the neutrino oscillation industry
Post on 31-Dec-2015
53 Views
Preview:
DESCRIPTION
TRANSCRIPT
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
Sources• Solar (made by nuclear fusion in the sun)
• Atmospheric • Accelerator • Supernova • Cosmological remnant • Reactor • Energetic Astrophysical Systems
The Neutrino Oscillation Industry
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
SNO
Water around Heavy Water (D2O)
Acrylic Vessel
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
MINOS
A neutrino beam fromIllinois to Minnesota
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
Outline
Neutrino HistoryOscillationsWorld Tour of Experiments
Solar Atmospheric Long-Baseline Accelerator
Nu opportunities– Superbeams/ factories
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
Testing Oscillations
In the design of any neutrino oscillation experiment, you want to measure something (x) which will be different if oscillations exist;
e.g. Nevent , R=NC/CC, Nkink
In general, x = x(,m2)
often x~ x(P12)
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
What SNO tells us
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
interaction discovery
• DONUT - Fermilab beam dump experiment published 2000
• expected from Ds decay
• 203 events in photographic emulsion • See 4 events, expect 4.1 • Background from charm & hadrons
0.41
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
Atmospheric ‘s
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
The truth about ’s
What we know:23~45o;
m223~.001-.01 eV2
12 & m223 SMA, LMA,
LOW or just-sosin213 < 0.05
What we want to knowm2
23 better
Which solar solution? See oscillations See’s------------------------------------------------
see 13 or limit to 10-3
CP violation Matter effects Sign of m2
23
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
How Long is Long?
Definitions of “Long-Baseline”(my use is for accelerator based experiments)
• Webster - (long - measuring much, or more than usual, from end-to-end in space or time)
• Practical - Off site
• Useful (Beam) - The distance from the source to the detector is much greater than the length of the decay pipe.
• Useful (Physics) - L >> E/m2
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
Advertisement
• Free monthly neutrino rumor newsletter --~100 lines, send “subscribe” to maury.goodman@anl.gov or see http://www.hep.anl.gov/ndk/longbnews/
• Neutrino Oscillation Industry Web Page http://www.hep.anl.gov/ndk/hypertext/nuindustry.html
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
Future spectra
Title:arXiv:hep-ph/0103052 v2 6 Mar 2001Creator:dvips(k) 5.86 Copyright 1999 Radical Eye SoftwarePreview:This EPS picture was not savedwith a preview included in it.Comment:This EPS picture will print to aPostScript printer, but not toother types of printers.
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
Superbeams
need $ on powerful proton drivers (0.5-4MW)
e.g. BNL to Homestake (SD) or WIPP (New Mexico)
JHF to Super-Kamiokande
Fermilab to Soudan/Homestake/WIPPmore protons yield more ’schallenges: target cooling; ground water radiation;
accelerator and power costs; e backgrounds
reach in sin22
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
factory
Physics Colloquium-28 November 2001
•“The Neutrino Oscillation Industry” Maury Goodman, Argonne National Lab
Conclusion
The world is one in which there has been much recent progress ( mass; mixing).
New insights are expected soon (KamLAND, Borexino, K2K, MINOS)
Another round of experiments at “superbeams” and factories will tell us more.
top related