Nuclear pasta structure in hot neutron stars

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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.
2 pages, 1figure, To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler

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Astrophysics, Nuclear Theory

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http://salesiana.dossiersoluciones.com/handle/123456789/6698

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0310290
 http://arxiv.org/abs/astro-ph/0310290

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arXiv