over view of t he pr oj ect acceler at or science updat e
play

Over view of t he pr oj ect acceler at or science Updat e - PowerPoint PPT Presentation

Plan Over view of t he pr oj ect acceler at or science Updat e since J une 2001 Next st eps A suite of light sources Why is an energy recovery linac so important? Because it allows you to take a MAJOR step beyond the


  1. Plan • Over view of t he pr oj ect • acceler at or • science • Updat e since J une 2001 • Next st eps

  2. A suite of light sources

  3. Why is an energy recovery linac so important? Because it allows you to take a MAJOR step beyond the stringent requirements and limitations of storage ring technology …. The single pass nature of the ERL gives rise to a number of very important advantages both in terms of the accelerator and the radiation produced.

  4. The benef its. . . � short pulses - f emt osecond regime � cont rol of pulse st ruct ure - pulse t ailoring � ef f ect ively inf init e beam lif et imes � larger peak current s � symmet rical beam and small emit t ance In addition, the ERL approach combined with high brightness injectors are ideal for free electron lasers, FELs. Photoinjector: The BNL Deep UV FEL project ERL Ring development JLAB

  5. Not a storage ring - ERL • spontaneous emission sources undulators and bending magnets • stimulated emission sources free electron lasers

  6. 4GLS undulator sources 1.0E+17 ERL 4GLS U28 ERL 4GLS U48 1.0E+16 • Opt imised f or high f lux and DIAMOND U48 Flux (photons/s/0.1%) ESRF U42 bright ness, in t he energy 1.0E+15 range 4-100 eV. 1.0E+14 • Up t o 500-600 eV available in 1.0E+13 t he higher harmonics. 1 10 100 1000 10000 100000 Photon Energy (eV) 1.0E+21 • Complement s Diamond by DIAMOND U48 2 /0.1%) ERL 4GLS U28 ESRF U42 reaching t o lower phot on 1.0E+20 2 /mrad energy and delivering an U48 Diffraction Limit Brightness (photons/s/mm 1.0E+19 order of magnit ude bet t er 1.0E+18 bright ness in t he sub-100 eV ERL 4GLS U48 energy range. 1.0E+17 1.0E+16 1 10 100 1000 10000 100000 Photon Energy (eV)

  7. 4GLS FELs

  8. 4GLS electron energy 600MeV Cavity based VUV-FEL � sub ps pulses � repetition rate, calcs for 6.25 MHz � photons 3-10 eV broad tunability up to 25 eV possible with restricted tunability � peak brightness 10 26 photons/(s mm 2 mr 2 0.1%BP) � photons per pulse ~10 13 XUV-FEL � fundamental 10-100 eV � seeded, 10s fs long, 10s µ s separation � peak power 1 mJ per pulse � peak brightness 10 29 photons/(s mm 2 mrad 2 laser BP) � photons per pulse ~10 14

  9. I R- FEL - electron energy ca. 50MeV IR-FEL 3-75 µ m Photocathode and superconducting linac, therefore � much greater average current � better energy stability � shorter pulse lengths better than anything around in Europe � synchronisation

  10. 4GLS FELs 1.E+30 XUV-FEL IR-FEL 2 .mrad 2 ) VUV-FEL 1.E+26 Peak Brightness ph/(s.0.1%bp.mm Undulators coherent enhancement 1.E+22 1.E+18 Bending Magnet 1.E+14 1.E+10 0.001 0.01 0.1 1 10 100 1000 Photon energy, eV

  11. Complementarity with table- top lasers

  12. 4GLS combines superconducting ERL, SR and FEL technology in a multi-source facility � ‘It incorporates the latest advances in machine design and builds upon those innovations to deliver a robust, flexible and cost-effective design.’ � ‘This project not only provides exceptional value, the flexibility of the design ensures that the facility can continue to grow as technological innovations occur’

  13. Accelerator challenges . . . • High cur r ent t ar get , 100mA, f or spont aneous SR user s (inj ect or and SC linac) • I nt egr at ion of a r ange of sour ces t hat ar e r equir ed t o oper at e as a user f acilit y • Synchronisat ion of individual sources t o levels appr opr iat e f or t he pump-pr obe experiment s

  14. 4GLS 4GLS of f er s … 10 7 t imes t hat � bright ness - XUV-FEL peak bright ness > of 3 rd generat ion sources Diamond/ Soleil spont aneous peak bright ness � short pulses - down t o f emt osecond regime � cont rol of pulse st ruct ure � coherence � ef f ect ively inf init e beam lif et imes � mult i-user access and � unique experiment al pot ent ial

