Search results for "matter [quantum chromodynamics]"

showing 10 items of 162 documents

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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Search for Electronic Recoil Event Rate Modulation with 4 Years of XENON100 Data

2017

We report on a search for electronic recoil event rate modulation signatures in the XENON100 data accumulated over a period of 4 years, from January 2010 to January 2014. A profile likelihood method, which incorporates the stability of the XENON100 detector and the known electronic recoil background model, is used to quantify the significance of periodicity in the time distribution of events. There is a weak modulation signature at a period of $431^{+16}_{-14}$ days in the low energy region of $(2.0-5.8)$ keV in the single scatter event sample, with a global significance of $1.9\,\sigma$, however no other more significant modulation is observed. The expected annual modulation of a dark matt…

Physics and Astronomy (all) XENON DARK MATTER MODULATION TPCPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterGeneral Physics and AstronomyFOS: Physical sciencesElectron01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Recoil0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsPseudovectorInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)Coupling (probability)ModulationAstrophysics - Instrumentation and Methods for AstrophysicsEvent (particle physics)Astrophysics - Cosmology and Nongalactic Astrophysics
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Stellar Wakes from Dark Matter Subhalos

2017

We propose a novel method utilizing stellar kinematic data to detect low-mass substructure in the Milky Way's dark matter halo. By probing characteristic wakes that a passing dark matter subhalo leaves in the phase space distribution of ambient halo stars, we estimate sensitivities down to subhalo masses $\sim 10^7\,M_\odot$ or below. The detection of such subhalos would have implications for dark-matter and cosmological models that predict modifications to the halo-mass function at low halo masses. We develop an analytic formalism for describing the perturbed stellar phase-space distributions, and we demonstrate through simulations the ability to detect subhalos using the phase-space model…

Physics010308 nuclear & particles physicsMilky WayDark matterGeneral Physics and AstronomyAstronomyFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstrophysics - Astrophysics of GalaxiesGalaxyDark matter haloFormalism (philosophy of mathematics)StarsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics of Galaxies (astro-ph.GA)0103 physical sciencesSubstructureHalo010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics
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A fresh look into the interacting dark matter scenario

2018

The elastic scattering between dark matter particles and radiation represents an attractive possibility to solve a number of discrepancies between observations and standard cold dark matter predictions, as the induced collisional damping would imply a suppression of small-scale structures. We consider this scenario and confront it with measurements of the ionization history of the Universe at several redshifts and with recent estimates of the counts of Milky Way satellite galaxies. We derive a conservative upper bound on the dark matter-photon elastic scattering cross section of $\sigma_{\gamma \rm{DM}} < 8 \times 10^{-10} \, \sigma_T \, \left(m_{\rm DM}/{\rm GeV}\right)$ at $95\%$~CL, abou…

PhysicsConservation lawCosmology and Nongalactic Astrophysics (astro-ph.CO)Photondark matter theory010308 nuclear & particles physicsDark matterFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxydwarfs galaxiesparticle physics-cosmology connection13. Climate actionIonization0103 physical sciencesreionizationSatellite010303 astronomy & astrophysicsReionizationAstrophysics - Cosmology and Nongalactic Astrophysics
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Sub-MeV dark matter and the Goldstone modes of superfluid helium

2019

We show how the relativistic effective field theory for the superfluid phase of helium-4 can replace the standard methods used to compute the production rates of low momentum excitations due to the interaction with an external probe. This is done by studying the scattering problem of a light dark matter particle in the superfluid, and comparing to some existing results. We show that the rate of emission of two phonons, the Goldstone modes of the effective theory, gets strongly suppressed for sub-MeV dark matter particles due to a fine cancellation between two different tree-level diagrams in the limit of small exchanged momenta. This phenomenon is found to be a consequence of the particular…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhononDark matterFOS: Physical sciencesdark matter detection01 natural sciencesHigh Energy Physics - ExperimentSuperfluidityMomentumHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)effective quantum field theoriesHigh Energy Physics - Phenomenology (hep-ph)Orders of magnitude (time)dark matter detection; effective quantum field theoriesQuantum electrodynamics0103 physical sciencesEffective field theory010306 general physicsLight dark matterSuperfluid helium-4Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Aidnogenesis via Leptogenesis and Dark Sphalerons

