Neutrino oscillations from CERN to Pyhäsalmi

Similar documents
Underground Physics in Pyhäsalmi Mine

Modane underground laboratory (Fréjus)

LBL projects and neutrino CP violation in Europe

A multipurpose detector for low energy

Application of GLoBES: GLACIER on conventional neutrino beams

Simulations of neutrino oscillations with a high-energy beta beam from CERN to LENA at Pyhäsalmi Mine

The LENA Neutrino Observatory

Underground Physics in the Pyhäsalmi mine

Longbase Neutrino Physics. Neil McCauley University of Liverpool Birmingham February 2013

A new underground laboratory at Frejus

NEUTRINO FACTORY / MUON STORAGE RING

GDR Neutrino at Saclay (INSTN) April Report on LAGUNA. Large Apparatus for Grand Unification and Neutrino Astrophysics.

Perspective from Fermilab NRC-DUSEL, December 15, 2010

Simulations of the Long Baseline Neutrino Experiment for the Sieroszowice Underground Laboratory (SUNLAB)

ScienceDirect. The LAGUNA-LBNO Project

LBNF Neutrino Beam. James Strait Fermi National Accelerator Laboratory P.O. Box 500, Batavia, IL , USA. on behalf of the LBNF/DUNE Team

1. Introduction on Astroparticle Physics Research options

BNL Very Long Baseline Neutrino Oscillation Expt.

The Long-Baseline Neutrino Experiment Kate Scholberg, Duke University NOW 2012

Astroparticle physics

Long & Very Long Baseline Neutrino Oscillation Studies at Intense Proton Sources. Jeff Nelson College of William & Mary

PoS(NEUTEL2015)037. The NOvA Experiment. G. Pawloski University of Minnesota Minneapolis, Minnesota 55455, USA

From Here to a Neutrino Factory: Neutrino Oscillations Now and Again

Physics Potential of existing and future LBL ν beams

Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University

Liquid Scintillator Technology Tobias Lachenmaier Universität Tübingen

Astroparticle physics

Neutrino oscillation physics potential of Hyper-Kamiokande

An Underground Laboratory for a Multi-Detector Experiment. Karsten Heeger Lawrence Berkeley National Laboratory

Measuring the neutrino mass hierarchy with atmospheric neutrinos in IceCube(-Gen2)

A Large Liquid Scintillator Detector for Neutrino Mass Hierarchy : RENO-50

The CNGS neutrino beam

CNGS beam monitor with LVD

PoS(FPCP2017)024. The Hyper-Kamiokande Project. Justyna Lagoda

BNL Very Long Baseline Neutrino Oscillation Expt.

NEUTRINOS II The Sequel

Mass hierarchy and CP violation with upgraded NOνA and T2K in light of large θ 13

The ESS neutrino facility for CP violation discovery

A lepton CP violation discovery experiment using a unique neutrino Super Beam

CERN Neutrino beams CERN Neutrino platform

Neutrino AstroPhysics

Marcos Dracos IPHC, Université de Strasbourg, CNRS/IN2P3, F Strasbourg, France

PoS(Nufact08)026. Summary of Working Group I: Theory. S. Choubey (a), P. Hernández (b), and C. W. Walter (c)

Future Experiments with Super Neutrino Beams

The NOνA Experiment and the Future of Neutrino Oscillations

MINOS. Luke A. Corwin, for MINOS Collaboration Indiana University XIV International Workshop On Neutrino Telescopes 2011 March 15

Neutrino mixing II. Can ν e ν µ ν τ? If this happens:

A New Low Background Laboratory in the Pyhäsalmi Mine: Towards 14C free liquid scintillator for low energy neutrino experiments

Accelerator Neutrino Experiments News from Neutrino 2010 Athens

Proposal for a lepton CP violation discovery experiment using a neutrino Super Beam from ESS

So, you want to build a neutrino detector?

Discovery of the Neutrino Mass-I. P1X* Frontiers of Physics Lectures October 2004 Dr Paul Soler University of Glasgow

Neutrino Masses and Mixing

Neutrinos & the MINOS Experiment

Neutrino Mass Hierarchy and Mixing Parameters: Long-baseline Measurements with IceCube Laura Bodine

LAGUNA-LBNO: design of an underground neutrino observatory coupled to long baseline neutrino beams from CERN

Sinergie fra ricerche con neutrini da acceleratore e atmosferici

Sensitivity of the DUNE Experiment to CP Violation. Lisa Whitehead Koerner University of Houston for the DUNE Collaboration

arxiv:hep-ex/ v1 15 Aug 2006

Physics with a detector at Homestake

The JUNO veto detector system. Haoqi Lu Institute of High Energy physics (On Behalf of the JUNO Collaboration) TIPP2017, May22-26,Beijing

Gadolinium Doped Water Cherenkov Detectors

Particle Physics: Neutrinos part I

Neutrino Oscillations

Long Baseline Neutrinos

Potential of Hyper-Kamiokande at some non-accelerator Physics and Nucleon Decay Searches

