標(biāo)題: Titlebook: Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants; Praveen Manoharan Book 2022 The Editor(s) (if applicable) an [打印本頁] 作者: Inoculare 時(shí)間: 2025-3-21 19:43
書目名稱Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants影響因子(影響力)
書目名稱Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants影響因子(影響力)學(xué)科排名
書目名稱Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants網(wǎng)絡(luò)公開度
書目名稱Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants被引頻次
書目名稱Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants被引頻次學(xué)科排名
書目名稱Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants年度引用
書目名稱Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants年度引用學(xué)科排名
書目名稱Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants讀者反饋
書目名稱Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants讀者反饋學(xué)科排名
作者: 狗舍 時(shí)間: 2025-3-21 22:35
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).作者: 難管 時(shí)間: 2025-3-22 03:29
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.作者: pulse-pressure 時(shí)間: 2025-3-22 08:04 作者: Yag-Capsulotomy 時(shí)間: 2025-3-22 09:50
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.作者: 售穴 時(shí)間: 2025-3-22 14:45 作者: 結(jié)合 時(shí)間: 2025-3-22 17:36
978-3-658-36840-1The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Fachmedien Wies作者: 歡騰 時(shí)間: 2025-3-22 22:22
Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants978-3-658-36841-8Series ISSN 2625-3577 Series E-ISSN 2625-3615 作者: Lumbar-Spine 時(shí)間: 2025-3-23 01:28 作者: 潛移默化 時(shí)間: 2025-3-23 06:03 作者: 血友病 時(shí)間: 2025-3-23 09:48 作者: 圍巾 時(shí)間: 2025-3-23 14:26 作者: OTTER 時(shí)間: 2025-3-23 18:54
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.作者: 用樹皮 時(shí)間: 2025-3-24 01:49
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.作者: 直覺沒有 時(shí)間: 2025-3-24 02:39 作者: 有組織 時(shí)間: 2025-3-24 08:19 作者: Spina-Bifida 時(shí)間: 2025-3-24 12:47 作者: hurricane 時(shí)間: 2025-3-24 16:11
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 作者: inclusive 時(shí)間: 2025-3-24 19:18 作者: Counteract 時(shí)間: 2025-3-25 02:27 作者: barium-study 時(shí)間: 2025-3-25 04:38
Praveen Manoharanearch by a group of experts led by Tiankui Jing, one of Chin.This book examines?the origins?and?basic concepts?of sociology in China?and traces the discipline’s evolutionary trajectory. Building on the premise that .qunxue., which goes back to Xunzi,?is essentially the Chinese antecedent of modern/W作者: 消瘦 時(shí)間: 2025-3-25 11:09 作者: 收養(yǎng) 時(shí)間: 2025-3-25 12:50 作者: 心神不寧 時(shí)間: 2025-3-25 15:55
Praveen Manoharanic circumstances surrounding their original?formation, and the differences in the political environments in which they later developed..978-3-319-81956-3978-3-319-39750-4Series ISSN 2523-336X Series E-ISSN 2523-3378 作者: constellation 時(shí)間: 2025-3-25 22:46 作者: Campaign 時(shí)間: 2025-3-26 02:44
ho used the text as a reference for graduate seminars and courses that the book would need to be updated to stay abreast of the discoveries and progress in this rapidly evolving field. After some discussion we concluded that a new edition of the book was warranted and that the goal of producing a ne作者: decode 時(shí)間: 2025-3-26 05:51
Praveen Manoharanrvational cos- mology. The realization of the new relevance of the subject of the workshop and the questions raised by the observational results, in addition to bring- ing TV crews and newspaper journalists, naturally influenced and stimulated many discussions among the participants. The success of 作者: Constitution 時(shí)間: 2025-3-26 09:25
Praveen Manoharanition to turbulence is initi- ated by free-stream oscillations inducing local separations near wall. Up to the 1940s, skepticism of the stability theory predominated, in particular due to the experimental results of Dryden (1934, 1936). Only the experiments of Schubauer and Skramstad (1948) revealed作者: Confess 時(shí)間: 2025-3-26 14:22 作者: 世俗 時(shí)間: 2025-3-26 20:08 作者: 新星 時(shí)間: 2025-3-26 21:29
Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants作者: 熒光 時(shí)間: 2025-3-27 03:20 作者: 改良 時(shí)間: 2025-3-27 06:41 作者: NADIR 時(shí)間: 2025-3-27 10:11 作者: 愛國者 時(shí)間: 2025-3-27 14:45 作者: Offensive 時(shí)間: 2025-3-27 20:24 作者: LAST 時(shí)間: 2025-3-27 23:07
