Upper bounds on signals due to WIMP self-annihilation: Comments on the case of the synchrotron radiation from the galactic center and the WMAP haze

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 77, Issue 12, 2008, Pages

  Bottino, A ^a   Donato, F ^a   Fornengo, N ^a   Scopel, S ^b  

^a UNIVERSITY OF TURIN   (Italy)

^b Korea Institute for Advanced Study   (South Korea)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 45749118662     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.77.127301     Document Type: Article

References (17)

1. D.P. Finkbeiner, arXiv:astro-ph/0409027.
2. D. Hooper, D.P. Finkbeiner, and G. Dobler, Phys. Rev. D 76, 083012 (2007). PRVDAQ 0556-2821 10.1103/PhysRevD.76.083012
3. D.N. Spergel (WMAP Collaboration), Astrophys. J. Suppl. Ser. 148, 175 (2003); APJSA2 0067-0049 10.1086/377226
4. D.N. Spergel Astrophys. J. Suppl. Ser. 170, 377 (2007). APJSA2 0067-0049 10.1086/513700
5. D. Hooper, arXiv:0801.4378.
6. A. Bottino, C. Favero, N. Fornengo, G. Mignola, and S. Scopel, Proceedings of the International Workshop Double-beta Decay and Related Topics, edited by, H.V. Klapdor-Kleingrothaus, and, S. Stoica, (World Scientific, Singapore, 1996), p. 281.
7. A. Bottino, F. Donato, N. Fornengo, and S. Scopel, Proceedings of Results and Perspectives in Particle Physics, edited by, M. Greco,, (INFN Laboratori Nazionali Frascati, Rome, Italy, 2001), p. 135.
8. A. Bottino, F. Donato, N. Fornengo, and P. Salati, Phys. Rev. D 72, 083518 (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.72.083518
9. T.K. Gaisser, G. Steigman, and S. Tilav, Phys. Rev. D 34, 2206 (1986). PRVDAQ 0556-2821 10.1103/PhysRevD.34.2206
10. A. Bottino, F. Donato, N. Fornengo, and S. Scopel, Phys. Rev. D 70, 015005 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.70.015005
11. F. Donato, N. Fornengo, D. Maurin, P. Salati, and R. Taillet, Phys. Rev. D 69, 063501 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.69.063501
12. S. Orito (BESS Collaboration), Phys. Rev. Lett. 84, 1078 (2000); PRLTAO 0031-9007 10.1103/PhysRevLett.84.1078
13. T. Maeno (BESS Collaboration), Astropart. Phys. 16, 121 (2001); APHYEE 0927-6505 10.1016/S0927-6505(01)00107-4
14. M Aguilar (AMS Collaboration), Phys. Rep. 366, 331 (2002). PRPLCM 0370-1573 10.1016/S0370-1573(02)00013-3
15. F. Donato, Astrophys. J. 563, 172 (2001). ASJOAB 0004-637X 10.1086/323684
16. Large values for the boost factor are unlikely, see V. Berezinsky, V. Dokuchaev, and Y. Eroshenko, Phys. Rev. D 68, 103003 (2003); PRVDAQ 0556-2821 10.1103/PhysRevD.68.103003
17. J. Lavalle, Q. Yuan, D. Maurin, and X.J. Bi, arXiv:0709.3634.