2015

Spin effects on the dynamics of compact binaries

Steinhoff, Jan

Understand

Compact binaries are the most promising source for the advanced gravitational wave detectors, which will start operating this year.

The influence of spin on the binary evolution is an important consequence of general relativity and can be large.
It is argued that the spin supplementary condition, which is related to the observer dependence of the center, gives rise to a gauge symmetry in the action principle of spinning point-particles.
These spinning point-particles serve as an analytic model for extended bodies.

Built on

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Similar

S. Hergt and G. Schäfer, “Higher-order-in-spin interaction Hamiltonians for binary black holes from Poincare invariance,” Phys. Rev
Original
2008
Cited alongside, same era.
R. A. Porto, “Next to leading order spin-orbit effects in the motion of inspiralling compact binaries,” Class. Quant. Grav
Original
2010
Cited alongside, same era.
M. Levi, “Next to Leading Order gravitational Spin-Orbit coupling in an Effective Field Theory approach,” Phys. Rev
Original
2010
Cited alongside, same era.
R. A. Porto and I. Z. Rothstein, “Next to Leading Order Spin(1)Spin(1) Effects in the Motion of Inspiralling Compact Binaries,” Phys. Rev
Original
2010
Cited alongside, same era.
R. A. Porto and I. Z. Rothstein, “Spin(1)Spin(2) Effects in the Motion of Inspiralling Compact Binaries at Third Order in the Post-Newtonian Expansion,” Phys. Rev
Original
2010
Cited alongside, same era.
M. Levi, “Next to Leading Order gravitational Spin1-Spin2 coupling with Kaluza-Klein reduction,” Phys. Rev
Original
2010
Cited alongside, same era.
World Scientific, Singapore, 2011
Original
D. L. Perrodin, “Subleading Spin-Orbit Correction to the Newtonian Potential in Effective Field Theory Formalism,” in Proceedings of the 12th Marcel Grossmann Meeting on General Relativity · 2011
Cited alongside, same era.
J. Hartung and J. Steinhoff, “Next-to-next-to-leading order post-Newtonian spin-orbit Hamiltonian for self-gravitating binaries,” Annalen Phys
Original
2011
Cited alongside, same era.
J. Hartung and J. Steinhoff, “Next-to-next-to-leading order post-Newtonian spin(1)-spin(2) Hamiltonian for self-gravitating binaries,” Annalen Phys
Original
2011
Cited alongside, same era.
J. Steinhoff, “Canonical formulation of spin in general relativity,” Annalen Phys
Original
2011
Cited alongside, same era.
M. Levi, “Binary dynamics from spin1-spin2 coupling at fourth post-Newtonian order,” Phys. Rev
Original
2012
Cited alongside, same era.
J. Hartung, J. Steinhoff, and G. Schäfer, “Next-to-next-to-leading order post-Newtonian linear-in-spin binary Hamiltonians,” Annalen Phys
Original
2013
Cited alongside, same era.

Then

T. Damour, P. Jaranowski, and G. Schäfer, “Nonlocal-in-time action for the fourth post-Newtonian conservative dynamics of two-body systems,” Phys. Rev
Original
2014
Later among the works it cites.
L. Blanchet, “Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries,” Living Rev. Rel
Original
2014
Later among the works it cites.
M. Levi and J. Steinhoff, “Equivalence of ADM Hamiltonian and Effective Field Theory approaches at next-to-next-to-leading order spin1-spin2 coupling of binary inspirals,” JCAP
Original
2014
Later among the works it cites.
G. Pappas and T. A. Apostolatos, “Effectively universal behavior of rotating neutron stars in general relativity makes them even simpler than their Newtonian counterparts,” Phys. Rev. Lett
Original
2014
Later among the works it cites.
S. Chakrabarti, T. Delsate, N. Gürlebeck, and J. Steinhoff, “I-Q relation for rapidly rotating neutron stars,” Phys. Rev. Lett
Original
2014
Later among the works it cites.
K. Yagi, K. Kyutoku, G. Pappas, N. Yunes, and T. A. Apostolatos, “Effective No-Hair Relations for Neutron Stars and Quark Stars: Relativistic Results,” Phys. Rev
Original
2014
Later among the works it cites.
M. Levi and J. Steinhoff, “Next-to-next-to-leading order gravitational spin-orbit coupling via the effective field theory for spinning objects in the post-Newtonian scheme,” JCAP (accepted)
Original
2015
Closest in time.
M. Levi and J. Steinhoff, “Next-to-next-to-leading order gravitational spin-squared potential via the effective field theory for spinning objects in the post-Newtonian scheme,” JCAP (accepted)
Original
2015
Closest in time.
M. Levi and J. Steinhoff, “Spinning gravitating objects in the effective field theory in the post-Newtonian scheme,” JHEP
Original
2015
Closest in time.
A. Bohé, G. Faye, S. Marsat, and E. K. Porter, “Quadratic-in-spin effects in the orbital dynamics and gravitational-wave energy flux of compact binaries at the 3PN order,” Class. Quant. Grav
Original
2015
Closest in time.
M. Levi and J. Steinhoff, “Leading order finite size effects with spins for inspiralling compact binaries,” JHEP
Original
2015
Closest in time.
S. Marsat, “Cubic order spin effects in the dynamics and gravitational wave energy flux of compact object binaries,” Class. Quant. Grav
Original
2015
Closest in time.
V. Vaidya, “Gravitational spin Hamiltonians from the S matrix,” Phys. Rev
Original
2015
Closest in time.
J. Steinhoff, “Spin and quadrupole contributions to the motion of astrophysical binaries,” Fund. Theor. Phys
Original
2015
Closest in time.
S. Hergt, J. Steinhoff, and G. Schäfer, “Reduced Hamiltonian for next-to-leading order Spin-Squared Dynamics of General Compact Binaries,” Class. Quant. Grav
Original
2093
Closest in time.
S. Hergt, J. Steinhoff, and G. Schäfer, “Elimination of the spin supplementary condition in the effective field theory approach to the post-Newtonian approximation,” Annals Phys
Original
2094
Closest in time.

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