SuperB and SuperKEKB * Y. Ohnishi KEK July 3, 2008 * SuperKEKB is the KEKB upgrade in the framework...
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Transcript of SuperB and SuperKEKB * Y. Ohnishi KEK July 3, 2008 * SuperKEKB is the KEKB upgrade in the framework...
![Page 1: SuperB and SuperKEKB * Y. Ohnishi KEK July 3, 2008 * SuperKEKB is the KEKB upgrade in the framework of the KEK roadmap 1.](https://reader036.fdocuments.net/reader036/viewer/2022062713/56649cf45503460f949c27ee/html5/thumbnails/1.jpg)
SuperB and SuperKEKB*
Y. OhnishiKEK
July 3, 2008
* SuperKEKB is the KEKB upgrade in the framework of the KEK roadmap
1
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Collaboration of INFN-KEK
• SuperB (INFN Super B(Flavor)-Factory)– Beam-beam issues (simulation work) – Lattice issues (dynamic aperture, IR design)– Coherent synchrotron radiation(CSR) calculations
• Crab waist study at DANE– Commissioning of machine– Beam-beam issues (simulation work)– Optics calculations (dynamic aperture)– (Electron-cloud issues)
2
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SuperB Accelerator CDR Contributors
• M. E. Biagini, M. Boscolo, A. Drago, S. Guiducci, M. Preger, P. Raimondi, S. Tomassini, C. Vaccarezza, M. Zobov (INFN/LNF, Italy)
• Y. Cai, A. Fisher, S. Heifets, A. Novokhatski, M.T. Pivi, J. Seeman, M. Sullivan, U. Wienands (SLAC, US)
• T. Agoh, K. Ohmi, Y. Ohnishi (KEK, Japan)
• I. Koop, S. Nikitin, E. Levichev, P. Piminov, D. Shatilov (BINP, Russia)
• A. Wolski (Liverpool University, UK)
• M. Venturini (LBNL, US)
• S. Bettoni (CERN, Switzerland)
• A. Variola (LAL/Orsay, France)
• E. Paoloni, G. Marchiori (Pisa University, Italy)
from M. Biagini, SuperB 2008 meeting 3
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Comparison of Machine Parameterssymbol SuperB SuperKEKB unit
E 4.0 7.0 3.5 8.0 GeV
C 1.8 3.02 km
I 1.85 1.85 9.4 4.1 A
nb 1251 5018
N/bunch 5.5 11.8 5.1 x1010
x 2.8 1.6 12 nm
y/x 0.4 0.5 %
x* 35 20 200 mm
y* 0.22 0.39 3 mm
z 5 3 mm
x* 48 30 to 0 mrad
x 0.0043 0.0025 0.27
y 0.15 0.30
RF Power 17 64 MW
L 10 5.5 x1035 cm-2s-14
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Two Approaches
5
€
L∝1
εxβ x*εyβ y
*
€
L∝N+N−nbεxβ x
*εyβ y*
€
x →εx10
εy →εy10
β x*→
β x*
10
β y*→
β y*
10€
L→100× L
→1.6 ×1036
(L =1.6 ×1034 )
€
N+N−nb →5.8 ×N+N−nb
εx →εx2
εy →εy2
β x*→
β x*
4
β y*→
β y*
2
€
z →σ z
€
z →σ z2
(hourglass)€
L→32× L
→5×1036
(L =1.6 ×1034 )
(crab waist)
(crab crossing)€
x,y = εx,yβ x,y
SuperBSuperB SuperKEKBSuperKEKB
with keeping N+N-nb
Beamcurrents
Attractive ! and are reachable !
Huge power consumption.
HOM/CSR
No evident for tiny and .
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Issues for SuperB• Ultra-low emittance
– 10 times smaller than the present KEKB– Small machine errors and good control of beam orbits– How to handle Bunch-by-Bunch feedback system ?
• Ultra-low beta at IP– 10 times smaller than the present KEKB– Short focal length generates a large chromatic effect– In order to compensate this, strong sextupoles are needed.– Strong sextupoles reduce dynamic aperture....short lifetime.
