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LNF-INFNFrascati
BTFBTF
Peak luminosity evolution in 2004-5
Luminosity is what matter…in our case
L = 1.46 1032 cm-2s-1 (to day)
…..and the physics….KLOEFINUDALUCE DI SINCROTRONEFISICA di MACCHINA-SRFFFASCI ESTRATTI
KLOE – (K LOng Exp.)
DAFNE e+e- KK is a source of monochromatic correlated low energy Kaons
FINUDA Kaons absorbed by nuclei
Sistematic study of exotic nuclei
DAFNE experiments
KLOE is running his year
KLOE
FINUDAexoticnuclei
SIDDHARTAKaonicatoms
SRFF ?
TODAY 2006 2007 2008
The program is well defined for the coming three years
FINUDAexoticnuclei
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 radiative decays eta decays KO-KObar interference
1) Collect 2 fbarn-1 on resonance – end of the current year
2) Scan over the resonance 50 pbarn-1
3) 250 pbarn-1 at 1000MeV , below the , 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
SC 1.3 GHz cavity
Experimental studies on short-bunches and bunch-length modulation at DANE
SRFF = Superconductive RadioFrequency FocusingEXPERIMENT
Longitudinal phase space
RF input
RF center
RF output
IP
Bunch length
Energyspread
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
What else are we doing
1)LNF Experiments in other Laboratories
ATLAS @ CERN LHCb @CERN
DIRAC @ CERN EXPLORER@CERN
LVD @ LNGS OPERA @ LNGS
BABAR @ SLAC AIACE @ TJNAF
CDF @ FNAL BTeV @ FNAL
HERMES @ DESY Accelerators @ DESY, SLAC,CERN
VIRGO @ Cascina
WIZARD @ Pamela
June 2005
30 proposals >70 users
June 2005
30 proposals >70 users
TARI1+I3
EU@SINBADEU@SINBAD
2) Use of the Synchrotron light lines2) Synchrotron light facility much used by external users
Control room
§ Flux: 1Flux: 1101010 10 particles/pulse particles/pulse
§ Energy: 25Energy: 25750 MeV750 MeV
§ Repetition rate Repetition rate 50 Hz 50 Hz
§ Pulse Duration Pulse Duration 1 or 10 1 or 10 nsns
§ p resolution: 1%p resolution: 1%
§ Spot sizeSpot size x,yx,y ≈ 2 mm ≈ 2 mm
ElectronsPositrons and
Tagged Photons beams
3)Beam Test Facility
4)CNAO
GSI RFQ+linac
Scanning and monitoring stations
Centro Nazionale di Adroterapia Oncologica
A proton synchrotronIn the hospital of Pavia
fast slow
horizontalscanning
verticalscanning
Energy variationfrom the
synchrotron
Totalthickness
Patient
Scanning system
Target volume
Field 22E22
Field 4E4
LNF-AD participates to the
AssemblingCommissioning
First runningTechnology transfer
Delay Loop and transfer linefinal 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
C L I CC L I C
151/24/01R. Corsini - CTF3 Meeting
CTF3 conceptual lay-outCTF3 conceptual lay-out
X 5 Combiner Ring
84 m
X 2Delay42 m
Drive Beam Injector
Main Beam Injector
30 GHz - 150 MV/m - 140 ns
Drive/Main Beam Modules
10 Modulators/Klystrons with LIPS (x 2.3) 3 GHz - 30 MW - 6.7 s
Drive Beam Accelerator 20 Accelerating Structures 3 GHz -7.0 MV/m - 1.3 m
~ 15 m 3.5 A - 2100 b of 2.33 nC 184 MeV - 1.4 s
35 A - 184 MeV140 ns
High PowerTest Stand
CTF3 - Test of Drive Beam Generation, Acceleration & RF Multiplication by a factor 10
5) At CERN CTF3 (CLIC Test Facility) Delay Loop, transfer line, combiner ring
SS orgenteorgente
PP ulsataulsata
AA uto-amplificatauto-amplificata
RR adiazioneadiazione
CC oerenteoerente
Self-Amplified Pulsed Coherent RadiationSelf-Amplified Pulsed Coherent Radiation
6) FEL nei LNF
L.Palumbo
LINAC
UNDULATOR
synchronisation
uncompressed pulse
vacuum compressor
acceleration chamber
detectorsarea
control& data
6) High Intensity Laser Laboratory
7) Experimental setup for LWFA acceleration of externally injected electrons in a gas-jet plasma
TeraWattGigaVolt/m
FrascatiLaser forAcceleration andMultidisciplinaryExperiments
Approved: The construction is starting now
FEL for X-raysCovering from the VUV
to the 1 Å X-ray spectral range
Approved
12.4 1.24 0.124 (nm)
Brilliance of X-ray radiation sourcesBrilliance of X-ray radiation sources
