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Quantum-Ordering Ambiguities in Weak Chern—Simons 4D Gravity and Metastability of the Condensate-Induced Inflation
Published 2025-01-01Subjects: “…cosmology…”
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Grand unification at the cosmological collider with chemical potential
Published 2025-01-01“…We show that, within high-scale inflation, chemical potential enhancement can lead to observably strong signals for trinification partners in future cosmological surveys.…”
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Warm Inflation with Nonminimal Derivative Coupling
Published 2014-01-01“…We present a detailed calculation of the cosmological perturbations in this setup. We use the recent observational data from the joint data set of WMAP9 + BAO + H0 and also the Planck satellite data to constrain our model parameters for natural and chaotic inflation potentials. …”
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Quantum Cosmology of Quadratic f(R) Theories with a FRW Metric
Published 2017-01-01“…We study the quantum cosmology of a quadratic fR theory with a FRW metric, via one of its equivalent Horndeski type actions, where the dynamic of the scalar field is induced. …”
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Mimetic Gravity: A Review of Recent Developments and Applications to Cosmology and Astrophysics
Published 2017-01-01“…Mimetic gravity is a Weyl-symmetric extension of General Relativity, related to the latter by a singular disformal transformation, wherein the appearance of a dust-like perfect fluid can mimic cold dark matter at a cosmological level. Within this framework, it is possible to provide a unified geometrical explanation for dark matter, the late-time acceleration, and inflation, making it a very attractive theory. …”
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Non-Gaussianity from Particle Production during Inflation
Published 2010-01-01“…In this review we show that interactions between the produced particles and the inflaton condensate can lead to a qualitatively new mechanism for generating cosmological fluctuations from inflation. We illustrate this effect using a simple prototype model g2(ϕ−ϕ0)2χ2 for the interaction between the inflaton, ϕ, and iso-inflaton, χ. …”
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Searches for other vacua. Part II. A new Higgstory at the cosmological collider
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Warm non-minimally coupled Peccei–Quinn inflation and de Sitter Swampland conjecture
Published 2025-03-01“…Our model incorporates a PQ scalar field that is non-minimally coupled to gravity, facilitating inflation through a dissipative process that sustains a thermal bath, thereby distinguishing it from conventional cold inflation. …”
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Primordial black holes from effective field theory of stochastic single field inflation at NNNLO
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From de Sitter to de Sitter: Decaying Vacuum Models as a Possible Solution to the Main Cosmological Problems
Published 2018-01-01“…Decaying vacuum cosmological models evolving smoothly between two extreme (very early and late time) de Sitter phases are able to solve or at least to alleviate some cosmological puzzles; among them we have (i) the singularity, (ii) horizon, (iii) graceful-exit from inflation, and (iv) the baryogenesis problem. …”
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Evaluation of the Single-component Thermal Dust Emission Model in Cosmic Microwave Background Experiments
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Aspects of Moduli Stabilization in Type IIB String Theory
Published 2016-01-01“…In particular, the associated inflation models such as racetrack inflation and Kähler inflation are analyzed. …”
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More on the Non-Gaussianity of Perturbations in a Nonminimal Inflationary Model
Published 2018-01-01“…We study nonlinear cosmological perturbations and their possible non-Gaussian character in an extended nonminimal inflation where gravity is coupled nonminimally to both the scalar field and its derivatives. …”
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Noether Gauge Symmetry of Dirac Field in (2 + 1)-Dimensional Gravity
Published 2015-01-01“…In this picture, it is shown that, for the nonminimal coupling case, the cosmological solutions indicate both an early-time inflation and late-time acceleration for the universe.…”
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Generalising axion-like particle as the curvaton: sourcing primordial density perturbation and non-Gaussianities
Published 2024-10-01“…The ALP is a spectator field during inflation but it starts to oscillate and dominates the energy density of the universe after inflation ends, thereby sourcing isocurvature perturbations, while standard curvature fluctuations from the inflaton are assumed to be sub-dominant. …”
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Will There Be Future Deceleration? A Study of Particle Creation Mechanism in Nonequilibrium Thermodynamics
Published 2015-01-01“…Motivated by thermodynamical point of view, cosmological solutions are evaluated for the particle creation rates in three cosmic phases, namely, inflation, matter dominated era, and present late time acceleration. …”
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