Search results for "axions"

showing 10 items of 19 documents

Hints of an axion-like particle mixing in the GeV gamma-ray blazar data?

2013

Axion-Like Particles (ALPs), if exist in nature, are expected to mix with photons in the presence of an external magnetic field. The energy range of photons which undergo strong mixing with ALPs depends on the ALP mass, on its coupling with photons as well as on the external magnetic field and particle density configurations. Recent observations of blazars by the Fermi Gamma-Ray Space Telescope in the 0.1-300 GeV energy range show a break in their spectra in the 1-10 GeV range. We have modeled this spectral feature for the flat-spectrum radio quasar 3C454.3 during its November 2010 outburst, assuming that a significant fraction of the gamma rays convert to ALPs in the large scale jet of thi…

AstrofísicaActive galactic nucleusPhotonAxionsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesPartícules (Física nuclear)Spectral lineHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBlazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsActive galactic nucleiRange (particle radiation)Cosmologia010308 nuclear & particles physicsGamma rayAstronomy and AstrophysicsQuasarHigh Energy Physics - Phenomenology13. Climate actionAstrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeJournal of Cosmology and Astroparticle Physics
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PBH assisted search for QCD axion dark matter

2022

The entropy production prior to BBN era is one of ways to prevent QCD axion with the decay constant $F_{a}\in[10^{12}{\rm GeV},10^{16}{\rm GeV}]$ from overclosing the universe when the misalignment angle is $\theta_{\rm i}=\mathcal{O}(1)$. As such, it is necessarily accompanied by an early matter-dominated era (EMD) provided the entropy production is achieved via the decay of a heavy particle. In this work, we consider the possibility of formation of primordial black holes during the EMD era with the assumption of the enhanced primordial scalar perturbation on small scales ($k>10^{4}{\rm Mpc}^{-1}$). In such a scenario, it is expected that PBHs with axion halo accretion develop to ultracomp…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)axionsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesmustat aukotAstrophysics::Cosmology and Extragalactic Astrophysicshiukkasfysiikkakosmologianeutron starspimeä aineHigh Energy Physics - Phenomenology (hep-ph)neutronitähdetParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEdark matter experimentsHigh Energy Physics::Phenomenologyprimordial black holesAstronomy and Astrophysicshep-phHigh Energy Physics - Phenomenologyastro-ph.COkvanttiväridynamiikkaHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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High magnetic fields for fundamental physics

2018

Various fundamental-physics experiments such as measurement of the birefringence of the vacuum, searches for ultralight dark matter (e.g., axions), and precision spectroscopy of complex systems (including exotic atoms containing antimatter constituents) are enabled by high-field magnets. We give an overview of current and future experiments and discuss the state-of-the-art DC- and pulsed-magnet technologies and prospects for future developments.

Astrophysics and AstronomyPhysics - Instrumentation and Detectorsmagnet: designmagnetic field: highAtomic Physics (physics.atom-ph)AxionsDark matterComplex systemOther Fields of PhysicsFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesphysics.atom-phNOPhysics - Atomic PhysicsNuclear physicsPhysics and Astronomy (all)Neutrino mass0103 physical sciencesDark matter[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Axions; Dark matter; High-field magnets; Neutrino mass; Spectroscopy; Vacuum birefringence; Physics and Astronomy (all)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental Techniques010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Axionphysics.ins-detSpectroscopyactivity reportExotic atomPhysicsVacuum birefringence010308 nuclear & particles physicsInstrumentation and Detectors (physics.ins-det)Polarization (waves)magnet: technology[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]3. Good healthMagnetic fieldHigh-field magnetsAntimatterMagnetAstrophysics - Instrumentation and Methods for Astrophysicsastro-ph.IM
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Design of New Resonant Haloscopes in the Search for the Dark Matter Axion: A Review of the First Steps in the RADES Collaboration

2022

This article belongs to the Special Issue Studying the Universe from Spain.

