Fetching the paper…
Reading the bibliography…
Gravastars have been recently proposed as potential alternatives to explain the astrophysical phenomenology traditionally associated to black holes, raising the question of whether the two objects can be distinguished at all.
Chandrasekhar S and Ferrari V 1991 On the non-radial oscillations of a star Proc. R. Soc. Lond
1991
Earlier work this paper cites.
Chandrasekhar S and Ferrari V 1991 On the non-radial oscillations of a star III. A reconsideration of the axial modes Proc. R. Soc. Lond
1991
Earlier work this paper cites.
Israel W 1966 Singular hypersurfaces and thin shells in general relativity Nuovo Cimento
1997
Earlier work this paper cites.
Kokkotas K D and Schmidt B G 1999 Quasi-normal modes of stars and black holes Living Rev. in Relativity
1999
Earlier work this paper cites.
Nollert H 1999 Quasinormal Modes: The characteristic ‘sound’ of black holes and neutron stars Class. Quantum Grav
1999
Earlier work this paper cites.
Mazur P O and Mottola E 2001 Gravitational condensate stars: an alternative to black holes
2001
Earlier work this paper cites.
Abramowicz M A, Kluzniak W and Lasota J P 2002 No observational proof of the black-hole event-horizon Astron. Astrophys
2002
Earlier work this paper cites.
Dev K and Gleiser M 2002 Anisotropic stars: Exact solutions Gen. Rel. Grav
2002
Earlier work this paper cites.
Dev K and Gleiser M 2003 Anisotropic stars. 2. Stability Gen. Rel. Grav
2003
Cited alongside, same era.
Chapline G 2004 Dark energy stars Proceedings of the 22nd Texas Conference on Relativistic Astrophysics (California)
2004
Cited alongside, same era.
Visser M and Wiltshire D L 2004 Stable gravastars - an alternative to black holes? Class. Quant. Grav
2004
Cited alongside, same era.
Carter B M N 2005 Stable gravastars with generalised exteriors Class. Quant. Grav
2005
Cited alongside, same era.
Cattoen C, Faber T and Visser M 2005 Gravastars must have anisotropic pressures Class. Quant. Grav
2005
Cited alongside, same era.
Dymnikova I 1992 Vacuum nonsingular black hole Gen. Rel. Grav
2005
Lobo F S N 2006 Stable dark energy stars Class. Quant. Grav
2006
Later among the works it cites.
DeBenedictis A, Horvat D, Ilijic S, Kloster S and Viswanathan K S 2006 Gravastar solutions with continuous pressures and equation of state Class. Quant. Grav
2006
Later among the works it cites.
Nagar A and Rezzolla L 2005 Gauge-invariant non-spherical perturbations of Schwarzschild black-hole spacetimes, Class. Quantum Grav
2006
Later among the works it cites.
Abdalla E, Chirenti C B M H and Saa A 2006 Quasinormal modes for the Vaidya metric Phys. Rev
2006
Later among the works it cites.
Abdalla E and Giugno D 2006 An extensive search for overtones in Schwarzschild black holes Preprint
2006
Later among the works it cites.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
Cited alongside, same era.
Mbonye M R and Kazanas D 2005 A non-singular black hole model as a possible end-product of gravitational collapse Phys. Rev
2005
Cited alongside, same era.
Bilić N, Tupper G B and Viollier R D 2006 Born-Infeld phantom gravastars JCAP
2006
Cited alongside, same era.
2006
Later among the works it cites.
Lobo F S N and Arellano A V B 2007 Gravastars supported by nonlinear electrodynamics Class. Quant. Grav
2007
Closest in time.