activity
20132025
most citedCosmic Structure Formation with Kinetic Field Theory

31 citations · 91 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2025

Free Cosmic Density Bispectrum on Small Scales

Ricardo Waibel, Sara Konrad, Matthias Bartelmann

We study the asymptotic behaviour of the free, cold-dark matter density fluctuation bispectrum in the limit of small scales. From an initially Gaussian random field, we draw phase-…

astro-ph.CO2025★ 5 cited

Gravitational Turbulence: the Small-Scale Limit of the Cold-Dark-Matter Power Spectrum

Yonadav Barry Ginat, Michael L. Nastac, Robert J. Ewart +3

The matter power spectrum, , is one of the fundamental quantities in the study of large-scale structure in cosmology. Here, we study its small-scale asymptotic limit, and sho…

astro-ph.CO2022★ 8 cited

Kinetic Field Theory for Cosmic Structure Formation

Sara Konrad, Matthias Bartelmann

We apply kinetic field theory to non-linear cosmic structure formation. Kinetic field theory decomposes the cosmic density field into particles and follows their trajectories throu…

astro-ph.CO2022★ 8 cited

On the asymptotic behaviour of cosmic density-fluctuation power spectra of cold dark matter

Sara Konrad, Yonadav Barry Ginat, Matthias Bartelmann

We study the small-scale asymptotic behaviour of the cold dark matter density fluctuation power spectrum in the Zel'dovich approximation, without introducing an ultraviolet cut-off…

astro-ph.CO2021★ 6 cited

On the asymptotic behaviour of cosmic density-fluctuation power spectra

Sara Konrad, Matthias Bartelmann

We study the small-scale asymptotic behaviour of the cosmic density-fluctuation power spectrum in the Zel'dovich approximation. For doing so, we extend Laplace's method in arbitrar…

math.CA2021

Asymptotic Expansion of Laplace-Fourier-Type Integrals

Sara Konrad, Matthias Bartelmann

We study the asymptotic behaviour of integrals of the Laplace-Fourier type with …

astro-ph.CO2020★ 2 cited

Kinetic field theory: Non-linear cosmic power spectra in the mean-field approximation

Matthias Bartelmann, Johannes Dombrowski, Sara Konrad +5

We use the recently developed Kinetic Field Theory (KFT) for cosmic structure formation to show how non-linear power spectra for cosmic density fluctuations can be calculated in a…

astro-ph.CO2019★ 31 cited

Cosmic Structure Formation with Kinetic Field Theory

Matthias Bartelmann, Elena Kozlikin, Robert Lilow +7

Kinetic Field Theory (KFT) is a statistical field theory for an ensemble of point-like classical particles in or out of equilibrium. We review its application to cosmological struc…

astro-ph.CO2017★ 1 cited

Analytic calculation of the non-linear cosmic density-fluctuation power spectrum in the Born approximation

Matthias Bartelmann, Felix Fabis, Sara Konrad +4

We derive a non-perturbative, closed, analytic equation for the non-linear power spectrum of cosmic density fluctuations. This result is based on our kinetic field theory (KFT) of…

astro-ph.CO2013★ 11 cited

Reconstructing the projected gravitational potential of galaxy clusters from galaxy kinematics

Eleonora Sarli, Sven Meyer, Massimo Meneghetti +3

We develop a method for reconstructing the two-dimensional, projected gravitational potential of galaxy clusters from observed line-of-sight velocity dispersions of cluster galaxie…

astro-ph.CO2013★ 4 cited

Joint reconstruction of galaxy clusters from gravitational lensing and thermal gas. II. Inversion of the thermal Sunyaev-Zel'dovich effect

Charles L. Majer, Sven Meyer, Sara Konrad +2

This paper continues a series in which we intend to show how all observables of galaxy clusters can be combined to recover the two-dimensional, projected gravitational potential of…

astro-ph.CO2013★ 15 cited

Joint reconstruction of galaxy clusters from gravitational lensing and thermal gas I. Outline of a non-parametric method

Sara Konrad, Charles L. Majer, Sven Meyer +2

We present a method to estimate the lensing potential from massive galaxy clusters for given observational X-ray data. The concepts developed and applied in this work can easily be…