1 / 9

Outline

Outline. Neutrino History n Oscillations World Tour of n Experiments Solar n Atmospheric n Long-Baseline Accelerator n Nu opportunities Superbeams/ n factories. Testing Oscillations.

izzy
Download Presentation

Outline

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Outline • Neutrino History • n Oscillations • World Tour of n Experiments • Solar n • Atmospheric n • Long-Baseline Accelerator n • Nu opportunities • Superbeams/ n factories

  2. 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(q,Dm2) often x~ x(Pn1n2)

  3. What SNO tells us Super-K has measured nene, which is a mixture of NC&CC • NCnienie , i=e,m,t have same cross section • CCneenee only  they measure a mix of ne nmnt SNO measures primarily ned ppe (CC breakup) Together, one gets ftotal, fe • ftotal is not low

  4. nt interaction discovery • DONUT - Fermilab beam dump experiment published 2000 • nt expected from Dstnt decay • 203 n events in photographic emulsion • See 4 events, expect 4.1  1.4 • Background from charm & hadrons 0.41  0.15

  5. What we know: q23~45o; Dm223~.001-.01 eV2 q12 &Dm223 SMA, LMA, LOW or just-so sin2q13 < 0.05 What we want to know Dm223 better Which solar solution? See oscillations See t’s ---------------------------------------- see q13 or limit to 10-3 CP violation Matter effects Sign of Dm223 The truth about n’s

  6. 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 n source to the detector is much greater than the length of the decay pipe. • Useful (Physics) - L >> En/Dm2

  7. MINOS A neutrino beam from Illinois to Minnesota

  8. 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

  9. Conclusion • The n world is one in which there has been much recent progress (n mass; mixing). • New insights are expected soon (KamLAND, Borexino, K2K, MINOS) • Another round of experiments at “superbeams” and n factories will tell us more.

More Related