Abstract
Abstract
Nonlinear sigma models on de Sitter background have proved a useful prototype for quantum gravity in summing the large logarithms which arise from loop corrections. We consider a model whose evolution is described, at leading logarithm order, by the trace of the coincident, doubly differentiated scalar propagator. An analytic approximation for this quantity on an arbitrary expansion history is applied to generalize the resummed de Sitter result to any cosmological background which has experienced primordial inflation. In addition to analytic expressions, we present explicit numerical results for the evolution in a plausible expansion history. The large scales of primordial inflation are transmitted to late times.
Publisher
Springer Science and Business Media LLC
Subject
Nuclear and High Energy Physics
Reference45 articles.
1. R.P. Woodard, Perturbative Quantum Gravity Comes of Age, Int. J. Mod. Phys. D 23 (2014) 1430020 [arXiv:1407.4748] [INSPIRE].
2. A.A. Starobinsky, Spectrum of relict gravitational radiation and the early state of the universe, JETP Lett. 30 (1979) 682 [INSPIRE].
3. V.F. Mukhanov and G.V. Chibisov, Quantum Fluctuations and a Nonsingular Universe, JETP Lett. 33 (1981) 532 [INSPIRE].
4. N.C. Tsamis and R.P. Woodard, One loop graviton selfenergy in a locally de Sitter background, Phys. Rev. D 54 (1996) 2621 [hep-ph/9602317] [INSPIRE].
5. S.P. Miao and R.P. Woodard, The Fermion self-energy during inflation, Class. Quant. Grav. 23 (2006) 1721 [gr-qc/0511140] [INSPIRE].
Cited by
3 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献