Tsuyoshi Nakaya (Kyoto Univ.)

Size: px
Start display at page:

Download "Tsuyoshi Nakaya (Kyoto Univ.)"

Transcription

1 TAUP Seattle September 8, 2003 Tsuyoshi Nakaya (Kyoto Univ.) Thanks to the Super-K, K2K, JHFν, UNO, LANNDD members. Special thanks to M. Shiozawa (ICRR, U. of Tokyo) and K. Kobayashi (SUNY at Stony Brook)

2 . Introduction (SUSY) SU(5), SO(0),E 6 SU(3) C SU(2) L U() Y GUT quark + lepton Proton Decay 2

3 No Evidence of Proton Decay so far No Direct Evidence of GUT however, Indications or Hints of GUT Running coupling constants may be unified with SUSY (Precise LEP data) Small but finite neutrino mass (neutrino oscillation) ν Discovery of Proton Decay may be just at the corner. 3

4 Dimension 6 operators: qqql (Gauge-Boson Mediated Decay) M 2 p u e 4 (34 35) M u Y τ 0 years 6 d d d π 0 p 0 GeV ~0 ~35 years Dimension 5 operators in SUSY models: M p u u d w ~ q ~ q ~ H ~ C minimal SU(5) ν s d minimal SUSY SU(5) Κ + τ p (5 6) M m SUSY 6 0 ~ years Super-K TeV ( q ~ q ~ q i j years k l SUSY SO(0) l + ) partial nucleon life time (year) 4

5 aim: τ p 0 35 years 0 35 protons (~300 ktons H 2 O) LANNDD UNO The MEMPHYS project: The Project of a Megaton (Y. Suzuki, NOON2000) ( Megaton Mass Physics) UNO type detector at Frejus: ~Mton Proton Decay detector (Luigi Mosca, TAUP2003) LANNDD 2 in Japan, USA and Europe. (David Cline, TAUP2003) 6

6 aim: τ p 0 35 years 0 35 protons (~300 ktons H 2 O) LANNDD UNO The MEMPHYS project: The Project of a Megaton (Y. Suzuki, NOON2000) ( Megaton Mass Physics) UNO type detector at Frejus: ~Mton Proton Decay detector (Luigi Mosca, TAUP2003) LANNDD 2 in Japan, USA and Europe. (David Cline, TAUP2003) 6

7 aim: τ p 0 35 years 0 35 protons (~300 ktons H 2 O) LANNDD UNO The MEMPHYS project: The Project of a Megaton (Y. Suzuki, NOON2000) ( Megaton Mass Physics) UNO type detector at Frejus: ~Mton Proton Decay detector (Luigi Mosca, TAUP2003) LANNDD 2 in Japan, USA and Europe. (David Cline, TAUP2003) 6

8 aim: τ p 0 35 years 0 35 protons (~300 ktons H 2 O) LANNDD UNO The MEMPHYS project: The Project of a Megaton (Y. Suzuki, NOON2000) ( Megaton Mass Physics) UNO type detector at Frejus: ~Mton Proton Decay detector in Japan, USA and Europe. (Luigi Mosca, TAUP2003) LANNDD 2 (David Cline, TAUP2003) 6

9 aim: τ p 0 35 years 0 35 protons (~300 ktons H 2 O) LANNDD UNO The MEMPHYS project: The Project of a Megaton (Y. Suzuki, NOON2000) ( Megaton Mass Physics) UNO type detector at Frejus: ~Mton Proton Decay detector LANNDD 2 in Japan, USA and Europe. (Luigi Mosca, TAUP2003) (David Cline, TAUP2003) 6

10 aim: τ p 0 35 years 0 35 protons (~300 ktons H 2 O) LANNDD UNO The MEMPHYS project: The Project of a Megaton (Y. Suzuki, NOON2000) ( Megaton Mass Physics) UNO type detector at Frejus: ~Mton Proton Decay detector (Luigi Mosca, TAUP2003) LANNDD 2 in Japan, USA and Europe. (David Cline, TAUP2003) 6

11 Unusual Nucleon Decay (Baryon number Lepton number) Nucleon Disappearance (Extra Dimensions with TeV gravity.) It is also important to look for p (n) invisible state For these modes, a gigantic scintillator detector may work better (KamLAND( and ) (Bob Svoboda, TAUP2003) 7

12 2. Review of proton decay experiments Water Cherenkov Detector (H 2 O) Super-Kamiokande for UNO, Hyper-K, and TITANIC Fine Grained Detector (Fe and Ar) Soudan2 for ICARUS and LANNDD 8

13 Fermi motion of parent nucleons in 6 O Nuclear potential Nucleon-nucleon correlation in 6 O Number of Events H 2 O O(p-state) O(s-state) uncorrelated Correlated (traditional) decay decay Entries correlated decay p+n e + +π 0 +N (0% of decays in 6 O) Reconstructed Mass of e + π 0 (MeV/c 2 ) H ~90% 9

14 Α π 0 from the proton decay may be interacted in a nucleus scattering absorption charged exchange e πp 0 n n p p p n n p p n p p n n n π + Probability ~ 50% 0

15 2.3 Super-Kamiokande 489 days data (92kt yr) Ring Imaging Water Cherenkov Detector 39 m 4 m C Scientific American 000 m underground 50kton (22.5kton fid.),46 20 inch PMTs,885 anti-counter PMTs

16 p eπ 0 Search MC Events NUM RUN SUBRUN EVENT 45 DATE 97-Jun-7 TIME 2:35:52 TOT PE: MAX PE: 68.2 e + γ γ γ Colour : Time Radius : Charge 2

17 2 or 3 rings All rings are electron-like no decay electron 85<m π <85MeV/c 2 (3-ring) 800<m p <050MeV/c 2 p total < 250MeV/c Efficiency = 40% Total momentum (MeV/c) Super-Kamiokande Preliminary p e + π 0 p e + π 0 MC Invariant proton mass (MeV/c 2 )

18 Total momentum (MeV/c) DATA (~4 years: 9.6 kt year) Super-Kamiokande Preliminary 489 days data Invariant proton mass (MeV/c 2 ) p eπ 0 Result 0 events τ p /BR(p e + π 0 ) > years (90% CL) Total momentum (MeV/c) Atmospheric ν MC (2,250 kt year : DATA 25) Super-Kamiokande Preliminary 00 years atmν MC Invariant proton mass (MeV/c 2 ) w/ 0.3 expected Background events Background: ν e N e ± π ± N, π ± N π 0 N (in the oxygen) 4

19 DATA and MC Comparison 6 4 Super-Kamiokande Preliminary days total momentum (MeV/c) L L (938,200) total mass (MeV/c 2 ) P total total momentum (MeV/c) 0 Super-Kamiokande Preliminary days MC:p eπ 0 Super-Kamiokande Preliminary days L in mass v.s. momentum plot distance L in mass v.s. momentum plot 0 MC:p eπ 0 (*) There is a measurement of the p µπ 0 background by K2K (Mine, TAUP2003) total invariant mass M P (MeV/c 2 ) 5

