Einstein-Cartan gravity, matter, and scale-invariant generalization

Abstract We study gravity coupled to scalar and fermion fields in the Einstein-Cartan framework. We discuss the most general form of the action that contains terms of mass dimension not bigger than four, leaving out only contributions quadratic in curvature. By resolving the theory explicitly for to...
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Gespeichert in:

Autor*in:	M. Shaposhnikov [verfasserIn] A. Shkerin [verfasserIn] I. Timiryasov [verfasserIn] S. Zell [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2020

Schlagwörter:	Classical Theories of Gravity Cosmology of Theories beyond the SM Models of Quantum Gravity Gauge Symmetry

Übergeordnetes Werk:	In: Journal of High Energy Physics - SpringerOpen, 2016, (2020), 10, Seite 18
Übergeordnetes Werk:	year:2020 ; number:10 ; pages:18

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.1007/JHEP10(2020)177

Katalog-ID:	DOAJ007976682

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callnumber-first	Q - Science
author	M. Shaposhnikov
spellingShingle	M. Shaposhnikov misc QC770-798 misc Classical Theories of Gravity misc Cosmology of Theories beyond the SM misc Models of Quantum Gravity misc Gauge Symmetry misc Nuclear and particle physics. Atomic energy. Radioactivity Einstein-Cartan gravity, matter, and scale-invariant generalization
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topic_title	QC770-798 Einstein-Cartan gravity, matter, and scale-invariant generalization Classical Theories of Gravity Cosmology of Theories beyond the SM Models of Quantum Gravity Gauge Symmetry
topic	misc QC770-798 misc Classical Theories of Gravity misc Cosmology of Theories beyond the SM misc Models of Quantum Gravity misc Gauge Symmetry misc Nuclear and particle physics. Atomic energy. Radioactivity
topic_unstemmed	misc QC770-798 misc Classical Theories of Gravity misc Cosmology of Theories beyond the SM misc Models of Quantum Gravity misc Gauge Symmetry misc Nuclear and particle physics. Atomic energy. Radioactivity
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title	Einstein-Cartan gravity, matter, and scale-invariant generalization
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title_sort	einstein-cartan gravity, matter, and scale-invariant generalization
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title_auth	Einstein-Cartan gravity, matter, and scale-invariant generalization
abstract	Abstract We study gravity coupled to scalar and fermion fields in the Einstein-Cartan framework. We discuss the most general form of the action that contains terms of mass dimension not bigger than four, leaving out only contributions quadratic in curvature. By resolving the theory explicitly for torsion, we arrive at an equivalent metric theory containing additional six-dimensional operators. This lays the groundwork for cosmological studies of the theory. We also perform the same analysis for a no-scale scenario in which the Planck mass is eliminated at the cost of adding an extra scalar degree of freedom. Finally, we outline phenomenological implications of the resulting theories, in particular to inflation and dark matter production.
abstractGer	Abstract We study gravity coupled to scalar and fermion fields in the Einstein-Cartan framework. We discuss the most general form of the action that contains terms of mass dimension not bigger than four, leaving out only contributions quadratic in curvature. By resolving the theory explicitly for torsion, we arrive at an equivalent metric theory containing additional six-dimensional operators. This lays the groundwork for cosmological studies of the theory. We also perform the same analysis for a no-scale scenario in which the Planck mass is eliminated at the cost of adding an extra scalar degree of freedom. Finally, we outline phenomenological implications of the resulting theories, in particular to inflation and dark matter production.
abstract_unstemmed	Abstract We study gravity coupled to scalar and fermion fields in the Einstein-Cartan framework. We discuss the most general form of the action that contains terms of mass dimension not bigger than four, leaving out only contributions quadratic in curvature. By resolving the theory explicitly for torsion, we arrive at an equivalent metric theory containing additional six-dimensional operators. This lays the groundwork for cosmological studies of the theory. We also perform the same analysis for a no-scale scenario in which the Planck mass is eliminated at the cost of adding an extra scalar degree of freedom. Finally, we outline phenomenological implications of the resulting theories, in particular to inflation and dark matter production.
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