BNL neutrino beam. Optimization and simulations Milind Diwan June 10.

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Presentation transcript:

BNL neutrino beam. Optimization and simulations Milind Diwan June 10

What was done Geant 3.0 simulations with details of horn geometry including materials. 180 m tunnel with 4 meter diameter Default parameters not quite the same as rest of report. pbeam study of parameters.

List of parameters for GEANT simulation target: radius: 3.2 mm, length: 60 cm, den:2.2 gm/cc beam: 28 GeV, radius: 1 mm horn: gap: 1 mm, H1length: 2.2m, H2length: 1.5 m tunnel: radius: 2 m, length: 180 m, Air- filled 2 horn distance: 8.3 m

Flux: things to optimize Total flux or event rate Width of flux: as wide as possible electron neutrino contamination: as low as possible.

Anti-neutrinos Lower event rate => 2 MW Much larger neutrino contamination. 30% of events due to wrong sign.

Canonical event rates 1.12e22 protons, 500 kT, 2540 km Neutrinos: CC: 52000, NC: Anti-neutrinos: CC: 14000, NC: 5400 Assumes extrapolation as 1/2540**2

Concerns Uncertainty on total flux or event rate probably still 20-30%. Large (50%) uncertainty above 4 GeV. Is off-axis running at all possible ? Can all be addressed by more beam power.

Hadronic models Good news: less backg at low energy. Bad news: less signal at high energy. Needs study

Data on beam ? E734 target Cu, different Horn design E734 data suggests enough flux at GeV GEANT MC

Ways to gain or lose high E flux Same flux if vacuum; lose 3-5% in window. if 1/8” thick steel window Gain 15%

Tunnel dimensions Lose low E by making narrow Gain high E by making longer

Horn placement and current Lose Low E if current goes beyond 500 kA Gain high E by placing horn 2 farther. Third horn ? But no He?

Target and beam dimension 6 mm/2mm good compromise Must take care to control beam size. 3mm6mm8mm 1mm mm mm Target rad. beam rad. Flux in arb. units Top: tot. flux; bot:>3 GeV

Target placement and gap Lose low E if target pushed in Lose low E if gap too large

What needs to be done Much better understanding of hadronic production. Much more detail of shielding and tunnel shape in the simulation. New simulation with optimized choices for parameters. 5 physicists needed for 2 years to perform studies and interface with AGS