On the onset of relativistic instability in highly centrally condensed stars

Details On the onset of relativistic instability in highly centrally condensed stars On the onset of relativistic instability in highly centrally condensed stars

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207p..13c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 207, March 15, 1984, p. 13P-16P.

Astronomy and Astrophysics

Astronomy

Dynamic Stability, Late Stars, Relativity, Stellar Models, Adiabatic Conditions, Nuclear Fusion, Polytropic Processes

Scientific paper

It is shown that, along the polytropic sequence, the criterion for relativistic instability due to radial perturbation can be written to less than 3 percent accuracy in where the adiabatic constant is close to 4/3. This criterion is expected to indicate when the relativistic instability will become relevant for highly centralized condensed stars like those in the late stages of stellar evolution when elements of higher atomic number are being synthesized.

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