Revival of Radiation Reaction Instability

Details Revival of Radiation Reaction Instability Revival of Radiation Reaction Instability

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000asthe..93..350k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 93, No. 7, p. 350 - 353 (2000)

Astronomy and Astrophysics

Astrophysics

Scientific paper

One of recent topics, r-mode instability is reviewed with great plainness. Unstable growing modes are induced by the reaction force of gravitational radiation in rotating stars. The mechanism may have important astrophysical implications in newly borne neutron stars, millisecond pulsars and accreting white dwarfs and so on. Present estimates are however based on (over-) simplified models, and further studies are indispensable. The article closes with the author's personal prospects.

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