What is the Universe made of? Where do the high-energy cosmic particles impinging the Earth’s atmosphere come from? How have they gained such a high energy, much higher than what man-made accelerators can produce? Can atmospheric neutrinos provide more information on neutrino properties? Scientists of KM3NeT are seeking answers using a network of neutrino detectors in the abyss of the Mediterranean Sea.

2-KM3NeT-NeutrinoToMuonKM3NeT is the future European deep-sea research infrastructure hosting new generation neutrino detectors located at the bottom of the deep seas of the Mediterranean. The ARCA detectors of KM3NeT will form a telescope that scientists will use to search for neutrinos from distant astrophysical sources in our Universe, like supernovae, gamma ray bursters or colliding stars. The ORCA detector of KM3NeT will be dedicated to the study of the properties of the high-energetic neutrino particles themselves. At the bottom of the Mediterranean Sea, several arrays of thousands of optical sensors will detect the faint light from charged particles created in the reactions of cosmic or atmospheric neutrinos with the water inside or close to the detector volumes in the deep sea. Several cubic kilometres – km3 of sea water will be instrumented forming a Neutrino Telescope of unprecedented size: KM3NeTThe facility will offer marine and Earth scientists the unique opportunity to house their instrumentation for long term and on-line monitoring of the deep-sea environment and the sea bottom at depths of several kilometers close to the South coasts of Europe.

Construction time  line

The realisation of the KM3NeT infrastructure will proceed in phases. The first phase of construction has started in 2015 and is expected to be finished in 2017. For the next phase of KM3NeT 2.0 a Letter of Intent has been published with the intention – pending funding – to finish construction in 2020. After that, the third and final phase of construction will include an extension of the detectors to several cubic kilometres, required for efficient detection of the neutrinos that are so shy to interact that huge detection volumes are required. The required large detection volumes explain the choice for instrumenting the abundant natural waters of the Mediterranean.

Read the Memorandum of Understanding for KM3NeT-phase1 for details about the funding of the first phase of construction of KM3NeT. In the Letter of Intent for KM3NeT 2.0  the plans for the second phase of construction of KM3NeT detailed.