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The Cosmic Ray Lepton Puzzle

Recent measurements of cosmic ray electrons and positrons by PAMELA, ATIC, Fermi and HESS have revealed interesting excesses and features in the GeV-TeV range. Many possible explanations have been suggested, invoking one or more nearby primary sources such as pulsars and supernova remnants, or dark...

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Autores principales: Brun, Pierre, Bertone, Gianfranco, Cirelli, Marco, Moulin, Emmanuel, Glicenstein, Jean-Francois, Iocco, Fabio, Pieri, Lidia
Formato: info:eu-repo/semantics/article
Lenguaje:eng
Publicado: 2010
Materias:
Acceso en línea:http://cds.cern.ch/record/1236947
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author Brun, Pierre
Bertone, Gianfranco
Cirelli, Marco
Moulin, Emmanuel
Glicenstein, Jean-Francois
Iocco, Fabio
Pieri, Lidia
author_facet Brun, Pierre
Bertone, Gianfranco
Cirelli, Marco
Moulin, Emmanuel
Glicenstein, Jean-Francois
Iocco, Fabio
Pieri, Lidia
author_sort Brun, Pierre
collection CERN
description Recent measurements of cosmic ray electrons and positrons by PAMELA, ATIC, Fermi and HESS have revealed interesting excesses and features in the GeV-TeV range. Many possible explanations have been suggested, invoking one or more nearby primary sources such as pulsars and supernova remnants, or dark matter. Based on the output of the TANGO in PARIS --Testing Astroparticle with the New GeV/TeV Observations in Positrons And electRons : Identifying the Sources-- workshop held in Paris in May 2009, we review here the latest experimental results and we discuss some virtues and drawbacks of the many theoretical interpretations proposed so far.
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spelling cern-12369472023-03-12T20:50:08Z http://cds.cern.ch/record/1236947 eng Brun, Pierre Bertone, Gianfranco Cirelli, Marco Moulin, Emmanuel Glicenstein, Jean-Francois Iocco, Fabio Pieri, Lidia The Cosmic Ray Lepton Puzzle Astrophysics and Astronomy Recent measurements of cosmic ray electrons and positrons by PAMELA, ATIC, Fermi and HESS have revealed interesting excesses and features in the GeV-TeV range. Many possible explanations have been suggested, invoking one or more nearby primary sources such as pulsars and supernova remnants, or dark matter. Based on the output of the TANGO in PARIS --Testing Astroparticle with the New GeV/TeV Observations in Positrons And electRons : Identifying the Sources-- workshop held in Paris in May 2009, we review here the latest experimental results and we discuss some virtues and drawbacks of the many theoretical interpretations proposed so far. info:eu-repo/grantAgreement/EC/FP7/237920 info:eu-repo/semantics/openAccess Education Level info:eu-repo/semantics/article http://cds.cern.ch/record/1236947 2010-02-01
spellingShingle Astrophysics and Astronomy
Brun, Pierre
Bertone, Gianfranco
Cirelli, Marco
Moulin, Emmanuel
Glicenstein, Jean-Francois
Iocco, Fabio
Pieri, Lidia
The Cosmic Ray Lepton Puzzle
title The Cosmic Ray Lepton Puzzle
title_full The Cosmic Ray Lepton Puzzle
title_fullStr The Cosmic Ray Lepton Puzzle
title_full_unstemmed The Cosmic Ray Lepton Puzzle
title_short The Cosmic Ray Lepton Puzzle
title_sort cosmic ray lepton puzzle
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/1236947
http://cds.cern.ch/record/1236947
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