- Access by Xinjiang University
Nonuniversal gaugino masses and seminatural supersymmetry in view of the Higgs boson discovery
Phys. Rev. D 89, 035011 – Published 20 February, 2014
DOI: https://doi.org/10.1103/PhysRevD.89.035011
Abstract
I consider models with nonuniversal gaugino masses at the gauge coupling unification scale, taking into account the Higgs boson discovery. Viable regions of parameter space are mapped and studied in the case of nonuniversality following from an -term in a linear combination of singlet and adjoint representations of . I consider, in particular, “seminatural” models that have small , with gaugino masses dominating the supersymmetry-breaking terms at high energies. Higgsino-like particles are then much lighter than all other superpartners, and the prospects for discovery at the Large Hadron Collider can be extremely challenging.
Article Text
References (146)
- G. Aad et al. (ATLAS Collaboration), Report No. ATLAS-CONF-2013-047, 2013.
- G. Aad et al. (ATLAS Collaboration), Report No. ATLAS-CONF-2013-062, 2013.
- G. Aad et al. (ATLAS Collaboration), arXiv:1308.1841.
- S. Chatrchyan et al. (CMS Collaboration), Report No. CMS-PAS-SUS-13-012.
- D. S. M. Alves, E. Izaguirre, and J. G. Wacker, Phys. Lett. B 702, 64 (2011).
- D. S. M. Alves, E. Izaguirre, and J. G. Wacker, J. High Energy Phys. 10 (2011) 012.
- T. J. LeCompte and S. P. Martin, Phys. Rev. D 84, 015004 (2011).
- T. J. LeCompte and S. P. Martin, Phys. Rev. D 85, 035023 (2012).
- H. Baer, V. Barger, P. Huang, A. Mustafayev, and X. Tata, Phys. Rev. Lett. 109, 161802 (2012).
- J. L. Feng, Annu. Rev. Nucl. Part. Sci. 63, 351 (2013).
- N. Craig, arXiv:1309.0528.
- H. Baer, V. Barger, and D. Mickelson, Phys. Rev. D 88, 095013 (2013).
- J. E. Kim and H. P. Nilles, Phys. Lett. 138B, 150 (1984).
- G. F. Giudice and A. Masiero, Phys. Lett. B 206, 480 (1988).
- U. Ellwanger, C. Hugonie, and A. M. Teixeira, Phys. Rep. 496, 1 (2010).
- M. Papucci, J. T. Ruderman, and A. Weiler, J. High Energy Phys. 09 (2012) 035.
- J. A. Evans, Y. Kats, D. Shih, and M. J. Strassler, arXiv:1310.5758.
- G. L. Kane and J. D. Wells, Phys. Rev. Lett. 76, 4458 (1996).
- G. L. Kane, in Perspectives on Supersymmetry, edited by G. L. Kane (World Scientific, Singapore, 2010), pp. 352–354.
- H. Baer, V. Barger, and P. Huang, J. High Energy Phys. 11 (2011) 031.
- C. Han, A. Kobakhidze, N. Liu, A. Saavedra, L. Wu, and J. M. Yang, arXiv:1310.4274.
- K. L. Chan, U. Chattopadhyay, and P. Nath, Phys. Rev. D 58, 096004 (1998).
- J. L. Feng, K. T. Matchev, and T. Moroi, Phys. Rev. Lett. 84, 2322 (2000).
- J. L. Feng, K. T. Matchev, and T. Moroi, Phys. Rev. D 61, 075005 (2000).
- J. L. Feng, K. T. Matchev, and F. Wilczek, Phys. Lett. B 482, 388 (2000).
- J. L. Feng, K. T. Matchev, and D. Sanford, Phys. Rev. D 85, 075007 (2012).
- J. L. Feng and D. Sanford, Phys. Rev. D 86, 055015 (2012).
- G. L. Kane and S. F. King, Phys. Lett. B 451, 113 (1999).
- M. Bastero-Gil, G. L. Kane, and S. F. King, Phys. Lett. B 474, 103 (2000).
- K. Huitu, J. Laamanen, P. N. Pandita, and S. Roy, Phys. Rev. D 72, 055013 (2005).
- H. Baer, A. Mustafayev, E.-K. Park, S. Profumo, and X. Tata, J. High Energy Phys. 04 (2006) 041.
- K. Huitu, J. Laamanen, P. N. Pandita, and S. Roy, Pramana 69, 823 (2007).
