july 3, 2006d. kielczewska, appec sc neutrino physics in pl (strength and weeknesses) danuta...

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July 3, 2006 D. Kielczewska, ApPEC SC Neutrino Physics in PL (strength and weeknesses) Danuta Kiełczewska Warsaw University & A.Sołtan Institute of Nuclear Studies Experiments we are involved ( including theoretical calculations closely connected to experiments) How many of us How we tried to unify our activities and problems we’ve incurred

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July 3, 2006 D. Kielczewska, ApPEC SC

Neutrino Physics in PL(strength and weeknesses)

Danuta Kiełczewska Warsaw University &A.Sołtan Institute of Nuclear Studies

Experiments we are involved ( including theoreticalcalculations closely connected to experiments)

How many of us How we tried to unify our activities and problems

we’ve incurred

July 3, 2006 D. Kielczewska, ApPEC SC

Involvement in Neutrino Experiments (with PL affiliation)

Atmospheric neutrinos• Super-Kamiokande (1996 -

Neutrino oscillations

Warsaw University

July 3, 2006 D. Kielczewska, ApPEC SC

Super-Kamiokande

~ 140 authors

JAPANUSAKOREAPOLAND

Institutions

1614 3 1

Discovery of oscillation of atmospheric neutrinos (1998)(the most often cited high energy experimental paper

in the SLAC HEP database (>2200 citations)

First „neutrino-graphy” of the Sun Search for proton decays Search for Dark Matter (via neutralino annihilation)

(Warsaw University)

July 3, 2006 D. Kielczewska, ApPEC SC

Oscillation of atmospheric neutrinos in SK

2 2

2

0.0019 0.0030 eV

sin 2 0.90 at 90% . .c l

m

Oscillation

Decay Decoherence

Evidence for oscillationOscillation parameters

July 3, 2006 D. Kielczewska, ApPEC SC

Involvement in Neutrino Experiments (with PL affiliation)

Atmospheric neutrinos• Super-Kamiokande (1996 -

Neutrino oscillations

Solar neutrinos:• Super-Kamiokande (1996 - • Gallex/GNO (1997-2001) • Borexino: (in preparation from 1994-

Warsaw University

Jagellonian University

July 3, 2006 D. Kielczewska, ApPEC SC

Deficit of solar neutrinosDeficit of solar neutrinos(also with participation of PL groups)

JagellonianUniversity

WarsawUniversity

July 3, 2006 D. Kielczewska, ApPEC SC

Borexino To study Be solar neutrinos.in Gran Sasso Lab.

17 Institutionsincl: Jagellonian University (M. Wójcik):- Selection of low radioactivity materials.- Radon permeability through nylon at different humidities

July 3, 2006 D. Kielczewska, ApPEC SC

Involvement in Neutrino Experiments (with PL affiliation)

Neutrino oscillations

Accelerator long-baseline experiments

• K2K (1998 – 2005) – analyses are still going onWarsaw Universityand Sołtan Instituteof Nuclear Studies

July 3, 2006 D. Kielczewska, ApPEC SC

K2K - KEK to Kamioka K2K - KEK to Kamioka

250 km~ 160 authors36 institutions(2 from Pl: Wa U, IPJ)

A beam of of energy around 1 GeVCompared at near detectors and at SK.

July 3, 2006 D. Kielczewska, ApPEC SC

Near Detectors at KEKNear Detectors at KEK

SciBar

PL contribution in:• Construction of SciFi• Cher. light calibration• Particle identification PhD student on site and acted as one of the experts of 1KT detector (J. Zalipska)

July 3, 2006 D. Kielczewska, ApPEC SC

Observation of oscillation in K2KObservation of oscillation in K2K

for 103.8

events 151 :expected

events 107 :observed1210

Final result:

w/o oscill.

