activity
20062026
most citedConditions for the cosmological viability of f(R) dark energy models

708 citations · 2.6k across the 50 of their papers we have counts for

collaborators

50 papers

gr-qc2026

Higher Lovelock Curvature Terms Favor Local Nakedness in Dust Collapse

Apratim Ganguly, Radouane Gannouji, Akshay Kumar

We show that higher-curvature Lovelock terms do not restore local cosmic censorship in spherical dust collapse, but instead promote the local visibility of central shell-focusing s…

gr-qc2026

Neutron stars in Poincaré gauge gravity with quadratic torsion

Chaitanya Vashistha, Radouane Gannouji, Apratim Ganguly

We study static neutron stars in an algebraic sector of Poincaré gauge gravity with parity-even and parity-odd quadratic torsion invariants. Since torsion is non-propagating, the c…

gr-qc2026

Oppenheimer-Snyder Collapse in f(R) Gravity : Stalemate or Resolution?

Soumya Chakrabarti, Apratim Ganguly, Radouane Gannouji +1

We study the Oppenheimer--Snyder (OS) collapse problem in metric gravity by matching a homogeneous dust Friedmann--Lemaître--Robertson--Walker (FLRW) interior to a generaliz…

hep-th2025

Entanglement inequalities, black holes and the architecture of typical states

Radouane Gannouji, Ayan Mukhopadhyay, Nicolas Pinochet

Using the holographic realization of the Araki--Lieb (AL) inequality, we argue that the leading entanglement plateau constrains the organization of typical pure states in a fixed-$…

gr-qc2025

Nonlinear dynamics in Horndeski gravity: a renormalized approach to effective gravitational coupling

Luca Amendola, Carla Bernal, Radouane Gannouji

This paper develops a renormalized perturbation theory framework for nonlinear structure formation in a broad class of modified gravity models that exhibit Vainshtein screening, wi…

gr-qc2025★ 3 cited

Characteristic initial value problems for the Einstein-Maxwell-scalar field equations in spherical symmetry

Thomas Mädler, Radouane Gannouji, Emanuel Gallo

The characteristic initial boundary problem is discussed in spherical symmetry for the Einstein-Maxwell-scalar field equations. It is formulated for an affine-null metric and the r…