- Access by Xinjiang University
Dark matter from hidden forces
Phys. Rev. D 89, 055026 – Published 25 March, 2014
DOI: https://doi.org/10.1103/PhysRevD.89.055026
Abstract
We examine the possibility that dark matter may be the manifestation of dark forces of a hidden sector, i.e. “.” As an illustrative and minimal example we consider the hidden gauge group. The hidden dynamics is indirectly coupled to the Standard Model (SM) through kinetic mixing of with the of hypercharge. We assume a hidden symmetry-breaking pattern analogous to that of the SM electroweak symmetry, augmented with an extra scalar that allows both the “hidden boson” and the “hidden photon” to be massive. The “hidden ” bosons are dark matter in this scenario. This generic setup can readily accommodate potential direct detection signals for light dark matter. For some choices of parameters, the model can lead to signals both in “dark matter beam” experiments, from , as well as in experiments that look for visible signals of dark photons, mediated by . Other possible phenomenological consequences are also briefly discussed.
Article Text
References (56)
- P. A. R. Ade et al. (Planck Collaboration), arXiv:1303.5076.
- O. Adriani et al. (PAMELA Collaboration), Nature (London) 458, 607 (2009). See also Refs. [3,4]
- M. Ackermann et al. (Fermi LAT Collaboration), Phys. Rev. Lett. 108, 011103 (2012).
- M. Aguilar et al. (AMS Collaboration), Phys. Rev. Lett. 110, 141102 (2013).
- N. Arkani-Hamed, D. P. Finkbeiner, T. R. Slatyer, and N. Weiner, Phys. Rev. D 79, 015014 (2009).
- R. Bernabei et al. (DAMA and LIBRA Collaborations), Eur. Phys. J. C 67, 39 (2010).
- C. E. Aalseth et al. (CoGeNT Collaboration), Phys. Rev. D 88, 012002 (2013).
- G. Angloher et al., Eur. Phys. J. C 72, 1971 (2012); A. Brown, S. Henry, H. Kraus, and C. McCabe, Phys. Rev. D 85, 021301 (2012).
- F. Petriello and K. M. Zurek, J. High Energy Phys. 09 (2008) 047; C. Savage, G. Gelmini, P. Gondolo, and K. Freese, J. Cosmol. Astropart. Phys. 04 (2009) 010; A. L. Fitzpatrick, D. Hooper, and K. M. Zurek, Phys. Rev. D 81, 115005 (2010); S. Chang, J. Liu, A. Pierce, N. Weiner, and I. Yavin, J. Cosmol. Astropart. Phys. 08 (2010) 018; V. Barger, M. McCaskey, and G. Shaughnessy, Phys. Rev. D 82, 035019 (2010); W.-Y. Keung, I. Low, and G. Shaughnessy, 82, 115019 (2010); M. R. Buckley, D. Hooper, and T. M. P. Tait, Phys. Lett. B 702, 216 (2011); K.-Y. Choi and O. Seto, Phys. Rev. D 88, 035005 (2013); R. C. Cotta, A. Rajaraman, T. M. P. Tait, and A. M. Wijangco, arXiv:1305.6609 [Phys. Rev. D (to be published)]; M. McCullough and L. Randall, J. Cosmol. Astropart. Phys. 10 (2013) 058.
- R. Agnese et al. (CDMS Collaboration), Phys. Rev. Lett. 111, 251301 (2013).
- For example of DM models based on such considerations see R. Foot, Int. J. Mod. Phys. D 13, 2161 (2004); M. Cirelli, N. Fornengo, and A. Strumia, Nucl. Phys. B753, 178 (2006); M. Pospelov, A. Ritz, and M. B. Voloshin, Phys. Lett. B 662, 53 (2008).
- T. Hambye, J. High Energy Phys. 01 (2009) 028; T. Hambye and M. H. G. Tytgat, Phys. Lett. B 683, 39 (2010); J. L. Diaz-Cruz and E. Ma, 695, 264 (2011); S. Bhattacharya, J. L. Diaz-Cruz, E. Ma, and D. Wegman, Phys. Rev. D 85, 055008 (2012); F. D’Eramo, M. McCullough, and J. Thaler, J. Cosmol. Astropart. Phys. 04 (2013) 030; T. Hambye and A. Strumia, Phys. Rev. D 88, 055022 (2013). C. D. Carone and R. Ramos, 88, 055020 (2013).
