% IMPORTANT: The following is UTF-8 encoded. This means that in the presence % of non-ASCII characters, it will not work with BibTeX 0.99 or older. % Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or % “biber”. @INPROCEEDINGS{Isern:295202, author = {Isern, J. and Althaus, L. and Catalan, S. and Corsico, A. and Garcia-Berro, E. and Salaris, M. and Torres, S. and Althaus, L. and Catalan, S. and Corsico, A. and Garcia-Berro, E. and Salaris, M. and Torres, S.}, title = {{W}hite dwarfs as physics laboratories: the case of axions}, reportid = {PUBDB-2016-01118, arXiv:1204.3565}, pages = {158-162}, year = {2011}, abstract = {White dwarfs are almost completely degenerate objects that cannot obtain energy from thermonuclear sources, so their evolution is just a gravothermal cooling process. Recent improvements in the accuracy and precision of the luminosity function and in pulsational data of variable white dwarfs suggest that they are cooling faster than expected from conventional theory. In this contribution we show that the inclusion of an additional cooling term due to axions able to interact with electrons with a coupling constant $g_ae$ $~(2-7)x10^{-13}$ allows to fit better the observations.}, month = {Jun}, date = {2011-06-27}, organization = {7th Patras Workshop on Axions, WIMPs and WISPs, Mykonos (Greece), 27 Jun 2011 - 1 Jul 2011}, keywords = {white dwarf (INSPIRE) / axion (INSPIRE) / WISP (INSPIRE) / WIMP (INSPIRE) / thermodynamics (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 = {1204.3565}, howpublished = {arXiv:1204.3565}, archivePrefix = {arXiv}, SLACcitation = {$\%\%CITATION$ = $arXiv:1204.3565;\%\%$}, doi = {10.3204/DESY-PROC-2011-04/isern_jordi}, url = {https://bib-pubdb1.desy.de/record/295202}, }