By Adnan Ghribi
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Van Nieuwenhuizen, Nucl. Phys. B147 (1979) 105  M. Yamaguchi, Class. and Quantum Grav. 28 (2011) 103001  H. Murayama, H. Suzuki, T. Yanagida and J. Yokoyama, Phys. Rev. V. Ketov, Quantum Non-linear Sigma-models, Springer-Verlag, 2000  M. Kawasaki, M. Yamaguchi and T. Yanagida, Phys. Rev. Lett. B. Binetruy and G. Dvali, Phys. Lett. B388 (1996) 241  P. Berglund and G. 1397 [hep-th]  P. Berglund and G. 3261 [hep-th]  M. R. Douglas and S. Kachru, Rev. Mod. Phys. 79 (2007) 733  R.
The supersymmetric case is similar: the nonminimal action (164) with the X-function (170) and the superpotential (169) also has only dimensionless coupling constants ξ and λ, while the same it true for the F (R)-supergravity action with the F-function (171), whose coupling constant f 3 is dimensionless too. Therefore, those actions are both superconformal, while inﬂation spontaneously breaks the superconformal invariance. A spontaneous breaking of the conformal symmetry necessarily leads to Goldstone particle (or dilaton) associated with spontaneously broken dilatations.
Endo, F. T. Yanagida, Phys. Rev. D76 (2007) 083509  W. Buchmüller, P. Di Bari and M. Plumacher, Annals of Phys. K. A. Y. Smirnov, Phys. Rev. Lett. 81 (1998) 1359. 0 2 Supersymmetric Dark Matter Csaba Balázs and Daniel Carter Centre of Excellence for Particle Physics at the Terascale and Monash Centre for Astrophysics School of Physics, Monash University Australia 1. Introduction The standard model of particle physics excellently describes all known fundamental particles and forces (with the exception of gravity).
Advances in Modern Cosmology by Adnan Ghribi