Is the cosmic microwave background telling us that dark matter is weaker than weakly interacting?

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 88, Issue 8, 2013, Pages

  Hooper, Dan ^a,b  

^a FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^b UNIVERSITY OF CHICAGO   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 84887110418     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.88.083519     Document Type: Article

References (68)

1. P. A. R. Ade (Planck Collaboration), arXiv:1303.5076.
2. G. Hinshaw (WMAP Collaboration), Astrophys. J. Suppl. Ser. 208, 19 (2013). APJSA2 0067-0049 10.1088/0067-0049/208/2/19
3. Z. Hou, arXiv:1212.6267.
4. J. L. Sievers, arXiv:1301.0824.
5. A. G. Riess, L. Macri, S. Casertano, H. Lampeitl, H. C. Ferguson, A. V. Filippenko, S. W. Jha, W. Li, and R. Chornock, Astrophys. J. 730, 119 (2011); ASJOAB 0004-637X 10.1088/0004-637X/730/2/119
6. A. G. Riess, L. Macri, S. Casertano, H. Lampeit, H. C. Ferguson, A. V. Filippenko, S. W. Jha, W. Li, R. Chornock, and J. M. Silverman, Astrophys. J. 732, 129(E) (2011). ASJOAB 0004-637X 10.1088/0004-637X/732/2/129
7. W. L. Freedman, B. F. Madore, V. Scowcroft, C. Burns, A. Monson, S. E. Persson, M. Seibert, and J. Rigby, Astrophys. J. 758, 24 (2012). ASJOAB 0004-637X 10.1088/0004-637X/758/1/24
8. W. J. Percival (SDSS Collaboration), Mon. Not. R. Astron. Soc. 401, 2148 (2010). MNRAA4 0035-8711 10.1111/j.1365-2966.2009.15812.x
9. N. Padmanabhan, X. Xu, D. J. Eisenstein, R. Scalzo, A. J. Cuesta, K. T. Mehta, and E. Kazin, Mon. Not. R. Astron. Soc. 427, 2132 (2012). MNRAA4 0035-8711 10.1111/j.1365-2966.2012.21888.x
10. C. Blake, Mon. Not. R. Astron. Soc. 418, 1707 (2011). MNRAA4 0035-8711 10.1111/j.1365-2966.2011.19592.x
11. L. Anderson, Mon. Not. R. Astron. Soc. 427, 3435 (2013). MNRAA4 0035-8711 10.1111/j.1365-2966.2012.22066.x
12. F. Beutler, C. Blake, M. Colless, D. Heath Jones, L. Staveley-Smith, L. Campbell, Q. Parker, W. Saunders, and F. Watson, Mon. Not. R. Astron. Soc. 416, 3017 (2011). MNRAA4 0035-8711 10.1111/j.1365-2966.2011.19250.x
13. K. Ichikawa, M. Kawasaki, K. Nakayama, M. Senami, and F. Takahashi, J. Cosmol. Astropart. Phys. JCAPBP 1475-7516 05 (2007) 008. 10.1088/1475-7516/2007/ 05/008
14. W. Fischler and J. Meyers, Phys. Rev. D 83, 063520 (2011). PRVDAQ 1550-7998 10.1103/PhysRevD.83.063520
15. J. Hasenkamp, Phys. Lett. B 707, 121 (2012). PYLBAJ 0370-2693 10.1016/j.physletb.2011.12.017
16. J. L. Menestrina and R. J. Scherrer, Phys. Rev. D 85, 047301 (2012). PRVDAQ 1550-7998 10.1103/PhysRevD.85.047301
17. T. Kobayashi, F. Takahashi, T. Takahashi, and M. Yamaguchi, J. Cosmol. Astropart. Phys. JCAPBP 1475-7516 03 (2012) 036. 10.1088/1475-7516/2012/03/036
18. D. Hooper, F. S. Queiroz, and N. Y. Gnedin, Phys. Rev. D 85, 063513 (2012). PRVDAQ 1550-7998 10.1103/PhysRevD.85.063513
19. K. S. Jeong and F. Takahashi, J. High Energy Phys. JHEPFG 1029-8479 08 (2012) 017. 10.1007/JHEP08(2012)017
