Stable gravastars: an alternative to black holes?
- Author
- VISSER, Matt1 ; WILTSHIRE, David L2
[1] School of Mathematical and Computing Sciences, Victoria University of Wellington, New Zealand
[2] Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand - Source
Classical and quantum gravity (Print). 2004, Vol 21, Num 4, pp 1135-1151, 17 p ; ref : 22 ref
- CODEN
- CQGRDG
- ISSN
- 0264-9381
- Scientific domain
- Theoretical physics
- Publisher
- Institute of Physics, Bristol
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Keyword (fr)
- Couche transition Equation état Etoile particulière Gravité Modèle Métrique de Sitter Stabilité dynamique Stabilité thermodynamique Symétrie sphérique Transition phase Trou noir Horizon événement
- Keyword (en)
- Transition layer Equations of state Peculiar stars Gravity Models De Sitter metric Dynamic stability Thermodynamic stability Spherical symmetry Phase transitions Black holes Event horizon
- Keyword (es)
- Capa transición Modelo Estabilidad termodinámica Simetría esférica Transición fase Horizonte acontecimiento
- Classification
- Pascal
- 001 Exact sciences and technology / 001B Physics / 001B00 General / 001B00D General relativity and gravitation / 001B00D40 Self-graviting systems; continuous media and classical fields in curved spacetime / 001B00D40D Relativistic stars: structure, stability and oscillations
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C60 Late stages of stellar evolution (including black holes) / 001E03C60L Black holes
- Discipline
- Astronomy Theoretical physics
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 15459784
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1088/0264-9381/21/4/027 
https://dx.doi.org/10.1088/0264-9381/21/4/027
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