Search results for " dark"

showing 10 items of 212 documents

Significant divergences between the temporal structure of the behavior in Wistar and in the spontaneously more anxious DA/Han strain of rats tested i…

2013

Abstract The aim of present research is to study the temporal structure of the behavior in two strains of rats with different basal level of emotionality. To this purpose, the temporal profile of the behavior in Wistar rat and in the spontaneously more anxious DA/Han strain was analyzed in the Elevated Plus Maze. Both quantitative and multivariate t-pattern analyses were carried out. In comparison with Wistar, DA/Han subjects showed a significant reduction of the permanence in open arm and a significant increase of the time spent in the central platform of the maze. Mean frequencies of each behavioral element showed significant modifications both in open and in closed arm. Multivariate t-pa…

MaleElevated plus mazemedicine.medical_specialty[ SCCO.PSYC ] Cognitive science/PsychologyAnxietySettore BIO/09 - FisiologiaRats Mutant StrainsTemporal lobeDevelopmental psychologyRats Sprague-Dawley03 medical and health sciencesBehavioral NeuroscienceBasal (phylogenetics)0302 clinical medicineSpecies SpecificityEmotionalityInternal medicinemedicineAnimalsStatistical analysisRats WistarMaze LearningComputingMilieux_MISCELLANEOUSStrain (chemistry)[SCCO.NEUR]Cognitive science/NeuroscienceAnxiety Elevated plus maze t-pattern analysis Multivariate analysis Wistar Dark Agouti RatRats030227 psychiatryEndocrinology[ SCCO.NEUR ] Cognitive science/NeuroscienceMultivariate Analysis[SCCO.PSYC]Cognitive science/PsychologyTime courseExploratory BehaviorTemporal organizationPsychology030217 neurology & neurosurgery
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Zvaigžņotā Debess: 2010, Vasara (208)

2010

Contents: N.Cimahoviča. Sun’s Researcher in the Far East ; A.Balklavs. A New Hypothesis on Formation of Galaxies ; A.Balklavs. Gravitation and Peculiar Galaxies ; A.Barzdis. First Population Stars and Galaxies ; Z.Alksne, A.Alksnis. Does Giant Planet Orbit Dwarf Star? ; A.Alksnis, Z.Alksne. Epsilon Aurigae Eclipsed by Dark Dust Disk ; M.Ābele, K.Adgere, E.Grabs, L.Osipova, E.Rutkovska, J.Vjaters, V.Veckalns. Latvian Students Take Part in the Project European Student Moon Orbiter ; Announcement on the 3rd International Symposium on Dark-Sky Parks: 6-10 September 2010, Croatia ; J.Jansons. Vladimir Afanasjev – Officer of the Baikonur Cosmodrom in the 1970s ; J.Limansky. The International Year…

Milzu planēta ap pundurzvaigzniStarptautiskā vasaras skola Rozhen BulgārijāViduslaiki un zinātneVaris Karitāns – SPIE stipendijaArturs Balklavs “Latvijas astronomija pēc Trešās atmodas”Latvijas studenti ESMO projektāAstrofest 2010KristietībaPirmās paaudzes zvaigznes galaktikasSaules Dinamikas observatorijaAstronomijas vēsture – Rīgas kalendāriPasaules iekārtojums Raiņa dzejāLatvijas astronomija - vēstureMārtiņs Gills – Artura Balklava balvaLeonids Roze (20.05.1925. – 1.06.2009.)Starptautiskais simpozijs Dark-Sky Parks HorvātijāPirmie cilvēki kosmosā – pastmarkasMarss – gaismas naktīVedēja Epsilona aptumsumsAstronomiskie novērojumiStarptautiskais astronomijas gads 2009 filatēlijā – sērija EUROPAAstronomiskās parādības - 2010Baikonuras kosmodroma virsnieks Vladimirs AfanasjevsAstrofiziķis Uldis Dzērvīte – 75 gadiRozeta – Lutēcija
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Systematic uncertainties from halo asphericity in dark matter searches

2015

Although commonly assumed to be spherical, dark matter halos are predicted to be non-spherical by N-body simulations and their asphericity has a potential impact on the systematic uncertainties in dark matter searches. The evaluation of these uncertainties is the main aim of this work, where we study the impact of aspherical dark matter density distributions in Milky-Way-like halos on direct and indirect searches. Using data from the large N-body cosmological simulation Bolshoi, we perform a statistical analysis and quantify the systematic uncertainties on the determination of local dark matter density and the so-called $J$ factors for dark matter annihilations and decays from the galactic …

N-body SimulationsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Milky WayDwarf galaxy problemDark matterScalar field dark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesMany-body problemHigh Energy Physics - Phenomenology (hep-ph)Baryonic dark matter0103 physical sciencesDark matter010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsPotential impactAnnihilation010308 nuclear & particles physicsHot dark matterGalactic CenterAstronomyAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxiestriaxial halosDark matter haloHigh Energy Physics - Phenomenology13. Climate actionAstrophysics of Galaxies (astro-ph.GA)Cuspy halo problemHaloDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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First Results on the Scalar WIMP-Pion Coupling, Using the XENON1T Experiment

