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Holographic Spacetime vs Banks-Fischler Holographic Space-Time
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Holographic Spacetime Frontier | Banks-Fischler Holographic Space-Time Frontier | |
|---|---|---|
| Proposed | 1997 / 2010 | 2001 / 2020 |
| Key figures | Juan Maldacena, Mark Van Raamsdonk, Shinsei Ryu, Tadashi Takayanagi, Leonard Susskind | Tom Banks, Willy Fischler |
| In one sentence | Spacetime geometry emerges from quantum entanglement in a lower-dimensional theory without gravity, as established by AdS/CFT in anti-de Sitter space. Whether this generalizes to our de Sitter universe is an open question. | Tom Banks and Willy Fischler are developing a de Sitter holography framework in which spacetime has a finite-dimensional Hilbert space tied to the area of the cosmological horizon. The program began with the 2001 'M-theory observables for cosmological space-times' paper and continues actively through 2020 (Banks-Fischler 'Holographic space-time, Newton's law, and the dynamics of horizons'). Holographic Space-Time (HST) is an alternative to AdS/CFT for our positive-cosmological constant universe: instead of an infinite-dimensional CFT on a conformal boundary, the framework posits a finite-dimensional Hilbert space whose size grows with the area of the cosmological event horizon. |
| Predictions |
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| Where it breaks |
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| Key unresolved problem | The wrong-universe problem: the entanglement-builds-geometry story works exactly only in anti-de Sitter space, a negatively curved, non-expanding kind of cosmos, and after 25 years no one has shown it carries over to our actually expanding de Sitter universe. | The no-fingerprint problem: the theory's central claim, that our universe holds only a finite number of quantum states set by the horizon, makes almost no unique observable prediction to tell it apart from rival de Sitter holography ideas or from standard cosmology. |
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Holographic Spacetime
1997 / 2010 · Frontier
Banks-Fischler Holographic Space-Time
2001 / 2020 · Frontier
Proposed
1997 / 2010
2001 / 2020
Key figures
Juan Maldacena, Mark Van Raamsdonk, Shinsei Ryu, Tadashi Takayanagi, Leonard Susskind
Tom Banks, Willy Fischler
In one sentence
Spacetime geometry emerges from quantum entanglement in a lower-dimensional theory without gravity, as established by AdS/CFT in anti-de Sitter space. Whether this generalizes to our de Sitter universe is an open question.
Tom Banks and Willy Fischler are developing a de Sitter holography framework in which spacetime has a finite-dimensional Hilbert space tied to the area of the cosmological horizon. The program began with the 2001 'M-theory observables for cosmological space-times' paper and continues actively through 2020 (Banks-Fischler 'Holographic space-time, Newton's law, and the dynamics of horizons'). Holographic Space-Time (HST) is an alternative to AdS/CFT for our positive-cosmological constant universe: instead of an infinite-dimensional CFT on a conformal boundary, the framework posits a finite-dimensional Hilbert space whose size grows with the area of the cosmological event horizon.
Predictions
- AdS/CFT predicts precise relationships between strongly coupled QFT correlators (e.g., quark-gluon plasma viscosity, condensed matter analogs) and gravitational dynamics in AdS bulk
- If holographic emergence generalizes to cosmological de Sitter spacetime, specific structural imprints should appear in cosmological correlators beyond standard [[inflation]] predictions
- Quantum error correction codes that reconstruct bulk from boundary make precise claims about which boundary degrees of freedom encode which bulk regions, testable in lattice realizations
- Spacetime has a finite-dimensional Hilbert space whose dimension grows with the area of the cosmological horizon, in Planck units
- The cosmological horizon is the carrier of physical degrees of freedom; observers in different causal diamonds have access to different finite-dimensional Hilbert spaces with consistent overlap structure
- Newton's law of gravity emerges from the holographic structure at large distances; the 2020 Banks-Fischler paper makes this connection technically explicit
- The framework predicts that black-hole and cosmological horizons evolve differently than standard approaches expect, because their physics is set by a finite count of horizon states rather than an infinite boundary theory; the concrete observable signatures that would distinguish it from AdS/CFT have not yet been worked out
Where it breaks
- AdS/CFT is exact only in anti-de Sitter spacetime; our universe is de Sitter, and de Sitter holography is unsolved despite multiple programs (dS/CFT, swampland, FRW holography)
- The 'holographic emergence' claim is tightly tied to special backgrounds; whether it tells us anything about real cosmology is contested
- ER=EPR is largely conceptual: it rephrases known relationships between entanglement and geometry rather than producing distinctive empirical predictions
- Holography provides many dualities but no unique emergent description of our specific universe
- The framework is a minority position in the broader holography landscape; the AdS/CFT correspondence dominates the empirical and conceptual conversation
- The de Sitter holography problem remains unsolved despite Banks-Fischler's work and parallel efforts (Anninos-Hartman-Strominger, others); no consensus de Sitter holography has emerged
- The framework's predictive content beyond consistency with known physics is limited; few unique observational signatures distinguish it from alternative de Sitter holographic programs
- Some of the central technical claims (finite-dimensional Hilbert space, specific causal-diamond structure) are framework-defining choices rather than derived properties; the choice itself shapes what can be calculated
Key unresolved problem
The wrong-universe problem: the entanglement-builds-geometry story works exactly only in anti-de Sitter space, a negatively curved, non-expanding kind of cosmos, and after 25 years no one has shown it carries over to our actually expanding de Sitter universe.
The no-fingerprint problem: the theory's central claim, that our universe holds only a finite number of quantum states set by the horizon, makes almost no unique observable prediction to tell it apart from rival de Sitter holography ideas or from standard cosmology.
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100% · 1 vote
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