Mechanism of thermonuclear burning propagation in a helium layer on a neutron star surface: A simplified adiabatic model

• Published in: Astronomy letters Vol. 38; no. 4; pp. 231 - 237
• Main Authors: Simonenko, V. A., Gryaznykh, D. A., Litvinenko, I. A., Lykov, V. A., Shushlebin, A. N.
• Format: Journal Article
• Language: English
• Published: Dordrecht SP MAIK Nauka/Interperiodica 01-04-2012; Pleiades; Springer Nature B.V
• Subjects: Astronomy; Astrophysics; Astrophysics and Astroparticles; Atmosphere; Helium; Numerical analysis; Observations and Techniques; Physics; Physics and Astronomy; Stars & galaxies; numerical simulations; thermonuclear burning; X-ray bursts
• ISSN: 1063-7737; 1562-6873
• DOI: 10.1134/S1063773712040056

Some thermonuclear X-ray bursters exhibit a high-frequency (about 300 Hz or more) brightness modulation at the rising phase of some bursts. These oscillations are explained by inhomogeneous heating of the surface layer on a rapidly rotating neutron star due to the finite propagation speed of thermonuclear burning. We suggest and substantiate a mechanism of this propagation that is consistent with experimental data. Initially, thermonuclear ignition occurs in a small region of the neutron star surface layer. The burning products rapidly rise and spread in the upper atmospheric layers due to turbulent convection. The accumulation of additional matter leads to matter compression and ignition at the bottom of the layer. This determines the propagation of the burning front. To substantiate this mechanism, we use the simplifying assumptions about a helium composition of the neutron star atmosphere and its initial adiabatic structure with a density of 1.75 × 10
8
g cm
−3
at the bottom. 2D numerical simulations have been performed using a modified particle method in the adiabatic approximation.