activity
20122024
most citedThe Effect of Nonlinear Landau Damping on Ultrarelativistic Beam Plasma Instabilities

55 citations · 118 across the 7 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2024

The theory of resonant cosmic ray-driven instabilities -- Growth and saturation of single modes

Rouven Lemmerz, Mohamad Shalaby, Christoph Pfrommer +1

Cosmic ray (CR) feedback is critical for galaxy formation as CRs drive galactic winds, regularize star formation in galaxies, and escape from active galactic nuclei to heat the coo…

astro-ph.HE20231 cited

Coupling multi-fluid dynamics equipped with Landau closures to the particle-in-cell method

Rouven Lemmerz, Mohamad Shalaby, Timon Thomas +1

The particle-in-cell (PIC) method is successfully used to study magnetized plasmas. However, this requires large computational costs and limits simulations to short physical run-ti…

astro-ph.HE201638 cited

The Linear Instability of Dilute Ultrarelativistic Pair Beams

Philip Chang, Avery E. Broderick, Christoph Pfrommer +4

The annihilation of TeV photons from extragalactic TeV sources and the extragalactic background light produces ultrarelativistic beams, which are subject to powerful plas…

astro-ph.HE201620 cited

Bow Ties in the Sky I: The Angular Structure of Inverse Compton Gamma-ray Halos in the Fermi Sky

Avery E. Broderick, Paul Tiede, Mohamad Shalaby +4

Extended inverse Compton halos are generally anticipated around extragalactic sources of gamma rays with energies above 100 GeV. These result from inverse Compton scattered cosmic…

astro-ph.HE201455 cited

The Effect of Nonlinear Landau Damping on Ultrarelativistic Beam Plasma Instabilities

Philip Chang, Avery E. Broderick, Christoph Pfrommer +3

Very-high energy gamma-rays from extragalactic sources pair-produce off of the extragalactic background light, yielding an electron-positron pair beam. This pair beam is unstable t…

gr-qc20121 cited

Dynamics and Light Propagation in a Universe with Discrete Matter Content

Mohamad Shalaby

We discuss a model for a universe with discrete matter content instead of the continuous perfect fluid taken in FRW models. We show how the redshift in such a universe deviates fro…