How Can the Statistical Properties of Cosmic Structures Be Calculated with Simple Physical Laws?
DOI:
https://doi.org/10.21036/LTPUB10453Researcher
Matthias Bartelmann is Full Professor of Theoretical Astrophysics at Heidelberg University. He is also Spokesman of the Commission for Research and Strategy at the same institution. From 2008 to 2016, he was board member of the German Physical Society. His current research interests include galaxy clusters, cosmology, and gravitational lenses. Both in 2008 and 2016, he was awarded the Teaching Prize of the Department of Physics and Astronomy of Heidelberg University.

Original Publication
A Microscopic, Non-equilibrium, Statistical Field Theory for Cosmic Structure Formation
Matthias Bartelmann
,Felix Fabis
,Daniel Berg
,Elena Kozlikin
,Robert Lilow
,Published in 2016
Kinetic Field Theory: Effects of Momentum Correlations on the Cosmic Density-fluctuation Power Spectrum
Matthias Bartelmann
,Felix Fabis
,Elena Kozlikin
,Robert Lilow
,Johannes Dombrowski
,Published in 2017
