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- W3089601595 abstract "Working within the post-Minkowskian approach to General Relativity, we prove that the radiation-reaction to the emission of gravitational waves during the large-impact-parameter scattering of two (classical) point masses modifies the conservative scattering angle by an additional contribution of order $G^3$ which involves a high-energy (or massless) logarithmic divergence of opposite sign to the one contained in the third-post-Minkowskian result of Bern et al. [Phys. Rev. Lett. {bf 122}, 201603 (2019)]. The high-energy limit of the resulting radiation-reaction-corrected (classical) scattering angle is finite, and is found to agree with the one following from the (quantum) eikonal-phase result of Amati, Ciafaloni and Veneziano [ Nucl. Phys. B {bf 347}, 550 (1990)]." @default.
- W3089601595 created "2020-10-08" @default.
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- W3089601595 date "2020-12-01" @default.
- W3089601595 modified "2023-10-17" @default.
- W3089601595 title "Radiative contribution to classical gravitational scattering at the third order in <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>G</mml:mi></mml:math>" @default.
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- W3089601595 doi "https://doi.org/10.1103/physrevd.102.124008" @default.
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