MiniBooNE: (Anti)Neutrino Appearance and Disappeareance Results SUSY11 01 Sep, 2011 Warren Huelsnitz, LANL 1.

Slides:



Advertisements
Similar presentations
Neutrinos from kaon decay in MiniBooNE Kendall Mahn Columbia University MiniBooNE beamline overview Kaon flux predictions Kaon measurements in MiniBooNE.
Advertisements

1 3+2 Neutrino Phenomenology and Studies at MiniBooNE PHENO 2007 Symposium May 7-9, 2007 U. Wisconsin, Madison Georgia Karagiorgi, Columbia University.
MINOS+ Sterile Neutrino Studies J.Thomas UCL J.Evans (UCL), A.Gavrilenko (W&M), M.Matthis (W&M)A.Sousa(Harvard) UCL.
05/31/2007Teppei Katori, Indiana University, NuInt '07 1 Charged Current Interaction measurements in MiniBooNE hep-ex/XXX Teppei Katori for the MiniBooNE.
P AUL N IENABER S AINT M ARY ’ S U NIVERSITY OF M INNESOTA FOR THE M INI B OO NE C OLLABORATION J ULY DPF2009.
11-September-2005 C2CR2005, Prague 1 Super-Kamiokande Atmospheric Neutrino Results Kimihiro Okumura ICRR Univ. of Tokyo ( 11-September-2005.
H. Ray, University of Florida1 MINIBOONE  e e .
Miami 2010 MINIBOONE  e e  2008! H. Ray, University of Florida.
MINERvA Overview MINERvA is studying neutrino interactions in unprecedented detail on a variety of different nuclei Low Energy (LE) Beam Goals: – Study.
Sam Zeller, NO-VE Workshop, 02/07/06 1 Neutrino and Antineutrino Cross Sections at MiniBooNE Sam Zeller Columbia University (for the MiniBooNE collaboration)
Sinergia strategy meeting of Swiss neutrino groups Mark A. Rayner – Université de Genève 10 th July 2014, Bern Hyper-Kamiokande 1 – 2 km detector Hyper-Kamiokande.
LSND/MiniBooNE Follow-up Experiment with DAEdALUS W.C. Louis Los Alamos National Laboratory August 6, 2010.
DPF Victor Pavlunin on behalf of the CLEO Collaboration DPF-2006 Results from four CLEO Y (5S) analyses:  Exclusive B s and B Reconstruction at.
F.Sanchez (UAB/IFAE)ISS Meeting, Detector Parallel Meeting. Jan 2006 Low Energy Neutrino Interactions & Near Detectors F.Sánchez Universitat Autònoma de.
SBNW11 Summary June 23, 2011 Louis – Experimental Results & Theoretical Interpretations Van de Water – Future Facilities & Experiments.
1 CC analysis update New analysis of SK atm. data –Somewhat lower best-fit value of  m 2 –Implications for CC analysis – 5 year plan plots revisited Effect.
First Results from MiniBooNE May 29, 2007 William Louis Introduction The Neutrino Beam Events in the MiniBooNE Detector Data Analysis Initial Results Future.
10/24/2005Zelimir Djurcic-PANIC05-Santa Fe Zelimir Djurcic Physics Department Columbia University Backgrounds in Backgrounds in neutrino appearance signal.
1 Updated Anti-neutrino Oscillation Results from MiniBooNE Byron Roe University of Michigan For the MiniBooNE Collaboration.
MiniBooNE Update Since Last PAC Meeting (Nov 2007) Steve Brice (FNAL) PAC Meeting 27 March 2008.
Atmospheric Neutrino Oscillations in Soudan 2
MINERvA Overview MINERvA is studying neutrino interactions in unprecedented detail on a variety of different nuclei Low Energy (LE) Beam Goals: – Study.
