Dark Matter interpretations of the e± excesses after FERMI

Nuclear Physics B

Volumn 831, Issue 1-2, 2010, Pages 178-203

  Meade, Patrick ^a   Papucci, Michele ^a   Strumia, Alessandro ^b   Volansky, Tomer ^a  

^a INSTITUTE FOR ADVANCED STUDY   (United States)

^b UNIVERSITY OF PISA   (Italy)

Author keywords

Dark Matter; FERMI; PAMELA

Indexed keywords

EID: 76749099675     PISSN: 05503213     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.nuclphysb.2010.01.012     Document Type: Article

References (93)

1. Moiseev A.A., Ormes J.F., and Moskalenko I.V. arXiv:0706.0882 [astro-ph]
2. Cirelli M., Kadastik M., Raidal M., and Strumia A. Nucl. Phys. B 813 (2009) 308. arXiv:0809.2409
3. FERMI/LAT Collaboration. arXiv:0905.0025
4. H.E.S.S. Collaboration. arXiv:0811.3894
5. H.E.S.S. Collaboration. arXiv:0905.0105
6. ATIC Collaboration. Nature 456 (2008) 362
7. New ATIC-4 results, compatible with the ATIC results published on Nature and incompatible with FERMI [3], have been presented at the TANGO conference, http://irfu.cea.fr/Meetings/tangoinparis
8. Atoian A.M., Aharonian F.A., and Volk H.J. Phys. Rev. D 52 (1995) 3265
9. Büshing I., et al. arXiv:0804.0220
10. Kobayashi T., Komori Y., Yoshida K., and Nishimura J. Astrophys. J. 601 (2004) 340. astro-ph/0308470
11. See also the recent study in. Hooper D., Blasi P., and Serpico P.D. arXiv:0810.1527
12. Yuksel H., Kistler M.D., and Stanev T. arXiv:0810.2784
13. Serpico P.D. arXiv:0810.4846
14. Profumo S. arXiv:0812.4457
15. Blasi P., and Serpico P.D. arXiv:0904.0871
16. Sommerfeld A. Ann. Phys. 11 (1931) 257
17. Hisano J., Matsumoto S., and Nojiri M.M. Phys. Rev. Lett. 92 (2004) 031303. hep-ph/0307216
18. Hisano J., Matsumoto S., Nojiri M.M., and Saito O. Phys. Rev. D 71 (2005) 063528. hep-ph/0412403
19. See also previous work in. Belotsky K., Fargion D., Khlopov M., Konoplich R.V., and Konoplich R.V. Phys. Atom. Nucl. 71 (2008) 147. arXiv:hep-ph/0411093 and references therein
20. A generic study of the Sommerfeld Abelian effect in DM annihilations was presented in DM annihilations was presented in. Cirelli M., Strumia A., and Tamburini M. Nucl. Phys. B 787 (2007) 152. arXiv:0706.4071
21. For a generic unbroken non-Abelian gauge interaction, the group theory needed to compute the Sommerfeld effect was presented in. Strumia A. arXiv:0806.1630
22. Arkani-Hamed N., Finkbeiner D.P., Slatyer T., and Weiner N. arXiv:0810.0713
23. Ibe M., Murayama H., and Yanagida T.T. arXiv:0812.0072 [hep-ph]
24. Kuhlen M., Diemand J., and Madau P. arXiv:0805.4416 [astro-ph]
25. Bertone G., Cirelli M., Strumia A., and Taoso M. JCAP 0901 (2009) 43. arXiv:0811.3744
26. Meade P., Papucci M., and Volansky T. arXiv:0901.2925 [hep-ph]
27. Mardon J., Nomura Y., Stolarski D., and Thaler J. arXiv:0901.2926 [hep-ph]
28. Bergstrom L., Bertone G., Bringmann T., Edsjo J., and Taoso M. arXiv:0812.3895 [astro-ph]
29. PAMELA Collaboration. arXiv:0810.4995
30. PAMELA Collaboration. arXiv:0810.4994
31. Talk by O. Adriani available at http://www.crlab.rise.waseda.ac.jp
32. Matthieu Vivier, Talk presented on behalf of HESS Collaboration, 44th Rencontres de Moriond, February 6, 2009
33. HESS Collaboration. Nature 439 (2006) 695. astro-ph/0603021
34. HESS Collaboration. Astropart. Phys. 29 (2008) 55. arXiv:0711.2369
35. VERITAS Collaboration. arXiv:0810.1913
36. Super-Kamiokande Collaboration. arXiv:hep-ex/0404025
37. SK Collaboration. arXiv:0711.0053
38. Donato F., Fornengo N., Maurin D., and Salati P. Phys. Rev. D 69 (2004) 063501. arXiv:astro-ph/0306207
39. Yin P.f., Yuan Q., Liu J., Zhang J., Bi X.j., and Zhu S.h. arXiv:0811.0176
