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Cosmic ray studies with PAMELA experiment
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2011 (Engelska)Ingår i: Proceedings of the 14th Lomonosov Conference on Elementary Particle Physics: Particle Physics at the Year of Astronomy: Dedicated to the Late Academician Alexey Sissakian, 2011, s. 200-206Konferensbidrag, Publicerat paper (Refereegranskat)
Abstract [en]

The instrument PAMELA, in orbit since June 15th, 2006 on board of the Russian satellite Resurs DK1, is daily delivering to ground 16 Gigabytes of data. The apparatus is designed to study charged particles in the cosmic radiation, with a particular focus on antiparticles for searching antimatter and signals of dark matter annihilation. A combination of a magnetic spectrometer and different detectors allows antiparticles to be reliably identified from a large background of other charged particles. New results on the antiproton-to-proton and positron-toall electron ratios over a wideenergy range (1-100 GeV) have been obtained from the PAMELA mission. These data are mainly interpreted in terms of dark matter annihilation or pulsar contribution.

Ort, förlag, år, upplaga, sidor
2011. s. 200-206
Nyckelord [en]
Dark matter, In-orbit, Magnetic spectrometers, New results, Wide energy range, Elementary particles, Galaxies, Protons, Cosmic rays
Nationell ämneskategori
Fysik
Identifikatorer
URN: urn:nbn:se:kth:diva-148731Scopus ID: 2-s2.0-84885907435ISBN: 9814329673 (tryckt)ISBN: 9789814329675 (tryckt)OAI: oai:DiVA.org:kth-148731DiVA, id: diva2:745456
Konferens
14th Lomonosov Conference on Elementary Particle Physics 2009, 19 August 2009 through 25 August 2009, Moscow
Anmärkning

QC 20140910

Tillgänglig från: 2014-09-10 Skapad: 2014-08-11 Senast uppdaterad: 2016-12-23Bibliografiskt granskad

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Pearce, Mark

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Carlson, PerGillard, WilliamPearce, MarkRossetto, LauraWu, J.
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