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.
面頁冊數:	XIX, 119 p. 20 illus., 16 illus. in color.online resource. :
Contained By:	Springer Nature eBook
標題:	Astronomy. -
電子資源:	https://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. - 1st ed. 2016. - XIX, 119 p. 20 illus., 16 illus. in color.online resource. - Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053. - Springer Theses, Recognizing Outstanding Ph.D. Research,.

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:

593935
Astronomy.

LC Class. No.: QB1-991

Dewey Class. No.: 520

Gravitational Wave Astrophysics with Pulsar Timing Arrays
LDR:02778nam a22004095i 4500 001 982085
003 DE-He213
005 20200705063514.0
007 cr nn 008mamaa
008 201211s2016 gw | s |||| 0|eng d
020 $a 9783319184012 $9 978-3-319-18401-2
024 7 $a 10.1007/978-3-319-18401-2 $2 doi
035 $a 978-3-319-18401-2
050 4 $a QB1-991
050 4 $a QB460-466
072 7 $a PG $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a PGC $2 thema
082 0 4 $a 520 $2 23
100 1 $a Mingarelli, Chiara M. F. $4 aut $4 http://id.loc.gov/vocabulary/relators/aut $3 1103323
245 1 0 $a Gravitational Wave Astrophysics with Pulsar Timing Arrays $h [electronic resource] / $c by Chiara M. F. Mingarelli.
250 $a 1st ed. 2016.
264 1 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2016.
300 $a XIX, 119 p. 20 illus., 16 illus. in color. $b online resource.
336 $a text $b txt $2 rdacontent
337 $a computer $b c $2 rdamedia
338 $a online resource $b cr $2 rdacarrier
347 $a text file $b PDF $2 rda
490 1 $a Springer Theses, Recognizing Outstanding Ph.D. Research, $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 Astronomy. $3 593935
650 0 $a Astrophysics. $3 646223
650 0 $a Gravitation. $3 591793
650 1 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 Nature eBook
776 0 8 $i Printed edition: $z 9783319184005
776 0 8 $i Printed edition: $z 9783319184029
830 0 $a Springer Theses, Recognizing Outstanding Ph.D. Research, $x 2190-5053 $3 1253569
856 4 0 $u https://doi.org/10.1007/978-3-319-18401-2
912 $a ZDB-2-PHA
912 $a ZDB-2-SXP
950 $a Physics and Astronomy (SpringerNature-11651)
950 $a Physics and Astronomy (R0) (SpringerNature-43715)