Thermal fluctuations in nuclear pasta
Author:
Funder
National Science Foundation
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.103.055810/fulltext
Reference36 articles.
1. Time-dependent Hartree-Fock approach to nuclear “pasta” at finite temperature
2. Colloquium: Astromaterial science and nuclear pasta
3. Akmal-Pandharipande-Ravenhall equation of state for simulations of supernovae, neutron stars, and binary mergers
4. A highly resistive layer within the crust of X-ray pulsars limits their spin periods
5. Disordered Nuclear Pasta, Magnetic Field Decay, and Crust Cooling in Neutron Stars
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1. Correlating isothermal compressibility to nucleon fluctuations in the inner crust of neutron stars;Physical Review C;2024-02-23
2. Do short range correlations inhibit the appearance of the nuclear pasta?;The European Physical Journal A;2023-09-13
3. The proto-neutron star inner crust in a multi-component plasma approach;Astronomy & Astrophysics;2023-09
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5. Anisotropic electron transport in the nuclear pasta phase;Monthly Notices of the Royal Astronomical Society;2023-02-21
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