storage ring compton light sources · 2010-09-09 · dfell, duke university 48th icfa future light...
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48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Work supported by U.S. Grant and Contract:
DOE DE-FG02-01ER41175 and AFOSR MFELFA9550-04-01-0086
Acknowledgment:
M. Busch, M. Emanian, J. Faircloth, S. Hartman, J. Li, S. Mikhailov, V. Popov, G. Swift, P. Wang, P. Wallace (DFELL)
M. Ahmed, T. Clegg, H. Gao, C. Howell, H. Karwowski, J. Kelley, A. Tonchev, W. Tornow, H. Weller (TUNL)
HIGS Collaborators
Y. K. Wu
DFELL, Triangle Universities Nuclear Laboratory
Department of Physics, Duke University
March 2, 2010
Storage Ring Compton Light Sources
Y. K. Wu
Outline
Compton Gamma-ray SourcesA brief historical overviewMajor Compton gamma-ray facilitiesNew projects
High Intensity Gamma-ray Source (HIGS)Accelerator facilityOperation modesBeam diagnosticsOptical resonator issuesHigh flux operation
Issues with Compton Light Sources: focus on Gamma-ray SourceAcceleratorsLaser beamsEnergy rangeImpacts on LS operation due to Compton gamma-ray source
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
History of Compton Light Sources
Early HistoryEarly 1920's, Arthur Compton, Discovery of Compton Effect
A. H. Compton, Bulletin Nat. Res. Council (U.S.) 20, 19 (1922); Phys. Rev. 21, 483 (1923)
1963, Milburn, and Arutyunian and Tumanian, first proposed γ-beam production via Compton back-scattering of photon with accelerator based high-energy electron beam
R. H. Milburn, Phys. Rev. Lett. 10, 75 (1963). F. R. Arutyunian and V. A. Tumanian, Phys. Lett. 4, 176 (1963).
1963 – 1965, the first Compton γ-ray beam experimental demonstrations,– Kulikov et al.with a 600 MeV synchrotron– Bemporad et al. with the 6.0 GeV Cambridge Electron Acclerator
O. F. Kulikov et al., Phys. Lett. 13, 344 (1964); C. Bemporad et al., Phys. Rev. B 138, 1546 (1965).
1967 – 1969, Ballam et al. with the 20 GeV Stanford linear Acclerator, first physics measurements using Compton γ-ray beam to study the photo-production cross section (~GeVs) with a hydrogen bubble chamber
J. J. Murray and P. R. Klein, SLAC Report No. SLAC-TN-67-19, unpublished (1967). J. Ballam et al., Phys. Rev. Lett. 23, 498 (1969).
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
History of Compton Light Sources
Major Compton Gamma Source Facilities (1970's – 1990's)1978 – 1993, LADON, ADONE storage ring, Frascati, ItalyThe first γ-ray Compton light source facility for nuclear physics research, by colliding electron beam
(1.5 GeV) inside a laser cavity. It produced polarized γ-ray beams up to 80 MeV with an on-target flux of up to 5x10^5 s−1 for nuclear experiments.
L. Casano et al., Laser and Unconv. Opt. J. 55, 3 (1975).G. Matone et al., Lect. Notes Phys. 62, 3 (1977).L. Federici et al., Nuovo Cimento Lett. 27, 339 (1980).L. Federici et al., Nuovo Cimento B 59, 247 (1980).D. Babusci et al., Nucl. Instrum. Methods A 305, 19 (1991).
1987 – 2006, LEGS, NSLS x-ray ring, Brookhaven National Lab, USA. M. Sandorfi et al., IEEE Trans.NS-30, 3083 (1984).
1993 – persent, ROKK-1/ROKK-2/ROKK-1M, Budker Institute of Nuclear Physics, RussiaG. Ya. Kezerashvili et al., Nucl. Instrum. Methods A. 328, 506 (1993).G. Ya. Kezerashvili et al., AIP Conference Proceedings 343, 260 (1995).G. Ya. Kezerashvili et al., Nucl. Instrum. Methods B. 145, 40 (1998).
