The Advanced Particle-astrophysics Telescope (APT) Project Status

Authors

James H. Buckley, Washington University in St. Louis
S. Alnussirat, Louisiana State University
C. Altomare, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
R. G. Bose, McDonnell Center for the Space Sciences
D. Braun, McDonnell Center for the Space Sciences
J. D. Buhler, McKelvey School of Engineering
E. Burns, Louisiana State University
R. D. Chamberlain, McKelvey School of Engineering
W. Chen, College of Science and Engineering
M. L. Cherry, Louisiana State University
L. Di Venere, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
J. Dumonthier, NASA Goddard Space Flight Center
M. Errando, McDonnell Center for the Space Sciences
S. Funk, Friedrich-Alexander-Universität Erlangen-Nürnberg
F. Giordano, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
J. Hoffman, McDonnell Center for the Space Sciences
Z. Hughes, McDonnell Center for the Space Sciences
D. J. Huth, McDonnell Center for the Space Sciences
P. L. Kelly, College of Science and Engineering
J. F. Krizmanic, College of Engineering and Information Technology
M. Kuwahara, University of Hawaiʻi at Mānoa
F. Licciulli, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
G. Liu, University of Hawaiʻi at Mānoa
M. N. Mazziotta, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
J. G. Mitchell, The George Washington University
J. W. Mitchell, College of Engineering and Information Technology
G. A. de Nolfo, NASA Goddard Space Flight Center
R. Paoletti, Università degli Studi di Siena
R. Pillera, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
B. F. Rauch, McDonnell Center for the Space Sciences
D. Serini, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
G. Simburger, McDonnell Center for the Space Sciences
M. Sudvarg, McKelvey School of Engineering

Document Type

Conference Proceeding

Publication Date

3-18-2022

Abstract

We describe the development of a future gamma-ray/cosmic-ray mission called the Advanced Particle-astrophysics Telescope (APT). The instrument will combine a pair tracker and Compton telescope in a single monolithic design. By using scintillating fibers for the tracker and wavelength-shifting fibers to readout CsI detectors, the instrument will achieve an order of magnitude improvement in sensitivity compared with Fermi but with fewer readout channels, and lower complexity. By incorporating multiple Compton imaging over a very large effective area, the instrument will also achieve orders of magnitude improvement in MeV sensitivity compared with other proposed instruments. The mission would have a broad impact on astroparticle physics, but the primary science drivers for the mission include: (1) probing WIMP dark matter across the entire natural mass range and annihilation cross section for a thermal WIMP, (2) providing a nearly all-sky instantaneous FoV, with prompt sub-degree localization and polarization measurements for gamma-ray transients such as neutron-star mergers and (3) making measurements of rare utraheavy cosmic ray nuclei to distinguish between n-star merger and SNae r-process synthesis of the heavy elements. We will describe ongoing work including a series of accelerator beam tests, a piggy-back Antactic flight (APTlite) and the recently funded long-duration balloon mission: the Antarctic Demonstrator for APT (ADAPT).

Publication Source (Journal or Book title)

Proceedings of Science

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