- H. Abe, T. Kobayashi, and Y. Omura, Phys. Rev. D 76, 015002 (2007).
- S. P. Martin, Phys. Rev. D 75, 115005 (2007).
- B. Ananthanarayan and P. N. Pandita, Int. J. Mod. Phys. A 22, 3229 (2007).
- S. P. Martin, Phys. Rev. D 76, 095005 (2007).
- S. F. King, J. P. Roberts, and D. P. Roy, J. High Energy Phys. 10 (2007) 106.
- H. Baer, A. Mustafayev, H. Summy, and X. Tata, J. High Energy Phys. 10 (2007) 088.
- D. Horton and G. G. Ross, Nucl. Phys. B830, 221 (2010).
- N. Okada, S. Raza, and Q. Shafi, Phys. Rev. D 84, 095018 (2011).
- J. E. Younkin and S. P. Martin, Phys. Rev. D 85, 055028 (2012).
- F. Brummer and W. Buchmuller, J. High Energy Phys. 05 (2012) 006.
- S. Caron, J. Laamanen, I. Niessen, and A. Strubig, J. High Energy Phys. 06 (2012) 008.
- S. Antusch, L. Calibbi, V. Maurer, M. Monaco, and M. Spinrath, J. High Energy Phys. 01 (2013) 187.
- I. Gogoladze, F. Nasir, and Q. Shafi, Int. J. Mod. Phys. A 28, 1350046 (2013).
- A. Spies and G. Anton, J. Cosmol. Astropart. Phys. 06 (2013) 022.
- I. Gogoladze, F. Nasir, and Q. Shafi, arXiv:1306.5699.
- T. T. Yanagida and N. Yokozaki, Phys. Lett. B 722, 355 (2013).
- D. J. Miller and A. P. Morais, arXiv:1307.1373.
- M. A. Ajaib, I. Gogoladze, and Q. Shafi, arXiv:1307.4882.
- M. Badziak, M. Olechowski, and S. Pokorski, arXiv:1307.7999.
- T. T. Yanagida and N. Yokozaki, J. High Energy Phys. 11 (2013) 020.
- A. Kaminska, G. G. Ross, and K. Schmidt-Hoberg, J. High Energy Phys. 11 (2013) 209.
- M. E. Cabrera, A. Casas, R. R. de Austri, and G. Bertone, arXiv:1311.7152.
- J. R. Ellis, C. Kounnas, and D. V. Nanopoulos, Nucl. Phys. B247, 373 (1984).
- J. R. Ellis, K. Enqvist, D. V. Nanopoulos, and K. Tamvakis, Phys. Lett. 155B, 381 (1985).
- M. Drees, Phys. Lett. 158B, 409 (1985).
- G. Anderson, C. H. Chen, J. F. Gunion, J. D. Lykken, T. Moroi, and Y. Yamada, arXiv:hep-ph/9609457.
- G. Anderson, H. Baer, C. h. Chen, and X. Tata, Phys. Rev. D 61, 095005 (2000).
- J. Chakrabortty and A. Raychaudhuri, Phys. Lett. B 673, 57 (2009).
- S. P. Martin, Phys. Rev. D 79, 095019 (2009).
- G. Aad et al. (ATLAS Collaboration), Phys. Lett. B 716, 1 (2012).
- S. Chatrchyan et al. (CMS Collaboration), Phys. Lett. B 716, 30 (2012).
- G. Aad et al. (ATLAS Collaboration), Report No. ATLAS-CONF-2013-014, 2013.
- S. Chatrchyan et al. (CMS Collaboration), Report No. CMS-PAS-HIG-12-045, 2012.
- J. R. Ellis, G. Ridolfi, and F. Zwirner, Phys. Lett. B 257, 83 (1991).
- Y. Okada, M. Yamaguchi, and T. Yanagida, Prog. Theor. Phys. 85, 1 (1991).
- H. E. Haber and R. Hempfling, Phys. Rev. Lett. 66, 1815 (1991).
- A. Brignole, Phys. Lett. B 281, 284 (1992).
- P. H. Chankowski, S. Pokorski, and J. Rosiek, Phys. Lett. B 286, 307 (1992).
- P. H. Chankowski, S. Pokorski, and J. Rosiek, Nucl. Phys. B423, 437 (1994).
- R. Hempfling and A. H. Hoang, Phys. Lett. B 331, 99 (1994).
- J. A. Casas, J. R. Espinosa, M. Quiros, and A. Riotto, Nucl. Phys. B436, 3 (1995); B439, 466(E) (1995).
