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Gauge-invariant quantum gravity corrections to Callan-Symanzik beta functions via the Vilkovisky-DeWitt method and gravity-assisted gauge unification
Phys. Rev. D 83, 125014 – Published 10 June, 2011
DOI: https://doi.org/10.1103/PhysRevD.83.125014
Abstract
Gravity is the weakest force in nature, and the gravitational interactions with all standard model (SM) particles can be well described by perturbative expansions of the Einstein-Hilbert action as an effective theory, all the way up to energies below the fundamental Planck scale. We use the Vilkovisky-DeWitt method to derive the first gauge-invariant nonzero gravitational power-law corrections to the Callan-Symanzik beta functions which make both Abel and non-Abel gauge interactions asymptotically free. We further demonstrate that the graviton-induced universal power-law runnings always assist the three SM gauge forces to reach unification around the Planck scale, irrespective of the detail of logarithmic corrections. We further compute the power-law corrections to the SM Higgs sector and derive modified triviality bound on the Higgs boson mass.
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[23] for the metric
which only differs from that in the present Eq.
(16) by an overall factor 2; this slightly changes the summed coefficient
in Eq.
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, but with the same sign. As a result, the present
-function
(32) has its coefficient
slightly different from its previous value
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