Observational consequences of chaotic inflation with nonminimal coupling to gravity
By Andrei Linde, Mahdiyar Noorbala, A. Westphal. Journal of Cosmology and Astroparticle Physics, 2011
156 citations recorded by the source corpus.
Recently there was an extensive discussion of Higgs inflation in the theory with the potential \lambda(\phi^2-v^2)^2 and nonminimal coupling to gravity {\xi\over 2}\phi^2R, for \xi >> 1 and v > 1.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/786078c695956b6935a7c874fe78fcc5184600a6
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
In Nuclear and High Energy Physics
Citations in the corpus
- Superconformal generalizations of the Starobinsky model (2013, unknown): “It appears, for example, in the Higgs model with a non-minimal coupling to gravity, ξ 2φ 2R − λ 4 (φ 2 − v2)2, for ξ < 0, in the limit 1 + ξv2 1 [5].”
- Inflationary Cosmology after Planck 2013 (2014, background): “This function, upon the change of variables Φ → Φ̃ + 1 2a , is equivalent to the function f = −ma(Φ2 − 1 (2a)2 ) used previously in [89, 92].”
- Universality classes of inflation (2013, unknown): “[3–5].”
- The landscape of QCD axion models (2020, result): “For this reason, a non-minimal coupling to gravity ξ is introduced to circumvent the bounds from the Planck mission, so that the potential at large values of ρa is flattened out and the model reconciles with observations [660].”
- Universality class in conformal inflation (2013, background): “The same observational predictions were made in the context of chaotic inflation in the theory λφ4 [10] with non-minimal coupling to gravity ξ 2φ 2R with ξ > 0 [11,12], in its supersymmetric extensions in [6,7,13,14] and in a certain limit of the model with the Higgs potential with ξ < 0 [15].”
- Superconformal generalization of the chaotic inflation model (2013, methodology): “In the subsequent set of papers, we will discuss other versions of inflationary models based on conformal and superconformal symmetry, and on supergravity, including the ones described in [14], [15], [35].”
- Multi-field conformal cosmological attractors (2013, background): “The same observational predictions were made in the context of chaotic inflation in the theory λφ4 [7] with non-minimal coupling to gravity ξ 2φ 2R with ξ > 0 [8–10], in its supersymmetric extensions in [11–15, 23] and in a certain limit of the model with the Higgs potential with ξ < 0 [16].”
- Non-minimal Inflationary Attractors (2013, methodology): “This paper would be incomplete without mentioning another type of cosmological attractors which was found some time ago in a very similar context [21].”