energy deposition for intense muon sources (chicane + the rest of the front end) pavel snopok...

17
Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4, 2014 Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014)

Upload: valerie-oneal

Post on 30-Dec-2015

213 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014)

Energy depositionfor intense muon sources

(chicane + the rest of the front end)

Pavel Snopok

Illinois Institute of Technology

and

Fermilab

December 4, 2014

Page 2: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 2

Outline

• Introduction• History• Current MARS simulations

– new data files for solid target

• Using other codes (ICOOL and G4beamline)• Summary

December 4, 2014

Page 3: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 3

Introduction

• In high-intensity sources muons are produced by firing high energy p onto a target to produce π.

• π decay to μ which are captured and accelerated.• Significant background from p and ē, which may result in

– heat deposition on superconducting materials;– activation of the machine preventing manual handling.

December 4, 2014

Page 4: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 4

Introduction, contd.

• Need a secondary particle handling system for a megawatt class solid C target– solenoidal chicane– followed by a proton absorber.

• Challenges of optimization and integration of the system with the rest of the muon front end.

• Main study tool – MARS, some analysis and validation by using ICOOL and G4beamline.

• Start with the chicane, use the same technique downstream to study the the buncher and phase-rotator sections.

December 4, 2014

Page 5: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

5

History: MARS simulations

• ROOT-based geometry• 12.5° single bend, Z=0 corresponds to 19 m downstream of the target

– consistent with RDR (IDS-NF).

• W density reduced to 60% to take into account packing fraction for beads.

Page 6: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 6

Reference: no shielding

December 4, 2014

DPD peaks at 15.8

mW/g, that translates

into 42.6 kW/m for Cu

coils or 33.3 kW/m for

SC coils.

Page 7: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

7

Uniform 35 cm shielding

Empty channel PD total, mW/g

Page 8: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

8

Non-uniform 30 and 40 cm shielding

Empty channel PD total, mW/g

Page 9: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

9

Overall DPD per coil/segment

Segmented coil analysis, total DPD, mW/g Average DPD per coil, mW/g

In both cases red line corresponds to 0.1 mW/g SC limit

Page 10: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 10

Current MARS simulations

• New target parameters:– 8 GeV => 6.75 GeV– 4 MW => 1 MW– 3.125e15 protons/sec => 0.925e15 protons/sec– new particle distribution– need to re-run MARS

• The hope is that the new parameters help reduce the amount of shielding required

December 4, 2014

Page 11: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

11

New results

Muon flux, top view Muon flux, side view

Page 12: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

12

New results 2

Proton flux, top view Proton flux, side view

Page 13: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

13

New results 3

Deposited power density, mW/g,top view

Deposited power density, mW/g,side view

Page 14: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

14

New results 4

Deposited power density, mW/gsegmented coil analysis

Deposited power density, mW/gaveraged

Page 15: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 15

Other codes

• Can G4beamline or ICOOL be used for energy loss/deposition calculations?

• Back in 2010 I did a comparison of the two codes for IDR:

December 4, 2014

Page 16: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 16

Summary

• Simulations of the new 1 MW graphite target are underway, first results presented.– power density > 0.1 mW/g only in a handful of cental

coils, very low everywhere else;– definitely do not need 35 cm of tungsten.

• Action item: implement a more sophisticated geometry (elliptical cross-section following the profile of the beam).– this will allow to significantly reduce the amount of W

used for shielding.

• MARS is the main tool, although G4beamline and ICOOL can also be used for some analyses.

December 4, 2014

Page 17: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,

Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 17

December 4, 2014

Thank you!