Giant Radio Array for Neutrino Detection information
Giant Radio Array for Neutrino Detection
Alternative names
GRAND
Telescope style
neutrino detector radio telescope
Website
grand.cnrs.fr
[edit on Wikidata]
This article may rely excessively on sources too closely associated with the subject, potentially preventing the article from being verifiable and neutral. Please help improve it by replacing them with more appropriate citations to reliable, independent, third-party sources.(November 2018) (Learn how and when to remove this message)
The Giant Radio Array for Neutrino Detection (GRAND) is a proposed large-scale detector designed to collect ultra-high energy cosmic particles as cosmic rays, neutrinos and photons with energies exceeding 1017 eV. This project aims at solving the mystery of their origin and the early stages of the universe itself. The proposal, formulated by an international group of researchers, calls for an array of 200,000 receivers to be placed on mountain ranges around the world.
and 24 Related for: Giant Radio Array for Neutrino Detection information
by the Square Kilometre Arrayradio telescope project. On 31 March 2021, the CHIME/FRB Collaboration reported the detection of FRB 20201124A and related...
also being sought with optical and radio searches. For a sufficiently advanced civilization, hyper energetic neutrinos from Planck scale accelerators should...
most accurate for cosmic rays at highest energies, in particular when combined with EAS arrays of particle detectors. Similar to the detection of Cherenkov-light...
et al. (26 August 2015). "First Detection of the Acoustic Oscillation Phase Shift Expected from the Cosmic Neutrino Background". Physical Review Letters...
Neutrino Study: Report of the Neutrino Astrophysics and Cosmology Working Group". arXiv:astro-ph/0412544. Myra, E. S.; Burrows, A. (1990). "Neutrinos...
protons combine to form neutrons via electron capture, releasing a flood of neutrinos. When densities reach a nuclear density of 4×1017 kg/m3, a combination...
station. The Telescope Array was constructed by a collaboration between the teams formerly operating the Akeno Giant Air Shower Array (AGASA), which was a...
neutrino astronomy, astronomers use heavily shielded underground facilities such as SAGE, GALLEX, and Kamioka II/III for the detection of neutrinos....
Manufactured, Lunar Far Side RadioArray Lynn Rothschild: A Flexible, Personalized, On-Demand Astropharmacy No projects were selected for continuation into Phase...
Virgo interferometer. A multi-messenger detection (electromagnetic and gravitational radiation, and neutrinos) would help to better understand the supernova...
the Milky Way galaxy, creating the first neutrino view of the Milky Way. Since 1970, various gamma-ray detection missions have discovered 511-keV gamma...
Brandt; et al. (14 April 2023). "Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star". Science. 380 (6641): 198–203...
152±20 pc or 500±65 ly. In 2008, measurements using the Very Large Array (VLA) produced a radio solution of 5.07±1.10 mas, equaling a distance of 197±45 pc or...
Precision Arrayfor Probing the Epoch of Reionization (PAPER), Low Frequency Array (LOFAR), Murchison Widefield Array (MWA), Giant Metrewave Radio Telescope...
the BSA/LPI large phased arrayradio telescope at the Pushchino Radio Astronomy Observatory. Astronomers report the detection of a star, named HD 139139...
CERN (LHC), India-based Neutrino Observatory (INO), ITER, Low Energy High Intensity Proton Accelerator (LEHIPA), Facility for Antiproton and Ion Research...
begins on the Giant Magellan Telescope in Chile. It is expected to be operational by 2024. 15 August – Astronomers report the detection of iron and titanium...
performance. 25 November The Borexino collaboration reports the detection of Solar neutrinos produced by the carbon–nitrogen–oxygen cycle, confirming prior...
experts access to raw data for detailed calibration and monitoring. TRIUMF first became actively involved in the Sudbury Neutrino Observatory (SNO) when the...
detection of gravitational waves came in the 1970s through observation of a pair of closely orbiting neutron stars, PSR B1913+16. The explanation for...
the Chandra X-ray Observatory and radio observations by the Karl G. Jansky Very Large Array complemented the detection. This was the first instance of a...
energy is lost as high-energy gamma radiation, and especially also as neutrinos, so that only about 40% of mc2 would actually be available if the antimatter...
Global Information
