activity
20032024
most citedGalaxy evolution in the metric of the Cosmic Web

209 citations · 1.5k across the 29 of their papers we have counts for

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Showing astro-ph.COShow all

18 papers · 1 filter

astro-ph.CO2024★ 3 cited

The energy shear of protohaloes

Marcello Musso, Giulia Despali, Ravi K. Sheth

As it collapses to form a halo, the shape of a protohalo patch is deformed by the initial shear field. This deformation is often modeled using the "deformation" tensor, constructed…

astro-ph.CO2020★ 24 cited

When do cosmic peaks, filaments or walls merge? A theory of critical events in a multi-scale landscape

Corentin Cadiou, Christophe Pichon, Sandrine Codis +5

The merging rate of cosmic structures is computed, relying on the Ansatz that they can be predicted in the initial linear density field from the coalescence of critical points with…

astro-ph.CO2020★ 56 cited

Application of peaks theory to the abundance of primordial black holes

Sam Young, Marcello Musso

We consider the application of peaks theory to the calculation of the number density of peaks relevant for primordial black hole (PBH) formation. For PBHs, the final mass is relate…

astro-ph.CO2019★ 14 cited

Excursion set peaks in energy as a model for haloes

Marcello Musso, Ravi K. Sheth

The simplest models of dark matter halo formation are based on the heuristic assumption, motivated by spherical collapse, that virialized haloes originate from initial regions that…

astro-ph.CO2017★ 97 cited

How does the cosmic web impact assembly bias?

M. Musso, C. Cadiou, C. Pichon +3

The mass, accretion rate and formation time of dark matter haloes near proto-filaments (identified as saddle points of the potential) are analytically predicted using a conditional…

astro-ph.CO2016★ 66 cited

Large-scale assembly bias of dark matter halos

Titouan Lazeyras, Marcello Musso, Fabian Schmidt

We present precise measurements of the assembly bias of dark matter halos, i.e. the dependence of halo bias on other properties than the mass, using curved "separate universe" N-bo…