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Detecting Planet 9 via Hawking radiation by Arbey, Alexandre; Auffinger, Jérémy is a scholarly article available to read on EtoBox.

What is Detecting Planet 9 via Hawking radiation about?

Concordant evidence points towards the existence of a ninth planet in the Solar System at more than $400\,$AU from the Sun. In particular, trans-Neptunian object orbits are perturbed by the presence of a putative gravitational source. Since this planet has not yet been observationally found with conventional telescope research, it has been argued that it could be a dark compact object, namely a black hole of probably primordial origin. Within this assumption, we discuss the possibility of detecting Planet 9 via a sub-relativistic spacecraft fly-by and the measure of its Hawking radiation in the radio band and conclude that it is too faint compared to the CMB. We thus present other perspectives with rather a satellite mission and conclude that smaller black holes would give much more interesting signals. We emphasize the importance of the study of such Hawking radiation laboratories in the Solar System.

Author

Arbey, Alexandre; Auffinger, Jérémy

Published

2020

Language

EN