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Titlebook: Globular Cluster Binaries and Gravitational Wave Parameter Estimation; Challenges and Effic Carl-Johan Haster Book 2017 Springer Internatio

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發(fā)表于 2025-3-21 17:44:23 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Globular Cluster Binaries and Gravitational Wave Parameter Estimation
副標(biāo)題Challenges and Effic
編輯Carl-Johan Haster
視頻videohttp://file.papertrans.cn/388/387016/387016.mp4
概述Nominated as an outstanding PhD thesis by the University of Birmingham, Birmingham, UK.Explores diverse aspects of the new field of gravitational wave astrophysics.Discusses the interface between the
叢書名稱Springer Theses
圖書封面Titlebook: Globular Cluster Binaries and Gravitational Wave Parameter Estimation; Challenges and Effic Carl-Johan Haster Book 2017 Springer Internatio
描述.This thesis presents valuable contributions to several aspects of the rapidly growing field of gravitational wave astrophysics. The potential sources of gravitational waves in globular clusters are analyzed using sophisticated dynamics simulations involving intermediate mass black holes and including, for the first time, high-order post-Newtonian corrections to the equations of motion. The thesis further demonstrates our ability to accurately measure the parameters of the sources involved in intermediate-mass-ratio inspirals of stellar-mass compact objects into hundred-solar-mass black holes. Lastly, it proposes new techniques for the computationally efficient inference on gravitational waves.. .On 14 September 2015, the LIGO observatory reported the first direct detection of gravitational waves from the merger of a pair of black holes. For a brief fraction of a second, the power emitted by this merger exceeded the combined output of all stars in the visible universe. This has since been followed by another confirmed detection and a third candidate binary black hole merger. These detections heralded the birth of an exciting new field: gravitational-wave astrophysics..
出版日期Book 2017
關(guān)鍵詞Gravitational Wave Parameters; Globular Clusters; Intermediate Mass Black Holes; Compact Binaries; LIGO;
版次1
doihttps://doi.org/10.1007/978-3-319-63441-8
isbn_softcover978-3-319-87556-9
isbn_ebook978-3-319-63441-8Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer International Publishing AG 2017
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 21:06:02 | 只看該作者
Book 2017 of gravitational waves in globular clusters are analyzed using sophisticated dynamics simulations involving intermediate mass black holes and including, for the first time, high-order post-Newtonian corrections to the equations of motion. The thesis further demonstrates our ability to accurately me
板凳
發(fā)表于 2025-3-22 01:09:10 | 只看該作者
978-3-319-87556-9Springer International Publishing AG 2017
地板
發(fā)表于 2025-3-22 06:42:41 | 只看該作者
Globular Cluster Binaries and Gravitational Wave Parameter Estimation978-3-319-63441-8Series ISSN 2190-5053 Series E-ISSN 2190-5061
5#
發(fā)表于 2025-3-22 09:26:33 | 只看該作者
https://doi.org/10.1007/978-3-319-63441-8Gravitational Wave Parameters; Globular Clusters; Intermediate Mass Black Holes; Compact Binaries; LIGO;
6#
發(fā)表于 2025-3-22 16:12:06 | 只看該作者
Thomas A. Arcury,Sara A. QuandtThe scientific field of observational gravitational wave astrophysics was, a century after the initial theoretical predictions [., .], initiated by the observation of the coalescence of a system of binary black holes named GW150914 [.].
7#
發(fā)表于 2025-3-22 19:06:07 | 只看該作者
8#
發(fā)表于 2025-3-22 21:49:37 | 只看該作者
Feine Linie: Gegenstandsbereiche,This chapter is adapted from a paper by ., Ilya Mandel and Will M. Farr.
9#
發(fā)表于 2025-3-23 03:16:27 | 只看該作者
Nonisothermal Incompressible Fluid Flow,In this thesis the concepts surrounding binaries of compact objects such as neutron stars and black holes have been considered in many of their aspects.
10#
發(fā)表于 2025-3-23 08:17:32 | 只看該作者
Introduction,The scientific field of observational gravitational wave astrophysics was, a century after the initial theoretical predictions [., .], initiated by the observation of the coalescence of a system of binary black holes named GW150914 [.].
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