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Inert Higgs doublet extension of the NMSSM
Phys. Rev. D 89, 075016 – Published 25 April, 2014
DOI: https://doi.org/10.1103/PhysRevD.89.075016
Abstract
We introduce one pair of inert Higgs doublets and singlets , and consider their couplings with the Higgs doublets of the minimal supersymmetric standard model (MSSM), . We assign extra gauge charges only to the extra vectorlike superfields, and so all the MSSM superfields remain neutral under the new . They can be an extension of the “ term,” in the next-to MSSM (NMSSM). Because of the , the maximally allowed low energy value of can be lifted up to 0.85, avoiding a Landau pole (LP) below the grand unification scale. Such colorless vectorlike superfields remarkably enhance the radiative MSSM Higgs mass particularly for large through the term and the corresponding holomorphic soft term. As a result, the lower bound of and the upper bound of can be relaxed to disappear from the restricted parameter space of the original NMSSM, and for a light stop, . Thus, the valid parameter space significantly expands up to , , and , evading the LP problem and also explaining the 126 GeV Higgs mass naturally.
Article Text
References (32)
- G. Aad et al. (ATLAS Collaboration), Phys. Lett. B 716, 1 (2012); S. Chatrchyan et al. (CMS Collaboration), 716, 30 (2012).
- For a review, for instance, see M. Drees, R. Godbole, and P. Roy, Theory and Phenomenology of Sparticles: An Account of Four-Dimensional N=1 Supersymmetry in High Energy Physics (World Scientific, Hackensack, NJ, 2004), and references therein.
- M. S. Carena and H. E. Haber, Prog. Part. Nucl. Phys. 50, 63 (2003); See also A. Djouadi, Phys. Rep. 459, 1 (2008).
- ATLAS Collaboration, Report No. ATLAS-CONF-2013-024; S. Chatrchyan et al. (CMS Collaboration), Eur. Phys. J. C 73, 2677 (2013).
- A. Arvanitaki, M. Baryakhtar, X. Huang, K. Van Tilburg, and G. Villadoro, J. High Energy Phys. 03 (2014) 022.
- ATLAS Collaboration, Report No. ATLAS-CONF-2013-061.
- J.-H. Huh and B. Kyae, Phys. Lett. B 726, 729 (2013).
- E. Hardy, J. High Energy Phys. 10 (2013) 133.
- N. Arkani-Hamed and H. Murayama, Phys. Rev. D 56, R6733 (1997).
- H. Abe, T. Kobayashi, and Y. Omura, Phys. Rev. D 76, 015002 (2007); D. Horton and G. G. Ross, Nucl. Phys. B830, 221 (2010); J. E. Younkin and S. P. Martin, Phys. Rev. D 85, 055028 (2012); H. Abe, J. Kawamura, and H. Otsuka, Prog. Theor. Exp. Phys. 2013, 013B02 (2013); I. Gogoladze, F. Nasir, and Q. Shafi, Int. J. Mod. Phys. A 28, 1350046 (2013).
- For a review, see U. Ellwanger, C. Hugonie, and A. M. Teixeira, Phys. Rep. 496, 1 (2010).
- For other types of singlet extensions of the MSSM, see, for instance, A. Delgado, C. Kolda, J. P. Olson, and A. de la Puente, Phys. Rev. Lett. 105, 091802 (2010); G. G. Ross and K. Schmidt-Hoberg, Nucl. Phys. B862, 710 (2012); B. Kyae and J.-C. Park, Phys. Rev. D 86, 031701 (2012); 87, 075021 (2013).
- L. J. Hall, D. Pinner, and J. T. Ruderman, J. High Energy Phys. 04 (2012) 131; E. Hardy, J. March-Russell, and J. Unwin, 10 (2012) 072.
- M. Masip, R. Munoz-Tapia, and A. Pomarol, Phys. Rev. D 57, R5340 (1998); For more recent discussions, see also R. Barbieri, D. Pappadopulo, V. S. Rychkov, L. J. Hall, and A. Y. Papaioannou, J. High Energy Phys. 03 (2008) 005.
- B. Kyae and C. S. Shin, Phys. Rev. D 88, 015011 (2013).
- B. Kyae and C. S. Shin, J. High Energy Phys. 06 (2013) 102.
- For early studies on vectorlike matter, see T. Moroi and Y. Okada, Mod. Phys. Lett. A 07, 187 (1992); Phys. Lett. B 295, 73 (1992); K. S. Babu, I. Gogoladze, and C. Kolda, arXiv:hep-ph/0410085; M. Endo, K. Hamaguchi, S. Iwamoto, and N. Yokozaki, Phys. Rev. D 84, 075017 (2011); T. Moroi, R. Sato, and T. T. Yanagida, Phys. Lett. B 709, 218 (2012); K. J. Bae, T. H. Jung, and H. D. Kim, Phys. Rev. D 87, 015014 (2013); W.-Z. Feng and P. Nath, 87, 075018 (2013); K. S. Babu, I. Gogoladze, M. U. Rehman, and Q. Shafi, 78, 055017 (2008).
- A. Joglekar, P. Schwaller, and C. E. M. Wagner, J. High Energy Phys. 07 (2013) 046.
- S. P. Martin, Phys. Rev. D 81, 035004 (2010).
- K.-Y. Choi, B. Kyae, and C. S. Shin, Phys. Rev. D 89, 055002 (2014).
- J. E. Kim and H. P. Nilles, Phys. Lett. 138B, 150 (1984).
- G. F. Giudice and A. Masiero, Phys. Lett. B 206, 480 (1988).
- S. M. Barr, Phys. Lett. 112B, 219 (1982); J. P. Derendinger, J. E. Kim, and D. V. Nanopoulos, 139B, 170 (1984); I. Antoniadis, J. R. Ellis, J. S. Hagelin, and D. V. Nanopoulos, Phys. Lett. B 194, 231 (1987).
- For instance, see J.-H. Huh, J. E. Kim, and B. Kyae, Phys. Rev. D 80, 115012 (2009); J. E. Kim, J.-H. Kim, and B. Kyae, J. High Energy Phys. 06 (2007) 034; See also J. E. Kim and B. Kyae, Nucl. Phys. B770, 47 (2007); Phys. Rev. D 77, 106008 (2008); K.-S. Choi and B. Kyae, Nucl. Phys. B855, 1 (2012).
- S. R. Coleman and E. J. Weinberg, Phys. Rev. D 7, 1888 (1973).
- K. Nakayama, N. Yokozaki, and K. Yonekura, J. High Energy Phys. 11 (2011) 021.
- M. S. Carena, M. Quiros, and C. E. M. Wagner, Nucl. Phys. B461, 407 (1996).
- P. Langacker, G. Paz, L.-T. Wang, and I. Yavin, Phys. Rev. Lett. 100, 041802 (2008); Phys. Rev. D 77, 085033 (2008).
- J. Beringer et al. (Particle Data Group), Phys. Rev. D 86, 010001 (2012); Phys. Lett. B 667, 1 (2008).
- M. Baak, M. Goebel, J. Haller, A. Hoecker, D. Kennedy, R. Kogler, K. Mönig, M. Schott, and J. Stelzer, Eur. Phys. J. C 72, 2205 (2012).
- S. P. Martin, K. Tobe, and J. D. Wells, Phys. Rev. D 71, 073014 (2005).
- B. Kyae (work in progress).