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LNF-INFN Frascati

LNF-INFN Frascati. BTF. Peak luminosity evolution in 2004-5. Luminosity is what matter…in our case. L = 1.46 10 32 cm -2 s -1 (to day). KLOE FINUDA LUCE DI SINCROTRONE FISICA di MACCHINA-SRFF FASCI ESTRATTI. …..and the physics…. KLOE – (K LOng Exp.).

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LNF-INFN Frascati

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  1. LNF-INFN Frascati

  2. BTF

  3. Peak luminosity evolution in 2004-5 Luminosity is what matter…in our case L = 1.46 1032 cm-2s-1 (to day) KLOE FINUDA LUCE DI SINCROTRONE FISICA di MACCHINA-SRFF FASCI ESTRATTI …..and the physics….

  4. KLOE – (K LOng Exp.) Sistematic study of exotic nuclei DAFNE experiments KLOE is running his year FINUDA Kaons absorbed by nuclei DAFNE e+e- F KK is a source of monochromatic correlated low energy Kaons

  5. The program is well defined for the coming three years KLOE FINUDA exotic nuclei FINUDA exotic nuclei SRFF ? SIDDHARTA Kaonic atoms 2006 2007 2008 TODAY

  6. KLOE physics results: Vus from KL, KS and charged K’s Kaon form factors Pion form factors/g-2 Ks rare decays charged kaon decays KS semileptonic decays KL branching ratios KL life time KS to gg F radiative decays eta decays KO-KObar interference

  7. Collect 2 fbarn-1 on F resonance – end of the current year • 2) Scan over the F resonance 50 pbarn-1 • 3) 250 pbarn-1 at 1000MeV , below the F, to measure pion form factors 1st April 2006 END of KLOE 2006 Nuclear Physics with FINUDA 2007 Kaonic Atoms with SIDDHARTA 2008 FINUDA and SRFF with DAFNE

  8. Experimental studies on short-bunches and bunch-length modulation at DAFNE SRFF = Superconductive RadioFrequency Focusing EXPERIMENT SC 1.3 GHz cavity Longitudinal phase space IP RF input RF center RF output Energy spread Bunch length

  9. The 7th and 8th of November we have in Frascati an international workshop on Bunch Dynamics. We hope to have the scientific case at the end of the workshop. You are invited to collaborate You can find the relevant information for the workshop on the web: www.lnf.infn.it

  10. What else are we doing

  11. 1)LNFExperiments in other Laboratories • ATLAS @ CERN LHCb@CERN • DIRAC@ CERN EXPLORER@CERN • LVD @ LNGSOPERA @ LNGS • BABAR@SLACAIACE@TJNAF • CDF@FNALBTeV @ FNAL • HERMES@ DESYAccelerators @ DESY, SLAC,CERN • VIRGO @ Cascina • WIZARD @ Pamela

  12. 2) Use of the Synchrotron light lines 2) Synchrotron light facility much used by external users EU@SINBAD • June 2005 • 30 proposals • >70 users TARI1+I3

  13. 3)Beam Test Facility Electrons Positrons and Tagged Photons beams Control room • Flux: 11010 particles/pulse • Energy: 25750 MeV • Repetition rate 50 Hz • Pulse Duration 1 or 10 ns • p resolution: 1% • Spot size sx,y ≈ 2 mm

  14. Centro Nazionale di Adroterapia Oncologica 4)CNAO GSI RFQ+linac A proton synchrotron In the hospital of Pavia Scanning and monitoring stations

  15. LNF-AD participates to the Assembling Commissioning First running Technology transfer

  16. Delay Loop and transfer line final lay-out Transfer line: installed and commissioned. Delay Loop: installation spring-summer 2005, commissioning autumn 2005 D.Alesini, G.Benedetti, C.Biscari, R.Boni, M.Castellano, A.Clozza, A.Drago, D.Filippetto, A.Gallo, A.Ghigo (resp), F.Marcellini, C.Milardi, L.Pellegrino, B.Preger, M.A.Preger, R.Ricci, C.Sanelli, M.Serio, F.Sgamma, A.Stecchi, A.Stella, M.Zobov + Accelerator Division Technical Staff

