Gravitational Field of A Radiating Star in Higher Dimensions
B. C. Paul, P. K. Chattopadhyay

TL;DR
This paper derives a new solution for the gravitational field of a radiating star in higher-dimensional spacetime, revealing that the star's radius oscillates with a period influenced by vibrational modes and the number of dimensions.
Contribution
It introduces a novel higher-dimensional solution for a radiating star that generalizes Vaidya's 4D model and shows oscillatory behavior of the star's radius.
Findings
Star radius oscillates in higher dimensions
Oscillation period depends on vibrational modes and dimensions
Solution reduces to Vaidya's 4D case
Abstract
We obtain fields of a relativistic radiating star of non-static mass in the framework of higher dimensional spacetime. Assuming energy-momentum tensor in Higher dimensions analogous to that considered by Vaidya in 4 dimensions we obtain solution of a radiating spherically symmetric star. The solution obtained here is new in higher dimensions which however reduces to that obtained by Vaidya in 4 dimensions. It is also different in form from that obtained by Iyer and Vishveshwara. The interesting observation is that the radius of a radiating star in higher dimensions oscillates. The radial size of radiating star oscillates with a period which depends on the modes of vibration and dimensions of the space-time.
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Taxonomy
TopicsCosmology and Gravitation Theories · Advanced Differential Geometry Research · Relativity and Gravitational Theory
