@article {21706,
	title = {Neutrinos, Cosmic Rays, and the MeV Band},
	volume = {51},
	year = {2019},
	month = {2019/05/1},
	pages = {431},
	abstract = {The Mev band holds the key to answering three astrophysical questions: the sites where cosmic Rays are produced and accelerated, the origins of high- energy neutrinos, and the physical mechanisms producing the high energy gamma- ray emission from blazars. Theoretical and experimental capabilities needed in the next decade are discussed.},
	keywords = {Astrophysics - High Energy Astrophysical Phenomena},
	url = {https://ui.adsabs.harvard.edu/abs/2019BAAS...51c.431O},
	author = {Ojha, Roopesh and Zhang, Haocheng and Kadler, Matthias and Neilson, Naoko K. and Kreter, Michael and McEnery, J. and Buson, S. and Caputo, R. and Coppi, P. and D{\textquoteright}Ammando, F. and De Angelis, A. and Fang, K. and Giannios, D. and Guiriec, S. and Guo, F. and Kopp, J. and Krauss, F. and Li, H. and Meyer, M. and Moiseev, A. and Petropoulou, M. and Prescod-Weinstein, C. and Rani, B. and Shrader, C. and Venters, T. and Wadiasingh, Z.}
}