- C.-W. Chiang, T. Nomura, and J. Tandean, arXiv:1306.0882.
- J. D. Bjorken, R. Essig, P. Schuster, and N. Toro, Phys. Rev. D 80, 075018 (2009).
- M. Reece and L.-T. Wang, J. High Energy Phys. 07 (2009) 051.
- S. Andreas, C. Niebuhr, and A. Ringwald, Phys. Rev. D 86, 095019 (2012).
- F. Bossi, in KLOE-2 Physics Workshop, Frascati, Italy, April 9–10, 2009 (unpublished); P.-f. Yin, J. Liu, and S.-h. Zhu, Phys. Lett. B 679, 362 (2009).
- H. Merkel et al. (A1 Collaboration), Phys. Rev. Lett. 106, 251802 (2011).
- S. Abrahamyan et al. (APEX Collaboration), Phys. Rev. Lett. 107, 191804 (2011).
- S. N. Gninenko, Phys. Lett. B 713, 244 (2012); arXiv:1308.6521 [Phys. Rev. D (to be published)].
- R. Essig, P. Schuster, and N. Toro, Phys. Rev. D 80, 015003 (2009); B. Batell, M. Pospelov, and A. Ritz, 79, 115008 (2009); 80, 095024 (2009).
- P. Adlarson et al. (WASA-at-COSY Collaboration), Phys. Lett. B 726, 187 (2013).
- S. N. Gninenko, Phys. Rev. D 87, 035030 (2013).
- R. M. Drees et al. (SINDRUM I Collaboration), Phys. Rev. Lett. 68, 3845 (1992).
- Y. Yamaguchi on behalf of the PHENIX Collaboration, in Proceedings of the 2013 Fall Meeting of the APS Division of Nuclear Physics, Newport News, VA, October 23–26, 2013 (to be published).
- D. Babusci et al. (KLOE-2 Collaboration), Phys. Lett. B 720, 111 (2013).
- H. Davoudiasl, H.-S. Lee, and W. J. Marciano, Phys. Rev. D 86, 095009 (2012).
- M. Endo, K. Hamaguchi, and G. Mishima, Phys. Rev. D 86, 095029 (2012).
- P. Fayet, Phys. Rev. D 75, 115017 (2007).
- M. Pospelov, Phys. Rev. D 80, 095002 (2009).
- H. Davoudiasl, H.-S. Lee, and W. J. Marciano, Phys. Rev. Lett. 109, 031802 (2012).
- G. W. Bennett et al. (Muon G-2 Collaboration), Phys. Rev. D 73, 072003 (2006).
- B. Wojtsekhowski, D. Nikolenko, and I. Rachek, arXiv:1207.5089.
- J. R. Boyce (LIPSS, DarkLight, HPS and APEX Collaborations), J. Phys. Conf. Ser. 384, 012008 (2012).
- H. Davoudiasl, H.-S. Lee, and W. J. Marciano, Phys. Rev. D 85, 115019 (2012).
- H.-C. Cheng, K. T. Matchev, and M. Schmaltz, Phys. Rev. D 66, 036005 (2002); G. Servant and T. M. P. Tait, Nucl. Phys. B 650, 391 (2003); H.-C. Cheng, J. L. Feng, and K. T. Matchev, Phys. Rev. Lett. 89, 211301 (2002); D. Hooper and G. D. Kribs, Phys. Rev. D 70, 115004 (2004).
- H.-C. Cheng and I. Low, J. High Energy Phys. 09 (2003) 051; 08 (2004) 061; A. Birkedal, A. Noble, M. Perelstein, and A. Spray, Phys. Rev. D 74, 035002 (2006).
- O. Lebedev, H. M. Lee, and Y. Mambrini, Phys. Lett. B 707, 570 (2012); T. Abe, M. Kakizaki, S. Matsumoto, and O. Seto, 713, 211 (2012); Y. Farzan and A. R. Akbarieh, J. Cosmol. Astropart. Phys. 10 (2012) 026; S. Baek, P. Ko, W.-I. Park, and E. Senaha, J. High Energy Phys. 05 (2013) 036; K.-Y. Choi, H. M. Lee, and O. Seto, Phys. Rev. D 87, 123541 (2013).
