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Methods of Local and Global Differential Geometry in General Relativity pp 126–136Cite as

The luminosity of a collapsing star

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Part of the book series: Lecture Notes in Physics ((LNP,volume 14))

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References

  1. M. A. Podurets, Astr. Zh. 41, 1090 (1964), (English trans. Soviet Ast.-AJ. 8, 868 (1965).

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  2. W. L. Ames and K. S. Thorne, Ap. J. 151, 659 (1968).

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  3. J. Kristian and R. K. Sachs, Ap. J. 143, 379 (1966).

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  4. R. K. Sachs, Proc. Roy. Soc. London, A, 264, 309 (1961).

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  5. R. Kantowski, Ap. J. 155, 89 (1969).

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  6. We are using Schwarzschild coordinates and units c =G=1 throughout.

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  7. R. Kantowski, J. Math. Phys. 9, 336 (1968).

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  8. The angle a is defined in Figure 1 (see equation (20)).

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Authors and Affiliations

  1. Department of Physics, University of Oklahoma, Oklahoma

    Pt. I. H. Dwivedi & R. Kantowski

Authors
  1. Pt. I. H. Dwivedi
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  2. R. Kantowski
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Editor information

D. Farnsworth J. Fink J. Porter A. Thompson

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© 1972 Springer-Verlag

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Dwivedi, P.I.H., Kantowski, R. (1972). The luminosity of a collapsing star. In: Farnsworth, D., Fink, J., Porter, J., Thompson, A. (eds) Methods of Local and Global Differential Geometry in General Relativity. Lecture Notes in Physics, vol 14. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-05793-5_8

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  • DOI: https://doi.org/10.1007/3-540-05793-5_8

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-05793-2

  • Online ISBN: 978-3-540-37434-3

  • eBook Packages: Springer Book Archive

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