无弹性
发表于 2025-3-25 06:08:09
Axisymmetric Rotating Compact Stars,to constrain compact star EoSs and hence on models of strong interaction. Such a constraint is made mainly via the inspiral GW signal. In fact, important clues could also be found in the post-merger phase by understanding the evolution of the merger remnant and its relation with the EM counterparts.
欢乐东方
发表于 2025-3-25 07:50:14
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Habituate
发表于 2025-3-25 14:17:42
Book 2020act stars is the subject of ongoing debates among astrophysicists and particle physicists, due to the non-perturbative property of strong interaction at low energy scales. The book investigates the tidal deformability and maximum mass of rotating quark stars and triaxially rotating quark stars, and
Ceramic
发表于 2025-3-25 19:04:46
Introduction,In this chapter, a brief history of the development of numerical relativity method, the 3+1 decompostion, initial data problem as well as equations of state of compact stars will be introduced. For more detailed introductions, one can find, for example, in [., .].
苦涩
发表于 2025-3-25 21:36:44
Triaxially Rotating Strange Stars,In the previous Chapter, we have discussed about the similarities and differences between uniformly rotating and differentially rotating neutron stars and strange stars, with axisymmetry. Nevertheless, in reality, due to the high mass, kinetic energy as well as strong magnetic fields of the merger remnant, the axisymmetry might be easily broken.
Lignans
发表于 2025-3-26 00:18:04
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Duodenitis
发表于 2025-3-26 07:01:48
Springer Theseshttp://image.papertrans.cn/t/image/881098.jpg
medium
发表于 2025-3-26 10:12:24
https://doi.org/10.1007/978-981-15-4151-3Numerical Relativity; Compact Star; Equation of State of Dense Matter; Star: Pulsar; Quark star model
Acetaldehyde
发表于 2025-3-26 13:33:20
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Bureaucracy
发表于 2025-3-26 19:09:31
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