activity
20102026
most cited-evolution: a relativistic N-body code for clustering dark energy

44 citations · 235 across the 26 of their papers we have counts for

collaborators

28 papers

astro-ph.CO2026

Mercury (Hg): a relativistic -body simulation for Horndeski gravity

Ahmad Nouri-Zonoz, Farbod Hassani, Julian Adamek +2

We present Mercury, a relativistic -body code for cosmological simulations in the -basis formulation of Horndeski gravity. Mercury extends a particle-mesh scheme by incorpora…

astro-ph.CO2026

Cosmological Signatures of Curvature-Coupled Dark Energy

Abdolali Banihashemi, Farbod Hassani, Alessandro Casalino +2

We study a curvature-coupled dark energy model that can modify cosmological evolution both before recombination and during the late-time accelerated era. The model belongs to the c…

astro-ph.CO2026

Signatures of kinetic gravity braiding in cosmological probes of the gravitational field

Ahmad Nouri-Zonoz, Farbod Hassani, Julian Adamek +2

We study the observational signatures of kinetic gravity braiding (KGB) models in relativistic cosmological probes constructed along the past light cone. Using the relativistic …

astro-ph.CO2025

KGB-evolution: a relativistic -body code for kinetic gravity braiding models

Ahmad Nouri-Zonoz, Farbod Hassani, Emilio Bellini +1

We present KGB-evolution, a relativistic -body simulation code that extends the -evolution code by incorporating an effective field theory parameterization of kinetic gravity…

astro-ph.CO2024

Matter Power Spectra in Modified Gravity: A Comparative Study of Approximations and -Body Simulations

Benjamin Bose, Ashim Sen Gupta, Bartolomeo Fiorini +9

Testing gravity and the concordance model of cosmology, CDM, at large scales is a key goal of this decade's largest galaxy surveys. Here we present a comparative study of dark m…

astro-ph.CO2024★ 1 cited

-elator: emulating clustering effects of the -essence dark energy

A. R. Nouri-Zonoz, F. Hassani, M. Kunz

We build an emulator based on the polynomial chaos expansion (PCE) technique to efficiently model the non-linear effects associated with the clustering of the -essence dark ener…

astro-ph.CO2024★ 4 cited

Environmental cosmic acceleration from a phase transition in the dark sector

Øyvind Christiansen, Farbod Hassani, David F. Mota

A new degravitation mechanism within the framework of scalar tensor gravity is postulated and included by prescription. The mechanism eliminates all constant contributions from the…

astro-ph.CO2024★ 6 cited

asimulation: Domain formation and impact on observables in resolved cosmological simulations of the (a)symmetron

Øyvind Christiansen, Farbod Hassani, David F. Mota

The symmetron is a dark energy and dark matter candidate that forms topological defects in the late-time universe and holds the promise of resolving some of the cosmological tensio…

astro-ph.CO2024★ 1 cited

Gravitational waves from dark domain walls

Øyvind Christiansen, Julian Adamek, Farbod Hassani +1

For most of cosmic history, the evolution of our Universe has been governed by the physics of a 'dark sector', consisting of dark matter and dark energy, whose properties are only…

astro-ph.CO2023★ 1 cited

Clustering of dark matter in the cosmic web as a probe of massive neutrinos

Mohadese Khoshtinat, Mohammad Ansarifard, Farbod Hassani +1

The large-scale structure of the Universe is distributed in a cosmic web. Studying the distribution and clustering of dark matter particles and halos may open up a new horizon for…

astro-ph.CO2023★ 3 cited

Clusternets: A deep learning approach to probe clustering dark energy

Amirmohammad Chegeni, Farbod Hassani, Alireza Vafaei Sadr +2

Machine Learning (ML) algorithms are becoming popular in cosmology for extracting valuable information from cosmological data. In this paper, we evaluate the performance of a Convo…

