Abstract
In this paper, two key issues related to electroweak symmetry breaking are addressed. First, how fine-tuned different models are that trigger this phenomenon? Second, even if a light Higgs boson exists, does it have to be necessarily elementary? After a brief introduction, the fine-tuning aspects of the MSSM, NMSSM, generalized NMSSM and GMSB scenarios shall be reviewed, then the little Higgs, composite Higgs and the Higgsless models shall be compared. Finally, a broad overview will be given on where we stand at the end of 2011.
Similar content being viewed by others
References
G Bhattacharyya, Rep. Prog. Phys. 74, 026201 (2011), arXiv:0910.5095 [hep-ph] and references therein
G F Giudice, arXiv:0801.2562 [hep-ph]
R Contino, arXiv:1005.4269 [hep-ph]
C Grojean, PoSEPS-HEP2009, 008 (2009), arXiv:0910.4976 [hep-ph]
See the textbooks on supersymmetry, R N Mohapatra, Unification and supersymmetry: The frontiers of quark-lepton physics (Springer-Verlag, NY, 1992) M Drees, R M Godbole and P Roy, Theory and phenomenology of sparticles: An account of four-dimensional N=1 supersymmetry in high energy physics (World Scientific, 2004) H Baer and X Tata, Weak scale supersymmetry: From superfields to scattering events (Cambridge University Press, Cambridge, UK, 2006) See also, R K Kaul, Supersymmetry and supergravity, in: Gravitation, gauge theories and the early universe edited by B R Iyer (Kluwer Academic Publishers, 1989) pp. 487–522
R Barbieri and G F Giudice, Nucl. Phys. B306, 63 (1988)
A Strumia, J. High Energy Phys. 1104, 073 (2011), arXiv:1101.2195 [hep-ph]
U Ellwanger, G Espitalier-Noel and C Hugonie, arXiv:1107.2472 [hep-ph]
S Cassel, D M Ghilencea, S Kraml, A Lessa and G G Ross, J. High Energy Phys. 1105, 120 (2011), arXiv:1101.4664 [hep-ph]
For reviews on NMSSM, see U Ellwanger, C Hugonie and A M Teixeira, Phys. Rep. 496, 1 (2010), arXiv:0910.1785 [hep-ph] M Maniatis, Int. J. Mod. Phys. A25, 3505 (2010), arXiv:0906.0777 [hep-ph]
M Drees, Int. J. Mod. Phys. A4, 3635 (1989)
G G Ross and K Schmidt-Hoberg, arXiv:1108.1284 [hep-ph]
S A Abel, S Sarkar and P L White, Nucl. Phys. B454, 663 (1995), arXiv:hep-ph/9506359
P Lodone, J. High Energy Phys. 1005, 068 (2010), arXiv:1004.1271 [hep-ph]
G Bhattacharyya and A Romanino, Phys. Rev. D55, 7015 (1997), arXiv:hep-ph/9611243
M Schmaltz and D Tucker-Smith, Ann. Rev. Nucl. Part. Sci. 55, 229 (2005), arXiv:hep-ph/0502182 M Perelstein, Prog. Part. Nucl. Phys. 58, 247 (2007), arXiv:hep-ph/0512128 M C Chen, Mod. Phys. Lett. A21, 621 (2006), arXiv:hep-ph/0601126
H C Cheng, arXiv:0710.3407 [hep-ph]
R K Kaul, arXiv:0803.0381 [hep-ph]
C Csaki, J Hubisz, G D Kribs, P Meade and J Terning, Phys. Rev. D67, 115002 (2003), arXiv:hep-ph/0211124 J L Hewett, F J Petriello and T G Rizzo, J. High Energy Phys. 0310, 062 (2003), arXiv:hep-ph/0211218 M C Chen and S Dawson, Phys. Rev. D70, 015003 (2004), arXiv:hep-ph/0311032
I Low, J. High Energy Phys. 0410, 067 (2004), arXiv:hep-ph/0409025 H C Cheng and I Low, J. High Energy Phys. 0408, 061 (2004), arXiv:hep-ph/0405243
J Hubisz, P Meade, A Noble and M Perelstein, J. High Energy Phys. 0601, 135 (2006), arXiv:hep-ph/0506042
J A Casas, J R Espinosa and I Hidalgo, J. High Energy Phys. 0503, 038 (2005), arXiv:hep-ph/0502066
T Han, H E Logan, B McElrath and L T Wang, Phys. Rev. D67, 095004 (2003), arXiv:hep-ph/0301040
G Burdman, M Perelstein and A Pierce, Phys. Rev. Lett. 90, 241802 (2003), Erratum, ibid. 92, 049903 (2004), arXiv:hep-ph/0212228
M Perelstein, M E Peskin and A Pierce, Phys. Rev. D69, 075002 (2004), arXiv:hep-ph/0310039
K Agashe, R Contino and A Pomarol, Nucl. Phys. B719, 165 (2005), hep-ph/0412089
S Rychkov, arXiv:1109.1180 [hep-ph]
M Serone, New J. Phys. 12, 075013 (2010), arXiv:0909.5619 [hep-ph]
R Contino, Y Nomura and A Pomarol, Nucl. Phys. B671, 148 (2003), arXiv:hep-ph/0306259
J R Espinosa, C Grojean and M Muhlleitner, J. High Energy Phys. 1005, 065 (2010), arXiv:1003.3251 [hep-ph]
R Contino and G Servant, J. High Energy Phys. 0806, 026 (2008), arXiv:0801.1679 [hep-ph]
For a review on Higgsless models, see C Csaki, J Hubisz and P Meade, arXiv:hep-ph/0510275 (TASI Lectures)
C Csaki, C Grojean, H Murayama, L Pilo and J Terning, Phys. Rev. D69, 055006 (2004), arXiv:hep-ph/0305237
R Barbieri, A Pomarol and R Rattazzi, Phys. Lett. B591, 141 (2004), arXiv:hep-ph/0310285 G Cacciapaglia, C Csaki, C Grojean and J Terning, Phys. Rev. D70, 075014 (2004), arXiv:hep-ph/0401160 H Davoudiasl, J L Hewett, B Lillie and T G Rizzo, Phys. Rev. D70, 015006 (2004), arXiv:hep-ph/0312193
A Birkedal, K Matchev and M Perelstein, Phys. Rev. Lett. 94, 191803 (2005), arXiv:hep-ph/0412278
R Barbieri, B Bellazzini, V S Rychkov and A Varagnolo, Phys. Rev. D76, 115008 (2007), arXiv:0706.0432 [hep-ph] J R Espinosa, C Grojean and M Muhlleitner, J. High Energy Phys. 1005, 065 (2010), arXiv:1003.3251 [hep-ph]
M E Peskin, arXiv:1110.3805 [hep-ph], These proceedings
R Heuer, Whither Colliders After LHC, These proceedings
H Bachacou, BSM Results from LHC, These proceedings
Acknowledgements
The author would like to acknowledge the hospitality of the CERN PH/TH Division during the writing of this draft and also would like to thank Emilian Dudas, Christophe Grojean, Palash B Pal, and Amitava Raychaudhuri for discussions and clarifications on several issues.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
BHATTACHARYYA, G. Electroweak symmetry breaking beyond the Standard Model. Pramana - J Phys 79, 675–690 (2012). https://doi.org/10.1007/s12043-012-0370-x
Published:
Issue Date:
DOI: https://doi.org/10.1007/s12043-012-0370-x