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Nonderivative Modified Gravity: a Classification

We analyze the theories of gravity modified by a generic nonderivative potential built from the metric, under the minimal requirement of unbroken spatial rotations. Using the canonical analysis, we classify the potentials $V$ according to the number of degrees of freedom (DoF) that propagate at the...

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Autores principales: Comelli, Denis, Nesti, Fabrizio, Pilo, Luigi
Lenguaje:eng
Publicado: 2014
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2014/11/018
http://cds.cern.ch/record/1744322
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author Comelli, Denis
Nesti, Fabrizio
Pilo, Luigi
author_facet Comelli, Denis
Nesti, Fabrizio
Pilo, Luigi
author_sort Comelli, Denis
collection CERN
description We analyze the theories of gravity modified by a generic nonderivative potential built from the metric, under the minimal requirement of unbroken spatial rotations. Using the canonical analysis, we classify the potentials $V$ according to the number of degrees of freedom (DoF) that propagate at the nonperturbative level. We then compare the nonperturbative results with the perturbative DoF propagating around Minkowski and FRW backgrounds. A generic $V$ implies 6 propagating DoF at the non-perturbative level, with a ghost on Minkowski background. There exist potentials which propagate 5 DoF, as already studied in previous works. Here, no $V$ with unbroken rotational invariance admitting 4 DoF is found. Theories with 3 DoF turn out to be strongly coupled on Minkowski background. Finally, potentials with only the 2 DoF of a massive graviton exist. Their effect on cosmology is simply equivalent to a cosmological constant. Potentials with 2 or 5 DoF and explicit time dependence appear to be a further viable possibility.
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publishDate 2014
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spelling cern-17443222023-10-04T06:50:00Zdoi:10.1088/1475-7516/2014/11/018http://cds.cern.ch/record/1744322engComelli, DenisNesti, FabrizioPilo, LuigiNonderivative Modified Gravity: a ClassificationParticle Physics - TheoryWe analyze the theories of gravity modified by a generic nonderivative potential built from the metric, under the minimal requirement of unbroken spatial rotations. Using the canonical analysis, we classify the potentials $V$ according to the number of degrees of freedom (DoF) that propagate at the nonperturbative level. We then compare the nonperturbative results with the perturbative DoF propagating around Minkowski and FRW backgrounds. A generic $V$ implies 6 propagating DoF at the non-perturbative level, with a ghost on Minkowski background. There exist potentials which propagate 5 DoF, as already studied in previous works. Here, no $V$ with unbroken rotational invariance admitting 4 DoF is found. Theories with 3 DoF turn out to be strongly coupled on Minkowski background. Finally, potentials with only the 2 DoF of a massive graviton exist. Their effect on cosmology is simply equivalent to a cosmological constant. Potentials with 2 or 5 DoF and explicit time dependence appear to be a further viable possibility.We analyze the theories of gravity modified by a generic nonderivative potential built from the metric, under the minimal requirement of unbroken spatial rotations. Using the canonical analysis, we classify the potentials V according to the number of degrees of freedom (DoF) that propagate at the nonperturbative level. We then compare the nonperturbative results with the perturbative DoF propagating around Minkowski and FRW backgrounds. A generic V implies 6 propagating DoF at the non-perturbative level, with a ghost on Minkowski background. There exist potentials which propagate 5 DoF, as already studied in previous works. Here, no V with unbroken rotational invariance admitting 4 DoF is found. Theories with 3 DoF turn out to be strongly coupled on Minkowski background. Finally, potentials with only the 2 DoF of a massive graviton exist. Their effect on cosmology is simply equivalent to a cosmological constant. Potentials with 2 or 5 DoF and explicit time dependence appear to be a further viable possibility.We analyze the theories of gravity modified by a generic nonderivative potential built from the metric, under the minimal requirement of unbroken spatial rotations. Using the canonical analysis, we classify the potentials $V$ according to the number of degrees of freedom (DoF) that propagate at the nonperturbative level. We then compare the nonperturbative results with the perturbative DoF propagating around Minkowski and FRW backgrounds. A generic $V$ implies 6 propagating DoF at the non-perturbative level, with a ghost on Minkowski background. There exist potentials which propagate 5 DoF, as already studied in previous works. Here, no $V$ with unbroken rotational invariance admitting 4 DoF is found. Theories with 3 DoF turn out to be strongly coupled on Minkowski background. Finally, potentials with only the 2 DoF of a massive graviton exist. Their effect on cosmology is simply equivalent to a cosmological constant. Potentials with 2 or 5 DoF and explicit time dependence appear to be a further viable possibility.arXiv:1407.4991CERN-PH-TH-2014-132CERN-PH-TH-2014-132oai:cds.cern.ch:17443222014-07-18
spellingShingle Particle Physics - Theory
Comelli, Denis
Nesti, Fabrizio
Pilo, Luigi
Nonderivative Modified Gravity: a Classification
title Nonderivative Modified Gravity: a Classification
title_full Nonderivative Modified Gravity: a Classification
title_fullStr Nonderivative Modified Gravity: a Classification
title_full_unstemmed Nonderivative Modified Gravity: a Classification
title_short Nonderivative Modified Gravity: a Classification
title_sort nonderivative modified gravity: a classification
topic Particle Physics - Theory
url https://dx.doi.org/10.1088/1475-7516/2014/11/018
http://cds.cern.ch/record/1744322
work_keys_str_mv AT comellidenis nonderivativemodifiedgravityaclassification
AT nestifabrizio nonderivativemodifiedgravityaclassification
AT piloluigi nonderivativemodifiedgravityaclassification