How Can the Statistical Properties of Cosmic Structures Be Calculated with Simple Physical Laws?

Abstract information

So far, the understanding we have of cosmic structures comes from numerical simulations. As MATTHIAS BARTELMANN explains in this video, his research group has developed a different method to calculate the statistical properties of cosmic structures in order to better understand why they evolve in the way they do. The researchers employed concepts of statistical field theory and could therefore use much simpler dynamical equations. They applied this new approach to describe the power spectrum of cosmic structures, i.e. the degree to which cosmic matter clusters. They thus obtained the same results as the numerical simulations, but in a much simpler way that saves considerable amounts of computation time, reducing it from months to a matter of seventy seconds. This will allow researchers to gain a much better understanding of the formation of cosmic structures in a feasible amount of time.

DOI:

https://doi.org/10.21036/LTPUB10453

Researcher

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.

Institution information

Heidelberg University (Ruprecht-Karls-Universität Heidelberg)

“Heidelberg University, founded in 1386, is Germany’s oldest university and one of the strongest research universities in all of Europe. The successes in both rounds of the Excellence Initiative and in internationally recognised rankings prove that Heidelberg’s excellent reputation and leading role in the scientific community are well deserved. In terms of educating students and promoting promising early-career academics, Heidelberg relies on research-based teaching and an outstanding, well-structured training for doctoral candidates. Heidelberg University is a comprehensive university, offering the full spectrum of disciplines in the humanities, law and the social sciences alongside the natural and life sciences, including medicine. As a comprehensive university, Heidelberg aims to continue to strengthen the individual disciplines and to further interdisciplinary cooperation, as well as to carry research results over into society and industry. With its aspiration of connecting traditional values with future-oriented scientific concepts in research and teaching, the university is building bridges to the future – Zukunft. Seit 1386.” ( Source )
Heidelberg University (Ruprecht-Karls-Universität Heidelberg)

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

Kinetic Field Theory: Effects of Momentum Correlations on the Cosmic Density-fluctuation Power Spectrum

Citation

Matthias Bartelmann, 

Latest Thinking, 

How Can the Statistical Properties of Cosmic Structures Be Calculated with Simple Physical Laws?, 

https://doi.org/10.21036/LTPUB10453, 

Credits:

© Matthias Bartelmann

and Latest Thinking

This work is licensed under CC-BY 4.0