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Phys."],"published-print":{"date-parts":[[2022,1]]},"abstract":"<jats:title>A<jats:sc>bstract<\/jats:sc>\n                     <\/jats:title><jats:p>Picture yourself in the wave zone of a gravitational scattering event of two massive, spinning compact bodies (black holes, neutron stars or stars). We show that this system of genuine astrophysical interest enjoys a hidden <jats:inline-formula><jats:alternatives><jats:tex-math>$$ \\mathcal{N} $$<\/jats:tex-math><mml:math xmlns:mml=\"http:\/\/www.w3.org\/1998\/Math\/MathML\">\n                  <mml:mi>N<\/mml:mi>\n                <\/mml:math><\/jats:alternatives><\/jats:inline-formula> = 2 supersymmetry, at least to the order of spin-squared (quadrupole) interactions in arbitrary <jats:italic>D<\/jats:italic> spacetime dimensions. Using the <jats:inline-formula><jats:alternatives><jats:tex-math>$$ \\mathcal{N} $$<\/jats:tex-math><mml:math xmlns:mml=\"http:\/\/www.w3.org\/1998\/Math\/MathML\">\n                  <mml:mi>N<\/mml:mi>\n                <\/mml:math><\/jats:alternatives><\/jats:inline-formula> = 2 supersymmetric worldline action, augmented by finite-size corrections for the non-Kerr black hole case, we build a quadratic-in-spin extension to the worldline quantum field theory (WQFT) formalism introduced in our previous work, and calculate the two bodies\u2019 deflection and spin kick to sub-leading order in the post-Minkowskian expansion in Newton\u2019s constant <jats:italic>G<\/jats:italic>. For spins aligned to the normal vector of the scattering plane we also obtain the scattering angle. All <jats:italic>D<\/jats:italic>-dimensional observables are derived from an eikonal phase given as the free energy of the WQFT that is invariant under the <jats:inline-formula><jats:alternatives><jats:tex-math>$$ \\mathcal{N} $$<\/jats:tex-math><mml:math xmlns:mml=\"http:\/\/www.w3.org\/1998\/Math\/MathML\">\n                  <mml:mi>N<\/mml:mi>\n                <\/mml:math><\/jats:alternatives><\/jats:inline-formula> = 2 supersymmetry transformations.<\/jats:p>","DOI":"10.1007\/jhep01(2022)027","type":"journal-article","created":{"date-parts":[[2022,1,8]],"date-time":"2022-01-08T16:02:41Z","timestamp":1641657761000},"update-policy":"https:\/\/doi.org\/10.1007\/springer_crossmark_policy","source":"Crossref","is-referenced-by-count":114,"title":["SUSY in the sky with gravitons"],"prefix":"10.1007","volume":"2022","author":[{"given":"Gustav Uhre","family":"Jakobsen","sequence":"first","affiliation":[]},{"given":"Gustav","family":"Mogull","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0003-2883-7825","authenticated-orcid":false,"given":"Jan","family":"Plefka","sequence":"additional","affiliation":[]},{"given":"Jan","family":"Steinhoff","sequence":"additional","affiliation":[]}],"member":"297","published-online":{"date-parts":[[2022,1,7]]},"reference":[{"key":"17519_CR1","doi-asserted-by":"publisher","first-page":"048","DOI":"10.1007\/JHEP02(2021)048","volume":"02","author":"G Mogull","year":"2021","unstructured":"G. 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