Search results for "Axion"

showing 10 items of 121 documents

Proposal to Detect Dark Matter using Axionic Topological Antiferromagnets

2019

Antiferromagnetically doped topological insulators (A-TI) are among the candidates to host dynamical axion fields and axion-polaritons; weakly interacting quasiparticles that are analogous to the dark axion, a long sought after candidate dark matter particle. Here we demonstrate that using the axion quasiparticle antiferromagnetic resonance in A-TI's in conjunction with low-noise methods of detecting THz photons presents a viable route to detect axion dark matter with mass 0.7 to 3.5 meV, a range currently inaccessible to other dark matter detection experiments and proposals. The benefits of this method at high frequency are the tunability of the resonance with applied magnetic field, and t…

Particle physicsPhotonPhysics - Instrumentation and DetectorsDark matterGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesResonance (particle physics)530High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Condensed Matter - Strongly Correlated ElectronsHigh Energy Physics - Phenomenology (hep-ph)Detect Dark Matter; Antiferromagnets0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Polariton010306 general physicsAxionPhysicsStrongly Correlated Electrons (cond-mat.str-el)Condensed Matter - Mesoscale and Nanoscale PhysicsInstrumentation and Detectors (physics.ins-det)Magnetic fieldHigh Energy Physics - PhenomenologyTopological insulatorQuasiparticleCondensed Matter::Strongly Correlated Electrons
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Axion search with BabyIAXO in view of IAXO

2020

Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun's core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to backgro…

Particle physicsPhysics - Instrumentation and Detectorssolar axion[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]experimental methodsDark matterFOS: Physical sciences7. Clean energyString (physics)Standard Modelaxion helioscopedesign [detector]International Axion Observatory (IAXO)ObservatoryPeccei-Quinn mechanismDark Matterdetector design[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental TechniquesAxionsun-tracking systemsphysics.ins-detactivity reportdetector: designPhysicsinstrumentationHelioscopeLarge Hadron Colliderdetectorsolar [axion]DESYInstrumentation and Detectors (physics.ins-det)[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]IAXOmagnetopticsaxion: solar
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Leptogenesis from oscillations and dark matter

2019

An extension of the Standard Model with Majorana singlet fermions in the 1–100 GeV range can explain the light neutrino masses and give rise to a baryon asymmetry at freeze-in of the heavy states, via their CP-violating oscillations. In this paper we consider extending this scenario to also explain dark matter. We find that a very weakly coupled B−L gauge boson, an invisible QCD axion model, and the singlet majoron model can simultaneously account for dark matter and the baryon asymmetry.

Particle physicsPhysics and Astronomy (miscellaneous)Dark matterFOS: Physical scienceslcsh:AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetrylcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclear Experiment010306 general physicsEngineering (miscellaneous)AxionMajoronPhysicsGauge boson010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHigh Energy Physics - PhenomenologyLeptogenesislcsh:QC770-798High Energy Physics::ExperimentNeutrinoThe European Physical Journal C
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Application of spin-exchange relaxation-free magnetometry to the Cosmic Axion Spin Precession Experiment

2018

The Cosmic Axion Spin Precession Experiment (CASPEr) seeks to measure oscillating torques on nuclear spins caused by axion or axion-like-particle (ALP) dark matter via nuclear magnetic resonance (NMR) techniques. A sample spin-polarized along a leading magnetic field experiences a resonance when the Larmor frequency matches the axion/ALP Compton frequency, generating precessing transverse nuclear magnetization. Here we demonstrate a Spin-Exchange Relaxation-Free (SERF) magnetometer with sensitivity $\approx 1~{\rm fT/\sqrt{Hz}}$ and an effective sensing volume of 0.1 $\rm{cm^3}$ that may be useful for NMR detection in CASPEr. A potential drawback of SERF-magnetometer-based NMR detection is …

Physics - Instrumentation and DetectorsMagnetometerAtomic Physics (physics.atom-ph)FOS: Physical sciences01 natural sciences7. Clean energylaw.inventionPhysics - Atomic Physics010309 opticsMagnetizationPhysics - Space Physicslaw0103 physical sciences010306 general physicsAxionLarmor precessionPhysicsSpinsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Magnetic fluxSpace Physics (physics.space-ph)Magnetic fieldSpace and Planetary SciencePrecessionAtomic physicsPhysics of the Dark Universe
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Quantum sensitivity limits of nuclear magnetic resonance experiments searching for new fundamental physics

2021

Nuclear magnetic resonance is a promising experimental approach to search for ultra-light axion-like dark matter. Searches such as the cosmic axion spin-precession experiments (CASPEr) are ultimately limited by quantum-mechanical noise sources, in particular, spin-projection noise. We discuss how such fundamental limits can potentially be reached. We consider a circuit model of a magnetic resonance experiment and quantify three noise sources: spin-projection noise, thermal noise, and amplifier noise. Calculation of the total noise spectrum takes into account the modification of the circuit impedance by the presence of nuclear spins, as well as the circuit back-action on the spin ensemble. S…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Materials Science (miscellaneous)Dark matterFOS: Physical sciences01 natural sciencesNoise (electronics)010305 fluids & plasmasNuclear magnetic resonanceHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530Sensitivity (control systems)Electrical and Electronic Engineering010306 general physicsAxionQuantumElectrical impedanceSpin-½PhysicsQuantum PhysicsSpinsInstrumentation and Detectors (physics.ins-det)Atomic and Molecular Physics and OpticsCondensed Matter - Other Condensed MatterHigh Energy Physics - PhenomenologyQuantum Physics (quant-ph)Other Condensed Matter (cond-mat.other)
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The cosmic axion spin precession experiment (CASPEr): a dark-matter search with nuclear magnetic resonance

