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Underground Physics Research in Finland

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Presentation on theme: "Underground Physics Research in Finland"— Presentation transcript:

1 Underground Physics Research in Finland
Jukka Maalampi Department of Physics University of Jyväskylä and Helsinki Institute of Physics RECFA Helsinki 8-9 October 2010

2 Underground Physics projects
An Underground Cosmic Ray Experiment EMMA (Experiment with MultiMuon Array) in Pyhäsalmi mine. Under construction and testing. Megaton observatory for neutrinos and proton decay (LAGUNA). In Design Study phase. Pyhäsalmi mine a candidate location.

3 CUPP - Center of Underground Physics in Pyhäsalmi mine
Administrated by University of Oulu. Supported by University of Jyväskylä. Research activity since 2000 Pyhäsalmi mine is the deepest operating hard rock mine in Europa (1444 m). Known ore reserves until ca Operated by Inmet Mining Corporation, Canada

4 Small scale pilot experiments
Radon migration in the rock China University of Geophysics Investigation of Neutron Multiplicity Khlopin Radium Institute of St. Petersburg MUG Muons UnderGround. Measured muon flux at different depths down to 210 m MUD Movable Underground Detector. Measured muon flux down to 1490 m

5 EMMA – Experiment with Multi-Muon Array
Experiment for studying the knee-area of the cosmic ray energy spectrum via multi-muon events Recycled LEP-DELPHI drift chambers & small scale scintillators (manufac-tured by IHEP, Protvino) Under construction at the depth of 75 m, to be completed in Total detector area  300 m2 Funded mainly by EU through the Regional Development Fund (ERDF) ~300 k€/yr. Funding also from the Academy of Finland and universities and grants from private foundations. Total funding so far ~2 M€. Scintillators 0.7 M€, drift chambers ~0 k€.

6 The concept Measures the laternal distribution of muons which depends on the chemical composition of the primary cosmic rays. Novelty: only the high-energy muons created close to the primary cosmic ray reach the detector Direction sensitivity < 1 degree

7 EMMA Collaboration T. Enqvist, J. Joutsenvaara, P. Kuusiniemi, T. Räihä, J. Sarkamo University of Oulu, Finland T. Kalliokoski, K. Loo, M. Slupecki, W.H. Trzaska, A. Virkajärvi University of Jyväskylä, Finland L. Bezrukov, L. Inzhechik, B. Lubsandorzhiev, V. Petkov, V. Volchenko, A. Yanin RAS/INR, Moscow, Russia H. Fynbo University of Århus, Denmark PhD-students underlined The Finnish EMMA team (+ summer students) U. Jyväskylä and U. Oulu

8 Scientific Advisory Board
Tiina Suomijärvi (Orsay), chair Leonid Bezrukov (INR, Russian Academy of Sciences) Anatoly Erlykin (Durham/LPI, Moscow) Andreas Haungs (Karlsruhe)

9 LAGUNA Large Apparatus for Grand Unification and Neutrino Astrophysics
Design study (FP 7, 1.7 M€) 9 countries, 28 institutions, ~100 members Finland: U. Jyväskylä, U. Oulu, Kalliosuunnittelu Oy Rockplan (rock engineering), ~10 persons involved, EU funding 0.24 M€. Salaries from other sources (Universities, foundations, Rockplan). Pyhäsalmi mine a candidate location (6 other) 3 detector options: GLACIER (LiAR), LENA (LScin), MEMPHYS (WC) Technical feasibility study done (~1200 pages)

10

11 Cite candidates

12 ASPERA Roadmap To be updated soon.

13 Scientific goals Long/Short Baseline neutrino physics
CP violation Mass hierarchy CERN-Pyhäsalmi offers a LBL (2300 km ≈ ”magic baseline”) not considered elsewhere in the world CERN-Fréjus offers a SBL (130 km) not considered elsewhere in the world Proton decay (testing GUTs) Solar neutrinos Supernova neutrinos (new&old) Geoneutrinos

14 Thank you for your attention!

15 Backup slides

16 Test run in spring 2010 A 29 track event in station C


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