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Metastable supersymmetry breaking in N=2 non-linear sigma-models

High Energy Physics - Theory · Submitted 14 May 2010

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

The authors' main claim This problem turns out to capture all the important qualitative features of the corresponding question in theories with local supersymmetry, where gravitational effects induce only quantitative modifications.

how it is stated · asserted 0.99 read the record →

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arXiv ID1005.2523 (version 2)
Pith IDPGK54LDT, Pith's permanent record of this paper and its review
CitationClaudio A. Scrucca, Jean-Claude Jacot. "Metastable supersymmetry breaking in N=2 non-linear sigma-models." arXiv:1005.2523 (2010). https://pith.science/paper/PGK54LDT
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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 7,756 input tokens, $0.0003 reported.

What the abstract itself states, as probabilities: claims first 0.07 · states limitation 0.26 · human participants 0.01 · controlled comparison 0.10 · randomized assignment 0.01 · states quantitative result 0.06 · compares with prior results 0.79 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

We perform a general study of the issue of metastability for supersymmetry-breaking vacua in theories with N=1 and N=2 global supersymmetry. This problem turns out to capture all the important qualitative features of the corresponding question in theories with local supersymmetry, where gravitational effects induce only quantitative modifications. Moreover, it allows to directly compare the conditions arising in the N=1 and N=2 cases, since the latter becomes particular case of the former in the rigid limit. Our strategy consists in a systematic investigation of the danger of instability coming from the sGoldstini scalars, whose masses are entirely due to supersymmetry breaking mass-splitting effects. We start by reviewing the metastability conditions arising in general N=1 non-linear sigma-models with chiral and vector multiplets. We then turn to the case of general N=2 non-linear sigma-models with hyper and vector multiplets. We first reproduce and clarify the known no-go theorems applying to theories with only Abelian vector multiplets and only hyper multiplets, and then derive new results applying to more general cases. To make the comparison with N=1 models as clear as possible, we rely on a formulation of N=2 models where one of the supersymmetries is manifestly realized in terms of ordinary superfields, whereas the other is realized through non-trivial transformations. We give a self-contained account of such a construction of N=2 theories in N=1 superspace, generalizing previous work on various aspects to reach a general and coordinate-covariant construction. We also present a direct computation of the supertrace of the mass matrix.

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 We perform a general study of the issue of metastability for supersymmetry-breaking vacua in theories with N=1 and N=2 global supersymmetry. contribution 0.98 0.94 0.06 asserted 0.89
s1 This problem turns out to capture all the important qualitative features of the corresponding question in theories with local supersymmetry, where gravitational effects induce only quantitative modifications. interpretation 0.64 0.66 0.14 asserted 0.99
s2 Moreover, it allows to directly compare the conditions arising in the N=1 and N=2 cases, since the latter becomes particular case of the former in the rigid limit. background 0.29 0.24 0.07 asserted 0.95
s3 Our strategy consists in a systematic investigation of the danger of instability coming from the sGoldstini scalars, whose masses are entirely due to supersymmetry breaking mass-splitting effects. method 0.95 0.68 0.07 asserted 0.97
s4 We start by reviewing the metastability conditions arising in general N=1 non-linear sigma-models with chiral and vector multiplets. method 0.80 0.47 0.03 asserted 0.87
s5 We then turn to the case of general N=2 non-linear sigma-models with hyper and vector multiplets. method 0.57 0.65 0.03 asserted 0.68
s6 We first reproduce and clarify the known no-go theorems applying to theories with only Abelian vector multiplets and only hyper multiplets, and then derive new results applying to more general cases. contribution 0.81 0.86 0.13 asserted 1.00
s7 To make the comparison with N=1 models as clear as possible, we rely on a formulation of N=2 models where one of the supersymmetries is manifestly realized in terms of ordinary superfields, whereas the other is realized through non-trivial transformations. method 1.00 0.63 0.03 asserted 0.97
s8 We give a self-contained account of such a construction of N=2 theories in N=1 superspace, generalizing previous work on various aspects to reach a general and coordinate-covariant construction. contribution 0.57 0.91 0.03 asserted 1.00
s9 We also present a direct computation of the supertrace of the mass matrix. contribution 0.55 0.93 0.04 asserted 0.99

What kind of paper the classifier reports this is: theoretical result 1.00 · 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

We perform a general study of the issue of metastability for supersymmetry-breaking vacua in theories with N=1 and N=2 global supersymmetry. This problem turns out to capture all the important qualitative features of the corresponding question in theories with local supersymmetry, where gravitational effects induce only quantitative modifications. Moreover, it allows to directly compare the conditions arising in the N=1 and N=2 cases, since the latter becomes particular case of the former in the rigid limit. Our strategy consists in a systematic investigation of the danger of instability coming from the sGoldstini scalars, whose masses are entirely due to supersymmetry breaking mass-splitting effects. We start by reviewing the metastability conditions arising in general N=1 non-linear sigma-models with chiral and vector multiplets. We then turn to the case of general N=2 non-linear sigma-models with hyper and vector multiplets. We first reproduce and clarify the known no-go theorems applying to theories with only Abelian vector multiplets and only hyper multiplets, and then derive new results applying to more general cases. To make the comparison with N=1 models as clear as possible, we rely on a formulation of N=2 models where one of the supersymmetries is manifestly realized in terms of ordinary superfields, whereas the other is realized through non-trivial transformations. We give a self-contained account of such a construction of N=2 theories in N=1 superspace, generalizing previous work on various aspects to reach a general and coordinate-covariant construction. We also present a direct computation of the supertrace of the mass matrix.

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9 arXiv papers cite this in 15 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 · 11 sentences without a confident label

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What it cites · 43 sentences without a confident label

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Uses the method or tool of 4 papers
  • To work out these restrictions, we follow again the logic of [ref] , with some additional ingredients taken from [ref] (see also [ref] ) to obtain the most general allowed superpotential, and also some generalization to make the formulation covariant under general field reparametrizations.

    Nonlinear N=2 Supersymmetry, Effective Actions and Moduli Stabilization · N=2 models with vector multiplets · 0.83

  • To work out these restrictions, we follow again the logic of [ref] , with some additional ingredients taken from [ref] (see also [ref] ) to obtain the most general allowed superpotential, and also some generalization to make the formulation covariant under general field reparametrizations.

    Nonlinear Supersymmetry, Brane-bulk Interactions and Super-Higgs without Gravity · N=2 models with vector multiplets · 0.83

  • Notice finally that it is possible to reshuffle the scalar potential ([ref]) by proceeding in the following way, with manipulations that are similar to those used in [ref] to discuss truncations of $N=2$ to $N=1$ supergravity theories.

    Supersymmetry reduction of N-extended supergravities in four dimensions · N=2 models with hyper and vector multiplets · 0.93

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