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Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

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Page 1: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Status on SuperB effort

Daresbury, April 26, 2006

P. Raimondi

Page 2: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Outline

• Basic Concepts (March-Sept,2005)• Parameters and layout optimization based on a

High-Disrupted regime (Nov, 2005)• Parameters and layout optimization for a

Minimal-Disrupted regime (Jan, 2006)• Layout for a Ring Collider with Linear Collider

Parameters (Mar, 2006)• Conclusions

Page 3: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Basic concepts• SuperB factories based on extrapolationg

current machines require:

• Higher currents

• Smaller damping time (weak function ^1/3)

• Shorter bunches

• Higher power

SuperB gets very expensive and hard tomanage, expecially all the problems relatedto the high current => look for alternatives

Page 4: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

• Basic Idea comes from the ATF2-FF experiment

In the proposed experiment it seems possible to acheive spot sizes at the focal point of about 2m*20nm at very low energy (1 GeV), out from the damping ring

• Rescaling at about 10GeV/CM we should get sizes of about 1m*10nm =>

• Is it worth to explore the potential of a Collider based on a scheme similar to the Linear Collider one

Idea presented at the Hawaii workshop on Super-B factory on March-2005

Page 5: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

LinearB scheme

IPLER Bunch compressor and FF

HER Bunch compressor and FF

LERHER

Overall rings lenght about 6Km,Collision frequency about 120Hz*10000bunch_trains=1.200MHzBunch train stays in the rings for 8.3msec, then is extracted, compressed and focused. After the collision is reinjected in its ring

LER injection Her injection

Page 6: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Scaling laws to optimize the IP parameters

• Disruption:

• Luminosity

• Energy spread:

yx

NL

2

yx

zN

D

zx

E

N

2

2

Decrease z + decrease NIncrease spotsize

Increase NDecrease spotsize

Increase z + decrease NIncrease spotsize

Contraddicting requests!

Page 7: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

A lot of homework done in collaboration at SLAC and at the LNF for a few months.

Explored the parameters phase in order to maximize the luminosity per crossing

Laid down all the other possible advantages (e.g. less current through the detector, smaller beams, smaller beam pipe etc)

Leading to a workshop held on Nov,11-12 2005 in Frascati to investigate and optimize the scheme and the feasibility of the different subsystems

Page 8: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Horizontal Collision Vertical collision

Effective horizontal size during collision about 10 times smaller, vertical size 10 times larger

Simulation by D.SchulteFirst attempt

Page 9: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Horizontal phase after the collision

Vertical phase after the collision

IP Parameters set considered at the workshop causedlarge increase of the emittance due to the collision:

x_out/x_in=12 y_out/y_in=300M. Biagini studies

Page 10: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Linear Super B schemes with accelerationand energy recovery, to reduce power

e- Gun2GeVe+ DR IP

5GeV e+ SC Linac

e- Dump7GeV e+

4 GeV e-

4GeV e- SC Linac

2 GeV e+ injection

2 GeV Linac1.5 GeV Linac 1.5 GeV Linac

Linac

Damping Rings2 GeV

Linac

e+ Gun e- Gun

• Use SC linacs to recover energy• Use lower energy damping rings to

reduce synchrotron radiation• No electron damping ring• Make electrons fresh every cycle

– Damping time means time to radiate all energy

– Why not make a fresh beam if storage time is greater than 1 damping time

Page 11: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Progress in design optimization after the 1° SuperB workshop

Between December-2005 and March-2006 a lot of studies have been made in order to understand what are the sources of the blow-ups in the collision and how to minimize then.

