Hydrostatic Expansion and Spin Changes During Type I X-Ray Bursts

Abstract

We present calculations of the spin-down of a neutron star atmosphere due to hydrostatic expansion during a Type I X-ray burst. We show that (i) Cumming and Bildsten overestimated the spin-down of rigidly-rotating atmospheres by a factor of two, and (ii) general relativity has a small (5-10%) effect on the angular momentum conservation law. We rescale our results to different neutron star masses, rotation rates and equations of state, and present some detailed rotational profiles. Comparing with recent observations of large frequency shifts in MXB 1658-298 and 4U 1916-053, we find that the spin-down expected if the atmosphere rotates rigidly is a factor of two to three less than the observed values. If differential rotation is allowed to persist, we find that the upper layers of the atmosphere spin down by an amount comparable to the observed values; however, there is no compelling reason to expect the observed spin frequency to be that of only the outermost layers. We conclude that hydrostatic expansion and angular momentum conservation alone cannot account for the largest frequency shifts observed during Type I bursts.

Submitted to the Astrophysical Journal (13 pages, including 4 figures)

References in corpus (4)

• The endpoint of the rp process on accreting neutron stars
• Millisecond Oscillations and Photospheric Radius Expansion in Thermonuclear X-Ray Bursts
• The first outburst of SAX J1808.4-3658 revisited
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