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Radial oscillations of a radiation-supported levitating shell in Eddington luminosity neutron stars

In general relativity, it has been shown that radiation-supported atmospheres exist outside the surface of a radiating spherical body close to a radius where the gravitational and radiative forces balance each other. We calculate the frequency of oscillation of the incompressible radial mode of such a thin atmospheric shell and show that in the optically thin case, this particular mode is overdamped by radiation drag.

preprint2016arXivOpen access
David AbarcaWłodek Kluźniak
astro-ph.HE
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Open access2 authors1 topic
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David AbarcaWłodek Kluźniak

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