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High-Energy Astrophysics and Cosmology

Interfaces between high-energy physics, astrophysics and cosmology are reviewed, with particular emphasis on the important roles played by high-energy cosmic-ray physics. These include the understanding of atmospheric neutrinos, the search for massive cold dark matter particles and possible tests of...

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Detalles Bibliográficos
Autor principal: Ellis, Jonathan Richard
Lenguaje:eng
Publicado: 2002
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0920-5632(03)01954-6
http://cds.cern.ch/record/588866
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author Ellis, Jonathan Richard
author_facet Ellis, Jonathan Richard
author_sort Ellis, Jonathan Richard
collection CERN
description Interfaces between high-energy physics, astrophysics and cosmology are reviewed, with particular emphasis on the important roles played by high-energy cosmic-ray physics. These include the understanding of atmospheric neutrinos, the search for massive cold dark matter particles and possible tests of models of quantum gravity. In return, experiments at the LHC may be useful for refining models of ultra-high-energy cosmic rays, and thereby contributing indirectly to understanding their origin. Only future experiments will be able to tell whether these are due to some bottom-up astrophysical mechanism or some top-down cosmological mechanism.
id cern-588866
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2002
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spelling cern-5888662019-09-30T06:29:59Zdoi:10.1016/S0920-5632(03)01954-6http://cds.cern.ch/record/588866engEllis, Jonathan RichardHigh-Energy Astrophysics and CosmologyAstrophysics and AstronomyInterfaces between high-energy physics, astrophysics and cosmology are reviewed, with particular emphasis on the important roles played by high-energy cosmic-ray physics. These include the understanding of atmospheric neutrinos, the search for massive cold dark matter particles and possible tests of models of quantum gravity. In return, experiments at the LHC may be useful for refining models of ultra-high-energy cosmic rays, and thereby contributing indirectly to understanding their origin. Only future experiments will be able to tell whether these are due to some bottom-up astrophysical mechanism or some top-down cosmological mechanism.astro-ph/0210580CERN-TH-2002-300oai:cds.cern.ch:5888662002-10-26
spellingShingle Astrophysics and Astronomy
Ellis, Jonathan Richard
High-Energy Astrophysics and Cosmology
title High-Energy Astrophysics and Cosmology
title_full High-Energy Astrophysics and Cosmology
title_fullStr High-Energy Astrophysics and Cosmology
title_full_unstemmed High-Energy Astrophysics and Cosmology
title_short High-Energy Astrophysics and Cosmology
title_sort high-energy astrophysics and cosmology
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1016/S0920-5632(03)01954-6
http://cds.cern.ch/record/588866
work_keys_str_mv AT ellisjonathanrichard highenergyastrophysicsandcosmology