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Conformal Transformations in Metric-Affine Gravity and Ghosts

General Relativity and Quantum Cosmology · Submitted 28 Apr 2012

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

The authors' main claim Therefore, metric-affine gravity provides an arena in which ghosts arising from conformal factor are avoided thanks to the independence of connection from the metric.

how it is stated · asserted 1.00 read the record →

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arXiv ID1204.6366 (version 2)
Pith IDTUOQNTHR, Pith's permanent record of this paper and its review
CitationCanan N. Karahan, Durmus A. Demir, Oktay Dogangun. "Conformal Transformations in Metric-Affine Gravity and Ghosts." arXiv:1204.6366 (2012). https://pith.science/paper/TUOQNTHR
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What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.46 · human participants 0.01 · controlled comparison 0.10 · randomized assignment 0.01 · states quantitative result 0.02 · compares with prior results 0.86 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

Conformal transformations play a widespread role in gravity theories in regard to their cosmological and other implications. In the pure metric theory of gravity, conformal transformations change the frame to a new one wherein one obtains a conformal-invariant scalar-tensor theory such that the scalar field, deriving from the conformal factor, is a ghost. In this work, conformal transformations and ghosts will be analyzed in the framework of the metric-affine theory of gravity. Within this framework, metric and connection are independent variables, and hence, transform independently under conformal transformations. It will be shown that, if affine connection is invariant under conformal transformations then the scalar field under concern is a non-ghost, non-dynamical field. It is an auxiliary field at the classical level, and might develop a kinetic term at the quantum level. Alternatively, if connection transforms additively with a structure similar to yet more general than that of the Levi-Civita connection, the resulting action describes the gravitational dynamics correctly, and more importantly, the scalar field becomes a dynamical non-ghost field. The equations of motion, for generic geometrical and matter-sector variables, do not reduce connection to the Levi-Civita connection, and hence, independence of connection from metric is maintained. Therefore, metric-affine gravity provides an arena in which ghosts arising from conformal factor are avoided thanks to the independence of connection from the metric.

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 Conformal transformations play a widespread role in gravity theories in regard to their cosmological and other implications. background 1.00 0.03 0.02 asserted 1.00
s1 In the pure metric theory of gravity, conformal transformations change the frame to a new one wherein one obtains a conformal-invariant scalar-tensor theory such that the scalar field, deriving from the conformal factor, is a ghost. background 1.00 0.06 0.04 asserted 1.00
s2 In this work, conformal transformations and ghosts will be analyzed in the framework of the metric-affine theory of gravity. contribution 1.00 0.55 0.04 asserted 0.80
s3 Within this framework, metric and connection are independent variables, and hence, transform independently under conformal transformations. background 0.59 0.14 0.03 asserted 1.00
s4 It will be shown that, if affine connection is invariant under conformal transformations then the scalar field under concern is a non-ghost, non-dynamical field. result 1.00 0.77 0.25 asserted 1.00
s5 It is an auxiliary field at the classical level, and might develop a kinetic term at the quantum level. result 0.56 0.41 0.05 speculative 0.57
s6 Alternatively, if connection transforms additively with a structure similar to yet more general than that of the Levi-Civita connection, the resulting action describes the gravitational dynamics correctly, and more importantly, the scalar field becomes a dynamical non-ghost field. result 1.00 0.83 0.33 asserted 0.99
s7 The equations of motion, for generic geometrical and matter-sector variables, do not reduce connection to the Levi-Civita connection, and hence, independence of connection from metric is maintained. result 0.98 0.81 0.10 asserted 1.00
s8 Therefore, metric-affine gravity provides an arena in which ghosts arising from conformal factor are avoided thanks to the independence of connection from the metric. interpretation 0.78 0.75 0.87 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.99.

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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

Conformal transformations play a widespread role in gravity theories in regard to their cosmological and other implications. In the pure metric theory of gravity, conformal transformations change the frame to a new one wherein one obtains a conformal-invariant scalar-tensor theory such that the scalar field, deriving from the conformal factor, is a ghost. In this work, conformal transformations and ghosts will be analyzed in the framework of the metric-affine theory of gravity. Within this framework, metric and connection are independent variables, and hence, transform independently under conformal transformations. It will be shown that, if affine connection is invariant under conformal transformations then the scalar field under concern is a non-ghost, non-dynamical field. It is an auxiliary field at the classical level, and might develop a kinetic term at the quantum level. Alternatively, if connection transforms additively with a structure similar to yet more general than that of the Levi-Civita connection, the resulting action describes the gravitational dynamics correctly, and more importantly, the scalar field becomes a dynamical non-ghost field. The equations of motion, for generic geometrical and matter-sector variables, do not reduce connection to the Levi-Civita connection, and hence, independence of connection from metric is maintained. Therefore, metric-affine gravity provides an arena in which ghosts arising from conformal factor are avoided thanks to the independence of connection from the metric.

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References
How the literature uses it

7 arXiv papers cite this in 12 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 · 9 sentences without a confident label

Cites it as background 3 papers

What it cites · 25 sentences without a confident label

Cites as background 4 papers
  • The metric-affine gravity (similar to the Palatini formalism [ref] in philosophy), which considers an independence of metric tensor and connection [ref] , encodes a more general approach to gravitation by breaking up the a priori relation ([ref]).

    On white dwarfs and neutron stars in Palatini f(R) gravity · Introduction · 0.83

  • The metric-affine gravity (similar to the Palatini formalism [ref] in philosophy), which considers an independence of metric tensor and connection [ref] , encodes a more general approach to gravitation by breaking up the a priori relation ([ref]).

    Cosmological constraints on f(R) gravity theories within the Palatini approach · Introduction · 0.83

  • The metric-affine gravity (similar to the Palatini formalism [ref] in philosophy), which considers an independence of metric tensor and connection [ref] , encodes a more general approach to gravitation by breaking up the a priori relation ([ref]).

    Actions for Gravity, with Generalizations: A Review · Introduction · 0.83

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