2017

The Cosmic Axion Spin Precession Experiment (CASPEr) is a nuclear magnetic resonance experiment (NMR) seeking to detect axion and axion-like particles which could make up the dark matter present in the universe. We review the predicted couplings of axions and axion-like particles with baryonic matter that enable their detection via NMR. We then describe two measurement schemes being implemented in CASPEr. The first method, presented in the original CASPEr proposal, consists of a resonant search via continuous-wave NMR spectroscopy. This method offers the highest sensitivity for frequencies ranging from a few Hz to hundreds of MHz, corresponding to masses $ m_{\rm a} \sim 10^{-14}$--$10^{-6}…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsMagnetometerMaterials Science (miscellaneous)Dark matterFOS: Physical sciencesApplied Physics (physics.app-ph)7. Clean energy01 natural scienceslaw.inventionHigh Energy Physics - Phenomenology (hep-ph)Nuclear magnetic resonancelaw0103 physical sciencesElectrical and Electronic Engineering010306 general physicsAxionPhysicsQuantum PhysicsCOSMIC cancer database010308 nuclear & particles physicsBandwidth (signal processing)RangingInstrumentation and Detectors (physics.ins-det)Physics - Applied PhysicsNuclear magnetic resonance spectroscopyAtomic and Molecular Physics and OpticsBaryonHigh Energy Physics - PhenomenologyPhysics - Data Analysis Statistics and ProbabilityQuantum Physics (quant-ph)Data Analysis Statistics and Probability (physics.data-an)Quantum Science and Technology
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The 3 Cavity Prototypes of RADES: An Axion Detector Using Microwave Filters at CAST

2019

The Relic Axion Detector Experimental Setup (RADES) is an axion search project that uses a microwave filter as resonator for Dark Matter conversion. The main focus of this publication is the description of the 3 different cavity prototypes of RADES. The result of the first tests of one of the prototypes is also presented. The filters consist of 5 or 6 stainless steel sub-cavities joined by rectangular irises. The size of the sub-cavities determines the working frequency, the amount of sub-cavities determine the working volume. The first cavity prototype was built in 2017 to work at a frequency of $\sim$ 8.4 GHz and it was placed at the 9 T CAST dipole magnet at CERN. Two more prototypes wer…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ResonatorOpticsDipole magnet0103 physical sciencesSensitivity (control systems)Detectors and Experimental Techniques010306 general physicsAxionphysics.ins-detPhysicsLarge Hadron Collider010308 nuclear & particles physicsbusiness.industryhep-exDetectorInstrumentation and Detectors (physics.ins-det)Filter (signal processing)Physics::Accelerator PhysicsbusinessMicrowaveParticle Physics - Experiment
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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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SO(3) family symmetry and axions

2018

Motivated by the idea of comprehensive unification, we study a gauged SO(3) flavor extension of the extended Standard Model, including right-handed neutrinos and a Peccei-Quinn symmetry with simple charge assignments. The model accommodates the observed fermion masses and mixings and yields a characteristic, successful relation among them. The Peccei-Quinn symmetry is an essential ingredient.

Physics010308 nuclear & particles physicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesCharge (physics)FermionComputer Science::Digital Libraries01 natural sciencesSymmetry (physics)High Energy Physics - PhenomenologyTheoretical physicsStandard Model (mathematical formulation)High Energy Physics - Phenomenology (hep-ph)Simple (abstract algebra)0103 physical sciencesNeutrino010306 general physicsAxionRotation group SOPhysical Review D
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Improved Limits on Axionlike-Particle-Mediated P , T -Violating Interactions between Electrons and Nucleons from Electric Dipole Moments of Atoms and…

2018

In the presence of P, T-violating interactions, the exchange of axionlike particles between electrons and nucleons in atoms and molecules induces electric dipole moments (EDMs) of atoms and molecules. We perform calculations of such axion-exchange-induced atomic EDMs using the relativistic Hartree-Fock-Dirac method including electron core polarization corrections. We present analytical estimates to explain the dependence of these induced atomic EDMs on the axion mass and atomic parameters. From the experimental bounds on the EDMs of atoms and molecules, including ^{133}Cs, ^{205}Tl, ^{129}Xe, ^{199}Hg, ^{171}Yb^{19}F, ^{180}Hf^{19}F^{+}, and ^{232}Th^{16}O, we constrain the P, T-violating s…

Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAtoms in moleculesHartree–Fock methodGeneral Physics and AstronomyElectron01 natural sciencesDipole0103 physical sciencesCP violationPhysics::Atomic PhysicsAtomic physics010306 general physicsRandom phase approximationNucleonAxionPhysical Review Letters
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