Non-perturbative effect on thermal relic abundance of dark matter

AIP Conference Proceedings

Volumn 957, Issue , 2007, Pages 401-404

  Hisano, J ^a   Matsumoto, S ^b   Nagai, M ^a   Saito, O ^c   Senami, M ^a  

^a UNIVERSITY OF TOKYO   (Japan)

^b TOHOKU UNIVERSITY   (Japan)

^c HIGH ENERGY ACCELERATOR RESEARCH ORGANIZATION KEK   (Japan)

Author keywords

Dark matter; Relic abundance; Sommerfeld effect; Wino

Indexed keywords

EID: 71849113481     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.2823813     Document Type: Conference Paper

References (10)

1. J. Hisano, S. Matsumoto, M. Nagai, O. Saito and M. Senami, Phys. Lett. B 646 (2007) 34.
2. J. Hisano, S. Matsumoto, M. M. Nojiri and O. Saito, Phys. Rev. D 71, 063528 (2005).
3. J. Hisano, S. Matsumoto and M. M. Nojiri, Phys. Rev. Lett. 92, 031303 (2004).
4. J. Hisano, S. Matsumoto, O. Saito and M. Senami, Phys. Rev. D 73, 055004 (2006).
5. D. N. Spergel et al., arXiv:astro-ph/0603449.
6. T. Appelquist, H. C. Cheng and B. A. Dobrescu, Phys. Rev. D 64, 035002 (2001).
7. For an example, see, M. Kakizaki, S. Matsumoto and M. Senami, Phys. Rev. D 74, 023504 (2006).
8. M. Kakizaki, S. Matsumoto, Y. Sato and M. Senami, Nucl. Phys. B 735, 84 (2006).
9. H. Baer, K. m. Cheung and J. F. Gunion, Phys. Rev. D 59, 075002 (1999).
10. A. Arvanitaki, C. Davis, P. W. Graham, A. Pierce and J. G. Wacker, Phys. Rev. D 72, 075011 (2005).