Equation of state of superfluid neutron matter with low-momentum interactions
Author:
Funder
Indo-French Centre for the Promotion of Advanced Research
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.107.025804/fulltext
Reference41 articles.
1. Physics of Neutron Star Crusts
2. Pulsar glitches and restlessness as a hard superfluidity phenomenon
3. Neutron conduction in the inner crust of a neutron star in the framework of the band theory of solids
4. Pulsar Glitches: The Crust is not Enough
5. Superfluid hydrodynamics in the inner crust of neutron stars
Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Effects of dilute neutron matter on the neutron star crust equation of state;The European Physical Journal A;2024-04-23
2. Effect of the equation of state for dilute neutron matter on the composition of the inner crust of neutron stars;Physical Review C;2024-04-08
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