Search results for "space science"

showing 10 items of 56 documents

Search for short baseline nu(e) disappearance with the T2K near detector

2015

8 pages.- 6 figures

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoAstronomy & AstrophysicsNeutrino beam7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physics0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNeutrino oscillation0206 Quantum PhysicsNeutrino fluxPhysicsScience & Technologyhep-ex010308 nuclear & particles physicsPhysicsDetectorT2K experimentNuclear & Particles Physics0201 Astronomical And Space SciencesPhysical Sciences
researchProduct

Recoil-α-fission and recoil-α–α-fission events observed in the reaction 48Ca + 243Am

2016

Products of the fusion-evaporation reaction 48Ca + 243Am were studied with the TASISpec set-up at the gas-filled separator TASCA at the GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany. Amongst the detected thirty correlated α-decay chains associated with the production of element Z=115, two recoil-α-fission and five recoil-α-α-fission events were observed. The latter five chains are similar to four such events reported from experiments performed at the Dubna gas-filled separator, and three such events reported from an experiment at the Berkeley gas-filled separator. The four chains observed at the Dubna gas-filled separator were assigned to start from the 2n-evaporation ch…

Nuclear and High Energy Physicsalpha decayFissionSuperheavy elementschemistry.chemical_elementSuperheavy Elementsnucl-exAtomic01 natural sciences7. Clean energyNuclear physicsParticle and Plasma PhysicsRecoil0103 physical sciencesNuclearElement 115α decayNuclear Experiment010306 general physicsUnunpentiumSpontaneous fissionPhysicsQuantum PhysicsUup010308 nuclear & particles physicsSpontaneous fissionMolecularNuclear & Particles PhysicsSuperheavy elementchemistryDecay chainAlpha decayAstronomical and Space SciencesExcitationNuclear Physics A
researchProduct

Precision calculations of dark matter relic abundance

2019

The dark matter annihilation channels sometimes involve sharp resonances. In such cases the usual momentum averaged approximations for computing the DM abundance may not be accurate. We develop an easily accessible momentum dependent framework for computing the DM abundance accurately and efficiently near such features. We apply the method to the case of a singlet scalar dark matter $s$ interacting with SM through higgs portal $\lambda_{\rm hs}s^2 h^2$ and compare the results with different momentum averaged methods. The accuracy of the latter depend strongly on the strength of the elastic interactions and corrections are large if WIMP has negligible interactions beyond the main annihilatio…

Particle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Dark matterFOS: Physical sciencesKinetic energykosmologia01 natural sciencesStandard ModelMomentumpimeä aineHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciencesphysics of the early universeCOSMIC ABUNDANCES010306 general physicsParticle Physics - PhenomenologyPhysicsdark matter theoryAnnihilation010308 nuclear & particles physicsdark matter experimentsAstronomy and Astrophysicshep-ph115 Astronomy Space scienceHigh Energy Physics - PhenomenologyHiggs bosonastro-ph.COAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Early Universe Higgs dynamics in the presence of the Higgs-inflaton and non-minimal Higgs-gravity couplings

2017

Apparent metastability of the electroweak vacuum poses a number of cosmological questions. These concern evolution of the Higgs field to the current vacuum, and its stability during and after inflation. Higgs-inflaton and non-minimal Higgs-gravity interactions can make a crucial impact on these considerations potentially solving the problems. In this work, we allow for these couplings to be present simultaneously and study their interplay. We find that different combinations of the Higgs-inflaton and non-minimal Higgs-gravity couplings induce effective Higgs mass during and after inflation. This crucially affects the Higgs stability considerations during preheating. In particular, a wide ra…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectHigh Energy Physics::LatticeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Metastability0103 physical sciencesphysics of the early universeinflationparticle physicscosmology connectionELECTROWEAK VACUUM010306 general physicscosmology of theories beyond the SMmedia_commonInflation (cosmology)PhysicsSTABILITY010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsBOSONInflaton115 Astronomy Space scienceUniverseHigh Energy Physics - PhenomenologyHiggs fieldHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Observational signatures of Higgs inflation

2016

We investigate the dependency of Higgs inflation on the non-renormalisable matching between the low energy Standard Model limit and the inflationary regime at high energies. We show that for the top mass range $m_t \gtrsim 171.8$ GeV the scenario robustly predicts the spectral index $n_s \simeq 0.97$ and the tensor-to-scalar ratio $r\simeq 0.003$. The matching is however non-trivial, even the best-fit values $m_h=125.09$ GeV and $m_t=173.21$ GeV require a jump $\delta \lambda \sim 0.01$ in the Higgs coupling below the inflationary scale. For $m_t\lesssim 171.8$ GeV, the matching may generate a feature in the inflationary potential. In this case the predicted values of $n_s$ and $r$ vary but…

Particle physicsMatching (statistics)Cosmology and Nongalactic Astrophysics (astro-ph.CO)STANDARD MODELFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesphysics of the early universeinflationELECTROWEAK VACUUM010306 general physicscosmology of theories beyond the SMBosonInflation (cosmology)PhysicsSpectral index010308 nuclear & particles physicsINDUCED GRAVITY INFLATIONHigh Energy Physics::PhenomenologySpectral densityBOSONAstronomy and Astrophysics115 Astronomy Space scienceHigh Energy Physics - Phenomenologyparticle physics - cosmology connectionJumpHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Measurement of the $\nu_{\mu}$ charged current quasi-elastic cross-section on carbon with the T2K on-axis neutrino beam