2018

We present first results on the scalar coupling of weakly interacting massive particles (WIMPs) to pions from 1 t yr of exposure with the XENON1T experiment. This interaction is generated when the WIMP couples to a virtual pion exchanged between the nucleons in a nucleus. In contrast to most nonrelativistic operators, these pion-exchange currents can be coherently enhanced by the total number of nucleons and therefore may dominate in scenarios where spin-independent WIMP-nucleon interactions are suppressed. Moreover, for natural values of the couplings, they dominate over the spin-dependent channel due to their coherence in the nucleus. Using the signal model of this new WIMP-pion channel, …

Nuclear TheoryPhysics::Instrumentation and DetectorsNuclear TheoryGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMPPions[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentS030UDMPhysicsStarke Wechselwirkung und exotische Kerne – Abteilung BlaumAstrophysics::Instrumentation and Methods for AstrophysicsnucleonsuppressionHigh Energy Physics - PhenomenologyWeakly interacting massive particlesmedicine.anatomical_structureWeakly interacting massive particlesNucleonCoherence (physics)Astrophysics - Cosmology and Nongalactic AstrophysicsWIMP nucleon: interactionParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]FOS: Physical sciencesWIMP: massspin: dependenceGravitation and Astrophysicsoperator: nonrelativisticDark matter Particle dark matter Pions Weakly interacting massive particles Dark matter detectorsNuclear Theory (nucl-th)PionParticle dark matter0103 physical sciencesmedicineDark mattercross section: upper limit010306 general physicsCouplingDark matter detectorsnucleusScalar (physics)coherenceDark Matter WIMP-Pion coupling Xenon Direct seartch[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Nucleus
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Search for dark matter from the Galactic halo with the IceCube neutrino telescope

2011

Self-annihilating or decaying dark matter in the Galactic halo might produce high energy neutrinos detectable with neutrino telescopes. We have conducted a search for such a signal using 276 days of data from the IceCube 22-string configuration detector acquired during 2007 and 2008. The effect of halo model choice in the extracted limit is reduced by performing a search that considers the outer halo region and not the Galactic Center. We constrain any large-scale neutrino anisotropy and are able to set a limit on the dark matter self-annihilation cross section of ⟨σAv⟩≃10-22 cm3 s-1 for weakly interacting massive particle masses above 1 TeV, assuming a monochromatic neutrino line spectrum.

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesIceCubeGalactic halo0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsGamma-Ray EmissionHot dark matterAstronomyCosmic-Rays004Dark matter haloParticlesNeutrino detectorAnisotropyHigh Energy Physics::ExperimentHaloDwarf Spheroidal GalaxiesNeutrinoNeutrino astronomyinfo:eu-repo/classification/ddc/004
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The DAMPE silicon–tungsten tracker

2016

Abstract The DArk Matter Particle Explorer (DAMPE) is a spaceborne astroparticle physics experiment, launched on 17 December 2015. DAMPE will identify possible dark matter signatures by detecting electrons and photons in the 5 GeV–10 TeV energy range. It will also measure the flux of nuclei up to 100 TeV, for the study of the high energy cosmic ray origin and propagation mechanisms. DAMPE is composed of four sub-detectors: a plastic strip scintillator, a silicon–tungsten tracker–converter (STK), a BGO imaging calorimeter and a neutron detector. The STK is composed of six tracking planes of 2 orthogonal layers of single-sided micro-strip detectors, for a total detector surface of ca. 7 m2. T…

Nuclear and High Energy PhysicsCosmic rays; Dark matter; Silicon tracker; Spaceborne experiment; Nuclear and High Energy Physics; InstrumentationPhysics::Instrumentation and DetectorsCosmic rayParticle detectorsTracking (particle physics)01 natural sciencesParticle detectorOpticscosmic rays0103 physical sciencesDark matterNeutron detection010303 astronomy & astrophysicsInstrumentationAstroparticle physicsPhysicsLarge Hadron ColliderCalorimeter (particle physics)010308 nuclear & particles physicsbusiness.industryDetectorSettore FIS/01 - Fisica SperimentaleParticle detectors cosmic raysSpaceborne experimentSilicon trackerHigh Energy Physics::Experimentbusiness
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Search for the dark photon in π0 decays

2015

A sample of $1.69\times 10^7$ fully reconstructed $\pi^0\to\gamma e^+e^-$ decay candidates collected by the NA48/2 experiment at CERN in 2003--2004 is analysed to search for the dark photon ($A'$) production in the $\pi^0\to\gamma A'$ decay followed by the prompt $A'\to e^+e^-$ decay. No signal is observed, and an exclusion region in the plane of the dark photon mass $m_{A'}$ and mixing parameter $\varepsilon^2$ is established. The obtained upper limits on $\varepsilon^2$ are more stringent than the previous limits in the mass range $9~{\rm MeV}/c^2<m_{A'}<70~{\rm MeV}/c^2$. The NA48/2 sensitivity to the dark photon production in the $K^\pm\to\pi^\pm A'$ decay is also evaluated.

