most citedStable gravastars with generalised exteriors

162 citations · 377 across the 7 of their papers we have counts for

collaborators

7 papers

hep-th2006★ 30 cited

Hybrid brane worlds in the Salam-Sezgin model

Benedict M. N. Carter, Alex B. Nielsen, David L. Wiltshire

We construct a 6-dimensional warped brane world compactification of the Salam-Sezgin supergravity model by generalizing an earlier hybrid Kaluza-Klein / Randall-Sundrum constructio…

gr-qc2005★ 2 cited

Series solutions for a static scalar potential in a Salam-Sezgin Supergravitational hybrid braneworld

Benedict M. N. Carter, Alex B. Nielsen

The static potential for a massless scalar field shares the essential features of the scalar gravitational mode in a tensorial perturbation analysis about the background solution.…

hep-th2005★ 61 cited

Towards inflation and dark energy cosmologies from modified Gauss-Bonnet theory

Ishwaree P Neupane, Benedict M N Carter

We consider a physically viable cosmological model that has a field dependent Gauss-Bonnet coupling in its effective action, in addition to a standard scalar field potential. The p…

hep-th2005★ 60 cited

Dynamical Relaxation of Dark Energy: A Solution to Early Inflation, Late-time Acceleration and the Cosmological Constant Problem

Ishwaree P. Neupane, Benedict M. N. Carter

In recent years different explanations are provided for both an inflation and a recent acceleration in the expansion of the universe. In this Letter we show that a model of physica…

gr-qc2005★ 162 cited

Stable gravastars with generalised exteriors

Benedict M. N. Carter

New spherically symmetric gravastar solutions, stable to radial perturbations, are found by utilising the construction of Visser and Wiltshire. The solutions possess an anti--de Si…

gr-qc2005★ 56 cited

Thermodynamics and Stability of Higher Dimensional Rotating (Kerr) AdS Black Holes

Benedict M. N. Carter, Ishwaree P Neupane

We study the thermodynamic and gravitational stability of Kerr anti-de Sitter black holes in five and higher dimensions. We show, in the case of equal rotation parameters, ,…