activity
20172020
most citedTopological signatures of interstellar magnetic fields - I. Betti numbers and persistence diagrams

18 citations · 35 across the 2 of their papers we have counts for

collaborators

8 papers

astro-ph.GA202017 cited

Magnetic fields in elliptical galaxies: an observational probe of the fluctuation dynamo action

Amit Seta, Luiz Felippe S. Rodrigues, Christoph Federrath +1

Fluctuation dynamos are thought to play an essential role in magnetized galaxy evolution, saturating within Gyr and thus potentially acting as seeds for large-scale dyna…

astro-ph.IM2020

The Pencil Code, a modular MPI code for partial differential equations and particles: multipurpose and multiuser-maintained

A. Brandenburg, A. Johansen, P. A. Bourdin +34

The Pencil Code is a highly modular physics-oriented simulation code that can be adapted to a wide range of applications. It is primarily designed to solve partial differential equ…

astro-ph.CO2020

Redshift estimates for fast radio bursts and implications on intergalactic magnetic fields

Stefan Hackstein, Marcus Brüggen, Franco Vazza +1

Context: Fast Radio Bursts are transient radio pulses from presumably compact stellar sources of extragalactic origin. With new telescopes detecting multiple events per day, statis…

astro-ph.GA2018

Evolution of galactic magnetic fields

Luiz Felippe S. Rodrigues, Luke Chamandy, Anvar Shukurov +2

We study the cosmic evolution of the magnetic fields of a large sample of spiral galaxies in a cosmologically representative volume by employing a semi-analytic galaxy formation mo…

astro-ph.HE2018

Fickian and non-Fickian diffusion of cosmic rays

L. F. S. Rodrigues, A. P. Snodin, G. R. Sarson +1

Fluid approximations to cosmic ray (CR) transport are often preferred to kinetic descriptions in studies of the dynamics of the interstellar medium (ISM) of galaxies, because they…

astro-ph.GA2018

A physical approach to modelling large-scale galactic magnetic fields

Anvar Shukurov, Luiz Felippe S. Rodrigues, Paul J. Bushby +2

A convenient representation of the structure of the large-scale galactic magnetic field is required for the interpretation of polarization data in the sub-mm and radio ranges, in b…