Acausality from a Dark Sector

Article, Preprint English OPEN
Carone, Christopher D.;
(2014)

Solutions to the hierarchy problem that require partners for each standard model particle often require that these states live at or above the electroweak scale, to satisfy phenomenological bounds. Partners to possible dark sector particles may be significantly lighter,... View more
  • References (15)
    15 references, page 1 of 2

    [1] O. Adriani, et al., PAMELA Collaboration, Nature 458 (2009) 607.

    [2] A.A. Abdo, et al., Fermi LAT Collaboration, Phys. Rev. Lett. 102 (2009) 181101.

    [3] Most recently: M. Aguilar, et al., AMS Collaboration, Phys. Rev. Lett. 110 (14) (2013) 141102.

    [4] N. Arkani-Hamed, D.P. Finkbeiner, T.R. Slatyer, N. Weiner, Phys. Rev. D 79 (2009) 015014.

    [5] M. Heikinheimo, A. Racioppi, M. Raidal, C. Spethmann, K. Tuominen, Nucl. Phys. B 876 (2013) 201; C. Cheung, J.T. Ruderman, L.-T. Wang, I. Yavin, Phys. Rev. D 80 (2009) 035008; S. Andreas, M.D. Goodsell, A. Ringwald, Phys. Rev. D 87 (2013) 025007; Y.F. Chan, M. Low, D.E. Morrissey, A.P. Spray, J. High Energy Phys. 1205 (2012) 155.

    [6] K.L. McDonald, D.E. Morrissey, J. High Energy Phys. 1005 (2010) 056; K.L. McDonald, D.E. Morrissey, J. High Energy Phys. 1102 (2011) 087.

    [7] B. Grinstein, D. O'Connell, M.B. Wise, Phys. Rev. D 77 (2008) 025012.

    [8] F.A. Barone, G. Flores-Hidalgo, A.A. Nogueira, arXiv:1311.2040 [hep-th]; R.F. Lebed, A.J. Long, R.H. TerBeek, Phys. Rev. D 88 (2013) 085014; K. Bhattacharya, Y.-F. Cai, S. Das, Phys. Rev. D 87 (2013) 083511; M. Dias, A.Y. Petrov, C.R. Senise Jr., A.J. da Silva, arXiv:1212.5220; I. Cho, O.-K. Kwon, Eur. Phys. J. C 73 (2013) 2341; I. Cho, O.-K. Kwon, Phys. Rev. D 82 (2010) 025013; R.F. Lebed, R.H. TerBeek, Phys. Rev. D 87 (2013) 015006; R.F. Lebed, R.H. TerBeek, J. High Energy Phys. 1209 (2012) 099; N. Kan, K. Kobayashi, K. Shiraishi, Acta Phys. Pol. B 44 (2013) 721; K. Bhattacharya, S. Das, Phys. Rev. D 86 (2012) 025009; T. Figy, R. Zwicky, J. High Energy Phys. 1110 (2011) 145; T.E.J. Underwood, R. Zwicky, Phys. Rev. D 79 (2009) 035016; K. Bhattacharya, S. Das, Phys. Rev. D 84 (2011) 045023; E. Alvarez, E.C. Leskow, J. Zurita, Phys. Rev. D 83 (2011) 115024; R.S. Chivukula, A. Farzinnia, R. Foadi, E.H. Simmons, Phys. Rev. D 82 (2010) 035015; R.S. Chivukula, A. Farzinnia, R. Foadi, E.H. Simmons, Phys. Rev. D 81 (2010) 095015; C.D. Carone, R. Primulando, Phys. Rev. D 80 (2009) 055020; C.D. Carone, Phys. Lett. B 677 (2009) 306; A. Rodigast, T. Schuster, Phys. Rev. D 79 (2009) 125017; B. Fornal, B. Grinstein, M.B. Wise, Phys. Lett. B 674 (2009) 330; C.D. Carone, R.F. Lebed, J. High Energy Phys. 0901 (2009) 043; C.D. Carone, R.F. Lebed, Phys. Lett. B 668 (2008) 221; T.G. Rizzo, J. High Energy Phys. 0706 (2007) 070; T.G. Rizzo, J. High Energy Phys. 0801 (2008) 042.

    [9] T.D. Lee, G.C. Wick, Nucl. Phys. B 9 (1969) 209; T.D. Lee, G.C. Wick, Phys. Rev. D 2 (1970) 1033.

    [10] R.E. Cutkosky, P.V. Landshoff, D.I. Olive, J.C. Polkinghorne, Nucl. Phys. B 12 (1969) 281.

  • Similar Research Results (4)
  • Related Organizations (3)
  • Metrics
Share - Bookmark