- B. Holdom, Phys. Lett. 166B, 196 (1986).
- Some recent works that employ kinetic mixing between the Standard Model and dark gauge sector include S. Gopalakrishna, S. Jung, and J. D. Wells, Phys. Rev. D 78, 055002 (2008); A. Hook, E. Izaguirre, and J. G. Wacker, Adv. High Energy Phys. 2011, 859762 (2011); Y. Mambrini, J. Cosmol. Astropart. Phys. 09 (2010) 022; 07 (2011) 009; A. Alves, E. R. Barreto, A. G. Dias, C. A. de S. Pires, F. S. Queiroz, and P. S. Rodrigues da Silva, Phys. Rev. D 84, 115004 (2011); A. Alves, A. G. Dias, E. Ramirez Barreto, C. A. de S.Pires, F. S.Queiroz, and P. S. Rodrigues da Silva, Eur. Phys. J. C 73, 2288 (2013).
- For discussions of non-Abelian dark gauge sectors, see M. Baumgart, C. Cheung, J. T. Ruderman, L.-T. Wang, and I. Yavin, J. High Energy Phys. 04 (2009) 014; F. Chen, J. M. Cline, and A. R. Frey, Phys. Rev. D 80, 083516 (2009); H. Zhang, C. S. Li, Q.-H. Cao and Z. Li, 82, 075003 (2010); C. D. Carone, Phys. Lett. B 721, 118 (2013); D. G. E. Walker, arXiv:1202.2348.
- J. Beringer et al. (Particle Data Group Collaboration), Phys. Rev. D 86, 010001 (2012).
- E. Kolb and M. Turner, The Early Universe (Westview Press, Boulder, CO, 1990).
- R. Bernabei et al., Phys. Lett. B 389, 757 (1996); M. Pospelov and T. ter Veldhuis, 480, 181 (2000).
- D. S. Akerib et al. (LUX Collaboration), arXiv:1310.8214 [Phys. Rev. Lett. (to be published)].
- J. Angle et al. (XENON10 Collaboration), Phys. Rev. Lett. 107, 051301 (2011); , 110, 249901(E) (2013).
See also Ref. [47].
- M. T. Frandsen, F. Kahlhoefer, C. McCabe, S. Sarkar, and K. Schmidt-Hoberg, J. Cosmol. Astropart. Phys. 07 (2013) 023.
- E. Aprile et al. (XENON100 Collaboration), Phys. Rev. Lett. 109, 181301 (2012).
- R. Agnese et al. (CDMS Collaboration), Phys. Rev. D 88, 031104 (2013).
- R. Agnese et al., Phys. Rev. Lett. 112, 041302 (2014).
- D. Hooper, J. Cosmol. Astropart. Phys. 09 (2013) 035.
- G. Belanger, A. Goudelis, J.-C. Park and A. Pukhov, arXiv:1311.0022; M. I. Gresham and K. M. Zurek, Phys. Rev. D 89, 016017 (2014); E. Del Nobile, G. B. Gelmini, P. Gondolo, and J.-H. Huh, arXiv:1311.4247; V. Cirigliano, M. L. Graesser, G. Ovanesyan, and I. M. Shoemaker, arXiv:1311.5886.
- B. Batell, M. Pospelov, and A. Ritz, Phys. Rev. D 80, 095024 (2009); P. deNiverville, M. Pospelov, and A. Ritz, 84, 075020 (2011); P. deNiverville, D. McKeen and A. Ritz, 86, 035022 (2012); R. Dharmapalan et al. (MiniBooNE Collaboration), arXiv:1211.2258.
- E. Izaguirre, G. Krnjaic, P. Schuster, and N. Toro, Phys. Rev. D 88, 114015 (2013); M. D. Diamond and P. Schuster, Phys. Rev. Lett. 111, 221803 (2013).
- M. Srednicki, R. Watkins, and K. A. Olive, Nucl. Phys. B310, 693 (1988).
- H. Davoudiasl, H.-S. Lee, I. Lewis, and W. J. Marciano, Phys. Rev. D 88, 015022 (2013).