Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1997-10-24
Phys.Lett. B426 (1998) 21-28
Physics
High Energy Physics
High Energy Physics - Phenomenology
14 pages, plain TeX, 7 Postscript files, uses psfig.sty
Scientific paper
10.1016/S0370-2693(98)00159-2
We consider the effect of various particles on the cosmic expansion rate relative to that of the graviton. Effectively massless fermions, gauge bosons and conformally coupled scalars make only minuscule contributions due to local conformal invariance. Minimally coupled scalars can give much stronger contributions, but they are still sub-dominant to those of gravitons on account of global conformal invariance. Unless effectively massless scalar particles with very particular couplings exist, the leading effect on the expansion rate is furnished solely by the graviton. An upper bound on the mass of such scalar particles is obtained.
Tsamis Nicholas C.
Woodard Richard P.
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