  17. 5) At CERN CTF3 (CLIC Test Facility) Delay Loop, transfer line, combiner ring

  18. 6) FEL nei LNF Sorgente Pulsata Auto-amplificata Radiazione Coerente Self-Amplified Pulsed Coherent Radiation L.Palumbo

  19. synchronisation uncompressed pulse vacuum compressor acceleration chamber detectors area control & data LINAC UNDULATOR

  20. 6) High Intensity Laser Laboratory

  21. 7) Experimental setup for LWFA acceleration of externally injected electrons in a gas-jet plasma TeraWatt GigaVolt/m Frascati Laser for Acceleration and Multidisciplinary Experiments Approved: The construction is starting now

  22. Brilliance of X-ray radiation sources 8) SPARC-X 12.4 1.24 0.124 l (nm) FEL for X-rays Covering from the VUV to the 1 Å X-ray spectral range Approved SPARX

  23. RF gun Linac1: Low Energy section

  24. Etot ~ w 4 S-band : 1.5 GeV e-,1GeV e+ Now : Etot ~ 1.2 GeV Etot ~ w 4 X-band 2 GeV e- Linac2: High energy section dogleg start

  25. PROGRAM 2005 2006 2007 2008 2009 2010 KLOE END------------------------------------- FINUDA ---------------------------------------END-------------- SIDDARTHA ---------------------------------------END-------------- LHC -------------------------------------------------------------------------------- SPARC ---------------------------------------END SPARCX ---------------------------------------------------------------START------ FLAME ----------------------------------------START------------------------------ CTF3 ---------------------------END CNAO ----------------------------------------END BTF -------------------------------------------------------------------------------- SYNCH.LIGHT------------------------------------------------------------------------------- BABAR ----------------------------------------END CDF ----------------------------------------------------END HERMES ----------------------------------------------------END OPERA ---------------------------END---------------------------------------------- ILC -------------------------------------------------------------------------------

  26. What about the short range future ? • WE ARE THINKING ABOUT the possible • DAFNE UPGRADE in luminosity AND energy • To do what? • To complete the Kaon physics program • To measure the P, N, L time like form factors • To measure gg interactions below 2.4 GeV • To measure the total cross section • To continue the systematic studies of exotic heavy and light nuclei • To have the most advanced accelerator technology • To have an even more intense Synchrotron light source

  27. Starting point for the accelerator design DAFNE2 e+ e- collider Optimized to run on the F meson but able to go up in energy

  28. DAFNE2 SKETCH OF NEW LAYOUT Two rings One IR EXP Rf cavities wigglers DAFNE HALL

  29. accumulator • Injection system • upgrade • The proposed transfer lines pass in existing controlled area • Additional shielding needed in the area between the accumulator and DAFNE buildings new e- line BTF SPARCX new e+ line DAFNE2

  30. RF system Higher frequencies – lower acceptance Lower frequencies – higher voltage A possible candidate cavity 500 MHz SC cavity operating at KEKB R&D on SC cavities with SRFF experiment in DAFNE

  31. We can make use of the recent progress in SUPERCONDUCTING wiggler technology Operating experiences: CESRc, ELETTRA, CAMD Why wigglers are important? • To achieve the short damping times and ultra-low beam emittances needed in LC Damping Rings • To increase the wavelength and/or brightness of emitted radiation in synchrotron light sources • To increase radiation damping and control emittance in colliders R&D in progress: ILC, ATF, PETRA3, … E. Levichev

  32. Use of DAFNE2 as Synchrotron light source New scenarios

  33. CONCLUSIONS VERY ACTIVE Laboratory for the coming three-four years INFN will define the future of the Lab in the course of 2006

  34. Frascati National Labs (LNF)

  35. DAFNE the 16th of September Lpeak = 1.46 cm-2 sec-1 KLOE WILL STOP DAQ END 2005 With 2000 pbarn-1 integrated Integrated luminosity = 8.8 pbarn-1/day

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