Normal modes of a rotating, charged and uniformly accelerated frame

Details Normal modes of a rotating, charged and uniformly accelerated frame Normal modes of a rotating, charged and uniformly accelerated frame

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ictp.rept.....a&link_type=abstract

Technical Report, International Centre for Theoretical Physics Trieste, Italy

Statistics

Computation

Black Holes (Astronomy), Gravitational Waves, Stellar Gravitation, Stellar Oscillations, Space-Time Functions, Computational Astrophysics, Frequency Response, Anisotropy, Perturbation Theory, Electromagnetic Fields

Scientific paper

The method for calculation of normal modes of black holes has been extended to a rotating charged and uniformly accelerated frame. The method not only extends the earlier methods in the case of black holes but also allows to calculate the normal modes of the black holes which are interesting from the point of view of inflationary scenario of the early universe. This method can also be applied for calculation of normal modes of many interesting spacetimes such as Kasner and NUT spacetimes which are considered as anisotropic model in the early universe.

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