Quasi-normal oscillations of a schwarzschild black hole

Details Quasi-normal oscillations of a schwarzschild black hole Quasi-normal oscillations of a schwarzschild black hole

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phla..100..231b&link_type=abstract

Physics Letters A, Volume 100, Issue 5, p. 231-234.

Physics

34

Scientific paper

The modes of oscillation of a Schwarzschild black hole are determined within an analytic framework. These quasi-normal modes are related to the bound states of the inverted black hole potential which is approximated by the inverted Eckart potential. For a given angular momentum parameter j, the real part of the quasi-normal frequency decreases as the mode number n (or, equivalently, the damping factor) increases, in agreement with the results of numerical studies.

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