Electron Linear Accelerators & Free-Electron Lasers

Similar documents
Free-electron laser SACLA and its basic. Yuji Otake, on behalf of the members of XFEL R&D division RIKEN SPring-8 Center

4 FEL Physics. Technical Synopsis

Linac Based Photon Sources: XFELS. Coherence Properties. J. B. Hastings. Stanford Linear Accelerator Center

Research with Synchrotron Radiation. Part I

Introduction to electron and photon beam physics. Zhirong Huang SLAC and Stanford University

SPARCLAB. Source For Plasma Accelerators and Radiation Compton. On behalf of SPARCLAB collaboration

Free Electron Laser. Project report: Synchrotron radiation. Sadaf Jamil Rana

Simulations of the IR/THz source at PITZ (SASE FEL and CTR)

Simulations of the IR/THz Options at PITZ (High-gain FEL and CTR)

3. Synchrotrons. Synchrotron Basics

Experimental Optimization of Electron Beams for Generating THz CTR and CDR with PITZ

Introduction to Synchrotron Radiation

Beam Echo Effect for Generation of Short Wavelength Radiation

Short Pulse, Low charge Operation of the LCLS. Josef Frisch for the LCLS Commissioning Team

VARIABLE GAP UNDULATOR FOR KEV FREE ELECTRON LASER AT LINAC COHERENT LIGHT SOURCE

Brightness and Coherence of Synchrotron Radiation and Free Electron Lasers. Zhirong Huang SLAC, Stanford University May 13, 2013

Synchrotron radiation: A charged particle constrained to move in curved path experiences a centripetal acceleration. Due to it, the particle radiates

Diagnostic Systems for Characterizing Electron Sources at the Photo Injector Test Facility at DESY, Zeuthen site

Potential use of erhic s ERL for FELs and light sources ERL: Main-stream GeV e - Up-gradable to 20 + GeV e -

Introduction to single-pass FELs for UV X-ray production

Liverpool Physics Teachers Conference July

Investigation of the Feasibility of a Free Electron Laser for the Cornell Electron Storage Ring and Linear Accelerator

Coherence Properties of the Radiation from X-ray Free Electron Lasers

Coherent X-Ray Sources: Synchrotron, ERL, XFEL

FURTHER UNDERSTANDING THE LCLS INJECTOR EMITTANCE*

Light Source I. Takashi TANAKA (RIKEN SPring-8 Center) Cheiron 2012: Light Source I

NON LINEAR PULSE EVOLUTION IN SEEDED AND CASCADED FELS

Part V Undulators for Free Electron Lasers

High Energy Gain Helical Inverse Free Electron Laser Accelerator at Brookhaven National Laboratory

Simple Physics for Marvelous Light: FEL Theory Tutorial

Insertion Devices Lecture 2 Wigglers and Undulators. Jim Clarke ASTeC Daresbury Laboratory

Echo-Enabled Harmonic Generation

Harmonic Lasing Self-Seeded FEL

USPAS course on Recirculated and Energy Recovered Linacs Ivan Bazarov, Cornell University Geoff Krafft, JLAB. ERL as a X-ray Light Source

X-ray Free-electron Lasers

PAL LINAC UPGRADE FOR A 1-3 Å XFEL

Synchrotron radiation: A charged particle constrained to move in curved path experiences a centripetal acceleration. Due to this acceleration, the

Research Topics in Beam Physics Department

The peak brilliance of VUV/X-ray free electron lasers (FEL) is by far the highest.

Linac Driven Free Electron Lasers (III)

LCLS-II SCRF start-to-end simulations and global optimization as of September Abstract

Generation and characterization of ultra-short electron and x-ray x pulses

Short Wavelength SASE FELs: Experiments vs. Theory. Jörg Rossbach University of Hamburg & DESY

Cooled-HGHG and Coherent Thomson Sca ering

Energy Recovery Linac (ERL) Properties. Physics Dept. & Cornell High Energy Synchrotron Source (CHESS) Ithaca, NY Cornell University

Undulator radiation from electrons randomly distributed in a bunch

arxiv: v1 [physics.acc-ph] 1 Jan 2014

ASTRA simulations of the slice longitudinal momentum spread along the beamline for PITZ

First operation of a Harmonic Lasing Self-Seeded FEL

Accelerator Physics NMI and Synchrotron Radiation. G. A. Krafft Old Dominion University Jefferson Lab Lecture 16

Transverse Coherence Properties of the LCLS X-ray Beam

START-TO-END SIMULATIONS FOR IR/THZ UNDULATOR RADIATION AT PITZ

SLAC Summer School on Electron and Photon Beams. Tor Raubenheimer Lecture #2: Inverse Compton and FEL s

INNOVATIVE IDEAS FOR SINGLE-PASS FELS

Two-Stage Chirped-Beam SASE-FEL for High Power Femtosecond X-Ray Pulse Generation

Introduction to Particle Accelerators & CESR-C

X-band RF driven hard X-ray FELs. Yipeng Sun ICFA Workshop on Future Light Sources March 5-9, 2012

