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Автор Sperhake, U
Автор Brügmann, B
Автор Müller, D
Автор Sopuerta, C F
Дата выпуска 2011-07-07
dc.description We analyse an 11-orbit inspiral of a non-spinning black-hole binary with mass ratio q ≡ M<sub>1</sub>/M<sub>2</sub> = 4. The numerically obtained gravitational waveforms are compared with post-Newtonian (PN) predictions including several subdominant multipoles up to multipolar indices (l = 5, m = 5). We find that (i) numerical and post-Newtonian predictions of the phase of the (2, 2) mode accumulate a phase difference of about 0.35 rad at the PN cut-off frequency Mω = 0.1 for the Taylor T1 approximant when numerical and PN waveforms are matched over a window in the early inspiral phase; (ii) in contrast to previous studies of equal mass and specific spinning binaries, we find the Taylor T4 approximant to agree less well with numerical results, provided the latter are extrapolated to infinite extraction radius; (iii) extrapolation of gravitational waveforms to infinite extraction radius is particularly important for subdominant multipoles with l ≠ m; (iv) 3PN terms in post-Newtonian multipole expansions significantly improve the agreement with numerical predictions for subdominant multipoles.
Формат application.pdf
Издатель Institute of Physics Publishing
Копирайт 2011 IOP Publishing Ltd
Название 11-orbit inspiral of a mass ratio 4:1 black-hole binary
Тип paper
DOI 10.1088/0264-9381/28/13/134004
Electronic ISSN 1361-6382
Print ISSN 0264-9381
Журнал Classical and Quantum Gravity
Том 28
Первая страница 134004
Последняя страница 134018
Аффилиация Sperhake, U; Institute of Space Sciences (CSIC-IEEC), Campus UAB, Torre C5 Parells, 08193 Bellaterra, Spain; California Institute of Technology, 1200 E California Boulevard, Pasadena, CA 91125, USA; Department of Physics and Astronomy, The University of Mississippi, University, MS 38677-1848, USA
Аффилиация Brügmann, B; Theoretisch Physikalisches Institut, Friedrich Schiller Universität, Max-Wien Platz 1, 07743 Jena, Germany
Аффилиация Müller, D; Theoretisch Physikalisches Institut, Friedrich Schiller Universität, Max-Wien Platz 1, 07743 Jena, Germany
Аффилиация Sopuerta, C F; Institute of Space Sciences (CSIC-IEEC), Campus UAB, Torre C5 Parells, 08193 Bellaterra, Spain
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