20 Other Gauge Boson Mediated Decays (90% C.L.) Total momentum (MeV/c) Total momentum (MeV/c) Super-Kamiokande Preliminary 489 days data p µ + π Invariant proton mass (MeV/c 2 ) τ/br > years Super-Kamiokande Preliminary 489 days data p e + ρ 0,ρ ππ Invariant proton mass (MeV/c 2 ) τ/br > years Total momentum (MeV/c) Total momentum (MeV/c) Super-Kamiokande Preliminary 489 days data p e + η 0,η γγ Invariant proton mass (MeV/c 2 ) τ/br > years Super-Kamiokande Preliminary 489 days data p e + ω 0,ω π 0 γ Invariant proton mass (MeV/c 2 ) τ/br > years 6

21 p νk + Search e + ν e MC Events γ (6.3MeV) ν µ ν K + µ + (236ΜeV/c) γ µ + 6 O ν µ γ µ + e + t 2ns 2.2µs 2,200ns 7

22 A Novel Idea: Prompt γ tag ν 6 O K + 5 N * γ A proton in 6 O decays (or disappears) 4% 6.3MeV γ-ray generates This propmt γ events will be measured at K2K by NC elastic scattering (ν+ 6 O ν+ 5 N * +p). 8

23 K + µν promptγ search -ring µ-like 25<p µ <260MeV/c Decay electron No proton ring 7<N γhit <60 (prompt γ) number of event data p νk + MC atmν MC Efficiency = 8.6% τ p /BR(p νk + ) >. x0 33 years (90% CL) w/ 0.7 expected Background events N γhit N γhit 9

24 number of event Other channels in p νk + () K + µν, µ eνν w/o γ tag (2) K + π + π 0, π + ( µν) eνν K + µν spectrum search data atmν+p νk + MC (90%CL) atmνmc µ momentum(mev/c) p µ (MeV/c) τp/br(p νk + ) >0.42x0 33 years Light Yield from not π 0,π Q res (PE) 50 Q res (PE) K + π + π 0 search p νk + MC Q +(PE) π K + π + π 0 search MC: K + π + π 0 DATA data Light Yield from π Q π +(PE) τp/br(p νk + ) >0.79x0 33 years Combined: τp/br(p νk + ) > 2.2 x 0 33 years (90% CL) 20

25 Other SUSY GUT Decays (90% C.L.) () n νk 0,K 0 ππ (2) p e + K 0,K 0 ππ (3) p µ + K 0,K 0 ππ K 0 momentum(mev/c) n νk 0, K 0 s π 0 π 0 search p e + K 0, K 0 s π 0 π 0 search p µ + K 0, K 0 s π 0 π 0 search K s π 0 π 0 K s π 0 π 0 K s π 0 π 0 data total momentum(mev/c) data total momentum(mev/c) data K 0 mass(mev/c 2 ) total mass(mev/c 2 ) total mass(mev/c 2 ) τ/br > years τ/br > years τ/br > years 2

26 Summary of Super-K K nucleon decay searches Summary of Nucleon Decay Searches mode exposure εb m observed B.G. τ/b limit (kt yr) (%) event (0 32 yrs) p e + + π p µ + + π p e + + η p µ + + η n ν + η p e + + ρ p e + + ω p e + + γ p µ + + γ p ν + K K + νµ + (spectrum) prompt γ + µ K + π + π n ν + K K 0 π 0 π K 0 π + π p e + + K K 0 π 0 π K 0 π + π - 2-ring ring p µ + + K K 0 π 0 π K 0 π + π - 2-ring ring

27 2.4 Soudan2 design for p νk + and multi-particles decays x224 (0.96kton) 2.7m Fine-Grained Tracking Calorimeter Detector Track resolution : 0.8 cm (X,Y) :.0 cm (Z) Trigger threshold (50 %) 75MeV for : 00MeV for e Energy resolution : E/E = 7.0/E / % e, = 8 % Partile ID : 95% 95% (60%) >400 (40) MeV e drift tube mm m m 4.7mm 23

28 p K +, K + + X TOP VIEW K + + e + Z SIDE VIEW FRONT VIEW 2 charged tracks (no proton) K range < 50 cm 28 < range < 58 cm decay electron ( 60 %) B(K + + ) = 9.0% 3.56 kt yr exposure Y Y observed candidate = exp d BG = 0.2 (atm )+0.9(rock) Z X 24

29 p K +, K + π + π - X + TOP VIEW K + 2 tracks and 2 showers K range < 50 cm 00 < M K < 660 MeV/c 2 80 < P + < 400 MeV/c 40 < P < 390 MeV/c 0 < M < 290 MeV/c 2 B(K ) = 5.5% 0 2 Z SIDE VIEW FRONT VIEW 3.56 kt yr exposure observed candidate = 0 exp d BG =.05 (atm )+0.09(rock Y Z Y X combined limit p /B(p K + ) > years (90% CL) 25

30 p νk + for Soudan2 and Super-K Exposure (Kton( Kton٠year ) Efficiency for K + µ + ν (K + π + π 0 ) #Observed Events for K + µ + ν (K + π + π 0 ) Expected Background 90%CL limit (years) Soudan (5.5) (0) 0.4 (.4) Super-K (6.0) 0 (0) 0.7 (0.6)

31 Nucleon Decay Searches in Soudan2 mode exposure εb m observed B.G. τ/b limit (kt yr) (%) event (0 32 yrs) p ν + K K + νµ K + π + π p µ + K 0 s K 0 s π + π <0.2 K 0 s π 0 π p e + K 0 s 4.4 K 0 s π + π K 0 s π 0 π p µ + K 0 l p e + K 0 l p µ + K 0 (K 0 l+k 0 s) <.2.2 p e + K 0 (K 0 l+k 0 s) n ν + K 0 s K 0 s π + π K 0 s π 0 π 0 3-shower shower n ν + K p µ + + η η γγ η π 0 π 0 π p e + + η η γγ η π 0 π 0 π n ν + η η γγ η π 0 π 0 π n ν + π p ν + π

32 Other Nucleon Decays Model-Independent limit for nucleon decay p > years (90% CL) study Xe isotopes of years old n ννν (Kamiokande) tagging nuclear γ (9MeV) from the residual nucleus /BR(n ννν) > years (90% CL) p invisible (SNO data, PLB 553 (2003) 35-40) tagging residual neutron /BR(p invisible) > years (90% CL) p n D 2 O A neutron NC signal 28

33 3. Future Experiments Several Proposals for the Water Cherenkov detectors. Hyper-Kamiokande (Japan): 540 ktons UNO (USA): 440 ktons TITANIC (Japan): >~,000 tons MEMPHYS (France): ~,000 tons Great success of Super-K K convinces people that the larger Water Cherenkov detector has an excellent sensitivity for the proton decay. All detectors have a common base of the design. I will show the study of Hyper-K K as a reference. 29