MiniBooNE Results & Future Experiments MiniBooNE Introduction Neutrino Oscillation Results MiniBooNE NuMI Data Antineutrino Oscillation Results Future.
5/1/20110 SciBooNE and MiniBooNE Kendall Mahn TRIUMF For the SciBooNE and MiniBooNE collaborations A search for   disappearance with:
The Muon Neutrino Quasi-Elastic Cross Section Measurement on Plastic Scintillator Tammy Walton December 4, 2013 Hampton University Physics Group Meeting.
Results and Implications from MiniBooNE LLWI, 25 Feb 2011 Warren Huelsnitz, LANL
Neutrino Oscillation Results from MiniBooNE Joe Grange University of Florida.
05/09/2011Teppei Katori, MIT1 Teppei Katori Massachusetts Institute of Technology Phenomenology 2011 symposium (Pheno11), Madison, WI, May 9, 2011 Test.
A Decade Later: Are We Any Closer to Resolving the LSND Puzzle? BNL Seminar September 23, 2010 Richard Van de Water, LANL, P-25 P-25 Subatomic Physics.
Monday, Feb. 24, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #11 Monday, Feb. 24, 2003 Dr. Jae Yu 1.Brief Review of sin 2  W measurement 2.Neutrino.
B c mass, lifetime and BR’s at CDF Masato Aoki University of Tsukuba For the CDF Collaboration International Workshop on Heavy Quarkonium BNL.
Sterile Neutrino Oscillations and CP-Violation Implications for MiniBooNE NuFact’07 Okayama, Japan Georgia Karagiorgi, Columbia University August 10, 2007.
Dec. 13, 2001Yoshihisa OBAYASHI, Neutrino and Anti-Neutrino Cross Sections and CP Phase Measurement Yoshihisa OBAYASHI (KEK-IPNS) NuInt01,
MiniBooNE Michel Sorel (Valencia U.) for the MiniBooNE Collaboration TAUP Conference September 2005 Zaragoza (Spain)
Teppei Katori Indiana University Rencontres de Moriond EW 2008 La Thuile, Italia, Mar., 05, 08 Neutrino cross section measurements for long-baseline neutrino.
1 MiniBooNE Update and Extension Request Richard Van de Water and Steve Brice for the MiniBooNE Collaboration Nov 2, 2007.
Preliminary Results from the MINER A Experiment Deborah Harris Fermilab on behalf of the MINERvA Collaboration.
MiniBooNE Oscillation Searches Steve Brice (Fermilab) for the MiniBooNE Collaboration Neutrino 2008.
Latest Results from the MINOS Experiment Justin Evans, University College London for the MINOS Collaboration NOW th September 2008.
MiniBooNE Cross Section Results H. Ray, University of Florida ICHEP Interactions of the future!
New Results from the Salt Phase of SNO Kathryn Miknaitis Center for Experimental Nuclear Physics and Astrophysics, Univ. of Washington For the Sudbury.
Search for Electron Neutrino Appearance in MINOS Mhair Orchanian California Institute of Technology On behalf of the MINOS Collaboration DPF 2011 Meeting.
Recent results from SciBooNE and MiniBooNE experiments Žarko Pavlović Los Alamos National Laboratory Rencontres de Moriond 18 March 2011.
Results from RENO Soo-Bong Kim (KNRC, Seoul National University) “17 th Lomosonov Conference on Elementary Particle Physics” Moscow. Russia, Aug ,
A Letter of Intent to Build a MiniBooNE Near Detector: BooNE W.C. Louis & G.B. Mills, FNAL PAC, November 13, 2009 Louis BooNE Physics Goals MiniBooNE Appearance.
