activity
20112026
most citedMach Number Dependence of Turbulent Magnetic Field Amplification: Solenoidal versus Compressive Flows

249 citations · 1.7k across the 41 of their papers we have counts for

collaborators

41 papers

physics.flu-dyn2026

No evidence of vorticity production from irrotational turbulent gravitational collapse yet

Axel Brandenburg, Evangelia Ntormousi, Jennifer Schober

Gravitational collapse creates large amounts of kinetic energy that could potentially seed turbulence. If such turbulence were also suitable to initiate dynamo action, the resultin…

astro-ph.CO2026

Relativistic Chiral MHD with application to the early Universe

Deepen Garg, Jennifer Schober

We present a systematic derivation of the equations of relativistic chiral magnetohydrodynamics (MHD) for a plasma of charged fermions in an expanding universe. Through a combinati…

astro-ph.CO2026

A charge-flow instability in plasmas with charge fluctuations

Deepen Garg, Jennifer Schober

We present a linear instability in magnetized plasmas with charge fluctuations. It is driven by an electric current proportional to the charge chemical potential and the bulk v…

physics.plasm-ph2024★ 1 cited

Efficiency of dynamos from an autonomous generation of chiral asymmetry

Jennifer Schober, Igor Rogachevskii, Axel Brandenburg

At high energies, the dynamics of a plasma with charged fermions can be described in terms of chiral magnetohydrodynamics. Using direct numerical simulations, we demonstrate that c…

astro-ph.GA2023★ 8 cited

Iterative removal of sources to model the turbulent electromotive force

Abhijit B. Bendre, Jennifer Schober, Prasun Dhang +1

We describe a novel method to compute the components of dynamo tensors from direct magnetohydrodynamic (MHD) simulations. Our method relies upon an extension and generalisation of…

physics.plasm-ph2023★ 9 cited

Chiral anomaly and dynamos from inhomogeneous chemical potential fluctuations

Jennifer Schober, Igor Rogachevskii, Axel Brandenburg

In the standard model of particle physics, the chiral anomaly can occur in relativistic plasmas and plays a role in the early Universe, protoneutron stars, heavy-ion collisions, an…

astro-ph.CO2023★ 9 cited

The effect of pressure-anisotropy-driven kinetic instabilities on magnetic field amplification in galaxy clusters

Y. Rappaz, J. Schober

The intracluster medium (ICM) is the low-density diffuse magnetized plasma in galaxy clusters, which reaches virial temperatures of up to 10^8 K. Under these conditions, the plasma…

hep-ph2023★ 14 cited

Chiral magnetohydrodynamics with zero total chirality

Axel Brandenburg, Kohei Kamada, Kyohei Mukaida +2

We study the evolution of magnetic fields coupled with chiral fermion asymmetry in the framework of chiral magnetohydrodynamics with zero initial total chirality. The initial magne…

astro-ph.GA2023★ 1 cited

Small-scale dynamo with finite correlation times

Yann Carteret, Dominik Schleicher, Jennifer Schober

Fluctuation dynamos occur in most turbulent plasmas in astrophysics and are the prime candidates for amplifying and maintaining cosmic magnetic fields. A few analytical models exis…

physics.plasm-ph2023★ 14 cited

Decay law of magnetic turbulence with helicity balanced by chiral fermions

Axel Brandenburg, Kohei Kamada, Jennifer Schober

In plasmas composed of massless electrically charged fermions, chirality can be interchanged with magnetic helicity while preserving the total chirality through the quantum chiral…

astro-ph.GA2022★ 12 cited

Dissipative magnetic structures and scales in small-scale dynamos

A. Brandenburg, I. Rogachevskii, J. Schober

Small-scale dynamos play important roles in modern astrophysics, especially on Galactic and extragalactic scales. Owing to dynamo action, purely hydrodynamic Kolmogorov turbulence…

astro-ph.GA2022★ 2 cited

Observational Signatures of Galactic Turbulent Dynamos

Yann Carteret, Abhijit B. Bendre, Jennifer Schober

We analyse the observational signatures of galactic magnetic fields that are self-consistently generated in magnetohydrodynamic simulations of the interstellar medium through turbu…

astro-ph.GA2022★ 3 cited

Rotation measure and synchrotron emission signatures in simulations of magnetized galactic discs

