f(R) and Brans-Dicke theories and the Swampland
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Publication:5862957
DOI10.1088/1475-7516/2019/05/042zbMath1481.83078arXiv1902.02849OpenAlexW3100908475MaRDI QIDQ5862957
Ido Ben-Dayan, Michal Artymowski
Publication date: 10 March 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1902.02849
String and superstring theories in gravitational theory (83E30) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
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Cites Work
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- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- The string swampland constraints require multi-field inflation
- The Landscape, the Swampland and the Era of Precision Cosmology
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- Further Refining the de Sitter Swampland Conjecture
- A Note on Inflation and the Swampland
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