Higher-order-in-spin interaction Hamiltonians for binary black holes from source terms of Kerr geometry in approximate ADM coordinates
Journal Article
·
· Physical Review. D, Particles Fields
- Friedrich-Schiller-Universitaet Jena, Max-Wien-Platz 1, 07743 Jena (Germany)
The Kerr metric outside the ergosphere is transformed into Arnowitt-Deser-Misner coordinates up to the orders 1/r{sup 4} and a{sup 2}, respectively, in radial coordinate r and reduced angular momentum variable a, starting from the Kerr solution in quasi-isotropic as well as harmonic coordinates. The distributional source terms for the approximate solution are calculated. To leading order in linear momenta, higher-order-in-spin interaction Hamiltonians for black hole binaries are derived.
- OSTI ID:
- 21210184
- Journal Information:
- Physical Review. D, Particles Fields, Journal Name: Physical Review. D, Particles Fields Journal Issue: 10 Vol. 77; ISSN PRVDAQ; ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
Similar Records
Higher-order-in-spin interaction Hamiltonians for binary black holes from Poincare invariance
ADM canonical formalism for gravitating spinning objects
Next-to-leading order gravitational spin(1)-spin(2) dynamics in Hamiltonian form
Journal Article
·
Sun Dec 14 23:00:00 EST 2008
· Physical Review. D, Particles Fields
·
OSTI ID:21251128
ADM canonical formalism for gravitating spinning objects
Journal Article
·
Thu May 15 00:00:00 EDT 2008
· Physical Review. D, Particles Fields
·
OSTI ID:21204987
Next-to-leading order gravitational spin(1)-spin(2) dynamics in Hamiltonian form
Journal Article
·
Tue Apr 15 00:00:00 EDT 2008
· Physical Review. D, Particles Fields
·
OSTI ID:21249984