Phys. Rev. D 55, 1112–1113 (1997)Comment on “Hypertime formalism for spherically symmetric black holes and wormholes”Received 16 January 1996; published in the issue dated 15 January 1997 The hypertime formalism for spherically symmetric spacetimes given by Braham suffers from the so-called spacetime problem of time. The canonical variables T± introduced there are not spacetime scalars, and thus fail to qualify as embedding variables for the theory. © 1997 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevD.55.1112
DOI:
10.1103/PhysRevD.55.1112
PACS:
04.20.Gz, 04.60.Ds, 04.70.Dy
See AlsoOriginal Article: Stephen P. Braham, Hypertime formalism for spherically symmetric black holes and wormholes, Phys. Rev. D 51, 536 (1995). |
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