Search results for "Massive particle"

showing 10 items of 47 documents

Determining the dark matter mass with DeepCore

2013

Cosmological and astrophysical observations provide increasing evidence of the existence of dark matter in our Universe. Dark matter particles with a mass above a few GeV can be captured by the Sun, accumulate in the core, annihilate, and produce high energy neutrinos either directly or by subsequent decays of Standard Model particles. We investigate the prospects for indirect dark matter detection in the IceCube/DeepCore neutrino telescope and its capabilities to determine the dark matter mass.

AstrofísicaNuclear and High Energy PhysicsLarge Underground Xenon experimentAstrophysics::High Energy Astrophysical PhenomenaDark matterScalar field dark matterFOS: Physical sciencesAnnihilationAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Baryonic dark matter0103 physical sciencesWarm dark matter010306 general physicsLight dark matterPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cosmologia010308 nuclear & particles physicsHot dark matterAstronomyDetectorsHigh Energy Physics - Phenomenology13. Climate actionWeakly interacting massive particlesHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
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Removing krypton from xenon by cryogenic distillation to the ppq level

2017

The XENON1T experiment aims for the direct detection of dark matter in a detector filled with 3.3 tons of liquid xenon. In order to achieve the desired sensitivity, the background induced by radioactive decays inside the detector has to be sufficiently low. One major contributor is the β-emitter 85Kr which is present in the xenon. For XENON1T a concentration of natural krypton in xenon natKr/Xe<200ppq (parts per quadrillion, 1ppq=10-15mol/mol) is required. In this work, the design, construction and test of a novel cryogenic distillation column using the common McCabe–Thiele approach is described. The system demonstrated a krypton reduction factor of 6.4 · 10 5 with thermodynamic stability a…

CryostatPhysics - Instrumentation and DetectorsXenonPhysics and Astronomy (miscellaneous)WIMPDark matterAnalytical chemistryFOS: Physical scienceschemistry.chemical_elementlcsh:AstrophysicsWeakly Interact Massive ParticleSciences de l'ingénieur01 natural sciences7. Clean energyXenonlcsh:QB460-4660103 physical sciencesDark Matterlcsh:Nuclear and particle physics. Atomic energy. RadioactivitySensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsComputer science information & general worksEngineering (miscellaneous)Liquid XenonComputingMilieux_MISCELLANEOUSPhysicsAir separationPhysique010308 nuclear & particles physicsDistillation ColumnKryptonKryptonOrder (ring theory)Instrumentation and Detectors (physics.ins-det)AstronomiechemistryDirect Searchddc:000lcsh:QC770-798TPCOrder of magnitude
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Electron-interacting dark matter: Implications from DAMA/LIBRA-phase2 and prospects for liquid xenon detectors and NaI detectors

2019

We investigate the possibility for the direct detection of low-mass (GeV scale) weakly interacting massive particles (WIMP) dark matter in scintillation experiments. Such WIMPs are typically too light to leave appreciable nuclear recoils but may be detected via their scattering off atomic electrons. In particular, the DAMA Collaboration [R. Bernabei et al., Nucl. Phys. At. Energy 19, 307 (2018)] has recently presented strong evidence of an annual modulation in the scintillation rate observed at energies as low as 1 keV. Despite a strong enhancement in the calculated event rate at low energies, we find that an interpretation in terms of electron-interacting WIMPs cannot be consistent with ex…

DAMA/LIBRACosmology and Nongalactic Astrophysics (astro-ph.CO)detector: performancePhysics::Instrumentation and DetectorsDark matterFOS: Physical scienceschemistry.chemical_elementElectron01 natural sciencesWIMP: dark matterNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)XenonWIMP0103 physical sciences010306 general physicsenhancementscintillation counterenergy: lowPhysicsScintillationxenon: liquid010308 nuclear & particles physicsatom: wave functionDAMAmodulationHigh Energy Physics - Phenomenologychemistryelectron: scatteringWeakly interacting massive particles[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]direct detection[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Astrophysics and astroparticle physicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review
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Dark Matter Search Results from a One Ton-Year Exposure of XENON1T

