Hans Arnold Winther

Associate professor

Norway

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Hans Arnold Winther is an Associate Professor at the University of Oslo Institute of Theoretical Astrophysics, located in Norway. His research focuses on cosmology, including topics such as the preparation for the Euclid mission, modeling nonlinear scales, and the role of voids in galaxy clustering. Recent articles authored by Professor Winther explore advanced methods for simulating dark matter and the implications of modified gravity on cosmic structures.

Articles (12)

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2025

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2025

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2024

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2023

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2023

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2023

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2022

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2022

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2022

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2022

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2021

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2020

Collaborators (10)

Sergio Di Domizio

Professore Associato

University of Genoa

ITALY

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Slađana Radinović

Institute of Space Sciences

SPAIN

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Kazuya Koyama

Professor

University of Portsmouth

UNITED KINGDOM

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Vivian Miranda

Assistant Professor

Stony Brook University

UNITED STATES

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pauline vielzeuf

Institute of High Pressure Physics

SPAIN

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Elena Massara

University of Waterloo

CANADA

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Alex Woodfinden

University of Waterloo

CANADA

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Nicolas Tessore

University College London

UNITED KINGDOM

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David F. Mota

Professor

University of Oslo

NORWAY

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Will J Percival

University of Waterloo

CANADA

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Hans Arnold Winther

Research Interests

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About

Articles (12)

Euclid preparation - LXII. Simulations and non-linearities beyond Lambda cold dark matter. 1. Numerical methods and validation

Euclid preparation - LXIII. Simulations and non-linearities beyond Lambda cold dark matter. 2. Results from non-standard simulations

Modeling nonlinear scales with the comoving Lagrangian acceleration method: Preparing for LSST Y1

Revisiting Vainshtein screening for fast N-body simulations

The void-galaxy cross-correlation function with massive neutrinos and modified gravity

Cosmological measurements from void-galaxy and galaxy-galaxy clustering in the Sloan Digital Sky Survey

Velocity profiles of matter and biased tracers around voids

Measurements of cosmic expansion and growth rate of structure from voids in the Sloan Digital Sky Survey between redshift 0.07 and 1.0

Enabling matter power spectrum emulation in beyond-ΛCDM cosmologies with COLA

Cosmological simulations of self-interacting Bose-Einstein condensate dark matter

Dynamical friction in Bose-Einstein condensed self-interacting dark matter at finite temperatures, and the Fornax dwarf spheroidal

Collapse of spherical overdensities in superfluid models of dark matter

Collaborators (10)

Sergio Di Domizio

Slađana Radinović

Kazuya Koyama

Vivian Miranda

pauline vielzeuf

Elena Massara

Alex Woodfinden

Nicolas Tessore

David F. Mota

Will J Percival

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