支形吊灯
发表于 2025-3-23 13:17:21
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镇压
发表于 2025-3-23 16:11:33
Pairing Interactions in Neutron Stars treated in a semi-empirical way, long-range fluctuations are incorporated consistently by solving coupled two-body equations for the particle-hole interaction and the scattering amplitude at the Fermi surface. The solutions determine the quasiparticle effective mass and the pairing matrix element f
Spangle
发表于 2025-3-23 18:33:15
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ULCER
发表于 2025-3-24 00:27:32
The Formation of Neutron Stars in The Galaxy accretion-induced collapse of heavy white dwarfs. This article discusses constraints on both scenarios based on observations of supernovae, supernova remnants, binary radio pulsars and radio pulsars in globular clusters.
FOIL
发表于 2025-3-24 03:53:25
Core Collapse Supernovae and Neutron Star Formationare likely to originate from massive stars, . ≳ 8.., at the end of their quiet hydrostatic nuclear burning and the final outcome is generally believed to be the birth event of most neutron stars. If this picture is correct the energy observed in the explosion must ultimately come from the gain in gr
Offensive
发表于 2025-3-24 09:56:02
Neutron Star Formation in Close Binary Systemsf accretion-induced collapse of white dwarfs are examined in relation to the origin of low mass X-ray binaries and binary millisecond pulsars. The outcome of the evolution of accreting white dwarfs is summarized as functions of accretion rate and the initial mass of the white dwarf. (2) Secondly dis
sparse
发表于 2025-3-24 13:44:50
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高贵领导
发表于 2025-3-24 17:27:28
Vaporizing Neutron Stars in Low-Mass X-Ray Binaries and the Statistics of Millisecond Pulsars companion irradiation. Here we discuss the main features of a radiation-driven (RD) evolutionary model that may be applicable to several LMXBs. According to this model, radiation from the accreting compact star in LMXBs ‘vaporizes’ the accretion disk and the companion star by driving a self-sustain
Crohns-disease
发表于 2025-3-24 21:17:23
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Processes
发表于 2025-3-25 01:10:14
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