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A note on the nonuniqueness of the massive Fierz-Pauli theory and spectator fields

High Energy Physics - Theory · Submitted 3 Jul 2013

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

The authors' main claim We argue that massive gravity models based on the Fierz-Pauli theory are not expected to be equivalent to possible local self-interacting theories built up on the top of the two new families of massive spin-2 models.

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arXiv ID1307.1109 (version 1)
Pith IDXQIZEFCA, Pith's permanent record of this paper and its review
CitationD. Dalmazi. "A note on the nonuniqueness of the massive Fierz-Pauli theory and spectator fields." arXiv:1307.1109 (2013). https://pith.science/paper/XQIZEFCA
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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 6,284 input tokens, $0.0003 reported.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.65 · human participants 0.01 · controlled comparison 0.05 · randomized assignment 0.01 · states quantitative result 0.74 · compares with prior results 0.73 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

It is possible to show that there are three independent families of models describing a massive spin-2 particle via a rank-2 tensor. One of them contains the massive Fierz-Pauli model, the only case described by a symmetric tensor. The three families have different local symmetries in the massless limit and can not be interconnected by any local field redefinition. We show here however, that they can be related with the help of a decoupled and non dynamic (spectator) field. The spectator field may be either an antisymmetric tensor $B_{\mu\nu}=-B_{\nu\mu}$, a vector $A_{\mu}$ or a scalar field $\varphi$, corresponding to each of the three families. The addition of the extra field allows us to formulate master actions which interpolate between the symmetric Fierz-Pauli theory and the other models. We argue that massive gravity models based on the Fierz-Pauli theory are not expected to be equivalent to possible local self-interacting theories built up on the top of the two new families of massive spin-2 models. The approach used here may be useful to investigate dual (nonsymmetric) formulations of higher spin particles.

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 It is possible to show that there are three independent families of models describing a massive spin-2 particle via a rank-2 tensor. result 0.52 0.35 0.12 hedged possibility 0.84
s1 One of them contains the massive Fierz-Pauli model, the only case described by a symmetric tensor. background 0.60 0.24 0.07 asserted 1.00
s2 The three families have different local symmetries in the massless limit and can not be interconnected by any local field redefinition. background 0.77 0.21 0.09 asserted 1.00
s3 We show here however, that they can be related with the help of a decoupled and non dynamic (spectator) field. contribution 0.57 0.92 0.50 asserted 1.00
s4 The spectator field may be either an antisymmetric tensor $B_{\mu\nu}=-B_{\nu\mu}$, a vector $A_{\mu}$ or a scalar field $\varphi$, corresponding to each of the three families. result 0.52 0.73 0.09 asserted 0.53
s5 The addition of the extra field allows us to formulate master actions which interpolate between the symmetric Fierz-Pauli theory and the other models. contribution 0.43 0.89 0.16 asserted 0.86
s6 We argue that massive gravity models based on the Fierz-Pauli theory are not expected to be equivalent to possible local self-interacting theories built up on the top of the two new families of massive spin-2 models. interpretation 0.96 0.49 0.64 hedged possibility 0.93
s7 The approach used here may be useful to investigate dual (nonsymmetric) formulations of higher spin particles. future work 0.98 0.21 0.05 hedged possibility 1.00

What kind of paper the classifier reports this is: theoretical result 0.99 · evidence from proof or derivation 0.98.

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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

It is possible to show that there are three independent families of models describing a massive spin-2 particle via a rank-2 tensor. One of them contains the massive Fierz-Pauli model, the only case described by a symmetric tensor. The three families have different local symmetries in the massless limit and can not be interconnected by any local field redefinition. We show here however, that they can be related with the help of a decoupled and non dynamic (spectator) field. The spectator field may be either an antisymmetric tensor $B_{\mu\nu}=-B_{\nu\mu}$, a vector $A_{\mu}$ or a scalar field $\varphi$, corresponding to each of the three families. The addition of the extra field allows us to formulate master actions which interpolate between the symmetric Fierz-Pauli theory and the other models. We argue that massive gravity models based on the Fierz-Pauli theory are not expected to be equivalent to possible local self-interacting theories built up on the top of the two new families of massive spin-2 models. The approach used here may be useful to investigate dual (nonsymmetric) formulations of higher spin particles.

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