The NO n A Experiment 11 April 2014 P5 Meeting SLAC 21 February - - PowerPoint PPT Presentation

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The NO n A Experiment 11 April 2014 P5 Meeting SLAC 21 February - - PowerPoint PPT Presentation

NO A Commissioning Status and Plans NO A Publishing Readiness and Plans Gary Feldman 12 April 2014 Gary Feldman The NO n A Experiment 11 April 2014 P5 Meeting SLAC 21 February 2008 Gary Feldman Readiness We are well along in


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SLIDE 1

Gary Feldman

The NOnA Experiment

P5 Meeting SLAC 21 February 2008

NOνA Commissioning Status and Plans

Gary Feldman 12 April 2014

NOνA Publishing Readiness and Plans

Gary Feldman 11 April 2014

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SLIDE 2

Readiness

 We are well along in preparation:

 We have two different physics-based beam simulations and

the standard GEANT4 detector simulation.

 Track, shower, and vertex finding algorithms are well

advanced.

 We have two very different, but equally powerful, νe

identification algorithms, library matching and neural net, and a likelihood-based νµ identification algorithm.

 We have had one successful data challenge and are

planning another, which will include the full near detector- far detector extrapolation.

 We have established a set of rules for blind analyses.

Gary Feldman EMG 11 April 2014 2

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SLIDE 3

NuMI Beam

 Good progress toward final high intensity configuration.  Metric = (Design

+ 2*Base)/3

 FY14 metric =

3.24 x 1020 pot

 FY15 metric =

3.62 x 1020 pot

 NOνA nominal year

= 6 x 1020 pot

Gary Feldman EMG 11 April 2014 3

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SLIDE 4

Effective Mass for Physics

Gary Feldman EMG 11 April 2014 4

2 4 6 8 10 12 14 16 15-Apr 15-May 15-Jun 15-Jul 15-Aug 15-Sep 15-Oct 15-Nov kt

Effective Number of Diblocks (kt)

Shutdown

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SLIDE 5

Plans for First Results

 Data up to the shutdown.  Analysis complete November-December 2014  How much data?

 Beam projection is 1.9 x 1020 pot.  Average mass is 11 kt  Efficiency = 80% for water leaks and other teething problems.  = 1.2 x 1020 pot equivalent or 20% of a nominal NOνA year.

 In a nominal NOνA year we expect about 15 νe events x/÷ 2

depending on the physics parameters and about an equal background, half from misidentification and half from cosmic

  • rays. So we would expect about 3 signal events with 3

background.

Gary Feldman NOνA Collaboration Meeting 4 April 2014 5