NeSS02 neutrinos

Information about NeSS02 neutrinos

Published on December 6, 2007

Author: Justine

Source: authorstream.com

Content

Neutrino Oscillations and Mass, and CP Violations:  Neutrino Oscillations and Mass, and CP Violations Review the status and prospects for measurements of the neutrino masses and mixings. Mainly concentrating on terrestrial neutrino beam sources How does this couple to an underground laboratory? Neutrino Oscillation Measurements:  q13 key parameter for osc. phenomenolgy since q12 and q23 are both large Determines whether CP violation is accessible Neutrino Oscillation Measurements Atmospheric: q23 Solar: q12 ??? Solar and Atmospheric results determine Dm122, q12, Dm232, q23 Why Are Neutrino Oscillation Measurements Important?:  Why Are Neutrino Oscillation Measurements Important? Give a window on physics at high mass scales: unification, physics of flavor, and extra dimensions Why are the neutrino masses so small? Are there additional “sterile” neutrinos? Why are their mixings so large? Is there a connection between the lepton and baryon sector? Is there CP violation, T violation, or CPT violation in the leptons? Neutrino masses and mixing are important to understanding astrophysical models of: Supernovae, galactic structure formation, etc. Should remember that neutrino oscillations only measure mass differences (m12-m22) Need tritium decay (KATRIN) or double beta decay to measure one mass  Are n masses hierarchical or degenerate? Neutrino Masses: Theoretical Ideas:  Neutrino Masses: Theoretical Ideas No fundamental reason why neutrinos must be massless But why are they much lighter than other particles? Modified Higgs sector to accommodate neutrino mass Extra Dimensions Neutrinos live outside of 3 + 1 space Grand Unified Theories Dirac and Majorana Mass  See-saw Mechanism Many of these models have at least one Electroweak isosinglet n Right-handed partner of the left-handed n Mass uncertain from light (< 1 eV) to heavy (>1016 eV) Would be “sterile” – Doesn’t couple to standard W and Z bosons Need neutrino oscillations to measure small neutrino masses Matter-Antimatter Asymmetry (B  0) from Leptogenesis:  Matter-Antimatter Asymmetry (B  0) from Leptogenesis Hard to generate a baryon asymmetry (B  0) using quark matrix CP violation Generate L  0 using CP or CPT violation in the lepton sector B-L processes then convert a neutrino excess to baryon excess. Sign and magnitude may be able to generate the observed baryon asymmetry in the universe d gives CP violation Why? Neutrino Oscillation Experiments:  Neutrino Oscillation Experiments Current Oscillation Experiments K2K nm dissappearance 250km from KEK to SuperK detector MiniBooNE nm ne appearance in the LSND Dm2 region NuMI/Minos at Fermilab and CNGS at CERN Long-baseline (~750km) nm experiments in atmospheric Dm2 region Near term offaxis experiments JHF to SuperK Offaxis experiment – 22kton detector NuMI/Minos Offaxis experiment (Proposed) – ~20kton detector Neutrino Superbeam Experiments (Combine with large p-decay detectors?) BNL (AGS upgrade) to NUSL Fermilab (proton driver upgrade) to NUSL JHF(Phase II) to HyperK at Kamiokande laboratory CERN SPL (Supercond. Proton Linac) to Frejus Future Neutrino Factory using a muon storage ring. Strawperson Roadmap:  Strawperson Roadmap Stage 0: Current near term program NuMI (K2K) checks atmospheric oscillations and measures m223 to about 10% MiniBooNE makes definitive check of LSND and measures associated m2 Stage 1 - Constrain / measure sin2213 NuMI /MINOS on-axis probes sin2213> 0.06 @ 90%CL NuMI/JHF offaxis could go down to sin2213> 0.01 @ 90%CL FNAL to NUSL with 100kton detector? Stage 2 - Measure CP violation and sign of m223 with conventional superbeams and very large detectors (500 to 1000ktons) Must have sin2213> 0.01 Need to measure P(e) then P(e) Need increased rate (especially for n’s)  Need high intensity proton sources Stage 3 - Measurements with Neutrino Factory Map out CP violation with precision for sin2213> 0.01 Probe e transitions down to sin2213> 0.001 Requirements for Neutrino Oscillation Experiments:  Requirements for Neutrino Oscillation Experiments Need high intensity beam with energy tuned at the oscillation