activity
19932026
most citedWarm Little Inflaton

200 citations · 3.7k across the 76 of their papers we have counts for

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Showing astro-ph.COShow all

12 papers · 1 filter

astro-ph.CO2023★ 2 cited

Non-thermal moduli production during preheating in -attractor inflation models

Khursid Alam, Mar Bastero-Gil, Koushik Dutta +1

Production of gravitationally coupled light moduli fields must be suppressed in the early universe, so that its decay products do not alter Big Bang Nucleosynthesis (BBN) predictio…

astro-ph.CO2019★ 12 cited

Reexamination of the warm inflation curvature perturbations spectrum

Mar Bastero-Gil, Arjun Berera, Jaime R. Calderón

The two approaches to compute perturbations in warm inflation are examined. It is shown that both approaches lead to different expressions for the amplitude of the primordial spect…

astro-ph.CO2018★ 48 cited

Dynamical and observational constraints on the Warm Little Inflaton scenario

Mar Bastero-Gil, Arjun Berera, Rafael Hernandez-Jimenez +1

We explore the dynamics and observational predictions of the Warm Little Inflaton scenario, presently the simplest realization of warm inflation within a concrete quantum field the…

astro-ph.CO2017★ 64 cited

Constraining Warm Inflation with CMB data

Mar Bastero-Gil, Sukannya Bhattacharya, Koushik Dutta +1

We confront the warm inflation observational predictions directly with the latest CMB data. We focus on a linear temperature (T) dissipative coefficient combined with the simplest…

astro-ph.CO2016★ 25 cited

The role of fluctuation-dissipation dynamics in setting initial conditions for inflation

Mar Bastero-Gil, Arjun Berera, Robert Brandenberger +3

We study the problem of initial conditions for slow-roll inflation along a plateau-like scalar potential within the framework of fluctuation-dissipation dynamics. We consider, in p…

astro-ph.CO2014★ 67 cited

Theory of non-Gaussianity in warm inflation

Mar Bastero-Gil, Arjun Berera, Ian G. Moss +1

The theory and methodology is developed to compute the bispectrum in warm inflation, leading to results for the non-linearity parameter and the shape of the bispectrum. Particular…

astro-ph.CO2014★ 57 cited

Observational implications of mattergenesis during inflation

Mar Bastero-Gil, Arjun Berera, Rudnei O. Ramos +1

The observed baryon asymmetry, as well as potentially an asymmetry in the dark matter sector, can be produced through dissipative particle production during inflation. A distinctiv…

astro-ph.CO2014★ 80 cited

Cosmological fluctuations of a random field and radiation fluid

Mar Bastero-Gil, Arjun Berera, Ian G. Moss +1

A generalization of the random fluid hydrodynamic fluctuation theory due to Landau and Lifshitz is applied to describe cosmological fluctuations in systems with radiation and scala…

astro-ph.CO2013★ 26 cited

On the power spectrum generated during inflation

Mar Bastero-Gil, Arjun Berera, Namit Mahajan +1

Recently there have been differing viewpoints on how to evaluate the curvature power spectrum generated during inflation. Since the primordial curvature power spectrum is the seed…

astro-ph.CO2012★ 47 cited

Stability analysis for the background equations for inflation with dissipation and in a viscous radiation bath

Mar Bastero-Gil, Arjun Berera, Rafael Cerezo +2

The effects of bulk viscosity are examined for inflationary dynamics in which dissipation and thermalization are present. A complete stability analysis is done for the background i…

astro-ph.CO2011★ 131 cited

Shear viscous effects on the primordial power spectrum from warm inflation

M. Bastero-Gil, A. Berera, R. O. Ramos

We compute the primordial curvature spectrum generated during warm inflation, including shear viscous effects. The primordial spectrum is dominated by the thermal fluctuations of t…

astro-ph.CO2009★ 7 cited

Towards Realizing Warm Inflation in String Theory

Mar Bastero-Gil, Arjun Berera, James B. Dent +1

We give a generic argument that string theory provides a natural setting for warm inflationary cosmology. We then explore a specific model with an inflaton modulus field coupled to…