Search results for "dark matter: mass"

showing 4 items of 4 documents

Search for a Stable Six-Quark State at BABAR

2019

Recent investigations have suggested that the six-quark combination uuddss could be a deeply bound state (S) that has eluded detection so far, and a potential dark matter candidate. We report the first search for a stable, doubly strange six-quark state in Upsilon -> S anti-Lambda anti-Lambda decays based on a sample of 90 million Upsilon(2S) and 110 million Upsilon(3S) decays collected by the BABAR experiment. No signal is observed, and 90% confidence level limits on the combined Upsilon(2S,3S) -> S anti-Lambda anti-Lambda branching fraction in the range (1.2-1.4)x10^-7 are derived for m_S < 2.05 GeV. These bounds set stringent limits on the existence of such exotic particles.

:Kjerne- og elementærpartikkelfysikk: 431 [VDP]branching ratio: upper limitElectron–positron annihilationBound stateGeneral Physics and AstronomyBaBar experimentQuarksUpsilon(10355): rare decayUpsilon(10355): electroproductionUpsilon(10020): branching ratioparticle: exoticupsilon mesons: hadronic decay01 natural sciencesdecayHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Upsilon(10020): electroproductionBound state[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]PhysicQCQBExotic particlesPhysicsnew physics: search forSettore FIS/01 - Fisica Sperimentaleelectron positron: colliding beamsdetector limits decay:Nuclear and elementary particle physics: 431 [VDP]ParticlesDark matter (Astronomy)Confidence levelbaryon: dark matterUpsilon(10020): rare decayBranching fractionMatèria fosca (Astronomia)QuarkParticle physicsDark matterFOS: Physical sciencesLambda: pair productionelectron positron: annihilationPartícules (Matèria)NOPhysics and Astronomy (all)BABAR experiment0103 physical sciencesAtomic physicUpsilon(10355): branching ratio010306 general physicsdetectorBranching fractiondark matter: massState (functional analysis)stabilitySLAC PEP StorHEPA-stableBaBarElementary Particles and FieldsHigh Energy Physics::Experimentlimitsexperimental results
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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 <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>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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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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Dark matter-neutrino interactions through the lens of their cosmological implications

2018

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. The aim of this paper is to determine whether there are viable particle physics frameworks in which dark matter can be coupled to active neutrinos. We use a simplified model approach to determine all possible renormalizable scenarios where there is such a coupling, and study their astrophysical and cosmological signatures. We find that dark matter-neutrino interactions have an impact on structure formation and lead to indirect detection signatures when the coupling between dark matter and neutrinos is …

Particle physicsStructure formationdark matter: interactionPhysics beyond the Standard ModelDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsParameter space01 natural sciencesdark matterdark matter: couplingHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesneutrino: coupling010306 general physicsneutrino: interactionPhysics010308 nuclear & particles physicsnew physicsdark matter: massdark matter: mediationHigh Energy Physics - PhenomenologyCoupling (physics)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Particle[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]NeutrinoDark fluiddark matter: parameter space
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