Dark matter detectorsResonant cavitiesaxionsdark matter detectorsPhysics - Instrumentation and Detectorshep-exAxionsGeneral Physics and AstronomyFOS: Physical sciencesElementary particle physicsInstrumentation and Detectors (physics.ins-det)QC793-793.5HaloscopesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)haloscopesDetectors and Experimental Techniquesphysics.ins-detParticle Physics - Experimentresonant cavities
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Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation

2021

Full list of authors: Abdalla, H.; Abe, H.; Acero, F.; Acharyya, A.; Adam, R.; Agudo, I; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Batista, R. Alves; Amati, L.; Amato, E.; Ambrosi, G.; Anguner, E. O.; Araudo, A.; Armstrong, T.; Arqueros, F.; Arrabito, L.; Asano, K.; Ascasibar, Y.; Ashley, M.; Backes, M.; Balazs, C.; Balbo, M.; Balmaverde, B.; Baquero Larriva, A.; Martins, V. Barbosa; Barkov, M.; Baroncelli, L.; de Almeida, U. Barres; Barrio, J. A.; Batista, P-, I; Becerra Gonzalez, J.; Becherini, Y.; Beck, G.; Tjus, J. Becker; Belmont, R.; Benbow, W.; Bernardini, E.; Berti, A.; Berton, M.; Bertucci, B.; Beshley, V; Bi, B.; Biasuzzi, B.; Biland, A.; Bissaldi, …

Gamma ray AstronomyCherenkov Telescope ArrayaxionsMATÉRIA ESCURAredshift: dependenceAstronomyGamma ray experimentsgamma ray experimentsAstrophysics01 natural sciencesCosmologyObservatorycosmological model: parameter spacegamma ray experimentHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsCherenkov telescopes ; IACT technique ; Gamma rays ; Cosmic raysnew physics4. EducationSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma-ray astronomyviolation: Lorentz3. Good healthobservatoryExtragalactic background lightastro-ph.COaxion-like particlesFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysicsgamma ray: propagationCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusAxionsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsinvariance: Lorentzjet: relativisticdark matter: halo0103 physical sciencesactive galactic nuclei; gamma ray experiments; axions; extragalactic magnetic fieldsAGNBlazarbackground010308 nuclear & particles physicsFísicaAstronomy and AstrophysicssensitivityCherenkov Telescope Arrayaxionextragalactic magnetic fieldsactive galactic nuclei[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]absorptionstatisticalBlazarsTelescopes
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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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Conceptual design of the International Axion Observatory (IAXO)

2014

The International Axion Observatory (IAXO) will be a forth generation axion helioscope. As its primary physics goal, IAXO will look for axions or axion-like particles (ALPs) originating in the Sun via the Primakoff conversion of the solar plasma photons. In terms of signal-to-noise ratio, IAXO will be about 4-5 orders of magnitude more sensitive than CAST, currently the most powerful axion helioscope, reaching sensitivity to axion-photon couplings down to a few $\times 10^{-12}$ GeV$^{-1}$ and thus probing a large fraction of the currently unexplored axion and ALP parameter space. IAXO will also be sensitive to solar axions produced by mechanisms mediated by the axion-electron coupling $g_{…

