by Eric Burns, S. Zhu, C. M. Hui, S. Ansoldi, S. Barthelmy, S. Boggs, S. B. Cenko, N. Christensen, C. Fryer, A. Goldstein, A. Harding, D. Hartmann, A. Joens, G. Kanbach, M. Kerr, C. Kierans, J. McEnery, B. Patricelli, J. Perkins, J. Racusin, P. Ray, J. Schlieder, H. Schoorlemmer, F. Schussler, A. Stamerra, J. Tomsick, Z. Wadiasingh, C. Wilson-Hodge, G. Younes, B. Zhang, and A. Zoglauer
Published onMay 31, 2019
Gamma Rays and Gravitational Waves
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Abstract
The first multimessenger detection of a neutron star merger was independently detected in gamma-rays and gravitational waves. The two messengers will jointly identify new sources in the next few years, beyond neutron star mergers. We present a summary of possible sources and discuss the capabilities needed to study them.
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