34 Site Candidiate and Construction Schedule Hyper-Kamiokande KAMIOKA SK UNO Under Survey of the site: Homestake WIPP ~0km MEMPHYS Frejus HK It takes about ~0 years for the construction after getting the approval of the project. (cost ~$500M??) ~20X? 30

35 Partial Lifetime (years) p e + π 0 sensitivity (90% CL) Standard momentum cut (<250MeV/c) Efficiency = 43% BG=3events/Mt٠yr HK 20 yr sensitivity for p eπ 0 (90% CL) efficiency=43% BG 3ev/Mtyr SK current limit (90% CL) 79.3ktyr, 5.0 x 0 33 yrs Super-K limit Hyper-K 20 years Exposure (kton year) Exposure (kton٠year) Partial Lifetime (years) Tight momentum cut (<00MeV/c) Efficiency = 7% BG=0.5events/Mt٠yr HK 20 yr sensitivity for p eπ 0 (90% CL) efficiency=7% High sensitivity BG 0.5ev/Mtyr for free proton Hyper-K 20 years SK current limit (90% CL) 79.3ktyr, Super-K 5.0 x limit 0 33 yrs 0 4 Exposure (kton٠year) Exposure (kton year) /BR > yr (Hyper-K 20yrs, 90%CL) 3

36 p νk + sensitivity (90% CL) 0 37 sensitivity for p νk + (90% CL) 0 36 Partial Lifetime (years) HK 20 yr SK current limit(90% CL) 79.3ktyr.6 x 0 33 yrs combined sensitivity π + π 0 prompt γ µ spectrum Exposure (kton year) Exposure (kton٠year) /BR > yr (Hyper-K 20yrs, 90%CL) 32

37 Feasibility of the construction of the huge Liquid Ar detector???? Proposal for the Fine tracking calorimeter detectors. LANNDD: Lq. Ar TPC 4.5 LANNDD No nuclear reinteractions Exposure: 300 kton year Efficiency (%) 42 p e + π p (years) Efficiency (%) 85 p K + p (years) Nuclear reinteractions (FLUKA) LANNDD Exposure: 000 kton year Efficiency (%) p e + π p (years) Efficiency (%) p K + p (years) No nuclear reinteractions Nuclear reinteractions (FLUKA)

38 µ-lanndd (active volume ~50L) Mini-LANNDD (~440ton) 34

39 4. Additional Physics Potential An Ultimate Neutrino Detector Super ν beam Hyper-K has a beam from JHF (J-PARC). The BNL very long baseline ν experiment assumes the UNO type of the detector. MEMPHYS plans to have a beam from CERN-SPL and a β-beam. Atmospheric ν Solar ν Supernova ν Supernova Relic ν 35

40 CP sensitivity (3σ) w/ Super-ν beam JHF-HK CPV Sensitivity sin 2 2θ CHOOZ excluded sin 2 2θ 3 <0.2@ m 32 ~3x0-3 ev no BG 0.04 signal stat only 0.02 stat+2%syst. stat+5%syst. (signal+bg) stat only stat+0%syst. JHF 3σ discovery sinδ 3σ CP sensitivity : δ >20 o for sin 2 2θ 3 >0.0 with 2% syst. 36

41 Supernova Neutrinos Supernova ν Reach ~Mpc Supernova rate will be /(0~5) years 37

42 5. Summary The discovery of the GUT is one of our dreams in physics. The Nucleon Decay is the direct evidence of the GUT. With a next generation nucleon decay detector, we explore the proton decays p e + π 0 ( >0 35 years) p ν K + ( >0 34 years) GUT SUSY-GUT A Nucleon Decay detector makes the neutrino physics more exciting. CP violation in neutrino oscillation Supernova-ν observatory High statistics atmospheric and solar neutrino experimets. 38

43 2005~200 What do you expect? An indication of θ 3 by MINOS or Super-K A candidate event of proton decay at Super-K 200~205 Discovery of θ 3 by Super-ν beam (JHF( JHFν). A few proton decay candidates. An absolute neutrino mass measurement from cosmology. >205 Discovery of CP violation in neutrino oscillation. Discovery of proton decay. 39

44 Supplement 40

45 typical p νk +, K + π + π 0 MC event Outer Detector RUN SUBRUN 0 EVENT 22 DATE 99-Nov- TIME :55:36 TOT PE: 232. MAX PE: 23.2 NHIT : 487 RunMODE:MonteCar Inner Detector Radius : Charge 4

46 Proton decays in ICARUS Excellent tracking and particle capabilities. Suitable for K events, multi-prong events. τ p > ~ x T(yr) x ε x % CL Operation in the underground will start soon 42

Proton Decays. -- motivation, status, and future prospect -- Univ. of Tokyo, Kamioka Observatory Masato Shiozawa

Proton Decays. -- motivation, status, and future prospect -- Univ. of Tokyo, Kamioka Observatory Masato Shiozawa Proton Decays -- motivation, status, and future prospect -- Univ. of Tokyo, Kamioka Observatory Masato Shiozawa Look for Baryon number violation B number conservation is experimental subject B number conservation

More information

Proton Decay searches -- sensitivity, BG and photo-coverage. Univ. of Tokyo, Kamioka Observatory Masato Shiozawa

Proton Decay searches -- sensitivity, BG and photo-coverage. Univ. of Tokyo, Kamioka Observatory Masato Shiozawa Proton Decay searches -- sensitivity, BG and photo-coverage -- Univ. of Tokyo, Kamioka Observatory Masato Shiozawa April-25 @ NNN5 Water as a proton decay detector Source H 2 O 2/1 free proton no nuclear

More information

UNO: Underground Nucleon Decay and Neutrino Observatory

UNO: Underground Nucleon Decay and Neutrino Observatory UNO: Underground Nucleon Decay and Neutrino Observatory Clark McGrew NESS, Jan 2002 NESS 2002 McGrew p. 1 The UNO Concept Build on well-established techniques Explore broad range of physics Provide a general

More information

Neutrino Oscillation and CP violation

Neutrino Oscillation and CP violation Neutrino Oscillation and CP violation Contents. Neutrino Oscillation Experiments and CPV. Possible CP measurements in TK 3. Summary Nov.4, 4 @Nikko K. Nishikawa Kyoto niversity CP Violation Asymmetry between

More information

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

Next-Generation Water Cherenkov Detectors (1) Hyper-Kamiokande Next-Generation Water Cherenkov Detectors (1) Hyper-Kamiokande Kenzo NAKAMURA KEK C.N. Yang Institute for Theoretical Physics Conference Neutrinos and Implications for Physics Beyond the Standard Model

More information

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

EXPLORING PARTICLE-ANTIPARTICLE ASYMMETRY IN NEUTRINO OSCILLATION. Atsuko K. Ichikawa, Kyoto University EXPLORING PARTICLE-ANTIPARTICLE ASYMMETRY IN NEUTRINO OSCILLATION Atsuko K. Ichikawa, Kyoto University Got PhD by detecting doubly-strange nuclei using emulsion After that, working on accelerator-based

