long pulses spallation source - cern · long pulses spallation source hannes 2bartosik1, jan...
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Long Pulses Spallation Source
Hannes Bartosik1, Jan Egberts 2,Oscar Gonzalez 3 1) CERN 2) CEA Saclay 3) ESS-Bilbao
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Power: 5 MW
Energy: 1 - 8 GeV
Rep. rate: 10 - 20 Hz
Pulse: 2 -3 ms
p+ or H-
Current: I > 5MW / 8GeV / 20 Hz / 2 ms = 15.6 mA
Linac
ESS
31.05.2011 [email protected] 1
Requirements
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31.05.2011 [email protected] 2
ESS Outline
352 MHz 704 MHz
Power: 5 MW
Energy: 2.5 GeV
Rep. rate: 14 Hz
Pulse: 3 ms
S. Pegs et al “Plans for the ESS Linac”, Proc. of LINAC 2010, Tsukuba, Japan, 2010
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ECR source like SILHI
Current: 50 – 60 mA
31.05.2011 [email protected] 3
Source
SILHI source @ CEA Saclay
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31.05.2011 [email protected] 4
RFQ
IPHI RFQ @ CEA Saclay
RFQ (4 vanes)
Energy: 3 MeV
Frequency: 352 MHz (like ESS, Linac4, SPL)
Issues:
Longer RFQ lower frequency required to fulfill L ≤ 4λ
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DTL @ low energies to account for rapid velocity changes
Energy: 50 MeV (like ESS, ESS Bilbao)
Normal conducting to
ease manufacturing
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DTL
DTL of ESS Bilbao
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Frequency: 352 – 704 MHz (like ESS, SPL)
Optimum neutron yield at 1.5 GeV
High gradient high cavities
Energy: ≥ 2 GeV
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Superconductive Linac
Roger Ruber, “The European Spallation Source (ESS)” presentation
M. Wohlmuther, “Targets and beam dumps”, CAS Bilbao 2011
Issues:
Klystrons
Budget
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Liquid target
Jet target (Hg or LBE) (like IFMIF, BNL E-951)
Reduced downtime
Increased reliability
Issues:
Bragg-peak depth: m
Energy ≈ 1 GeV
31.05.2011 [email protected] 7
Target Option 1
IFMIF liquid Li target mockup
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Liquid target
(Hg or LBE)
Issues:
No 5 MW target existing so far…
31.05.2011 [email protected] 8
Target Option 2
B. W. Riemer “The SNS mercury Target”, presentation
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NOT presented Issues:
Beam dynamics
Diagnostics
MPS / PPS
Commissioning
Cryostat
Klystrons / power supplies
Irradiation cells
location
etc...
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NOT presented Issues
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ESS Outline
ECR source (e.g. SILHI)
ESS RFQ
ESS DTL
scLinac (> 2 GeV like ESS)
Hg Target (like SNS)
2 GeV, 50 mA, 20 Hz, 3 ms pulse 6 MW
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Conclusion
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Sincere thanks to Lali Tchelidze (ESS)
and Rihua Zeng (ESS) for
information and support!
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Acknowledgement