90°-Cavities With Improved Inner-Cell HOM Properties Shannon Hughes Advisor: Valery Shemelin.

Slides:



Advertisements
Similar presentations
BL TIER 3 TIER 3 Identify suitable experimental procedures for measuring rates of reactions Identify the factors affecting the rate of a reaction Calculate.
Advertisements

Tom Powers Practical Aspects of SRF Cavity Testing and Operations SRF Workshop 2011 Tutorial Session.
Frequency modulation and circuits
Beam-based Measurements of HOMs in the HTC Adam Bartnik for ERL Team, Daniel Hall, John Dobbins, Mike Billing, Matthias Liepe, Ivan Bazarov.
Grey Level Enhancement Contrast stretching Linear mapping Non-linear mapping Efficient implementation of mapping algorithms Design of classes to support.
D. Lipka, MDI, DESY Hamburg, July 2012 Simulation of fields around spring and cathode for photogun D. Lipka, MDI, DESY Hamburg.
Accelerator Science and Technology Centre Prospects of Compact Crab Cavities for LHC Peter McIntosh LHC-CC Workshop, CERN 21 st August 2008.
CLIC Main linac structure and Crab cavity Vasim Khan
S. N. “ Cavities for Super B-Factory” 1 of 38 Sasha Novokhatski SLAC, Stanford University Accelerator Session April 20, 2005 Low R/Q Cavities for Super.
Challenge the future Delft University of Technology Blade Load Estimations by a Load Database for an Implementation in SCADA Systems Master Thesis.
INVESITGATION OF AN ALTERNATE MEANS OF WAKEFIELD SUPPRESSION IN CLIC MAIN LINACS CLIC_DDS.
INVESITGATION OF AN ALTERNATE MEANS OF WAKEFIELD SUPPRESSION IN CLIC MAIN LINACS CLIC_DDS.
ABSTRACT The main accelerating structures for the CLIC are designed to operate at 100 MV/m accelerating gradient. The accelerating frequency has been optimised.
Wakefield suppression in the CLIC main accelerating structures Vasim Khan & Roger Jones.
DUAL FEED RF GUN DESIGN FOR LCLS Liling XIAO, Zenghai LI Advanced Computations Department Stanford Linear Accelerator Center Nov , SLAC-LCLS Injector.
Design of Standing-Wave Accelerator Structure
ABSTRACT The main accelerating structures for the CLIC are designed to operate at 100 MV/m accelerating gradient. The accelerating frequency has been optimised.
Problem Solving Part 2 Resonance.
DESIGN OF A 7-CELLS, HOM DAMPED, SUPERCONDUCTING CAVITY FOR THE STRONG RF FOCUSING EXPERIMENT AT DANE David Alesini, Caterina Biscari, Roberto Boni, Alessandro.
DDS limits and perspectives Alessandro D’Elia on behalf of UMAN Collaboration 1.
SRF Results and Requirements Internal MLC Review Matthias Liepe1.
Dr. Richard Young Optronic Laboratories, Inc..  Uncertainty budgets are a growing requirement of measurements.  Multiple measurements are generally.
Investigation of Wake Fields in Optimized SRF Cavities for the ILC The Cockcroft Institute of Accelerator Science and Technology, Daresbury WA4 4AD, UK.
Course B: rf technology Normal conducting rf Part 5: Higher-order-mode damping Walter Wuensch, CERN Sixth International Accelerator School for Linear Colliders.
Photocathode 1.5 (1, 3.5) cell superconducting RF gun with electric and magnetic RF focusing Transversal normalized rms emittance (no thermal emittance)
The design of elliptical cavities Gabriele Costanza.
The Fundamental Physics of Directive Beaming at Microwave and Optical Frequencies in Terms of Leaky Waves Saman Kabiri, Master’s Student Dept. of Electrical.
