Search results for " axion"

showing 10 items of 19 documents

Constraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penn…

2021

We constrain the coupling between axionlike particles (ALPs) and photons, measured with the superconducting resonant detection circuit of a cryogenic Penning trap. By searching the noise spectrum of our fixed-frequency resonant circuit for peaks caused by dark matter ALPs converting into photons in the strong magnetic field of the Penning-trap magnet, we are able to constrain the coupling of ALPs with masses around $2.7906-2.7914\,\textrm{neV/c}^2$ to $g_{a\gamma}< 1 \times 10^{-11}\,\textrm{GeV}^{-1}$. This is more than one order of magnitude lower than the best laboratory haloscope and approximately 5 times lower than the CERN axion solar telescope (CAST), setting limits in a mass and cou…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonAtomic Physics (physics.atom-ph)Dark matterOther Fields of PhysicsFOS: Physical sciencesGeneral Physics and Astronomyphysics.atom-ph01 natural sciences7. Clean energyPhysics - Atomic PhysicsNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530Physics::Atomic Physics010306 general physicsParticle Physics - PhenomenologySuperconductivityPhysicshep-phPenning trapCoupling (probability)Magnetic fieldHigh Energy Physics - PhenomenologyAntiprotonastro-ph.COPräzisionsexperimente - Abteilung BlaumCERN Axion Solar TelescopeAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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Infrasonic, Acoustic and Seismic Waves Produced by the Axion Quark Nuggets

2022

We advocate an idea that the Axion Quark Nuggets (AQN) hitting the Earth can be detected by analysing the infrasound, acoustic and seismic waves which always accompany the AQN's passage in the atmosphere and underground. Our estimates for the infrasonic frequency $\nu\simeq 5$ ~Hz and overpressure $\delta p\sim 0.3 ~$Pa for relatively large size dark matter (DM) nuggets suggest that sensitivity of presently available instruments is already sufficient to detect very intense (but very rare) events today with existing technology. A study of much more frequent but less intense events requires a new type of instruments. We propose a detection strategy for a systematic study to search for such re…

Earth and Planetary Astrophysics (astro-ph.EP)570Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)General MathematicsFOS: Physical sciencesGeophysics (physics.geo-ph)Physics - GeophysicsHigh Energy Physics - PhenomenologyPhysics - Atmospheric and Oceanic PhysicsHigh Energy Physics - Phenomenology (hep-ph)Chemistry (miscellaneous)ddc:570Atmospheric and Oceanic Physics (physics.ao-ph)Computer Science (miscellaneous)dark matter; axion; quark nuggetsAstrophysics - Cosmology and Nongalactic AstrophysicsAstrophysics - Earth and Planetary AstrophysicsSymmetry
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Spectroscopy of Alkali Atoms in Solid Matrices of Rare Gases: Experimental Results and Theoretical Analysis

2022

We present an experimental and theoretical investigation of the spectroscopy of dilute alkali atoms in a solid matrix of inert gases at cryogenic temperatures, specifically Rubidium atoms in a solid Argon or Neon matrix, and related aspects of the interaction energies between the alkali atoms and the atoms of the solid matrix. The system considered is relevant for matrix isolation spectroscopy, and it is at the basis of a recently proposed detector of cosmological axions, exploiting magnetic-type transitions between Zeeman sublevels of alkali atoms in a magnetic field, tuned to the axion mass, assumed in the meV range. Axions are one of the supposed constituents of the dark matter (DM) of t…

Fluid Flow and Transfer ProcessesCondensed Matter::Quantum GasesQuantum PhysicsAtomic Physics (physics.atom-ph)Process Chemistry and Technologymatrix isolation spectroscopy; axion detection; interatomic interactionsGeneral EngineeringFOS: Physical sciencesInteratomic interactionsSettore FIS/03 - Fisica Della MateriaPhysics - Atomic PhysicsComputer Science ApplicationsMatrix isolation spectroscopyAxion detectionPhysics::Atomic and Molecular ClustersGeneral Materials SciencePhysics::Atomic PhysicsQuantum Physics (quant-ph)InstrumentationApplied Sciences; Volume 12; Issue 13; Pages: 6492
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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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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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Light Dark Matter Search with Ionization Signals in XENON1T

