Static axially symmetric sources of the gravitational field

Daniele Malafarina, Giulio Magli, Luis Herrera

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The gamma metric, a static axially symmetric vacuum solution of Einstein field equations, is reviewed, the nature of its singularity and the shape of its sources are studied. This space-time is matched with an interior metric satisfying physically viable conditions. The model obtained, which can represent a dense astrophysical object, is used to investigate the boundary between black hole (i.e. Schwarzschild) and naked singularity as a function of the shape of the source.

Original languageEnglish
Title of host publicationAIP Conference Proceedings
Pages185-187
Number of pages3
Volume751
DOIs
Publication statusPublished - 2005
Externally publishedYes
Event16th SIGRAV Conference on General Relativity and Gravitational Physics, SIGRAV04 - Vietri sul Mare, Italy
Duration: Sep 13 2004Sep 16 2004

Other

Other16th SIGRAV Conference on General Relativity and Gravitational Physics, SIGRAV04
CountryItaly
CityVietri sul Mare
Period9/13/049/16/04

Fingerprint

gravitational fields
naked singularities
astrophysics
vacuum

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Malafarina, D., Magli, G., & Herrera, L. (2005). Static axially symmetric sources of the gravitational field. In AIP Conference Proceedings (Vol. 751, pp. 185-187) https://doi.org/10.1063/1.1891547

Static axially symmetric sources of the gravitational field. / Malafarina, Daniele; Magli, Giulio; Herrera, Luis.

AIP Conference Proceedings. Vol. 751 2005. p. 185-187.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Malafarina, D, Magli, G & Herrera, L 2005, Static axially symmetric sources of the gravitational field. in AIP Conference Proceedings. vol. 751, pp. 185-187, 16th SIGRAV Conference on General Relativity and Gravitational Physics, SIGRAV04, Vietri sul Mare, Italy, 9/13/04. https://doi.org/10.1063/1.1891547
Malafarina D, Magli G, Herrera L. Static axially symmetric sources of the gravitational field. In AIP Conference Proceedings. Vol. 751. 2005. p. 185-187 https://doi.org/10.1063/1.1891547
Malafarina, Daniele ; Magli, Giulio ; Herrera, Luis. / Static axially symmetric sources of the gravitational field. AIP Conference Proceedings. Vol. 751 2005. pp. 185-187
@inproceedings{e40b60f440524a06b76043215d8ab602,
title = "Static axially symmetric sources of the gravitational field",
abstract = "The gamma metric, a static axially symmetric vacuum solution of Einstein field equations, is reviewed, the nature of its singularity and the shape of its sources are studied. This space-time is matched with an interior metric satisfying physically viable conditions. The model obtained, which can represent a dense astrophysical object, is used to investigate the boundary between black hole (i.e. Schwarzschild) and naked singularity as a function of the shape of the source.",
author = "Daniele Malafarina and Giulio Magli and Luis Herrera",
year = "2005",
doi = "10.1063/1.1891547",
language = "English",
isbn = "0735402361",
volume = "751",
pages = "185--187",
booktitle = "AIP Conference Proceedings",

}

TY - GEN

T1 - Static axially symmetric sources of the gravitational field

AU - Malafarina, Daniele

AU - Magli, Giulio

AU - Herrera, Luis

PY - 2005

Y1 - 2005

N2 - The gamma metric, a static axially symmetric vacuum solution of Einstein field equations, is reviewed, the nature of its singularity and the shape of its sources are studied. This space-time is matched with an interior metric satisfying physically viable conditions. The model obtained, which can represent a dense astrophysical object, is used to investigate the boundary between black hole (i.e. Schwarzschild) and naked singularity as a function of the shape of the source.

AB - The gamma metric, a static axially symmetric vacuum solution of Einstein field equations, is reviewed, the nature of its singularity and the shape of its sources are studied. This space-time is matched with an interior metric satisfying physically viable conditions. The model obtained, which can represent a dense astrophysical object, is used to investigate the boundary between black hole (i.e. Schwarzschild) and naked singularity as a function of the shape of the source.

UR - http://www.scopus.com/inward/record.url?scp=78751618040&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=78751618040&partnerID=8YFLogxK

U2 - 10.1063/1.1891547

DO - 10.1063/1.1891547

M3 - Conference contribution

SN - 0735402361

SN - 9780735402362

VL - 751

SP - 185

EP - 187

BT - AIP Conference Proceedings

ER -