Dark Stars: Dod och Ateruppstandelse TeX Export

@article{Spolyar:2009rs, abstract = {The first phase of stellar evolution in the history of the universe may be Dark Stars, powered by dark matter heating rather than by fusion. Weakly interacting massive particles, which are their own antiparticles, can annihilate and provide an important heat source for the first stars in the universe. This and the previous contribution present the story of Dark Stars. In this second part, we describe the structure of Dark Stars and predict that they are very massive (\\\\$\\\\sim 800 M\_\\\\odot\\\\$), cool (6000 K), bright (\\\\$\\\\sim 10^6 L\_\\\\odot\\\\$), long-lived (\\\\$\\\\sim 10^6\\\\$ years), and probable precursors to (otherwise unexplained) supermassive black holes. Later, once the initial dark matter fuel runs out and fusion sets in, dark matter annihilation can predominate again if the scattering cross section is strong enough, so that a Dark Star is born again.}, archivePrefix = {arXiv}, author = {Spolyar, Douglas and Freese, Katherine and Gondolo, Paolo and Aguirre, Anthony and Bodenheimer, Peter and Sellwood, Jeremy A. and Yoshida, Naoki}, citeulike-article-id = {4013242}, citeulike-linkout-0 = {http://arxiv.org/abs/0901.4574}, citeulike-linkout-1 = {http://arxiv.org/pdf/0901.4574}, citeulike-linkout-2 = {http://arxiv.org/abs/0901.4574}, day = {28}, eprint = {0901.4574}, eprint = {0901.4574}, keywords = {cosmology, dark-matter, dark-stars}, month = {Jan}, posted-at = {2009-02-05 16:10:06}, priority = {2}, title = {Dark Stars: Dod och Ateruppstandelse}, url = {http://arxiv.org/abs/0901.4574}, year = {2009} }

TY - JOUR ID - Spolyar:2009rs L3 - citeulike-article-id:4013242 N2 - The first phase of stellar evolution in the history of the universe may be Dark Stars, powered by dark matter heating rather than by fusion. Weakly interacting massive particles, which are their own antiparticles, can annihilate and provide an important heat source for the first stars in the universe. This and the previous contribution present the story of Dark Stars. In this second part, we describe the structure of Dark Stars and predict that they are very massive (\\\\$\\\\sim 800 M_\\\\odot\\\\$), cool (6000 K), bright (\\\\$\\\\sim 10^6 L_\\\\odot\\\\$), long-lived (\\\\$\\\\sim 10^6\\\\$ years), and probable precursors to (otherwise unexplained) supermassive black holes. Later, once the initial dark matter fuel runs out and fusion sets in, dark matter annihilation can predominate again if the scattering cross section is strong enough, so that a Dark Star is born again. TI - Dark Stars: Dod och Ateruppstandelse KW - cosmology KW - dark-matter KW - dark-stars AU - Spolyar, Douglas AU - Freese, Katherine AU - Gondolo, Paolo AU - Aguirre, Anthony AU - Bodenheimer, Peter AU - Sellwood, Jeremy AU - Yoshida, Naoki PY - 2009/Jan/28/ UR - http://arxiv.org/abs/0901.4574 ER -