Power requirements could be greatly reduced if collision is less disruptive

Search for a trade off between luminosity delivered in one collision and power spent for each collision

Search for the simplest and more economic solution

Page 12: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

x=10m y=10nm z=250um

x=33mm y=1mm

x=3.3*10-9 y=10-13

Lnorm=Ld/log(y_out/y_in)=2.27 at Npart=2.5*1010

Introduced the luminosity merit function: Lnorm=L/log(ey_out/ey_in) => Luminosity per energy cost

Luminosity vs bunch charge for a given set of IP parameters

Outgoing/incoming emittances ratiovs bunch charge for a given set of IP parameters

Page 13: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Ey_after collision increases fast with current and 1/x: with Npart=2*10^10 Lnorm=2.27

Cure 1: decrease y from 1mm to 250um =>

y_in=4*10-13 y_out=23.4*10-13 y_out/y_in=6 instead of 24 Ld drops from 7.22*1032 to 5.6*1032 (hourglass) Lnorm=3.12 Cure 2: travelling focus (waist position is shifted by z wrt

the IP for the slice ‘z-z+dz’=> Ld goes back up to 7.01*1032 Lnorm=3.91

Cure 3: further decrease y from 250um to 100um and use the pinch to keep the beams from diverging rather than to disrupt them with overfocusing=>

BB FOCUS COMPENSATION CONCEPT !!!!!!!!!

y_in=10*10-13 , y_out(slice)=15.0*10-13,

y_out/y_in=1.5 instead of the initial 24 Ld drops to 5.77*1032 Lnorm=14.1 !!

Page 14: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

With travel focus

Without travel focus

Horizontal collisions in a round beam case

Page 15: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

3 planes slice emittances after the collision (round beams case), each color is a different slice: red head of the bunch, black tail

Without Travel Focus

y_out/y_in=3

With Travel Focus

y_out/y_in=1.1

Page 16: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

In summary, the small disruption regime requires:

small z (=> large e from compressor)

big x

small y (for luminosity) and y

BB-compensation by traveling focus all the requirements do fit togheter with the horizontal monocromator:

betatron x small, and made large by adding horizontal dispersion with opposite sign for the 2 beams. High energy particles of first beam collide with low energy particles of the sencond one

it simultaneneously enlarge x and decrease the luminosity energy spread moreover since the natural horizontal emittance is small,

the emittance ratio of about 0.5% ensures the small y

Page 17: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Single pass Collider

Ring with compressor

Ring without compressor

Sigx* m 30 (2 betatron) 18 (2 betatron) 2.67Etax mm +-1.5 +-5.0 0.0Sigy nm 12.6 63.2 12.6Betx mm 5.0 5.0 9.0Bety mm 0.080 0.500 0.080Sigz_IP mm 0.100 0.600 6.0Sige_IP 2.0e-2 3.5e-3 1.3e-3Sige_Lum 1.0e-3 1.0e-3 0.9e-3Emix nm

0.8 0.8 0.8

Emiy nm

0.002 0.008 0.002

Emiz m 2.0 2.0 8.0Cross_angle mrad Optional >2*12 2*25Sigz_DR mm 4.0 4.0 6.0Sige_DR 0.5e-3 0.5e-3 1.3e-3Np 10e10 7.0 2.0 2.3Nbunches 12000 12000 12000DR_length km 6.0 6.0 6.0Damping_time msec 20 20 20Nturns_betwe_coll 50 1 1Collision freq MHz 12.0 600 600Lsingleturn 1e36 1.5 1.7 1.2Lmultiturn 1e36 1.1 0.9 1.0

Page 18: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Single pass Collider with Np=7*1010

Nbunches=12000 (6Km ring)

Travel focus in vertical plane

x=1.5mm (opposite sign for the two beams), x*=30m

z=100m z=4mm in DR

e=100MeV e/e=2*10-2 e/e=5*10-4 in DR

e_Luminosity=7MeV

x=0.8nm x_norm=8m

y=0.002nm y_norm=20pm

z=2.0m Stored time between collision=1msec=50turns

Lmultiturn=0.9*1036 (Lsingleturn=1.5*1036)

FF with large energy spread tricky

Page 19: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Multiturn Simulation for flat case6Km ring,Np= 7*1010

coll_freq=1Khz*12000 Lmultiturn=0.9*1036

Page 20: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Compressor

Compressor Decompressor

DeCompressor

IP

OptionalAccelerationand deceleration

OptionalAccelerationand deceleration

FF FF

ILC ring with ILC FFILC compressorColliding every 50 turnAcceleration optionalCrossing angle optional

