THESEUS: a key space mission concept for Multi-Messenger Astrophysics
G. Stratta, R. Ciolfi, L. Amati, G. Ghirlanda, N. Tanvir, E. Bozzo, D., Gotz, P. O'Brien, F. Frontera, J. P. Osborne, L. Rezzolla, A. Rossi, E., Maiorano, S. Vinciguerra, C. Guidorzi, A. Drago, L. Nicastro, E. Palazzi, M., Branchesi, M. Boer, E. Brocato, A. Bulgarelli, S. Covino

TL;DR
THESEUS is a proposed space mission designed to significantly advance multi-messenger astrophysics by detecting high-frequency gravitational waves and neutrinos, complementing future ground and space telescopes for early Universe and transient event studies.
Contribution
The paper introduces the THESEUS mission concept, highlighting its potential to enhance multi-messenger astronomy and early Universe science in synergy with upcoming gravitational wave and neutrino detectors.
Findings
Identification of promising high-frequency gravitational wave sources.
Expected synergy between THESEUS and future multi-messenger detectors.
Potential for groundbreaking discoveries in early Universe phenomena.
Abstract
The recent discovery of the electromagnetic counterpart of the gravitational wave source GW170817, has demonstrated the huge informative power of multi-messenger observations. During the next decade the nascent field of multi-messenger astronomy will mature significantly. Around 2030, third generation gravitational wave detectors will be roughly ten times more sensitive than the current ones. At the same time, neutrino detectors currently upgrading to multi km^3 telescopes, will include a 10 km^3 facility in the Southern hemisphere that is expected to be operational around 2030. In this review, we describe the most promising high frequency gravitational wave and neutrino sources that will be detected in the next two decades. In this context, we show the important role of the Transient High Energy Sky and Early Universe Surveyor (THESEUS), a mission concept proposed to ESA by a large…
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