- A. Dabelstein, Z. Phys. C 67, 495 (1995).
- M. S. Carena, J. R. Espinosa, M. Quiros, and C. E. M. Wagner, Phys. Lett. B 355, 209 (1995).
- M. S. Carena, M. Quiros, and C. E. M. Wagner, Nucl. Phys. B461, 407 (1996).
- S. Heinemeyer, W. Hollik, and G. Weiglein, Phys. Rev. D 58, 091701 (1998).
- S. Heinemeyer, W. Hollik, and G. Weiglein, Phys. Lett. B 440, 296 (1998).
- R.-J. Zhang, Phys. Lett. B 447, 89 (1999).
- J. R. Espinosa and R.-J. Zhang, J. High Energy Phys. 03 (2000) 026.
- M. S. Carena, H. E. Haber, S. Heinemeyer, W. Hollik, C. E. M. Wagner, and G. Weiglein, Nucl. Phys. B580, 29 (2000).
- J. R. Espinosa and R.-J. Zhang, Nucl. Phys. B586, 3 (2000).
- G. Degrassi, P. Slavich, and F. Zwirner, Nucl. Phys. B611, 403 (2001).
- A. Brignole, G. Degrassi, P. Slavich, and F. Zwirner, Nucl. Phys. B631, 195 (2002).
- A. Brignole, G. Degrassi, P. Slavich, and F. Zwirner, Nucl. Phys. B643, 79 (2002).
- S. P. Martin, Phys. Rev. D 65, 116003 (2002).
- S. P. Martin, Phys. Rev. D 66, 096001 (2002).
- S. P. Martin, Phys. Rev. D 67, 095012 (2003).
- S. P. Martin, Phys. Rev. D 68, 075002 (2003).
- S. P. Martin, Phys. Rev. D 71, 016012 (2005).
- S. P. Martin and D. G. Robertson, Comput. Phys. Commun. 174, 133 (2006).
- Stephen P. Martin, Phys. Rev. D 75, 055005 (2007).
- R. V. Harlander, P. Kant, L. Mihaila, and M. Steinhauser, Phys. Rev. Lett. 100, 191602 (2008).
- S. Heinemeyer, W. Hollik, and G. Weiglein, Comput. Phys. Commun. 124, 76 (2000).
- S. Heinemeyer, W. Hollik, and G. Weiglein, Eur. Phys. J. C 9, 343 (1999).
- G. Degrassi, S. Heinemeyer, W. Hollik, P. Slavich, and G. Weiglein, Eur. Phys. J. C 28, 133 (2003).
- M. Frank, T. Hahn, S. Heinemeyer, W. Hollik, H. Rzehak, and G. Weiglein, J. High Energy Phys. 02 (2007) 047.
- T. Hahn, S. Heinemeyer, W. Hollik, H. Rzehak, and G. Weiglein, Comput. Phys. Commun. 180, 1426 (2009).
- B. C. Allanach, Comput. Phys. Commun. 143, 305 (2002).
- A. Djouadi, J. L. Kneur, and G. Moultaka, Comput. Phys. Commun. 176, 426 (2007).
- W. Porod, Comput. Phys. Commun. 153, 275 (2003).
- J. S. Lee, A. Pilaftsis, M. S. Carena, S. Y. Choi, M. Drees, J. R. Ellis, and C. E. M. Wagner, Comput. Phys. Commun. 156, 283 (2004).
- J. S. Lee, M. Carena, J. Ellis, A. Pilaftsis, and C. E. M. Wagner, Comput. Phys. Commun. 180, 312 (2009).
- J. S. Lee, M. Carena, J. Ellis, A. Pilaftsis, and C. E. M. Wagner, Comput. Phys. Commun. 184, 1220 (2013).
- F. E. Paige, S. D. Protopopescu, H. Baer, and X. Tata, arXiv:hep-ph/0312045.
- P. Kant, R. V. Harlander, L. Mihaila, and M. Steinhauser, J. High Energy Phys. 08 (2010) 104.
- J. L. Feng, P. Kant, S. Profumo, and D. Sanford, arXiv:1306.2318.
- C. F. Berger, J. S. Gainer, J. L. Hewett, and T. G. Rizzo, J. High Energy Phys. 02 (2009) 023.
- M. W. Cahill-Rowley, J. L. Hewett, A. Ismail, and T. G. Rizzo, Phys. Rev. D 86, 075015 (2012).
