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Adiabatic equatorial inspirals of a spinning body into a Kerr black hole

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00558962" target="_blank" >RIV/67985815:_____/22:00558962 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/22:10446336

  • Result on the web

    <a href="https://doi.org/10.1103/PhysRevD.105.084033" target="_blank" >https://doi.org/10.1103/PhysRevD.105.084033</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1103/PhysRevD.105.084033" target="_blank" >10.1103/PhysRevD.105.084033</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Adiabatic equatorial inspirals of a spinning body into a Kerr black hole

  • Original language description

    The detection of gravitational waves from extreme mass ratio inspirals (EMRIs) by the future space based gravitational-wave detectors demands the generation of accurate enough waveform templates. Since the spin of the smaller secondary body cannot be neglected for the detection and parameter estimation of EMRIs, we study its influence on the phase of the gravitational waves from EMRIs with a spinning secondary. We focus on generic eccentric equatorial orbits around a Kerr black hole. To model the spinning secondary object, we use the Mathisson-Papapetrou-Dixon equations in the pole-dipole approximation. Furthermore, we linearize in spin the orbital variables and the gravitational-wave fluxes from the respective orbits. We obtain these fluxes by using the Teukolsky formalism in the frequency domain. We derive the evolution equations for the spin-induced corrections to the adiabatic evolution of an inspiral. Finally, through their numerical integration, we find the gravitational-wave phase shift between an inspiral of a spinning and a nonspinning body.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/EF19_073%2F0016935" target="_blank" >EF19_073/0016935: Grant schemes at Charles University</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2022

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Physical Review D

  • ISSN

    2470-0010

  • e-ISSN

    2470-0029

  • Volume of the periodical

    105

  • Issue of the periodical within the volume

    8

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    23

  • Pages from-to

    084033

  • UT code for WoS article

    000807557100002

  • EID of the result in the Scopus database

    2-s2.0-85129235255