40. Chen C.R., Takahashi F., and Yanagida T.T. arXiv:0811.0477
41. Ibarra A., and Tran D. arXiv:0811.1555
42. Chen C.R., Takahashi F., and Yanagida T.T. arXiv:0811.3357
43. Arvanitaki A., Dimopoulos S., Dubovsky S., Graham P.W., Harnik R., and Rajendran S. arXiv:0904.2789 [hep-ph]
44. Grajek P., Kane G., Phalen D., Pierce A., and Watson S. arXiv:0812.4555 [hep-ph]
45. Hisano J., Kawasaki M., Kohri K., and Nakayama K. Phys. Rev. D 79 (2009) 063514. arXiv:0810.1892 [hep-ph]
46. Hooper D., and Zurek K.M. arXiv:0902.0593 [hep-ph]
47. Huh J.H., Kim J.E., and Kyae B. arXiv:0809.2601
48. Ishiwata K., Matsumoto S., and Moroi T. arXiv:0811.0250
49. Harnik R., and Kribs G.D. arXiv:0810.5557
50. Pospelov M., and Ritz A. arXiv:0810.1502
51. Nelson A.E., and Spitzer C. arXiv:0810.5167
52. Nomura Y., and Thaler J. arXiv:0810.5397
53. Feldman D., Liu Z., and Nath P. arXiv:0810.5762
54. Hambye T. arXiv:0811.0172
55. Bai Y., and Han Z. arXiv:0811.0387
56. Fox P.J., and Poppitz E. arXiv:0811.0399
57. Goh H.-S., Hall L.J., and Kumar P. arXiv:0902.0814
58. Rothstein I.Z., Schwetz T., and Zupan J. arXiv:0903.3116 [astro-ph.HE]
59. CDF Collaboration. arXiv:0810.5357
60. Giromini P., et al. arXiv:0810.5730
61. Barbieri R., et al. arXiv:0902.2145
62. Cholis I., Dobler G., Finkbeiner D.P., Goodenough L., and Weiner N. arXiv:0811.3641
63. Borriello E., Cuoco A., and Miele G. arXiv:0903.1852
64. Regis M., and Ullio P. arXiv:0904.4645 IC was computed without running GALPROP also in [38]
65. Blumenthal G.R., and Gould R.J. Rev. Modern Phys. 42 (1970) 237
66. Delahaye T., Lineros R., Donato F., Fornengo N., and Salati P. arXiv:0712.2312
67. Cirelli M., Franceschini R., and Strumia A. Nucl. Phys. B 800 (2008) 204. arXiv:0802.3378
68. Hisano J., Kawasaki M., Kohri K., and Nakayama K. arXiv:0812.0219 [hep-ph]
69. Cirelli M., and Panci P. arXiv:0904.3830
70. Finkbeiner D.P. arXiv:astro-ph/0409027
71. Hooper D., Finkbeiner D.P., and Dobler G. Phys. Rev. D 76 (2007) 083012. arXiv:0705.3655
72. Navarro J., Frenk C., and White S. Astrophys. J. 490 (1997) 493. arXiv:astro-ph/9611107
73. Graham A.W., Merritt D., Moore B., Diemand J., and Terzic B. Astron. J. 132 (2006) 2685. arXiv:astro-ph/0509417
74. Navarro J.F., et al. arXiv:0810.1522
75. Bahcall J.N., and Soneira R.M. Astrophys. J. Suppl. 44 (1980) 73
76. Davis R.D., Walsh D., and Booth R.S. MNRAS 177 (1976) 319-333
77. Genzel R., et al. Nature 425 (2003) 934. astro-ph/0310821
78. Essig R., Sehgal N., and Strigari L.E. arXiv:0902.4750 [hep-ph]
79. Nardi E., Sannino F., and Strumia A. JCAP 0903 (2009) 009. arXiv:0811.4153
80. Arvanitaki A., et al. arXiv:0812.2075
81. Hisano J., Kawasaki M., Kohri K., Moroi T., and Nakayama K. arXiv:0901.3582 [hep-ph]
82. Belikov A.V., and Hooper D. arXiv:0904.1210 [hep-ph]
83. Galli S., Iocco F., Bertone G., and Melchiorri A. Phys. Rev. D 80 (2009) 023505. arXiv:0905.0003
84. Slatyer T.R., Padmanabhan N., and Finkbeiner D.P. Phys. Rev. D 80 (2009) 043526. arXiv:0906.1197
85. Huetsi G., Hektor A., and Raidal M. arXiv:0906.4550
86. Cirelli M., Iocco F., and Panci P. arXiv:0907.0719
87. Cyr-Racine F.Y., Profumo S., and Sigurdson K. arXiv:0904.3933 [astro-ph.CO]
88. Moskalenko I.V., and Strong A.W. Astrophys. J. 493 (1998) 694. arXiv:astro-ph/9710124
89. Baltz E.A., and Edsjo J. Phys. Rev. D 59 (1999) 023511. arXiv:astro-ph/9808243
90. Strong A.W., and Moskalenko I.V. arXiv:astro-ph/9906228
91. Porter T.A., and Strong A.W. arXiv:astro-ph/0507119
92. Moskalenko I.V., and Strong A.W. Astrophys. J. 528 (2000) 357. arXiv:astro-ph/9811284
93. Bergstrom L., Edsjo J., and Zaharijas G. arXiv:0905.0333 [astro-ph.HE]