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@INPROCEEDINGS{Erken:295125,
author = {Erken, Ozgur and Sikivie, Pierre and Tam, Heywood and Yang,
Qiaoli},
title = {{A}xion {BEC} {D}ark {M}atter},
reportid = {PUBDB-2016-01073, arXiv:1111.3976},
pages = {43-46},
year = {2011},
abstract = {Cold dark matter axions thermalize through gravitational
self-interactions and form a Bose-Einstein condensate when
the photon temperature reaches approximately 500 eV. Axion
Bose-Einstein condensation provides an opportunity to
distinguish axions from the other dark matter candidates on
the basis of observation. The rethermalization of axions
that are about to fall in a galactic potential well causes
them to acquire net overall rotation, whereas ordinary cold
dark matter falls in with an irrotational velocity field.
The inner caustics of galactic halos are different in the
two cases.},
month = {Jun},
date = {2011-06-27},
organization = {7th Patras Workshop on Axions, WIMPs
and WISPs, Mykonos (Greece), 27 Jun
2011 - 1 Jul 2011},
keywords = {condensation: Bose-Einstein (INSPIRE) / axion: dark matter
(INSPIRE) / dark matter: galaxy: halo (INSPIRE) / photon:
temperature (INSPIRE) / galaxy: halo (INSPIRE) / gravitation
(INSPIRE) / rotation (INSPIRE) / velocity (INSPIRE) / WISP
(INSPIRE) / WIMP (INSPIRE)},
cin = {L},
cid = {I:(DE-H253)L-20120731},
pnm = {899 - ohne Topic (POF3-899)},
pid = {G:(DE-HGF)POF3-899},
experiment = {EXP:(DE-H253)HERA(machine)-20150101},
typ = {PUB:(DE-HGF)8 / PUB:(DE-HGF)15},
eprint = {1111.3976},
howpublished = {arXiv:1111.3976},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:1111.3976;\%\%$},
doi = {10.3204/DESY-PROC-2011-04/sikivie_pierre},
url = {https://bib-pubdb1.desy.de/record/295125},
}