More information

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

Potential of Hyper-Kamiokande at some non-accelerator Physics and Nucleon Decay Searches Potential of Hyper-Kamiokande at some non-accelerator Physics and Nucleon Decay Searches Instituto de Física Teórica, UAM/CSIC University Autonoma Madrid E-mail: luis.labarga@uam.es on behalf of The Hyper-Kamiokande

More information

Future Experiments with Super Neutrino Beams

Future Experiments with Super Neutrino Beams 1 Future Experiments with Super Neutrino Beams T. Nakaya a a Faculty of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502, JAPAN The recent status of future neutrino experiments with super neutrino beams

More information

( Some of the ) Lateset results from Super-Kamiokande

( Some of the ) Lateset results from Super-Kamiokande 1 ( Some of the ) Lateset results from Super-Kamiokande Yoshinari Hayato ( Kamioka, ICRR ) for the SK collaboration 1. About Super-Kamiokande 2. Solar neutrino studies in SK 3. Atmospheric neutrino studies

More information

Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University

Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University 1 Outline 2 Lecture 1: Experimental Neutrino Physics Neutrino Physics and Interactions Neutrino Mass Experiments Neutrino Sources/Beams and

More information

Recent Nucleon Decay Results from Super-Kamiokande

Recent Nucleon Decay Results from Super-Kamiokande Recent Nucleon Decay Results from Super-Kamiokande Jennifer L. Raaf Boston University April 14, 28 Motivation Super-Kamiokande n ν π decay search Results Motivation Interesting candidate for grand unification:

More information

Recent results from Super-Kamiokande

Recent results from Super-Kamiokande Recent results from Super-Kamiokande ~ atmospheric neutrino ~ Yoshinari Hayato ( Kamioka, ICRR, U-Tokyo ) for the Super-Kamiokande collaboration 1 41.4m Super-Kamiokande detector 50000 tons Ring imaging

More information

Hyper-Kamiokande. Kenzo NAKAMURA KEK. August 1-2, 2005 Neutrino Meeting IIT-Bombay, Mumbai, India

Hyper-Kamiokande. Kenzo NAKAMURA KEK. August 1-2, 2005 Neutrino Meeting IIT-Bombay, Mumbai, India Hyper-Kamiokande --- Concept and R&D --- Kenzo NAKAMURA KEK August 1-2, 2005 Neutrino Meeting IIT-Bombay, Mumbai, India K. Nakamura Neutrino Meeting, IIT-Bombay, Mumbai, India, August 1-2, 2005 1 Science

More information

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

Impression of NNN05. Kenzo NAKAMURA KEK. April 7-9, 2005 NNN05 Aussois, Savoie, France. K. Nakamura NNN05, Aussois, April 7-9, Impression of NNN05 Kenzo NAKAMURA KEK April 7-9, 2005 NNN05 Aussois, Savoie, France K. Nakamura NNN05, Aussois, April 7-9, 2005 1 History of NNN Workshop NNN99, Stony Brook: Initiated by CKJ NNN00, UC

More information

The Hyper-Kamiodande Project A New Adventure in n Physics

The Hyper-Kamiodande Project A New Adventure in n Physics http://hyperk.org The Hyper-Kamiodande Project A New Adventure in n Physics ICNFP2017 Kolymbari, Crete August 26, 17 Alessandro Bravar on behalf of the HK Proto-Collaboration Hyper-K Physics Overview 2

More information

Recent Results from K2K. Masashi Yokoyama (Kyoto U.) For K2K collaboration 2004 SLAC Summer Institute

Recent Results from K2K. Masashi Yokoyama (Kyoto U.) For K2K collaboration 2004 SLAC Summer Institute Recent Results from K2K Masashi Yokoyama (Kyoto U.) For K2K collaboration 2004 SLAC Summer Institute Introduction What is K2K? KEK to Kamioka first accelerator-based long baseline neutrino experiment!

More information

The Neutrino Physics at Accelerators: the High Intensity Frontier

The Neutrino Physics at Accelerators: the High Intensity Frontier Feb. 23, 2005 Neutrino Telescopes 2005 at Venice The Neutrino Physics at Accelerators: the High Intensity Frontier T. Nakaya (Kyoto Univ.) 1 1. Introduction ±Δm 23(13) 2 θ 13 Proton Decay CP 2 High Intensity

More information

Gadolinium Doped Water Cherenkov Detectors

Gadolinium Doped Water Cherenkov Detectors Gadolinium Doped Water Cherenkov Detectors David Hadley University of Warwick NuInt-UK Workshop 20th July 2015 Water Cherenkov Detector Super-Kamiokande 22.5 kt fiducial mass 2 Physics with Large Scale

More information

1. Neutrino Oscillations

1. Neutrino Oscillations Neutrino oscillations and masses 1. Neutrino oscillations 2. Atmospheric neutrinos 3. Solar neutrinos, MSW effect 4. Reactor neutrinos 5. Accelerator neutrinos 6. Neutrino masses, double beta decay 1.

More information

Neutrino Oscillations

Neutrino Oscillations Neutrino Oscillations Heidi Schellman June 6, 2000 Lots of help from Janet Conrad Charge mass,mev tandard Model of Elementary Particles 3 Generations of Fermions Force Carriers Q u a r k s u d 2/3 2/3

More information

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

PoS(FPCP2017)024. The Hyper-Kamiokande Project. Justyna Lagoda National Centre for Nuclear Research Otwock-Swierk, Poland E-mail: justyna.lagoda@ncbj.gov.pl The Hyper-Kamiokande is a project of a large water Cherenkov detector to be built in Japan. The design allows

More information

Single π production in MiniBooNE and K2K

Single π production in MiniBooNE and K2K Single π production in MiniBooNE and K2K Yoshinari Hayato (ICRR, Univ. Tokyo) 1. Introduction 2. Study of neutral current single π 0 production at K2K 3. Study of charged current coherent π + production

More information

Solar and atmospheric ν s

Solar and atmospheric ν s Solar and atmospheric ν s Masato SHIOZAWA Kamioka Observatory, Institute for Cosmic Ray Research, U of Tokyo, and Kamioka Satellite, Kavli Institute for the Physics and Mathematics of the Universe (WPI),

More information

Introduction to Super-K and Hyper-K. Roger Wendell Kyoto U. High-Energy Group Meeting

Introduction to Super-K and Hyper-K. Roger Wendell Kyoto U. High-Energy Group Meeting Introduction to Super-K and Hyper-K Roger Wendell Kyoto U. High-Energy Group Meeting First Things First Super-Kamiokande has been operating for 20 years It is a large experiment, with many physics topics

