prof. mario calvetti infn-lnf director university of...

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Report on LNF activities Prof. Mario Calvetti INFN-LNF director University of Florence e + e - Collider DAFNE (Super B) Free Electron Laser SPARC_X Advanced Accelerator Concepts PLASMONX Linear Colliders CLIC & ILC Hadron Therapy CNAO KLOE experiment Educational

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Page 1: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

QuickTime™ and aTIFF (Uncompressed) decompressor

are needed to see this picture.

Report on LNF activitiesProf. Mario Calvetti INFN-LNF director

University of Florence

•e+e- Collider DAFNE (Super B)

•Free Electron Laser SPARC_X

•Advanced Accelerator Concepts PLASMONX

•Linear Colliders CLIC & ILC

•Hadron Therapy CNAO

•KLOE experiment

•Educational

Page 2: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

DAFNE

DAFNE- LIGHTLaboratory

Two new soft X-ray lines under construction

Syncrotron ligth from DAFNESPARCSPARX

Conventional sources

LNF are part of the European Infrastructurefor syncrotron light

Page 3: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

•In 2007 the DAΦNE accelerator complex has been upgraded. •Large Piwinski angle, low–β and Crab-Waist compensation of the synchrobetatron resonances

•Since May 2008 DAΦNE has been delivering luminosity to the SIDDHARTA experiment.

High Luminosity at DAΦNE

(Courtesy of Catia Milardi)

Page 4: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

KLOE experiment

Page 5: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date
Page 6: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date
Page 7: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date
Page 8: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

0

1 1032

2 1032

3 1032

4 1032

5 1032

0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6

L CW SXT. OFF Feb. 9th 2009

L March 13th 2009

Lum

inos

ity [

cm-2

s-1

]

I+ * I- [A2]

Lpeak at DAΦNE 2001 ÷2009

Expected L∫day = 20 pb-1

L versus Crab-Waist compensation

(Courtesy of Catia Milardi)

DAΦNE Luminosity measurements

Page 9: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

S-band Gun

Velocity Bunching

Long Solenoid

s

Diagnostic and

Matching

Seeding

THz Source

150 MeVS-band linac

12 mUndulator

s

λu = 2.8 cm

Kmax = 2.2

λr = 500 nm

15 mQuickTime™ and a

decompressorare needed to see this picture.

Page 10: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date
Page 11: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date
Page 12: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

240 fs

Electron Pulse Length versus injection phase

VELOCITY BUNCHING

Page 13: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

Free Electron Laser ranging from 40 nm a 0.5 nm4 different Beamlines with dedicated experimental stationsPeak Brillance: 1027 sec.mrad².mm.0.1 % BW – 80-200 fs pulsesSito choice: Università di Roma Tor VergataCostruction of the 500 m tunnel: 2010 - 2014

Applications:•Time-resolved X-ray techniques

•Coherent x-ray imaging •Photon hungry measurements

•Spectromicroscopy•Structural studies of biological systems, allowing

crystallographic studies on biological macromolecules

www.sparx-fel.eu

Page 14: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

2008-2013

A new Project : X-FEL SPARX

The TDR is ready

Page 15: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

Brilliance of X-rayradiation sources

New FEL Covering from the VUV tothe 1 Å X-ray spectral range:

new Research Frontiers

SPARX

TTF

12.4 1.24 0.124 λ (nm)

L.Palumbo

A NEW PROJECTan X-FEL at TORVERGATA

Approuved and funded : 2007-2011

Page 16: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

S-band Gun

Velocity Bunching

Long Solenoid

s

Diagnostic and

Matching

150 MeVS-band linac

12 mUndulator

s

λu = 2.8 cm

Kmax = 2.2

λr = 500 nm

15 mQuickTime™ and a

decompressorare needed to see this picture.

50 fs, 800 nm , 300 TW @10 Hz

Page 17: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

Tuneable X-ray radiation source based on Thomson Scattering

X ray pulses : 101099 photonsphotons/s/s, 3 ps, 20 20 keVkeV -- 1 1 MeVMeV

Page 18: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

LWFA acceleration of externally injected electrons in a gas-jet plasma

300 TW 25 fs 0.8 μ laser

VERY HIGH POWER INFRARED LASER

Page 19: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

μs

4

24

INFN Contribution in CLIC Test Facility:Beam recombination system

100 MV/m

Page 20: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

DLTL1

CRM

CR

TL2CLEX

Measured currents in CTF3: [28A in CR]

Page 21: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

LNF activity is focused on ILC damping rings

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

Documented in Reference Design Report (RDR), Beijing February 2007

• 5 Gev damping rings for e+ and e- in a shared tunnel• Circumference 6.4 km• Number of bunches 2700 - 5400• extremely low emittance values

– εx = 0.6 nm– εy = 2 pm (minimum ever achieved)

• Short damping time τx = 21 ms• Wigglers needed: total length ~ 200 m, peak field 1.6 T

Page 22: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

Damping Rings LNF Activity• Fast kickers R&D

– kickers with ultra short rise/fall time (< 3 (6) ns for 3 (6) ns bunch distance) are one of the most critical issues since the bunch distance and ring circumference are related to kicker pulse duration

• Electron cloud studies at DAFNE– Comparison between measurements and simulation– Test of mitigation techniques

• Design of low impedance bellows• Beam dynamics in wiggler magnets• Low emittance lattice design

Accelerator Physics and Technology

Page 23: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date
Page 24: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

250 Mev protons

400 MeV/u Carbon

Page 25: Prof. Mario Calvetti INFN-LNF director University of …theor.jinr.ru/meetings/2009/rt/talks/Calvetti.pdfMicrosoft PowerPoint - Calvetti Mario1-DUBNA_09.ppt Author kea Created Date

CONCLUSION:

Accelerator physics and technologyFEL physics and technologyFlavour physics and the KLOE experimentSpace physics (future experiment in space)High density nuclear matter (ALICE)Detector technologySynchrotron light form DAFNE

Frascati school of physics

….we could set up a DUBNA-LNF working group….“light, fast and efficient”

“……….thank you”