maximum for the given baseline. Neutrino sources (Labs) and possible detector sites Many detector technologies do not need to be underground Due to beam duty cycle, only need small overburden to reduce cosmic background Superbeam experiments measuring CP violation require very large, costly detectors Couple detectors to p-decay, supernova, etc. measurements  Detector needs to be in an Underground Lab Detector technology needs to be compatible with p-decay etc. but compromises may be necessary Water Cerenkov Detector or Liquid Argon Detector If MiniBooNE Confirms LSND:  If MiniBooNE Confirms LSND Three distinct Dm2 values  How do we fit everything in? Need more long and short-baseline experiments Difficult to fit everything with the three standard neutrinos But may be uncertainties in some of the Dm2 measurements or other explanations for one of the oscillation results? Need accurate Dm2 and oscillatory behavior measurements Terrestrial nm and ne beams and reactor sources Sterile Neutrinos (Add one or more sterile neutrinos) Sterile/active mixing Need better measurements of sterile component in “solar” and “atmospheric” oscillations CPT violation LSND measures anti-neutrino oscillations and Solar experiments measure neutrino oscillations  Need to make measurements with both neutrino and anti-neutrino sources ( + KAMLAND) Neutrino Oscillation Program Thru ~2010:  Neutrino Oscillation Program Thru ~2010 Pursue oscillation parameter measurements with longbaseline experiments! Need to measure sin2q13, sign of m223, and probe for CP violation Some information will come from on-axis experiments at Fermilab/CERN For example, NuMI/Minos has sensitivity for sin2213> 0.06 @ 90%CL Off-axis experiments (Probe sin2213> 0.01 @ 90%CL) Off-axis gives beam with narrow energy distribution that is tunable JHF to SuperK Fermilab NuMI to Offaxis detector May also see first signs of CP violation Combination of two baselines (JHF and NuMI) may be important for removing correlations and ambiguities Sensitivity of Off-Axis NuMI and JHF:  Sensitivity of Off-Axis NuMI and JHF NuMI Offaxis Sensitivity: 5yrs @ 4x1020 p/yr with 20 kton detector Above event samples assume sin22q13=0.1 and Dm2 = 3x10-3eV2 JHF Offaxis Sensitivity: 5yrs with JHF Phase I and SuperK detector Next Step: Neutrino Superbeam Experiments:  Next Step: Neutrino Superbeam Experiments If sin2213> 0.01, design experiment to measure d (CP violation parameter) and the sign of m223 Need high intensity proton sources coupled with very large underground combined function detectors JHF Phase II to HyperK detector <En>700 MeV beam using 4MW JHF to 1000kton water Cerenkov CP violation 3s discovery reach for sin22q13>0.02 (2yr for nu’s and 6 yrs for nubars) BNL Upgraded AGS to NUSL Very longbaseline with wide-band beam gives dramatically large effects Use 1MW AGS beam with 0.5<En<5 GeV and 500 kton water Cerenkov Combined oscillation measurements for the 1st,2nd,3rd….. osc. maximum gives 0.5-1 GeV Solar LMA, 1-3 GeV CP effects, 3-5 GeV matter effects Fermilab Proton Driver to NUSL Upgrade proton driver to 1-4MW combined with 500kton water Cerenkov or Liq. Argon  Fit first and second maximum for neutrinos and antineutrinos Possibly also NuMI to Canada CERN SPL to UNO-type detector at Frejus <En>250MeV with L=133km for 5 years UNO-type detector (660tons)  sin2213> 0.002 @ 90%CL Example Sensitivities for Superbeam Experiments:  Example Sensitivities for Superbeam Experiments Can measure dCP to  Summary of Neutrino Osc. In an Underground Lab:  Summary of Neutrino Osc. In an Underground Lab If CP violation is accessible experimentally, a very high-intensity neutrino superbeam coupled with a ~500 kton detector in an underground lab will be important for precision measurements It is natural to couple the detector to a p-decay experiment which would need to be constructed in an underground Lab. Program will cost on order ~$1Billion for detector and beam. But the combined scientific measurements from such an experiment are really impressive and important Unique way to probe physics at ultra high energy scales through proton decay and neutrino mass measurements May provide the key to understanding the baryon asymmetry in the universe

