2023
DOI: 10.1007/jhep02(2023)107
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The ultrarelativistic limit of Kerr

Abstract: The massless (or ultrarelativistic) limit of a Schwarzschild black hole with fixed energy was determined long ago in the form of the Aichelburg-Sexl shockwave, but the status of the same limit for a Kerr black hole is less clear. In this paper, we explore the ultrarelativistic limit of Kerr in the class of Kerr-Schild impulsive pp-waves by exploiting a relation between the metric profile and the eikonal phase associated with scattering between a scalar and the source of the metric. This gives a map between can… Show more

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Cited by 12 publications
(2 citation statements)
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“…This connects our work again to an important set of ideas in the literature relating scattering amplitudes to classical physics. The fact that perturbative amplitudes, in the classical regime, can be resummed into an exponential form is the key idea of the eikonal approximation [85,86,[89][90][91][92][93][94][95][96][97][98][99][100][101][102][103][104]. A closely-related resummation connects scattering amplitudes to the classical radial action and the Hamilton-Jacobi equation [105][106][107].…”
Section: Discussionmentioning
confidence: 99%
“…This connects our work again to an important set of ideas in the literature relating scattering amplitudes to classical physics. The fact that perturbative amplitudes, in the classical regime, can be resummed into an exponential form is the key idea of the eikonal approximation [85,86,[89][90][91][92][93][94][95][96][97][98][99][100][101][102][103][104]. A closely-related resummation connects scattering amplitudes to the classical radial action and the Hamilton-Jacobi equation [105][106][107].…”
Section: Discussionmentioning
confidence: 99%
“…This is a topic which has been considered many times in the past, often by using a ladder approximation in the Bethe-Salpeter equation [46][47][48], but this is not sufficient to establish a direct connection to classical bound states when relativistic effects are relevant. 1 Other approaches (e.g., making use of 'generalized ladder' approximations) have gotten closer [49][50][51][52][53][54][55][56], but all these attempts are at least partially incomplete due to lacking an appropriate classical limit at amplitude level [7,57] or failing to recover probe limit results [13,14,[58][59][60][61][62][63] at leading order in the resummation.…”
Section: A Exponentiation Of the 3-pt Function For The Classical Lore...mentioning
confidence: 99%