Future Neutrino Beams at Fermilab Gina Rameika NNN10 Toyama, - - PowerPoint PPT Presentation

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Future Neutrino Beams at Fermilab Gina Rameika NNN10 Toyama, - - PowerPoint PPT Presentation

Future Neutrino Beams at Fermilab Gina Rameika NNN10 Toyama, Japan December 14-16, 2010 Outline Neutrinos and the Intensity Frontier Neutrino Beams at Fermilab Booster Neutrino Beam (BNB) : MiniBooNE NuMI : MINOS, MINERvA


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SLIDE 1

Future Neutrino Beams at Fermilab

Gina Rameika NNN10 – Toyama, Japan December 14-16, 2010

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SLIDE 2

Outline

  • Neutrinos and the Intensity Frontier
  • Neutrino Beams at Fermilab
  • Booster Neutrino Beam (BNB) : MiniBooNE
  • NuMI : MINOS, MINERvA
  • Near-term upgrades and operations
  • NuMI for NOvA
  • Proton economics and the BNB : MicroBooNE,

future expt.

  • Longer-term projects and prospects
  • LBNE
  • Project X

Rameika - NNN10 2

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SLIDE 3

Three Frontiers for U.S. Particle Physics

Rameika - NNN10 3

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SLIDE 4

Fermilab Intensity Frontier Experiments

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MINOS MiniBooNE MINERvA SeaQuest NOvA MicroBooNE g-2? SeaQuest Now 2016 LBNE Mu2e Project X+LBNE mu, K, nuclear, … Factory ?? 2013 2019 2022

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SLIDE 5

Present and Planned Accelerator Complex

Rameika - NNN10 5

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SLIDE 6

Rameika - NNN10 6

  • High energy protons hit a target
  • Unstable pion and kaon charged particles are produced
  • The pions and kaons are “focused” by a magnetic field

to go in the desired direction

  • The pions and kaons decay into muons and muon type

neutrinos

  • The direction of the magnetic field determines whether

neutrinos or anti-neutrinos are (predominantly) generated

Components of a conventional accelerator neutrino beam

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SLIDE 7

Booster Neutrino Beam (BNB)

Rameika - NNN10 7

Short baseline – Near surface

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SLIDE 8

BNB flux

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Small intrinsic rate  event ratio ~6x10-3

e e /µ

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SLIDE 9

Event spectra (for arbitrary POTs)

Rameika - NNN10 9

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SLIDE 10

Proton Delivery to BNB

Rameika - NNN10 10

Depends on other demands for the protons

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SLIDE 11

Neutrinos at the Main Injector (NuMI)

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Constructed 2000-2004 to send Neutrinos to Soudan, Minnesota For the MINOS experiment

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SLIDE 12

Rameika - NNN10 12

1200m 100m

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SLIDE 13

Components of the NuMI Beam

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Neutrino beam spectra is tunable by arrangement of target-horn separations

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SLIDE 14

POT delivery to NuMI

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~11x1017/day

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SLIDE 15

Off-axis Neutrino Beams

Rameika - NNN10 15

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SLIDE 16

NuMI to NOvA

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Need to upgrade the proton delivery rate to the NuMI target

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SLIDE 17

Accelerator and NuMI Upgrades (ANU) for NOvA

  • Changes to the FNAL Accelerator complex to
  • Turn Recycler from pbar to proton ring
  • Injection and extraction lines
  • Associated kickers and instrumentation
  • 53 MHz RF
  • Decommission/remove pbar devices
  • Shorten MI cycle to 1.33 seconds
  • RF upgrades
  • Power Supply upgrades
  • Decommission/remove pbar devices
  • NuMI target station to 700 kW
  • Target & Horns to handle power
  • Configuration to maximize neutrino flux (Medium

Energy configuration)

Rameika - NNN10 17

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SLIDE 18

Context of ANU

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  • Collider Era operation: 11 booster batches (2 to pbar), 3.5e13 on target, 2.2

second cycle

18

  • NOvA Era operation: 12 booster batches, 4.9e13 on target, 1.33 second

cycle 5 Hz from Booster 7.8e16/hour 9 Hz from Booster 1.4e17/hour

No cycles to the BNB in this plan

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SLIDE 19

Rameika - NNN10 19 Mike Martens, NOvA Target and Horns 19

Primary Beamline Horn Power Supply

Target Pile Air Cooling System

(above shielding)

Target & Baffle Work Cell

(above shielding)

Horn 1 Horn 2 Low Energy Configuration

Stripline

Horn

  • Med. Energy

Configuration

Morgue

NuMI Design

NOvA†

Beam Power (kW)

