Heat release in accreting neutron stars
Author:
Funder
Foundation for the Advancement of Theoretical Physics and Mathematics
Russian Foundation for Basic Research
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.103.L101301/fulltext
Reference38 articles.
1. Constraints on Thermal X‐Ray Radiation from SAX J1808.4−3658 and Implications for Neutron Star Neutrino Emission
2. Neutron Reactions in Accreting Neutron Stars: A New Pathway to Efficient Crust Heating
3. Strong neutrino cooling by cycles of electron capture and β− decay in neutron star crusts
4. Mass Measurement ofSc56Reveals a SmallA=56Odd-Even Mass Staggering, Implying a Cooler Accreted Neutron Star Crust
5. Cooling of Accretion-Heated Neutron Stars
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1. Thermodynamically consistent accreted crust of neutron stars: The role of proton shell effects;Physical Review D;2024-06-24
2. Gapless neutron superfluidity in the crust of the accreting neutron stars KS 1731−260 and MXB 1659−29;The European Physical Journal A;2024-05-29
3. Gapless Neutron Superfluidity Can Explain the Late Time Cooling of Transiently Accreting Neutron Stars;Physical Review Letters;2024-04-29
4. Virialized equation of state for warm and dense stellar plasmas in proto-neutron stars and supernova matter;Monthly Notices of the Royal Astronomical Society;2024-01-22
5. Impact of Pycnonuclear Fusion Uncertainties on the Cooling of Accreting Neutron Star Crusts;The Astrophysical Journal;2023-09-01
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