activity
19962011
most citedMagnetic Fields in Starburst Galaxies and The Origin of the FIR-Radio Correlation

228 citations · 1.2k across the 23 of their papers we have counts for

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Showing 2006 · astro-phShow all

6 papers · 2 filters

astro-ph200611 cited

Assessing The Starburst Contribution to the Gamma-Ray and Neutrino Backgrounds

Todd A. Thompson, Eliot Quataert, Eli Waxman +1

If cosmic ray protons interact with gas at roughly the mean density of the interstellar medium in starburst galaxies, then pion decay in starbursts is likely to contribute signific…

astro-ph200671 cited

Nonthermal gamma-ray and X-ray flashes from shock breakout in gamma-ray bursts/supernovae

Xiang-Yu Wang, Zhuo Li, Eli Waxman +1

Thermal X-ray emission which is simultaneous with the prompt gamma-rays has been detected for the first time from a supernova connected with a gamma-ray burst (GRB), namely GRB0602…

astro-ph200667 cited

Gamma-ray bursts and collisionless shocks

E. Waxman

Particle acceleration in collisionless shocks is believed to be responsible for the production of cosmic-rays over a wide range of energies, from few GeV to >10^{20}eV, as well as…

astro-ph2006161 cited

The Starburst Contribution to the Extra-Galactic Gamma-Ray Background

Todd A. Thompson, Eliot Quataert, Eli Waxman

Cosmic ray protons interacting with gas at the mean density of the interstellar medium in starburst galaxies lose energy rapidly via inelastic collisions with ambient nuclei. The r…

astro-ph2006228 cited

Magnetic Fields in Starburst Galaxies and The Origin of the FIR-Radio Correlation

Todd A. Thompson, Eliot Quataert, Eli Waxman +2

We estimate minimum energy magnetic fields (B_min) for a sample of galaxies with measured gas surface densities, spanning from normal spirals to starbursts. We show that the ratio…

astro-ph2006

The Cumulative Bakground of High-Energy Neutrinos from Starburst Galaxies

Abraham Loeb, Eli Waxman

We show that starburst galaxies convert efficiently cosmic-rays into pions, which in turn decay into high-energy neutrinos and photons. The cumulative background of GeV neutrinos i…