Add to ORKGSome analytical spherical-symmetric equilibrium solutions are cosidered in the Newtonian theory of gravitation with deviations from 1/r law. Stability of star against a first-order phase-transition is shown to be particularly influenced by the deviations of degree in the power-law potential
The Newtonian theory of gravitation is modified to include the gravitational energy as a source of g...
Shortly after the addition of a 1/R term to the Einstein-Hilbert action was proposed as a solution t...
Shortly after the addition of a 1/R term to the Einstein-Hilbert action was proposed as a solution t...
Although general relativistic cosmological solutions, even in the presence of pressure, can be mimic...
16 pages, 3 figuresWe gratefully acknowledge support for this work under NSF Grant Nos. PHY-0554367 ...
A Newtonian-like theory inspired by the Brans–Dicke gravitational Lagrangian has been recently propo...
In this paper, the gravitational field equations for static sphericallysymmetric perfect fluid model...
We construct equilibrium sequences of axisymmetric Newtonian clusters that tend toward singular stat...
First post-Newtonian (1PN) hydrostatic equations for an irrotational fluid which have been recently ...
The PPN formalism which encompasses the post-Newtonian limit of nearly every metric theory of gravit...
A complete theory of the non-radial oscillations of a static spherically symmetric distribution of m...
Thesis (Ph.D.)-University of KwaZulu-Natal, Westville, 2012.In this thesis we study classes of stati...
We present numerical results on the hydrodynamic stability of coalescing binary stars in the first p...
Stellar structures are investigated by considering the modified Lan´e- Emden equation coming out fro...
We investigate spherically symmetric equilibrium states of the Vlasov-Poisson system, relevant in ga...
The Newtonian theory of gravitation is modified to include the gravitational energy as a source of g...
Shortly after the addition of a 1/R term to the Einstein-Hilbert action was proposed as a solution t...
Shortly after the addition of a 1/R term to the Einstein-Hilbert action was proposed as a solution t...
Although general relativistic cosmological solutions, even in the presence of pressure, can be mimic...
16 pages, 3 figuresWe gratefully acknowledge support for this work under NSF Grant Nos. PHY-0554367 ...
A Newtonian-like theory inspired by the Brans–Dicke gravitational Lagrangian has been recently propo...
In this paper, the gravitational field equations for static sphericallysymmetric perfect fluid model...
We construct equilibrium sequences of axisymmetric Newtonian clusters that tend toward singular stat...
First post-Newtonian (1PN) hydrostatic equations for an irrotational fluid which have been recently ...
The PPN formalism which encompasses the post-Newtonian limit of nearly every metric theory of gravit...
A complete theory of the non-radial oscillations of a static spherically symmetric distribution of m...
Thesis (Ph.D.)-University of KwaZulu-Natal, Westville, 2012.In this thesis we study classes of stati...
We present numerical results on the hydrodynamic stability of coalescing binary stars in the first p...
Stellar structures are investigated by considering the modified Lan´e- Emden equation coming out fro...
We investigate spherically symmetric equilibrium states of the Vlasov-Poisson system, relevant in ga...
The Newtonian theory of gravitation is modified to include the gravitational energy as a source of g...
Shortly after the addition of a 1/R term to the Einstein-Hilbert action was proposed as a solution t...
Shortly after the addition of a 1/R term to the Einstein-Hilbert action was proposed as a solution t...