ESSnuSB

Funded by the Horizon 2020 Framework Programme of the European Union

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    • Definition
    • WP1 – Management Team
    • WP2 – Linac upgrade
    • WP3 – Accumulator
    • WP4 – Target Station
    • WP5 – Detector performance
    • WP6 – Physics Reach
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WP2 – Linac upgrade

  • Coordinator: Mamad Eshraqi (ESS, Sweden)
  • Co-coordinator: Roger Ruber (University of Uppsala, Sweden)
  • Team members:
    • Sebastien Bousson (CNRS, FR)
    • Hakan Danared (ESS, SE)
    • Jean-Pierre Delahaye (CERN, CH)
    • Tord Ekelof (Uppsala University, SE)
    • Björn Galander (ESS, SE)
    • Frank Gerigk (CERN, CH)
    • Mats Lindroos (ESS, SE)
    • Eric Montesinos (CERN, CH)
    • Roger Ruber (Uppsala University, SE)

Providing a proton beam of 5 MW with short pulses to the neutrino target requires the ESS linac, Figure 1, to be upgraded to deliver a total of 10 MW average beam power. The additional 5 MW of beam power has H⁻ as the accelerated species to enhance the injection into the accumulator ring using charge exchange injection scheme.

Figure 1: Layout of the ESS linac (violet), ESS target (red) and instruments (orange) on the ESS site. The darkblue line shows the extraction and transfer line from the linac, the accumulator, the target station and the near neutrino detector.

The main deliverable of this Work Package is the CDR chapters for the ESS linac modifications, including the cost and safety issues and, most importantly, the interactions with the generation of spallation neutrons which is the main purpose of the ESS. This WP will study the integration, installation and operation of an H– ion source, Figure 2, and the acceleration of H– in the linac to the higher energy of 2.5 GeV.

Figure 2: Two possibilities of adding an H- source and beam to the ESS linac

Increasing the linac energy to 2.5 GeV from the 2.0 GeV requires adding 8 additional cryomodules of the High beta type downstream of the high beta linac, Figure 3. Increases energy of the H- beam reduces the space charge tune shift in the accumulator ring, and reduces the average current in the linac.

 

Figure 3: Block diagram of the ESS linac, including added block for increasing the beam energy to 2.5 GeV (khaki block titled "UP").

Amongst the items to be studied for the H⁻ beam transport, this work-package looks in particular on the effects of beam losses, and of the requirements on the RF power sources and the upgrade of the cooling system to handle the increase of the RF power of the linac by injecting and accelerating H– pulses between the ordinary H+ pulses, thereby increasing the pulse frequency to 28 Hz, Figure 4.

 

Baseline pulse structure for the proton and H⁻ beams

Other pulse train sequences are being considered that could raise the frequency to 70 Hz by inserting 4 lower power H– pulses between successive H+ pulses. During the course of the Design Study the ESS linac will be built up. The study will have, as an early priority task, the identification of minor modifications that can be made during the construction phase of the linac that will minimise the disturbance and cost of the later upgrade of the power and the enabling of H– acceleration in extra pulses. Costing aspects will also be addressed.

European Unions’ Horizon 2020 : ESSnuSB has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 777419.The webpage reflects only the author’s view. The Commission is not responsible for any use that may be made of the information it contains.

Working Groups

  • ○ WP1 – Management
  • ○ WP2 – Linac upgrade
  • ○ WP3 – Accumulator
  • ○ WP4 – Target Station
  • ○ WP5 – Detector performance
  • ○ WP6 – Physics Reach
  • IPN
  • CNRS
  • AGH
  • Lunds Universitet
  • CB
  • cukurova university
  • KTH
  • ESS
  • IPHC
  • UPPSALA UNIVERSITET
  • Université de genève
  • RB
  • CERN
  • DEMOKRITOS
  • INFN
  • UAM Universidad

ESSNUSB CALENDAR

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