SPARX
8) SPARC-X
Linac1: Low Energy section
RFgun
Linac2: High energy section
Now : Etot ~ 1.2 GeV
dogleg start
Etot ~ w 4 S-band :
1.5 GeV e-, 1GeV e+Etot ~ w 4 X-band 2 GeV e-
PROGRAM 2005 2006 2007 2008 2009 2010
KLOE END-------------------------------------FINUDA ---------------------------------------END--------------SIDDARTHA ---------------------------------------END--------------LHC --------------------------------------------------------------------------------SPARC ---------------------------------------ENDSPARCX ---------------------------------------------------------------START------FLAME ----------------------------------------START------------------------------CTF3 ---------------------------ENDCNAO ----------------------------------------ENDBTF --------------------------------------------------------------------------------SYNCH.LIGHT-------------------------------------------------------------------------------BABAR ----------------------------------------ENDCDF ----------------------------------------------------ENDHERMES ----------------------------------------------------ENDOPERA ---------------------------END----------------------------------------------ILC -------------------------------------------------------------------------------
What about the short range future ?
WE ARE THINKING ABOUT the possible DAFNE UPGRADE in luminosity AND energy
To do what?
1) To complete the Kaon physics program2) To measure the P, N, time like form factors3) To measure interactions below 2.4 GeV4) To measure the total cross section5) To continue the systematic studies of exotic heavy
and light nuclei6) To have the most advanced accelerator technology 7) To have an even more intense Synchrotron light
source
Starting point for the accelerator design
Total Energy (GeV) 1.02 2.4
Integrated Luminosity per year (ftbarn-1) 8
Total integrated luminosity 20 3
Peak luminosity > (cm-1sec-2) 8 1032 1032
DAFNE2 e+ e- collider
Optimized to run on the meson but able to go up in energy
Two rings
One IR
SKETCH OF NEW LAYOUT
DAFNE HALL
EXP
Rf cavitieswigglers
DAFNE2
Injection systemupgrade
• The proposed
transfer lines pass
in existing
controlled area
• Additional
shielding needed
in the area
between the
accumulator and
DAFNE buildings
new e- line
new e+ line
accumulator
BTF
DAFNE2
SPARCX
RF system
A possible candidate cavity
500 MHz SC cavity operating at KEKB
Higher frequencies – lower acceptanceLower frequencies – higher voltage
R&D on SC cavities with SRFF experiment in DAFNE
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
E. Levichev
We can make use of the recent progress in SUPERCONDUCTING wiggler technology
Operating experiences:CESRc, ELETTRA, CAMD
R&D in progress:ILC, ATF, PETRA3, …
Use of DAFNE2 as Synchrotron light source
Beam Energy (GeV)
0.51 1.2
Beam Current (A)
2.5 0.5
B dipoles field (T)
0.77 1.8
B wigglers field (T)
4. 4.
New scenarios
CONCLUSIONS
VERY ACTIVE Laboratory for the coming three-four years
INFN will define the future of the Lab in the course of 2006
Frascati National Labs (LNF)
Lab footprint
135000 m2
Total Staff
368
Researchers
98
Technologist/
Engineers62
Technicians
167
Administration/ Services
41
External Users 323
Italian 252
Foreigners71
Visitors3200
Stages170
N-NEnergy per beam E GeV 0.51 1.2
Circumference C m 100 100
Luminosity L cm-2 sec-1 8 1032 1032
Current per beam I A 2.5 0.5
N of bunches Nb 150 30
Particles per bunch N 1010 3.1 3.4
Emittance mm mrad 0.3 0.6
Horizontal beta* x m 1 1
Vertical beta* y cm 1 2
Bunch length L cm 1 2
Coupling % 1 1
Energy lost per turn Uo (keV) 25 189
H damping time x (msec) 13 5
Beam Power Pw (kW) 62 (55w + 7d) 94.6 (42w + 53d)
Power per meter Pw/m (kW/m) 8.6w + 0.5d 8.4w + 3.8d
DANE the 16th of September
Lpeak = 1.46 cm-2 sec-1
Integrated luminosity = 8.8 pbarn-1/day
KLOE WILL STOP DAQ END 2005With 2000 pbarn-1 integrated