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20242026
most citedNon-thermal emission from mildly relativistic dynamical ejecta of neutron star mergers: spectrum and sky image

9 citations · 27 across the 10 of their papers we have counts for

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astro-ph.HE2024★ 1 cited

The non-thermal emission following GW170817 is consistent with a conical radially-stratified outflow with initial Lorentz factor

Gilad Sadeh, Eli Waxman

We show that the non-thermal radio to X-ray emission following the neutron star merger GW170817 is consistent with synchrotron emission from a collisionless shock driven into the i…

astro-ph.HE2024

Shock cooling emission from explosions of massive stars: III. Blue Super Giants

J. Morag, N. Sapir, E. Waxman

Light emission in the first hours and days following core-collapse supernovae is dominated by the escape of photons from the expanding shock-heated envelope. In preceding papers, w…

astro-ph.HE2024★ 9 cited

The thermalization of -rays in radioactive expanding ejecta: A simple model and its application for Kilonovae and Ia SNe

Or Guttman, Ben Shenhar, Arnab Sarkar +1

A semi-analytic approximation is derived for the time-dependent fraction of the energy deposited by radioactive decay -rays in a homologously expanding plasma of genera…

astro-ph.HE2024★ 4 cited

An Analytic Description of Electron Thermalization in Kilonovae Ejecta

Ben Shenhar, Or Guttman, Eli Waxman

A simple analytic description is provided of the rate of energy deposition by -decay electrons in the homologously expanding radioactive plasma ejected in neutron star mergers,…

astro-ph.HE2024★ 9 cited

Non-thermal emission from mildly relativistic dynamical ejecta of neutron star mergers: spectrum and sky image

Gilad Sadeh, Noya Linder, Eli Waxman

Binary neutron star mergers are expected to produce fast dynamical ejecta, with mildly relativistic velocities extending to . In a preceding paper, we derived an analyti…