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Thomas Tram

Researcher at Aarhus University

Publications -  85
Citations -  6703

Thomas Tram is an academic researcher from Aarhus University. The author has contributed to research in topics: Neutrino & Dark matter. The author has an hindex of 31, co-authored 77 publications receiving 5270 citations. Previous affiliations of Thomas Tram include Institute of Cosmology and Gravitation, University of Portsmouth & École Polytechnique Fédérale de Lausanne.

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The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes

TL;DR: Three approximations used by CLASS for basic �CDM models are described, namely: a baryon-photon tight-coupling approximation which can be set to first order, second order or to a compromise between the two; an ultra-relativistic fluid approximation which had not been implemented in public distributions before; and finally a radiation streaming approximation taking reionisation into account.
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The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

TL;DR: In this article, the newly released code CLASS (Cosmic Linear Anisotropy Solving System) incorporates improved approximation schemes leading to a simultaneous gain in speed and precision, namely a baryon-photon tight-coupling approximation which can be set to first order, second order or to a compromise between the two.
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The Cosmic Linear Anisotropy Solving System (CLASS) IV: efficient implementation of non-cold relics

TL;DR: In this article, the authors present a new flexible, fast and accurate way to implement massive neutrinos, warm dark matter and any other non-cold dark matter relics in Boltzmann codes.
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How Self-Interactions can Reconcile Sterile Neutrinos with Cosmology

TL;DR: It is shown that new interactions in the sterile neutrino sector can prevent their production in the early Universe and reconcile short baseline oscillation experiments with cosmology.
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Reconciling CMB and structure growth measurements with dark energy interactions

TL;DR: In this article, a coupled quintessence model with pure momentum exchange was proposed and the effects of such an interaction on the cosmic microwave background (CMB) and matter power spectrum were investigated.