2019

We report constraints on light dark matter (DM) models using ionization signals in the XENON1T experiment. We mitigate backgrounds with strong event selections, rather than requiring a scintillation signal, leaving an effective exposure of (22±3) tonne day. Above ∼0.4 keVee, we observe &lt;1 event/(tonne day keVee), which is more than 1000 times lower than in similar searches with other detectors. Despite observing a higher rate at lower energies, no DM or CEvNS detection may be claimed because we cannot model all of our backgrounds. We thus exclude new regions in the parameter spaces for DM-nucleus scattering for DM masses mχ within 3–6 GeV/c2, DM-electron scattering for mχ&gt;30 MeV/c2, a…

Light Dark Matter TPC Ionization Axion-Like particlesCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonFOS: Physical sciencesGeneral Physics and AstronomyS030DI5S029AECAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)S030DE5Ionization0103 physical sciencesionization[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsAbsorption (electromagnetic radiation)Light dark matterscintillation counterPhysicsDark Matter WIMP Dark-Matter detectors Time-projection chamber detectorsScintillationScatteringbackgrounddark matter: massphotonscatteringS029HPHS030DN5* Automatic Keywords *Scintillation counterElementary Particles and Fieldsaxion-like particles[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)absorptionAstrophysics - Cosmology and Nongalactic Astrophysics
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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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Constraining interactions mediated by axion-like particles with ultracold neutrons

2015

We report a new limit on a possible short range spin-dependent interaction from the precise measurement of the ratio of Larmor precession frequencies of stored ultracold neutrons and Hg199 atoms confined in the same volume. The measurement was performed in a ~1μT vertical magnetic holding field with the apparatus searching for a permanent electric dipole moment of the neutron at the Paul Scherrer Institute. A possible coupling between freely precessing polarized neutron spins and unpolarized nucleons of the wall material can be investigated by searching for a tiny change of the precession frequencies of neutron and mercury spins. Such a frequency change can be interpreted as a consequence o…

Nuclear and High Energy PhysicsNeutron magnetic momentNeutron electric dipole momentFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsPHYSICSHigh Energy Physics - Experiment (hep-ex)Complementary experimentsHigh Energy Physics - Phenomenology (hep-ph)AxionMOMENTS[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]SEARCH0103 physical sciencesAxion-like particleultracold neutronsNeutron010306 general physicsCoupling constantLarmor precessionPhysics[PHYS]Physics [physics]010308 nuclear & particles physicsNeutron electric dipole moment[SPI.PLASMA]Engineering Sciences [physics]/Plasmaslcsh:QC1-999neutron electric dipole momentShort range spin-dependent interactionElectric dipole momentHigh Energy Physics - PhenomenologyCP violationaxion-like particleaxionUltracold neutronsshort range spin-dependent interactionFORCESUltracold neutronsCP violation; Short range spin-dependent interaction; Axion; Axion-like particle; Ultracold neutrons; Neutron electric dipole momentlcsh:Physics
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Next Generation Search for Axion and ALP Dark Matter with the International Axion Observatory

2018

International audience; More than 80 years after the postulation of dark matter, its nature remains one of the fundamental questions in cosmology. Axions are currently one of the leading candidates for the hypothetical, non-baryonic dark matter that is expected to account for about 25% of the energy density of the Universe. Especially in the light of the Large Hadron Collider at CERN slowly closing in on Weakly-Interacting Massive Particle (WIMP) searches, axions and axion-like particles (ALPs) provide a viable alternative approach to solving the dark matter problem. The fact that makes them particularly appealing is that they were initially introduced to solve a long-standing problem in qu…

Particle physicsCERN LabPhysics::Instrumentation and DetectorsDark matterObservatoriesaxion: detector7. Clean energy01 natural sciencesCosmologyHigh Energy Physics::TheoryPrimakoff effectSensitivityWIMP0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAxionPrimakoff effectactivity reportPhysicsHelioscopeLarge Hadron Collider010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyToroidal magnetic fieldsDetectorsobservatory13. Climate actionCouplingsaxion-like particlesproposed experimentCERN Axion Solar Telescopeaxion: solarTelescopes
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