Search results for "background radiation"

showing 5 items of 55 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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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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Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

2008

Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival directions of the cosmic rays with the ighest-energies, which are correlated with the positions of relatively nearby active galactic nuclei (AGN) [Pierre Auger Collaboration, Science 318 (2007) 938]. The correlation has maximum significance for cosmic rays with energy greater than ~6 x 1019 eV and AGN at a distance less than ~75 Mpc. We have confirmed the anisotropy at a confidence level of more than 99% through a test with parameters specified a priori, using an independent data set. The observed correlation is compatible with the hypothesis that cosmic rays with the highest-energies originate fro…

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyOsservatorio Pierre AugerAstrophysicsGALAXY CLUSTER SURVEYAstrophysicsauger01 natural sciencesHigh energy cosmic rayRaggi cosmiciAstrophysical jetGMFObservatoryUltra-high-energy cosmic ray010303 astronomy & astrophysicsPhysicsBL-LACERTAEGreisen–Zatsepin–Kuz’min effect[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]ORIGINUHECRAstrophysics (astro-ph)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryGZKRadiación cósmicaAnisotropíaCATALOGobservatoryddc:540EGMFCUTOFFComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRELATIVISTIC JETSActive galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaCosmic background radiationFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsACCELERATION[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesextra-galacticPARTICLESAGNAstrophysics::Galaxy AstrophysicsCiencias ExactasPierre Auger ObservatoryANISOTROPYhigh energy cosmic raysSciami atmosferici010308 nuclear & particles physicsFísicaAstronomyAstronomy and AstrophysicsCENTAURUSGalaxyExperimental High Energy Physics
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Chronic Background Radiation Correlates With Sperm Swimming Endurance in Bank Voles From Chernobyl

2022

Sperm quantity and quality are key features explaining intra- and interspecific variation in male reproductive success. Spermatogenesis is sensitive to ionizing radiation and laboratory studies investigating acute effects of ionizing radiation have indeed found negative effects of radiation on sperm quantity and quality. In nature, levels of natural background radiation vary dramatically, and chronic effects of low-level background radiation exposure on spermatogenesis are poorly understood. The Chernobyl region offers a unique research opportunity for investigating effects of chronic low-level ionizing radiation on reproductive properties of wild organisms. We captured male bank voles (Myo…

reproductionbackground radiationEcologyEvolutionMyodes glareolusQH359-425performanceQH540-549.5sperm morphometryFrontiers in Ecology and Evolution
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