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Pyhäsalmi (site review) W. H. Trzaska on behalf of the Finnish LAGUNA team.

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Presentation on theme: "Pyhäsalmi (site review) W. H. Trzaska on behalf of the Finnish LAGUNA team."— Presentation transcript:

1 LAGUNA @ Pyhäsalmi (site review) W. H. Trzaska on behalf of the Finnish LAGUNA team

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3  125 km 2 of the lake (Pyhä-järvi = Holy-lake)  6000 inhabitants around the shores 60 % in Pyhäsalmi and Ruotanen 60 % in Pyhäsalmi and Ruotanen The deepest mine in Europe The deepest mine in Europe  In 1993, after administrative decision, Pyhäjärvi became the 5 th largest town in Finland (by area)! Located close to the geometrical center of Finland; Half way between Jyväskylä and Oulu

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13 Productivity of the Pyhäsalmi mine

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15 EMMA Experiment with MultiMuon Array - a cosmic ray experiment located in the mine

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17 50 m 1-layer 3-layer Parking etc. 10 m EMMA (at the depth of 75 m)  50 m 

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19 CUPP Surfrace Lab

20 CUPP Surface Lab

21 What is required of a LAGUNA site?  Quality of the rock  Ready infrastructure  Low background from nuclear power plants (essential for geo- and supernova diffusion neutrinos)  Seismic stability  Presence of scientific activity on site  Experienced industrial partner

22 Bedrock zones on Earth:  Red: very old bedrock, hard crystalline rock usually very good usually very good  Green: mobile belts (mountains, etc.), hard rock fair / variable fair / variable  White: sedimentary covers (soft rock) often bad often bad

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24 Seismic levels

25 Pyhäsalmi mine

26 This tunnel would be extended 500 m to the proposed LENA site

27 Dry, room temperature conditions at the 1400m level (below the ground)

28 Samples drilled from the LENA tunnel

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30 All 3 LAGUNA detectors could be placed in Pyhäsalmi

31 All caverns are within mine territory! MEMPHYS GLACIER

32 Nuclear power plants in Europe (2008)

33 Reactor neutrinos Fuel composition: 235 U, 238 U, 239 Pu, 241 Pu Reactor: -Produces electron antineutrinos -Production rate: ~2e20 GW -1 s -1 -prop. to thermal power Propagation through the Earth -Neutrino oscillation -Matter effects negligible Detection: -via inverse  -decay (E thr ≈ 1.8 MeV) Background for geo- and supernova diffusion neutrinos

34 Neutrino Background from Power Plants based on 2008 data Measured spectra of reactor neutrinos for U-235,Pu-239 and Pu-241 were used. For U-238 calculated spectra were used. Event rates were calculated for a KamLand-type scintillator det.

35 Olkiluoto 3 (to open in 2012) EPR (European Pressurized water Reactor) 4.3 GW Thermal 1.6 GW Electrical

36 Geo- luminosity of the Earth U-238: Total: 6.65 Above E thr : 0.43 Th-232: Total: 5.30 Above E thr : 0.206 Luminosities [x 10 24 1/s ]

37 Effect of reactor neutrinos on Geo-neutrino background Geo -window U + Th: 1.806 - 2.254 MeV U only: 2.254 - 3.27 MeV

38 Rockplan Ltd – Finnish industrial partner Underground coal storage for Helsingin Energia, 520.000 m3 District cooling station for Helsingin Energia, 30.000 m3 SALMISAARI underground coal storage

39 The underground silos are each 65 m-high x 40 m-diameter with circular plan cross-section. The volumetric capacity of each silo is 81.000 m3. The Salmisaari coal transport tunnel will be re-equipped to charge the silos and a newly-mined conveyor retrieval tunnel will be used to discharge the coal. SALMISAARI underground coal storage

40 Summary: Phyäsalmi fulfills all LAGUNA requirements  Quality of the rock (the best)  Low reactor background (the lowest)  Low seismic activity (the lowest)  Ready infrastructure (all in place)  Clear legal status (signed MoU; all excavation within the mine area)  All LAGUNA detectors can be located in Pyhäsalmi (the only site with this distinction?)  Experienced industrial partner (Rockplan Ltd.)  Competitive excavation & operation costs (yes!)  Local support (enthusiastic!)

41 Thank you for your attention! ν

42 Backup

43 Reactor background vs. calculated Geo-neutrino flux [events/a/kton] (1.8 – 3.3 MeV)

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45 What can be deduced from muons registered underground? 50 GeV cutoff  Energy of the initial CR particle Muon density at the core Muon density at the core  Approximate Z (but not on the event-by-event basis) Lateral distribution Lateral distribution

46 Example of muon distribution induced by a 4 PeV proton

47 Simulated change of p / Fe ratio from 80/20 to 20/80 reconstructed by EMMA after 12 months running


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