Implications of purely classical gravity for inflationary tensor modes

DOI10.1142/S0217732314501636zbMath1301.83023arXiv1211.4678MaRDI QIDQ2932708

P. S. Bhupal Dev, Anupam Mazumdar, Amjad Ashoorioon

Publication date: 9 December 2014

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1211.4678

zbMATH Keywords

inflationgravitational wavesclassical gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05) Gravitational waves (83C35)

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Cites Work

• THE ONE-LOOP APPROXIMATION OF THE TRANSITION AMPLITUDE IN KREIN SPACE QUANTIZATION
• ON THE REST AND FLAT LIMITS OF THE SCALAR MODES ON THE DE SITTER SPACETIME
• Is quantum gravity necessary?
• RADIAL CASIMIR EFFECT IN A SPHERE THROUGH THE KREIN SPACE QUANTIZATION
• GRAVITATIONAL FIELD OF A ROTATING GLOBAL MONOPOLE IN f(R) THEORY
• Bouncing universes in string-inspired gravity

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