No-scale Brans-Dicke gravity — ultralight scalar boson & heavy inflaton

Abstract It is very much intriguing if the Planck scale M Pl is not a fundamental parameter. The Brans-Dicke gravity is nothing but the theory where the Planck scale M Pl is indeed an illusional parameter. The theory predicts a massless scalar boson whose exchanges between matters induce unwanted long range forces. We solve this problem imposing there is no dimensionful parameter in the theory, even at the quantum level. We further extend the theory by including a R 2 term and a non-minimal coupling of the Standard Model Higgs to gravity, as their coefficients are dimensionless. This extension provides a heavy inflaton field that is consistent with all cosmological observations, with a potential very similar to that of the Starobinsky model. The inflaton necessarily decays into the massless scalar bosons, resulting in a non-negligible amount of dark radiation in the present universe. We demonstrate that the inflation model yields a sufficiently high reheating temperature for successful leptogenesis, and we also discuss a possible candidate for dark matter.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2025-10-01
DOI
https://doi.org/10.1088/1475-7516/2025/10/032
Citations
3
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
3.46
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article

No-scale Brans-Dicke gravity — ultralight scalar boson & heavy inflaton

Muzi Hong, Kyohei Mukaida, Tsutomu T. Yanagida
3 citations
Journal of Cosmology and Astroparticle Physics
Cosmology and Gravitation Theories
3.46
article

No-scale Brans-Dicke gravity — ultralight scalar boson & heavy inflaton

Muzi Hong, Kyohei Mukaida, Tsutomu T. Yanagida
article en
3 citations

Abstract

Abstract It is very much intriguing if the Planck scale M Pl is not a fundamental parameter. The Brans-Dicke gravity is nothing but the theory where the Planck scale M Pl is indeed an illusional parameter. The theory predicts a massless scalar boson whose exchanges between matters induce unwanted long range forces. We solve this problem imposing there is no dimensionful parameter in the theory, even at the quantum level. We further extend the theory by including a R 2 term and a non-minimal coupling of the Standard Model Higgs to gravity, as their coefficients are dimensionless. This extension provides a heavy inflaton field that is consistent with all cosmological observations, with a potential very similar to that of the Starobinsky model. The inflaton necessarily decays into the massless scalar bosons, resulting in a non-negligible amount of dark radiation in the present universe. We demonstrate that the inflation model yields a sufficiently high reheating temperature for successful leptogenesis, and we also discuss a possible candidate for dark matter.

Journal of Cosmology and Astroparticle PhysicsVol. 2025(10)
High Energy Accelerator Research Organization (JP), Kavli Institute for the Physics and Mathematics of the Universe (JP), The Graduate University for Advanced Studies, SOKENDAI (JP), Institute of Natural Science (KP), Institute of Particle and Nuclear Studies, The University of Tokyo (JP)
Openalex Percentile: Top 7%
Cosmology and Gravitation Theories
3.46
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No-scale Brans-Dicke gravity — ultralight scalar boson & heavy inflaton — Muzi Hong, Kyohei Mukaida, et al. · Journal of Cosmology and Astroparticle Physics (2025) | TGRS Research Map | TGRS