2018

We report on a search for Weakly Interacting Massive Particles (WIMPs) using 278.8 days of data collected with the XENON1T experiment at LNGS. XENON1T utilizes a liquid xenon time projection chamber with a fiducial mass of $(1.30 \pm 0.01)$ t, resulting in a 1.0 t$\times$yr exposure. The energy region of interest, [1.4, 10.6] $\mathrm{keV_{ee}}$ ([4.9, 40.9] $\mathrm{keV_{nr}}$), exhibits an ultra-low electron recoil background rate of $(82\substack{+5 \\ -3}\textrm{ (sys)}\pm3\textrm{ (stat)})$ events/$(\mathrm{t}\times\mathrm{yr}\times\mathrm{keV_{ee}})$. No significant excess over background is found and a profile likelihood analysis parameterized in spatial and energy dimensions exclude…

Dark matterGeneral Physics and Astronomychemistry.chemical_elementS030DI5WIMP: massElectronParameter spacedark matter: direct detectionGravitation and AstrophysicsS030DI101 natural sciencesS030DI3S030DI2Nuclear physicsXenonRecoilWIMPelectron: recoil0103 physical sciencesS046DM2[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsnumerical calculationsDark Matter WIMP TPC XENON Direct searchPhysicsxenon: liquidTime projection chamber010308 nuclear & particles physicsbackgrounddark matter: massGran SassoWIMP nucleonchemistryWeakly interacting massive particles[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]time projection chamber: xenon[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Search for magnetic monopoles with the MoEDAL prototype trapping detector in 8 TeV proton-proton collisions at the LHC

2016

The MoEDAL experiment is designed to search for magnetic monopoles and other highly-ionising particles produced in high-energy collisions at the LHC. The largely passive MoEDAL detector, deployed at Interaction Point 8 on the LHC ring, relies on two dedicated direct detection techniques. The first technique is based on stacks of nuclear-track detectors with surface area $\sim$18 m$^2$, sensitive to particle ionisation exceeding a high threshold. These detectors are analysed offline by optical scanning microscopes. The second technique is based on the trapping of charged particles in an array of roughly 800 kg of aluminium samples. These samples are monitored offline for the presence of trap…

ExoticsParticle physicsNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsProtonMagnetic monopoleFOS: Physical sciencesddc:500.2Particle and resonance production114 Physical sciences7. Clean energy01 natural sciencesMathematical SciencesHigh Energy Physics - Experimentlaw.inventionCOLLIDERHigh Energy Physics - Experiment (hep-ex)MAGNETIC MONOPOLESSTOPPING-POWERlawHadron-Hadron scattering (experiments)0103 physical sciencesFIELD010306 general physicsColliderHIGHLY IONIZING PARTICLESphysics.ins-detPhysicsOPALLarge Hadron ColliderSTABLE MASSIVE PARTICLEShep-ex010308 nuclear & particles physicsInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicsPair productionMoEDAL experimentPhysical SciencesProduction (computer science)CHARGEParticle Physics - ExperimentEnergy (signal processing)Exotic
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Testing freeze-in with axial and vector Z′ bosons

2021

The freeze-in production of Feebly Interacting Massive Particle (FIMP) dark matter in the early universe is an appealing alternative to the well-known - and constrained - Weakly Interacting Massive Particle (WIMP) paradigm. Although challenging, the phenomenology of FIMP dark matter has been receiving growing attention and is possible in a few scenarios. In this work, we contribute to this endeavor by considering a $Z^\prime$ portal to fermionic dark matter, with the $Z^\prime$ having both vector and axial couplings and a mass ranging from MeV up to PeV. We evaluate the bounds on both freeze-in and freeze-out from direct detection, atomic parity violation, leptonic anomalous magnetic moment…

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectDark matterMassive particleFOS: Physical sciencesContext (language use)QC770-7987. Clean energy01 natural sciencesPartícules (Física nuclear)law.inventionHigh Energy Physics - Phenomenology (hep-ph)WIMPlawNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesBeam dump010306 general physicsmedia_commonBosonHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCosmologia010308 nuclear & particles physicsCosmology of Theories beyond the SMUniverse3. Good healthHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Beyond Standard ModelAstrophysics - High Energy Astrophysical PhenomenaPhenomenology (particle physics)Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy 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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Fitting formulae for photon spectra from WIMP annihilation

2011

Annihilation of different dark matter (DM) candidates into Standard Model (SM) particles could be detected through their contribution to the gamma ray fluxes that are measured on the Earth. The magnitude of such contributions depends on the particular DM candidate, but certain imprints of produced photon spectra may be analyzed in a model-independent fashion. In this work we provide the fitting formulae for the photon spectra generated by WIMP annihilation into quarks, leptons and gauge bosons channels in a wide range of WIMP masses.