SwissFEL INJECTOR DESIGN: AN AUTOMATIC PROCEDURE

Linac optimisation for the New Light Source

Experimental Path to Echo-75 at NLCTA

Needle cathodes for high-brightness beams. Chase Boulware Jonathan Jarvis Heather Andrews Charlie Brau

Transverse dynamics Selected topics. Erik Adli, University of Oslo, August 2016, v2.21

Start-to-End Simulations

The Linac Coherent Light Source II (LCLS II) at SLAC

parameter symbol value beam energy E 15 GeV transverse rms beam size x;y 25 m rms bunch length z 20 m charge per bunch Q b 1nC electrons per bunch N b

New Electron Source for Energy Recovery Linacs

Greenfield FELs. John Galayda, SLAC Kwang-Je Kim, ANL (Presenter) James Murphy, BNL

SCSS Prototype Accelerator -- Its outline and achieved beam performance --

Coherence properties of the radiation from SASE FEL

Update on and the Issue of Circularly-Polarized On-Axis Harmonics

Accelerator Physics. Tip World Scientific NEW JERSEY LONDON SINGAPORE BEIJING SHANGHAI HONG KONG TAIPEI BANGALORE. Second Edition. S. Y.

Excitements and Challenges for Future Light Sources Based on X-Ray FELs

Excitements and Challenges for Future Light Sources Based on X-Ray FELs

LCLS Accelerator Parameters and Tolerances for Low Charge Operations

An Adventure in Marrying Laser Arts and Accelerator Technologies

Free-Electron Lasers

Femto-second FEL Generation with Very Low Charge at LCLS

Introduction to Free Electron Lasers and Fourth-Generation Light Sources. 黄志戎 (Zhirong Huang, SLAC)

The Free Electron Laser: Properties and Prospects 1

Energy Recovery Linac (ERL) Science Workshop

FLASH/DESY, Hamburg. Jörg Rossbach University of Hamburg & DESY, Germany - For the FLASH Team -

Electron Spectrometer for FLASHForward Plasma-Wakefield Accelerator

FEL SIMULATION AND PERFORMANCE STUDIES FOR LCLS-II

Traveling Wave Undulators for FELs and Synchrotron Radiation Sources

Observation of Coherent Optical Transition Radiation in the LCLS Linac

Towards a Low Emittance X-ray FEL at PSI

Compact Wideband THz Source

2. X-ray Sources 2.1 Electron Impact X-ray Sources - Types of X-ray Source - Bremsstrahlung Emission - Characteristic Emission

OPTIMIZATION OF COMPENSATION CHICANES IN THE LCLS-II BEAM DELIVERY SYSTEM

LCLS Commissioning Status

Performance Metrics of Future Light Sources. Robert Hettel, SLAC ICFA FLS 2010 March 1, 2010

Characterization of an 800 nm SASE FEL at Saturation

Expected properties of the radiation from VUV-FEL / femtosecond mode of operation / E.L. Saldin, E.A. Schneidmiller, M.V. Yurkov

CONCEPTUAL STUDY OF A SELF-SEEDING SCHEME AT FLASH2

Simulation of transverse emittance measurements using the single slit method

Opportunities and Challenges for X

Low Emittance Machines

PHYS Introduction to Synchrotron Radiation

How Does It All Work? A Summary of the IDEAS Beamline at the Canadian Light Source

CSR calculation by paraxial approximation

Transcription:

Electron Linear Accelerators & Free-Electron Lasers Bryant Garcia Wednesday, July 13 2016. SASS Summer Seminar Bryant Garcia Linacs & FELs 1 of 24

Light Sources Why? Synchrotron Radiation discovered in 1947 at the 70 MeV GE synchrotron Originally a loss mechanism for electron synchrotrons ( On the maximal energy attainable in betatron, (1944)) Spells the doom for (circular) electron machines as energy frontier devices but... Bryant Garcia Linacs & FELs 2 of 24

Electron Machine Basics Why? m e = 0.511MeV /c 2 ; m p = 938MeV /c 2 ; m p /m e 1835! The beginning of the beamline: E gun 1MeV Electrons are almost immediately relativistic This affects synchrotron radiation: P s 1/m 4 Bryant Garcia Linacs & FELs 3 of 24

Synchrotron Radiation Basics A tough (but straightforward) EM calculation gives, dw dω = 3e 2 4πɛ 0 c γ ω ω c ω/ω c K 5/3 (x)dx ω c 3 c 2 ρ γ3, λ c = 4π 3 ρ γ 3 Wavelength spectrum peaked near λ c γ 500, ρ 10m, λ c 10 nm! (but broad!) Enables the tunable production of high energy, BRIGHT photon pulses Bryant Garcia Linacs & FELs 4 of 24

The Evolution of Light Sources 1st generation: Parasitic synchrotron radiation from high energy physics machines 2nd generation: Dedicated synchrotron machines for production of light 3rd generation: Evolved facilities with insertion devices, many beamlines 4th generation: Free-electron Lasers and Electron-recirculating linacs APS Bryant Garcia Linacs & FELs 5 of 24

