Perturbative quantum gravity and Newton's law on a flat Robertson-Walker background

被引:39
作者
Iliopoulos, J
Tomaras, TN
Tsamis, NC
Woodard, RP
机构
[1] Ecole Normale Super, Phys Theor Lab, F-75231 Paris 05, France
[2] Univ Crete, Dept Phys, GR-71003 Iraklion, Greece
[3] Res Ctr Crete, GR-71003 Iraklion, Greece
[4] Univ Florida, Dept Phys, Gainesville, FL 32611 USA
基金
美国国家科学基金会;
关键词
quantum gravity; cosmology;
D O I
10.1016/S0550-3213(98)00528-8
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We derive the Feynman rules for gravity in the presence of a flat Robertson-Walker background and give explicit expressions for the propagator in the physically interesting cases of inflation, radiation domination, and matter domination. The aforementioned background is generated by a scalar field source which should be taken to be dynamical, As an elementary application, we compute the corrections to the Newtonian gravitational force in the present matter dominated era and conclude - as expected - that they are negligible except for the largest scales. (C) 1998 Elsevier Science B.V.
引用
收藏
页码:419 / 446
页数:28
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