Melbourne X-band Status and Plans CLIC meeting 5/10/2021 - Dr. Suzie Sheehy Senior Lecturer, University of Melbourne Baker/ANSTO Fellow in Medical ...
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Melbourne X-band Status and Plans CLIC meeting 5/10/2021 Dr. Suzie Sheehy Senior Lecturer, University of Melbourne Baker/ANSTO Fellow in Medical Accelerator Physics suzie.sheehy@unimelb.edu.au @suziesheehy 1 Image: M. Volpi
Accelerator Physics @ Melbourne University X-band (Compact) Accelerators: • Dr. Matteo Volpi • Prof. Geoff Taylor • A/Prof. Roger Rassool • Scott Williams (PhD) • Paarangat Pushkarna (MSc) • James Dawkins (MSc) Hadron Therapy & Medical Accelerators: • Dr. Jacinta Yap • Greg Peiris (PhD) • Frank Zhang (PhD) An outstanding accelerator R&D programme to underpin training of • Adam Steinberg (PhD – Manchester) future accelerator experts was highlighted as a key recommendation • Hannah Norman (PhD – Manchester) • Elodie Higgins (MSc – completed) in the 2015 Australian Academy of Science Honoraryreport Members: • Dr. Rohan Dowd (ANSTO) Some of the group visiting the Australian Synchrotron • Dr. Rebecca Auchettl (ANSTO) • Dr. Eugene Tan (ANSTO) 2 • Choiphy Zhao
The “X-BOX3” formerly at CERN… Total power < 50 MW 2 x Toshiba 6MW 5us klystron 2 x Scandinova Modulators Nominal Rep Rate 400Hz Developed for ‘CLIC’ Compact Linear Collider Project
Melbourne is hosting the first high-frequency high- gradient accelerator lab in the Southern Hemisphere 7
X-LAB: X-band Laboratory for Accelerators and Beams PROGRAM 2021 - 2026 Note: synchronized with ANSTO/Australian Synchrotron plans Phase 1: X-band Research & Establishment Conditioning of Reconfigure to ARC Linkage Proposal Design for Rf pulses with TD24 & accelerating R3, 2020 applications beam algorithm mode Baker Foundation (TBC) Phase 2: 40 MeV tunable, pulsed electrons & applications ARC LIEF proposal R1 2021 (TBC) Design & Procurement Beamline • Progress application-based research: space w. ANSTO, Wollongong & simulation of beamline commissioning dosimetry, biophysics, radiotherapy, etc… Sydney 2022 2023 2024 2025/6 Heavy work, First X- water & Electron Compton light source band rf experiments? electricity gun added pulses completed
Phase 0: 1: Accelerator Refurb & Installation Test Stand E D Bunker used to OV house a 35 MeV P R betatron N G AP N D I FU 9
M.VOLPI FLUKA simulation
M.VOLPI Structure Shielding – at CERN Lead bricks around the downstream Faraday Cup (default shielding) 5-10 cm tick lead box
M.VOLPI Dose Equivalent Setup Summary • 20 MeV • 100ns flat top • 0.5 mA dark current • 200 Hz repetition rate • 2000 working hours per year, (40h/week x 50 weeks) • Extra shields: – Lead bricks around downstream faraday cup – Wall bricks around the structures 13
M.VOLPI P. PUSHKARNA A Phase 1 Research Avenue… - RF breakdown is destructive to beam & accelerator - Need to be able to: - predict breakdown - Optimise “conditioning” (variation of input pulses over time) - With up to 400Hz pulse rate, potential for high data rate Can we build a machine learning algorithm to optimize conditioning process TD24 structure so far reached 40.45 MW (97.9 MV/m) (ns) 14 CLIC structures high power tested so far.
Phase 2: Electron beamline project Co-develop accelerators for applications Potential electron and X-ray users: Accelerator developments: • Biophysics studies • Compact Light Source development • Electronics and dosimetry (space applications) • VHEE accelerating structures • Diagnostics development • Structures for in-field industrial scanning applications • Novel radiotherapy technology + much more!
