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High-energy neutrino astronomy
Invited talk presented at the ''NuPhys2023: Prospects in Neutrino Physics''openaire +1 more source
High energy gamma-ray astronomy
AIP Conference Proceedings, 1992The status and prospects for high energy gamma‐ray astronomy are reviewed, emphasizing potential relevance to nuclear and particle physics.
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Cosmic Rays: High Energy Astronomy
1969To-day one investigates primary cosmic rays, before they have started to interact with the material of the Earth’s atmosphere, by use of balloons, rockets and artificial satellites. They include protons, α-particles and heavy nuclei. By means of tracks in photographic emulsions, one can determine their charge-number Z and then one finds the following ...
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High energy neutrino astronomy: first light
Nuclear Physics B - Proceedings Supplements, 2001Abstract We review: 1. The compelling case for doing neutrino astronomy, 2. Why we anticipate that we need kilometer-scale observatories to do the science, 3. The recent successful commissioning of the Lake Baikal and South Pole neutrino detectors.
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Gravitational-wave physics and astronomy in the 2020s and 2030s
Nature Reviews Physics, 2021Matthew Bailes +2 more
exaly
High Energy Neutrino and Gamma-Ray Astronomy
2010There are at least three arguments why we need a new type of astronomy — high energy neutrino astronomy. Low energy (MeV) neutrino astronomy exists. It detected the neutrinos from SN 1987a and continuously monitors the emission of solar neutrinos in different energy ranges.
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Ultra High Energy Gamma-Ray Astronomy
1986The experimental data on ultra high energy γ-rays are reviewed and a comparison of the properties of photon and proton initiated shower is made.
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HIGH ENERGY NEUTRINO ASTRONOMY
Relativistic Astrophysics and Cosmology, 2004openaire +1 more source