Contribution to a conference proceedings/Internal Report | PUBDB-2016-01348 |
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2010
Verlag Deutsches Elektronen-Synchrotron
Hamburg
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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2010-03/isern_jordi
Report No.: DESY-PROC-2010-03; arXiv:1010.5351
Abstract: White dwarfs are almost completely degenerate objects that cannot obtain energy from the thermonuclear sources and their evolution is just a gravothermal process of cooling. The simplicity of these objects, the fact that the physical inputs necessary to understand them are well identified, although not always well understood, and the impressive observational background about white dwarfs make them the most well studied Galactic population. These characteristics allow to use them as laboratories to test new ideas of physics. In this contribution we discuss the robustness of the method and its application to the axion case.
Keyword(s): axion ; background ; simplex ; galaxy ; WIMP ; WISP
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Proceedings/Internal Report
Proceedings, 6th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2010)
6th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2010, ZürichZürich, Switzerland, 5 Jul 2010 - 9 Jul 2010
Hamburg : Verlag Deutsches Elektronen-Synchrotron (2010)
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