The Spectral Brightness Race Bryant Garcia Linacs & FELs 6 of 24

The typical beamlines Bryant Garcia Linacs & FELs 7 of 24

The Typical X-FEL Layout Electron source (Gun) Linear accelerating sections Bunch compression Undulators (radiation generation) Bryant Garcia Linacs & FELs 8 of 24

The LCLS Video http://lcls.slac.stanford.edu/animationviewlcls.aspx Bryant Garcia Linacs & FELs 9 of 24

In the beginning... Electron Guns Cathode emits electrons (Thermionic or Photoelectric) Typically UV Laser λ 260nm on Cu Cathode High gradient RF Field ( 100MV/m) accelerates electrons to relativistic speeds Fighting against beam space charge to preserve a pristine electron beam Bryant Garcia Linacs & FELs 10 of 24

The Electron Acceleration High-frequency RF accelerates the electrons in conducting cavities Matched phase velocity ensures electrons are continuously accelerated in each cell Possible superconducting (LCLS-II), or PWFA (FACET) technologies at this step Bryant Garcia Linacs & FELs 11 of 24

The magnetic undulator Series of alternating magnetic poles with periodicity λ u, K eb 0 k umc x(z) = K γk u cos k u z Lorentz transform to the beam rest frame: k u = γk u or λ u = λ u /γ This is larmor radiation, and has wavelength λ u In the lab frame, this radiation is blueshifted again by a factor of 2γ, so we expect lab radiation λ r λ u 2γ 2 Estimate λ r = λ u 2γ 2 ( 1 + K 2 /2 + γ 2 θ 2) Reality Bryant Garcia Linacs & FELs 12 of 24

Undulator Radiation The undulator radiation is then simply described as { E0 e E(t) = iωr t, N u λ u /2c < t < N u λ u /2c 0, otherwise Frequency response is found via fourier transform (T N u λ u /2c) F (ω) = E(t)e iωt dt = T T E 0 e i(ω ωr )t dt Bryant Garcia Linacs & FELs 13 of 24

Undulator Radiation Cont d. F (ω) = 2TE 0 sinc(t (ω ω 0 )) This spectrum has a FWHM ω = ω 0 /N u Bryant Garcia Linacs & FELs 14 of 24

Coherent Radiation Normally, electron radiation is incoherent, that is, the phase of each electron s emission is random. Incoherent power P N e. If the electron bunch has a size < λ r, the phases are all roughly equal Coherent emission P N 2 e for Coherent emission ( 10 9!) Bryant Garcia Linacs & FELs 15 of 24

Free-Electron Lasers - Oscillators We can achieve coherence through low-gain operation and a cavity, as in a traditional laser Can use low energy e beams to make Visible-Microwave radiation Requires reflective optics at the wavelengths of interest no X-rays Bryant Garcia Linacs & FELs 16 of 24

Free-Electron Lasers - High Gain Devices Another option is to have a very LONG undulator, and allow an instability to develop: Bryant Garcia Linacs & FELs 17 of 24

The FEL instability The radiated light becomes intense enough to back-react on the electron bunch The effect is to bunch the electrons up at the radiation wavelength [ Video ] The bunching more coherent emission stronger EM field more bunching Bryant Garcia Linacs & FELs 18 of 24

Some FEL Physics The physics of the FEL process is all (basically) controlled by a single parameter ρ: ( ) 2/3 ( ρ = 1 ) ˆKλu I 1/3 2γ 2πσ b I A P sat = ρ ( ) IEb = ρp beam e L g = λ u 4π 3ρ For reference, modern X-ray FELs have ρ 5 10 4, λ u cm. So L g few meters. Turns out you need 20L g to saturate very long undulators Bryant Garcia Linacs & FELs 19 of 24

More FEL Physics λ r 1nm ɛ < 0.1nm! This is very small! Storage rings have a natural emittance nm at best, so cannot be used for X-ray FELs linac sources Bryant Garcia Linacs & FELs 20 of 24 To maintain spatial coherence, the phase space volume of the electrons should be less than the phase space volume of the photons: ɛ electrons < ɛ photon ɛ electrons < λ r 4π

Beam requirements for High-Gain XFELs Require very low emittance (for transverse matching) Require high energy electrons (for low λ r ) Require high peak current I /I A (for high ρ) Bryant Garcia Linacs & FELs 21 of 24

SASE Operation Mode Random electron beam seeds the instability with noise Locations/size of lasing regions are stochastic Many spectral spikes, non-utilization of full electron beam Spatially but not temporally coherent radiation Bryant Garcia Linacs & FELs 22 of 24

Coherence Length The reason for the many spikes is that information is generally not propagated through the whole electron beam λ r = λ u 2γ 2 ( 1 + K 2 /2 ) This is also a resonance condition: Bryant Garcia Linacs & FELs 23 of 24

Coherence Length 2 The light slips forward by one radiation wavelength per undulator period Coherence Length: Slippage in one gain length L c λ r /πρ l beam So the individual SASE spikes never have time to fully communicate Bryant Garcia Linacs & FELs 24 of 24