Search results for "COSMIC"

showing 10 items of 656 documents

Revisiting cosmological bounds on sterile neutrinos

2014

We employ state-of-the art cosmological observables including supernova surveys and BAO information to provide constraints on the mass and mixing angle of a non-resonantly produced sterile neutrino species, showing that cosmology can effectively rule out sterile neutrinos which decay between BBN and the present day. The decoupling of an additional heavy neutrino species can modify the time dependence of the Universe's expansion between BBN and recombination and, in extreme cases, lead to an additional matter-dominated period; while this could naively lead to a younger Universe with a larger Hubble parameter, it could later be compensated by the extra radiation expected in the form of neutri…

Sterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic microwave backgroundCosmic background radiationFOS: Physical sciencesNeutrino decouplingAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaAstronomy and Astrophysicshep-phUniverseHigh Energy Physics - Phenomenology13. Climate actionsymbolsastro-ph.COHigh Energy Physics::ExperimentBaryon acoustic oscillationsNeutrinoHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Cosmological origin of anomalous radio background

2012

The ARCADE 2 collaboration has reported a significant excess in the isotropic radio background, whose homogeneity cannot be reconciled with clustered sources. This suggests a cosmological origin prior to structure formation. We investigate several potential mechanisms and show that injection of relativistic electrons through late decays of a metastable particle can give rise to the observed excess radio spectrum through synchrotron emission. However, constraints from the cosmic microwave background (CMB) anisotropy, on injection of charged particles and on the primordial magnetic field, present a challenge. The simplest scenario is with a greater than or similar to 9 GeV particle decaying i…

Structure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaDark matterCosmic microwave backgroundCosmic background radiationFOS: Physical sciencesAstrophysicsElectronAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesParticle decayHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsPhysicsdark matter theory010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsCosmology of Theories beyond the SMRedshiftCharged particleHigh Energy Physics - Phenomenologyextragalactic magnetic fieldsAstrophysics - Cosmology and Nongalactic Astrophysics
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Structure finding in cosmological simulations: the state of affairs

2013

The ever increasing size and complexity of data coming from simulations of cosmic structure formation demands equally sophisticated tools for their analysis. During the past decade, the art of object finding in these simulations has hence developed into an important discipline itself. A multitude of codes based upon a huge variety of methods and techniques have been spawned yet the question remained as to whether or not they will provide the same (physical) information about the structures of interest. Here we summarize and extent previous work of the "halo finder comparison project": we investigate in detail the (possible) origin of any deviations across finders. To this extent we decipher…

Structure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)Ciencias FísicasDark matterFOS: Physical sciencesAstrophysicsGALAXIES HALOESAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences//purl.org/becyt/ford/1 [https]0103 physical sciencesGalaxy formation and evolutionStatistical physics010303 astronomy & astrophysicsGalaxy rotation curveComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]COSMIC cancer database010308 nuclear & particles physicsAstronomy and AstrophysicsObservable//purl.org/becyt/ford/1.3 [https]AstronomíaGravitational lensSpace and Planetary ScienceLUMINOSITY FUNCTIONHaloGALAXIES EVOLUTION[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]CIENCIAS NATURALES Y EXACTASAstrophysics - Cosmology and Nongalactic AstrophysicsGALAXIES STATISTICS
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Late decaying 2-component dark matter scenario as an explanation of the AMS-02 positron excess

2016

The long standing anomaly in the positron flux as measured by the PAMELA and AMS-02 experiments could potentially be explained by dark matter (DM) annihilations. This scenario typically requires a large "boost factor" to be consistent with a thermal relic dark matter candidate produced via freeze-out. However, such an explanation is disfavored by constraints from CMB observations on energy deposition during the epoch of recombination. We discuss a scenario called late-decaying two-component dark matter (LD2DM), where the entire DM consists of two semi-degenerate species. Within this framework, the heavier species is produced as a thermal relic in the early universe and decays to the lighter…

