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000296195 0881_ $$aarXiv:1010.5351; DESY-PROC-2010-03
000296195 088__ $$2arXiv$$aarXiv:1010.5351
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000296195 1001_ $$0P:(DE-HGF)0$$aIsern, J.$$b0
000296195 1112_ $$a6th Patras Workshop on Axions, WIMPs and WISPs$$cZürich$$d2010-07-05 - 2010-07-09$$gAXION-WIMP 2010$$wSwitzerland
000296195 245__ $$aAxions and White Dwarfs
000296195 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2010
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000296195 520__ $$aWhite 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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000296195 7001_ $$0P:(DE-HGF)0$$aCatalan, S.$$b1
000296195 7001_ $$0P:(DE-HGF)0$$aGarcia-Berro, E.$$b2
000296195 7001_ $$0P:(DE-HGF)0$$aSalaris, M.$$b3
000296195 7001_ $$0P:(DE-HGF)0$$aTorres, S.$$b4
000296195 773__ $$a10.3204/DESY-PROC-2010-03/isern_jordi
000296195 7870_ $$0PUBDB-2016-01334$$aBaudis, Laura et.al.$$dHamburg : Verlag Deutsches Elektronen-Synchrotron, 2010$$iIsPartOf$$rDESY-PROC-2010-03$$tProceedings, 6th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2010)
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