Publication:
Dark matter and Higgs sector

Loading...
Thumbnail Image
Full text at PDC
Publication Date
2011
Authors
Montes de Oca Y, Jose H.
Prado, Lilian
Advisors (or tutors)
Editors
Journal Title
Journal ISSN
Volume Title
Publisher
IOP Publishing
Citations
Google Scholar
Research Projects
Organizational Units
Journal Issue
Abstract
The inert doublet model is an extension of the Standard Model of Elementary Particles that is defined by the only addition of a second Higgs doublet without couplings to quarks or leptons. This minimal framework has been studied for many reasons. In particular, it has been suggested that the new degrees of freedom contained in this doublet can account for the Dark Matter of the Universe.
Description
© 2011 IOP Publishing Ltd. International Workshop on the Dark Side of the Universe (6º. 2010. Guanajuato, México). This work is supported in part by CONACYT, DOE grant DOE/DE-FG02-94ER40823, FPA 2005-02327 project (DGICYT, Spain), CAM/UCM 910309 project, and MICINN Consolider-Ingenio MULTIDARK CSD2009-00064.
Unesco subjects
Keywords
Citation
[1] P. Jordan, Nature (London) 164, 637 (1949); M. Fierz, Helv. Phys. Acta 29, 128 (1956); C. Brans and R. Dicke, Phys. Rev. 124, 925 (1961); P. G. Bergmann, Int. J. Theor. Phys. 1, 25 (1968); K. Nordtvedt, Astrophys. J. 161, 1059 (1970); R. Wagoner, Phys. Rev. D1, 3209 (1970); T. Damour and K. Nordtvedt, Phys. Rev. Lett. 70, 2217 (1993); ibid., Phys. Rev. D 48, 3436 (1993); T. Damour and B. Pichon, Phys. Rev. D 59, 123502 (1999) [astro-ph/9807176]; C. Schimd, J. P. Uzan, and A. Riazuelo, Phys. Rev. D 71, 083512 (2005); J. A. R. Cembranos, Phys. Rev. D 73, 064029 (2006) [arXiv:gr-qc/0507039]; AIP Conf. Proc. 1182, 288 (2009) [arXiv:0906.5297 [astro-ph.CO]]; J. A. R. Cembranos, K. A. Olive, M. Peloso and J. P. Uzan, JCAP 0907, 025 (2009) [0905.1989 [astro-ph.CO]]; A. de la Cruz-Dombriz et al., Phys. Rev. D 74, 087501 (2006) [gr-qc/0607118]; Phys. Rev. D 77, 123515 (2008) [0802.2999 [astro-ph]]; A. Coc, K. A. Olive, J. P. Uzan and E. Vangioni, Phys. Rev. D 73, 083525 (2006) [astro-ph/0601299]; [0811.1845 [astro-ph]]. [2] E. Witten, Nucl. Phys. B 268, 253 (1986); V. A. Kostelecky and S. Samuel, Phys. Lett. B 207, 169 (1988); Nucl. Phys. B 336, 263 (1990); I. Y. Aref’eva, A. S. Koshelev, D. M. Belov and P. B. Medvedev, Nucl. Phys. B 638, 3 (2002) [arXiv:hep-th/0011117]; I. Y. Aref’eva, L. V. Joukovskaya and A. S. Koshelev, JHEP 0309, 012 (2003) [arXiv:hep-th/0301137]; M. Fujita and H. Hata, Phys. Rev. D 70, 086010 (2004) [arXiv:hep-th/0403031]; T. Biswas, J. A. R. Cembranos and J. I. Kapusta, Phys. Rev. Lett. 104, 021601 (2010) [arXiv:0910.2274 [hep-th]]; arXiv:1005.0430 [hep-th]; arXiv:1006.4098 [hep-th]. [3] L. Bergstrm and A.Goobar, Cosmology and Particle Astrophysics (Springer, 2006). [4] E.W. Kolb and M.S. Turner, The Early Universe (Addison-Wesley, 1990) [5] M. Srednicki, R. Watkins and K.A. Olive, Nucl. Phys. B310, 693 (1988). [6] P. Gondolo and G. Gelmini, Nucl. Phys. B360, 145 (1991). [7] L. Covi, J. E. Kim and L. Roszkowski, Phys. Rev. Lett. 82, 4180 (1999) [hep-ph/9905212]; J. L. Feng, A. Rajaraman and F. Takayama, Phys. Rev. D 68, 085018 (2003) [hep-ph/0307375]; J. L. Feng, A. Rajaraman and F. Takayama, Int. J. Mod. Phys. D 13, 2355 (2004) [hep-th/0405248]; J. A. R. Cembranos, J. L. Feng, A. Rajaraman and F. Takayama, Phys. Rev. Lett. 95, 