Nuclear pasta structure in hot neutron stars

Details Nuclear pasta structure in hot neutron stars Nuclear pasta structure in hot neutron stars

2003-10-10

arxiv.org/abs/astro-ph/0310290v1

Astronomy and Astrophysics

Astrophysics

2 pages, 1figure, To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), e

Scientific paper

Structure of cold and hot dense matter at subnuclear densities is
investigated by quantum molecular dynamics (QMD) simulations. Obtained phase
diagrams show that the density of the phase boundaries between the different
nuclear structures decreases with increasing temperature due to the thermal
expansion of nuclear matter region.

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