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Wormholes without averaging
Abstract
A bstract: After averaging over fermion couplings, SYK has a collective field description that sometimes has “wormhole” solutions. We study the fate of these wormholes when the couplings are fixed. Working mainly in a simple model, we find that the wormhole saddles persist, but that new saddles also appear elsewhere in the integration space — “half-wormholes.” The wormhole contributions depend only weakly on the specific choice of couplings, while the half-wormhole contributions are strongly sensitive. The half-wormholes are crucial for factorization of decoupled systems with fixed couplings, but they vanish after averaging, leaving the non-factorizing wormhole behind.
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“However, from the gravity side, evaluating such a wavefunction O I with the gravitational path integral by filling in the bulk will require some microscopic ingredient beyond the semiclassical description of the thin shell and it is not obvious that such a level of microscopic detail should be accessible semiclassically [70].”
From The baby universe is fine and the CFT knows it: on holography for closed universes (2025) · cites this paper as [70]
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Cites
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“• How can we confirm the picture presented in section 3 for full SYK? Are there circumstances where we should expect these arguments to fail? • Do these ideas apply to tensor models,(22) which can be viewed as particular, highly structured members of an SYK ensemble? Is the sparse SYK model [46] a useful stepping-ston…”
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Cited by
Sorted by citations
Carlip, S. (2023) · Reports on Progress in Physics · doi:10.1088/1361-6633/acceb4 · Cited by 41
The baby universe is fine and the CFT knows it: on holography for closed universes
Antonini, S., Rath, P., Sasieta, M., Swingle, B., & Vilar López, A. (2025) · Journal of High Energy Physics · doi:10.1007/jhep12(2025)159 · Cited by 35
Metadata
- Authors
- Saad, P., Shenker, S. H., Stanford, D., & Yao, S.
- Venue
- Journal of High Energy Physics
- Published
- 2024-09-19
- Volume
- 2024
- Issue
- 9
- ISSN
- 1029-8479
- Cited by
- 31
- References
- 9
- Language
- en
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