Abstract
We model a radiating star undergoing dissipative gravitational collapse in the form of radial heat flux. The exterior of the collapsing star is described by the generalised Vaidya solution representing a mixture of null radiation and strings. Our model generalises previously known results of constant string density atmosphere to include inhomogeneities in the exterior spacetime. By utilising a causal heat transport equation of the Maxwell–Cattaneo form we show that relaxational effects are enhanced in the presence of inhomogeneities due to the string density.
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Acknowledgements
The authors are grateful to the National Research Foundation (NRF) and both the Durban Institute of Technology and University of KwaZulu-Natal. SDM acknowledges that this research is supported by the South African Research Chair Initiative of the Department of Science and Technology and the NRF.
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Naidu, N.F., Govender, M., Thirukkanesh, S. et al. Radiating fluid sphere immersed in an anisotropic atmosphere. Gen Relativ Gravit 49, 95 (2017). https://doi.org/10.1007/s10714-017-2258-z
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DOI: https://doi.org/10.1007/s10714-017-2258-z