You need JavaScript to view this
ETDEWEB   /       /    Dressing up a Kerr naked singularity

Dressing up a Kerr naked singularity

Journal Article:

SAVE / SHARE

XML RIS EndNote CSV/Excel JSON

Abstract

The evolution of a naked singularity surrounded by an accreting disk of matter is studied; two kinds of disks are considered: the standard thin-disk model and the thick barytropic model, for several initial conditions. It is shown that any Kerr naked singularity slows down in a finite time to a maximal Kerr black hole. The final mass, the luminosity and the time of evolution of the singularity are evaluated.
Authors:
Calvani, M; [1]  Nobili, L [2] 
  1. Padua Univ. (Italy). Ist. di Astronomia
  2. Padua Univ. (Italy). Ist. di Fisica
Publication Date:
Jun 11, 1979
DOI:
https://doi.org/10.1007/BF02743434
Product Type:
Journal Article
Reference Number:
AIX-13-682146; EDB-82-116497
Resource Relation:
Journal Name: Nuovo Cimento B; (Italy); Journal Volume: 51:2
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; BLACK HOLES; GRAVITATIONAL COLLAPSE; MASS; KERR METRIC; SINGULARITY; ACCRETION DISKS; LUMINOSITY; TIME DEPENDENCE; METRICS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; 640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources; 640106 - Astrophysics & Cosmology- Cosmology
OSTI ID:
5402308
Country of Origin:
Italy
Language:
English
Other Identifying Numbers:
Journal ID: CODEN: NCIBA
Submitting Site:
HEDB
Size:
Pages: 247-261
Announcement Date:
Jun 01, 1982

Journal Article:

SAVE / SHARE

XML RIS EndNote CSV/Excel JSON

Citation Formats

Calvani, M, and Nobili, L. Dressing up a Kerr naked singularity. Italy: N. p., 1979. Web. doi:10.1007/BF02743434.
Calvani, M, & Nobili, L. Dressing up a Kerr naked singularity. Italy. https://doi.org/10.1007/BF02743434
Calvani, M, and Nobili, L. 1979. "Dressing up a Kerr naked singularity." Italy. https://doi.org/10.1007/BF02743434.
@misc{etde_5402308,
title = {Dressing up a Kerr naked singularity}
 author = {Calvani, M, and Nobili, L}
 abstractNote = {The evolution of a naked singularity surrounded by an accreting disk of matter is studied; two kinds of disks are considered: the standard thin-disk model and the thick barytropic model, for several initial conditions. It is shown that any Kerr naked singularity slows down in a finite time to a maximal Kerr black hole. The final mass, the luminosity and the time of evolution of the singularity are evaluated.}
 doi = {10.1007/BF02743434}
 journal = []
 volume = {51:2}
 journal type = {AC}
 place = {Italy}
 year = {1979}
 month = {Jun}
 }