1995 – 2008, GRAAL, ESRF storage ring, ESRF, Grenoble, FranceA. A. Kazakov et al., JETP Lett. 40, 445 (1984).
1996 – present, HIγS, Duke FEL storage ring, Duke University, USV. N. Litvinenko et al., Phys. Lett. 78, 4569 (1997).
1998 – present, LEPS, Spring-8 storage ring, Spring-8, JapanT. Nakano et al., Nucl. Phys. A 629, 559c (1998). T. Nakano et al., Nucl. Phys. A 684, 71c (2001).
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
History of Compton Light Sources
H.R. Weller et al. Progress in Particle and Nuclear Physics 62, p. 257-303 (2009).
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
New Compton Source Projects
A Few New Compton Source Projects in Planning and Development Shanghai Laser Electron Gamma Source (SLEGS), Shanghai Synchrotron Radiation Facility
(SSRF)– 3.5 GeV electron beam and a 500 W CO2 polarized laser– An energy up to 22 MeV and a flux of 109-10γ/s
Q. Y. Pan et al., Synchrotron Radiation News, Volume 22, Issue 3, p. 11 (2009).
Compton Gamma Source Project at MAX-lab– 3 GeV electron beam from the MAX IV storage ring to be built, up to 500 mA– An ultraviolet (UV) laser beam– The maximum gamma-ray energy around 500 MeV– A tagged flux as high as a few times 107 γ/s
L. Isaksson, MAX-lab, Lund, Sweden, private communication (2009).
Laser-Electron Photon 2 (LEPS2), Spring-8– For conducting research in the quark-nuclear physics– Higher intensity and higher maximum energy compared with LEPS– Expanded detector acceptance for a 4π γ-detector.
The LEPS2 website, www.hadron.jp; and the 2006 RCNP Annual Report, for example, www.rcnp.osaka-u.ac.jp/~annurep/2006/topics/yosoi.pd
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Major Compton Gamma Source Facilities Around the World
HIGSLEGS
GRAAL
LADON
ROKK
LEPSSLEGS
MAX-Lab
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
A Storage Ring Compton Gamma Source
High Intensity Gamma-ray Source (HIGS)
at Duke University
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
HIGS AcceleratorsHigh Intensity Gamma-ray Source (HIGS) Accelerators
Recent Accelerator UpgradesNew lattice for OK-5 FELNew HOM-damped RF cavityNew OK-5 FEL with circular polarizationA New Booster synchrotron for top-off injection
Typical User Operation Modes
FEL: single-bunch, up to 95 mAHIGS: two-bunch, 80 - 110 mA
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
HIGS AcceleratorsOK-5 and OK-4 FELs (Since Aug. 2005)
OK-5 wigglers
OK-4 wigglers
OK-4 Planar wigglers
OK-5 helical wiggler, OK-5A
OK-5 helical wiggler, OK-5B
20.15 m
e-beam
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
HIGS ResearchOperation Principle of HIGS
52.8 m
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
HIGS ResearchOperation Modes of HIGS Operation Modes of HIGSQusi-CW operation vs PulsedHigh-flux vs high energy resolution
FWHM
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
HIGS ResearchHigh Energy-Resolution Operation
Asymmetric Bunch Pattern: one large (lasing) and one small (non-lasing)
Improving stability of gamma energy resolution and increase fluxDevelop a reliable way to measure bunch pattern, andAn automatic injection scheme to maintain charge distribution
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Beam Diagnostics/FeedbackElectron/Photon Collision Angle Monitor
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Beam Diagnostics/FeedbackBunch Length and FEL Spectrum Monitors
Beam DiagnosticsLive Spectrum Monitor
Live bunch length monitors
349 MeV, 27 mA
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Beam Diagnostics/FeedbackBunch-by-bunch Longitudinal Feedback
Providing bunch-by-bunch damping of longitudinal instabilities
Part of Ph.D. thesis work of Wenzhong Wu
Commissioned for User Operation (Oct., 2008)
With .
iGp-64F Digital signalprocessing system
MILMEGA 200 WPower amplifier
LFB BPM
Pill-box cavity
Feed through
Nose cone
Beam pipe
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Beam Diagnostics/FeedbackLFB Stabilizing Longitudinal Motion
Synchrotron sidebands LFB OFF574 MeV, 4-bunch, 15 mASynchrotron sidebands?
