SciPost Submission Page
Horizon Strings as 3d Black Hole Microstates
by Arjun Bagchi, Daniel Grumiller, and Mohammad Mehdi Sheikh-Jabbari
This is not the latest submitted version.
Submission summary
| Authors (as registered SciPost users): | Arjun Bagchi · Daniel Grumiller |
| Submission information | |
|---|---|
| Preprint Link: | scipost_202308_00041v1 (pdf) |
| Date submitted: | Aug. 28, 2023, 8:03 a.m. |
| Submitted by: | Daniel Grumiller |
| Submitted to: | SciPost Physics Core |
| Ontological classification | |
|---|---|
| Academic field: | Physics |
| Specialties: |
|
| Approach: | Theoretical |
Abstract
We propose that 3d black holes are an ensemble of tensionless null string states. These microstates typically have non-zero winding. We evaluate their partition function in the limit of large excitation numbers and show that their combinatorics reproduces the Bekenstein-Hawking entropy and its semiclassical logarithmic corrections.
Current status:
Reports on this Submission
Report #2 by Anonymous (Referee 2) on 2023-10-5 (Invited Report)
- Cite as: Anonymous, Report on arXiv:scipost_202308_00041v1, delivered 2023-10-05, doi: 10.21468/SciPost.Report.7901
Strengths
The manuscript describes 3d Black Hole microstates as arising from quantum states of tensionless strings. The authors consider wound tensionless strings encompassing the black hole horizon and from the degeneracy of the string spectrum calculate the entropy of the black hole and relevant log corrections.
-
The paper is very clearly written with appropriate introduction to the tensionless strings and quantization thereof. The calculation of microstates has also been presented in a lucid way.
-
Both near horizon physics and tensionless worldsheet physics have the inherent structure of BMS symmetries, albeit one is a global symmetry and the other a gauge one. The proposal to put them together is bold and intriguing, however mathematically very well-constructed.
Weaknesses
- The authors discuss a 3d BTZ Black Hole for their purpose, which could have a non-trivial B field. I do not find a reference to this. As far as I understand the corresponding techniques in Null string theory are also not well developed, so probably this is justified.
Report
Report #1 by Anonymous (Referee 1) on 2023-10-2 (Invited Report)
- Cite as: Anonymous, Report on arXiv:scipost_202308_00041v1, delivered 2023-10-02, doi: 10.21468/SciPost.Report.7882
Strengths
- provide a novel understanding of black hole entropy
Weaknesses
- The physical picture of horizon string is not completely clear
Report
However, I am not convincing about the coupling constant $\kappa$ introduced first in (2). It is different from the usual string tension, and is fixed to be $3/16G^2$ by matching with the blackhole entropy. The numerical factor was argued to be a nontrivial input, and $1/G^2$ comes from the dimensional analysis. I am confused by the discussion here. In the usual string theory, the string tension is an intrinsic parameter of the theory. Now if we generalize naively the discussion to other dimensions, say 4D Schwartzschild black hole, the dimension of 4D Newton constant is different, and we would expect the coupling constant takes a different form. Is the horizon string picture universal? or we have to adjust the coupling constant case by case? It would be nice for the authors to give more clarification on this point.
Requested changes
The authors missed some references. For example, there's one paper ePrint: 2211.06926 on BMS free fermion, which appeared at the same time with Ref. [82] (ePrint: 2211.06927). Besides, the critical dimensions of tensionless (super)string has been studied from path-integral point of view in e-Print: 2302.05975.
Author: Daniel Grumiller on 2023-10-07 [id 4028]
(in reply to Report 2 on 2023-10-05)We thank the referee for their comments.
The point about the addition of the B-field is an interesting one. An upcoming paper by one of the authors (with coworkers) will explore null strings with a B-field background. However, as far as our proposal and 3d black hole microstates are concerned, we do not think that the B-field background is relevant.