Underground Physics Research in Finland

Slides:

Advertisements

Similar presentations

Sep 26, 2003Katri Huitu, HIP/Dept.of Phys.Sciences1 PARTICLE PHENOMENOLOGY Helsinki: Department of Physical Sciences, Helsinki Institute of Physics Turku:

Advertisements

J. Strait Fermilab October 21, 2005 The Neutrino Detector of the Future: A Massive Liquid Argon TPC.

M3.1 JYFL fission model Department of Physics, University of Jyväskylä, FIN-40351, Finland V.G. Khlopin Radium Institute, , St. Petersburg, Russia.

Cosmic Ray Using for Monitoring and Forecasting Dangerous Solar Flare Events Lev I. Dorman (1, 2) 1. Israel Cosmic Ray & Space Weather Center and Emilio.

New Large* Neutrino Detectors

Recent Discoveries in Neutrino Physics: Understanding Neutrino Oscillations 2-3 neutrino detectors with variable baseline 1500 ft nuclear reactor Determining.

Cosmic Rays with the LEP detectors Charles Timmermans University of Nijmegen.

COSMIC RAY PHYSICS IN BOLIVIA 4TH School on Cosmic Rays and Astrophysics UFABC-Santo André-SP-Brasil August 2010 Alfonso Velarde Cosmic Ray Laboratory.

Low Energy Neutrino Astrophysics

LAGUNA and Neutrino Physics NOW 2008 Lothar Oberauer TU München, Germany.

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

Cosmic Rays Basic particle discovery. Cosmic Rays at Earth – Primaries (protons, nuclei) – Secondaries (pions) – Decay products (muons, photons, electrons)

Committee on Science, Engineering and Public Policy Board on Physics and Astronomy Committee on Setting Priorities for NSF’s Large Research Facility Projects.

An accelerator beam of muon neutrinos is manufactured at the Fermi Laboratory in Illinois, USA. The neutrino beam spectrum is sampled by two detectors:

HPC-Europa2 Funding research visits in Europe

October 12th, 2006L. Mosca LAGUNA Meeting in Zurich 1 IPP- ETH Zurich October 12th, 2006 LAGUNA Meeting WG 7: Safety and Environment Report by L. Mosca.

INDIA-BASED NEUTRINO OBSERVATORY (INO) STATUS REPORT Naba K Mondal Tata Institute of Fundamental Research Mumbai, India NUFACT Scoping Study Meeting at.

CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm %0.6%0.4% Δm %0.4%0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix,

KM3NeT The Birth of a Giant V. Popa, KM3NeT Collaboration Institute for Space Sciences, Magurele-Bucharest, Romania.

1 LENA Low Energy Neutrino Astronomy NOW 2010, September 6, 2010 Lothar Oberauer, TUM, Physik-Department.

Petten 29/10/99 ANTARES an underwater neutrino observatory Contents: – Introduction – Neutrino Astronomy and Physics the cosmic ray spectrum sources of.

L. MoscaEPIPHANY Conf 6-8 Jan EPIPHANY Conference at Cracow “Physics in Underground Laboratories and its connection with LHC” - 6 to 8 January 2010.

ESSnuSB Project for Leptonic CP Violation Discovery based on the European Spallation Source Linac NOW 2014, 10/9E. Wildner, CERN 2 Elena WILDNER CERN for.

ECRS – 2010 in Finland. What about it? Good location and interesting site (most N location); First time ECRS is in a Nordic country (Lodz-00, Moscow-02,

LAGUNA Large Apparatus for Grand Unification and Neutrino Astrophysics Launch meeting, Heidelberg, March 2007, Lothar Oberauer, TUM.

Request to join MICE collaboration from MOMENT (IHEP and Sichuan Uni.) Jingyu Tang Institute of High Energy Physics, CAS MICE Collaboration Board Meeting.

ESS based neutrino Super Beam for CP Violation discovery Marcos DRACOS IPHC-IN2P3/CNRS Strasbourg 1 20 August 2013M. Dracos.

Pyramid Scanning (~1970) Luis Alvarez (1970): Are there undiscovered chambers in the Chephren pyramid? Investigate with cosmic rays Detector installed.

The NOvA Experiment Ji Liu On behalf of the NOvA collaboration College of William and Mary APS April Meeting April 1, 2012.

Present and future detectors for Geo-neutrinos: Borexino and LENA Applied Antineutrino Physics Workshop APC, Paris, Dec L. Oberauer, TU München.

Neutrino Point Sources (Looking for) (with Underground Detectors) THE HIGTE ST ENERGY COSMIC RAYS AND THEIR SOURCES: Moscow May 21-23, 2004 S.P. Mikheyev.

Alain Blondel. AIDA-Neutrino meeting AIDA Neutrino detector studies 1. News from the neutrino scene 2. Beam requirements for AIDA 3. Discuss.

Counting Electrons to Measure the Neutrino Mass Hierarchy J. Brunner 17/04/2013 APC.

Neutrinoless double-beta decay and the SuperNEMO project. Darren Price University of Manchester 24 November, 2004.

R-ECFA Meeting, Warsaw, Astroparticle Physics in Poland Grzegorz Wrochna Sołtan Institute for Nuclear Studies Józef Chełmoński ( )

QuarkNet and Cosmic Ray Muon Flux Experiments Florida Academy of Sciences Spring Conference 2009 Alfred Menendez and Michael Abercrombie with Dr. Marcus.

