activity
20032026
most citedConstraining the population of cosmic ray protons in cooling flow clusters with gamma-ray and radio observations: Are radio mini-halos of hadronic origin?

282 citations · 9.3k across the 182 of their papers we have counts for

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Showing 2018 · astro-ph.HEShow all

5 papers · 2 filters

astro-ph.HE2018★ 20 cited

The Sunyaev-Zel'dovich effect of simulated jet-inflated bubbles in clusters

Kristian Ehlert, Christoph Pfrommer, Rainer Weinberger +2

Feedback by active galactic nuclei (AGNs) is essential for regulating the fast radiative cooling of low-entropy gas at the centers of galaxy clusters and for reducing star formatio…

astro-ph.HE2018★ 48 cited

Missing Gamma-ray Halos and the Need for New Physics in the Gamma-ray Sky

Avery E. Broderick, Paul Tiede, Philip Chang +5

An intergalactic magnetic field stronger than ~G would explain the lack of a bright, extended degree-scale, GeV-energy inverse Compton component in the gamma-ray s…

astro-ph.HE2018★ 13 cited

Constraining the coherence scale of the interstellar magnetic field using TeV gamma-ray observations of supernova remnants

Matteo Pais, Christoph Pfrommer, Kristian Ehlert +2

Galactic cosmic rays (CRs) are believed to be accelerated at supernova remnant (SNR) shocks. In the hadronic scenario the TeV gamma-ray emission from SNRs originates from decaying…

astro-ph.HE2018★ 39 cited

The effect of cosmic-ray acceleration on supernova blast wave dynamics

M. Pais, C. Pfrommer, K. Ehlert +1

Non-relativistic shocks accelerate ions to highly relativistic energies provided that the orientation of the magnetic field is closely aligned with the shock normal (quasi-parallel…

astro-ph.HE2018★ 29 cited

Growth of beam-plasma instabilities in the presence of background inhomogeneity

Mohamad Shalaby, Avery E. Broderick, Philip Chang +3

We explore how inhomogeneity in the background plasma number density alters the growth of electrostatic unstable wavemodes of beam plasma systems. This is particularly interesting…