血友病
发表于 2025-3-23 09:48:57
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围巾
发表于 2025-3-23 14:26:40
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OTTER
发表于 2025-3-23 18:54:20
Theory, models for non-rotating neutron stars and numerically solving the corresponding TOV equations, as well as the computation of their tidal deformabilities. We will also briefly introduce the concept of quasi-normal modes of neutron stars which will be important for our subsequent analyses.
用树皮
发表于 2025-3-24 01:49:34
Results, we discussed in Chapter ., before we turn towards the novel results we developed in the context of this thesis: first, we relate the tidal deformability of a non-rotating star to the .-mode frequency of a rotating counterpart.
直觉没有
发表于 2025-3-24 02:39:45
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有组织
发表于 2025-3-24 08:19:51
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Spina-Bifida
发表于 2025-3-24 12:47:33
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hurricane
发表于 2025-3-24 16:11:45
Praveen Manoharanof Structure in the Universe" was organized to bring together workers in various aspects of relativistic cosmology with the aim of assessing the present status of our knowledge on the formation and evolution of structure. As it happened, the meeting was particularly timely. Only two days before the
inclusive
发表于 2025-3-24 19:18:29
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Counteract
发表于 2025-3-25 02:27:55
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