2010

We discuss aidnogenesis, the generation of a dark matter asymmetry via new sphaleron processes associated to an extra non-abelian gauge symmetry common to both the visible and the dark sectors. Such a theory can naturally produce an abundance of asymmetric dark matter which is of the same size as the lepton and baryon asymmetries, as suggested by the similar sizes of the observed baryonic and dark matter energy content, and provide a definite prediction for the mass of the dark matter particle. We discuss in detail a minimal realization in which the Standard Model is only extended by dark matter fermions which form "dark baryons" through an SU(3) interaction, and a (broken) horizontal symme…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsParticle physicsmedia_common.quotation_subjectDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaAstrophysics::Cosmology and Extragalactic AstrophysicsAsymmetrySphaleronStandard ModelDark matter haloBaryonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)LeptogenesisAnomaly (physics)Astrophysics - High Energy Astrophysical Phenomenamedia_common
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Update on decaying and annihilating heavy dark matter with the 6-year IceCube HESE data

2019

In view of the IceCube's 6-year high-energy starting events (HESE) sample, we revisit the possibility that the updated data may be better explained by a combination of neutrino fluxes from dark matter decay and an isotropic astrophysical power-law than purely by the latter. We find that the combined two-component flux qualitatively improves the fit to the observed data over a purely astrophysical one, and discuss how these updated fits compare against a similar analysis done with the 4-year HESE data. We also update fits involving dark matter decay via multiple channels, without any contribution from the astrophysical flux. We find that a DM-only explanation is not excluded by neutrino data…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)dark matter theoryultra high energy photons and neutrinos010308 nuclear & particles physicsIsotropyDark matterFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)13. Climate action0103 physical sciencesNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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The degenerate gravitino scenario

2010

In this work, we explore the "degenerate gravitino" scenario where the mass difference between the gravitino and the lightest MSSM particle is much smaller than the gravitino mass itself. In this case, the energy released in the decay of the next to lightest sypersymmetric particle (NLSP) is reduced. Consequently the cosmological and astrophysical constraints on the gravitino abundance, and hence on the reheating temperature, become softer than in the usual case. On the other hand, such small mass splittings generically imply a much longer lifetime for the NLSP. We find that, in the constrained MSSM (CMSSM), for neutralino LSP or NLSP, reheating temperatures compatible with thermal leptogen…

PhysicsHigh Energy Physics - TheoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Supersymmetry and cosmologyDegenerate energy levelsDark matter theoryHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and AstrophysicsCosmology of Theories beyond the SMGeneral Relativity and Quantum CosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)LeptogenesisThermalNeutralinoLeptogenesisGravitinoHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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Geometry, pregeometry and beyond

2005

This article explores the overall geometric manner in which human beings make sense of the world around them by means of their physical theories; in particular, in what are nowadays called pregeometric pictures of Nature. In these, the pseudo-Riemannian manifold of general relativity is considered a flawed description of spacetime and it is attempted to replace it by theoretical constructs of a different character, ontologically prior to it. However, despite its claims to the contrary, pregeometry is found to surreptitiously and unavoidably fall prey to the very mode of description it endeavours to evade, as evidenced in its all-pervading geometric understanding of the world. The question r…

PhysicsHistorySpacetimeGeneral relativityMode (statistics)General Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Matter of factGeneral Relativity and Quantum CosmologyEpistemologyComprehensionCharacter (mathematics)Pregeometry (physics)History and Philosophy of ScienceMeaning (existential)
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Connection between certain massive and massless diagrams

1996

A useful connection between two-loop massive vacuum integrals and one-loop off-shell triangle diagrams with massless internal particles is established for arbitrary values of the space-time dimension {ital n}. {copyright} {ital 1996 The American Physical Society.}

PhysicsNuclear and High Energy PhysicsComputer Science::Information RetrievalSpace timeDimension (graph theory)Massive particlePropagatorMatter creationMassless particlesymbols.namesakeQuantum mechanicssymbolsFeynman diagramConnection (algebraic framework)Mathematical physicsPhysical Review D
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