Survey
* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Efficient RF sources for Linear Accelerators Dr Chris Lingwood Motivation From CLIC CDR (2012) • LARGE numbers of RF sources are required for future linear colliders. • According to CDR 2012 CLIC requires 1638 @ 15 MW • Supply large amount of power at affordable cost (high efficiency) • Current state of the art – 15 MW klystrons can achieve 65% efficiency CLIC MBK Study • Collaboration with CERN and Thales (Erk Jensen, Igor Syratchev, Phillipe Thouvenin, Rodohple Marchesin). • Efficiency as main target • Evaluated configuration options, multiple beam klystron • Targeted a conservative (plausible) design • Targeted TESLA/ILC specification • Theoretical efficiency: 80% (beyond state of the art) Why many beams? • Low perveance leads to higher efficiency. 𝑝𝑒𝑟𝑣𝑒𝑎𝑛𝑐𝑒 𝐾 = 𝐼 𝑉 3/2 • Low current -> lower space charge forces -> better bunching -> higher efficiency • 20 beams – trade off between beam voltage and complexity due to beams Ib = 8.2A Vb = 115V Cavity choices • Comparison of multiple cavity types. • Re-entrant & HOM cavities -> Low R/Q • Recessed re-entrant and coax cavity -> high R/Q 1. Re-entrant 2. Recessed Re-entrant TM 0 1 3. & 4. Coaxial Cavity TM 0 1 TM 10 1 5. Whispering Gallery Interaction structure • Optimised 6 cavity • (single 2nd harmonic) • Low R/Q structure 70% • High R/Q structure 20 beam structure up to 80% Optimisation • Developed and published a new way to design klystron amplifiers: – ~14 Decisions (frequencies, drifts, Qe’s) – 3-4 objectives (efficiency, length, bandwidth, slowest electron – 5000-10,000 evaluations • Novel publishable optimisation concepts (recombination operator). • Impractical without high throughput computing (CI HTCondor Pool) • Use spare clock cycles of desktop pcs So it’s all done then? • Conservative approach lead to complex tube • Many, many, many beams • Push the voltage (always the plan) • Don’t rule out newer techniques • Be braver on layout • Fundamentally: do you want 50MW in an MBK? Cavity HOMs CPI (estimated) Can model coaxial cavity as a piece of ridged waveguide Very good agreement even for HOMs Ours Normalised frequency Quadrupole R Cavity radius • Large diameter (35cm) at 15MW • More power -> more beams -> larger still – Dipole mode gets closer for larger cavities Current Collaboration with CERN • Working with I. Syratchev, C. Marelli • Attempting to formalise empirical relationship between efficiency and perveance 85 80 75 xNo harm x2nd Harm 70 65 60 0 0.2 0.4 0.6 0.8 1 1.2 Proposed task • Many questions still surround the RF sources • Requirements still push state of the art – Power, efficiency, cost, lifetime • Evaluate options (SBK, MBK, MBIOT…) • Solution is probably klystrons – Configuration (MBK/SBK) • Work towards helping CERN become the intelligent customer Maximising Efficiency • Tight bunching isn’t enough • The key to higher efficiency is: – slow all your electrons down as much as possible in the output gap without stopping or reflecting them • This isn’t trivial • Potential improvements – Low frequency penultimate cavities – Travelling wave output structures Higher harmonic cavities • To get the tightest bunch from a single cavity – sawtooth waveform (includes high harmonics) • 2nd harmonic cavities well understood • Will 3rd or higher harmonic cavities help more? – Effect on bandwidth? – Effect on velocity spread? Reduce velocity spread IVEC 2013 • Detune penultimate cavity to achieve π phase change – When phase change is good, coupling to the beam is bad – Two gap cavity can help with control • Tested in 63 W C-band tube, increase efficiency by 8%, 25% reduced voltage. • Does this approach scale to MW? Klystron Configuration • Some interesting configuration options under consideration. • Some beyond state of the art • Some just beyond …. New software • A number of klystron specific codes exist. Only one generally available – AJDisk • For instance cavity voltages can be unreliable disagree as much as 50% between GdfidL and AJDisk and 1500% (!) with klys2D (Thales). • Closed source so difficult to identify the issue • Also difficult to integrate with other codes • Propose to develop new “open” disk model code for klystron research from existing code at Lancaster. PIC Simulations • Simplified models can only get us so far • Detailed verification of designs to demonstrate improvements • 1 week simulation time for klystron 1GHz up to 10 μs – 8 cores • Scope for improvement with HPC (available at Hartree Centre, Sci-Tech Daresbury) • Careful benchmarking of code (V-SIM) against MAGIC MB-IOTs for Linear Accelerators • Reduce power lost to collector by switch beam • Short “excursions” above rated power allowable. • Very useful when high efficiency and variable output power are needed. • Even better if “headroom” is needed • IOTs exist up to about 100kW • Not a great deal in the context of proposed large LINACs Klystron IOT • Just like klystron MBK -> MB-IOT • 10 beams -> 1MW, more plausible. • ESS seriously considering. • Road block - guns • Worth doing the sums. Figures from IOT based High Power Amplifiers, Morten Jensen, TIARA Workshop on RF Power Generation for Accelerators – Uppsala June 2013 Milestones • 2014 Investigate suitability of single and multi-beam klystrons, MBIOTs, magnetrons. • 2014 Produce a bunched beam vacuum tube model. Transcode and improve existing code to interface with PIC codes for output cavity. Benchmark against existing codes. • 2015 Evaluate new and existing techniques to improve efficiency. • 2015 Benchmark V-SIM and CST against MAGIC for bunched vacuum tubes. • 2016 Design most appropriate tube and validate using PIC. Deliverables • 2014: Tube model complete and open sourced • 2015: Design of tube interaction structure for drive beam - report • 2016: PIC simulations and verification of proposed interaction structure - report Financial Staff (Lingwood) RA3 Student (TBD) Materials Travel 1 6+6 12 5+7 1+2 1 RA and 1 Phd student for three years 1 6+6 12 4+5 1+2 1 6+6 12 0+0 1+2 3 18+18 36 9+12 3+6 Summary • • • • Re-evaluate options for RF sources Push efficiency and plausibility Scope for improvement in simulation times Develop more flexible and open klystron simulation tools. • Produce candidate structure using lessons learned.