- Gibbons-Hawking-York boundary term
In
general relativity , the Gibbons-Hawking-York boundary term is a term that needs to be added to theEinstein-Hilbert action when the underlyingspacetime manifold has a boundary.The Einstein-Hilbert action is the basis for the most elementary
variational principle from which the field equations of general relativity can be defined. However, the use of the Einstein-Hilbert action is appropriate only when the underlying spacetime manifold is closed, i.e., a manifold which is both compact and without boundary. In the event that the manifold has a boundary , the action should be supplemented by a boundary term so that the variational principle is well-defined. The necessity of such a boundary term was first realised by York and later refined in a minor way by Gibbons and Hawking. For a closed manifold the appropriate action is:,
where is the Einstein-Hilbert action, is the Gibbons-Hawking-York boundary term, is the induced metric on the boundary and is the trace of the second fundamental form. Varying the action with respect to the metric gives the Einstein equations; the addition of the boundary term means that in performing the variation, the geometry of the boundary encoded in the induced metric is fixed. There remains ambiguity in the action up to an arbitrary functional of the induced metric .
References
*cite journal|url=http://prola.aps.org/abstract/PRL/v28/i16/p1082_1|author=J. W. York|title=Role of conformal three-geometry in the dynamics of gravitation|journal=Phys. Rev. Lett.|volume=28|pages=1082|year=1972|doi=10.1103/PhysRevLett.28.1082|format=abstract
*cite journal|url=http://prola.aps.org/abstract/PRD/v15/i10/p2752_1|author=G. W. Gibbons and S. W. Hawking|title=Action integrals and partition functions in quantum gravity|journal=Phys. Rev. D|volume=15|pages=2752|year=1977|doi=10.1103/PhysRevD.15.2752|format=abstract
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