Gravitational Wave Templates from Extreme Mass Ratio Inspirals

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F20%3A10423662" target="_blank" >RIV/00216208:11320/20:10423662 - isvavai.cz</a>
Result on the web
<a href="https://www.mff.cuni.cz/veda/konference/wds/proc/pdf20/WDS20_07_f1_Skoupy.pdf" target="_blank" >https://www.mff.cuni.cz/veda/konference/wds/proc/pdf20/WDS20_07_f1_Skoupy.pdf</a>
DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Gravitational Wave Templates from Extreme Mass Ratio Inspirals
Original language description
An extreme mass ratio inspiral takes place when a compact stellar object is inspiraling into a supermassive black hole due to gravitational radiation reaction. Gravitational waves (GWs) from this system can be calculated using the Teukolsky equation (TE). In our case, we compute the asymptotic GW fluxes of a spinning body orbiting a Kerr black hole by solving numerically the TE both in time and frequency domain. Our ultimate goal is to produce GW templates for space-based detectors such as LISA.
Czech name
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Czech description
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Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
WDS'20 Proceedings of Contributed Papers — Physics
ISBN
978-80-7378-435-5
ISSN
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e-ISSN
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Number of pages
7
Pages from-to
52-58
Publisher name
Matfyzpress
Place of publication
Praha
Event location
Praha/ZOOM
Event date
Sep 22, 2020
Type of event by nationality
EUR - Evropská akce
UT code for WoS article
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