400 700

Energy Spectrum Low Energy Medium Energy Cycle time (s)

1.87 1.33

Intensity (ppp)

4.0×1013 4.9×1013

Spot Size (mm)

1.0 1.3

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SLIDE 20

Rameika - NNN10 20

Baffle: Minor Changes

Aperture Increased from 11 mm to 13 mm diameter Alternative Clamp Material

Target: New Design

No Remote Longitudinal Motion Larger Target Casing Same Graphite Material, but wider target fins

Carrier: New Design

No Remote Longitudinal Motion Simpler Construction

Horn 1: Modifications for 700 kW

Thinner Outer Conductor Modified Stripline Geometry Additional Spray Cooling

Horn 2 : No Change

20

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SLIDE 21

NOvA Numbers

  • “700 kW” peak
  • 4.3e12 protons/batch from Booster
  • 12 spills every 4/3 second = 9 Hz
  • 13.9e16 p/hr.
  • 95% efficiency in MI
  • Comes out to 707 kW
  • Booster has never provided this much
  • 6e20 Protons per year
  • 44 weeks of running
  • 61% total efficiency
  • Downtimes (accelerator and NuMI)
  • Average vs peak
  • Getting NOvA protons means that both the peak proton power

and the efficiency need to be maximized

Rameika - NNN10 21

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SLIDE 22

Current Booster Performance

  • ~7.5 Hz (6.7 Hz w/ beam)

Hardware capable of ~9 Hz

  • 1e17/hour (pushing administrative operational limits):

aperture improvements and loss reduction

  • 89% efficiency

Rameika - NNN10 22

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SLIDE 23

Outlook for Booster Performance

  • The Booster appears presently able to produce about 13e16 protons/

hr at peak power

  • Within ~10% of NOvA peak demand
  • Recent Record week: 1.62e19 protons (9.6e16 p/hr)
  • Good operational efficiency
  • Limited by beam budget
  • Reliability becomes an increasing issue as rep rate increases
  • Not only a radiation problem
  • Magnitude of this effect is not understood
  • Another looming issue is additional users
  • mu2e @ 4.5 Hz (same or higher batch intensity)
  • MicroBooNE at up to 5 Hz
  • g-2 at up to 4 Hz
  • These can add up to easily 22e16 if Booster runs at 15 Hz
  • Not enough cycles to service all experiments simultaneously
  • Booster reliability is an issue

Rameika - NNN10 23

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SLIDE 24

Prospects for Increased Intensity

  • Booster performance has been improving, but

must remain an issue for future operation

  • Per batch intensity is at NOvA levels
  • Running rate is near the (present) operational limit
  • Extrapolating from the overhead in loss rates puts

Booster performance near NOvA levels (at peak)

  • Reliability of running at higher rates is a significant

question and is not accounted for in the extrapolation

  • Further experiments provide an additional risk
  • New study group formed
  • What needs to be done to make the Booster run for ~15

years?

  • What can be done to improve intensity reliability

Rameika - NNN10 24

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SLIDE 25

Rameika - NNN10 25

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SLIDE 26

From Report Summary

Rameika - NNN10 26

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SLIDE 27

Rameika - NNN10 27

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SLIDE 28

The Plan

  • To support program operation through 2025
  • Both the 8 GeV and the 120 GeV programs do need

additional improvements

 Booster Solid State Upgrade

 Improved reliability of RF Power Amplifiers

 Increase repetition rate to 15 Hz

 Improved electrical infrastructure  Improved cooling for RF cavities  Requires solid state upgrade

 New shielding assessment and associated shielding improvements

 Operational limits  Additional shielding in tunnel  Office occupancy

Rameika - NNN10 28

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SLIDE 29

NOvA Timeline

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When 700kW operation begins depends on if the Tevtron collider runs past 2011 2011 2012 2013 2014 2015 2016 Requires $$$ for collider ops

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SLIDE 30

BNB/MicroBooNE Timeline

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Proton Intensity and running time depend on Collider schedule and NOvA readiness and run plan

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SLIDE 31

Take Away

  • Intensity frontier neutrino program for the next

decade puts demands on the accelerator complex

  • Improvements in both hardware and operational

efficiency of the Booster complex will be required if the currently approved physics program is to be successful

Rameika - NNN10 31

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SLIDE 32

2008 P5 Report

Rameika - NNN10 32

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SLIDE 33

Fermilab to Homestake Mine – 1300km

Rameika - NNN10 33

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SLIDE 34

Why longer baseline is better

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(GeV)

!

E 1 10 POT

21

CC evts/GeV/100kT/10

!

! 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000

2

= 2.5e-03 eV

31 2

m " CC spectrum at 1300km,

!