MICROPICPhysics - Instrumentation and DetectorsPhotonaxionsParameter space7. Clean energyHigh Energy Physics - ExperimentDark Matter detectors (WIMPs axions etc.)High Energy Physics - Experiment (hep-ex)Observatoryetc.)Micropattern gaseous detectors (MSGC GEM THGEM RETHGEM MHSP MICROPIC MICROMEGAS InGrid etc)Detectors and Experimental TechniquesInstrumentationMathematical PhysicsPhysicsGEMsolar [axion]Dark Matter Detectors (Wimps Axions etc.)MicroMegas detectorX-ray detectorsInstrumentation and Detectors (physics.ins-det)Dark Matter detectors (WIMPs axions etc.); Large detector systems for particle and astroparticle physics; Micropattern gaseous detectors (MSGC GEM THGEM RETHGEM MHSP MICROPIC MICROMEGAS InGrid etc); X-ray detectors; Instrumentation; Mathematical PhysicssolarobservatoryMICROMEGASMHSPaxion-like particlesproposed experimentaxions ; dark matter detectors ; x-ray detectors ; Micropattern gaseous detectors ; large detector systems for particle and astroparticle physicsMicromegasX-ray detectorParticle physicsoptics [X-ray]FOS: Physical sciencesSuperconducting magnetMicropattern gaseous detectors (MSGCddc:610Axionactivity reportDark Matter detectors (WIMPssuperconductivity [magnet]etc)HelioscopeLarge detector systems for particle and astroparticle physicssensitivityInGridRETHGEMOrders of magnitude (time)axionLarge detector systems for particle and astroparticle physicTHGEMMicropattern Gaseous Detectors (MSGC Gem THGEM Rethgem MHSP Micropic Micromegas In Grid; etc)
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New Physics adventures in the LHC age

2017

La física de partículas está viviendo actualmente una era de exploración que comenzó con la observación en el LHC del bosón de Higgs, proporcionando así al Modelo Estándar de la Física de Partículas la elusiva pieza final que lo completa. Si bien esta teoría es extremadamente exitosa, se acepta comúnmente que no es la teoría final ya que no puede responder a todas las preguntas teóricas ni a ciertas observaciones experimentales. Por lo tanto, se espera que Nueva Física que extienda al Modelo Estándar aparezca pronto, aunque esto bien podría ser sólo una esperanza. Esta tesis recoge algunas de las aventuras en la búsqueda de Nueva Física. Se organiza en tres partes: la Parte I introduce, en …

New PhysicsAxionsTwo-Higgs-doublet model:FÍSICA::Física de altas energías::Física teórica altas energías [UNESCO]Strong CP problemEffective Field TheoriesFlavor anomaliesGauge extended sectorsUNESCO::FÍSICA::Física de altas energías::Física teórica altas energíasB physics
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DARWIN: Towards the ultimate dark matter detector

2016

DARk matter WImp search with liquid xenoN (DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core. Its primary goal will be to explore the experimentally accessible parameter space for Weakly Interacting Massive Particles (WIMPs) in a wide mass-range, until neutrino interactions with the target become an irreducible background. The prompt scintillation light and the charge signals induced by particle interactions in the xenon will be observed by VUV sensitive, ultra-low background photosensors. Besides its excellent sensitivity to WIMPs above a mass of 5 GeV/c2, such a detector with its large mass, low-energy …

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsdouble beta decay7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsNeutrino detectorHigh Energy Physics - Experiment (hep-ex)XenonWIMPPHOTOMULTIPLIERAXIONSphysics.ins-detsolar and atmospheric neutrinosPhysicsDark matter detectorTime projection chamberdark matter detectorsPhysicsSolar and atmospheric neutrinoInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicsNeutrino detectorSOLAR NEUTRINOSGASPhysical SciencesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsGRAN SASSODark matter detectors; Double beta decay; Neutrino detectors; Solar and atmospheric neutrinosDark matterchemistry.chemical_elementFOS: Physical sciencesAstronomy & AstrophysicsLIQUID-XENON DETECTOR0202 Atomic Molecular Nuclear Particle And Plasma PhysicsSettore FIS/05 - Astronomia e AstrofisicaSEARCH0103 physical sciencesIsotopes of xenonZEPLIN-III[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAxionInstrumentation and Methods for Astrophysics (astro-ph.IM)Science & Technology010308 nuclear & particles physicshep-exAstronomyAstronomy and Astrophysics0201 Astronomical And Space ScienceschemistryHigh Energy Physics::ExperimentSCINTILLATIONneutrino detectorsastro-ph.IMJournal of Cosmology and Astroparticle Physics
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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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