Yoan Rappaz, Jennifer Schober, Philipp Girichidis

We analyse observational signatures of magnetic fields for simulations of a Milky-Way like disc with supernova-driven interstellar turbulence and self-consistent chemical processes…

physics.plasm-ph2021★ 14 cited

Dynamo instabilities in plasmas with inhomogeneous chiral chemical potential

Jennifer Schober, Igor Rogachevskii, Axel Brandenburg

We study the dynamics of magnetic fields in chiral magnetohydrodynamics, which takes into account the effects of an additional electric current related to the chiral magnetic effec…

physics.plasm-ph2021★ 20 cited

Production of a chiral magnetic anomaly with emerging turbulence and mean-field dynamo action

Jennifer Schober, Igor Rogachevskii, Axel Brandenburg

In relativistic magnetized plasmas, asymmetry in the number densities of left- and right-handed fermions, i.e., a non-zero chiral chemical potential mu_5, leads to an electric curr…

astro-ph.CO2021★ 30 cited

Relic gravitational waves from the chiral magnetic effect

Axel Brandenburg, Yutong He, Tina Kahniashvili +2

Relic gravitational waves (GWs) can be produced by primordial magnetic fields. However, not much is known about the resulting GW amplitudes and their dependence on the details of t…

astro-ph.GA2020★ 130 cited

The infrared-radio correlation of star-forming galaxies is strongly M-dependent but nearly redshift-invariant since z4

I. Delvecchio, E. Daddi, M. T. Sargent +25

Several works in the past decade have used the ratio between total (rest 8-1000m) infrared and radio (rest 1.4~GHz) luminosity in star-forming galaxies (q), often referre…

astro-ph.IM2020★ 192 cited

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.GA2020★ 35 cited

Constraining the primordial magnetic field with dwarf galaxy simulations

Mahsa Sanati, Yves Revaz, Jennifer Schober +2

Using a set of cosmological hydro-dynamical simulations, we constrained the properties of primordial magnetic fields by studying their impact on the formation and evolution of dwar…

physics.plasm-ph2020★ 18 cited

Generation of chiral asymmetry via helical magnetic fields

Jennifer Schober, Tomohiro Fujita, Ruth Durrer

It is well known that helical magnetic fields undergo a so-called inverse cascade by which their correlation length grows due to the conservation of magnetic helicity in classical…

astro-ph.SR2019★ 10 cited

Magneto-hydrodynamical origin of eclipsing time variations in post-common-envelope binaries for solar mass secondaries

Felipe H. Navarrete, Dominik R. G. Schleicher, Petri J. Käpylä +3

Eclipsing time variations have been observed for a wide range of binary systems, including post-common-envelope binaries. A frequently proposed explanation, apart from the possibil…

physics.plasm-ph2018★ 25 cited

Chiral fermion asymmetry in high-energy plasma simulations

Jennifer Schober, Axel Brandenburg, Igor Rogachevskii

The chiral magnetic effect (CME) is a quantum relativistic effect that describes the appearance of an additional electric current along a magnetic field. It is caused by an asymmet…

physics.flu-dyn2018★ 14 cited

Energetics of turbulence generated by chiral MHD dynamos

Jennifer Schober, Axel Brandenburg, Igor Rogachevskii +1

An asymmetry in the number density of left- and right-handed fermions is known to give rise to a new term in the induction equation that can result in a dynamo instability. At high…

physics.flu-dyn2017★ 67 cited

Laminar and turbulent dynamos in chiral magnetohydrodynamics. II. Simulations

Jennifer Schober, Igor Rogachevskii, Axel Brandenburg +4

Using direct numerical simulations (DNS), we study laminar and turbulent dynamos in chiral magnetohydrodynamics (MHD) with an extended set of equations that accounts for an additio…