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Anapole dark matter at the LHC
Phys. Rev. D 89, 045006 – Published 12 February, 2014
DOI: https://doi.org/10.1103/PhysRevD.89.045006
Abstract
The anapole moment is the only allowed electromagnetic moment for Majorana fermions. Fermionic dark matter acquiring an anapole can have a standard thermal history and be consistent with current direct detection experiments. In this paper, we calculate the collider monojet signatures of anapole dark matter and show that the current LHC results exclude anapole dark matter with mass less than 100 GeV, for an anapole coupling that leads to the correct thermal relic abundance.
Article Text
References (32)
- L. D. Duffy and K. van Bibber, New J. Phys. 11, 105008 (2009).
- P. Langacker and G. Steigman, Phys. Rev. D 84, 065040 (2011).
- M. Pospelov and T. ter Veldhuis, Phys. Lett. B 480, 181 (2000).
- K. Sigurdson, M. Doran, A. Kurylov, R. R. Caldwell, and M. Kamionkowski, Phys. Rev. D 70, 083501 (2004); 73, 089903(E) (2006).
- S. Gardner, Phys. Rev. D 79, 055007 (2009).
- E. Masso, S. Mohanty, and S. Rao, Phys. Rev. D 80, 036009 (2009).
- A. L. Fitzpatrick and K. M. Zurek, Phys. Rev. D 82, 075004 (2010).
- W. S. Cho, J.-H. Huh, I.-W. Kim, J. E. Kim, and B. Kyae, Phys. Lett. B 687, 6 (2010); 694, 496(E) (2011).
- J. H. Heo, Phys. Lett. B 693, 255 (2010).
- J. H. Heo, Phys. Lett. B 702, 205 (2011).
- T. Banks, J.-F. Fortin, and S. Thomas, arXiv:1007.5515.
- V. Barger, W.-Y. Keung, and D. Marfatia, Phys. Lett. B 696, 74 (2011).
- J.-F. Fortin and T. M. P. Tait, Phys. Rev. D 85, 063506 (2012).
- E. Del Nobile C. Kouvaris, P. Panci, F. Sannino, and J. Virkajarvi, J. Cosmol. Astropart. Phys. 08 (2012) 010.
- V. Barger, W.-Y. Keung, D. Marfatia, and P.-Y. Tseng, Phys. Lett. B 717, 219 (2012).
- J. H. Heo and C. S. Kim, Phys. Rev. D 87, 013007 (2013).
- Ya. B. Zel’dovich, Sov. Phys. JETP 6, 1184 (1958).
- C. M. Ho and R. J. Scherrer, Phys. Lett. B 722, 341 (2013).
- A. L. Fitzpatrick and K. M. Zurek, Phys. Rev. D 82, 075004 (2010).
- Y. Bai, P. J. Fox, and R. Harnik, J. High Energy Phys. 12 (2010) 048; P. J. Fox, R. Harnik, J. Kopp, and Y. Tsai, Phys. Rev. D 85, 056011 (2012).
- P. J. Fox, R. Harnik, J. Kopp, and Y. Tsai, Phys. Rev. D 84, 014028 (2011).
- L. M. Carpenter, A. Nelson, C. Shimmin, T. M. P. Tait, and D. Whiteson, Phys. Rev. D 87, 074005 (2013).
- A. A. Petrov and W. Shepherd, arXiv:1311.1511; L. Carpenter, A. DiFranzo, M. Mulhearn, C. Shimmin, S. Tulin, and D. Whiteson, arXiv:1312.2592.
- T. Hapola, M. Jarvinen, C. Kouvaris, P. Panci, and J. Virkajarvi, arXiv:1309.6326.
- J. Pumplin, D. R. Stump, J. Huston, H. L. Lai, P. M. Nadolsky, and W. K. Tung, J. High Energy Phys. 07 (2002) 012.
- Cern Report No. CMS-PAS-EXO-12-048, available at http://cds.cern.ch/record/1525585?ln=en.
- Cern Report No. ATLAS-CONF-2012-147, http://cds.cern.ch/record/1493486.
- R. J. Scherrer and M. S. Turner, Phys. Rev. D 33, 1585 (1986).
- E. W. Kolb and M. S. Turner, The Early Universe (Addison-Wesley, New York, 1990).
- P. A. R. Ade et al., arXiv:1303.5076.
- E. Aprile et al., Phys. Rev. Lett. 109, 181301 (2012).
- D. S. Akerib et al. (LUX Collaboration), arXiv:1310.8214.