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PreprintCC BY 4.0arXiv

Stringy resolution of bouncing singularities

Abstract

We study the near-horizon geometry of near-extremal NS5 branes, which admits an exact worldsheet description in terms of the SL(2,ℝ)k/U(1) coset. In the supergravity limit, the analytically continued time-domain reflection amplitude exhibits a singularity associated with a null geodesic bouncing off the black-hole singularity, analogous to the bouncing singularities of boundary correlators in asymptotically AdS spacetimes. We show that finite-string-length effects render this amplitude an entire function of complex time, completely resolving the bouncing singularity. This resolution is nonperturbative in the inverse coset level: the singularity persists at every finite order in the expansion.

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BibTeX
@misc{buric2026stringy,
  title = {{Stringy resolution of bouncing singularities}},
  author = {Ilija Burić and Ivan Gusev and Andrei Parnachev},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.12311},
  eprint = {2610.12311},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.12311},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Stringy resolution of bouncing singularities
AU  - Ilija Burić
AU  - Ivan Gusev
AU  - Andrei Parnachev
PY  - 2026
DA  - 2026/10/08
PB  - arXiv
DO  - 10.48550/arxiv.2610.12311
UR  - https://arxiv.org/abs/2610.12311
AB  - We study the near-horizon geometry of near-extremal NS5 branes, which admits an exact worldsheet description in terms of the SL(2,ℝ)_k/U(1) coset. In the supergravity limit, the analytically continued time-domain reflection amplitude exhibits a singularity associated with a null geodesic bouncing off the black-hole singularity, analogous to the bouncing singularities of boundary correlators in asymptotically AdS spacetimes. We show that finite-string-length effects render this amplitude an entire function of complex time, completely resolving the bouncing singularity. This resolution is nonperturbative in the inverse coset level: the singularity persists at every finite order in the expansion.
ER  -