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20112026
most citedCosmology with the Laser Interferometer Space Antenna

359 citations · 5.5k across the 111 of their papers we have counts for

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71 papers · 1 filter

astro-ph.CO2026

Universal CMB Phase Coherence from Single-Field Inflation

Siméon Vareilles, Thomas Colas, Julien Grain +2

The phase coherence of primordial perturbations shapes the acoustic peaks of the CMB and is regarded as a key signature of inflation. Inflationary scenarios at different energy sca…

astro-ph.CO2026

Compaction function in stochastic inflation: a \texttt{FOREST} of type I and II primordial black holes

Chiara Animali, Pierre Auclair, Baptiste Blachier +2

We show how to compute the compaction function within stochastic inflation, by solving the random field dynamics on stochastic binary trees. In this framework, the compaction funct…

astro-ph.CO2026

Excursion-set for Primordial Black Holes I: white noise and moving barrier

Pierre Auclair, Baptiste Blachier, Vincent Vennin

In the excursion-set formalism, the mass distribution of primordial black holes (PBHs) is derived from the first-passage time of a random walk describing the density contrast as th…

astro-ph.CO2025★ 8 cited

Stochastic inflation with gradient interactions

Vadim Briaud, Ryodai Kawaguchi, Vincent Vennin

Stochastic inflation rests on the separate-universe approximation, i.e. the ability to describe long-wavelength fluctuations in an inflating universe as homogeneous perturbations o…

astro-ph.CO2025★ 3 cited

Primordial black holes from a curvaton: the role of bimodal distributions

Tomotaka Kuroda, Atsushi Naruko, Vincent Vennin +1

We investigate the formation of primordial black holes in curvaton models of inflation, where the curvature perturbation is not only generated by the inflaton but also by a light s…

astro-ph.CO2025★ 4 cited

On the Hamilton-Jacobi approach to inflation beyond slow roll

Danilo Artigas, Emmanuel Frion, Tays Miranda +2

The Hamilton-Jacobi approach is a powerful tool to describe super-Hubble dynamics during cosmological inflation in a non-linear way. A key assumption of this framework is to neglec…

astro-ph.CO2025

How deep is the dip and how tall are the wiggles in inflationary power spectra?

Vadim Briaud, Alexandros Karam, Niko Koivunen +3

We study linear scalar perturbations in single-field models of inflation featuring a non-attractor phase. These models lead to a peak in the curvature power spectrum that may resul…

astro-ph.CO2025

Harvesting primordial black holes from stochastic trees with

Chiara Animali, Pierre Auclair, Baptiste Blachier +1

We introduce a novel framework to implement stochastic inflation on stochastic trees, modelling the inflationary expansion as a branching process. Combined with the formalism,…

astro-ph.CO2024★ 17 cited

Stochastic inflation beyond slow roll: noise modelling and importance sampling

Joseph H. P. Jackson, Hooshyar Assadullahi, Andrew D. Gow +3

We simulate the distribution of very rare, large excursions in the primordial density field produced in models of inflation in the very early universe which include a strong enhanc…

astro-ph.CO2024★ 13 cited

Vanilla Inflation Predicts Negative Running

Jerome Martin, Christophe Ringeval, Vincent Vennin

We show that the simplest, and currently favoured, theoretical realizations of cosmic inflation yield a sharp prediction for the running of the spectral index . Using…

astro-ph.CO2024★ 33 cited

Cosmic Inflation at the Crossroads

Jerome Martin, Christophe Ringeval, Vincent Vennin

The capability of Cosmic Inflation to explain the latest Cosmic Microwave Background and Baryonic Acoustic Oscillation data is assessed by performing Bayesian model comparison with…

astro-ph.CO2024★ 15 cited

Quantum diffusion and large primordial perturbations from inflation

Vincent Vennin, David Wands

Quantum diffusion describes the inflow of vacuum quantum fluctuations as they get amplified by gravitational instability, and stretched to large distances during inflation. In this…

astro-ph.CO2024★ 32 cited

Clustering of primordial black holes from quantum diffusion during inflation

Chiara Animali, Vincent Vennin

We study how large fluctuations are spatially correlated in the presence of quantum diffusion during inflation. This is done by computing real-space correlation functions in the st…

astro-ph.CO2023★ 1 cited

Inflation (2025)

John Ellis, Vincent Vennin, David Wands

This is a review article for The Review of Particle Physics 2026 (aka the Particle Data Book), appearing as Chapter 23. It forms a compact review of our understanding of cosmologic…

astro-ph.CO2023

Revisiting the stochastic QCD axion window: departure from equilibrium during inflation

Vadim Briaud, Kenji Kadota, Shinji Mukohyama +2

If dark matter is made of QCD axions, its abundance is determined by the vacuum expectation value acquired by the axion field during inflation. The axion is usually assumed to foll…

astro-ph.CO2023★ 40 cited

The separate-universe approach and sudden transitions during inflation

Joseph H. P. Jackson, Hooshyar Assadullahi, Andrew D. Gow +3

The separate-universe approach gives an intuitive way to understand the evolution of cosmological perturbations in the long-wavelength limit. It uses solutions of the spatially-hom…

astro-ph.CO2023★ 31 cited

Primordial black holes and their gravitational-wave signatures

Eleni Bagui, Sebastien Clesse, Valerio De Luca +17

In the recent years, primordial black holes (PBHs) have emerged as one of the most interesting and hotly debated topics in cosmology. Among other possibilities, PBHs could explain…

astro-ph.CO2023★ 1 cited

Why does inflation look single field to us?

Koki Tokeshi, Vincent Vennin

Most high-energy constructions that realise a phase of cosmic inflation contain many degrees of freedom. Yet, cosmological observations are all consistent with single-field embeddi…

astro-ph.CO2023★ 7 cited

Spatial Curvature from Super-Hubble Cosmological Fluctuations

Baptiste Blachier, Pierre Auclair, Christophe Ringeval +1

We revisit how super-Hubble cosmological fluctuations induce, at any time in the cosmic history, a non-vanishing spatial curvature of the local background metric. The random nature…

astro-ph.CO2023★ 25 cited

Uphill inflation

Vadim Briaud, Vincent Vennin

Primordial black holes (PBH) may form from large cosmological perturbations, produced during inflation when the inflaton's velocity is sufficiently slowed down. This usually requir…

astro-ph.CO2022★ 108 cited

Non-perturbative non-Gaussianity and primordial black holes

Andrew D. Gow, Hooshyar Assadullahi, Joseph H. P. Jackson +3

We present a non-perturbative method for calculating the abundance of primordial black holes given an arbitrary one-point probability distribution function for the primordial curva…

astro-ph.CO2022★ 61 cited

Primordial black holes from stochastic tunnelling

Chiara Animali, Vincent Vennin

If the inflaton gets trapped in a local minimum of its potential shortly before the end of inflation, it escapes by building up quantum fluctuations in a process known as stochasti…

astro-ph.CO2022★ 2 cited

Massive galaxy clusters like "El Gordo'' hint at primordial quantum diffusion

Jose María Ezquiaga, Juan García-Bellido, Vincent Vennin

It is generally assumed within the standard cosmological model that initial density perturbations are Gaussian at all scales. However, primordial quantum diffusion unavoidably gene…

astro-ph.CO2022★ 30 cited

Numerical simulations of stochastic inflation using importance sampling

Joseph H. P. Jackson, Hooshyar Assadullahi, Kazuya Koyama +2

We show how importance sampling can be used to reconstruct the statistics of rare cosmological fluctuations in stochastic inflation. We have developed a publicly available package,…