More information

Neutrino oscillation physics potential of Hyper-Kamiokande

Neutrino oscillation physics potential of Hyper-Kamiokande Neutrino oscillation physics potential of Hyper-Kamiokande on behalf of the Hyper-Kamiokande Collaboration Queen Mary University of London E-mail: l.cremonesi@qmul.ac.uk Hyper-Kamiokande (Hyper-K) is a

More information

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

Status and Neutrino Oscillation Physics Potential of the Hyper-Kamiokande Project in Japan Status and Neutrino Oscillation Physics Potential of the Hyper-Kamiokande Project in Japan Gianfranca De Rosa Univ. Federico II and INFN Naples On behalf of Hyper-Kamiokande Collaboration Hyper-Kamiokande:

More information

Search for Neutron Antineutron Oscillations at Super Kamiokande I. Brandon Hartfiel Cal State Dominguez Hills May

Search for Neutron Antineutron Oscillations at Super Kamiokande I. Brandon Hartfiel Cal State Dominguez Hills May Search for Neutron Antineutron Oscillations at Super Kamiokande I Brandon Hartfiel Cal State Dominguez Hills May 1 2007 n a neutron oscillates into an antineutron Oxygen 16 time 10 33 years π + π 0 π 0

More information

The Factors That Limit Time Resolution for Photon Detection in Large Cherenkov Detectors

The Factors That Limit Time Resolution for Photon Detection in Large Cherenkov Detectors The Factors That Limit Time Resolution for Photon Detection in Large Cherenkov Detectors Kate Scholberg, Duke University Chicago, April 2011 OUTLINE - Overview/physics motivation - Event reconstruction

More information

Super-Kamiokande ~The Status of n Oscillation ~

Super-Kamiokande ~The Status of n Oscillation ~ May 26, 2006 Vulcano Workshop 2006 Super-Kamiokande ~The Status of n Oscillation ~ Yoshihisa OBAYASHI (ICRR, Univ. of Tokyo) for Super-Kamiokande Collaboration May 26, 2006 Y.Obayashi @ Vulcano 2006 1

More information

NEW νe Appearance Results from the. T2K Experiment. Matthew Malek Imperial College London. University of Birmingham HEP Seminar 13 June 2012

NEW νe Appearance Results from the. T2K Experiment. Matthew Malek Imperial College London. University of Birmingham HEP Seminar 13 June 2012 NEW νe Appearance Results from the T2K Experiment Matthew Malek Imperial College London University of Birmingham HEP Seminar 13 June 2012 Outline Physics motivation: Neutrinos & Oscillations Overview of

More information

Super-K Gd. M.Ikeda(ICRR) for Super-K collaboration Workshop for Neutrino Programs with facilities in Japan

Super-K Gd. M.Ikeda(ICRR) for Super-K collaboration Workshop for Neutrino Programs with facilities in Japan Super-K Gd M.Ikeda(ICRR) for Super-K collaboration 20150804@JPARC Workshop for Neutrino Programs with facilities in Japan 1 Contents Introduction to SK-Gd Physics motivations Study of Gd effect to SK Plan

More information

Search for Proton Decay in Super-Kamiokande

Search for Proton Decay in Super-Kamiokande Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute for Physics, Nov. 24, 2017 Who am I I am Yusuke Suda from Univ. of Tokyo,

More information

The Hyper-Kamiokande project

The Hyper-Kamiokande project 22-July-2017 @Quy Nhon The Hyper-Kamiokande project Yasuo Takeuchi Kobe University Hyper-Kamiokande detector & current R&Ds Current status of the project Physics/Observation targets in HK Summary 1 Hyper-Kamiokande

More information

JHFnu at J-PARC neutrino oscillation experiment

JHFnu at J-PARC neutrino oscillation experiment @IAC Mar.0,00 JHFnu at J-PARC neutrino oscillation experiment 50 GeV PS LOI # International collaboration Recent developments in neutrino physics Readiness Summary Koichiro Nishikawa Kyoto niversity for

More information

Multi-Megaton Water Cherenkov Detector for a Proton Decay Search TITAND (former name: TITANIC)

Multi-Megaton Water Cherenkov Detector for a Proton Decay Search TITAND (former name: TITANIC) Multi-Megaton Water Cherenkov Detector for a Proton Decay Search TITAND (former name: TITANIC) arxiv:hep-ex/0110005v1 2 Oct 2001 Y. Suzuki Kamioka Observatory, ICRR, University of Tokyo Higashi-Mozumi,

More information

Recent Results from T2K and Future Prospects

Recent Results from T2K and Future Prospects Recent Results from TK and Future Prospects Konosuke Iwamoto, on behalf of the TK Collaboration University of Rochester E-mail: kiwamoto@pas.rochester.edu The TK long-baseline neutrino oscillation experiment

More information

Super-Kamiokande (on the activities from 2000 to 2006 and future prospects)

Super-Kamiokande (on the activities from 2000 to 2006 and future prospects) Super-Kamiokande (on the activities from 2000 to 2006 and future prospects) M. Nakahata for Neutr ino and astr opar ticle Division Super-Kamiokande detector Atmospheric neutrinos Solar Neutrinos Proton

More information

The future of neutrino physics (at accelerators)

The future of neutrino physics (at accelerators) Mauro Mezzetto, Istituto Nazionale Fisica Nucleare, Padova The future of neutrino physics (at accelerators) Present Status Concepts, strategies, challenges The two players: Dune and Hyper-Kamiokande Conclusions

More information

Neutrino Oscillations and the Matter Effect

Neutrino Oscillations and the Matter Effect Master of Science Examination Neutrino Oscillations and the Matter Effect RAJARSHI DAS Committee Walter Toki, Robert Wilson, Carmen Menoni Overview Introduction to Neutrinos Two Generation Mixing and Oscillation

More information

Neutrino Oscillations

Neutrino Oscillations Neutrino Oscillations Elisa Bernardini Deutsches Elektronen-Synchrotron DESY (Zeuthen) Suggested reading: C. Giunti and C.W. Kim, Fundamentals of Neutrino Physics and Astrophysics, Oxford University Press

More information

Supernova Neutrino Detectors: Current and Future. Kate Scholberg, Duke University June 24, 2005

Supernova Neutrino Detectors: Current and Future. Kate Scholberg, Duke University June 24, 2005 Supernova Neutrino Detectors: Current and Future Kate Scholberg, Duke University June 24, 2005 OUTLINE Supernovae and the Neutrino Signal What We Will Learn Supernova Neutrino Detection Current SN ν Detectors

More information

GADZOOKS! project at Super-Kamiokande

GADZOOKS! project at Super-Kamiokande GADZOOKS! project at Super-Kamiokande M.Ikeda (Kamioka ICRR, U.of Tokyo) for Super-K collaboration 2015,6,9@WIN2015 Contents GADZOOKS! project Supernova Relic Neutrino search R&D status and Plan Summary

More information

What should be considered and improved for CP study.