LFB ON574 MeV, 4-bunch, 15 mA
Part of Ph.D. thesis work of Wenzhong Wu
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Beam Diagnostics/FeedbackIn-cavity Aperture System for High Current Operation
Electron Beam
Part of Ph.D. thesis work of Senlin HuangNIM A 606, p. 762 (2009).
WIG01 WIG02 WIG03 WIG03 Mirror
16.54 m6.72 m6.72 m6.72 m
22.29 mCollision
Point
Mirror
Lw = 4 m 4.58 m
Aperture
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Beam Diagnostics/FeedbackCorrecting Mirror Deformation
45 MeV Setup with OK-5 FEL
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
HIGS SummaryStability of Gamma Operation in Electron Loss Mode
Current
Gamma flux
Current
Gamma flux
with closed apertures
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
High-Finesse FEL ResonatorHigh Reflectivity FEL Mirrors
780 nm MirrorsMinimal round-trip loss: ~ 0.107%Finesse @ Low power ~ 3,000
Effective: R ~ 99.95%
761 nm, Loss ~0.00107
Kicker firing
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
High-Finesse FEL ResonatorHigh Reflectivity FEL Mirrors
Mirror degradationCarbon deposition on the surface
Horizontal
Vertical
780 nm, CCV020, downstream cavity mirror, D=50 mm
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Intracavity FEL Power MeasurementExperimental Layout
12m
Collimated (d=3/4”), γ-beam image
Collimated flux: 3.68%
Ebeam: 514 MeV, about 88 mA in two equally populated bunches
FEL beam λ = 545 nm;
Gamma-beam collimator: d = 0.75”
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Intracavity FEL Power MeasurementIntracavity FEL Power Measurements: γ-Spectrum
Ebeam: 514 MeV, about 88 mA in two equally populated bunches
FEL beam λ = 545 nm;
Gamma-beam collimator: d = 0.75”
True γ-spectrum
Avg Flux Density from 11B at 8.916 MeV
11B data: Pb = 800 (+/-100) W, PFEL = 1.6 kW (+/- 0.2 kW)
C. Sun et al. NIMA 605, p 312(2009)
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Intracavity FEL Power MeasurementIntracavity FEL Power Measurements
Ebeam: 514 MeV; FEL beam λ = 545 nm; Collimator: d = 0.75”
HPGe data
Preliminary Results: HPGe data
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Gamma Energy Tuning Range with OK-5 FEL (3.5 kA)
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Highest Total Flux (2009): > 1010 γ/s @ 9 – 11 MeV
H. R. Weller et al., “Research Opportunities at the Upgraded HIγS Facility,” Prog. Part. Nucl. Phys. Vol 62, Issue 1, p. 257-303 (2009).
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Nuclear Physics and AstrophysicsNuclear Physics and Astrophysics Research at HIGS
Nuclear StructureFew-Nucleon PhysicsAstro-physicsGerasimov-Drell-Hearn (GDH) Sum RuleCompton Scattering from NucleonsPhoton-Pion Physics
H. R. Weller et al., “Research Opportunities at the Upgraded HIγS Facility,” Prog. Part. Nucl. Phys. Vol 62, Issue 1, p. 257-303 (2009).