RF Cavity Design with Superfish
SRF CAVITY GEOMETRY OPTIMIZATION FOR THE ILC WITH MINIMIZED SURFACE E.M. FIELDS AND SUPERIOR BANDWIDTH The Cockcroft Institute of Accelerator Science and.
704MHz Warm RF Cavity for LEReC Binping Xiao Collider-Accelerator Department, BNL July 8, 2015 LEReC Warm Cavity Review Meeting  July 8, 2015.
Design of an Isochronous FFAG Ring for Acceleration of Muons G.H. Rees RAL, UK.
Study of absorber effectiveness in ILC cavities K. Bane, C. Nantista, C. Adolphsen 12 October 2010.
L-band (1.3 GHz) 5-Cell SW Cavity High Power Test Results Faya Wang, Chris Adolphsen SLAC National Accelerator Laboratory
Minimizing the RF Fields on the Surface of an SRF Cavity by Optimizing its Shape David Stark Advisor: Valery Shemelin Cornell University Cornell Laboratory.
Group 6 / A RF Test and Properties of a Superconducting Cavity Mattia Checchin, Fabien Eozénou, Teresa Martinez de Alvaro, Szabina Mikulás, Jens Steckert.
Beam breakup and emittance growth in CLIC drive beam TW buncher Hamed Shaker School of Particles and Accelerators, IPM.
Aaron Farricker 107/07/2014Aaron Farricker Beam Dynamics in the ESS Linac Under the Influence of Monopole and Dipole HOMs.
Sensitivity of HOM Frequency in the ESS Medium Beta Cavity Aaron Farricker.
POWER REQUIREMENTS FOR THE LHC HARMONIC CAVITIES WITH THE FULL-DETUNING SCHEME P. Baudrenghien, T. Mastoridis, CERN BE-RF 2nd LHC Harmonic Cavity meeting,
UK-Jlab-TechX Designs for the LHC Crab Cavity Dr G Burt Lancaster University / Cockcroft Institute.
ILC 07 May 30-June 3, 2007 N.Solyak 1 MULTIPACTORING SIMULATIONS IN CAVITIES AND HOM COUPLERS Nikolay Solyak, Ivan Gonin, Jiajian Li Fermilab.
TISSUE HARMONIC IMAGING (THI)
Midterm Review 28-29/05/2015 Progress on wire-based accelerating structure alignment Natalia Galindo Munoz RF-structure development meeting 13/04/2016.
Aaron Farricker 107/07/2014Aaron Farricker Beam Dynamics in the ESS Linac Under the Influence of Monopole and Dipole HOMs.
RESONANCE FREQUENCY SHIFT EFFECTS DUE TO CAVITY LENGTH AND WINDOW VARIATION By Gabriela Arriaga 1.
Sub-Task HOM-BPM HOM based Beam Position Monitors – Planned and Extant Measurements N. Baboi, DESY, Hamburg EuCARD WP 10: SRF, Annual Review Meeting.
XFEL beamline loads and HOM coupler for CW
WP10.5: HOM Distribution Task 2 – Presentation 2.
FPC Coupler RF Dipole Kick
Update of CLIC accelerating structure design
High Q Cavity Operation in the Cornell Horizontal Test Cryomodule
Electron collider ring Chromaticity Compensation and dynamic aperture
Case study 6 Properties and test of a Superconducting RF cavity
Optimization of Elliptical SRF Cavities where
Statistics Review ChE 477 Winter 2018 Dr. Harding.
Minimizing the RF fields
Overview Multi Bunch Beam Dynamics at XFEL
Implications of HOMs on Beam Dynamics at ESS
RF modes for plasma processing
TCLIA/TCTV transverse impedance simulation
The new 7BA design of BAPS
NanoBPM Status and Multibunch Mark Slater, Cambridge University
CEPC Main Ring Cavity Design with HOM Couplers
Progress in the design of a damped an
PEPX-type BAPS Lattice Design and Beam Dynamics Optimization
Accelerator Physics Particle Acceleration
Modified Modal Methods in Asymmetric Systems
ERL Director’s Review Main Linac
Evgenij Kot XFEL beam dynamics meeting,
Antenna Theory By CONSTANTINE A.BALANIS Ch1.4, 2.1~2.2.4 O Yeon Jeong.
Presentation transcript:

