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Dark Matter Research and the PAMELA Space Mission
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2009 (English)In: SOURCES AND DETECTION OF DARK MATTER AND DARK ENERGY IN THE UNIVERSE / [ed] Cline, DB, 2009, Vol. 1166, 141-150 p.Conference paper, Published paper (Other academic)
Abstract [en]

On the 15th of June 2006, the PAMELA satellite-borne experiment was launched from the Bajkonur cosmodrome and since July 2006 it has been collected data. The core of the apparatus is a silicon-microstrip magnetic spectrometer combined with a time-of-flight system, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail counter scintillator and a neutron detector. The overall devices allow precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV - 100's GeV) with high statistics. The primary scientific goal is the measurement of the antiproton and positron energy spectra in order to search for exotic sources, such as dark matter particle annihilation. PAMELA is also searching for primordial antinuclei ((He) over bar). Concomitant, but not secondary, goals are the measurements of light nuclei and their isotopes for studying the energy dependence of cosmic ray lifetimes in the Galaxy, the monitoring of the solar activity and the study of the radiation belts.

Place, publisher, year, edition, pages
2009. Vol. 1166, 141-150 p.
Series
AIP Conference Proceedings, ISSN 0094-243X ; 1166
Keyword [en]
Dark matter, Normal galaxies; extragalactic objects and systems, Neutrino mass and mixing
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-80165DOI: 10.1063/1.3232171ISI: 000279741300019Scopus ID: 2-s2.0-70450191300OAI: oai:DiVA.org:kth-80165DiVA: diva2:496158
Conference
8th UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe. Marina del Rey, CA. FEB 20-22, 2008
Note
QC 20120305Available from: 2012-02-09 Created: 2012-02-09 Last updated: 2012-03-05Bibliographically approved

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Pearce, Mark

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  • apa
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