astro-ph.CO2023★ 11 cited

asevolution: a relativistic N-body implementation of the (a)symmetron

Øyvind Christiansen, Farbod Hassani, Mona Jalilvand +1

We present asevolution, a cosmological N-body code developed based on gevolution, which consistently solves for the (a)symmetron scalar field and metric potentials within the weak-…

astro-ph.CO2022★ 26 cited

Euclid: Modelling massive neutrinos in cosmology -- a code comparison

J. Adamek, R. E. Angulo, C. Arnold +133

The measurement of the absolute neutrino mass scale from cosmological large-scale clustering data is one of the key science goals of the Euclid mission. Such a measurement relies o…

astro-ph.CO2022

Biased tracers as a probe of beyond-CDM cosmologies

Farbod Hassani, Julian Adamek, Ruth Durrer +1

Cosmological models beyond CDM, like those featuring massive neutrinos or modifications of gravity, often display a characteristic change (scale-dependent suppression or enhance…

math-ph2022★ 6 cited

Instabilities Appearing in Cosmological Effective Field theories: When and How?

Jean-Pierre Eckmann, Farbod Hassani, Hatem Zaag

Nonlinear partial differential equations appear in many domains of physics, and we study here a typical equation which one finds in effective field theories (EFT) originated from c…

astro-ph.CO2022★ 4 cited

A new instability in clustering dark energy?

Farbod Hassani, Julian Adamek, Martin Kunz +2

In this paper, we study the effective field theory (EFT) of dark energy for the -essence model beyond linear order. Using particle-mesh -body simulations that consistently so…

astro-ph.CO2021

Cosmic velocity, density and halo mass function: Insights from deep learning

Saba Etezad-Razavi, Erfan Abbasgholinejad, Mohammad-Hadi Sotoudeh +3

We discuss an implementation of a deep learning framework to gain insight into dark matter (DM) structure formation. We investigate the contribution of velocity and density field i…

astro-ph.CO2021★ 7 cited

A new nonlinear instability for scalar fields

Farbod Hassani, Pan Shi, Julian Adamek +2

In this letter we introduce the non-linear partial differential equation (PDE) showing a new type of instability. Such equations appear in…

astro-ph.CO2021

Structure of cosmic web in non-linear regime: the nearest neighbour and spherical contact distributions

Mohammad Ansari Fard, Zahra Baghkhani, Laya Ghodsi +3

In non-linear scales, the matter density distribution is not Gaussian. Consequently, the widely used two-point correlation function is not adequate anymore to capture the matter de…

astro-ph.CO2020★ 21 cited

Clustering dark energy imprints on cosmological observables of the gravitational field

Farbod Hassani, Julian Adamek, Martin Kunz

We study cosmological observables on the past light cone of a fixed observer in the context of clustering dark energy. We focus on observables that probe the gravitational field di…

astro-ph.CO2020★ 38 cited

-body simulations for parametrised modified gravity

Farbod Hassani, Lucas Lombriser

We present , an -body code simulating the cosmological structure formation for parametrised modifications of gravity. It is built from the combination of…

astro-ph.CO2019★ 25 cited

Parametrising non-linear dark energy perturbations

Farbod Hassani, Benjamin L'Huillier, Arman Shafieloo +2

In this paper, we quantify the non-linear effects from -essence dark energy through an effective parameter that encodes the additional contribution of a dark energy fluid or…

astro-ph.CO2019★ 44 cited

-evolution: a relativistic N-body code for clustering dark energy

Farbod Hassani, Julian Adamek, Martin Kunz +1

We introduce -evolution, a relativistic -body code based on , which includes clustering dark energy among its cosmological components. To describe dark e…

math.NA2019

The detection of relativistic corrections in cosmological N-body simulations

Jean-Pierre Eckmann, Farbod Hassani

Cosmological N-body simulations are done on massively parallel computers. This necessitates the use of simple time integrators, and, additionally, of mesh-grid approximations of th…