Adrian Jenkins

Professor

United Kingdom

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About

Adrian Jenkins is a Professor at the Institute for Computational Cosmology, Durham University, UK. His research areas include dark matter properties, cosmic large-scale structure, and the influence of baryons on galaxy formation. His recent articles explore various projects focusing on cosmic simulations, the behavior of neutrinos, and the dynamics of galaxies within the Milky Way.

Articles (22)

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2025

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2021

Collaborators (9)

Christine M Simpson

University of Chicago

UNITED STATES

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John Lucey

University of Durham

UNITED KINGDOM

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John Helly

Durham University

UNITED KINGDOM

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Alis J Deason

University of Durham

UNITED KINGDOM

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Peter Johansson

University of Helsinki

FINLAND

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Baojiu Li

Professor

University of Durham

UNITED KINGDOM

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Jens Jasche

Associate Professor

Stockholm University

SWEDEN

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Carlos Frenk

Ogden Professor of Fundamental Physics

University of Durham

UNITED KINGDOM

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Oliver Hahn

Universität Wien

AUSTRIA

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Adrian Jenkins

Research Interests

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About

Articles (22)

cosmICweb: Cosmological Initial Conditions for Zoom-in Simulations in the Cloud

Constraints on the properties of νMSM dark matter using the satellite galaxies of the Milky Way

The MillenniumTNG project: impact of massive neutrinos on the cosmic large-scale structure and the distribution of galaxies

The Manticore Project I: a digital twin of our cosmic neighbourhood from Bayesian field-level analysis

The emperor’s new arc: gigaparsec patterns abound in a ΛCDM universe

Negative neutrino masses as a mirage of dark energy

The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the S8 tension

The influence of baryons on low-mass haloes

Overview and public data release of the augmented Auriga Project: cosmological simulations of dwarf and Milky Way-mass galaxies

The abundance of dark matter haloes down to Earth mass

Star Stream Velocity Distributions in Cold Dark Matter and Warm Dark Matter Galactic Halos

The mass accretion history of dark matter haloes down to Earth mass

The Milky Way’s plane of satellites is consistent with ΛCDM

Higher order initial conditions with massive neutrinos

Apostle–Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies

SIBELIUS-DARK: a galaxy catalogue of the local volume from a constrained realization simulation

The SIBELIUS Project: E Pluribus Unum

Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation

An optimal non-linear method for simulating relic neutrinos

Indra: a public computationally accessible suite of cosmological N-body simulations

The origin of X-ray coronae around simulated disc galaxies

Setting the stage: structures from Gaussian random fields

Collaborators (9)

Christine M Simpson

John Lucey

John Helly

Alis J Deason

Peter Johansson

Baojiu Li

Jens Jasche

Carlos Frenk

Oliver Hahn

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