Dark stars: Begynnelsen

Update Item Information
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
Back to Search Results