181301 (2005) [hep-ph/0507150]; J. A. R. Cembranos, J. L. Feng, L E. Strigari, Phys. Rev. D 75, 036004 (2007) [hepph/0612157]; 0708.0247 [hep-ph]; Phys. Rev. Lett. 99, 191301 (2007) [0704.1658 [astro-ph]]; 0708.0239[hepph]; J. A. R. Cembranos, Phys. Rev. Lett. 102, 141301 (2009)[arXiv:0809.1653 [hep-ph]]. [8] H. Goldberg, Phys. Rev. Lett. 50, 1419 (1983). [9] J. R. Ellis et al., Nucl. Phys. B 238, 453 (1984). [10] G. Servant and T. M. P. Tait, Nucl. Phys. B 650, 391 (2003) [hep-ph/0206071]. [11] H. C. Cheng, J. L. Feng and K. T. Matchev, Phys. Rev. Lett. 89, 211301 (2002) [hep-ph/0207125]. [12] J. A. R. Cembranos, A. Dobado and A. L. Maroto, Phys. Rev. Lett. 90, 241301 (2003) [hep-ph/0302041]; and Phys. Rev. D 68, 103505 (2003) [hep-ph/0307062]. [13] J. Alcaraz et al., Phys. Rev.D67, 075010 (2003) [hep-ph/0212269]; J. A. R. Cembranos, A. Dobado and A. L. Maroto, AIP Conf.Proc. 670, 235 (2003) [hep-ph/0301009]; hep-ph/0402142; hep-ph/0406076; Int. J. Mod. Phys. D13, 2275 (2004) [hep-ph/0405165]; hep-ph/0411076; astro-ph/0411262; Phys. Rev. D 73, 035008 (2006) [hep-ph/0510399]; astro-ph/0503622; astro-ph/0512569; astro-ph/0611911; A. L. Maroto, Phys. Rev. D 69, 043509 (2004) [hep-ph/0310272]; Phys. Rev. D 69, 101304 (2004) [hepph/0402278]; J. A. R. Cembranos et al., 0708.0235 [hep-ph]; JCAP 0810, 039 (2008) [0803.0694 [astro-ph]]; J. A. R. Cembranos and L. E. Strigari, Phys. Rev. D 77, 123519 (2008) [0801.0630 [astro-ph]]. [14] P. Achard et al., Phys. Lett. B597, 145 (2004) [hep-ex/0407017]; S. Heinemeyer et al., hep-ph/0511332; J. A. R. Cembranos, A. Rajaraman and F. Takayama, hep-ph/0512020; Europhys. Lett. 82, 21001 (2008) [hep-ph/0609244]; J. A. R. Cembranos, A. Dobado and A. L. Maroto, hep-ph/0107155; Phys. Rev. D65 026005 (2002) [hep-ph/0106322]; hep-ph/0307015; Phys. Rev. D70, 096001 (2004) [hep-ph/0405286]; hep-ph/0512302; Phys. Rev. D 73, 057303 (2006) [hep-ph/0507066]; J. Phys. A 40, 6631 (2007) [hepph/0611024]; A. Juste et al., hep-ph/0601112; J. A. R. Cembranos et al., hep-ph/0603067; AIP Conf. Proc. 903, 591 (2007) [hep-ph/0701011]; ILC Collaboration, 0709.1893 [hep-ph]; 0712.1950 [physics.accph]; 0712.2356 [physics.ins-det]; [15] T.D. Lee, Phys. Rev. D8, 1226 (1973). [16] S.L. Glashow and S. Weinberg, Phys. Rev. D15, 1958 (1977). [17] J.F. Donoghue and L. F. Li, Phys. Rev. D19, 945 (1979). [18] H.E. Haber, G.L. Kane and T. Sterling, Nucl. Phys. B161, 493 (1979). [19] L.J. Hall and M.B. Wise, Nucl. Phys. B187, 397 (1981). [20] J. F. Gunion, H. E. Haber, G. Kane and S. Dawson, The Higgs Hunters Guide (Perseus Publishing, 1990). [21] A. Dege and I.P. Ivanov, Phys. Rev. D. 81, 015012 (2010) [arXiv:0910.4492 [hep-ph]]. [22] D. Kominis and R. Sekhar Chivukula, hep-ph/9301222 [23] E.M. Dolle and S. Su, Phys. Rev. D 80, 055012 (2009) [arXiv:0906.1609v1 [hep-ph]]. [24] E.Ma, Phys. Rev. D 73, 077301 (2006) [arXiv hep-ph/0601225]. [25] M. Cirelli, N. Fornengo and A. Sturmia, Nucl. Phys. B753, 178-194 (2006) [arXiv hep-ph/0512090]. [26] R.Barbieri, L. J. Hall and V. S. Rychkov, Phys Rev D 74 015007 (2006) [arXiv hep-ph/0603188]. [27] L. López-Honorez, E. Nezri, J. F. Oliver and M. H. G. Tytgat, JCAP 02 (2007) 028 . [28] E. Dolle, X. Miao, S. Su and B. Thomas, arXiv:hep-ph 0909.3094(2009). [29] M. Krawczyk, arXiv:hep-ph 0512371 (2005); M. Krawczyk and D. Sokolowska, arXiv:hep-ph 0911.2457 (2009).
Collections