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arXiv · 1209.5962

Impact of r-modes on the cooling of neutron stars

Mark G. Alford·Simin Mahmoodifar·Kai Schwenzer
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Abstract

Studying the frequency and temperature evolution of a compact star can give us valuable information about the microscopic properties of the matter inside the star. In this paper we study the effect of dissipative reheating of a neutron star due to r-mode oscillations on its temperature evolution. We find that there is still an impact of an r-mode phase on the temperature long after the star has left the instability region and the r-mode is damped completely. With accurate temperature measurements it may be possible to detect this trace of a previous r-mode phase in observed pulsars.

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Mark G. Alford, Simin Mahmoodifar, Kai Schwenzer. 2012-09-26. Impact of r-modes on the cooling of neutron stars. https://doi.org/10.1063/1.4763528

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