaxy AstrophysicsPhysical Review D
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Impeded Dark Matter

2016

We consider dark matter models in which the mass splitting between the dark matter particles and their annihilation products is tiny. Compared to the previously proposed Forbidden Dark Matter scenario, the mass splittings we consider are much smaller, and are allowed to be either positive or negative. To emphasize this modification, we dub our scenario "Impeded Dark Matter". We demonstrate that Impeded Dark Matter can be easily realized without requiring tuning of model parameters. For negative mass splitting, we demonstrate that the annihilation cross-section for Impeded Dark Matter depends linearly on the dark matter velocity or may even be kinematically forbidden, making this scenario al…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy PhysicsAnnihilation010308 nuclear & particles physicsPhysics beyond the Standard ModelDark matterCosmic microwave backgroundFOS: Physical sciencesObservableAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Negative mass0103 physical sciences010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaLight dark matterDwarf galaxy
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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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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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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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Planck-scale effects on WIMP dark matter

2014

There exists a widely known conjecture that gravitational effects violate global symmetries. We study the effect of global-symmetry violating higher-dimension operators induced by Planck-scale physics on the properties of WIMP dark matter. Using an effective description, we show that the lifetime of the WIMP dark matter candidate can satisfy cosmological bounds under reasonable assumptions regarding the strength of the dimension-five operators. On the other hand, the indirect WIMP dark matter detection signal is significantly enhanced due to new decay channels.

High Energy Physics - TheoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)WIMPMaterials Science (miscellaneous)Scalar field dark matterBiophysicsFOS: Physical sciencesGeneral Physics and AstronomyAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesdark matterHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciencesWarm dark matterindirect detectionparticle physicsPhysical and Theoretical Chemistry010306 general physicsLight dark matterMathematical PhysicsDark Matter PhenomenologyPhysics010308 nuclear & particles physicsHot dark matterPhysicsWIMP dark matterFísicalcsh:QC1-999decaying dark matterHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)astroparticle physicsWeakly interacting massive particlesPlanck scale effectsMixed dark matterdirect detectionHigh Energy Physics::Experimentlcsh:PhysicsDark fluidAstrophysics - Cosmology and Nongalactic AstrophysicsFrontiers in Physics
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Limits on the parameters of the equation of state for interacting dark energy

2010

Under the assumption that cold dark matter and dark energy interact with each other through a small coupling term, $Q$, we constrain the parameter space of the equation of state $w$ of those dark energy fields whose variation of the field since last scattering do not exceed Planck's mass. We use three parameterizations of $w$ and two different expressions for $Q$. Our work extends previous ones.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsEquation of stateCosmology and Nongalactic Astrophysics (astro-ph.CO)Hot dark matterScalar field dark matterFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyThermodynamics of the universeHigh Energy Physics - Theory (hep-th)Quantum mechanicsQuantum electrodynamicsMixed dark matterWarm dark matterDark energyLight dark matterDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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