OCTO
发表于 2025-3-25 06:49:57
General relativistic stationary axisymmetric rotating systems,Following the 3+1 formalism of General Relativity we write the Einstein equations for a stationary rotating neutron star specially suited to be solved numerically with spectral methods. We also provide the equations of motion to study the normal modes once the star is perturbed from the stationary axisymmetric equilibrium configuration.
compose
发表于 2025-3-25 09:46:01
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expunge
发表于 2025-3-25 12:54:47
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发酵剂
发表于 2025-3-25 19:46:53
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施舍
发表于 2025-3-25 23:05:55
On the regularity of spherically symmetric static spacetimes,It is shown that the regularity of spherically symmetric static spacetimes is independent of the monotic behaviour of the equation of state and the isotropy of the pressure.
Focus-Words
发表于 2025-3-26 02:11:48
Shock capturing methods in 1D numerical relativity,A numerical code is presented which uses modern shock capturing methods to evolve spherically symmetric perfect fluid space-times. Harmonic slicing is used to ensure singularity avoidance, which is crucial in strong field situations. Some tests are presented, including an application to the stellar collapse problem.
无弹性
发表于 2025-3-26 05:03:40
Lecture Notes in Physicshttp://image.papertrans.cn/r/image/831834.jpg
GOUGE
发表于 2025-3-26 08:58:01
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为宠爱
发表于 2025-3-26 13:29:32
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恶名声
发表于 2025-3-26 18:11:02
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