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Coherent State Transforms for Spaces of Connections

General Relativity and Quantum Cosmology · Submitted 5 Dec 1994

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

The authors' main claim The resulting ``coherent state transform'' provides a holomorphic representation of the holonomy $C^\star$ algebra of real gauge fields.

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arXiv IDgr-qc/9412014 (version 1)
Pith IDMCORADJ7, Pith's permanent record of this paper and its review
CitationAbhay Ashtekar, Donald Marolf, Jerzy lewandowski, Jos\'e Mour\~ao, Thomas Thiemann. "Coherent State Transforms for Spaces of Connections." arXiv:gr-qc/9412014 (1994). https://pith.science/paper/MCORADJ7
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What the abstract itself states, as probabilities: claims first 0.09 · states limitation 0.16 · human participants 0.01 · controlled comparison 0.01 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.82 · mentions code or data availability 0.01.

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arXiv listing abstract v1. Results and the main claim are underlined; .

The Segal-Bargmann transform plays an important role in quantum theories of linear fields. Recently, Hall obtained a non-linear analog of this transform for quantum mechanics on Lie groups. Given a compact, connected Lie group $G$ with its normalized Haar measure $\mu_H$, the Hall transform is an isometric isomorphism from $L^2(G, \mu_H)$ to ${\cal H}(G^{\Co})\cap L^2(G^{\Co}, \nu)$, where $G^{\Co}$ the complexification of $G$, ${\cal H}(G^{\Co})$ the space of holomorphic functions on $G^{\Co}$, and $\nu$ an appropriate heat-kernel measure on $G^{\Co}$. We extend the Hall transform to the infinite dimensional context of non-Abelian gauge theories by replacing the Lie group $G$ by (a certain extension of) the space ${\cal A}/{\cal G}$ of connections modulo gauge transformations. The resulting ``coherent state transform'' provides a holomorphic representation of the holonomy $C^\star$ algebra of real gauge fields. This representation is expected to play a key role in a non-perturbative, canonical approach to quantum gravity in 4-dimensions.

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What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 The Segal-Bargmann transform plays an important role in quantum theories of linear fields. background 1.00 0.04 0.02 asserted 1.00
s1 Recently, Hall obtained a non-linear analog of this transform for quantum mechanics on Lie groups. background 1.00 0.03 0.03 asserted 1.00
s2 Given a compact, connected Lie group $G$ with its normalized Haar measure $\mu_H$, the Hall transform is an isometric isomorphism from $L^2(G, \mu_H)$ to ${\cal H}(G^{\Co})\cap L^2(G^{\Co}, \nu)$, where $G^{\Co}$ the complexification of $G$, ${\cal H}(G^{\Co})$ the space of holomorphic functions on $G^{\Co}$, and $\nu$ an appropriate heat-kernel measure on $G^{\Co}$. background 1.00 0.07 0.06 asserted 1.00
s3 We extend the Hall transform to the infinite dimensional context of non-Abelian gauge theories by replacing the Lie group $G$ by (a certain extension of) the space ${\cal A}/{\cal G}$ of connections modulo gauge transformations. contribution 0.71 0.92 0.26 asserted 1.00
s4 The resulting ``coherent state transform'' provides a holomorphic representation of the holonomy $C^\star$ algebra of real gauge fields. result 0.88 0.89 0.55 asserted 1.00
s5 This representation is expected to play a key role in a non-perturbative, canonical approach to quantum gravity in 4-dimensions. interpretation 0.96 0.10 0.28 hedged possibility 0.90

What kind of paper the classifier reports this is: theoretical result 0.57 · evidence from proof or derivation 0.96.

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The paper
Original abstract

The Segal-Bargmann transform plays an important role in quantum theories of linear fields. Recently, Hall obtained a non-linear analog of this transform for quantum mechanics on Lie groups. Given a compact, connected Lie group $G$ with its normalized Haar measure $\mu_H$, the Hall transform is an isometric isomorphism from $L^2(G, \mu_H)$ to ${\cal H}(G^{\Co})\cap L^2(G^{\Co}, \nu)$, where $G^{\Co}$ the complexification of $G$, ${\cal H}(G^{\Co})$ the space of holomorphic functions on $G^{\Co}$, and $\nu$ an appropriate heat-kernel measure on $G^{\Co}$. We extend the Hall transform to the infinite dimensional context of non-Abelian gauge theories by replacing the Lie group $G$ by (a certain extension of) the space ${\cal A}/{\cal G}$ of connections modulo gauge transformations. The resulting ``coherent state transform'' provides a holomorphic representation of the holonomy $C^\star$ algebra of real gauge fields. This representation is expected to play a key role in a non-perturbative, canonical approach to quantum gravity in 4-dimensions.

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How the literature uses it

15 arXiv papers cite this in 26 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 · 16 sentences without a confident label

Uses its method or tool 2 papers
  • Applying the heat-kernel technique to several copies of $SU(2)$ allows to build coherent spin-network states for LQG [ref] .

    Coherent states for FLRW space-times in loop quantum gravity · Coherent spin-networks · 0.87

  • Using this map, the vertex amplitude in the holonomy representation can be written as [equation] The integrals on $Spin(4)$ impose the Euclidean invariance of the vertex, and the integrand is given by a product of `face' terms $P$ given by the following distribution over $L^2(SU(2))⊗L^2(Spin(4))≃L^2(SU(2)^3)$: [equation] Expression ([ref]) can be easily put in the holomorphic representation using the Segal-Bargamann transform [ref] : [equation] where [equation] Notice that the last expression can be seen as a distribution on $ℋL^2(SL(2,ℂ))⊗L^2(Spin(4))$.

    Spinfoams in the holomorphic representation · III. 4d Euclidean vertex amplitude in the holomorphic representation · 0.83

Cites it as background 8 papers

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