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Main Authors: Tang, Jining, Huang, Yang, Zhang, Hongsheng
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2412.19157
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author Tang, Jining
Huang, Yang
Zhang, Hongsheng
author_facet Tang, Jining
Huang, Yang
Zhang, Hongsheng
contents Gravitational collapse and bubble evolution in the asymptotical Friedmann-Lemaitre-Robertson-Walker (FLRW) Universe is an intriguing and intricate problem. We systematically analyze dynamics for contact \sch-FLRW (McVittie) spacetimes, focusing on their general junction conditions and introducing a novel function to simplify the extrinsic curvature and surface stress-energy tensor. We explore both static and dynamic scenarios, including special cases such as Schwarzschild, FLRW, and Einstein-Straus configurations by using our general framework. Numerical calculations further reveal the evolution of the concentric McVittie spacetimes with various initial conditions, offering deep insights into the interplay between the McVittie mass parameter and initial peculiar velocity. These results provide a unified perspective for understanding gravitational collapse and bubble evolution in cosmology and astrophysics.
format Preprint
id arxiv_https___arxiv_org_abs_2412_19157
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Matching McVittie spacetimes
Tang, Jining
Huang, Yang
Zhang, Hongsheng
General Relativity and Quantum Cosmology
Gravitational collapse and bubble evolution in the asymptotical Friedmann-Lemaitre-Robertson-Walker (FLRW) Universe is an intriguing and intricate problem. We systematically analyze dynamics for contact \sch-FLRW (McVittie) spacetimes, focusing on their general junction conditions and introducing a novel function to simplify the extrinsic curvature and surface stress-energy tensor. We explore both static and dynamic scenarios, including special cases such as Schwarzschild, FLRW, and Einstein-Straus configurations by using our general framework. Numerical calculations further reveal the evolution of the concentric McVittie spacetimes with various initial conditions, offering deep insights into the interplay between the McVittie mass parameter and initial peculiar velocity. These results provide a unified perspective for understanding gravitational collapse and bubble evolution in cosmology and astrophysics.
title Matching McVittie spacetimes
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2412.19157