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001     296195
005     20211110133659.0
024 7 _ |a 10.3204/DESY-PROC-2010-03/isern_jordi
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024 7 _ |a arXiv:1010.5351
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024 7 _ |a inspire:874436
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037 _ _ |a PUBDB-2016-01348
041 _ _ |a English
088 1 _ |a arXiv:1010.5351; DESY-PROC-2010-03
088 _ _ |a arXiv:1010.5351
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088 _ _ |a DESY-PROC-2010-03
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100 1 _ |a Isern, J.
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111 2 _ |a 6th Patras Workshop on Axions, WIMPs and WISPs
|g AXION-WIMP 2010
|c Zürich
|d 2010-07-05 - 2010-07-09
|w Switzerland
245 _ _ |a Axions and White Dwarfs
260 _ _ |a Hamburg
|c 2010
|b Verlag Deutsches Elektronen-Synchrotron
300 _ _ |a 77-80
336 7 _ |a Conference Paper
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336 7 _ |a Contribution to a conference proceedings
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336 7 _ |a Internal Report
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336 7 _ |a INPROCEEDINGS
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520 _ _ |a 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.
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700 1 _ |a Catalan, S.
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700 1 _ |a Garcia-Berro, E.
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700 1 _ |a Salaris, M.
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700 1 _ |a Torres, S.
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773 _ _ |a 10.3204/DESY-PROC-2010-03/isern_jordi
787 0 _ |a Baudis, Laura et.al.
|d Hamburg : Verlag Deutsches Elektronen-Synchrotron, 2010
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|r DESY-PROC-2010-03
|t Proceedings, 6th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2010)
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