S. WILLIAMS M. VOLPI Beamline Simulations After capture and acceleration, simulations show the system will be able to provide: • electron beam energies of 3-40 MeV, • 125 keV energy spread, • emittance of 1 .mm.mrad • pulse length of 150 μm. • Pulse rate 3 Hz based on the S-band gun but could be upgraded in future. • Charge per bunch is 0.1 nC and dose rate is 12 mJ/sec. All parameters are tunable, these represent the optimum set. 16
Building the ‘ecosystem’ as well as the lab…
Other applications/partnerships: • Successfully established links with ANFF (Adelaide) to produce the FIRST X-band high power RF components ever made in Australia • …now preparing to invest in $millions for a “nanomill”
Thankyou Dr. Suzie Sheehy @suziesheehy Pictured: X-LAB visit by Moira O’Bryan, Dean of Science, UniMelb (Photo: M. Volpi)
Extra slides
UoM limits The calculation assume that a person will work 50 weeks a year. Annual dose limit at UoM 1mSv , weekly dose rate cannot exceed 20 uSv/week over 50 weeks. 21
Running conditions Minimum Maximum Average NOTE Power n/a 18MeV < 10MeV Max=20MeV if PC is detuned +1.5MHz Dark Current 0.25mA/pulse 1.25mA/pulse 0.5mA The DC decrease during the conditioning Flat Top 50ns 200ns 100ns The DC decrease at high pulse because the conditioning started stated with small pulse Repetition 50Hz 200Hz 100Hz At 200Hz, hard keep tuned the PC Rate/structure Working time n/a 40h/week We can’t stay longer in the bunker due to the klystron noise 22
Dose Equivalent Setup Summary • 20 MeV • 100ns flat top • 0.5 mA dark current • 200 Hz repetition rate • 2000 working hours per year, (40h/week x 50 weeks) • Extra shields: – Lead bricks around downstream faraday cup – Wall bricks around the structures 23
Dose Rate Setup Summary • 20 MeV • 100ns flat top • 0.5 mA dark current • 200 Hz repetition rate • 2000 working hours per year, (40h/week x 50 weeks) • Extra shields: – Lead bricks around downstream faraday cup – Wall bricks around the structures 24
Dose-Equivalent (not Dose) • For some quantities, there is the possibility to get built-in conversions, without the need for user routines, rather through dedicated generalized particles. The most commonly used is dose equivalent (ambient dose equivalent or effective dose): DOSE-EQ Dose Equivalent [pSv] DOSE total absorbed dose in GeV/g • DOSE-EQ is calculated by folding particle fluences with conversion coefficient sets, selected by the user among a list (see manual) through AUXSCORE. The default set (not requiring the AUXSCORE association) is “AMB74”. • I am using EWT74 (Valencia Setup) Renormalization factor • Dark current ~0.5mA/pulse • 1A= 6.24x10^18 e/sec => 6.24x10^18 * 0.4x10^-4 = 2.5 x10^14 25
Normalisation We need to times the dark current by the duty factor which is 10^-7 roughly (100ns flat top). • They have 0.5mA for say 100ns, which is 50pC, at 200Hz this gives an average current of 10nA • Current per pulse ~0.5mA Repetition rate is 200Hz (400Hz/2 two test stands) • Then 2.5 x10^14 x 200= 5x10^16x10^-7 = 5x10^9 Summary • 5e9 : beam intensity is 5e16 electrons/s • 1e-6 conversion pSv to uSv • 3600 conversion from 1/s to 1/h • 2000 working hours per year 40h/week x 50 weeks Electron energy :20 MeV DOSE • DOSE with the same normalization of DOSE-EQ * 1.6e-7 • Does unit transfers from GeV/g to Gy by a factor 1.6e-7. 26
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