Search results for "Galactic Cosmic-Rays"

showing 2 items of 2 documents

In situ observations of new particle formation in the tropical upper troposphere: the role of clouds and the nucleation mechanism

2011

New particle formation (NPF), which generates nucleation mode aerosol, was observed in the tropical Upper Troposphere (UT) and Tropical Tropopause Layer (TTL) by in situ airborne measurements over South America (January–March 2005), Australia (November–December 2005), West Africa (August 2006) and Central America (2004–2007). Particularly intense NPF was found at the bottom of the TTL. Measurements with a set of condensation particle counters (CPCs) with different <i>d</i><sub>p50</sub> (50% lower size detection efficiency diameter or "cut-off diameter") were conducted on board the M-55 <i>Geophysica</i> in the altitude range of 12.0–20.5 km and on board …

Atmospheric Science010504 meteorology & atmospheric sciencesDISPERSION MODEL FLEXPARTaerosolnucleationNucleationclouds010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencestropicsTropospherelcsh:Chemistrynew particle formationddc:550Cloud condensation nucleiLife ScienceStratosphere0105 earth and related environmental sciencesGeophysica[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereIce cloudAtmosphärische SpurenstoffeFalconlcsh:QC1-999AerosolJAQUEOUS SULFURIC-ACIDlcsh:QD1-99913. Climate actionClimatologyupper troposphereEnvironmental scienceOutflowAEROSOL NUCLEATIONLOWER STRATOSPHERETropopauselcsh:PhysicsGALACTIC COSMIC-RAYS
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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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