Neutral pion emission from accelerated protons in the supernova remnant W44
A. Giuliani, M. Cardillo, M. Tavani, Y. Fukui, S. Yoshiike, K. Torii,, G. Dubner, G. Castelletti, G. Barbiellini, A. Bulgarelli, P. Caraveo, E., Costa, P. W. Cattaneo, A. Chen, T. Contessi, E. Del Monte, I. Donnarumma, Y., Evangelista, M. Feroci, F. Gianotti, F. Lazzarotto

TL;DR
This study uses AGILE gamma-ray observations to confirm that neutral pion decay from accelerated protons is the primary source of gamma-ray emission in supernova remnant W44, providing direct evidence of hadronic cosmic-ray production.
Contribution
First direct evidence of pion emission in an SNR, confirming hadronic origin of gamma rays and detailing the proton energy spectrum in W44.
Findings
Gamma-ray emission aligns with the SNR shocked plasma.
Spectrum shows a peak near 1 GeV consistent with pion decay.
Hadron-dominated models fit all multiwavelength data.
Abstract
We present the AGILE gamma-ray observations in the energy range 50 MeV - 10 GeV of the supernova remnant (SNR) W44, one of the most interesting systems for studying cosmic-ray production. W44 is an intermediate-age SNR (20, 000 years) and its ejecta expand in a dense medium as shown by a prominent radio shell, nearby molecular clouds, and bright [SII] emitting regions. We extend our gamma-ray analysis to energies substantially lower than previous measurements which could not conclusively establish the nature of the radiation. We find that gamma-ray emission matches remarkably well both the position and shape of the inner SNR shocked plasma. Furthermore, the gamma-ray spectrum shows a prominent peak near 1 GeV with a clear decrement at energies below a few hundreds of MeV as expected from neutral pion decay. Here we demonstrate that: (1) hadron-dominated models are consistent with all…
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