HIGS
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Accelerators for Compton Light Sources
Advantages of storage rings– High repetition rate– Orbit stability and beam stability (at higher energies)– Adequate ebeam emittance and energy spread– Known technologies– Powering a high average flux Compton source
Other Accelerators– Warm temperature Linacs:
• Low rep-rate pulsed operation• Expensive laser• Less stable• Powering a high peak flux source
– Super-conducting linac (e.g. ERL)• High rep-rate• Costly• Less mature technology• A potential driver for very high average flux source
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
– Tuneable wavelength => a large Compton photon energy range– Self-synchronization and self alignment– Complex and Expensive– High intracavity power– Driver for a versatile, high-flux Compton source for a wide range of research
programsExternal Lasers
– Ti:sapphire m TW lasers, low reprate, time syn, low stability, costly– CW lasers–––
Laser Cavities– Used in LADON project (low finesse)– High finesse Fabry-Perot cavity
• DC laser with high finesse– JLAB, Compton polarimeter, 1064 nm, finesse 30,000, 1.6
kW• CW pulsed laser
– Laboratoire de l’Acce´le´rateur Line´aire, C.N.R.S./IN2P3, Orsay, France
– Ti:sapph, 76 MHz, 1 ps, finesse 30,000
V. Brisson, e t al. Nucl. Instrum. Meth. A 608(2009)S75–S77
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
– 0.1 eV photons, 10 – 100 keV x-rays, e-beam: 80 – 250 MeV;– 1eV photons, 10 – 100 keV x-rays, e-beam: 25 – 80 MeV;– E-beam, 2 GeV, 0.1 eV photons, γ-ray: 6 MeV– E-beam, 2 GeV, 1 eV photons, γ-ray: 60 MeV– E-beam, 3 GeV, 0.1 eV photons, γ-ray: 14 MeV– E-beam, 3 GeV, 1 eV photons, γ-ray: 140 MeV
Figure of Merits for Gamma-ray Beams:– Brightness is no longer a good figure of merit for gamma-ray beam– New merits: flux (γ/s), spectral flux (γ/s/eV, avg, peak), relative energy spread
(FWHM)Compton X-ray Source Driven by a Storage Ring
– Don Ruth, SLAC, www.lynceantech.com.– Next talk: “Experience with the Compact light source”
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Critical Issues for Storage Ring Compton Gamma SourcesImpact On the Storage Ring Light Source when
Operating Compton Gamma Source as an Optical Insertion Device (OID)Effect of Electron LossWhen Compton scattered electron loses more energy than allowed by the energy aperture (smaller of energy
dynamic aperture and energy acceptance limited by RF/vacuum chambers).Two strategies:
– “Hide” loss among beam lifetime• Electron-loss mode operation (Energy loss > Aperture)• Good for higher energy gamma operation• Limited flux: 10^6 – few 10^7 γ/s• Gamma-ray energy determination: Tagging of electrons
– Prevent electron loss• No-loss mode (Energy loss < Aperture)• Good for lower energy gamma operation• High flux possible (greater than 10^9 γ/s)• Gamma-ray energy selection: Collimation of gamma-beam
Impact on Electron Beam Parameters– An issue with extremely high flux operation– Impact on e-beam energy and longitudinal distributions– (estimates using damping wiggler model; need real simulation)– Impact on transverse beam distribution (emittance)
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
– High gamma beam energies <=> User research programs– Additional flux limitation due to tagging rate, 10^5 – 10^6 e-/s per tagging channel– High efficincy: tagging a large amount of Compton gamma-rays: 30% - 60%– Energy resolution as limited by the absolute energy spread of the e-beam
• Example: 3 GeV e-beam, 0.1% (sigmaE), 150 MeV gamma-ray • dE (FWHM) = 7.1 MeV; dE/E (γ,FWHM) = 5%;
– Reliability of tagging signal at high ratesCollimation
– Low gamma beam energies <=> User research programs– If OID, fixed gamma energy with a fixed e-beam energy; how to vary gamma energy?– Potentially very high flux– Low efficiency: collimation selects only a few percent Compton gamma-rays– Challenge in high precision flux measurement (pileups, scattering, secondary particles, etc)– Energy spread issues: collimation effect, e-beam energy spread, emittance effect
