Accretion and burning on neutron stars
Yuri
Cavecchi has done more than anyone IMO to understand the broad properties of thermonuclear
bursts. In his latest paper (arXiv:2506.11966)
he describes further refinement of his
phenomenological model that
explains the relative inefficiency of unstable thermonuclear burning at high accretion
rates.
The model has several requirements, including a varying distribution of accretion over the neutron star; stable burning (at the equator) coexisting with unstable (at higher latitudes); and significant "pollution" of the burst fuel by ashes dredged up into the fuel layer, possibly by convection. This pollution contribution is now on a firmer basis with support from MESA simulations, and as a whole the model matches the burst observations and potentially allows us to deduce changes in the accretion disk geometry close to the star. The paper is under review by ApJL.