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Globular cluster binaries and gravit...

Haster, Carl-Johan.

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Globular cluster binaries and gravitational wave parameter estimation = challenges and efficient solutions /

Record Type:	Electronic resources : Monograph/item
Title/Author:	Globular cluster binaries and gravitational wave parameter estimation/ by Carl-Johan Haster.
Reminder of title:	challenges and efficient solutions /
Author:	Haster, Carl-Johan.
Published:	Cham :Springer International Publishing : : 2017.,
Description:	xii, 92 p. :ill., digital ;24 cm.
[NT 15003449]:	Introduction -- N-body Dynamics of Intermediate Mass Ratio Inspirals -- Inference on Gravitational Waves from Coalescences of Stellar-mass Compact Objects and Intermediate-mass Black Holes -- Efficient Method for Measuring the Parameters Encoded in a Gravitational-wave Signal -- Conclusion.
Contained By:	Springer eBooks
Subject:	Astrophysics. -
Online resource:	http://dx.doi.org/10.1007/978-3-319-63441-8
ISBN:	9783319634418

Globular cluster binaries and gravitational wave parameter estimation = challenges and efficient solutions /
Haster, Carl-Johan.

Globular cluster binaries and gravitational wave parameter estimationchallenges and efficient solutions /[electronic resource] :by Carl-Johan Haster. - Cham :Springer International Publishing :2017. - xii, 92 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- N-body Dynamics of Intermediate Mass Ratio Inspirals -- Inference on Gravitational Waves from Coalescences of Stellar-mass Compact Objects and Intermediate-mass Black Holes -- Efficient Method for Measuring the Parameters Encoded in a Gravitational-wave Signal -- Conclusion.

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.

ISBN: 9783319634418

Standard No.: 10.1007/978-3-319-63441-8doiSubjects--Topical Terms:

535904
Astrophysics.

LC Class. No.: QB461

Dewey Class. No.: 523.01

Globular cluster binaries and gravitational wave parameter estimation = challenges and efficient solutions /
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300 $a xii, 92 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a Introduction -- N-body Dynamics of Intermediate Mass Ratio Inspirals -- Inference on Gravitational Waves from Coalescences of Stellar-mass Compact Objects and Intermediate-mass Black Holes -- Efficient Method for Measuring the Parameters Encoded in a Gravitational-wave Signal -- Conclusion.
520 $a 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.
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650 0 $a Gravitational waves. $3 805566
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650 2 4 $a Numerical and Computational Physics, Simulation. $3 2209853
650 2 4 $a Classical and Quantum Gravitation, Relativity Theory. $3 1067066
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