2003
DOI: 10.1088/1126-6708/2003/07/058
|View full text |Cite
|
Sign up to set email alerts
|

Remarks on 't Hooft's brick wall model

Abstract: A semi-classical reasoning leads to the non-commutativity of the space and time coordinates near the horizon of Schwarzschild black hole. This non-commutativity in turn provides a mechanism to interpret the brick wall thickness hypothesis in 't Hooft's brick wall model as well as the boundary condition imposed for the field considered. For concreteness, we consider a noncommutative scalar field model near the horizon and derive the effective metric via the equation of motion of noncommutative scalar field. Thi… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...

Citation Types

0
4
0

Year Published

2005
2005
2022
2022

Publication Types

Select...
5
1

Relationship

0
6

Authors

Journals

citations
Cited by 9 publications
(4 citation statements)
references
References 32 publications
0
4
0
Order By: Relevance
“…How to solve this dilemma? Recently Yans' works [5][6][7] solved the dilemma using the semi-classical effect at the horizon, which naturally led to the space-time noncommutative at the horizon, called as quantum horizon. In this treatment the classical horizon spreads, so the trouble due to the singularity on the horizon disappears.…”
mentioning
confidence: 99%
See 1 more Smart Citation
“…How to solve this dilemma? Recently Yans' works [5][6][7] solved the dilemma using the semi-classical effect at the horizon, which naturally led to the space-time noncommutative at the horizon, called as quantum horizon. In this treatment the classical horizon spreads, so the trouble due to the singularity on the horizon disappears.…”
mentioning
confidence: 99%
“…(29), we can see that the integration of Eq. (24) is rigorous, so that the considerations to quantum event horizon presented in Yans' paper [5,6,7] have indeed solved the puzzle caused by the singularity at the classical horizon in Hawking radiation calculations naturally. At the new horizon r H + (ω) the field has an infinite red-shift, an observer can't detect the at r r H + (ω), so we can calculate the entropy of the black hole in this quantum horizon model using the BWM method proposed by 't Hooft.…”
mentioning
confidence: 99%
“…However, the investigation for testing those noncommutative effects near black hole is extremely difficult due to the fact that a consistent theory of quantum gravity is not available at present, let alone a theory of noncommutative quantum gravity. Still, some efforts have been made on this subject [7][8][9]. It should be mentioned that by considering a semi-classical theory of noncommutative fields, the authors of Ref.…”
mentioning
confidence: 99%
“…It should be mentioned that by considering a semi-classical theory of noncommutative fields, the authors of Ref. [8] give some remarks on 't Hooft's brick wall model [10].…”
mentioning
confidence: 99%