What should be considered and improved for CP study. P violation Physics at a J-PAR Beam Water herenkov Detector Kenji Kaneyuki Univ. of Tokyo, Institute for osmic Ray Research, Research enter for osmic Neutrinos What should be considered and improved for

More information

Current status of T2K experiment

Current status of T2K experiment ICEPP Symposium @Hakuba Feb 1 st 005 Current status of TK experiment 1.Introduction.TK experiment 3.Near neutrino detector 4.Summary Jun Kubota (Kyoto University) Feb 1 005 ICEPP@Hakuba005 1 Introduction

More information

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

Long & Very Long Baseline Neutrino Oscillation Studies at Intense Proton Sources. Jeff Nelson College of William & Mary Long & Very Long Baseline Neutrino Oscillation Studies at Intense Proton Sources Jeff Nelson College of William & Mary Outline A highly selective neutrino primer Oscillations (what & why we believe) >

More information

Recent Results from Alysia Marino, University of Colorado at Boulder Neutrino Flux Workshop, University of Pittsburgh, Dec 6 8,2012

Recent Results from Alysia Marino, University of Colorado at Boulder Neutrino Flux Workshop, University of Pittsburgh, Dec 6 8,2012 Recent Results from Alysia Marino, University of Colorado at Boulder Neutrino Flux Workshop, University of Pittsburgh, Dec 6 8,2012 Outline T2K Beamline and Detectors Uncertainties from prior measurements

More information

Particle Physics: Neutrinos part I

Particle Physics: Neutrinos part I Particle Physics: Neutrinos part I José I. Crespo-Anadón Week 8: November 10, 2017 Columbia University Science Honors Program Course policies Attendance record counts Up to four absences Lateness or leaving

More information

Recent results on neutrino oscillations and CP violation measurement in Neutrinos

Recent results on neutrino oscillations and CP violation measurement in Neutrinos Recent results on neutrino oscillations and CP violation measurement in Neutrinos M.Nakahata Kamioka observatory, ICRR, IPMU, Univ. of Tokyo CP Violation in Elementary Particles and Composite ystems, Feb.19,

More information

Super-KamiokaNDE: Beyond Neutrino Oscillations. A. George University of Pittsburgh

Super-KamiokaNDE: Beyond Neutrino Oscillations. A. George University of Pittsburgh Super-KamiokaNDE: Beyond Neutrino Oscillations A. George University of Pittsburgh PART 1: NUCLEON DECAY What s in a name? Various stages of the experiment have been called: o Kamiokande o Kamiokande-II

More information

PoS(NOW2016)003. T2K oscillation results. Lorenzo Magaletti. INFN Sezione di Bari

PoS(NOW2016)003. T2K oscillation results. Lorenzo Magaletti. INFN Sezione di Bari INFN Sezione di Bari E-mail: lorenzo.magaletti@ba.infn.it The TK (Tokai-to-Kamioka) experiment is a second generation long baseline neutrino oscillation experiment that probes physics beyond the Standard

More information

Indication of ν µ ν e appearance in the T2K EXPERIMENT

Indication of ν µ ν e appearance in the T2K EXPERIMENT Indication of ν µ ν e appearance in the T2K EXPERIMENT θ 13 Alain Blondel University of Geneva On behalf of the T2K collaboration Alain Blondel UNIGE seminar -- The T2K experiment theta_13 1 There are

More information

The T2K Neutrino Experiment

The T2K Neutrino Experiment The T2K Neutrino Experiment Tokai to Kamioka TPC-Group, Institute 3b Achim Stahl, Stefan Roth, Karim Laihem, Dennis Terhorst, Jochen Steinmann 03.09.2009, Bad Honnef 2009-09-03 1 Overview 1. Neutrinos

More information

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

The ICARUS Project FRONTIERS IN CONTEMPORARY PHYSICS II. Vanderbilt University, March 5-10, Sergio Navas (ETH Zürich)  Atmospheric neutrinos The ICARUS Project FRONTIERS IN CONTEMPORARY PHYSICS II Vanderbilt University, March 5-10, 2001 Sergio Navas (ETH Zürich) Detection Principle The T600 Module Physics Programme: " Atmospheric neutrinos

More information

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

Discovery of the Neutrino Mass-I. P1X* Frontiers of Physics Lectures October 2004 Dr Paul Soler University of Glasgow -I P1X* Frontiers of Physics Lectures 19-0 October 004 Dr Paul Soler University of Glasgow Outline 1. Introduction: the structure of matter. Neutrinos:.1 Neutrino interactions. Neutrino discovery and questions.3

More information

Search for double electron capture on 124 Xe with the XMASS-I detector

Search for double electron capture on 124 Xe with the XMASS-I detector Search for double electron capture on 124 Xe with the XMASS-I detector KATSUKI HIRAIDE (ICRR, THE UNIVERSITY OF TOKYO) SEPTEMBER 7 TH, 2015 TAUP2015 1 124 Xe 2n double electron capture Natural xenon contains

More information

Measurement of q 13 in Neutrino Oscillation Experiments. Stefan Roth, RWTH Aachen Seminar, DESY, 21 st /22 nd January 2014

Measurement of q 13 in Neutrino Oscillation Experiments. Stefan Roth, RWTH Aachen Seminar, DESY, 21 st /22 nd January 2014 Measurement of q 13 in Neutrino Oscillation Experiments Stefan Roth, RWTH Aachen Seminar, DESY, 21 st /22 nd January 2014 Overview Experiments with neutrinos Neutrino oscillations Reactor and accelerator

More information

Neutrino Physics II. Neutrino Phenomenology. Arcadi Santamaria. TAE 2014, Benasque, September 19, IFIC/Univ. València

Neutrino Physics II. Neutrino Phenomenology. Arcadi Santamaria. TAE 2014, Benasque, September 19, IFIC/Univ. València Neutrino Physics II Neutrino Phenomenology Arcadi Santamaria IFIC/Univ. València TAE 2014, Benasque, September 19, 2014 Neutrino Physics II Outline 1 Neutrino oscillations phenomenology Solar neutrinos

More information

T2K neutrino oscillation results

T2K neutrino oscillation results T2K neutrino oscillation results K. Okumura (ICRR Univ. of Tokyo) for T2K collaboration The 19th Particles and Nuclei International Conference (PANIC 11) Contents Introduction n e appearance result n m

More information

Radio-chemical method

Radio-chemical method Neutrino Detectors Radio-chemical method Neutrino reactions: n+ν e => p+e - p+ν e => n+e + Radio chemical reaction in nuclei: A N Z+ν e => A-1 N(Z+1)+e - (Electron anti-neutrino, right) (Z+1) will be extracted,

More information

Review of Nucleon Decay Searches at Super-Kamiokande

Review of Nucleon Decay Searches at Super-Kamiokande Review of Nucleon Decay Searches at Super-Kamiokande Volodymyr Takhistov (for the Super-Kamiokande Collaboration) Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA Baryon

More information

K2K and T2K. 2006/10/19 For the 2006 External Review Panel. Masato Shiozawa Kamioka Observatory