20. T. Higaki, K. Kamada, and F. Takahashi, J. High Energy Phys. JHEPFG 1029-8479 09 (2012) 043. 10.1007/JHEP09(2012)043
21. K. Choi, K.-Y. Choi, and C. S. Shin, Phys. Rev. D 86, 083529 (2012). PRVDAQ 1550-7998 10.1103/PhysRevD.86.083529
22. P. Graf and F. D. Steffen, J. Cosmol. Astropart. Phys. JCAPBP 1475-7516 02 (2013) 018. 10.1088/1475-7516/2013/02/018
23. M. Cicoli, J. P. Conlon, and F. Quevedo, Phys. Rev. D 87, 043520 (2013). PRVDAQ 1550-7998 10.1103/PhysRevD.87.043520
24. T. Higaki and F. Takahashi, J. High Energy Phys. JHEPFG 1029-8479 11 (2012) 125. 10.1007/JHEP11(2012)125
25. M. C. Gonzalez-Garcia, V. Niro, and J. Salvado, J. High Energy Phys. JHEPFG 1029-8479 04 (2013) 052. 10.1007/JHEP04(2013)052
26. K. J. Bae, H. Baer, and A. Lessa, J. Cosmol. Astropart. Phys. JCAPBP 1475-7516 04 (2013) 041. 10.1088/1475-7516/2013/04/041
27. K. S. Jeong and F. Takahashi, J. High Energy Phys. JHEPFG 1029-8479 04 (2013) 121. 10.1007/JHEP04(2013)121
28. P. Graf and F. D. Steffen, arXiv:1302.2143.
29. J. P. Conlon and M. C. D. Marsh, arXiv:1304.1804.
30. J. P. Conlon and M. C. D. Marsh, arXiv:1305.3603.
31. C. Kelso, S. Profumo, and F. S. Queiroz, Phys. Rev. D 88, 023511 (2013). PRVDAQ 1550-7998 10.1103/PhysRevD.88.023511
32. S. Angus, J. P. Conlon, U. Haisch, and A. J. Powell, arXiv:1305.4128.
33. J. Hasenkamp and J. Kersten, J. Cosmol. Astropart. Phys. JCAPBP 1475-7516 08 (2013) 024. 10.1088/1475-7516/2013/08/024
34. T. Moroi and L. Randall, Nucl. Phys. B570, 455 (2000). NUPBBO 0550-3213 10.1016/S0550-3213(99)00748-8
35. K. Choi, A. Falkowski, H. P. Nilles, and M. Olechowski, Nucl. Phys. B718, 113 (2005). NUPBBO 0550-3213 10.1016/j.nuclphysb.2005.04.032 (Pubitemid 40771454)
36. B. S. Acharya, P. Kumar, K. Bobkov, G. Kane, J. Shao, and S. Watson, J. High Energy Phys. JHEPFG 1029-8479 06 (2008) 064. 10.1088/1126-6708/2008/06/064
37. R. Blumenhagen, J. P. Conlon, S. Krippendorf, S. Moster, and F. Quevedo, J. High Energy Phys. JHEPFG 1029-8479 09 (2009) 007. 10.1088/1126-6708/2009/09/ 007
38. B. de Carlos, J. A. Casas, F. Quevedo, and E. Roulet, Phys. Lett. B 318, 447 (1993). PYLBAJ 0370-2693 10.1016/0370-2693(93)91538-X
39. G. D. Coughlan, W. Fischler, E. W. Kolb, S. Raby, and G. G. Ross, Phys. Lett. 131B, 59 (1983). PYLBAJ 0370-2693 10.1016/0370-2693(83)91091-2
40. J. R. Ellis, D. V. Nanopoulos, and M. Quiros, Phys. Lett. B 174, 176 (1986). PYLBAJ 0370-2693 10.1016/0370-2693(86)90736-7
41. T. Banks, D. B. Kaplan, and A. E. Nelson, Phys. Rev. D 49, 779 (1994). PRVDAQ 0556-2821 10.1103/PhysRevD.49.779
42. T. Higaki, K. Nakayama, and F. Takahashi, J. High Energy Phys. JHEPFG 1029-8479 07 (2013) 005. 10.1007/JHEP07(2013)005
43. D. J. H. Chung, E. W. Kolb, and A. Riotto, Phys. Rev. D 60, 063504 (1999). PRVDAQ 0556-2821 10.1103/PhysRevD.60.063504 (Pubitemid 40632806)
44. N. Fornengo, A. Riotto, and S. Scopel, Phys. Rev. D 67, 023514 (2003). PRVDAQ 0556-2821 10.1103/PhysRevD.67.023514 (Pubitemid 44796925)
45. C. Pallis, Astropart. Phys. 21, 689 (2004). APHYEE 0927-6505 10.1016/j.astropartphys.2004.05.006 (Pubitemid 39216315)
