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From $R^2$ Gravity to No-Scale Supergravity

We show that R2 gravity coupled conformally to scalar fields is equivalent to the real bosonic sector of SU(N,1)/SU(N)×U(1) no-scale supergravity, where the conformal factor can be identified with the Kähler potential, and we review the construction of Starobinsky-like models of inflation within thi...

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Detalles Bibliográficos
Autores principales: Ellis, John, Nanopoulos, Dimitri V., Olive, Keith A.
Lenguaje:eng
Publicado: 2017
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.97.043530
http://cds.cern.ch/record/2294838
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author Ellis, John
Nanopoulos, Dimitri V.
Olive, Keith A.
author_facet Ellis, John
Nanopoulos, Dimitri V.
Olive, Keith A.
author_sort Ellis, John
collection CERN
description We show that R2 gravity coupled conformally to scalar fields is equivalent to the real bosonic sector of SU(N,1)/SU(N)×U(1) no-scale supergravity, where the conformal factor can be identified with the Kähler potential, and we review the construction of Starobinsky-like models of inflation within this framework.
id cern-2294838
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2017
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spelling cern-22948382023-10-04T06:48:13Zdoi:10.1103/PhysRevD.97.043530http://cds.cern.ch/record/2294838engEllis, JohnNanopoulos, Dimitri V.Olive, Keith A.From $R^2$ Gravity to No-Scale Supergravityhep-phParticle Physics - Phenomenologygr-qcGeneral Relativity and Cosmologyastro-ph.COAstrophysics and Astronomyhep-thParticle Physics - TheoryWe show that R2 gravity coupled conformally to scalar fields is equivalent to the real bosonic sector of SU(N,1)/SU(N)×U(1) no-scale supergravity, where the conformal factor can be identified with the Kähler potential, and we review the construction of Starobinsky-like models of inflation within this framework.We show that $R^2$ gravity coupled conformally to scalar fields is equivalent to the real bosonic sector of SU(N,1)/SU(N)$\times$U(1) no-scale supergravity, where the conformal factor can be identified with the K\"ahler potential, and we review the construction of Starobinsky-like models of inflation within this framework.arXiv:1711.11051KCL-PH-TH-2017-60CERN-PH-TH-2017-248CERN-TH-2017-248ACT-06-17MI-TH-1771UMN-TH-3706-17FTPI-MINN-17-22oai:cds.cern.ch:22948382017-11-29
spellingShingle hep-ph
Particle Physics - Phenomenology
gr-qc
General Relativity and Cosmology
astro-ph.CO
Astrophysics and Astronomy
hep-th
Particle Physics - Theory
Ellis, John
Nanopoulos, Dimitri V.
Olive, Keith A.
From $R^2$ Gravity to No-Scale Supergravity
title From $R^2$ Gravity to No-Scale Supergravity
title_full From $R^2$ Gravity to No-Scale Supergravity
title_fullStr From $R^2$ Gravity to No-Scale Supergravity
title_full_unstemmed From $R^2$ Gravity to No-Scale Supergravity
title_short From $R^2$ Gravity to No-Scale Supergravity
title_sort from $r^2$ gravity to no-scale supergravity
topic hep-ph
Particle Physics - Phenomenology
gr-qc
General Relativity and Cosmology
astro-ph.CO
Astrophysics and Astronomy
hep-th
Particle Physics - Theory
url https://dx.doi.org/10.1103/PhysRevD.97.043530
http://cds.cern.ch/record/2294838
work_keys_str_mv AT ellisjohn fromr2gravitytonoscalesupergravity
AT nanopoulosdimitriv fromr2gravitytonoscalesupergravity
AT olivekeitha fromr2gravitytonoscalesupergravity