22

2

eV0028.0

0.12sin

m

effect4

A combination of oberved:

• event deficit• spectrum

July 3, 2006 D. Kielczewska, ApPEC SC

Involvement in Neutrino Experiments (with PL affiliation)

Neutrino oscillations

Accelerator long-baseline experiments

• K2K (1998 – 2005) – analyses are still going on

• MINOS (2005 –

Warsaw Universityand Sołtan Instituteof Nuclear Studies

Warsaw University(K. Grzelak)

July 3, 2006 D. Kielczewska, ApPEC SC

MINOS – first results

D.A. Petyt, Fermilab, Mar. 30

July 3, 2006 D. Kielczewska, ApPEC SC

Involvement in Neutrino Experiments (with PL affiliation)

Neutrino oscillations

Accelerator long-baseline experiments

• K2K (1998 – 2005) – analyses are still going on

• MINOS (2005 –• Noa (R&D)

• ICARUS/T600

Warsaw Universityand Sołtan Instituteof Nuclear Studies

Warsaw University(K. Grzelak)

Polish neutrino group (2000 -

In an effort to form a large, strong group involved in an innovating technology:

participated in T600 tests in Pavia

July 3, 2006 D. Kielczewska, ApPEC SC

Polish neutrino group Senior (18)

Junior(21) (incl

PhD,MSc)Katowice University of Silesia US J. Kisiel, W. Zipper 2

Kraków:Cracow University of Technology H. Kuna-Ciskal, M. MaślakInstitute of Nuclear Physics IFJ A. Dąbrowska, J. W. Mietelski, 4

M. Szarska, A. ZalewskaJagellonian University UJ M. Wójcik 2Univ. of Science and Technology AGH R. Rumian 1

Warszawa Institute for Nuclear Studies IPJ T. Kozłowski, E. Rondio, 3

J. Stepaniak, M. SzeptyckaWarsaw University WaU W. Dominik, D. Kiełczewska 4Warsaw University of Technology K. Zaremba 1

WrocławWrocław University WrU J. Sobczyk 4

(Neutrino phenomenology)

July 3, 2006 D. Kielczewska, ApPEC SC

Polish participation in Icarus Test in Pavia

• One of the triggers was prepared by PL groups.• Shifts• Data analysis: - study of the propagation of scintillation light

- reconstruction of 0 events - reconstruction of muon energies - data compression

(7 papers published in 2003-2006)

Icarus in LNGS (examples) • modification of the readout electronics• neutrino interactions (analytical and MC) • procedures for tau event selection• a check of mechanical parameters for cryostats

Production of anode wires for next modules

July 3, 2006 D. Kielczewska, ApPEC SC

T600 analysis: π0 mass reconstruction

tt00 = 12.4 = 12.4 s, s, e e = 1.65 ms= 1.65 ms

E(E(11) = 182.5) = 182.5±±22.2 MeV22.2 MeV

E(E(22) = 180.8) = 180.8±±20.1 MeV20.1 MeV

Run 712 Evt 7 (Left Collection View)

MM = 150.6 = 150.6±±11.8 11.8 MeV/cMeV/c22

51 0 candidate events

= 40= 40ºº

Main vertex

Poland+ Pavia analysis

Preliminary

in agreement with expectede.m. resolution!

comb. backgroundin events

with > 2 showers

July 3, 2006 D. Kielczewska, ApPEC SC

Anode wires for T1200 - production in

Poland Present status: • All the equipment has been constructed, purchased or borrowed from Pavia with many improvements as compared to the original Pavia setup for the wire production of T600.• Common work of the experimental groups from Warsaw, Katowice and Cracow, in close collaboration with the Pavia group.• Laboratory in Cracow (12x5.5 m2) prepared for production.

P. Sala

July 3, 2006 D. Kielczewska, ApPEC SC

Involvement in Neutrino Experiments (with PL affiliation)

Neutrino oscillations

Future accelerator long-baseline experiment: T2K

Polish neutrino group

However the road to additional ICARUS modules appears to be a very rocky one…….