K2K and T2K. 2006/10/19 For the 2006 External Review Panel. Masato Shiozawa Kamioka Observatory K2K and T2K 2006/10/19 For the 2006 External Review Panel Masato Shiozawa Kamioka Observatory University of Barcelona, Boston University, Chonnam National University, Dongshin University, University of

More information

Recent T2K results on CP violation in the lepton sector

Recent T2K results on CP violation in the lepton sector Recent T2K results on CP violation in the lepton sector presented by Per Jonsson Imperial College London On Behalf of the T2K Collaboration, December 14-20 2016, Fort Lauderdale, USA. Outline Neutrino

More information

KamLAND. Studying Neutrinos from Reactor

KamLAND. Studying Neutrinos from Reactor KamLAND : Studying Neutrinos from Reactor Atsuto Suzuki KEK : High Energy Accelerator Research Organization KamLAND Collaboration Outline 1. KamLAND Overview 2. Reactor Neutrinos 3. e Detection in Liquid

More information

Interactions/Weak Force/Leptons

Interactions/Weak Force/Leptons Interactions/Weak Force/Leptons Quantum Picture of Interactions Yukawa Theory Boson Propagator Feynman Diagrams Electromagnetic Interactions Renormalization and Gauge Invariance Weak and Electroweak Interactions

More information

Interactions/Weak Force/Leptons

Interactions/Weak Force/Leptons Interactions/Weak Force/Leptons Quantum Picture of Interactions Yukawa Theory Boson Propagator Feynman Diagrams Electromagnetic Interactions Renormalization and Gauge Invariance Weak and Electroweak Interactions

More information

PHYS 5326 Lecture #6. 1. Neutrino Oscillation Formalism 2. Neutrino Oscillation Measurements

PHYS 5326 Lecture #6. 1. Neutrino Oscillation Formalism 2. Neutrino Oscillation Measurements PHYS 5326 Lecture #6 Wednesday, Feb. 14, 2007 Dr. 1. Neutrino Oscillation Formalism 2. Neutrino Oscillation Measurements 1. Solar Neutrinos 2. Atmospheric neutrinos 3. Accelerator Based Oscillation Experiments

More information

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

Longbase Neutrino Physics. Neil McCauley University of Liverpool Birmingham February 2013 Longbase Neutrino Physics Neil McCauley University of Liverpool Birmingham February 2013 1 Neutrino mixing Neutrino mixing is characterised by the PMNS matrix. U PMNS cosq12 sinq 0 12 sinq cosq 0 12 12

More information

Current Results from Reactor Neutrino Experiments

Current Results from Reactor Neutrino Experiments Current Results from Reactor Neutrino Experiments Soo-Bong Kim (KNRC, Seoul National University) Tsukuba Global Science Week (TGSW015), Tsukuba, Sep. 8-30, 015 Neutrino Physics with Reactor 1956 Discovery

More information

Results from T2K. Alex Finch Lancaster University ND280 T2K

Results from T2K. Alex Finch Lancaster University ND280 T2K Results from T2K Alex Finch Lancaster University ND280 T2K 1 Contents T2K Overview Tokai Kamioka Neutrino Oscillations Results Muon neutrino disappearance Electron neutrino appearance Charged Current inclusive

More information

Long baseline experiments

Long baseline experiments Mauro Mezzetto, Istituto Nazionale Fisica Nucleare, Padova Long baseline experiments Present Status Concepts, strategies, challenges The two players: Dune and Hyper-Kamiokande Conclusions M. Mezzetto,

More information

Atmospheric muons & neutrinos in neutrino telescopes

Atmospheric muons & neutrinos in neutrino telescopes Atmospheric muons & neutrinos in neutrino telescopes Neutrino oscillations Muon & neutrino beams Muons & neutrinos underground Berlin, 1 October 2009 Tom Gaisser 1 Atmospheric neutrinos Produced by cosmic-ray

More information

1 Introduction. 2 Nucleon Decay Searches

1 Introduction. 2 Nucleon Decay Searches RECENT RESULTS FROM SUPERKAMIOKANDE SHUNICHI MINE Department of Physics and Astronomy, University of California, Irvine, USA I will summarize the most recent nucleon decay and sterile neutrino results

More information

Performance of the ICARUS T600 detector

Performance of the ICARUS T600 detector Performance of the ICARUS T600 detector CIPANP 2003 Conference on the Intersections of Particle and Nuclear Physics New York City May 19-24, 2003 Sergio Navas University of Granada, Spain Sergio Navas

More information

BNL Very Long Baseline Neutrino Oscillation Expt.

BNL Very Long Baseline Neutrino Oscillation Expt. Mary Bishai, BNL 1 p.1/36 BNL Very Long Baseline Neutrino Oscillation Expt. Next Generation of Nucleon Decay and Neutrino Detectors 8/04/2005 Mary Bishai mbishai@bnl.gov Brookhaven National Lab. Mary Bishai,

More information

A new underground laboratory at Frejus

A new underground laboratory at Frejus Jacques Bouchez CEA-SACLAY NNN05-Aussois April 7, 2005 A new underground laboratory at Frejus Historical overview Latest developments Outlook PROTON DRIVER FOR CERN NEUTRINO FACTORY Frejus lab is 130 km

More information

Detectors for astroparticle physics

Detectors for astroparticle physics Detectors for astroparticle physics Teresa Marrodán Undagoitia marrodan@physik.uzh.ch Universität Zürich Kern und Teilchenphysik II, Zürich 07.05.2010 Teresa Marrodán Undagoitia (UZH) Detectors for astroparticle

More information

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

Particle Physics. Michaelmas Term 2009 Prof Mark Thomson. Handout 11 : Neutrino Oscillations. Neutrino Experiments Particle Physics Michaelmas Term 2009 Prof Mark Thomson Handout 11 : Neutrino Oscillations Prof. M.A. Thomson Michaelmas 2009 340 Neutrino Experiments Before discussing current experimental data, need

More information

Grand Unified Theories & Proton Decay. Ed Kearns Boston University NEPPSR 2009

Grand Unified Theories & Proton Decay. Ed Kearns Boston University NEPPSR 2009 Grand Unified Theories & Proton Decay Ed Kearns Boston University NEPPSR 2009 Planetary Mo

More information

Review of Nucleon Decay Searches at Super-Kamiokande

Review of Nucleon Decay Searches at Super-Kamiokande Review of Nucleon Decay Searches at Super-Kamiokande Volodymyr Takhistov (for the Super-Kamiokande Collaboration) Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA Baryon

More information

Analyzing Data. PHY310: Lecture 16. Road Map

Analyzing Data. PHY310: Lecture 16. Road Map PHY310: Lecture 16 Analyzing Data Road Map Step One: Defining the Data Set Where it came from Understanding the background physics What are the measured variables Second Topic Third Topic 1 Example Analysis

More information

Neutrino interaction at K2K

Neutrino interaction at K2K Neutrino interaction at K2K KEK Yoshinari Hayato for the K2K collaboration Contents Introduction Neutrino flux measurements and neutrino interaction studies in K2K Charged current quasi-elastic scattering

