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P.Kooijman, UVA-GRAPPA, UU, Nikhef
Status of KM3NeT P.Kooijman, UVA-GRAPPA, UU, Nikhef On behalf of KM3NeT ICRC, Beijing, 2011
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Most manageable sea in Northern hemisphere→ Mediterranean
Motivation Build the worlds most sensitive neutrino telescope with a view incorporating the Galactic centre → Northern hemisphere Most manageable sea in Northern hemisphere→ Mediterranean August 15, 2011, Beijing
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Experience with NEMO, NESTOR and especially ANTARES
August 15, 2011, Beijing
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Progress and Planning 2009 - Design Study completed
Technical Design Report Preparatory Phase will be completed 2010 – Technical Decisions 2011/2012 – Prototyping 2011 – Funding requests in several countries (~50% of 220 M€ budget) 2011 – Prepare the collaboration structure for after PP 2013 – Preparation for mass production Finalise design Sourcing materials and tendering 2014 – Start Construction August 15, 2011, Beijing
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Sensor Module Concentrator ring
Increase of Photocathode area by % Digital Optical Module: 17” sphere 31 photomultiplier tubes (3”) All HV and readout and control electronics inside Features: Photon counting Uniform acceptance Coincidences Anomalous large pulse rejection Large photocathode area per pressure feed-through Two manufacturers have prototype PMTs with good specifications: ETEL (USA/UK) Hamamatsu (Japan) Two further manufacturers are preparing prototype PMTs MELZ (Russia) Zhen Chuang (China) August 15, 2011, Beijing
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Read out Electronics: Low power Cockroft-Walton HV base
Time over threshold of each PMT External DC/DC converter for galvanic isolation FPGA central logic PC functionality External or internal timestamping I2C or SPI bus for slow control August 15, 2011, Beijing
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Timing accuracy 50 ps shore to DOM over 100 km
Fibre-optic read-out Timing accuracy 50 ps shore to DOM over 100 km August 15, 2011, Beijing
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Vertical Structure Tower Structure: 20 storeys with each 2 DOMs
6 m length 40 m between Alternately perpendicular Connected by four 5 mm Dyneema ropes Buoy at top Anchor at bottom Stacked for deployment (4x5) Unfurling from the seafloor 860 m high Drag gives top displacement of 150 m at 30 cm/s water current (very rare) 6m Advantage length: Triggering and low energy Torsional stability August 15, 2011, Beijing
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Seafloor Layout TDR Present reference ~6 km3 instrumented volume
Network of smaller detectors Deployment and connection easier 180 m inter tower distance Less “alignment” Other option very sparse for high energies ~6 km3 instrumented volume August 15, 2011, Beijing
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Optimisation Optimisation is ongoing taking into account:
Optimal sensitivity for Galactic sources Cut-off power spectrum à la RXJ1713 Safe and reliable deployment (Maintenance of) Seafloor cable network Power distribution Data network Risk analysis Tracking Backgrounds August 15, 2011, Beijing
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Status now for Galactic Sources
RXJ1713 flux assuming 100% hadronic TDR 154 in 1100 m radius 50 in 650 m radius 50 in 500 m radius 3-4 signal/year 4-5 background /year Depends on quality cuts Only up-going tracks Can go 10-20º above? For showers > 10 PeV 15-20 km3 August 15, 2011, Beijing
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Great Progress Care to join?
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