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Multi-messenger astrophysics with THESEUS in the 2030s

Ciolfi, R; Stratta, G; Branchesi, M; Gendre, B; Grimm, S; Harms, J; Lamb, GP; ... Zhang, B; + view all (2021) Multi-messenger astrophysics with THESEUS in the 2030s. Experimental Astronomy 10.1007/s10686-021-09795-9. (In press). Green open access

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Abstract

Multi-messenger astrophysics is becoming a major avenue to explore the Universe, with the potential to span a vast range of redshifts. The growing synergies between different probes is opening new frontiers, which promise profound insights into several aspects of fundamental physics and cosmology. In this context, THESEUS will play a central role during the 2030s in detecting and localizing the electromagnetic counterparts of gravitational wave and neutrino sources that the unprecedented sensitivity of next generation detectors will discover at much higher rates than the present. Here, we review the most important target signals from multi-messenger sources that THESEUS will be able to detect and characterize, discussing detection rate expectations and scientific impact.

Type: Article
Title: Multi-messenger astrophysics with THESEUS in the 2030s
Open access status: An open access version is available from UCL Discovery
DOI: 10.1007/s10686-021-09795-9
Publisher version: https://doi.org/10.1007/s10686-021-09795-9
Language: English
Additional information: This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
Keywords: Multi-messenger astrophysics, Gamma-ray burst, Compact binary merger, Kilonova, X-ray sources, Neutrino sources
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10137899
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