Search for Sterile Neutrino Oscillations with MiniBooNE
Beam Extrapolation Fit Peter Litchfield  An update on the method I described at the September meeting  Objective;  To fit all data, nc and cc combined,
1 Luca Stanco, INFN-Padova (for the OPERA collaboration) Search for sterile neutrinos at Long-BL The present scenario and the “sterile” issue at 1 eV mass.
Medium baseline neutrino oscillation searches Andrew Bazarko, Princeton University Les Houches, 20 June 2001 LSND: MeVdecay at rest MeVdecay in flight.
MiniBooNE MiniBooNE Motivation LSND Signal Interpreting the LSND Signal MiniBooNE Overview Experimental Setup Neutrino Events in the Detector The Oscillation.
Status of MiniBooNE Short Baseline Neutrino Oscillation Experiment Jonathan Link Columbia University International Conference on Flavor Physics October.
Outline: IntroJanet Event Rates Particle IdBill Backgrounds and signal Status of the first MiniBooNE Neutrino Oscillation Analysis Janet Conrad & Bill.
Results and Implications from MiniBooNE: Neutrino Oscillations and Cross Sections 15 th Lomonosov Conference, 19 Aug 2011 Warren Huelsnitz, LANL
Extrapolation Techniques  Four different techniques have been used to extrapolate near detector data to the far detector to predict the neutrino energy.
Future Sterile Neutrino Searches from Stopped Pions and Muons SNAC 11 VPI September 26-28, 2011 Gerry Garvey Los Alamos Nat. Lab.
Observation Gamma rays from neutral current quasi-elastic in the T2K experiment Huang Kunxian for half of T2K collaboration Mar. 24, Univ.
T2K Experiment Results & Prospects Alfons Weber University of Oxford & STFC/RAL For the T2K Collaboration.
Precision Measurement of Muon Neutrino Disappearance with T2K Alex Himmel Duke University for the The T2K Collaboration 37 th International Conference.
Recent Results from the T2K ND280 detector Jonathan Perkin on behalf of the T2K collaboration KAMIOKA TOKAI 295 km.
MINERνA Overview  MINERνA is studying neutrino interactions in unprecedented detail on a variety of different nuclei  Low Energy (LE) Beam Goals: t Study.
New Results from MINOS Matthew Strait University of Minnesota for the MINOS collaboration Phenomenology 2010 Symposium 11 May 2010.
1 Oscillations results from the MiniBooNE experiment Alexis Aguilar-Arévalo (ICN-UNAM), for the MiniBooNE collaboration SILAFAE December 2010,
R. Tayloe, Indiana University CPT '07 1 Neutrino Oscillations and and Lorentz Violation Results from MiniBooNE Outline: - LSND - signal for oscillations.
The XXII International Conference on Neutrino Physics and Astrophysics in Santa Fe, New Mexico, June 13-19, 2006 The T2K 2KM Water Cherenkov Detector M.
Systematics Sanghoon Jeon.
NESSiE and Muon Detection in magnetized Detectors
An Accelerator-Produced, Sub-GeV Dark Matter Search with the MiniBooNE Neutrino Detector Robert Cooper, New Mexico State University on behalf of the MiniBooNE.
F.Sánchez for the K2K collaboration UAB/IFAE
First Anti-neutrino results!
Impact of neutrino interaction uncertainties in T2K
Presentation transcript:

