Nonlinear wave equations for relativity

Maurice H. P. M. van Putten and Douglas M. Eardley
Phys. Rev. D 53, 3056 – Published 15 March 1996
PDFExport Citation

Abstract

Gravitational wave motion is described by nonlinear wave equations using the tetrad and its connection as field variables. The wave equations result from a Lorentz gauge on the connections. This description separates the physics of wave motion from the causal structure, which is evolved in the tangent space. The initial data constraints are derived in this approach using Yang-Mills scalar and vector potentials, resulting in Lie constraints associated with the additional Poincaré gauge invariance. The analogy of the constraint equations with those in Ashtekar's variables is emphasized.

  • Received 15 May 1995

DOI:https://doi.org/10.1103/PhysRevD.53.3056

©1996 American Physical Society

Authors & Affiliations

Maurice H. P. M. van Putten*

  • Center for Radiophysics and Space Research and Cornell Theory Center, Cornell University, Ithaca, New York 14853-6801

Douglas M. Eardley

  • Institute for Theoretical Physics, University of California, Santa Barbara, California 93106-4030

  • *Electronic address: vanputte@spacenet.tn.cornell.edu
  • Electronic address: doug@itp.ucsb.edu

References (Subscription Required)

Click to Expand
Issue

Vol. 53, Iss. 6 — 15 March 1996

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×