More information

Solar spectrum. Nuclear burning in the sun produce Heat, Luminosity and Neutrinos. pp neutrinos < 0.4 MeV

Solar spectrum. Nuclear burning in the sun produce Heat, Luminosity and Neutrinos. pp neutrinos < 0.4 MeV SOLAR NEUTRINOS Solar spectrum Nuclear burning in the sun produce Heat, Luminosity and Neutrinos pp neutrinos < 0.4 MeV Beryllium neutrinos 0.86 MeV Monochromatic since 2 body decay 2 kev width due to

More information

NEUTRINOS II The Sequel

NEUTRINOS II The Sequel NEUTRINOS II The Sequel More About Neutrinos Ed Kearns Boston University NEPPSR V - 2006 August 18, 2006 Ed Kearns Boston University NEPPSR 2006 1 There is something unusual about this neutrino talk compared

More information

RECENT RESULTS FROM THE OPERA EXPERIMENT

RECENT RESULTS FROM THE OPERA EXPERIMENT RECENT RESULTS FROM THE OPERA EXPERIMENT P. DEL AMO SANCHEZ on behalf of the OPERA Collaboration LAPP, 9, Chemin du Bellevue, BP 110 74941 Annecy-le-Vieux, FRANCE The OPERA neutrino experiment recently

More information

Neutrinos From The Sky and Through the Earth

Neutrinos From The Sky and Through the Earth Neutrinos From The Sky and Through the Earth Kate Scholberg, Duke University DNP Meeting, October 2016 Neutrino Oscillation Nobel Prize! The fourth Nobel for neutrinos: 1988: neutrino flavor 1995: discovery

More information

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

PoS(Nufact08)003. Status and Prospects of Long Baseline ν Oscillation Experiments Status and Prospects of Long Baseline ν Oscillation Experiments Fermi National Accelerator Laboratory E-mail: niki@fnal.gov We will start with a brief overview of neutrino oscillation physics with emphasis

More information

Other Physics with Geo-Neutrino Detectors

Other Physics with Geo-Neutrino Detectors Other Physics with Geo-Neutrino Detectors M. Lindner Technical University Munich Neutrino Geophysics Workshop Hawaii, Dec. 14-16, 2005 Neutrinos & New Physics neutrinos as probes neutrino properties &

More information

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

Neutrino mixing II. Can ν e ν µ ν τ? If this happens: Can ν e ν µ ν τ? If this happens: Neutrino mixing II neutrinos have mass (though there are some subtleties involving the MSW mechanism) physics beyond the (perturbative) Standard Model participates Outline:

More information

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

MINOS. Luke A. Corwin, for MINOS Collaboration Indiana University XIV International Workshop On Neutrino Telescopes 2011 March 15 MINOS Luke A. Corwin, for MINOS Collaboration Indiana University XIV International Workshop On Neutrino Telescopes 2011 March 15 2 Overview and Current Status Beam Detectors Analyses Neutrino Charged Current

More information

Perspectives of neutrino oscillation physics with long baseline beams

Perspectives of neutrino oscillation physics with long baseline beams Perspectives of neutrino oscillation physics with long baseline beams The European Program OPERA ICARUS The US Program MINOS The Japanese Program JHF-Kamioka Karlsruhe 31.1.2002 Lucia Votano L.N.F. Neutrino

More information

Sinergie fra ricerche con neutrini da acceleratore e atmosferici

Sinergie fra ricerche con neutrini da acceleratore e atmosferici Sinergie fra ricerche con neutrini da acceleratore e atmosferici Michele Maltoni International Centre for Theoretical Physics IFAE 26, Pavia 2 Aprile 26 I. Parameter degeneracies and neutrino data II.

More information

XI. Beyond the Standard Model

XI. Beyond the Standard Model XI. Beyond the Standard Model While the Standard Model appears to be confirmed in all ways, there are some unclear points and possible extensions: Why do the observed quarks and leptons have the masses

More information

Neutrino Physics: an Introduction

Neutrino Physics: an Introduction Neutrino Physics: an Introduction Lecture 2: Neutrino mixing and oscillations Amol Dighe Department of Theoretical Physics Tata Institute of Fundamental Research, Mumbai SERC EHEP School 2017 NISER Bhubaneswar,

More information

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

From Here to a Neutrino Factory: Neutrino Oscillations Now and Again NuMI From Here to a Neutrino Factory: Neutrino Oscillations Now and Again University of the Tevatron April 11, Deborah Harris Fermilab Outline of this Talk History of Neutrino Physics Neutrino Oscillation

More information

Physics Potential of existing and future LBL ν beams

Physics Potential of existing and future LBL ν beams Mauro Mezzetto Istituto Nazionale di Fisica Nucleare, Sezione di Padova Physics Potential of existing and future LBL ν beams NBI 2002, March 14-18,2002, - CERN M. Mezzetto, Physics Potential of existing

More information

Prospects of Reactor ν Oscillation Experiments

Prospects of Reactor ν Oscillation Experiments Prospects of Reactor ν Oscillation Experiments F.Suekane RCNS, Tohoku Univ. Erice School 3/09/009 1 Contents * Motivation * Physics of Neutrino Oscillation * Accessible Parameters of Reactor Neutrinos

More information

Atmospheric Neutrinos MINOS MINOS Far Detector Type of Atmospheric Neutrinos at MINOS Two MINOS Atmospheric Analyses.

Atmospheric Neutrinos MINOS MINOS Far Detector Type of Atmospheric Neutrinos at MINOS Two MINOS Atmospheric Analyses. Atmospheric Neutrinos MINOS MINOS Far Detector Type of Atmospheric Neutrinos at MINOS Two MINOS Atmospheric Analyses 1 Produced in the atmosphere from interactions of primary cosmic rays. p + N π ± + X

More information

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

Measuring the neutrino mass hierarchy with atmospheric neutrinos in IceCube(-Gen2) Measuring the neutrino mass hierarchy with atmospheric neutrinos in IceCube(-Gen2) Beyond the Standard Model with Neutrinos and Nuclear Physics Solvay Workshop November 30, 2017 Darren R Grant The atmospheric

More information

The First Results of K2K long-baseline Neutrino Oscillation Experiment

The First Results of K2K long-baseline Neutrino Oscillation Experiment The First Results of K2K long-baseline Neutrino Oscillation Experiment Taku Ishida, representing K2K collaboration arxiv:hep-ex/0008047v1 23 Aug 2000 Institute for Particle and Nuclear Studies(IPNS) High

More information

XMASS: a large single-phase liquid-xenon detector

XMASS: a large single-phase liquid-xenon detector XMASS: a large single-phase liquid-xenon detector Katsuki Hiraide, the university of Tokyo for the XMASS Collaboration October 3 rd, 2016 IPRD16@Siena, Italy 1 XMASS project XMASS: a multi purpose experiment

More information