2016
DOI: 10.1007/jhep11(2016)117
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Light-like scattering in quantum gravity

Abstract: We consider scattering in quantum gravity and derive long-range classical and quantum contributions to the scattering of light-like bosons and fermions (spin-0, spin-1 2 , spin-1) from an external massive scalar field, such as the Sun or a black hole. This is achieved by treating general relativity as an effective field theory and identifying the non-analytic pieces of the one-loop gravitational scattering amplitude. It is emphasized throughout the paper how modern amplitude techniques, involving spinor-helici… Show more

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Cited by 118 publications
(188 citation statements)
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“…Moreover, the case can be made that all gravitational theories display some causal uncertainty, due to their spacetime fluctuations. As an example of this we note that even in the effective theory, quantum corrections to the trajectories of massless particles are spin dependent and the particles no longer follow geodesic motion [8]. This makes the concept of a lightcone uncertain.…”
Section: Pacs Numbersmentioning
confidence: 98%
“…Moreover, the case can be made that all gravitational theories display some causal uncertainty, due to their spacetime fluctuations. As an example of this we note that even in the effective theory, quantum corrections to the trajectories of massless particles are spin dependent and the particles no longer follow geodesic motion [8]. This makes the concept of a lightcone uncertain.…”
Section: Pacs Numbersmentioning
confidence: 98%
“…Alternatively, there exist many techniques for using scattering amplitudes to compute classical and quantum corrections to gravitational potentials [38][39][40][41][42][43][44][45][46][47][48][49][50][51], and there has been significant recent progress in obtaining such corrections in the PM approximation [52][53][54][55][56][57].…”
Section: Introductionmentioning
confidence: 99%
“…The only clear information that we have about DM is that very likely it is there and interacts gravitationally with the ordinary matter. If this is the only type of coupling with the ordinary matter or fields, the scattering cross section would be of the infinitesimal order of magnitude O m 2 χ /M 4 P with M P = 1.22 × 10 19 GeV/c 2 is the Planck mass [70]. The simple WIMP model of DM primordial production in the Hot Universe before the Baryogenesis appears to be at the moment seriously questionable, because both the limits from the Fermi-LAT gamma ray telescope and the HEP Collider, that are compatible only with a mass largely in excess of 100 GeV/c 2 ( or ∼400 GeV/c 2 for the compatibility of the LHC Run 2 upper limit with the WIMP's thermal production).…”
Section: Discussionmentioning
confidence: 99%