The top quark and Higgs boson masses and the stability of the electroweak vacuum, S. Alekhin, A. Djouadi, S. Moch (see also: arXiv:1205.2893)


En conclusiones se: escribió:
it would open a wide range of interesting possibilities for new physics model building such as asymptotically safe gravitational theories 1 or inflation models that use the standard Higgs particle as the inflaton 2
1 See for instance Asymptotic safety of gravity and the Higgs boson mass.(external link) By Mikhail Shaposhnikov, Christof Wetterich. [arXiv:0912.0208 hep-th]. Phys.Lett. B683 (2010) 196-200.
2 See for instance, F. Bezrukov and M. Shaposhnikov, Phys.Lett. B659, 703 (2008); I. Masina and A. Notari, Phys.Rev.Lett. 108, 191302 (2012).

En la Introducción de 1 se escribió:
Within this setting a very economical description of all interactions in Nature may be possible. One can assume that there is no new physics associated with any intermediate energy scale (such as Grand Unified scale or low energy supersymmetry) between the weak scale and ktr. All confirmed observational signals in favor of physics beyond the Standard Model as neutrino masses and oscillations, dark matter and dark energy, baryon asymmetry of the Universe and inflation can be associated with new physics below the electroweak scale, for reviews see 20 and 21 and references therein. The minimal model—νMSM, contains, in addition to the SM particles, 3 relatively light singlet Majorana fermions and the dilaton. These fermions could be responsible for neutrino masses, dark matter and baryon asymmetry of the Universe. The dilaton may lead to dynamical dark energy 22 and 23 and realizes spontaneously broken scale invariance which either emerges from the cosmological approach to a fixed point 22 and 24 or is an exact quantum symmetry 25 and 26. Inflation can take place either due to the SM Higgs 2 or due to the asymptotically safe character of gravity 28. Yet another part of new physics, related, for example, to the strong CP problem or to the flavor problem, may be associated with the Planck energy. In this Letter we show that this scenario leads to a prediction of the Higgs mass, which can be tested at the LHC.


20 M. Shaposhnikov, arXiv:0708.3550 hep-th
21 A. Boyarsky, O. Ruchayskiy, M. Shaposhnikov, Annu. Rev. Nucl. Part. Sci., 59 (2009), p. 191
22 C. Wetterich, Nucl. Phys. B, 302 (1988), p. 668
24 C. Wetterich, Phys. Rev. Lett., 90 (2003), p. 231302; Phys. Rev. Lett., 102 (2009), p. 141303, arXiv:0911.1063 hep-th
25 M. Shaposhnikov, D. Zenhausern, Phys. Lett. B, 671 (2009), p. 187
26 M. Shaposhnikov, D. Zenhausern, Phys. Lett. B, 671 (2009), p. 162