Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Hu, Yu, Guo, Jun-Qi, Li, Junbin, Shao, Cheng-Gang, Zhang, Hongsheng
Format: Preprint
Veröffentlicht: 2024
Schlagworte:
Online-Zugang:https://arxiv.org/abs/2405.06351
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866929339328626688
author Hu, Yu
Guo, Jun-Qi
Li, Junbin
Shao, Cheng-Gang
Zhang, Hongsheng
author_facet Hu, Yu
Guo, Jun-Qi
Li, Junbin
Shao, Cheng-Gang
Zhang, Hongsheng
contents We study the energy issue in critical collapse of a spherically symmetric scalar field. It is found that in critical collapse, the contribution from the material energy is greater than that from the gravitational energy. The quantity $m/r$ plays an important role in identifying the formation of apparent horizon in gravitational collapse, where $m$ is the Misner-Sharp mass and $r$ the areal radius. We observe that in critical collapse, the maximum value of $m/r$ fluctuates between $2/15$ and $4/15$. This denotes a large gap between critical collapse and black hole formation for which the criterion is $m/r=1/2$.
format Preprint
id arxiv_https___arxiv_org_abs_2405_06351
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Energy in critical collapse
Hu, Yu
Guo, Jun-Qi
Li, Junbin
Shao, Cheng-Gang
Zhang, Hongsheng
General Relativity and Quantum Cosmology
We study the energy issue in critical collapse of a spherically symmetric scalar field. It is found that in critical collapse, the contribution from the material energy is greater than that from the gravitational energy. The quantity $m/r$ plays an important role in identifying the formation of apparent horizon in gravitational collapse, where $m$ is the Misner-Sharp mass and $r$ the areal radius. We observe that in critical collapse, the maximum value of $m/r$ fluctuates between $2/15$ and $4/15$. This denotes a large gap between critical collapse and black hole formation for which the criterion is $m/r=1/2$.
title Energy in critical collapse
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2405.06351