Structure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)Satellitesmedia_common.quotation_subjectPhysics beyond the Standard ModelCosmic microwave backgroundDark matterCosmic background radiationFOS: Physical sciencesAnnihilationAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsDark Matter TheoryGalactic Cosmic-Rays01 natural sciencesCosmic Ray ExperimentsParticle Physics - Cosmology ConnectionHigh Energy Physics - Phenomenology (hep-ph)AbundanceReionization0103 physical sciencesGamma010303 astronomy & astrophysicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilation010308 nuclear & particles physicsAstronomy and AstrophysicsGalaxiesUniverseHaloesHigh Energy Physics - PhenomenologySolar ModulationConstraintsDark AgesMinimumAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsIndraStra Global
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Commissioning of the ATLAS Muon Spectrometer with cosmic rays

2010

The ATLAS detector at the Large Hadron Collider has collected several hundred million cosmic ray events during 2008 and 2009. These data were used to commission the Muon Spectrometer and to study the performance of the trigger and tracking chambers, their alignment, the detector control system, the data acquisition and the analysis programs. We present the performance in the relevant parameters that determine the quality of the muon measurement. We discuss the single element efficiency, resolution and noise rates, the calibration method of the detector response and of the alignment system, the track reconstruction efficiency and the momentum measurement. The results show that the detector i…

SystemAstrofísicaDriftPhysics - Instrumentation and DetectorsMuon SpectrometerPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsTracking (particle physics)01 natural sciences7. Clean energyHigh Energy Physics - ExperimentDrift TubeMDTHigh Energy Physics - Experiment (hep-ex)Data acquisitionATLAS muon spectrometer[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental TechniquesNuclear ExperimentPhysicsLarge Hadron Collidercosmic ray eventsDetectorSettore FIS/01 - Fisica SperimentaleBeamInstrumentation and Detectors (physics.ins-det)ATLASmedicine.anatomical_structureTrack ReconstructionPhysical SciencesFísica nuclearLHCmuon measurementFOS: Physical sciencesCosmic rayddc:500.2530Nuclear physicsAtlas (anatomy)0103 physical sciencesCalibrationmedicineFysikddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsEngineering (miscellaneous)Ciencias ExactasMuonChambersMuon TrackCosmologiaATLAS detector010308 nuclear & particles physicsFísicaTrack SegmentPhysics::Accelerator Physicsproton-proton collisionsHigh Energy Physics::Experiment
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Readiness of the ATLAS Tile Calorimeter for LHC collisions

2010

67 páginas.-- El PDF es la versión pre-print (arXiv:1007.5423v2).-- The ATLAS Collaboration.-- et al.

SystemPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsPerformance7. Clean energy01 natural sciences030218 nuclear medicine & medical imagingSettore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0302 clinical medicine[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental TechniquesDetectors de radiaciócosmic rayPhysicsLarge Hadron ColliderDetectorSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)ATLASmedicine.anatomical_structureScintillatorsPhysical Sciencesmagnetic-fields; scintillators; electronics; performance; systemLHCCol·lisionadors d'hadronsPhotomultiplierFOS: Physical sciencesCosmic rayddc:500.2Noise (electronics)530LHC collisions; AtlasNuclear physics03 medical and health sciencesAtlas (anatomy)0103 physical sciencesCalibrationmedicinetile hadronic calorimeterFysikddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsEngineering (miscellaneous)Ciencias ExactasCalorimeter (particle physics)010308 nuclear & particles physicsFísicaMagnetic-FieldsHigh Energy Physics::ExperimentElectronics
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Large bulk Micromegas detectors for TPC applications

2009

A large volume TPC will be used in the near future in a variety of experiments including T2K. The bulk Micromegas detector for this TPC is built using a novel production technique particularly suited for compact, thin and robust low mass detectors. The capability to pave a large Surface with a simple mounting Solution and small dead space is of particular interest for these applications. We have built several large bulk Micromegas detectors (36 x 34 cm(2)) and we have tested one in the former HARP field cage with a magnetic field. Prototypes cards of the T2K front end electronics, based on the AFTER ASIC chip, have been used in this TPC test for the first time. Cosmic ray data have been acq…

