Note on Type $III_1$ Algebras in $ c= 1$ String Theory and Bulk Causal Diamonds

We argue that the Leutheusser-Liu procedure of isolating a von Neumann algebra in the $N = \infty$ limit of string theories, leads to the algebra of relativistic fermion fields on a half line for the $c = 1$ string theory. This is a Type $I$ von Neumann algebra, since it is the algebra of the Rindler wedge in the Rindler vacuum state. Subalgebras of finite regions are Type $III_1$. The argument uses the elegant results of Moore and of Alexandrov, Kazakov and Kostov. This model is well known to be integrable and have no black hole excitations. We have speculated that adding an interaction invisible in perturbation theory to a large finite number, $M$, of copies of the model, produces a non-integrable model with meta-stable excitations having all of the properties of linear dilaton black holes. The algebra of fields is the tensor product of $M$ copies of the $c = 1$ model's algebra, whether or not we add the non-integrable interaction. We argue that the infinite dimensional $c = 1$ algebras are analogous to those of the boundary field theory in AdS/CFT, even though they appear to encode bulk causal structure. An IR cutoff on the boundary renders them finite and causal structure must be formulated in terms of an analog of the Tensor Network Renormalization Group. This is a time dependent Hamiltonian flow, embedding smaller Hilbert spaces into larger ones. It is the analog of one sided modular inclusion in quantum field theory.

Publication Details

Journal
ArXiv.org
Published
2025-04-21
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Note on Type $III_1$ Algebras in $ c= 1$ String Theory and Bulk Causal Diamonds

ArXiv.org
Black Holes and Theoretical Physics
article

Note on Type $III_1$ Algebras in $ c= 1$ String Theory and Bulk Causal Diamonds

article en

Abstract

We argue that the Leutheusser-Liu procedure of isolating a von Neumann algebra in the $N = \infty$ limit of string theories, leads to the algebra of relativistic fermion fields on a half line for the $c = 1$ string theory. This is a Type $I$ von Neumann algebra, since it is the algebra of the Rindler wedge in the Rindler vacuum state. Subalgebras of finite regions are Type $III_1$. The argument uses the elegant results of Moore and of Alexandrov, Kazakov and Kostov. This model is well known to be integrable and have no black hole excitations. We have speculated that adding an interaction invisible in perturbation theory to a large finite number, $M$, of copies of the model, produces a non-integrable model with meta-stable excitations having all of the properties of linear dilaton black holes. The algebra of fields is the tensor product of $M$ copies of the $c = 1$ model's algebra, whether or not we add the non-integrable interaction. We argue that the infinite dimensional $c = 1$ algebras are analogous to those of the boundary field theory in AdS/CFT, even though they appear to encode bulk causal structure. An IR cutoff on the boundary renders them finite and causal structure must be formulated in terms of an analog of the Tensor Network Renormalization Group. This is a time dependent Hamiltonian flow, embedding smaller Hilbert spaces into larger ones. It is the analog of one sided modular inclusion in quantum field theory.

ArXiv.org
Openalex Percentile: Top 75%
Black Holes and Theoretical Physics
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Note on Type $III_1$ Algebras in $ c= 1$ String Theory and Bulk Causal Diamonds · ArXiv.org (2025) | TGRS Research Map | TGRS