• Crab waist scheme– Dynamic aperture (Touscheck lifetime/injection or BG)
• Dynamic aperture deteriorates to be about half if the crab waist scheme is applied to the KEKB lattice (results from simulations).
6
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Issues for SuperB (cont’d)• Polarization of electron beam
– longitudinal polarization ~80 %.– Need polarized rf gun in linac injector.– Extremely strong spin rotators and/or geometrical
matching are needed. Are there any realistic solutions ?• Flavor factory
– Energy should go down for tau-charm physics.– Quality of magnetic field for bends, quads ?– XY-coupling is designed for a fixed energy in general.
XY-coupling should be zero at IP. Machine tuning becomes very difficult unless a detector solenoid changes proportonl to the energy.
7
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SPARX 1st stage SuperB LINAC SPARX future
SuperB footprint on Tor Vergata siteSuperB footprint on Tor Vergata site
600 m
500 m
S. Tomassini’s talk, Monday
New tunnel !New linac injector !New infrastructures !
cooling systemAC power station
New buildings formany power supplies,klystrons!
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Issues for SuperKEKB• Ultra-high currents
– a factor of 5 larger than the present KEKB– Strong synchrtron radiation– HOM heating– Can a bunch-by-bunch feedback system work ?– Electron-cloud in a positron ring ?
• Large beam-beam tune shift– a factor of 3 larger than the resent KEKB– Beam size in the vicinity of IP becomes large due to
dynamic emittance and dynamic beta.– Difficulties in the IR design. Physical aperture and
syncrtron radiation from IR magnets affect detector backgrounds.
9
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Issues for SuperKEKB• Short bunch length
– half of the present KEKB– HOM heating– CSR instabilities
• Smaller beam pipe can suppress CSR. Down from 96 to 50.• 4 mm bunch length can suppress CSR. Luminosity deteriorates
by 16%.• Crab crossing scheme
– Development of crab cavities for the ultra-high current • LER: 9.4 A
– Is large beam-beam tune shift feasible ?• y ~ 0.2-0.3
• No polarization scheme 10
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11
KEKB on KEK SiteKEKB on KEK Site
Mt. Tsukuba
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Question ?
12
ILC Damping Ring + ILC FF = SuperB ?ILC Damping Ring + ILC FF = SuperB ?
ILC Damping Ring realizes small emittance,however NO IP and NO BEAM-BEAM !
ILC FF realizes small beta at IP,however colliding beams are SINGLE-PASS !
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IR design for SuperB and SuperKEKB
13
HER 7 GeV HER 8 GeV
LER 3.5 GeVLER 4 GeV
?
LER 4 GeV
?
No detector solenoidNo compensation solenoid
Symmetric layoutalthough asymmetric collider !
SuperBSuperB SuperKEKBSuperKEKB
Bz
(T)
Bz
(T) 1.5 T
e- e-
e+B
eta
Bet
a
Bet
a
Bz
(T)
These are not latest version.
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Crab waist study at DANE• 2 people from KEKB visited DANE and joined
commissioning in March 2008.
• We have a plan to send one or two people from KEKB for Autumn run to study the crab waist.
• We are very interested in a specific luminosity as a function of bunch current products between the crab sextupoles ON and OFF.– Both simulations and experimental data 14
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SIDDHARTA
K monitor
Bhabha calorimeter
monitor
IP LAYOUT AND LUMINOSITY MONITORS
GEM Bhabha Monitor
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SIDDHARTA K monitor
Bhabha calorimeter
monitor
IP LAYOUT AND LUMINOSITY MONITORS
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CRAB SEXTUPOLES WORK !!
e- sextupoles off
e- sextupoles on
Transverse beam sizes at Synchrotron Light Monitors
LUMINOMETERS
Sextupoles can change beta, XY-coupling, dispersion, namely beam size at IP. Quantitative evaluation ?Sextupoles can change beta, XY-coupling, dispersion, namely beam size at IP. Quantitative evaluation ?
from P. Raimondi
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DANE Machine Parameters
18
KLOEAchieved
SiddhartaDesign
Siddharta Achieved
Ib 13 13 12 mA
nb 110 110 95
x 340 200 250 nm
y/x 0.2-0.3 0.5 0.7 %
x* 170 20 24 cm
y* 1.7 0.65 0.96 cm
z 25 20 18 mm
x/2 12.5 25 25 mrad
x 0.04 0.008 0.009
y 0.04 0.055 0023
L 1.5 > 5 2.6 x1032 cm-2s-1
Specific luminosity is still lower than the target for the crab waist.Specific luminosity is still lower than the target for the crab waist.
