Abstract
We analyse a new family of solutions to the Einstein field equations describing the collapse of a fluid sphere in the presence of heat flux and shear. These solutions ensure that the collapsing fluid is accelerating and provide a generalisation of the geodesic fluid models studied in earlier treatments. In particular, we demonstrate the role played by pressure in the dynamics of the collapse process.
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Govender, M., Govinder, K.S. & Fleming, D. The Role of Pressure During Shearing, Dissipative Collapse. Int J Theor Phys 51, 3399–3409 (2012). https://doi.org/10.1007/s10773-012-1221-8
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DOI: https://doi.org/10.1007/s10773-012-1221-8