RT Journal Article T1 Dark matter and Higgs sector A1 Ruiz Cembranos, José Alberto A1 Montes de Oca Y, Jose H. A1 Prado, Lilian AB 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. PB IOP Publishing SN 1742-6588 YR 2011 FD 2011 LK https://hdl.handle.net/20.500.14352/44918 UL https://hdl.handle.net/20.500.14352/44918 LA spa NO [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). NO © 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. NO Consejo Nacional de Ciencia y Tecnologia (CONACYT), México NO U. S. Department of Energy (DOE) NO Dirección General de Investigación Científica y Técnica (DGICYT), MINECO, España NO Ministerio de Ciencia e Innovación (MICINN), España NO Programa Consolider-Ingenio, MULTIDARK (MICINN), España NO Ministerio de Economía y Competitividad (MINECO), España NO Universidad Complutense de Madrid (UCM) NO Comunidad Autónoma de Madrid (CAM) DS Docta Complutense RD 3 may 2024