1996
DOI: 10.1103/physrevd.54.4185
|View full text |Cite
|
Sign up to set email alerts
|

Remarks on the issue of time and complex numbers in canonical quantum gravity

Abstract: Upon using some special example in the homogeneous cosmological model we develop the idea that, as a result of the arbitrariness of the factor ordering in Wheeler-DeWitt equation, gauge phases can not, in general, being completely removed from the wave functional in quantum gravity. The latter may be conveniently described by means of a remnant complex term in WDW equation depending on the factor ordering. Taking this equation for granted we can obtain WKB complex solutions and, therefore, we should be able to… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1

Citation Types

0
2
0

Year Published

1998
1998
2017
2017

Publication Types

Select...
1
1

Relationship

1
1

Authors

Journals

citations
Cited by 2 publications
(2 citation statements)
references
References 13 publications
0
2
0
Order By: Relevance
“…The intransparent mixture of quantity and structure however may lead to confusion about the meaning and role of complex numbers in quantum mechanics and physics in general. This is indicated by the discussion about the meaning of complex numbers in QM that is ongoing for decades [22][23][24][25][26][27][28][29][30][31][32][33][34] .…”
Section: Some Formal Considerationsmentioning
confidence: 99%
“…The intransparent mixture of quantity and structure however may lead to confusion about the meaning and role of complex numbers in quantum mechanics and physics in general. This is indicated by the discussion about the meaning of complex numbers in QM that is ongoing for decades [22][23][24][25][26][27][28][29][30][31][32][33][34] .…”
Section: Some Formal Considerationsmentioning
confidence: 99%
“…In other words, the reality of the wave function implies that the asymptotically flat spacetime is just the extreme Reissner-Nordström black hole. Since time is absent from this quantum theory , such a complex conjugation invariance could be required by the consistence of the quantisation procedure (although, quantum gravity might not satisfy this requirement strictly 11 ). On the other hand, the existence of a finite differences equation seems to be a fact related with the speculations of Wheeler 1 in the sense that spacetime might not be considered as classical on scales of the order of the Planck length (a ∼ M −1 ), i.e., in our terms, that the continuous character of spacetime can only be recovered, we will see, as an approximated phenomenon having a semiclassical meaning.…”
Section: Lorentzian Wormholesmentioning
confidence: 99%