Bulletin of the American Physical Society
2024 APS April Meeting
Wednesday–Saturday, April 3–6, 2024; Sacramento & Virtual
Session G03: Particle Astrophysics and the Galactic Center
10:45 AM–12:33 PM,
Thursday, April 4, 2024
SAFE Credit Union Convention Center
Room: Ballroom A4, Floor 2
Sponsoring
Unit:
DAP
Chair: Erika Holmbeck, LLNL
Abstract: G03.00007 : POEMMA-Balloon with radio: A balloon born Multi-Messenger Multi-Detector Observatory
11:57 AM–12:09 PM
Presenter:
Johannes Eser
(University of Chicago)
Authors:
Johannes Eser
(University of Chicago)
Angela V Olinto
(University of Chicago)
Giuseppe Osteria
(Istituto Nazionale di Fisica Nucleare - Sezione di Napoli)
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is a proposed dual-satellite mission with the goal of observing Ultra-High-Energy Cosmic Rays (UHECRs) to increase the statistics at the highest energies and Very-High-Energy Neutrinos (VHENs) following multi-messenger alerts of astrophysical transient events, such as gamma-ray bursts and gravitational wave events, throughout the universe.
POEMMA-Balloon with radio (PBR) is a small-scale version of the POEMMA design, adapted to be flown as a payload on one of NASA's suborbital Super Pressure Balloons (SPBs) circling over the Southern Ocean for up to 100 days after a launch from Wanaka, New Zealand.
The main science objectives of PBR are: (1) to observe UHECRs via the fluorescence technique from suborbital space; (2) to observe horizontal high-altitude air showers (HAHAs) with energies above the cosmic ray knee (E>3PeV) using the optical and radio detection for the first time; and (3) to follow astrophysical event alerts in the search of VHENs.
This overview will provide a brief summary of the mission with its science goals, the instruments and the current status of PBR.
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