English

A reference for the covariant Hamiltonian boundary term

General Relativity and Quantum Cosmology 2012-10-24 v1

Abstract

The Hamiltonian for dynamic geometry generates the evolution of a spatial region along a vector field. It includes a boundary term which determines both the value of the Hamiltonian and the boundary conditions. The value gives the quasi-local quantities: energy-momentum, angular-momentum/center-of-mass. The boundary term depends not only on the dynamical variables but also on their reference values; the latter determine the ground state (having vanishing quasi-local quantities). For our preferred boundary term for Einstein's GR we propose 4D isometric matching and extremizing the energy to determine the reference metric and connection values.

Keywords

Cite

@article{arxiv.1210.6148,
  title  = {A reference for the covariant Hamiltonian boundary term},
  author = {James M. Nester and Chiang-Mei Chen and Jian-Liang Liu and Gang Sun},
  journal= {arXiv preprint arXiv:1210.6148},
  year   = {2012}
}

Comments

submitted to the proceedings of the conference on Relativity and Gravitation: 100 Years after Einstein in Prague

R2 v1 2026-06-21T22:26:18.095Z