2015

17 pages.- 21 figures

Particle physicsNuclear and High Energy Physicschemistry.chemical_elementPion productionAstronomy & AstrophysicsMASSNeutrino beamPION-PRODUCTION7. Clean energy01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - ExperimentNuclear physicsScatteringCross section (physics)0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutron010306 general physicsNeutrino oscillationNuclear Experiment0206 Quantum PhysicsCharged currentPhysicsScience & Technologyhep-ex010308 nuclear & particles physicsScatteringPhysicsDetectorNuclear & Particles PhysicsMODEL0201 Astronomical And Space ScienceschemistryPhysical SciencesHigh Energy Physics::ExperimentNeutrinoCarbonNuclear targets
researchProduct

Measurement of the Top Quark Mass Using the Matrix Element Technique in Dilepton Final States

2016

We present a measurement of the top quark mass in ppbar collisions at a center-of-mass energy of 1.96 TeV at the Fermilab Tevatron collider. The data were collected by the D0 experiment corresponding to an integrated luminosity of 9.7 fb-1. The matrix element technique is applied to ttbar events in the final state containing leptons (electrons or muons) with high transverse momenta and at least two jets. The calibration of the jet energy scale determined in the lepton + jets final state of ttbar decays is applied to jet energies. This correction provides a substantial reduction in systematic uncertainties. We obtain a top quark mass of mt = 173.93 +- 1.84 GeV.

Particle physicsTop quarkCOLLISIONSPAIR PRODUCTIONJET IDENTIFICATIONAstrophysics::High Energy Astrophysical PhenomenaTevatronFOS: Physical sciencesJet (particle physics)Astronomy & Astrophysics01 natural sciencesD0 EXPERIMENTlaw.inventionPhysics Particles & FieldsHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0202 Atomic Molecular Nuclear Particle And Plasma Physicslaw0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]HADRON COLLIDERSFermilabHigh Energy Physics010306 general physicsColliderRUN-IIDETECTOR0206 Quantum PhysicsPhysicsScience & Technology010308 nuclear & particles physicsPhysicsSEMILEPTONIC DECAYSHigh Energy Physics::PhenomenologyD0 experimentNuclear & Particles Physics0201 Astronomical And Space SciencesPair productionPhysical SciencesExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHigh Energy Physics::ExperimentCROSS-SECTIONLepton
researchProduct

Baryogenesis and gravity waves from a UV-completed electroweak phase transition

2021

We study gravity wave production and baryogenesis at the electroweak phase transition, in a real singlet scalar extension of the Standard Model, including vector-like top partners to generate the CP violation needed for electroweak baryogenesis (EWBG). The singlet makes the phase transition strongly first-order through its coupling to the Higgs boson, and it spontaneously breaks CP invariance through a dimension-5 contribution to the top quark mass term, generated by integrating out the heavy top quark partners. We improve on previous studies by incorporating updated transport equations, compatible with large bubble wall velocities. The wall speed and thickness are computed directly from th…

Particle physicsTop quarkCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)FOS: Physical scienceskosmologia01 natural sciences7. Clean energy114 Physical sciencesStandard ModelBaryon asymmetryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsPhysics010308 nuclear & particles physicsGravitational waveHiggsin bosoniElectroweak interactionHigh Energy Physics::Phenomenologyhiukkasfysiikan standardimalligravitaatio115 Astronomy Space scienceBaryogenesisHigh Energy Physics - PhenomenologyHiggs bosongravitaatioaallotAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review
researchProduct

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
researchProduct

The DArk Matter Particle Explorer mission

2017

The DArk Matter Particle Explorer (DAMPE), one of the four scientific space science missions within the framework of the Strategic Pioneer Program on Space Science of the Chinese Academy of Sciences, is a general purpose high energy cosmic-ray and gamma-ray observatory, which was successfully launched on December 17th, 2015 from the Jiuquan Satellite Launch Center. The DAMPE scientific objectives include the study of galactic cosmic rays up to $\sim 10$ TeV and hundreds of TeV for electrons/gammas and nuclei respectively, and the search for dark matter signatures in their spectra. In this paper we illustrate the layout of the DAMPE instrument, and discuss the results of beam tests and calib…

Physics - Instrumentation and DetectorsSatellite launchesGamma ray observatoriesAstrophysicsGalactic cosmic rays01 natural sciencesCosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ObservatoryDetectors and Experimental TechniquesCosmic rays dark matter space experiments010303 astronomy & astrophysicsphysics.ins-detSpace science missionsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)CosmologyCosmology Galaxies Gamma rays Tellurium compounds Chinese Academy of Sciences Dark matter particles Explorer missions Galactic cosmic rays Gamma ray observatories Satellite launches Scientific objectives Space science missions Cosmic raysSpace ScienceAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaParticle Physics - ExperimentAstrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic raydark matterTellurium compounds0103 physical sciencesCosmic raysInstrumentation and Methods for Astrophysics (astro-ph.IM)010308 nuclear & particles physicshep-exGamma raysAstronomyAstronomy and AstrophysicsGalaxiesChinese academy of sciencesGalaxyScientific objectivesDark matter particlesChinese Academy of SciencesSatellitespace experimentsExplorer missionsastro-ph.IM
researchProduct