! Appearance Probability 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1

/2 # =

cp

$ = 0.02,

13

% 2

2

sin =0

cp

$ = 0.02,

13

% 2

2

sin

/2 # =-

cp

$ = 0.02,

13

% 2

2

sin

= n/a

cp

$ =0,

13

% 2

2

sin (GeV)

!

E 1 10 POT

21

CC evts/GeV/100kT/10

!

! 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000

2

= -2.5e-03 eV

31 2

m " CC spectrum at 1300km,

!

! Appearance Probability 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1

/2 # =

cp

$ = 0.02,

13

% 2

2

sin =0

cp

$ = 0.02,

13

% 2

2

sin

/2 # =-

cp

$ = 0.02,

13

% 2

2

sin

= n/a

cp

$ =0,

13

% 2

2

sin

s

e

  • Number of

50 100 150 200 250 300 350 400

  • bars

e

  • Number of

20 40 60 80 100 120 140 160 180 200

=1.

  • bar, 700kW, 10kT
  • , 5yr
  • 1300km, 5yr

NH IH

s

e

  • Number of

50 100 150 200 250 300 350 400

  • bars

e

  • Number of

10 20 30 40 50 60 70 80 90 100

=1.

  • bar, 700kW, 10kT
  • , 5yr
  • 5yr

1300km 810km

sin2 2θ13 = 0.08,0.04,0.02,0.01

sin2 2θ13 = 0.04

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SLIDE 35

Rameika - NNN10 35

NEW

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SLIDE 36

Rameika - NNN10 36

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SLIDE 37

Rameika - NNN10 37

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SLIDE 38

Neutrino Beam Components

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Reference design for CDR Cost & Schedule Horn PS can switch polarity via control system Nu-nubar data in same time period

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SLIDE 39

Rameika - NNN10 39

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SLIDE 40

Rameika - NNN10 40

This intensity implies that The Long Baseline Exp. will need to run for a LONG time

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SLIDE 41

Rameika - NNN10 41

NEW Radiation exposures

Why 2.3 MW?

Need a plan to deal with the proton economics and ageing Accelerator complex

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SLIDE 42

Project X Mission

  • A neutrino beam for long baseline neutrino oscillation

experiments

  • 2 MW proton source at 60-120 GeV
  • High intensity, low energy protons

for kaon and muon based precision experiments

  • Operations simultaneous with the

neutrino program

  • A path toward a muon source for

possible future Neutrino Factory and/or a Muon Collider

  • Requires ~4 MW at ~5-15 GeV .
  • Possible missions beyond P5
  • Standard Model Tests with nuclei and energy applications

Rameika - NNN10 42

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SLIDE 43

Project X Reference Design

Rameika - NNN10 43

This design has emerged

  • ver a 3 year period
  • f consideration of various
  • ptions
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SLIDE 44

Project X Scope

  • 3 GeV CW superconducting H- linac, capable of delivering 1

mA average beam current.

  • Flexible provision for variable beam structures to multiple users
  • Starts at ion source; ends at 3-way split (with stubs)
  • Supports rare processes programs
  • Provision for 1 GeV extraction for nuclear energy program
  • 3-8 GeV pulsed linac capable of delivering 300 kW at 8 GeV
  • Supports the neutrino program
  • Establishes a path toward a muon based facility
  • Upgrades to the Recycler and Main Injector to provide

≥ 2 MW to the neutrino production target at 60-120 GeV.

  • Ends at MI extraction kicker
  • Supports the long baseline neutrino program
  • All interconnecting beamlines

Rameika - NNN10 44

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SLIDE 45

LBNE Project Time Line

  • DOE CD-0 (Approve Mission Need)

January 2010

  • CD-1 2nd half CY2011*
  • CD-2 (Project baseline) depending on

funding . . . mid/late FY2013

  • CD-3 (start construction) depending
  • n funding . . . 2014 ~ 2015
  • Project complete : no sooner than 2020

Rameika - NNN10 45

Currently dealing with TPC (total project funding) issues and DOE-NSF partnership issues

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SLIDE 46

Project X Timeline

  • Assumed Critical Decision dates
  • CD-0: January 2011
  • CD-1: July 2012
  • CD-2: August 2013
  • CD-3: September 2014
  • CD-4: September 2019

Project X could also be up and running in ~2020 : All depends on funding profiles…

Rameika - NNN10 46

5 yr construction

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SLIDE 47

Evolution of the Intensity Frontier : it’s all about the protons

Rameika - NNN10 47

20x1020 POT/yr 10x1020 POT/yr : not current plan 6 - 7x1020 POT/yr 3x1020 POT/yr

NuMI to MINOS

ProjectX