Abstract
We have studied the behaviour of a radiating star when the interior expanding, shearing fluid particles are traveling in geodesic motion. A systematic approach enables us to write the junction condition as a Riccati equation. In this article we obtained two new solutions in terms of elementary functions with assuming a separation of variables and also have discussed the physical significance of these solutions.
We have studied the behaviour of a radiating star when the interior expanding, shearing fluid particles are traveling in geodesic motion. A systematic approach enables us to write the junction condition as a Riccati equation. In this article we obtained two new solutions in terms of elementary functions with assuming a separation of variables and also have discussed the physical significance of these solutions.
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Dr. M. A. Helal. 2012. “. Global Journal of Science Frontier Research – F: Mathematics & Decision GJSFR-F Volume 12 (GJSFR Volume 12 Issue F9): .
Crossref Journal DOI 10.17406/GJSFR
Print ISSN 0975-5896
e-ISSN 2249-4626
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