90°-Cavities With Improved Inner-Cell HOM Properties Shannon Hughes Advisor: Valery Shemelin

Introduction Ideal cavities have geometry for working π-mode frequency Real cavities have many minor defects… – Frequency can be different than intended Non-propagating frequency → trapped higher-order modes – Trapped HOMs can’t get to damping couplers, so their energy can’t be removed – has negative effect on beam quality Goal: Stop trapped modes from occurring.

Introduction How do we avoid trapped modes? All frequencies within each dipole-mode bandwidth propagate. – Broader bandwidths → fewer non-propagating modes, so less likelihood of trapping Bandwidths can be broadened by modifying elliptic arc parameters (i.e. geometry) – Need to find geometry that yields widest bandwidths

Programs Used SLANS/SLANS2 – creates meshes – calculates frequencies – plots electric fields – SLANS → monopole mode – SLANS2 → dipole modes TunedCell – wrapper program for SLANS/SLANS2 – calculates figures of merit (e, h, etc) – writes half-cell geometries for each set of elliptic arc parameters MathCAD – fits curves to data using splines – generates random numbers (for Monte Carlo technique) – plots data, and a lot more

Geometry A cell is made up of two elliptic arcs (AB and ab) connected by a line l, as shown in the half-cell figure Many figures of merit determined by elliptic arc parameters (A, B, a and b) α = cell wall slope angle Three types of cells – non- reentrant, 90°, and reentrant Non-reentrant: α > 90 Reentrant: α < 90

Geometry Half-Cell MeshSingle-Cell Mesh

Geometry Six-Cell Mesh

Why 90°-Cavities? Frequency vs Phase Shift for Fundamental Mode Red → α ≤ 90° Blue → α > 90° ERL: TESLA: Greater difference between 0- and π-mode → larger bandwidth (B 0 = f π - f 0 ) Geometries with α ≤ 90° dominate the lower part of both graphs, tending to have the broadest bandwidths for a given e. e = Epk/2Eacc

Why 90°-Cavities? Cell-to-Cell Coupling vs Cell Wall Slope Angle for Fundamental Mode Multiple cells per cavity – cells must work well together Higher k → better coupling Geometries with α ≤ 90° tend to have the highest k values for a given e.

Why 90°-Cavities? h vs α for e = 1 Best acceleration gradient comes from – minimizing peak magnetic field (H pk ) – maximizing accelerating field (E acc ) So minimizing h = H pk /42E acc yields best acceleration gradient 95% of overall decrease in h occurs from α = 105° to α = 90° Geometries with α ≤ 90° tend to have the lowest h values for a given e.

Why 90°-Cavities? Geometries with α ≤ 90° tend to have the best h, k and B 0 values for a given e. Reentrant cavities (α < 90°) have some practical problems – Difficult to remove water/chemicals during cleaning – Difficult to fabricate properly 90°-cavities do not share these problems 90°-cavities can be used for small-angle benefits without reentrant drawbacks.

Why 90°-Cavities? Other groups interested in 90°-cavities – Examples: LL, Ichiro, LSF, NLSF Our minimized h vs e values just as good or better than these others h vs e Ichiro 51: the goal gradient (MV/m) for the 9-cell low-loss “Ichiro” cavity

Higher-Order Modes Frequency vs Phase Shift for 7 Dipole Modes Graph shows frequencies of first seven dipole modes in initial 90°-cavity – Focus on these because we limit maximum frequency to 4 GHz Some bands very broad, some very narrow Is it possible to broaden these bands? – How much can these bands be broadened? e and h are limited to 5% increase α must remain at 90° → a = L - A

