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Constraints on cosmic-ray propagation and acceleration models from recent data
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics. Oskar Klein Centre for Cosmoparticle Physics, Sweden .
LPSC, UJF Grenoble 1, CNRS/IN2P3, INP de Grenoble, France.
Department of Physics, Stockholm University.
Oskar Klein Centre for Cosmoparticle Physics, Sweden.ORCID iD: 0000-0001-7011-7229
2011 (English)In: Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011, Institute of High Energy Physics , 2011, Vol. 6, 228-231 p.Conference paper, Published paper (Refereed)
Abstract [en]

We are studying the constraints obtained on transport and acceleration mechanisms of galactic cosmic rays by using statistical tools in combination with the propagation package GALPROP and recent PAMELA data. Using only PAMELA data allows us to avoid inconsistencies between data sets from different experiments, minimise uncertainties on solar modulation parameters, and have a complementary and precise data set on (anti-)matter as well as primary and secondary nuclei over 3 orders of magnitude in energy. This allows us to simultaneously place strong constraints on cosmic-ray propagation and acceleration models. We describe our methodology and present some preliminary results in this paper.

Place, publisher, year, edition, pages
Institute of High Energy Physics , 2011. Vol. 6, 228-231 p.
Keyword [en]
cosmic-ray, propagation models, statistics
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-80726DOI: 10.7529/ICRC2011/V06/0160Scopus ID: 2-s2.0-84899558594OAI: oai:DiVA.org:kth-80726DiVA: diva2:496699
Conference
32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China, 11 August 2011 through 18 August 2011
Note

QC 20120214

Available from: 2012-02-14 Created: 2012-02-10 Last updated: 2015-04-22Bibliographically approved

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Pearce, Mark

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