  15. 4GLS f lux, bright ness, t iming � nanoscience � dynamics � t r ansient s, excit ed st at es � imaging � non-linear / high f ield phenomena

  16. Spintronics . . . � the next generation of electronics devices � study of individual nanoclusters of only a few atoms � modifications resulting from deposition � spin dependent transport, excitons spin resolved photoemission photoemission VUV-FEL cluster beam IR-FEL SHGMO, SPPES, MXCD, PEEM, pump-probe

  17. Devices that utilise electron spin . . . IBM Travelstar disc drive uses spintronic read head sensors. Areal bit densities up to 25.7 Gb per square inch achieved IBM web pages, James DaughtonWTEC Workshop on Spin- Electronics

  18. Future devices . . . Monsma et al., PRL 74 (1995) 5260, Science 281 (1998) 407

  19. Structure to f unction . . . � crystal structures - static � need to understand dynamics � protein folding just one specific aspect � complex coupling problem - far IR (collective modes) to electronic levels in UV - coupling critical to protein action � variety of timescales - sub picosecond to Science minutes � multi-wavelength pump-probe, time resolved CD, TR 3 , IR, ROA CONNECT STRUCTURE TO DYNAMICAL CONNECT STRUCTURE TO DYNAMICAL BEHAVIOUR AND FUNCTION BEHAVIOUR AND FUNCTION

  20. Dynamics . . . � IR-FEL, VUV-FEL, spontaneous radiation and TT laser/4GLS � Real time protein folding; understanding how biomolecular structure relates to function; human diseases and novel therapies - advanced molecular dynamics simulations HPCx

  21. I maging Second Harmonic Generated Magneto Optics Terahertz I R Dynamic sof t- XPEEM clusters, spintronics

  22. I maging: spectroscopy and dynamics . . . � intercellular signalling, receptor systems on membrane rafts � functional imaging in live cells, effects of pollutants, in vivo study of radiation damage � material-biological matrix interface, surface nanostructuring e.g. near field IR, UV RR spectroscopy, scanning near field SFS - localised imaging of sub cellular structures with resolutions approaching 30 nm IR AND VUV IR AND VUV FELs FELs - - SPATIAL SPATIAL AND DYNAMICAL INFO AND DYNAMICAL INFO

  23. 4GLS 4GLS TESLA technical design report, March 2001

  24. Pushing the limits … astrophysics/ astrochemistry � key fundamental measurements on multiply charged species - remove reliance on computed parameters � chemistry of the interstellar medium - ion-surface and gas Molecular interactions on ultracold surfaces phase interactions, formation of complex ions and molecules � enabling us to understand the origins of the universe PES, TOF-MS, RAIRS, circularly polarised light from VUV-FEL

  25. Non- linear phenomena Examples � mult iphot on excit at ion dynamics of at oms, molecules and ions � second harmonic magnet o opt ics at short er wavelengt hs � spect roscopy of excit ed solids Light -mat t er int eract ion in t he high int ensit y, high f requency regime is lit t le explored. Bet t er underst anding of coherent cont rol mechanisms. STRONG FIELD STRONG FIELD � resonanant behaviour > t uneabilit y PHYSICS PHYSICS � st rong communit y of t heoret ical groups uncharted territory

  26. Unique experimental f lexibility SR/FEL probe pulse � covers IR-XUV pump pulse � tailor pulses - selectable detector sample characteristics FEL/table- toplaser variable time delay � pump-probe options � combine SR and lasers

  27. Current position Science Case 17 th December 2001- Science Case (220 authors) submitted � � January/February - Peer reviewed by EPSRC on behalf of OST � April 2002 - RCUK recommend that 4GLS goes forward to Gateway 1. Project asked to undergo Gateway 1 by Nov/Oct Business Case 15 th October 2002 - Business Case prepared � OGC Gateway 1 Review 4 days October 29 th to November 1 st - Recommendations to improve � the probability of success of the project

  28. Business Case � Major stakeholders identified UK Scientific Community, DTI(OST), NWDA,CCLRC & other Research Councils � Major risks identified and assessed � Options appraised: 4GLS is the option of choice Other ways of meeting the science need not cost-effective The facility should be: � located at Daresbury - for rapid and efficient implementation � managed by CCLRC - consistent with post-QQR2 policy for large-scale facilities Influence release of R&D and Design Study funds ...

  29. The bottom line . . . � £5M to design � £113M to build and commission (including VAT) � £9.1M per annum to run (split approximately equally between staff and non-staff costs) NWDA

  30. The next steps . . . � R&D � build international and national collaborations establish new links where needed � identify and pursue funding streams � develop science case � design study

  31. ht t p:/ / www.4gls.ac.uk

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend