Search results for "QB"

showing 10 items of 522 documents

Spontaneous baryogenesis in spiral inflation

2019

We examined the possibility of spontaneous baryogenesis driven by the inflaton in the scenario of spiral inflation, and found the parametric dependence of the late-time baryon number asymmetry. As a result, it is shown that, depending on the effective coupling of baryon/lepton number violating operators, it is possible to obtain the right amount of asymmetry even in the presence of a matter-domination era as long as such era is relatively short. In a part of the parameter space, the required expansion rate during inflation is close to the current upper-bound, and hence can be probed in the near future experiments.

Particle physicsPhysics and Astronomy (miscellaneous)media_common.quotation_subjectFOS: Physical scienceslcsh:AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsParameter space01 natural sciencesAsymmetryHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)media_commonInflation (cosmology)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyInflatonLepton numberBaryonBaryogenesisHigh Energy Physics - Phenomenologylcsh:QC770-798Baryon numberEuropean Physical Journal C: Particles and Fields
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Cosmology and CPT violating neutrinos

2017

The combination Charge Conjugation-Parity-Time Reversal(CPT) is a fundamental symmetry in our current understanding of nature. As such, testing CPT violation is a strongly motivated path to explore new physics. In this paper we study CPT violation in the neutrino sector, giving for the first time a bound, for a fundamental particle, in the CPT violating particle-antiparticle gravitational mass difference. We argue that cosmology is nowadays the only data sensitive to CPT violation for the neutrino-antineutrino mass splitting and we use the latest data release from Planck combined with the current Baryonic-Acoustic-Oscillation measurement to perform a full cosmological analysis. To show the …

Particle physicsPhysics::General PhysicsPhysics and Astronomy (miscellaneous)Physics beyond the Standard ModelFOS: Physical sciencesElementary particlelcsh:Astrophysics7. Clean energy01 natural sciencesCosmologyGravitationsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. RadioactivityPlanck010306 general physics010303 astronomy & astrophysicsEngineering (miscellaneous)PhysicsHigh Energy Physics::PhenomenologyCharge (physics)Symmetry (physics)High Energy Physics - Phenomenologysymbolslcsh:QC770-798High Energy Physics::ExperimentNeutrino
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Icecube/DeepCore tests for novel explanations of the MiniBooNE anomaly

2019

While the low-energy excess observed at MiniBooNE remains unchallenged, it has become increasingly difficult to reconcile it with the results from other sterile neutrino searches and cosmology. Recently, it has been shown that non-minimal models with new particles in a hidden sector could provide a better fit to the data. As their main ingredients they require a GeV-scale $Z'$, kinetically mixed with the photon, and an unstable heavy neutrino with a mass in the 150 MeV range that mixes with the light neutrinos. In this letter we point out that atmospheric neutrino experiments (and, in particular, IceCube/DeepCore) could probe a significant fraction of the parameter space of such models by l…

Particle physicsSterile neutrinoPhotonPhysics and Astronomy (miscellaneous)FOS: Physical scienceslcsh:AstrophysicsParameter space01 natural sciencesCosmologyHigh Energy Physics - ExperimentMiniBooNEHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)lcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHidden sectorHigh Energy Physics - Phenomenologylcsh:QC770-798High Energy Physics::ExperimentAnomaly (physics)NeutrinoThe European Physical Journal C
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Anisotropies and magnetic phase transitions in insulating antiferromagnets determined by a Spin-Hall magnetoresistance probe

2019

Antiferromagnets possess a number of intriguing and promising properties for electronic devices, which include a vanishing net magnetic moment and thus insensitivity to large magnetic fields and characteristic terahertz frequency dynamics. However, probing the antiferromagnetic ordering is challenging without synchrotron-based facilities. Here, we determine the material parameters of the insulating iron oxide hematite, α-Fe2O3, using the surface sensitive spin-Hall magnetoresistance (SMR). Combined with a simple analytical model, we extract the antiferromagnetic anisotropies and the bulk Dzyaloshinskii-Moriya field over a wide range of temperatures and magnetic fields. Across the Morin phas…

Phase transitionMaterials scienceMagnetoresistanceQC1-999General Physics and AstronomyFOS: Physical sciencesLarge scale facilities for research with photons neutrons and ionslcsh:Astrophysics02 engineering and technologyPhysics and Astronomy(all)Astrophysics01 natural sciences0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)lcsh:QB460-466Antiferromagnetism010306 general physicsSpin (physics)AnisotropySpin-½Magnetic momentCondensed matter physicsCondensed Matter - Mesoscale and Nanoscale PhysicsPhysics021001 nanoscience & nanotechnologyMagnetic susceptibilitylcsh:QC1-999Magnetic fieldQB460-466Condensed Matter::Strongly Correlated Electrons0210 nano-technologylcsh:Physics
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Interlayer exciton dynamics in van der Waals heterostructures

2019

Atomically thin transition metal dichalcogenides can be stacked to van der Waals heterostructures enabling the design of new materials with tailored properties. The strong Coulomb interaction gives rise to interlayer excitons, where electrons and holes are spatially separated in different layers. In this work, we reveal the time- and momentum-dependent elementary processes behind the formation, thermalization and photoemission of interlayer excitons for the exemplary MoSe2–WSe2 heterostructure. We identify tunneling of holes from MoSe2 to WSe2 on a ps timescale as the crucial process for interlayer exciton formation. We also predict a drastic reduction of the formation time as a function of…

PhotoluminescenceMaterials scienceOscillator strengthExcitonStackingGeneral Physics and Astronomylcsh:Astrophysics02 engineering and technologyElectron01 natural sciencesCondensed Matter::Materials ScienceCondensed Matter::Superconductivity0103 physical scienceslcsh:QB460-466two-dimensional materials010306 general physicsQuantum tunnellingCondensed matter physicsHeterojunction021001 nanoscience & nanotechnologyCondensed Matter::Mesoscopic Systems and Quantum Hall Effectlcsh:QC1-999ThermalisationCondensed Matter::Strongly Correlated Electrons0210 nano-technologylcsh:Physics
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The liquid-argon scintillation pulseshape in DEAP-3600

2020

AbstractDEAP-3600 is a liquid-argon scintillation detector looking for dark matter. Scintillation events in the liquid argon (LAr) are registered by 255 photomultiplier tubes (PMTs), and pulseshape discrimination (PSD) is used to suppress electromagnetic background events. The excellent PSD performance of LAr makes it a viable target for dark matter searches, and the LAr scintillation pulseshape discussed here is the basis of PSD. The observed pulseshape is a combination of LAr scintillation physics with detector effects. We present a model for the pulseshape of electromagnetic background events in the energy region of interest for dark matter searches. The model is composed of (a) LAr scin…

PhotomultiplierPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsDark matterFOS: Physical scienceslcsh:AstrophysicsScintillatorWavelength shifter01 natural sciencesParticle detectorDEAPOptics0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)PhysicsScintillation010308 nuclear & particles physicsbusiness.industryInstrumentation and Detectors (physics.ins-det)Scintillation counterlcsh:QC770-798businessEuropean Physical Journal C: Particles and Fields
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Bounds on mixed state entanglement

2020

In the general framework of d 1 &times

Physical systemFOS: Physical sciencesGeneral Physics and Astronomylcsh:AstrophysicsQuantum entanglementCharacterization (mathematics)01 natural sciencesArticle010305 fluids & plasmas[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical scienceslcsh:QB460-466negativityStatistical physics010306 general physicslcsh:ScienceQuantumThermal entanglementPhysicsQuantum PhysicsState (functional analysis)lcsh:QC1-999Bipartite graphComputer Science::Programming Languageslcsh:QQuantum Physics (quant-ph)entanglementlcsh:PhysicsCurse of dimensionality
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First operation of the KATRIN experiment with tritium

2020

AbstractThe determination of the neutrino mass is one of the major challenges in astroparticle physics today. Direct neutrino mass experiments, based solely on the kinematics of $$\upbeta $$β-decay, provide a largely model-independent probe to the neutrino mass scale. The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to directly measure the effective electron antineutrino mass with a sensitivity of $$0.2\hbox { eV}$$0.2eV ($$90\%$$90% CL). In this work we report on the first operation of KATRIN with tritium which took place in 2018. During this commissioning phase of the tritium circulation system, excellent agreement of the theoretical prediction with the recorded spectra was …

Physics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsFOS: Physical scienceslcsh:Astrophysics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]TritiumKATRIN01 natural sciencesantineutrino/e: massHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)lcsh:QB460-4660103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]lcsh:Nuclear and particle physics. Atomic energy. RadioactivityMass scaleddc:530Electron Capture[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)010306 general physicsEngineering (miscellaneous)Nuclear ExperimentAstroparticle physicsPhysics010308 nuclear & particles physicstritiumPhysicsQuímicaInstrumentation and Detectors (physics.ins-det)sensitivityddc:lcsh:QC770-798TritiumHigh Energy Physics::ExperimentNeutrinoPräzisionsexperimente - Abteilung BlaumNeutrino Mass[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Electron neutrinoperformanceKATRINAstrophysics - Cosmology and Nongalactic Astrophysicsexperimental results
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Material radioassay and selection for the XENON1T dark matter experiment

2017

The XENON1T dark matter experiment aims to detect weakly interacting massive particles (WIMPs) through low-energy interactions with xenon atoms. To detect such a rare event necessitates the use of radiopure materials to minimize the number of background events within the expected WIMP signal region. In this paper we report the results of an extensive material radioassay campaign for the XENON1T experiment. Using gamma-ray spectroscopy and mass spectrometry techniques, systematic measurements of trace radioactive impurities in over one hundred samples within a wide range of materials were performed. The measured activities allowed for stringent selection and placement of materials during the…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsDark matterMonte Carlo methodmeasurement methodsFOS: Physical scienceschemistry.chemical_elementRadiopuritylcsh:AstrophysicsWIMP: detectorSciences de l'ingénieur01 natural sciencesgamma ray: energy spectrumNuclear physicsmass spectrumXENONXenonWIMPlcsh:QB460-4660103 physical sciencesDark Matterlcsh:Nuclear and particle physics. Atomic energy. Radioactivity[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsSpectroscopy[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Engineering (miscellaneous)background: radioactivityPhysicsRange (particle radiation)Physique010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)AstronomiesensitivitychemistryWeakly interacting massive particleslcsh:QC770-798TPCnumerical calculations: Monte Carlo
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Cosmic-ray muon flux at Canfranc Underground Laboratory

2019

Residual flux and angular distribution of high-energy cosmic muons have been measured in two underground locations at the Canfranc Underground Laboratory (LSC) using a dedicated Muon Monitor. The instrument consists of three layers of fast scintillation detector modules operating as 352 independent pixels. The monitor has flux-defining area of 1 m${}^{2}$, covers all azimuth angles, and zenith angles up to $80^\circ$. The measured integrated muon flux is $(5.26 \pm 0.21) \times 10^{-3}$ m${}^{-2}$s${}^{-1}$ in the Hall A of the LAB2400 and $(4.29 \pm 0.17) \times 10^{-3}$ m${}^{-2}$s${}^{-1}$ in LAB2500. The angular dependence is consistent with the known profile and rock density of the sur…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsFOS: Physical sciencesFluxlcsh:AstrophysicsCosmic rayApplied Physics (physics.app-ph)hiukkasfysiikkaScintillator01 natural sciencesNuclear physicslcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010303 astronomy & astrophysicsEngineering (miscellaneous)ZenithPhysicsMuon010308 nuclear & particles physicsCanfranc Underground LaboratoryPhysics - Applied PhysicsInstrumentation and Detectors (physics.ins-det)Azimuthilmaisimethigh-energy cosmic muonsMuon fluxlcsh:QC770-798High Energy Physics::Experimentkosminen säteily
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