Neutrino Oscilla8ons

Study of possible opportunities for leptonic CP violation and mass hierarchy at LNGS

The CERN-Gran Sasso Neutrino Program

Experimental results on the atmospheric muon charge ratio

reνolution Three Neutrino Oscillation Lecture Two Lindley Winslow Massachusetts Institute of Technology

Today: Part I: Neutrino oscillations: beam experiments. Part II: Next tutorials: making distributions with histograms and ntuples

New Results from the MINOS Experiment

THE DISTANCE FROM CERN TO LNGS

New Physics with a High Intensity PS (in Italy)

Neutron flux measurement using fast-neutron activation of 12 B and 12 N isotopes in hydrocarbonate scintillators

CNGS - CERN NEUTRINOS TO GRAN SASSO

Impression of NNN05. Kenzo NAKAMURA KEK. April 7-9, 2005 NNN05 Aussois, Savoie, France. K. Nakamura NNN05, Aussois, April 7-9,

The Short Baseline Neutrino Program at Fermilab

Atmospheric Neutrinos and Neutrino Oscillations

EXPLORING PARTICLE-ANTIPARTICLE ASYMMETRY IN NEUTRINO OSCILLATION. Atsuko K. Ichikawa, Kyoto University

Status and Neutrino Oscillation Physics Potential of the Hyper-Kamiokande Project in Japan

Underground cosmic-ray experiment EMMA

The future of neutrino physics (at accelerators)

The DAEδALUS at Hyper-K Experiment: Searching for CP Violation. Mike Shaevitz - Columbia University for the DAEδALUS ALUS Collaboration

Advanced Neutrino Sources

Particle Physics. Michaelmas Term 2009 Prof Mark Thomson. Handout 11 : Neutrino Oscillations. Neutrino Experiments

European Underground Laboratories and ILIAS

Search for sterile neutrino mixing in the muon neutrino to tau neutrino appearance channel with the OPERA detector

Neutrino Experiments with Reactors

Neutrino beamline prospects, concepts Milorad Popovic

The ICARUS Project FRONTIERS IN CONTEMPORARY PHYSICS II. Vanderbilt University, March 5-10, Sergio Navas (ETH Zürich) " Atmospheric neutrinos

Recent Discoveries in Neutrino Physics

Neutrino Event Tagging Based On Nucleon Energy Spectra

Next-Generation Water Cherenkov Detectors (1) Hyper-Kamiokande

Neutrino Physics. Neutron Detector in the Aberdeen Tunnel Underground Laboratory. The Daya Bay Experiment. Significance of θ 13

Giant Liquid Argon Observatory for Proton Decay, Neutrino Astrophysics and CP-violation in the Lepton Sector (GLACIER)

PHYS 5326 Lecture #2. Wednesday, Jan. 24, 2007 Dr. Jae Yu. Wednesday, Jan. 24, 2007 PHYS 5326, Spring 2007 Jae Yu

Leptons and the Weak Interaction

PoS(Nufact08)003. Status and Prospects of Long Baseline ν Oscillation Experiments

Transcription:

Neutrino oscillations from CERN to Pyhäsalmi Juha Peltoniemi CUPP-project cupp.oulu.fi

The CUPP project CUPP Centre for Underground Physics in Pyhäsalmi The purpose is to establish an underground research centre in the Pyhäsalmi mine Funded by EU regional development fund University of Oulu Oulu Southern Institute director Dr Eelis Kokko University of Jyväskylä Pyhäsalmi Mine Ltd Stonello Software Ltd Rockplan Ltd CUPP project Pyhäjärvi town

Location of the site Main office University of Oulu Pyhäsalmi mine in Pyhäjärvi town Also an abandoned sidemine, down to 700 m available nearby Connections roads open all year round Pyhäjärvi-Oulu: 2 h car drive Pyhäjärvi-Jyväskylä: 2 h car drive Pyhäjärvi-Helsinki: bus & train connections 4 aiports within 2 hours drive, connections Oulu-Helsinki: ca 20 flights a day Oulu-Stockholm: 1 4 flights a day Oulu-Copenhagen: 1 flight a day Oulu-Tampere: 2 flights To London, Stockholm, Copenhagen, Tallinn Kuopio

Pyhäsalmi Mine Pyhäsalmi Mine Ltd Inmet Mining Corporation, Canada produces zinc, copper and pyrite The old mine about 1050 m deep operated 1962 2001 The new mine active since July 2001 known ore reserves until ca 2017 greatest depth 1444 m the deepest metal mine in Europe access by lift (2 min) or via decline by car (40 min) or by running (1 h 4 min) old mine new mine fast lift new orebody

Neutrino baseline from CERN to Pyhäsalmi Distance 2288 km The baseline density profile modelled Kozlovskaya, Peltoniemi and Sarkamo, hep-ph/0305042 good geophysical data available Can do accurate simulations for matter effect

Neutrino beams to Pyhäsalmi Neutrino factory 10-50 GeV pure muon (anti)neutrino beam Conventional beams (by pion decay) Wide band beam Narrow band beam/off-axis beam Betabeams Pure electron (anti)neutrino beam Need higher energies

