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Directional Optical Module Integration
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Outline Several solutions were proposed to increase the number of active elements in the km3 detector Genova group proposed a directional OM based on a 4-anode photomultiplier Simulations shows that the detector efficiency increases at low energies, if full instrumented with directional OMs A 4-anode, 10” PMT was built by Hamamatsu The light guides to achieve directional sensitivity were designed and developed in Genova The front-end electronics was realized to be compliant with the standard NEMO readout chain The first directional OM is being instrumented in these weeks
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Genova Directional OM PMT support structure 4-anode PMT
High reflectivity mirrors Light guide ~10 cm thick Pressure resistant glass sphere
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Detector Efficiency Increase
The detector efficiency change was evaluated if directional OM be used A net effect on the effective area is predicted The effect is large up to 10TeV Further reconstruction code optimization is possible A further improvement of the efficiency is expected Results obtained with NEMO km3 geometry
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Hamamatsu 4-anode PMT Hamamatsu produced (on our request) a 10” 4-anode PMT based on model R7081 Two prototypes were supplied The response (summed on the four anodes) was measured at the factory and resulted slightly better (more uniform) than the single anode model
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PMT Characterization Several measurements were performed on the directional PMTs both in Genova and in Catania LNS ANODS A1 A2 A3 A4 TT [ns] 105 106 TTS [ns] (FWHM) 4.62 3.95 3.54 4.16 P/V 3.03 3.09 2.95 2.75 GAIN 5.0·107 5.4·107 3.9·107 RSE % (sigma) 33.62 30.62 37.34 35.15
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4-Anode Performances Single Photoelectron Distribution
Transit Time Distribution
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Cross-Talk Cross-Talk signal contamination is roughly proportional to PE number Cross-Talk between dynode cascades due to capacitive coupling Can be filtered Cross talk due to internally reflected photons Small w.r.t. signal A1
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Cross-Talk Analysis Channel 3: avg -15mV Quadrant 1 lighted with 16 PE equivalent laser pulses Cross talk signals are few % of direct ones Cross talk signals are significantly smaller than direct Channel 1: avg -250mV
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High Reflectivity Mirrors
Several different materials were tested to build the mirrors Aluminum coated film Polypropylene multilayer 3M polypropylene multilayer (Vikuiti® film) gave the best performances A simple mirror structure made of plexiglas and Vikuiti film has been realized LASER PHOTODIODE WATTMETER LENSES TARGET BEAM STRIP OF REFLECTING MATERIAL ROTATING AND TRANSLATING SUPPORT
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Light Guides To achieve directionality, a thick (~10 cm) light guide is needed Plexiglas and optical gel solutions were studied Plexiglas is more transparent Optical gel is simpler to handle Optical gel is elastic ➙ no problem at high pressures The first directional OM has been realized with optical gel
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Front-End Electronics (i)
Custom power supply was developed and built It is based on Cockroft-Walton voltage multiplier Voltage up to 2000V Independent setting of K to D1 and D1 to A voltages Single 5V Low current absorption: 500 mW Remote switching, regulation and monitoring Onboard thermometer 4 independent outputs
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Front-End Electronics (ii)
The 4 outputs must be conditioned match the NEMO DAQ A big effort was made to reduce the dynode cascades cross-talk A solution based on passive filters, a summer and 4 comparators was developed and built This board is actually under test in Genova
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Prototype Integration (i)
Mirror positioning Optical gel preparation
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Prototype Integration (ii)
PMT positioning in the optical gel Optical gel degassing
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Prototype Integration (iii)
OM front view OM side view
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