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The Front End MAP Review Fermi National Accelerator Lab August 24-26, 2010 Harold G. Kirk Brookhaven...

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The Front End MAP Review Fermi National Accelerator Lab August 24-26, 2010 Harold G. Kirk Brookhaven National Laboratory
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The Front End

MAP Review

Fermi National Accelerator Lab August 24-26, 2010

Harold G. KirkBrookhaven National Laboratory

August 24-26, 2010MAP Review-Front End Harold G. Kirk

2

Outline

Define Front End

Major Sub-systems

Key Challenges

Milestones

August 24-26, 2010MAP Review-Front End Harold G. Kirk

3

The Muon Collider/Neutrino Factory Front End

The Front End is that portion of the facility after the proton driver which is common to both the Muon Collider and the Neutrino Factory

The proton source will have different bunch structures and possibly beam power.

NeutrinoFactory

MuonCollider

August 24-26, 2010MAP Review-Front End Harold G. Kirk

4

The Major Front EndSub-Systems

Target/Capture

Drift (π→μ)

Buncher/Rotator

Cooler

18.9 m ~40m

FE Targ

etSolenoid Drift Buncher Rotator Cooler

~33m 34 m ~80 m

p

π→μ

August 24-26, 2010MAP Review-Front End Harold G. Kirk

5

The Target Concept

Maximize Pion/Muon Production• Soft-pion production• High-Z materials• High-magnetic field

August 24-26, 2010MAP Review-Front End Harold G. Kirk

6

Cryostat Upstream End

Neutrino Factory Study 2 Target Concept

August 24-26, 2010MAP Review-Front End Harold G. Kirk

7

Upstream Target Exploded View

All insertion/extraction from upstream end

Locating & supporting features not shown – will require additional space

August 24-26, 2010MAP Review-Front End Harold G. Kirk

8

The Key Target Parameters

Proton Driver• 4 MW Beam power• 5-15 GeV KE (8 GeV is currently favored)• NF: 50 Hz / MC: 15 Hz• NF: 3 bunch structure (320 μs total) / MC: 1 bunch

Target System• 20-T solenoid magnet• Liquid metal jet• 20 m/s flow rate (“new” target every pulse @ 50 Hz)• High-Z (Hg favored)

August 24-26, 2010MAP Review-Front End Harold G. Kirk

9

Key Buncher/RotatorParameters

Buncher• 37 rf cavities• 320 to 233.6 MHz (13 frequencies)• 8 MV/m Peak rf gradient• 24 MW Peak rf power (NF: 0.7 MW avg)• 1.5T Peak magnetic field• 33 m total length

Rotator• 56 rf cavities• 230 to 202.3 MHz (15 frequencies)• 12 MV/m Peak rf gradient• 140 MW Peak rf power (MF: 4 MW avg)• 1.5 T Peak magnetic field• 42 m total length

August 24-26, 2010MAP Review-Front End Harold G. Kirk

10

The Buncher/RotatorP

ion

/Mu

on K

inet

ic E

ner

gy

Drift

Buncher Rotator

Target

August 24-26, 2010MAP Review-Front End Harold G. Kirk

11

Key Parameters of the Cooler

• 100 rf cavities

• 201.25 MHz • 15 MV/m Peak rf gradient• 400 MW Peak rf power (NF: 12 MW avg)• 2.8 T Peak magnetic field• 75 m Total length

August 24-26, 2010MAP Review-Front End Harold G. Kirk

12

Front End Challenges

Target• Shielding of the SC coils• Thermal Management• Containment of Hg• Delivery of stable 20 m/s Hg jet

Buncher/Rotator/Cooler• Performance of rf cavities in magnetic field• Shielding of beam line components• Proof-of-principle cooling demonstration (MICE)

August 24-26, 2010MAP Review-Front End Harold G. Kirk

13

Front End Challenges: RF

Machine performance reduced

• μ/p ratio reduced with rf gradient limitations

Mitigation Strategies: Alan Bross, D. Li rf talks

• Beryllium cavities• High pressure (GH2 filled) rf

cavities• Atomic Layer Deposition• Magnetic insulation cavities

0

0.01

0.02

0.03

0.04

0.05

0.06

0.07

0.08

0.09

0 5 10 15 20

rf Voltage

mu

/p

D/ Neuffer

August 24-26, 2010MAP Review-Front End Harold G. Kirk

14

Front End Challenges:Beamline Shielding

Mitigation Strategies• Upstream bent solenoid• Beryllium “beam stop” plugs

J.C. Gallardo

electrons

00

20

40

60

80

100

120

50 100 150z (m)

200 250 300

Ele

ctro

nbe

ampo

wer

(kW

)protons

0 50 100 150z (m)

200 250 3000

100

200

300

400

500

Pro

ton

bea

mp

ower

(kW

)

Buncher

RotatorCooler

Buncher

RotatorCooler

August 24-26, 2010MAP Review-Front End Harold G. Kirk

15

Front End Challenges:Target Shielding

Mitigation Strategies:• Increase SC IDs• Replace Cu resistive insert with HTS insert• Design and engineer thermal management solution

−130

−65

0

65

130130

cm

0 300 600600cm

Hg Jet

WC Shield

STST Bottle

Hg Pool

Air

SC5SC4SC3SC2SC1

FeCo

Pre-Trgt

Res Sol

Be Window (z=600 cm)

0

30

60

90

120120

cm

0 300 600600cm

10−310−410−510−610−710−810−910−1010−1110−1210−1310−1410−1510−1610−1710−1810−19

4.2e−04 0

25 KW ofEnergydepositionIn SC1

~3 MW inShielding

X. Ding

August 24-26, 2010MAP Review-Front End Harold G. Kirk

16

Front End Challenges: Hg Nozzle

Hg Jet• 8 mm OD

• 20 m/s for 50Hz operations• Hg jet performance in MERIT not optimal

Mitigation Strategies

• MHD simulations of jet/magnet/proton interactions

• Design and engineer nozzle delivery system • Fabricate and test prototypical nozzle design

August 24-26, 2010MAP Review-Front End Harold G. Kirk

17

Front End Challenges: Hg Target

Mercury• Low vapor pressure

• Toxic• Disperses easily upon spilling

Mitigation Strategies• Design and engineer double containment Hg system

• Explore alternatives:– PbBi eutectic– Tungsten powder flow

August 24-26, 2010MAP Review-Front End Harold G. Kirk

18

Front End Challenges: Pion Production

Current pion production modeling based on MARS15 simulations

HARP data does not support sharp falloff of pion production for proton KE < 8 GeV

Mitigation Strategies• Incorporate HARP (and MIPP)

results into MARS (underway Mokhov, et al)

• Contribute high-Z target for production experiment at 5 and 8 GeV (MIPP proposal, Torun, et al.)

August 24-26, 2010MAP Review-Front End Harold G. Kirk

19

Front End Milestones

FY10 Initial target configurationFY10 IDS-NF IDRFY11 Establish initial FE configurationFY12 Down selection of 201 rf cavity designFY12 Engineering design of Front EndFY13 Complete costing of Front EndFY14 IDS-NF RDRFY14 Interim MC DFS

August 24-26, 2010MAP Review-Front End Harold G. Kirk

20

Summary

• A Front End baseline has been established• Optimization studies have resulted in a 0.08 μ/p

throughput ratio for 8 GeV incoming protons • Key Front End challenges

– Performance of rf cavities in magnetic field– Shielding of superconducting solenoids

• Mitigation strategies have been developed to address these challenges


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