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Higher dimensional spherically symmetric inhomogeneous cosmological model with heat flow

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Abstract

We study spherically symmetric inhomogeneous cosmological model with heat flow in higher dimensional space-time and present a class of solutions in which the velocity field is shear-free. Some of these solutions are analogous to the known solutions in 4-dimension while some are totally new.

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References

  1. O Bergmann,Phys. Lett. A82, 383 (1981)

    ADS  MathSciNet  Google Scholar 

  2. S R Maiti,Phys. Rev. D25, 2518 (1982)

    ADS  MathSciNet  Google Scholar 

  3. B Modak,J. Astrophys. Astron. 5, 317 (1984)

    Article  ADS  Google Scholar 

  4. A Banerjee, S B Dutta Chaudhury and B K Bhui,Pramana — J. Phys. 34, 397 (1990)

    Article  ADS  Google Scholar 

  5. Y Deng,Gen. Relativ. Gravit. 21, 503 (1989)

    Article  ADS  Google Scholar 

  6. A Banerjee, S B Dutta Chaudhury and S Chatterjee,Gen. Relativ. Gravit. 24, 991 (1992)

    Article  ADS  Google Scholar 

  7. E N Glass,J. Math. Phys. 20, 1508 (1979);Phys. Lett. A86, 351 (1981)

    Article  ADS  MathSciNet  Google Scholar 

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Chakraborty, S., Shah, M.F. Higher dimensional spherically symmetric inhomogeneous cosmological model with heat flow. Pramana - J. Phys. 44, 495–500 (1995). https://doi.org/10.1007/BF02878860

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  • DOI: https://doi.org/10.1007/BF02878860

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