NewEvery arXiv paper, its researchers & institutions — mapped.
papers

Publications (16)

astro-ph.CO2016

Constraining dark matter properties with Cosmic Microwave Background observations

Daniel B. Thomas, Michael Kopp, Constantinos Skordis

astro-ph.CO2014

Beyond single-stream with the Schrödinger method

Cora Uhlemann, Michael Kopp

astro-ph.CO2013

Spherical collapse and halo mass function in f(R) theories

Michael Kopp, Stephen A. Appleby, Ixandra Achitouv +1

cs.CY2016

Potential of EPUB3 for Digital Textbooks in Higher Education

Martin Ebner, Christian Gailer, Mohammad Khalil +3

physics.comp-ph2012

GPU-accelerated simulation of colloidal suspensions with direct hydrodynamic interactions

Michael Kopp, Felix Höfling

astro-ph.CO2015

Coarse-grained cosmological perturbation theory: stirring up the dust model

Cora Uhlemann, Michael Kopp

astro-ph.CO2018

The Dark Matter equation of state through cosmic history

Michael Kopp, Constantinos Skordis, Daniel B. Thomas +1

gr-qc2018

Dark energy after GW170817, revisited

Edmund J. Copeland, Michael Kopp, Antonio Padilla +2

astro-ph.CO2014

Newton to Einstein - dust to dust

Michael Kopp, Cora Uhlemann, Thomas Haugg

astro-ph.CO2016

An extensive investigation of the Generalised Dark Matter model

Michael Kopp, Constantinos Skordis, Dan B. Thomas

astro-ph.CO2014

Schrödinger method as N-body double and UV completion of dust

Cora Uhlemann, Michael Kopp, Thomas Haugg

astro-ph.CO2011

Separate Universes Do Not Constrain Primordial Black Hole Formation

Michael Kopp, Stefan Hofmann, Jochen Weller

astro-ph.CO2017

Solving the Vlasov equation in two spatial dimensions with the Schrödinger method

Michael Kopp, Kyriakos Vattis, Constantinos Skordis

astro-ph.CO2016

Choose to smooth: Gaussian streaming with the truncated Zel'dovich approximation

Michael Kopp, Cora Uhlemann, Ixandra Achitouv

astro-ph.CO2015

Edgeworth streaming model for redshift space distortions

Cora Uhlemann, Michael Kopp, Thomas Haugg

astro-ph.CO2012

Newtonian N-body simulations are compatible with cosmological perturbation theory

Thomas Haugg, Stefan Hofmann, Michael Kopp