T2KPhysicsNuclear and High Energy PhysicsEnergy lossField (physics)Physics::Instrumentation and Detectorsbusiness.industryDetectorMicroMegas detectorCosmic rayNuclear physicsOpticsApplication-specific integrated circuitPoint (geometry)TPCbusinessInstrumentationMicromegasHARPNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Trigger and aperture of the surface detector array of the Pierre Auger Observatory

2010

The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detectors, for the study of extensive airshowers (EAS) generated by ultra-high-energy cosmic rays. We describe the trigger hierarchy, from the identification of candidates howers at the level of a single detector, amongst a large background (mainly random single cosmic ray muons), up to the selection of real events and the rejection of random coincidences. Such trigger makes the surface detector array fully efficient for the detection of EAS with energy above 3 x 1018 eV, for all zenith angles between 03 and 603, independently of the position of the impact point and of the mass of the primary particl…

Ultra high energy cosmic rays; Auger Observatory; Extensive air showers; Trigger; ExposurePhysics::Instrumentation and DetectorsAstronomyHigh-Energy Cosmi Ray7. Clean energy01 natural sciencesAugerAcceptance and Trigger Efficiency010303 astronomy & astrophysicsInstrumentationComputingMilieux_MISCELLANEOUSPhysicsRange (particle radiation)PhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryHigh energyFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AIR SHOWERSApertureInstrumentationAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerFOS: Physical sciencesCosmic rayENERGIACosmic RayUltra high energy cosmic rayExposureOpticsultra high energy cosmic rays Auger Observatory extensive airshowers trigger exposure0103 physical sciencesPARTICLESExtensive air showersSurface DetectorInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithCiencias ExactasNuclear and High Energy PhysicPierre Auger Observatory010308 nuclear & particles physicsbusiness.industryFísicaUltra high energy cosmic raysUltra-high energy cosmic rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]TriggerAuger ObservatoryExperimental High Energy PhysicsHigh Energy Physics::Experimentbusiness
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The General Antiparticle Spectrometer (GAPS) - Hunt for dark matter using low energy antideuterons

2011

The GAPS experiment is foreseen to carry out a dark matter search using a novel detection approach to detect low-energy cosmic-ray antideuterons. The theoretically predicted antideuteron flux resulting from secondary interactions of primary cosmic rays with the interstellar medium is very low. So far not a single cosmic antideuteron has been detected by any experiment, but well-motivated theories beyond the standard model of particle physics, e.g., supersymmetry or universal extra dimensions, contain viable dark matter candidates, which could led to a significant enhancement of the antideuteron flux due to self-annihilation of the dark matter particles. This flux contribution is believed to…

Universal extra dimensionNuclear physicsInterstellar mediumPhysicsAntiparticleAnnihilationPhysics beyond the Standard ModelDark matterCosmic rayExotic atomProceedings of Identification of Dark Matter 2010 — PoS(IDM2010)
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The Voyage of Metals in the Universe from Cosmological to Planetary Scales: the need for a Very High-Resolution, High Throughput Soft X-ray Spectrome…

2019

Metals form an essential part of the Universe at all scales. Without metals we would not exist, and the Cosmos would look completely different. Metals are primarily born through nuclear processes in stars. They leave their cradles through winds or explosions, and then start their journey through space. This can lead them in and out of astronomical objects on all scales, ranging from comets, planets, stars, entire galaxies, groups and clusters of galaxies to the largest structures of the Universe. Their wanderings are fundamental in determining how these objects, and the entire universe, evolve. In addition, their bare presence can be used to trace what these structures look like. The scope …

Very high resolutionAstronomical ObjectsCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesGalaxy-ISM-CGM-IGM feedbackFOS: Physical sciencesSpace (mathematics)Cycle of baryons and metals7. Clean energy01 natural sciencesCycle of baryons and metals; Galaxy-ISM-CGM-IGM feedback; High-resolution X-ray spectrometer; X-ray gratingsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]X-ray gratingsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsThroughput (business)0105 earth and related environmental sciencesCycle of baryons and metalHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSoft x rayCOSMIC cancer databaseSpectrometerSettore FIS/05AstronomyAstronomy and AstrophysicsHigh-resolution X-ray spectrometerAstrophysics - Astrophysics of GalaxiesStars13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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