mercury beam dump simulations tristan davenne ottone caretta stfc rutherford appleton laboratory, uk...

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Mercury Beam Dump Simulations Tristan Davenne Ottone Caretta STFC Rutherford Appleton Laboratory, UK November-2008

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Mercury Beam Dump Simulations

Tristan Davenne Ottone Caretta

STFC Rutherford Appleton Laboratory, UK

November-2008

Mercury beam dump design from NUFACT Feasibility Study

Peter Loveridge, November-2008

Mercury beam dump design from NUFACT Feasibility Study

Thermal shocks and magnetohydrodynamics in

highpower mercury jet targets

J Lettry, A Fabich, S Gilardoni, M Benedikt, M

Farhat and E Robert

Agitation ‘eruption’ of mercury pool surface due to 24GeV proton beam Fluka Simulation - Energy deposition in mercury pool

How much of the beam energy is absorbed in the beam dump?

Agitation ‘eruption’ of mercury pool surface due to 24GeV proton beam Autodyne simulation

Splash following pulse of 20Terra protons

Agitation ‘eruption’ of mercury pool surface due to 24GeV proton beam

Autodyne simulationDamage to underside of 15mm stainless steel plate (maybe need sprung baffles!)

Damage as a result of high speed impact of a mercury dropletStainless Steel vs. Ti-6Al-4V

Consider helium bubbles in beam dump to reduce splash velocity

helium

Proton beam

Mercury beam dump design from NUFACT Feasibility Study

Agitation of mercury pool surface due to impinging mercury jet

2 phase CFX modelmercury jet velocity = 20m/s

Angle of attack = 5.7°mercury pool surface area = 0.05m2

Summary

Conclusions

Simulations indicate that mercury splashes with a maximum velocity of 75m/s will result when a pulse from the undisrupted 24GeV beam is absorbed by the mercury beam dump.

Mercury splash velocity of 30m/s has been observed experimentally when a 1GeV proton beam interacted with a trough of mercury. Lettry et al.

A 3mm diameter mercury droplet impacting a stainless steel plate at 75m/s are predicted to cause significant damage. Ti-6Al-4V is predicted to be more resistant to damage due to higher ultimate strength and shear strength.

Significant agitation of the mercury surface also results from the impingement of the mercury jet.

Questions

1. How many pulses from the beam must the beam dump be able to survive?

2. Are sprung baffles a useful approach to containing a mercury splash from the beam dump?

3. Would helium bubbles be a useful addition to the beam dump in order to move the energy deposition deeper in to the mercury pool?

04/18/23

Tungsten Powder Jet Update

Ottone Caretta

STFC Rutherford Appleton Laboratory, UK

November-2008

High speed videos: some of the tests

2cm

Thank you to EIP at RAL for providing the video equipment used for these experiments

propelled by air ~3 bar

=3/10bar=~atmwater supply

8

1

45

11

10

36

9

31-32-33

38

302

3

141617 20-21

25

24

23

22

29

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26

37

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40To the pneumatics

6

44

Rig Flow Diagram

Powder Jet Rig 31st Oct 2008

Powder Jet Rig 31st oct 2008

Schedule

November 10-18 system and control wiring

November 19-27 system control development

November 27-28 system commissioning

November 27-christmas preliminary experiments

Helmholtz Capture Solenoid Update

Peter Loveridge

[email protected]

STFC Rutherford Appleton Laboratory, UK

November-2008

Overview

• Purpose– To investigate the feasibility of a proposed capture solenoid with an axial (“Helmholtz”) gap

• Method– Development of Study-2 design…

• Split both the 1st SC coil and the NC insert coil in two• Downstream coils remain unchanged• Introduce current grading in the SC “Helmholtz” coils

– Investigate a potential mechanical design with lateral target entry/exit slots• Start with min slot size 20 mm x 200 mm, -an optimistic case!

Conceptual layout of the Helmholtz capture solenoid

On-axis Field Profile

Peter Loveridge, November-2008

On-Axis Field

0

5

10

15

20

-2 0 2 4 6

Z Position (m)

Fie

ld (

Tes

la)

Total

NC Contribution

SC Contribution

Magnetic field plot (Tesla) On-axis field profile

• SC contribution– ~12 Tesla, flat plateau in target region

• NC contribution– ~7 Tesla, unwanted trough in target region

• Total– Close approximation to the study-2 field with the exception of the trough in the target region

Peter Loveridge, November-2008

Inter-Coil Forces

Magnetic force plot from an early Helmholtz geometry iteration

• Axial Forces– Cumulative axial compressive force ~ 16,000

metric tonnes!– Axial Forces balanced between first 6 SC coils

• Must house all these coils in a single cryostat to avoid transferring loads up to room temperature

– Huge attractive axial forces must be transferred across the Helmholtz gap

• Requires careful mechanical design

• Radial forces– Equivalent to an internal pressure of ~1500 bar!

In coils SC01and SC02– Leads to large hoop-stresses as seen in study-

2 design– Strength of NC insert coil is a particular concern

Peter Loveridge, November-2008

Summary

Status• Have developed a (very) conceptual design for a capture solenoid with lateral target entry/exit

slots (200 mm x 20 mm)– Includes a basic level of realism:

• “Reasonable” current densities in SC and NC coils• 1st guess at space envelopes for cryostat, coil support-structure, shielding

Issues• Effect of field trough on pion capture (John Back)• How to cope with the huge inter-coil forces• Large tensile hoop stresses in coils

• How to integrate with a solid target system

Comments:• The combination of very high field and large bore required by the capture solenoid constitutes

a formidable engineering challenge• We should keep an open mind about what kind of magnet geometry would best suit a solid target

system.

Peter Loveridge, November-2008