activity
20062026
most citedCondensed Surfaces of Magnetic Neutron Stars, Thermal Surface Emission, and Particle Acceleration Above Pulsar Polar Caps

105 citations · 616 across the 15 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2016★ 16 cited

A Survey of Chemical Separation in Accreting Neutron Stars

Ryan Mckinven, Andrew Cumming, Zach Medin +1

The heavy element ashes of rp-process hydrogen and helium burning in accreting neutron stars are compressed to high density where they freeze, forming the outer crust of the star.…

astro-ph.SR2014★ 20 cited

Time-dependent, compositionally driven convection in the oceans of accreting neutron stars

Zach Medin, Andrew Cumming

We discuss the effect of chemical separation as matter freezes at the base of the ocean of an accreting neutron star, and the subsequent enrichment of the ocean in light elements a…

astro-ph.SR2013★ 32 cited

A signature of chemical separation in the cooling curves of transiently accreting neutron stars

Zach Medin, Andrew Cumming

We show that convection driven by chemical separation can significantly affect the cooling curves of accreting neutron stars after they go into quiescence. We calculate the thermal…

astro-ph.SR2012★ 27 cited

Direct MD simulation of liquid-solid phase equilibria for three-component plasma

J. Hughto, C. J. Horowitz, A. S. Schneider +3

The neutron rich isotope 22Ne may be a significant impurity in carbon and oxygen white dwarfs and could impact how the stars freeze. We perform molecular dynamics simulations to de…

astro-ph.SR2010★ 35 cited

Compositionally-driven convection in the oceans of accreting neutron stars

Zach Medin, Andrew Cumming

We discuss the effect of chemical separation as matter freezes at the base of the ocean of an accreting neutron star, and argue that the retention of light elements in the liquid a…

astro-ph.SR2010★ 78 cited

Crystallization of classical multi-component plasmas

Zach Medin, Andrew Cumming

We develop a method for calculating the equilibrium properties of the liquid-solid phase transition in a classical, ideal, multi-component plasma. Our method is a semi-analytic cal…