46. G. B. Gelmini and P. Gondolo, Phys. Rev. D 74, 023510 (2006). PRVDAQ 1550-7998 10.1103/PhysRevD.74.023510
47. G. Gelmini, P. Gondolo, A. Soldatenko, and C. E. Yaguna, Phys. Rev. D 74, 083514 (2006). PRVDAQ 1550-7998 10.1103/PhysRevD.74.083514 (Pubitemid 44601579)
48. R. Allahverdi, B. Dutta, R. N. Mohapatra, and K. Sinha, Phys. Rev. Lett. 111, 051302 (2013). PRLTAO 0031-9007 10.1103/PhysRevLett.111.051302
49. M. Kamionkowski and M. S. Turner, Phys. Rev. D 42, 3310 (1990). PRVDAQ 0556-2821 10.1103/PhysRevD.42.3310
50. S. Watson, in Perspectives on Supersymmetry II, edited by, G. L. Kane, (World Scientific, Singapore, 2010), pp. 305-324.
51. For an up-to-date summary, see https://twiki.cern.ch/twiki/bin/view/ AtlasPublic/SupersymmetryPublicResults and https://twiki.cern.ch/twiki/bin/view/ CMSPublic/PhysicsResultsSUS.
52. For these calculations, we have used the publicly available tool micrOMEGAs: G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, Nuovo Cimento Soc. Ital. Fis. C 33, 111 (2010). NIFCAS 0390-5551
53. E. Aprile (XENON100 Collaboration), Phys. Rev. Lett. 109, 181301 (2012). PRLTAO 0031-9007 10.1103/PhysRevLett.109.181301
54. K. Griest and D. Seckel, Phys. Rev. D 43, 3191 (1991). PRVDAQ 0556-2821 10.1103/PhysRevD.43.3191
55. D. Hooper, C. Kelso, P. Sandick, and W. Xue, Phys. Rev. D 88, 015010 (2013). PRVDAQ 1550-7998 10.1103/PhysRevD.88.015010
56. T. Han, Z. Liu, and A. Natarajan, arXiv:1303.3040.
57. O. Buchmueller, Eur. Phys. J. C 72, 2243 (2012). EPCFFB 1434-6044 10.1140/epjc/s10052-012-2243-3
58. N. Arkani-Hamed, A. Delgado, and G. F. Giudice, Nucl. Phys. B741, 108 (2006); NUPBBO 0550-3213 10.1016/j.nuclphysb.2006.02.010 (Pubitemid 43422598)
59. M. Farina, M. Kadastik, D. Pappadopulo, J. Pata, M. Raidal, and A. Strumia, Nucl. Phys. B853, 607 (2011); NUPBBO 0550-3213 10.1016/j.nuclphysb. 2011.08.003
60. C. Cheung, L. J. Hall, D. Pinner, and J. T. Ruderman, J. High Energy Phys. JHEPFG 1029-8479 05 (2013) 100. 10.1007/JHEP05(2013)100
61. J. L. Feng, K. T. Matchev, and D. Sanford, Phys. Rev. D 85, 075007 (2012). PRVDAQ 1550-7998 10.1103/PhysRevD.85.075007
62. D. S. Akerib (LUX Collaboration), Astropart. Phys. 45, 34 (2013). APHYEE 0927-6505 10.1016/j.astropartphys.2013.02.001
63. E. Aprile (XENON1T Collaboration), arXiv:1206.6288.
64. For a model independent treatment, see M. Beltran, D. Hooper, E. W. Kolb, and Z. C. Krusberg, Phys. Rev. D 80, 043509 (2009). PRVDAQ 1550-7998 10.1103/PhysRevD.80.043509
65. G. Steigman, B. Dasgupta, and J. F. Beacom, Phys. Rev. D 86, 023506 (2012). PRVDAQ 1550-7998 10.1103/PhysRevD.86.023506
66. A. Geringer-Sameth and S. M. Koushiappas, Phys. Rev. Lett. 107, 241303 (2011). PRLTAO 0031-9007 10.1103/PhysRevLett.107.241303
67. M. Ackermann (Fermi-LAT Collaboration), Phys. Rev. Lett. 107, 241302 (2011). PRLTAO 0031-9007 10.1103/PhysRevLett.107.241302
68. D. Hooper, C. Kelso, and F. S. Queiroz, Astropart. Phys. 46, 55 (2013). APHYEE 0927-6505 10.1016/j.astropartphys.2013.04.007