High Energy Physics - TheoryQuarkHistoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciences01 natural sciencesEducationStandard ModelNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences010306 general physicsPhysicsGauge bosonAnnihilation010308 nuclear & particles physicsFísicaComputer Science ApplicationsHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Weakly interacting massive particlesAstrophysics - Cosmology and Nongalactic AstrophysicsLeptonJournal of Physics: Conference Series
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Analysis of the XENON100 dark matter search data

2014

The XENON100 experiment, situated in the Laboratori Nazionali del Gran Sasso, aims at the direct detection of dark matter in the form of weakly interacting massive particles (WIMPs), based on their interactions with xenon nuclei in an ultra low background dual-phase time projection chamber. This paper describes the general methods developed for the analysis of the XENON100 data. These methods have been used in the 100.9 and 224.6 live days science runs from which results on spin-independent elastic, spin-dependent elastic and inelastic WIMP-nucleon cross-sections have already been reported.

Large Underground Xenon experimentPhysics - Instrumentation and DetectorsXenonWIMPPhysics::Instrumentation and DetectorsDirect detectionDark matterchemistry.chemical_elementFOS: Physical sciencesDarkSideWIMP Argon ProgrammeNuclear physicsXenonDark matterStatistical analysisNuclear ExperimentInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsTime projection chamberAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)WIMPschemistryWeakly interacting massive particlesDark matter; Direct detection; WIMPs; XenonAstrophysics - Instrumentation and Methods for AstrophysicsAstroparticle Physics
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Search for Magnetic Monopoles with the MoEDAL Forward Trapping Detector in 13 TeV Proton-Proton Collisions at the LHC

2017

MoEDAL is designed to identify new physics in the form of long-lived highly-ionising particles produced in high-energy LHC collisions. Its arrays of plastic nuclear-track detectors and aluminium trapping volumes provide two independent passive detection techniques. We present here the results of a first search for magnetic monopole production in 13 TeV proton-proton collisions using the trapping technique, extending a previous publication with 8 TeV data during LHC run-1. A total of 222 kg of MoEDAL trapping detector samples was exposed in the forward region and analysed by searching for induced persistent currents after passage through a superconducting magnetometer. Magnetic charges excee…

Magnetic monopolesProtonMagnetismPhysics beyond the Standard ModelGeneral Physics and Astronomy01 natural sciences7. Clean energyHigh Energy Physics - Experimentlaw.inventionCOLLIDERHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)STOPPING-POWERlawPhysics02 Physical SciencesLarge Hadron ColliderSTABLE MASSIVE PARTICLESPhysicsMagnetismDrell–Yan processhep-phPersistent currents3. Good healthHigh Energy Physics - PhenomenologyPhysical SciencesELECTROWEAK MONOPOLEParticle Physics - ExperimentGeneral PhysicsMagnetometerPhysics MultidisciplinaryMagnetic monopoleFOS: Physical sciencesNuclear track detector114 Physical sciencesNuclear physicsPhysics and Astronomy (all)Tellurium compoundsHigh energy physics Magnetism Magnetometers Highly ionizing particles Magnetic charges Magnetic monopoles Nuclear track detector Passive detection Persistent currents Proton proton collisions Trapping techniques Tellurium compounds0103 physical sciencesHigh energy physics010306 general physicsColliderIONIZING PARTICLESScience & TechnologyProton proton collisionshep-ex010308 nuclear & particles physicsMagnetometers Highly ionizing particlesMagnetic chargesTrapping techniquesPassive detectionSTATES
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