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The third structure function
DOI:10.1088/1361-6382/adcfe9.png)
Abstract
En 中文
We re-consider the graviton self-energy induced by a loop of massless, minimally coupled scalars on de Sitter background. On flat space background it can be represented as a sum of two tensor differential operators acting on scalar structure functions. On a general background these differential operators can be constructed from the linearized Ricci scalar and the linearized Weyl tensor. However, in cosmology one requires a third contribution which we derive here.
Keywords:
de Sitter
quantum gravity
graviton self-energy
structure functions
Journal
IF:
3.7
Papers:
1.3W
Citations:
3.0W

