Comment on “Hypertime formalism for spherically symmetric black holes and wormholes”

Joseph D. Romano

doi:10.1103/PhysRevD.55.1112

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Comment on “Hypertime formalism for spherically symmetric black holes and wormholes”

Joseph D. Romano

Department of Physics, University of Wisconsin–Milwaukee, Milwaukee, Wisconsin 53201

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Phys. Rev. D 55, 1112 – Published 15 January, 1997

DOI: https://doi.org/10.1103/PhysRevD.55.1112

Abstract

The hypertime formalism for spherically symmetric spacetimes given by Braham suffers from the so-called spacetime problem of time. The canonical variables $T^{\pm}$ introduced there are not spacetime scalars, and thus fail to qualify as embedding variables for the theory.

Original Article

Hypertime formalism for spherically symmetric black holes and wormholes

Stephen P. Braham

Phys. Rev. D 51, 536 (1995)

References (4)

K. V. Kuchař, J. Math. Phys. (N.Y.)13, 768 (1972).
K. V. Kuchař, in Proceedings of the 4th Canadian Conference on General Relativity and Relativistic Astrophysics, edited by G. Kunstatter, D. Vincent, and J. Williams (World Scientific, Singapore, 1992).
K. V. Kuchař, Phys. Rev. D45, 4443 (1992).
S. P. Braham, Phys. Rev. D51, 536 (1995).

[c1] K. V. Kuchař, J. Math. Phys. (N.Y.)13, 768 (1972).

[c2] K. V. Kuchař, in Proceedings of the 4th Canadian Conference on General Relativity and Relativistic Astrophysics, edited by G. Kunstatter, D. Vincent, and J. Williams (World Scientific, Singapore, 1992).

[c3] K. V. Kuchař, Phys. Rev. D45, 4443 (1992).

[c4] S. P. Braham, Phys. Rev. D51, 536 (1995).

Physical Review D

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Comment on “Hypertime formalism for spherically symmetric black holes and wormholes”

Abstract

Original Article

Hypertime formalism for spherically symmetric black holes and wormholes

References (4)

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