Oscillation probabilities for L=2300 km Sample plots for muon neutrino appearance from electron neutrino beam usual best fit parameters matter enhance normal hierarchy Inverted hierarchy Sin 2 θ 13 =0.1

Experimental potential Reach in sin 2 2θ 13 20 GeV, 10 20 muons per year 10 and 100 ktonyears

Conventional beam 10-30 GeV Duplication of CERN CNGS beam facility Beam cost some 50 MEUR Energy range 10-30 GeV Study tau appearance Relevance depends on the results of OPERA/ICARUS Flux density ca 1/10 of that in Gran Sasso Need larger detectors Technically realistic

Conventional wide band beam 1-6 GeV Observation of multiple nodes E.g., with 1 MW beam (from CERN) and 100 kton year: 10 000 muon CC events, 3 500 NC events with no oscillations Planned SPL not sufficient need higher energy or SPS for acceleration CERN-PYHÄSALMI Diwan et al

Off-axis detectors Sharper energy spectrum off-axis Several other mines (200-800 m) for off-axis detectors Or vice versa 3 degrees 0.5 degrees 2 degrees

Physically interesting range: High energy beta beam antineutrinos: γ ~ 1000 (<E ν > ~ 4 GeV) for 6 He decay neutrinos: γ ~ 2000 (<E ν > ~ 7 GeV) for 18 Ne decay Use LHC to accelerate ions Technically possible Availability and economic feasibility not yet clear Longer baseline and higher energy as compared to 130 km Matter effects visible Expect clear difference between neutrinos and antineutrinos Other kind of detector may be preferred e.g. liquid argon, iron calorimeter Event rates an order of magnitude larger For fixed number of decays and fixed L/E May study tau appearance

Other baselines Magic baseline 7250 km (Winter et al) Clean measurement of mixing angle, insensitive to CP angle Distance to Pyhäsalmi: JHF: ca 7200 km [almost perfect baseline!] Fermilab: 6500-7000 km BNL: ca 6200 km

Possibilities to host detectors in Pyhäsalmi Technically possible to construct large caverns relatively easy Rock mechanics of 20 m x 20 m x 100 m cavern analysed Very large caverns (1 000 000 m 3 ) not studied in detail No unavoidable restrictions for any detector component or material usually considered Can build own pipeline for liquids Own ventilation system to be built Large local production (and demand) of liquid argon World's largest cold process unit of steel in Outokumpu's gigantic stainless steel factories in Northern Finland (Tornio). Several (idependent/competing) factories of liquified gases (Ar, N) within 300 km distance (transport radius) Railway transport of heavy items to the site possible Environmental risks small Laboratories separated from biosphere Broken experiments can be closed and sealed

Costs for constructing a deep underground laboratory Large underground laboratory hall: typically 200 EUR/m 3 Rock construction 40 % excavation, rock removal, shotcreting, bolting, water shielding, etc Building technical works (inner structures etc) 20 % HVAC 5 % Plans, permissions etc 15 % Surprises 20 % Additional shielding (for neutrons) or special equipment Extra costs not excessive Access construction: Decline (tunnel, ramp) with heavy truck access: 3000 EUR/m Narrow tunnel: 1000 EUR/m Shaft (7 m) 5000 EUR/m, (2 m) 1000 EUR/m. Own hoist (lift) to surface 2-10 MEUR

Cost summary Basic costs (general halls, HVAC, etc): ca 5-10 MEUR Access: 2-20 MEUR, depending on depth, location and capacity Caverns for experiments LENA: 10 MEUR Compare: an underground oil tank of 45 000 m 3 : 7 MEUR Cavern for a 100 kton detector (e.g. Neutrino factory): 12 MEUR Caverns for a Megaton detector (UNO-like): 200 MEUR Several ca 30 m wide caverns - one large sphere with r=70 m very expensive. Surface buildings 1-5 MEUR, depending on needs

Level 1100 m (3000 m.w.e) Depths and locations Most cost-effective solution Excavated rock can be skipped directly to stopes for backfilling Minimal disturbance to mining Own lift/decline not required (but would be nice) Level 1400-1500 m (4000 m.w.e) Need special arrangement if done during mining Own access (lift) necessary Additional cost 3-10 MEUR Improves the usability of the lab May need own decline from 1100 m level Additional cost 5-10 MEUR Depths 1500-2500 m (4000-7000 m.w.e.) Possible, but expensive, additional cost ca 30 000 EUR/m.

Conclusions Pyhäsalmi site very suitable for long baseline neutrino oscillation studies CERN Pyhäsalmi baseline 2300 km JHF Pyhäsalmi baseline 7200 km Several neutrino sources technically possible Neutrino factory 5-50 GeV Wide band beam 1-6 GeV Beta beam 4-8 GeV Large halls can be constructed deep underground Good logistics Good opportunities for large detectors Good transport options Liquid argon nearby Environmentally robust and safe site