Abstract
A new, globally regular model describing a static, non spherical gravitating object in General Relativity is presented. The model is composed by a vacuum Weyl-Levi-Civita special field - the so called gamma metric - generated by a regular static distribution of mass-energy. Standard requirements of physical reasonableness such as, energy, matching and regularity conditions are satisfied. The model is used as a toy in investigating various issues related to the directional behavior of naked singularities in static spacetimes and the black hole (Schwarzschild) limit.
| Original language | English |
|---|---|
| Pages (from-to) | 1371-1383 |
| Number of pages | 13 |
| Journal | General Relativity and Gravitation |
| Volume | 37 |
| Issue number | 8 |
| DOIs | |
| Publication status | Published - Aug 2005 |
| Externally published | Yes |
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Keywords
- No-hair theorem
- Static gravitational field
ASJC Scopus subject areas
- Physics and Astronomy(all)
Cite this
Non-spherical sources of static gravitational fields : Investigating the boundaries of the no-hair theorem. / Herrera, L.; Magli, G.; Malafarina, D.
In: General Relativity and Gravitation, Vol. 37, No. 8, 08.2005, p. 1371-1383.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Non-spherical sources of static gravitational fields
T2 - Investigating the boundaries of the no-hair theorem
AU - Herrera, L.
AU - Magli, G.
AU - Malafarina, D.
PY - 2005/8
Y1 - 2005/8
N2 - A new, globally regular model describing a static, non spherical gravitating object in General Relativity is presented. The model is composed by a vacuum Weyl-Levi-Civita special field - the so called gamma metric - generated by a regular static distribution of mass-energy. Standard requirements of physical reasonableness such as, energy, matching and regularity conditions are satisfied. The model is used as a toy in investigating various issues related to the directional behavior of naked singularities in static spacetimes and the black hole (Schwarzschild) limit.
AB - A new, globally regular model describing a static, non spherical gravitating object in General Relativity is presented. The model is composed by a vacuum Weyl-Levi-Civita special field - the so called gamma metric - generated by a regular static distribution of mass-energy. Standard requirements of physical reasonableness such as, energy, matching and regularity conditions are satisfied. The model is used as a toy in investigating various issues related to the directional behavior of naked singularities in static spacetimes and the black hole (Schwarzschild) limit.
KW - No-hair theorem
KW - Static gravitational field
UR - http://www.scopus.com/inward/record.url?scp=24944469913&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=24944469913&partnerID=8YFLogxK
U2 - 10.1007/s10714-005-0120-1
DO - 10.1007/s10714-005-0120-1
M3 - Article
AN - SCOPUS:24944469913
VL - 37
SP - 1371
EP - 1383
JO - General Relativity and Gravitation
JF - General Relativity and Gravitation
SN - 0001-7701
IS - 8
ER -