- M. Cahill-Rowley, J. L. Hewett, A. Ismail, and T. G. Rizzo, arXiv:1307.8444.
- G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, Comput. Phys. Commun. 180, 747 (2009).
- G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, Comput. Phys. Commun. 176, 367 (2007).
- G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, Comput. Phys. Commun. 174, 577 (2006).
- G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, Comput. Phys. Commun. 149, 103 (2002).
- L. Covi, J. E. Kim, and L. Roszkowski, Phys. Rev. Lett. 82, 4180 (1999).
- L. Covi, H.-B. Kim, J. E. Kim, and L. Roszkowski, J. High Energy Phys. 05 (2001) 033.
- J. L. Feng, A. Rajaraman, and F. Takayama, Phys. Rev. Lett. 91, 011302 (2003).
- K.-Y. Choi, L. Covi, J. E. Kim, and L. Roszkowski, J. High Energy Phys. 04 (2012) 106.
- E. Aprile et al. (XENON100 Collaboration), Phys. Rev. Lett. 109, 181301 (2012).
- D. S. Akerib et al. (LUX Collaboration), arXiv:1310.8214.
- C. L. Bennett et al. (WMAP Collaboration), Astrophys. J. Suppl. Ser. 208, 20 (2013).
- P. A. R. Ade et al. (Planck Collaboration), arXiv:1303.5076.
- E. Cremmer, S. Ferrara, C. Kounnas, and D. V. Nanopoulos, Phys. Lett. 133B, 61 (1983).
- J. R. Ellis, C. Kounnas, and D. V. Nanopoulos, Nucl. Phys. B247, 373 (1984).
- A. B. Lahanas and D. V. Nanopoulos, Phys. Rep. 145, 1 (1987).
- K. Inoue, M. Kawasaki, M. Yamaguchi, and T. Yanagida, Phys. Rev. D 45, 328 (1992).
- D. E. Kaplan, G. D. Kribs, and M. Schmaltz, Phys. Rev. D 62, 035010 (2000).
- Z. Chacko, M. A. Luty, A. E. Nelson, and E. Ponton, J. High Energy Phys. 01 (2000) 003.
- A. Birkedal-Hansen and B. D. Nelson, Phys. Rev. D 64, 015008 (2001).
- H. Baer, A. Mustafayev, E.-K. Park, and S. Profumo, J. High Energy Phys. 07 (2005) 046.
- H. Baer, T. Krupovnickas, A. Mustafayev, E.-K. Park, S. Profumo, and X. Tata, J. High Energy Phys. 12 (2005) 011.
- M. Ibe, A. Kamada, and S. Matsumoto, arXiv:1311.2162.
- N. Arkani-Hamed, A. Delgado, and G. F. Giudice, Nucl. Phys. B741, 108 (2006).
- M. Drees and M. M. Nojiri, Phys. Rev. D 47, 376 (1993).
- M. E. Gomez, G. Lazarides, and C. Pallis, Phys. Rev. D 61, 123512 (2000).
- C. Boehm, A. Djouadi, and M. Drees, Phys. Rev. D 62, 035012 (2000).
- J. R. Ellis, K. A. Olive, and Y. Santoso, Astropart. Phys. 18, 395 (2003).
- C. Balazs, M. Carena, and C. E. M. Wagner, Phys. Rev. D 70, 015007 (2004).
- S. Gori, S. Jung, and L.-T. Wang, arXiv:1307.5952.
- H. Baer, V. Barger, P. Huang, D. Mickelson, A. Mustafayev, W. Sreethawong, and X. Tata, Phys. Rev. Lett. 110, 151801 (2013).
- T. Han, S. Padhi, and S. Su, Phys. Rev. D 88, 115010 (2013).
- G. F. Giudice, T. Han, K. Wang, and L.-T. Wang, Phys. Rev. D 81, 115011 (2010).
- B. Dutta, A. Gurrola, W. Johns, T. Kamon, P. Sheldon, and K. Sinha, Phys. Rev. D 87, 035029 (2013).
- A. G. Delannoy, B. Dutta, A. Gurrola, W. Johns, T. Kamon, E. Luiggi, A. Melo, P. Sheldon et al., Phys. Rev. Lett. 111, 061801 (2013).
- D. McKinsey and R. Gaitskell (for the LUX Collaboration), at Sanford Underground Research Facility, 2013 (unpublished).
- K. Arisaka (for the XENON Collaboration), in Snowmass on the Mississippi (CSS 2013), 2013 (unpublished).