Smaller betathan KLOE !
Eb = 500 MeVC ~ 100 m
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Conclusions• INFN SuperB is very attractive.
– Smaller currents can get larger luminosity (above 1036).– a future generation for factory machine...Need more study.
• We keep the present design concept for the KEKB upgrade unless we obtain a good result of the crab waist at DANE.
• The KEKB upgrade is a natual extension of the present KEKB. We do not have to build the collider in a whole-new way.
• We have many resources and experiences for the high current scheme. We have studied the design of SuperKEKB since 2001 and already published LoI 2004 (corresponds to SuperB CDR).
19
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20
5 years A. Suzuki
SuperKEKB fits in with KEK roadmap !
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Backup Slides
21
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Geometric luminosity gain
low vertical tune shift
Geometric luminosity gain
Very low horizontal tune shift
No parasitic collisions
short overlap region
Crab waist transformation(realized with two sextupoles@ in x and 1.5 in y from IP)
Geometric luminosity gain
Suppression of X-Y betatron and synchrobetatron resonances
Large Piwinski angle P=z / x
small y* (y* x /)
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DANE
(KLOE run)
DANE Upgrade
Ibunch (mA) 13 13
Nbunch 110 110
y* (cm) 1.7 0.65
x* (cm) 170 20
y* (m) 7 2.6
x* (m) 700 200
z (mm) 25 20
Horizontal tune shift 0.04 0.008
Vertical tune shift 0.04 0.055
cross (mrad) (half) 12.5 25
Piwinski 0.45 2.5
L (cm-2s-1) 1.5x1032 >5x1032
DANE (KLOE run)
DANE Upgrade
BEAM PROFILES @IP AND NEW PARAMETERS
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Old layout
New layout
splitters removed
new vacuum chambers @ IP
Bending angles changed, new independent power supplies
Crab sextupoles
XX
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• Aluminum
•Window thickness 0.3 mm
IP
5.5cm
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Time schedule is restricted.
Baseline is “HIGH current scheme”.
Alternative is low beta+low emittance+crab waist scheme
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Luminosity upgradeLuminosity gain and upgrade items (preliminary)
Item Gain Purpose
beam pipe x 1.5high current, short bunch, electron cloud
IR(*x/y=20 cm/ 3mm) x 1.5 small beam size at IP
low emittance(12 nm) x → 0.5
x 1.3mitigate nonlinear effects with beam-beam
crab crossing x 2mitigate nonlinear effects with beam-beam
RF/infrastructure x 3 high current
DR/e+ source x 1.5low * injection, improve e+ injection
charge switch x ? electron cloud, lower e+ current
3 ye
ars
shut
dow
n
27
KEK
road
map
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operation time : 240 days/year
Target forroadmap
Target forroadmap
Inte
grat
e lu
min
osity
(a
b-1)
Peak
lum
inos
ity (c
m-2
s-1)
Year
3 yearsshutdown
DampingRing
RF upgrade
KEKroadmap
Peak
cur
rent
(A)
KEK roadmap includes RF/DR (after 3 years shutdown)
Projected Luminosity (preliminary)
28
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SuperKEKBIbunch (LER) = 1.87 mAIbunch (HER) = 0.82 mA
Specific luminosity with crab crossing
Beam-beamsimulation(strong-strong)
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Specific Luminosity
Crab crossing•49-sp x*=80, 84cm x=18, 24 nm•3.5-sp x*=80cm•3.06-sp x*=80cm•3.06-sp x*=90cm
22 mrad crossing
y=-16.35x+26.54 Green Ratio=100%
Green line
y~0.093 (HER) (4/3)
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31
x* = 0.8m
x* = 1.5m
= 1%
x* = 1.5m
= 1.3%
w/o crabx
* = 0.8m
Machine studyx
* = 1.5m