Therefore we are using the acquired expertise in LAr techniquein simulations for T2K-LAr. We also consider hardware contributions to T2K.

July 3, 2006 D. Kielczewska, ApPEC SC

T2K (Tokai to Kamioka)

Dec.2002 : LOI submitted to J-PARC office signed by45 physicists from Japan, 110 physicists from:Canada, China, France, Italy, Korea, Poland, Russia, Spain,Switzerland, UK and USA

K. Nishikawa, Venice 2003

beam of <1GeV

0.75 MW 50 (40) GeV PS

4MW 50GeV PS

→ → xx disappearance

→ → ee appearance NC measurement

CP violation proton decay

July 3, 2006 D. Kielczewska, ApPEC SC

T2K detectors

100 ton LAr TPC:(together with other European groupsand coordinated byA. Rubbia) LOI is now

preparedwith PLparticipation

SK

For precision measurement of:• cross sections• beam contamination

July 3, 2006 D. Kielczewska, ApPEC SC

T2K Schedule

Possible future upgrade:– 4MW Super-J-PARC + Hyper-K (1Mt)– CP violation in lepton

sector– Proton Decay

2004 2005 2006 2007 2008

SK full rebuild

T2K construction physics run K2K

2009

PS commisionning

132 2sin

Sensitivity to

down to 0.006

July 3, 2006 D. Kielczewska, ApPEC SC

Involvement in Neutrino Experiments (with PL affiliation)

• NEMO-3 and Super-NEMO

• GERDA

2 0

Warsaw Universityand Sołtan Instituteof Nuclear Studies

Jagellonian University

July 3, 2006 D. Kielczewska, ApPEC SC

M. Wójcik

M. Smoluchowski Institute of Physics

Jagellonian University Measurements of low background

radio-activity

July 3, 2006 D. Kielczewska, ApPEC SC

On April 27-28 S. Jullian (NEMO-3 spokesman) and D. Lalannewere in Warsaw to discuss a possibility to join the collaborations.

was formed

see thepresentationby Z. Janasthis afternoon

July 3, 2006 D. Kielczewska, ApPEC SC

July 3, 2006 D. Kielczewska, ApPEC SC

Theoretical groups closely related to the experimental activities

Neutrino interactions with special attention to nuclear effects for long- baseline accelerator neutrinos. Preparation of MC

generator - Wrocław neutrino group (J. Sobczyk)

Neutrino emission from pre-supernova Of great interest to Super-Kamiokande Collaboration in connexion to a possible upgrade: adding Gd for neutron detection. Purpose – early warning for a SN gravitational collapseA. Odrzywolek, M. Misiaszek, M. Kutschera (Kraków)

Astroparticle Physics 21 303 (2004); astro-ph/0511555

Double beta decays W. Kaminski (Lublin)

see the presentation on WWW

July 3, 2006 D. Kielczewska, ApPEC SC

PhD theses (since 2002):

Completed >6

Current >10

MSc theses (since1998):Completed >20

Topical Neutrino conferences organized in PL:

1. Nuclear effects in neutrino interactions20th Max Born Symposium, Dec. 7-10, 2005, Wrocław, Poland

2. Cracow Epiphany Conference on Neutrinos and Dark Matter, Cracow, Poland, 5-8 January 2006.

July 3, 2006 D. Kielczewska, ApPEC SC

Summary Strength of experimental neutrino physics in PL:

We are involved in the most successful neutrino experiments Elsevier awarded its SCOPUS award for the most cited science

papers with Polish authors for publications in neutrino physics

The groups (experimental and theoretical) collaborate very closely - with regular meetings/workshops in Katowice, Kraków, Warszawa or Wrocław. This is very helpful in sharing our expertise in various fields.

9 institutions, 39 physicists (18 senior & 21 junior)

Our Weakness:my personal view

We are involved in too many different projects and our initial plan to unify and to have significant contribution in one attractive experiment has not come to fruition yet.

To help that we organize a Polish Neutrino Network this afternoon.