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Quantum Observables and Recollapsing Dynamics

General Relativity and Quantum Cosmology · Submitted 27 Apr 1994

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim Furthermore, many of these observables have a clear interpretation in the classical limit and we use this to demonstrate that, for a class of minisuperspace models including LRS Bianchi IX and the Kantowski-Sachs model this quantization agrees with classical physics in predicting that such spacetimes recollapse.

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arXiv IDgr-qc/9404053 (version 5)
Pith IDESR3CHUS, Pith's permanent record of this paper and its review
CitationDonald Marolf. "Quantum Observables and Recollapsing Dynamics." arXiv:gr-qc/9404053 (1994). https://pith.science/paper/ESR3CHUS
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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,068 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.28 · human participants 0.01 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.04 · compares with prior results 0.46 · mentions code or data availability 0.02.

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arXiv listing abstract v5. Results and the main claim are underlined; .

Within a simple quantization scheme, observables for a large class of finite dimensional time reparametrization invariant systems may be constructed by integration over the manifold of time labels. This procedure is shown to produce a complete set of densely defined operators on a physical Hilbert space for which an inner product is identified and to provide reasonable results for simple test cases. Furthermore, many of these observables have a clear interpretation in the classical limit and we use this to demonstrate that, for a class of minisuperspace models including LRS Bianchi IX and the Kantowski-Sachs model this quantization agrees with classical physics in predicting that such spacetimes recollapse.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 Within a simple quantization scheme, observables for a large class of finite dimensional time reparametrization invariant systems may be constructed by integration over the manifold of time labels. contribution 0.48 0.70 0.15 hedged possibility 1.00
s1 This procedure is shown to produce a complete set of densely defined operators on a physical Hilbert space for which an inner product is identified and to provide reasonable results for simple test cases. result 0.91 0.93 0.12 asserted 1.00
s2 Furthermore, many of these observables have a clear interpretation in the classical limit and we use this to demonstrate that, for a class of minisuperspace models including LRS Bianchi IX and the Kantowski-Sachs model this quantization agrees with classical physics in predicting that such spacetimes recollapse. result 0.88 0.91 0.68 asserted 1.00

What kind of paper the classifier reports this is: method or tool 0.57 · evidence from proof or derivation 1.00.

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Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

Within a simple quantization scheme, observables for a large class of finite dimensional time reparametrization invariant systems may be constructed by integration over the manifold of time labels. This procedure is shown to produce a complete set of densely defined operators on a physical Hilbert space for which an inner product is identified and to provide reasonable results for simple test cases. Furthermore, many of these observables have a clear interpretation in the classical limit and we use this to demonstrate that, for a class of minisuperspace models including LRS Bianchi IX and the Kantowski-Sachs model this quantization agrees with classical physics in predicting that such spacetimes recollapse.

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References
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20 arXiv papers cite this in 42 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 27 sentences without a confident label

Uses its method or tool 2 papers
  • Fortunately, however, one may use the standard Fock space (which we call the `auxiliary' Hilbert space $$) to build a new `physical' Hilbert space $$ of de Sitter-invariant states via group averaging [ref] [See [ref] for independent introductions of similar techniques in related contexts.].

    Group Averaging of massless scalar fields in 1+1 de Sitter · Introduction · 0.85

  • In order to do that, we can follow two alternative strategies: =0pt * We can apply the group averaging procedure [ref] .

    Introduction to Loop Quantum Cosmology · Physical Hilbert space · 0.92

Cites it as background 11 papers

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