Related presentations


Other presentations created by Justine

Flex PLM 2004
27. 11. 2007
0 views

Flex PLM 2004

osa slides 041215
28. 11. 2007
0 views

osa slides 041215

ps ria
01. 12. 2007
0 views

ps ria

344
10. 12. 2007
0 views

344

Understanding Islam
05. 11. 2007
0 views

Understanding Islam

halloween 4
05. 11. 2007
0 views

halloween 4

catering
05. 11. 2007
0 views

catering

schwarz
15. 11. 2007
0 views

schwarz

DKGRAN02
16. 11. 2007
0 views

DKGRAN02

linux firewall
26. 11. 2007
0 views

linux firewall

506 EMF Concerns
18. 12. 2007
0 views

506 EMF Concerns

thebusinesscase
28. 11. 2007
0 views

thebusinesscase

Security Openess
25. 12. 2007
0 views

Security Openess

sca02
29. 12. 2007
0 views

sca02

MPH 2005
29. 12. 2007
0 views

MPH 2005

bsc201 week09
01. 01. 2008
0 views

bsc201 week09

robot cwe
02. 01. 2008
0 views

robot cwe

Cotton
07. 01. 2008
0 views

Cotton

Energy in the Cell
07. 01. 2008
0 views

Energy in the Cell

SleepDisorders
29. 11. 2007
0 views

SleepDisorders

HydrothermalVentsand OilPlumes
09. 10. 2007
0 views

HydrothermalVentsand OilPlumes

CCH20AgFor
31. 12. 2007
0 views

CCH20AgFor

CS202Last2006Grokste rDMCA
26. 02. 2008
0 views

CS202Last2006Grokste rDMCA

General Marshall revised
28. 02. 2008
0 views

General Marshall revised

apr11 ticoll
11. 03. 2008
0 views

apr11 ticoll

wc game
12. 03. 2008
0 views

wc game

AAIupdateJan06
14. 03. 2008
0 views

AAIupdateJan06

Yr7GermanAssign
18. 03. 2008
0 views

Yr7GermanAssign

Art Millet
01. 10. 2007
0 views

Art Millet

TEFinal3
30. 03. 2008
0 views

TEFinal3

U S Economic History
13. 04. 2008
0 views

U S Economic History

apco presentation 2
02. 11. 2007
0 views

apco presentation 2

Yu sdm 2006 ft
21. 11. 2007
0 views

Yu sdm 2006 ft

78
05. 12. 2007
0 views

78

holiday safety tips
29. 11. 2007
0 views

holiday safety tips

NOFA 5 MAR 05
27. 12. 2007
0 views

NOFA 5 MAR 05

module2
07. 01. 2008
0 views

module2

cryptographie camp
05. 01. 2008
0 views

cryptographie camp

Bell 1
08. 11. 2007
0 views

Bell 1

ASegal
28. 12. 2007
0 views

ASegal

RTH Beijing
27. 09. 2007
0 views

RTH Beijing

Sturgeon
07. 01. 2008
0 views

Sturgeon

Recommenders HCC01
23. 12. 2007
0 views

Recommenders HCC01