Davidson, Sacha (Corresponding author)

2014
Verlag Deutsches Elektronen-Synchrotron Hamburg
ISBN: 978-3-935702-59-1

2014Davidson, Sacha "The Pressure of Misalignment Axions:a Difference from WIMPs in Galaxy Formation?" in Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva
10th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2014, GenevaGeneva, Switzerland, 29 Jun 2014 - 4 Jul 20142014-06-292014-07-04 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 51-54 (2014) [10.3204/DESY-PROC-2014-03/davidson_sacha]2014  

Abstract: Two populations of axions can contribute to cold dark matter: the classical field produced via the misalignment mechanism, and the modes produced in the decay of strings. The classical field has extra pressure, as compared to WIMPs, which could have observable consequences in non-linear galaxy formation.

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Book/Proceedings/Report Tsesmelis, E. (Editor) ; Maroudas, M. (Editor)
Axions, WIMPs and WISPs: Proceedings, 10th Patras workshop, PATRAS 2014, AXION-WIMP 2014, Geneva, Switzerland, June 29-July 4, 2014
201410th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2014, GenevaGeneva, Switzerland, 29 Jun 2014 - 4 Jul 20142014-06-292014-07-04 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 207 p (2014) [10.3204/DESY-PROC-2014-03]2014     Files  full text BibTeX | EndNote: XML, Text | RIS