arXiv · hep-th/0101156
Infrared Behaviour of Massive Scalar Matter coupled to Gravity
Abstract
In the framework of causal perturbation theory we consider a massive scalar field coupled to gravity. In the field theoretic approach to quantum gravity (QG) we start with a massless second rank tensor field. This tensor field is then quantized in a covariant way in Minkowski space. This article deals with the adiabatic limit for graviton radiative corrections in a scattering process of two massive scalar particles. We compute the differential cross-section for bremsstrahlung processes in which one of the outgoing particles emites a graviton of low energy, a so called soft graviton. Since the emited graviton will not be detected we have to integrate over all soft gravitons.
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M. Wellmann. 2001-02-01. Infrared Behaviour of Massive Scalar Matter coupled to Gravity. https://doi.org/10.1006/aphy.2001.6192
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