MiniBooNE: (Anti)Neutrino Appearance and Disappeareance Results SUSY11 01 Sep, 2011 Warren Huelsnitz, LANL 1

2 Electron Neutrino and Antineutrino Appearance Review of previous results Updated antineutrino appearance results Muon Neutrino and Antineutrino Disappearance Review of previous results New MiniBooNE/SciBooNE joint analysis

LSND Saw an excess of e : 87.9 ± 22.4 ± 6.0 events. With an oscillation probability of (0.264 ± ± 0.045)%. 3.8  evidence for oscillation. 3 The three oscillation signals cannot be reconciled without introducing Beyond Standard Model Physics!

Keep L/E same as LSND while changing systematics, energy & event signature P    e  sin   sin   m  L  Booster K+K+ target and horndetectordirtdecay regionabsorber primary beamtertiary beamsecondary beam (protons)(mesons)(neutrinos)    e   LSND: E ~ 30 MeV MiniBooNE: E ~ 500 MeV L ~ 30 m L/E ~ 1 L ~ 500 m L/E ~ 1 MiniBooNE was designed to test the LSND signal Neutrino mode: search for ν μ -> ν e appearance with 6.5E20 POT  assumes CP/CPT conservation Antineutrino mode: search for ν μ -> ν e appearance with 8.58E20 POT  direct test of LSND  Two neutrino fits FNAL FNAL has done a great job delivering beam! 818 ton mineral oil 1280 PMTs inner region 240 PMTs veto region 4

5

6

7

8 Reduces uncertainty. reduces uncertainty. (accepted by Phys. Rev. D)

9 search

10

11

12 Antineutrino Mode Low Energy Excess: How does it scale

13

14

15

16 Muon Neutrino & Antineutrino Disappearance

A.A. Aguilar-Arevalo et al., PRL 103, (2009) 17 Neutrino Antineutrino MiniBooNE Muon Neutrino & Antineutrino Disappearance Limits

18

19 Use the CC rate measured at SciBooNE to constrain the MiniBooNE rate and test for disappearance Two analysis methods: arXiv: (submitted to PRL) Simultaneous fit 1)Fit SciBooNE and MiniBooNE data simultaneously for oscillation 2)Constraint applied within fit, effectively removes systematic uncertainties shared by both detectors Spectrum fit 1)Extract neutrino energy spectrum from SciBooNE data Phys.Rev.D83:012005,2011 2)Apply correction to MiniBooNE energy spectrum 3)Fit for oscillation at MiniBooNE 4)Systematics reduced by extraction process

20

21 MiniBooNE like detector at 200m Flux, cross section and optical model errors cancel in 200m/500m ratio analysis Gain statistics quickly, already have far detector data Measure   e &   e oscillations and CP violation 6.5e20 Far + 1e20 Near POT Sensitivity (Neutrinos) Sensitivity (Antineutrinos) 10e20 Far + 1e20 Near POT (LOI arXiv: )

22 Much better sensitivity for  &  disappearance Look for CPT violation 6.5e20 Far/1e20 Near POT 10e20 Far/1e20 Near POT

23 Electron Neutrino and Antineutrino Appearance Significant excesses above background in both neutrino and antineutrino mode at low energy. With new data update, excess in antineutrino mode looks more like excess in neutrino mode. Antineutrino data are still consistent with LSND result; significance of oscillation signal relative to null is reduced. See also Georgia Karagiorgi’s talk from DPF 2011 for fits to 3+1 and 3+2 models, and non-standard interactions. Muon Neutrino and Antineutrino Disappearance SciBooNE data used in joint neutrino-mode analysis. Joint analysis underway for anti-neutrino mode; also taking advantage of improved reconstructions in MiniBooNE. Ultimately, would like to have two identical detectors at different distances for SBL disappearance to cover region of interest.

24 Backup slides

25

3 independent, complementary measurements   + /  - angular distribution   - capture    absorption (CC1   sample) 26 First measurement of neutrino contribution to anti-neutrino beam with non-magnetized detector: arxiv: [hep-ex], submitted to Phys. Rev. D (arXiv: )

27

28 Identify events using timing and hit topology Use primarily Cherenkov light Can’t distinguish electron from photon Charge Current Quasi Elastic Neutral Current Interactions in MiniBooNE (neutrino mode): (similar mix for antineutrino mode, except rate down by factor of 5) QE

29 Expected backgrounds (6.46 ⋅ POT) Every major source of background can be internally constrained by MiniBooNE

30

31

32

33

34

35

36

37

38 J. Grange, NuInt11 Antineutrino Cross Sections

Is the Neutrino Energy Estimated Correctly in CCQE? Amaro, et al, PHYSICAL REVIEW C 82, (2010) Meson Exchange Diags.Correlation Diags. 56 Fe, q=0.55GeV/c One body RFG 2p-2h fin. sts. Meson exchange Correlation Electron Scattering

40

41

42

43