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arXiv · 2311.04856

The High Energy X-ray Probe (HEX-P): Sensitive broadband X-ray observations of transient phenomena in the 2030s

Murray Brightman·Raffaella Margutti·Ava Polzin·Amruta Jaodand·Kenta Hotokezaka·Jason A. J. Alford·Gregg Hallinan·Elias Kammoun·Kunal Mooley·Megan Masterson·Lea Marcotulli·Arne Rau·George A. Younes·Daniel Stern·Javier A. García·Kristin Madsen
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Abstract

HEX-P will launch at a time when the sky is being routinely scanned for transient gravitational wave, electromagnetic and neutrino phenomena that will require the capabilities of a sensitive, broadband X-ray telescope for follow up studies. These include the merger of compact objects such as neutron stars and black holes, stellar explosions, and the birth of new compact objects. \hexp\ will probe the accretion and ejecta from these transient phenomena through the study of relativistic outflows and reprocessed emission, provide unique capabilities for understanding jet physics, and potentially revealing the nature of the central engine.

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Murray Brightman, Raffaella Margutti, Ava Polzin, Amruta Jaodand, Kenta Hotokezaka, Jason A. J. Alford, Gregg Hallinan, Elias Kammoun, Kunal Mooley, Megan Masterson, Lea Marcotulli, Arne Rau, George A. Younes, Daniel Stern, Javier A. García, Kristin Madsen. 2023-11-08. The High Energy X-ray Probe (HEX-P): Sensitive broadband X-ray observations of transient phenomena in the 2030s. https://arxiv.org/abs/2311.04856

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