SPACE AND COSMIC RAY PHYSICS SEMINAR

University of Maryland
Atlantic Building, Room 2400
4:30 PM Monday, April 10, 2017
Coffee, Tea & Snacks 4:15-4:30 PM

Alexander Moiseev
NASA Goddard Space Flight Center

Perspectives in MeV Astronomy:All-Sky Medium Energy Gamma-ray Observatory (AMEGO)

The gamma-ray energy range from a few hundred keV to a few hundred MeV has remained largely unexplored since the pioneering but limited observations by COMPTEL on the CGRO (1991-2000). Fundamental astrophysics questions can be addressed by a mission in the MeV range, from astrophysical jets and extreme physics of compact objects to a large population of unidentified objects. To address these questions, we are developing AMEGO: All-sky Medium Energy Gamma-ray Observatory, within the NASA Probe class mission, to investigate the energy range from 300 keV to >10 GeV with good energy (ranging from <1% at low end to ~10% at high end) and angular resolution (from 2 to 6 degrees depending on energy) and with sensitivity approaching a factor of 20-50 better than previous measurements. Measurements at these energies are challenging, mainly due to specifics of photon detection: it is a range where two processes of photon interaction, Compton scattering and pair production compete. These two interaction processes require different approaches in both detection and data analysis, and consequently in the instrument concept. AMEGO will be capable of measuring both Compton-scattering events at lower energies and pair-production events at higher energies. Also, AMEGO will have sensitivity to the linear polarization of detected radiation.