Discovering neutrinos of extreme energies with the Radio Neutrino Observatory Greenland
The RNO-G project aims to enhance ultra-high energy neutrino detection using advanced simulations and calibration techniques to uncover cosmic ray sources and new particle physics insights.
Projectdetails
Introduction
The discovery of neutrinos above energies of 1e16 eV promises to uncover the following:
- The unknown sources of ultra-high energy cosmic rays
- New insights into the astrophysics of these sources
- Particle propagation through the Universe
- New particle physics at energies far higher than those accessible to man-made accelerators
Project Overview
The Radio Neutrino Observatory Greenland (RNO-G) is currently under construction and is scheduled to reach 35 stations in 2026. The in-ice radio array RNO-G is the first large-scale implementation of the radio Askaryan technique and will provide an order of magnitude better discovery sensitivity than existing experiments.
Leadership and Collaboration
Its construction and operation is led by me and two colleagues from the US and Europe. This proposal maximizes RNO-G's potential to discover the long-awaited ultra-high energy neutrinos.
Research Approach
My research group will achieve this by enabling high-efficiency and high-purity neutrino searches in data through:
- Novel simulations with improved accuracy
- High-precision instrument calibration
- Unique exploitation of cosmic ray signals as a training tool
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 1.500.000 |
Totale projectbegroting | € 1.500.000 |
Tijdlijn
Startdatum | 1-12-2023 |
Einddatum | 30-11-2028 |
Subsidiejaar | 2023 |
Partners & Locaties
Projectpartners
- DEUTSCHES ELEKTRONEN-SYNCHROTRON DESYpenvoerder
Land(en)
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Why a new neutrino telescope? Because we can.
NEUTRINOSHOT aims to develop a multi-cubic-kilometre neutrino telescope in the Pacific Ocean to enhance detection of ultra-high energy cosmic rays and advance our understanding of the universe.
Optimization of Radio Detectors of Ultra-High-Energy Neutrinos through Deep Learning and Differential Programming
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RES-NOVA aims to revolutionize neutrino detection from supernovae using cryogenic archaeological Pb detectors, enabling precise measurements of neutrino signals and advancing multi-messenger astronomy.
Optimal Particle identification Of Single Site events with Underground MKIDs detectors
OPOSSUM aims to enhance the detection of neutrinoless double-beta decay using advanced sensors in CUORE crystals, significantly reducing background noise to improve sensitivity and understanding of neutrinos.
Air shower interferometry to advance astroparticle physics
This project develops a novel interferometric technique for enhanced air shower reconstruction, aiming to uncover the origins and properties of high-energy cosmic rays using advanced detection facilities.
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