Loosely trapped surface for slowly rotating black hole

Fuente: arXiv
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Auteurs principaux: Izumi, Keisuke, Shiromizu, Tetsuya, Yoshida, Daisuke, Tomikawa, Yoshimune, Yoshino, Hirotaka
Format: Preprint
Publié: 2024
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author Izumi, Keisuke
Shiromizu, Tetsuya
Yoshida, Daisuke
Tomikawa, Yoshimune
Yoshino, Hirotaka
author_facet Izumi, Keisuke
Shiromizu, Tetsuya
Yoshida, Daisuke
Tomikawa, Yoshimune
Yoshino, Hirotaka
contents We construct the marginal loosely trapped surface (marginal LTS) for the Kerr spacetime with a small Kerr parameter perturbatively, where the LTS condition is saturated. An LTS is a surface that specifies the strong gravity region, which is a generalization of the photon sphere in the Schwarzschild spacetime. It turns out that there are an infinite number of marginal LTSs. At the leading order of the small Kerr parameter, all of the marginal LTSs have the same area. However, one can see that the maximal marginal LTS among them is uniquely determined at the higher order.
format Preprint
id arxiv_https___arxiv_org_abs_2407_04175
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Loosely trapped surface for slowly rotating black hole
Izumi, Keisuke
Shiromizu, Tetsuya
Yoshida, Daisuke
Tomikawa, Yoshimune
Yoshino, Hirotaka
General Relativity and Quantum Cosmology
We construct the marginal loosely trapped surface (marginal LTS) for the Kerr spacetime with a small Kerr parameter perturbatively, where the LTS condition is saturated. An LTS is a surface that specifies the strong gravity region, which is a generalization of the photon sphere in the Schwarzschild spacetime. It turns out that there are an infinite number of marginal LTSs. At the leading order of the small Kerr parameter, all of the marginal LTSs have the same area. However, one can see that the maximal marginal LTS among them is uniquely determined at the higher order.
title Loosely trapped surface for slowly rotating black hole
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2407.04175