Seeing into the immediate post-merger environment of a neutron star collision
APA
Tohuvavohu, A. (2023). Seeing into the immediate post-merger environment of a neutron star collision. Perimeter Institute. https://pirsa.org/23100105
MLA
Tohuvavohu, Aaron. Seeing into the immediate post-merger environment of a neutron star collision. Perimeter Institute, Oct. 20, 2023, https://pirsa.org/23100105
BibTex
@misc{ pirsa_PIRSA:23100105, doi = {10.48660/23100105}, url = {https://pirsa.org/23100105}, author = {Tohuvavohu, Aaron}, keywords = {Particle Physics}, language = {en}, title = {Seeing into the immediate post-merger environment of a neutron star collision}, publisher = {Perimeter Institute}, year = {2023}, month = {oct}, note = {PIRSA:23100105 see, \url{https://pirsa.org}} }
The rich EM phenomenology in the seconds, minutes, and hours just before, during, and after a compact object merger encodes the magnetization of the binary components, the nature of the post-merger remnant, the neutron star equation of state, the free neutron abundance, and a wide array of other compelling physics. Unfortunately, the requirement to search, find, and classify an electromagnetic counterpart within the large GW localization regions before targeted follow-up with sensitive instruments can begin, excludes access to these earliest times, even for the most well localized GW sources. The ability to promptly localize a GW source to within the field-of-view of a narrow-field sensitive facility, would enable extraordinary science. I will discuss the science cases that require extremely early time observations, and the coordination, instruments, and analyses necessary to achieve it. These include gamma-ray imaging, novel data analysis techniques, pre-merger GW detection, faster space telescopes, and new experiments.
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Zoom link https://pitp.zoom.us/j/96186614241?pwd=R0xpT0dDZVZzek5RT0x4Q1c3Z1RuUT09