Neutrino Oscillations at Homestake from Chlorine to the Megadetector Ancient Origins of the Question ~1860 Darwin publishes “On The Origin of Species”-

Villa Olmo Search for neutrino bursts from gravitational collapse of stars at the Baksan Underground Scintillation Telescope Yu.F. Novoseltsev,

ESS based neutrino Super Beam for CP Violation discovery Marcos DRACOS IPHC-IN2P3/CNRS Strasbourg 1 10 September 2013M. Dracos.

Build on success to show feasibility of scale-up and physics capability [Brunel, Durham, Sheffield, Sussex, AAE Ltd., e2v Ltd., Rhyal Ltd., Technodyne.

Astroparticle physics with large neutrino detectors  Existing detectors  Physics motivation  Antares project  KM3NeT proposal M. de Jong.

Daya Bay Reactor Neutrino Experiment On behalf of the DayaBay collaboration Virginia Polytechnic Institute and State University Joseph ykHor YuenKeung,

Cosmic ray physics in ALICE Katherin Shtejer Díaz For the ALICE Collaboration LatinoAmerican Workshop on High Energy Physics: Particles and Strings, Havana,

E. W. Grashorn and A. Habig, UMD, for the MINOS Collaboration The Detectors of The Main Injector Neutrino Oscillation Search (MINOS) Experiment The MINOS.

What we do know about cosmic rays at energies above eV? A.A.Petrukhin Contents 4 th Round Table, December , Introduction. 2. How these.

Birth of Neutrino Astrophysics

The Proposed India-based Neutrino Observatory (INO) Naba K Mondal Tata Institute of Fundamental Research Indian meet on linear collider Indore, April,

NEVOD-DECOR experiment: results and future A.A.Petrukhin for Russian-Italian Collaboration Contents MSU, May 16, New method of EAS investigations.

A New Upper Limit for the Tau-Neutrino Magnetic Moment Reinhard Schwienhorst      ee ee

32nd International Cosmic Ray Conference, August , 2011,Beijing 1 R.V. Novoseltseva, M.M. Boliev, I.M. Dzaparova, M.M. Kochkarov,Yu.F. Novoseltsev,

PARTICLE PHYSICS IN RUSSIA R-ECFA Meeting in Moscow, 9-10 October, 2009V.Matveev Participating Institutes and Universities Participating Institutes and.

Status of the NO A Experiment Kirk Bays (Caltech) on behalf of the NO A collaboration Lake Louise Winter Institute Saturday, Feb 22, 2014.

Neutrino telescopes: ANTARES and KM3NeT Maarten de Jong Programme: Group composition (current): 6+2 staff, 4 post-doc, 4 PhD. Vidi 1, Veni 1+1.

E. W. Grashorn, for the MINOS Collaboration Observation of Shadowing in the Underground Muon Flux in MINOS This poster was supported directly by the U.S.

Alex Howard, Imperial College Slide 1 July 2 nd 2001 Underground Project UNDERGROUND PROJECT – Overview and Goals Alex Howard Imperial College, London.

LAGUNA Design of a pan- European Infrastructure for Large Apparatus studying Grand Unification and Neutrino Astrophysics Guido Nuijten.

Marcos DRACOS IPHC-IN2P3/CNRS Université de Strasbourg

LAGUNA and beyond GDR Neutrino at Orsay-PNO October 11th, 2010

The “Carpet-2” multipurpose air shower array of the Baksan Neutrino Observatory INR of RAS A.U. Kudzhaev Institute for Nuclear Research, Russian Academy.

IPHC-IN2P3/CNRS Strasbourg

Determination of 14C abundance in liquid scintillator

Overview of the Jiangmen Underground Neutrino Observatory (JUNO)

Neutrinoastrophysik bei niedrigen Energien BOREXINO and LAGUNA

Introduction of IHEP.

WP4 Positioning European Astroparticle Physics in the world-wide context WP leader CNRS Partners: FOM, IFIN-HH, FRS-FNRS/FWO, FCT Total work: 22 months.

Introduction of IHEP.

EMMA-experiment (Experiment with MultiMuon Array) Juho Sarkamo

XVth International Workshop on Neutrino Factories, Betabeams and Superbeams LAGUNA-LBNO Many thanks to D. Duchesneau, F. Di Lodovico, T. Patzak, A. Rubbia.

The European Consortium working on the ESSνSB project

Overview of the Jiangmen Underground Neutrino Observatory (JUNO)

Presentation transcript:

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

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.

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 2018. Operated by Inmet Mining Corporation, Canada

Small scale pilot experiments Radon migration in the rock 2000-2001 China University of Geophysics Investigation of Neutron Multiplicity Khlopin Radium Institute of St. Petersburg MUG 2000-2002 Muons UnderGround. Measured muon flux at different depths down to 210 m MUD 2004-2005 Movable Underground Detector. Measured muon flux down to 1490 m

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 2011. 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€.

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

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

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

LAGUNA Large Apparatus for Grand Unification and Neutrino Astrophysics Design study 2009-2011 (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)

Cite candidates

ASPERA Roadmap To be updated soon.

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

Thank you for your attention!

Backup slides

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