國立虎尾科技大學 |

Gravitational wave astrophysics with pulsar timing arrays

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/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. -
電子資源:	http://dx.doi.org/10.1007/978-3-319-18401-2
ISBN:	9783319184012

Gravitational wave astrophysics with pulsar timing arrays
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:

592106
Gravitational waves.

LC Class. No.: QC179

Dewey Class. No.: 539.754

Gravitational wave astrophysics with pulsar timing arrays
LDR:02374nam a2200337 a 4500 001 861141
003 DE-He213
005 20160729172234.0
006 m d
007 cr nn 008maaau
008 170720s2016 gw s 0 eng d
020 $a 9783319184012 $q (electronic bk.)
020 $a 9783319184005 $q (paper)
024 7 $a 10.1007/978-3-319-18401-2 $2 doi
035 $a 978-3-319-18401-2
040 $a GP $c GP
041 0 $a eng
050 4 $a QC179
072 7 $a PGC $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a SCI005000 $2 bisacsh
082 0 4 $a 539.754 $2 23
090 $a QC179 $b .M664 2016
100 1 $a Mingarelli, Chiara M. F. $3 1103323
245 1 0 $a Gravitational wave astrophysics with pulsar timing arrays $h [electronic resource] / $c by Chiara M. F. Mingarelli.
260 $a Cham : $c 2016. $b Springer International Publishing : $b Imprint: Springer,
300 $a xix, 119 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a 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.
520 $a 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.
650 0 $a Gravitational waves. $3 592106
650 0 $a Astrophysics. $3 646223
650 1 4 $a Physics. $3 564049
650 2 4 $a Astronomy, Astrophysics and Cosmology. $3 593936
650 2 4 $a Classical and Quantum Gravitation, Relativity Theory. $3 769093
710 2 $a SpringerLink (Online service) $3 593884
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 831604
856 4 0 $u http://dx.doi.org/10.1007/978-3-319-18401-2
950 $a Physics and Astronomy (Springer-11651)