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Gravitational wave astrophysics with pulsar timing arrays[electronic resource] /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
杜威分類號:	539.754
書名/作者:	Gravitational wave astrophysics with pulsar timing arrays/ by Chiara M. F. Mingarelli.
作者:	Mingarelli, Chiara M. F.
出版者:	Cham : : Springer International Publishing :, 2016.
面頁冊數:	xix, 119 p. : : ill., digital ;; 24 cm.
Contained By:	Springer eBooks
標題:	Gravitational waves.
標題:	Astrophysics.
標題:	Physics.
標題:	Astronomy, Astrophysics and Cosmology.
標題:	Classical and Quantum Gravitation, Relativity Theory.
ISBN:	9783319184012
ISBN:	9783319184005
內容註:	Introduction -- Characterizing Gravitational Wave Stochastic Background Anisotropy with Pulsar Timing Arrays -- The Effect of Small Pulsar Distance Variations in Stochastic GW -- Observing the Dynamics of Supermassive Black Hole Binaries with Pulsar Timing -- Conclusions -- Appendix -- Bibliography.
摘要、提要註:	This Ph.D. thesis from the University of Birmingham UK opens new research avenues in the use of Pulsar Timing Arrays (PTAs) to study populations of super-massive black hole binaries through gravitational-wave observations. Chiara Mingarelli's work has shown for the first time that PTAs can yield information about the non-linear dynamics of the gravitational field. This is possible because PTAs capture, at the same time, radiation from the same source emitted at stages of its binary evolution that are separated by thousands of years. Dr. Mingarelli, who is the recipient of a Marie Curie International Outgoing Fellowship, has also been amongst the pioneers of the technique that will allow us to probe the level of anisotropy of the diffuse gravitational-wave background radiation from the whole population of super-massive black hole binaries in the Universe. Indeed, future observations will provide us with hints about the distribution of galaxies harboring massive black holes and insights into end products of hierarchical mergers of galaxies.
電子資源:	http://dx.doi.org/10.1007/978-3-319-18401-2

Gravitational wave astrophysics with pulsar timing arrays[electronic resource] /
Mingarelli, Chiara M. F.

Gravitational wave astrophysics with pulsar timing arrays[electronic resource] /by Chiara M. F. Mingarelli. - Cham :Springer International Publishing :2016. - xix, 119 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- Characterizing Gravitational Wave Stochastic Background Anisotropy with Pulsar Timing Arrays -- The Effect of Small Pulsar Distance Variations in Stochastic GW -- Observing the Dynamics of Supermassive Black Hole Binaries with Pulsar Timing -- Conclusions -- Appendix -- Bibliography.

This Ph.D. thesis from the University of Birmingham UK opens new research avenues in the use of Pulsar Timing Arrays (PTAs) to study populations of super-massive black hole binaries through gravitational-wave observations. Chiara Mingarelli's work has shown for the first time that PTAs can yield information about the non-linear dynamics of the gravitational field. This is possible because PTAs capture, at the same time, radiation from the same source emitted at stages of its binary evolution that are separated by thousands of years. Dr. Mingarelli, who is the recipient of a Marie Curie International Outgoing Fellowship, has also been amongst the pioneers of the technique that will allow us to probe the level of anisotropy of the diffuse gravitational-wave background radiation from the whole population of super-massive black hole binaries in the Universe. Indeed, future observations will provide us with hints about the distribution of galaxies harboring massive black holes and insights into end products of hierarchical mergers of galaxies.

ISBN: 9783319184012

Standard No.: 10.1007/978-3-319-18401-2doiSubjects--Topical Terms:

611534
Gravitational waves.

LC Class. No.: QC179

Dewey Class. No.: 539.754

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