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Titlebook: Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants; Praveen Manoharan Book 2022 The Editor(s) (if applicable) an

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发表于 2025-3-21 19:43:26 | 显示全部楼层 |阅读模式
书目名称Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
编辑Praveen Manoharan
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丛书名称BestMasters
图书封面Titlebook: Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants;  Praveen Manoharan Book 2022 The Editor(s) (if applicable) an
描述In the last 25 years, an extensive body of work has developed various equation of state independent - or (approximately) universal - relations that allow for the inference of neutron star parameters from gravitational wave observations. These works, however, have mostly been focused on singular neutron stars, while our observational efforts at the present, and in the near future, will be focused on binary neutron star (BNS) mergers. In light of these circumstances, the last five years have also given rise to more attempts at developing universal relations that relate BNS pre-merger neutron stars to stellar parameters of the post-merger object, mostly driven by numerical relativity simulations. In this thesis a first attempt at perturbatively deriving universal relations for binary neutron star mergers with long-lived neutron star remnants is presented. The author succeeds in confirming previous results relating pre-merger binary tidal deformabilities to the f-mode frequency of the post-merger object. Combining this result with recent advances of computing the f-mode frequency of fast rotating neutron stars, he also derives a combined relation that relates the pre-merger binary tida
出版日期Book 2022
关键词Binary Neutron Star Merger; Perturbation Theory; Theoretical Astrophysics; Universal Relations; Neutron
版次1
doihttps://doi.org/10.1007/978-3-658-36841-8
isbn_softcover978-3-658-36840-1
isbn_ebook978-3-658-36841-8Series ISSN 2625-3577 Series E-ISSN 2625-3615
issn_series 2625-3577
copyrightThe Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Fachmedien Wies
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发表于 2025-3-21 22:35:49 | 显示全部楼层
Introduction,bled a new avenue into probing and understanding the structure of neutron stars: through the observation of these mergers, we can put constraints on the bulk properties of neutron stars [RMW18, MWRS18, BBV+20], which in turn will allow us to uncover their true equation of state (EoS).
发表于 2025-3-22 03:29:02 | 显示全部楼层
Related Work,te properties of neutron stars in an EoS independent manner. In the following, we outline some of these works involving the oscillations modes and tidal deformability of single neutron stars, before we tackle more recently proposed relations for binary neutron star mergers.
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发表于 2025-3-22 09:50:07 | 显示全部楼层
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.
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978-3-658-36840-1The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Fachmedien Wies
发表于 2025-3-22 22:22:16 | 显示全部楼层
Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants978-3-658-36841-8Series ISSN 2625-3577 Series E-ISSN 2625-3615
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