activity
20162025
most citedViable tensor-to-scalar ratio in a symmetric matter bounce

27 citations · 130 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.CO2025★ 2 cited

The validity of separate-universe approach in transient ultra-slow-roll inflation

Rathul Nath Raveendran

We investigate the breakdown of the separate-universe approximation during transitions in transient ultra-slow-roll inflation by analyzing the evolution of the comoving curvature p…

gr-qc2024

Violation of Bell inequality from a squeezed coherent state of inflationary perturbations

Aurindam Mondal, Rathul Nath Raveendran

We investigate the quantum nature of primordial perturbations by studying the violation of Bell inequality when the initial state is taken to be a coherent state rather than the us…

astro-ph.CO2023★ 8 cited

Conserved cosmological perturbations in USR inflation and bouncing scenarios

Rathul Nath Raveendran

Inflationary and bouncing scenarios are two frameworks that provide the mechanism to overcome the horizon problem as well as generate the primordial perturbations. In this work, we…

astro-ph.CO2023

Mimicking two field inflationary features with a single field

Anvy Moly Tom, Rathul Nath Raveendran

It is well known that damped superimposed oscillations at large scales in the primordial power spectrum can be generated in both single field and two field models. In single field…

gr-qc2023★ 3 cited

Amplifying quantum discord during inflationary magnetogenesis through violation of parity

Sagarika Tripathy, Rathul Nath Raveendran, Krishnamohan Parattu +1

It is well known that, during inflation, the conformal invariance of the electromagnetic action has to be broken in order to produce magnetic fields of observed strengths today. Of…

astro-ph.CO2023★ 8 cited

Distinguishing cosmological models through quantum signatures of primordial perturbations

Rathul Nath Raveendran, Sumanta Chakraborty

We study the evolution of various measures of quantumness of the curvature perturbation by integrating out the inaccessible entropic fluctuations in the multi-field models of infla…

astro-ph.CO2022★ 25 cited

Enhanced power on small scales and evolution of quantum state of perturbations in single and two field inflationary models

Rathul Nath Raveendran, Krishnamohan Parattu, L. Sriramkumar

With the detection of gravitational waves from merging binary black holes, over the last few years, there has been a considerable interest in the literature to understand if these…

astro-ph.CO2021★ 11 cited

Reconstruction of potentials of the hybrid inflation in the light of primordial black hole formation

Ki-Young Choi, Su-beom Kang, Rathul Nath Raveendran

The large enhancement of the primordial power spectrum of the curvature perturbation can seed the formation of primordial black hole, that can play as a dark matter component in th…

gr-qc2019★ 7 cited

A gauge invariant prescription to avoid -crossing instability in Galileon bounce

Rathul Nath Raveendran

We revisit the evolutions of scalar perturbations in a non-singular Galileon bounce. It is known that the second order differential equation governing the perturbations is numerica…

astro-ph.CO2018★ 16 cited

Viable scalar spectral tilt and tensor-to-scalar ratio in near-matter bounces

Rathul Nath Raveendran, L. Sriramkumar

In a recent work, we had constructed a model consisting of two fields---a canonical scalar field and a non-canonical ghost field---that had sourced a symmetric matter bounce scenar…

astro-ph.CO2018★ 21 cited

Primordial features from ekpyrotic bounces

Rathul Nath Raveendran, L. Sriramkumar

Certain features in the primordial scalar power spectrum are known to improve the fit to the cosmological data. We examine whether bouncing scenarios can remain viable if future da…

gr-qc2017★ 27 cited

Viable tensor-to-scalar ratio in a symmetric matter bounce

Rathul Nath Raveendran, Debika Chowdhury, L. Sriramkumar

Matter bounces refer to scenarios wherein the universe contracts at early times as in a matter dominated epoch until the scale factor reaches a minimum, after which it starts expan…

astro-ph.CO2016★ 2 cited

Numerical evaluation of the tensor bispectrum in two field inflation

Rathul Nath Raveendran, L. Sriramkumar

We evaluate the dimensionless non-Gaussianity parameter , that characterizes the amplitude of the tensor bispectrum, numerically for a class of two field inflationar…