Chapter 6 Multimessenger Physics *

Abstract

Combining observations of multi-messengers help in boosting the sensitivity of astrophysical source searches, and probe various aspects of the source physics. In this chapter we discuss how LHAASO observations of very high energy (VHE) gamma rays in combination with telescopes for the other messengers can help in solving the origins of VHE neutrinos and galactic and extragalactic cosmic rays.

Highlights from the Large High-Altitude Air-Shower Observatory (LHAASO)

“…It is also evident how LHAASO will be the most sensitive instrument above 50 TeV for the next decades. A broad overview of the Physics potential of LHAASO can be found in the LHAASO science book, a special issue of the Chinese Physics C, released in 2021 where all science topics are discussed as Galactic [2] and Extra-galactic Physics [3], Cosmic rays Physics [4], Dark Matter and BSM Physics [5], Multi-messenger astronomy [6], and Solar and Heliosphere Physics [7].…”

Highlights from the Large High-Altitude Air-Shower Observatory (LHAASO)

“…A detailed overview of the Physics potential of LHAASO can be found in the special issue of the Chinese Physics released in 2021 where all science topics are discussed, as Galactic [2] and Extragalactic Physics [3], Cosmic rays Physics [4], Dark Matter and BSM Physics [5], Multi-messenger astronomy [6], and Solar and Heliosphere Physics [7].…”