Publication Type |
Journal Article |
School or College |
College of Science |
Department |
Physics |
Creator |
Gondolo, Paolo |
Other Author |
Freese, Katherine; Spolyar, Douglas; Aguirre, Anthony; Bodenheimer, Peter; Sellwood, Jeremy A.; Yoshida, Naoki |
Title |
Dark stars: Begynnelsen |
Date |
2009 |
Description |
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 following contribution present the story of Dark Stars. In this first part, we describe the conditions under which dark stars form in the early universe: 1) high dark matter densities, 2) the annihilation products get stuck inside the star, and 3) dark matter heating wins over all other cooling or heating mechanisms. |
Type |
Text |
Publisher |
Proceedings of Science |
First Page |
18 |
Last Page |
22 |
Subject |
Dark stars; WIMP; Weakly interacting massive particles; Annihilations |
Subject LCSH |
Dark matter (Astronomy); Annihilation reactions; Stars -- Evolution |
Language |
eng |
Bibliographic Citation |
Gondolo, P., Freese, K., Spolyar, D., Aguirre, A., Bodenheimer, P., Sellwood, J. A., & Yoshida, N. (2009). Dark stars: Begynnelsen. Identification of Dark Matter 2008, August 18-22, 2008, Stockholm, Sweden. 1-4. |
Rights Management |
(c)Gondolo, P., Freese, K., Spolyar, D., Aguirre, A., Bodenheimer, P., Sellwood, J. A. & Yoshida, N. Preprint arxiv:0901.4578 |
Format Medium |
application/pdf |
Format Extent |
277,828 bytes |
Identifier |
ir-main,9262 |
ARK |
ark:/87278/s60g43nm |
Setname |
ir_uspace |
ID |
705982 |
Reference URL |
https://collections.lib.utah.edu/ark:/87278/s60g43nm |