Multimessenger Astronomy with Neutrinos
arXiv:2110.11817 · doi:10.3390/universe7110397
Abstract
Multimessenger astronomy is arguably the branch of the astroparticle physics field that has seen the most significant developments in recent years. In this manuscript, we will review the state-of-the-art, the recent observations, and the prospects and challenges for the near future. We will give special emphasis to the observation carried out with neutrino telescopes.
12 pages, 3 figures, review for Universe journal
References in corpus (11)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Multi-messenger Observations of a Binary Neutron Star Merger
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV
- Time-integrated Neutrino Source Searches with 10 years of IceCube Data
- The contribution of Fermi-2LAC blazars to the diffuse TeV-PeV neutrino flux
- First Detection of sub-PeV Diffuse Gamma Rays from the Galactic Disk: Evidence for Ubiquitous Galactic Cosmic Rays beyond PeV Energies
- The diffuse -ray background is dominated by star-forming galaxies
- Astro-COLIBRI -- The COincidence LIBrary for Real-time Inquiry for multimessenger astrophysics
- ANTARES search for point-sources of neutrinos using astrophysical catalogs: a likelihood stacking analysis
- Multi-messenger and real-time astrophysics with the Baikal-GVD telescope