• Long beamline• Good e-beam aiming stability• Example: 3 GeV e-beam, ~5% γ-beam energy spread (FWHM)
– Half opening angle: 30 micro-radians– If collimator aperture r = 3 mm, beamline length ~ 100 m;– Stability of ebeam aiming; a few micro-radians
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Part of Ph.D. thesis work of Changchun SunPhys. Rev. ST Accel. Beams 12, 062801 (2009)
Energy Spread of γ-beamEnergy Distribution of Compton Gamma-beam
Monochromatic electron and photon beamsEmittance Effect (Scaled)E-beam Energy Spread Effect (Scaled)Collimator EffectCollimator Effect (Scaled)
New Merit:Degree of Collimation
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Industrial and Medical ApplicationsCompton Gamma-beam Imaging at HIGS
Polarization Effect: Linear vs Circular22.5 MeV Gamma-beam
680 MeV-ebeam, 378 nm FEL, 27 m from collision
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Industrial and Medical ApplicationsCompton Gamma-beam Imaging at HIGS
Imager Resolution Test with a bar phantom test and 2.75 MeV gamma-beam
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Industrial and Medical ApplicationsCompton Gamma-beam Radiograph
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
The End
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
1 MeV Gamma-beamHigh Resolution Mode:
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Switch-yard for OK-4 and OK-5 Wigglers
Photon-pion physics150 – 160 MeV operation with the OK-5 FEL lasing around 150 nm
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Summary
High Intensity Gamma-ray Source Development and User ResearchAn Overview of HIGS Accelerator Facility and Development Program: Accelerator Physics and FEL ResearchAn Overview of HIGS User Research Program: Nuclear Physics Program
HIGS Capabilities (2009) Energy Tuning: 1 - 100 MeV Maximum Total Flux: > 1010 γ/s around 9 - 10 MeV
Maximum Spectrum Flux: : ~ 103 γ/s/eV around 5 - 10 MeV
High Energy Resolution: 0.8% (< = 5 MeV) Polarization: linear, and switchable left- and right-circular
HIGS Near-Term Development Higher Gamma-beam Energy: 100 - 160 MeV for photon-pion physics research Higher Flux Operation: 1011 γ/s total below 20 MeV
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
HIGS beam-on-target: 1584 hr
HIGS Operation Summary (Aug. 1, 2008 – Jul . 31, 2009)
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Industrial and Medical ApplicationsCompton Gamma-beam Imaging
RadiographTH571A Tetrode tube
H. Toyokawa, NIM A545, p. 469 (2005) Sample CT images using 10 MeV LCS photon beam
AIST, Tsukaba, Ibaraki, Japan
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
High-Finesse FEL ResonatorHigh Reflectivity FEL Mirrors
General Optics, GSI (2008)
Tmin ~ 0.0015%
High Reflectivity Mirrors (1060 – 520 nm)Spec: R > 99.95%Example: transmission 15 ppm @ 780 nm (Vendor measurement)
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Intracavity FEL Power MeasurementIntracavity FEL Power MeasurementsEbeam: 514 MeV; FEL beam λ = 545 nm; Collimator: d = 0.75”
HPGe data
Preliminary Results: HPGe data
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Industrial and Medical ApplicationsRadiation Therapy and Diagnostics
K. J. Weeks., NIM A393 (1997) p. 544-547.
15 MeV Compton g-beam
g-beam from 15 MeV Linac
Radioisotopes
Cancer treatment: 1012 – 1014 g/s
Diagnostic: 1012 g/s
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu
Industrial and Medical ApplicationsRadiation Therapy and Diagnostics
B Girolami et al. Phys. Med. Biol._v41, p1581(1996).
Radiation Dose for Cancer Treatment
A solid epithelial tumor ranges: 60 - 80 Gy
Lymphoma tumor: 20 – 40 Gy
48th ICFA Future Light Sources Workshop (FLS2010), SLACDFELL, Duke University Y. K. Wu