Nuclear and High Energy PhysicsDark matterKAON DECAYSSocio-culturaleAstronomy & Astrophysics01 natural sciencesDark photondark matterHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physics0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciencesdark matter meson decays010306 general physicsDETECTORPhysicsNuclear and High Energy Physics dark photon photon pion neutral pionneutral pionRange (particle radiation)Large Hadron ColliderScience & Technology010308 nuclear & particles physicsPhysicsphotonDark Photon; KAON DECAYSpionmeson decaysNuclear & Particles Physicslcsh:QC1-999Physics NuclearPhysical Sciencesdark photonFotoneHigh Energy Physics::ExperimentParticle Physics - Experimentlcsh:PhysicsHigh Energy Physics - Experiment; Dark Photon
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A search for neutron to mirror-neutron oscillations using the nEDM apparatus at PSI

2021

It has been proposed that there could be a mirror copy of the standard model particles, restoring the parity symmetry in the weak interaction on the global level. Oscillations between a neutral standard model particle, such as the neutron, and its mirror counterpart could potentially answer various standing issues in physics today. Astrophysical studies and terrestrial experiments led by ultracold neutron storage measurements have investigated neutron to mirror-neutron oscillations and imposed constraints on the theoretical parameters. Recently, further analysis of these ultracold neutron storage experiments has yielded statistically significant anomalous signals that may be interpreted as …

Nuclear and High Energy PhysicsNeutron electric dipole momentmedia_common.quotation_subjectmagnetic fieldWeak interaction[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Astronomy & Astrophysics01 natural sciences7. Clean energyAsymmetryrotationPhysics Particles & FieldsELECTRIC-DIPOLE MOMENTweak interaction0103 physical sciencesDark matterDARK-MATTERNeutron010306 general physicsnumerical calculationsmirrorNuclear mattermedia_commonoscillation: timePhysicsn: electric momentProperties of neutrons Ultracold neutrons Nuclear matter Mirror matter Dark matter Particle symmetriesScience & TechnologyProperties of neutronsParticle symmetries010308 nuclear & particles physicsparity: symmetryPhysicsNuclear matter[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]lcsh:QC1-999Mirror matterMagnetic fieldMODELPhysics Nuclear[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Physical SciencesUltracold neutronsAtomic physicsUltracold neutronsMirror matterasymmetrylcsh:PhysicsPhysics Letters B
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The Hunt for New Physics at the Large Hadron Collider

2010

233 páginas.-- AHEP Group: et al..-- El Pdf del artículo es la versión pre-print: arXiv.1001.2693v1.-- Trabajo presentado al "The International Workshop on Beyond the Standard Model Physics and LHC Signatures (BSM-LHC) celebrado en Boston (USA) del 2 al 4 de junio de 2009.

Nuclear and High Energy PhysicsParticle physicsCold dark matterPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelFOS: Physical sciencesRANDALL-SUNDRUM MODEL01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)R-PARITY BREAKING0103 physical sciencesHigh Energy PhysicsANOMALOUS MAGNETIC-MOMENT010306 general physicsParticle Physics - PhenomenologyPhysicsEXPLICIT CP VIOLATIONDARK-MATTER DETECTIONLarge Hadron Collider010308 nuclear & particles physicsPhysicsElectroweak interactionHigh Energy Physics::PhenomenologyFísicaRENORMALIZATION-GROUP EQUATIONSHierarchy problemSupersymmetryAtomic and Molecular Physics and OpticsGRAND UNIFIED THEORIESSUPERSYMMETRIC STANDARD MODELHidden sectorExtra dimensionsHigh Energy Physics - PhenomenologyMINIMAL FLAVOR VIOLATION[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]PhenomenologyHigh Energy Physics::ExperimentHIGGS-BOSON PRODUCTION
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Direct and indirect singlet scalar dark matter detection in the lepton-specific two-Higgs-doublet model

2011

A recent study of gamma-ray data from the Galactic Center motivates the investigation of light (~7-10 GeV) particle dark matter models featuring tau lepton pairs as dominant annihilation final state. The Lepton-Specific two-Higgs-doublet Model (2HDM-L) provides a natural framework where light, singlet scalar dark matter can pair-annihilate dominantly into tau leptons. We calculate the nucleon-dark matter cross section for singlet scalar dark matter within the 2HDM-L framework, and compare with recent results from direct detection experiments. We study how direct dark matter searches can be used to constrain the dark matter interpretation of gamma ray observations, for different dominant ann…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaDark matterScalar field dark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesNuclear physicsTwo-Higgs-doublet modelHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsLight dark matterHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHot dark matterHigh Energy Physics::PhenomenologyHigh Energy Physics - PhenomenologyWeakly interacting massive particlesAstrophysics - High Energy Astrophysical PhenomenaDark fluidAstrophysics - Cosmology and Nongalactic AstrophysicsLeptonPhysical Review D
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