Broadening One Mode Frequency vs Phase Shift for 3 rd Dipole Mode For 3 rd dipole mode, 90°-cavity bandwidth is narrow – Especially compared with TESLA and ERL! How much can this particular bandwidth be broadened? Several broadening methods using geometry – Changing A incrementally – Changing A, B, and b in the direction of the gradient of increasing B 3 – Changing only B and b in the direction of the gradient of increasing B 3

Changing A Incrementally Of all the elliptic arc parameters, changing A has the biggest impact on B 3 A changed incrementally – B and b held at initial values – a held at a = L – A – Stopped when h increased by 5% B 3 increased from MHz to MHz B 3 vs ΔA

Changing A, B and b Derivatives of B 3 with respect to A, B and b were calculated – Used to create a 3-D gradient vector with length k in direction of increasing B 3 k increased until h increased 5% B 3 increased from MHz to MHz B 3 vs k

Changing B and b Idea: changing A affects h too much – Changes stopping too soon because of h – B and b have less effect on h → change just these two B and b derivatives used to create 2-D gradient vector with length k in direction of increasing B 3 k increased until e increased 5% – h increased less but e increased more! B 3 increased from MHz to MHz B 3 vs k

Broadening One Mode All three methods successfully broadened the 3 rd Dipole mode Changing A, B and b as a 3-D gradient → most successful method – B 3 grew 6 times wider! It is possible to significantly increase the bandwidth of one dipole mode of a 90°-cavity with limits on e and h by modifying only the elliptic arc parameters.

Broadening All Modes Next step: increase net bandwidth of all seven modes Need to maximize goal function: Monte Carlo Method 1.Derivatives taken for each B n with respect to each elliptic arc parameter (EAP) 2.Equations created predicting change in B n for change in EAPs (assuming linear dependence of B n on EAP) 3.10,000 random numbers generated from a set range for each EAP → 10,000 values for each B n prediction 4.EAPs maximizing predicted G without exceeding e or h limit recorded 5.Prediction tested Monte Carlo Casino

Broadening All Modes Predictions become much less accurate after range amplitude exceeds 1.0 – So different by range amplitude of 5.0 that calculations were stopped – Maybe derivatives continue to change with range → must be recalculated for every increase of 1.0? G was increased by MHz when the range amplitude was 5.0 ΔG vs Range of Random Numbers

Broadening All Modes In this case, derivatives were recalculated for each step of 1.0 in range Predicted and actual values are closer but differences more erratic G was increased by MHz when the range amplitude was 5.0 – Slightly less than when derivatives were kept the same! ΔG vs Range of Random Numbers

Broadening All Modes Both Monte Carlo approaches successfully increased the net bandwidth of all seven modes – Leaving derivatives the same → better results than recalculating at each step Small increase compared with initial G, but final value still better than ERL or TESLA It is possible to increase the net bandwidth of a 90°-cavity with limits on e and h by using a Monte Carlo technique to modify elliptic arc parameters. 90°, initial90°, finalERLTESLA G Frequency vs Phase Shift for 7 Dipole Modes Final: dashed Initial: solid line Brillouin light lines : dotted

Sixth Dipole Mode A special case: B 6 = f π – f π/4, not |f π - f 0 | as with all other modes – When general calculation is applied to this mode → B 6 is half what it should be – If half- or single-cell geometries are used for calculation, correct bandwidth is overlooked Multicell cavity must be used! More accurate bandwidth formula necessary for future broadening of bands – B = f max – f min ? Frequency vs Phase Shift for 6 th Dipole Mode

Conclusion Several successful ways to reduce trapped modes by broadening bandwidth were determined – A single mode was broadened significantly using a 3-D gradient vector to modify elliptic arc parameters – Net bandwidth was broadened using a Monte Carlo random number technique

Acknowledgements I would like to thank my advisor Valery Shemelin for his help and guidance throughout this project. Thanks also to everyone who made the CLASSE REU program possible. This work was supported by the NSF REU grant PHY