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Amplitudes for astrophysicists: known knowns
Authors:Daniel J Burger  Raúl Carballo-Rubio  Jeff Murugan  Amanda Weltman
Institution:1.The Laboratory for Quantum Gravity and Strings,University of Cape Town,Rondebosch,South Africa;2.The Cosmology and Gravity Group, Department of Mathematics and Applied Mathematics,University of Cape Town,Rondebosch,South Africa;3.SISSA, International School for Advanced Studies,Trieste,Italy;4.INFN Sezione di Trieste,Trieste,Italy;5.School of Natural Sciences,Institute for Advanced Study,Princeton,USA;6.Department of Astrophysical Sciences, Peyton Hall,Princeton University,Princeton,USA
Abstract:The use of quantum field theory to understand astrophysical phenomena is not new. However, for the most part, the methods used are those that have been developed decades ago. The intervening years have seen some remarkable developments in computational quantum field theoretic tools. In particle physics, this technology has facilitated calculations that, even ten years ago would have seemed laughably difficult. It is remarkable, then, that most of these new techniques have remained firmly within the domain of high energy physics. We would like to change this. As alluded to in the title, this paper is aimed at showcasing the use of modern on-shell methods in the context of astrophysics and cosmology. In this article, we use the old problem of the bending of light by a compact object as an anchor to pedagogically develop these new computational tools. Once developed, we then illustrate their power and utility with an application to the scattering of gravitational waves.
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