activity
20142025
most citedConstraining Primordial non-Gaussianity with Bispectrum and Power Spectum from Upcoming Optical and Radio Surveys

136 citations · 359 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.CO2025★ 1 cited

Power Spectrum Emulators from Neural Networks and Tree-Based Methods

Andrei Lazanu

We use two subsets of 2000 and 1000 Quijote simulations to build two power spectrum emulators, allowing for fast computations of the non-linear matter power spectrum. The first emu…

astro-ph.CO2025★ 2 cited

Primordial gravitational waves in DHOST inflation

Philippe Brax, Andrei Lazanu

We consider DHOST inflationary models with a shift symmetry leading to a de Sitter space-time at the background cosmological level. Deviations from scale invariance of the scalar a…

astro-ph.CO2024

A DHOST model of inflation: CMB constraints from the power spectrum and the bispectrum

Andrei Lazanu

We build an inflationary model based on Degenerate Higher Order Scalar Tensor (DHOST) theories in a de Sitter background. We determine the scale-dependent power spectrum of curvatu…

astro-ph.CO2023★ 3 cited

CMB bispectrum constraints on DHOST inflation

Wuhyun Sohn, Andrei Lazanu, Philippe Brax +1

We present the first direct constraints on a Degenerate Higher Order Scalar Tensor (DHOST) inflation model using the Planck 2018 Cosmic Microwave Background (CMB) results on non-Ga…

astro-ph.CO2021★ 7 cited

Non-Gaussianity in DHOST inflation

Philippe Brax, Andrei Lazanu

DHOST inflation models where deviations from a pure de Sitter background are induced by an axion-like potential can lead to large non-Gaussianities. We investigate the nature of no…

astro-ph.CO2021★ 2 cited

The reach of next-to-leading-order perturbation theory for the matter bispectrum

Davit Alkhanishvili, Cristiano Porciani, Emiliano Sefusatti +4

We provide a comparison between the matter bispectrum derived with different flavours of perturbation theory at next-to-leading order and measurements from an unprecedentedly large…