Work

Late-time behavior of stellar collapse and explosions. II. Nonlinear evolution

Year: 1994

Type: article

Abstract: We compare the predictions of linearized theory for the radiation produced in the collapse of a spherically symmetric scalar field with a full numerical integration of the Einstein equations. We find power-law tails and quasinormal ringing remarkably similar to predictions of linearized theory even in cases where nonlinearities are crucial. We also show that power-law tails develop even when the collapsing scalar field fails to produce a black hole.

Source: Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields

DOI: 10.1103/physrevd.49.890

Authors: Carsten Gundlach, Richard H. Price, Jorge Pullin

Institution: University of Utah

Language: English

Topic: Pulsars and Gravitational Waves Research

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

Funders: National Science Foundation, University of California, Santa Barbara

OpenAlex ID: W2170786743

FWCI: 13.26

Cites: 13

Cited by: 247

Related to: 9