Next-to-next-to-leading order post-Newtonian spin-orbit Hamiltonian for self-gravitating binaries

Annalen der Physik (Leipzig)

Volumn 523, Issue 10, 2011, Pages 783-790

  Hartung, J ^a   Steinhoff, J ^a  

^a FRIEDRICH SCHILLER UNIVERSITY JENA   (Germany)

Author keywords

approximation methods; binary stars.; canonical formalism; equations of motion; Post Newtonian approximation

Indexed keywords

APPROXIMATION METHODS; BINARY STARS.; BLACK HOLES; CANONICAL FORMALISM; CENTER-OF-MASS; COMPACT OBJECTS; NEXT-TO-NEXT-TO-LEADING ORDERS; POINCARE; POST-NEWTONIAN APPROXIMATION; SPIN ORBITS;

ALGEBRA; APPROXIMATION THEORY; EQUATIONS OF MOTION; GRAVITATION; ROTATION; STARS;

HAMILTONIANS;

EID: 80052982788     PISSN: 00033804     EISSN: 15213889     Source Type: Journal    
DOI: 10.1002/andp.201100094     Document Type: Article

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