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A quasi-Keplerian parameterisation for the solutions of second post-Newtonian (PN) accurate equations of motion for spinning compact binaries is obtained including leading order spin-spin and next-to-leading order spin-orbit interactions.
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2001
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R.-M. Memmesheimer, A. Gopakumar, and G. Schäfer, “Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits,” Phys. Rev. D
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2008
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2008
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2008
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2008
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2008
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2008
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2008
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J. Majár and M. Vasúth, “Gravitational waveforms for spinning compact binaries,” Phys. Rev. D
2008
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2009
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P. Ajith, S. Babak, Y. Chen, M. Hewitson, B. Krishnan, A. M. Sintes, J. T. Whelan, B. Brügmann, P. Diener, N. Dorband, J. Gonzalez, M. Hannam, S. Husa, D. Pollney, L. Rezzolla, L. Santamaría, U. Sperhake, and J. Thornburg, “Erratum: Template bank for gravitational waveforms from coalescing binary black holes: Nonspinning binaries,” Phys. Rev. D
2009
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2009
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unpublished
C. Sohr, “Chaos in gravitativ-gebundenen Binärsystemen mit Spin.,” diploma thesis, Friedrich-Schiller-Universität Jena, 2009 · 2009
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2009
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L. Blanchet, A. Buonanno, and G. Faye, “Erratum: Higher-order spin effects in the dynamics of compact binaries. II. Radiation field,” Phys. Rev. D
2010
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2010
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2010
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