Now the acceleration is not needed anymore in order to reduce the power

Simplified layout in the Small Disruption Regime

Page 21: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

• Equilibrium Emittance Vertical blowup about 60%• Blowup as function of beam currents almost linear• Blowup as function of damping time goes like Tau1/3

• Reducing the bunch charge by a factor 6 (1010), the blowup at the equilibrium decreases to 10%

• Reducing the damping by a factor 50 (collision every turn) equilibrium blowup increases by a factor 4 (501/3)

• Final Blowup in this case is about 40%• Geometric Luminosity decreases by a factor 36 due to

less charge and increases by a factor 50 for increased collision rate

• With the same parameters but colliding in the ring (bunch compressor and FF in the ring), we get:

L=1036 with Npart=1010 and L=4*1036 with N=2*1010 => overhead in luminosity

Possible to reoptimize the parameters in this scenario

Scaling the parameters to a Ring Colliding Machine

Page 22: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Ring Collider Compressed Bunches

With proper tunes choice (.503, .55) the BB compensation with travel focus is not needed

e=16MeV e/e=3.5*10-3 e_Luminosity=10MeV

x=0.8nm y=0.008nm z=2.0m

Lmultiturn=0.84*1036 (Lsingleturn=1.7*1036) with Npart=2*1010

FF with large energy spread tricky

Bunch compressor (z 4mm=>0.6mm) in the ring tricky:

150MeV 1.3GHz

Page 23: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Betx_dyn=3.0mmsigx_dyn=2umsigxp_dyn=0.7mradEmix_dyn=1.5nmEtax_dyn=+-5mmSigx_eta=18umSigz_dyn=0.57mmSige_dyn=5*10-3Bety_dyn=0.5mmSigy_dyn=93.0nmSigyp_dyn=0.2mradEmiy_dyn=0.020nm

Betx=5.0mmsigx=2umsigxp=0.4mradEmix=0.8nmEtax=+-5mmSigx_eta=18umSigz=0.6mmSige=3.5*10-3Bety=0.5mmSigy=63.2nmSigyp=0.11mradEmiy=0.008nm

L0=1.7*10^36, Ldyn=0.84*10^36, sige_lum=11MeV

Npart=2*10^10, fcoll=600MHz

Page 24: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Compressor Compressor

Decompressor Decompressor

IPFF FF

ILC ring with ILC FFILC Compressor, 0.4GeV S-Band or 1GeV L-BandCrossing angle optional

Simplified layout in the Small Disruption Regime Collisions every Turn

Page 25: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Do we need to compress the bunches?

Sz

Sx

Both cases have the same luminosity,(2) has longer bunch and smaller x

1) Standardshort bunches

2) Crossing angle

Overlapping region

Sx

Sz

Overlapping region

Page 26: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Colliding every turn very promising but requires a bunch compressors and a decompressor in the ring

In principle not needed to compress the beams if we collide with a crossing angle such as:

z*xcross=24m (same projected horizontal size)

x/xcross=100m (same effective longitudinal interaction region)

y=12.6nm, y=80um like in the compressed case These parameters gives the same geometric luminosity like the

compressed case:

If z=4mm we need:

x_cross=6mrad, x=0.6um However now beam-beam worsened because the beams

see each other also at non-minimum betay locations

Scaling the parameters for an every-turn colliding machine, with Uncompressed Bunches

Page 27: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

With large crossing angle X and Z quanties are swapped Very important!!!

Sz

Sx

z

x

Sx/

Sz*

e-e+

Page 28: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Easy way to decrease the ‘Long Range Beam Beam’ is to increase the crossing angle by a factor 4 at a direct luminosity cost of a factor 4:

xcrossing_angle=2*24mrad x=2.4m This still gives a luminosity of 1.2*1036 with

N=2*1010 if the vertical blowup were none

Unfortunately the blowup is still large and y at the equilibrium is about 6 times larger:

Lmutiturn=0.4*1036

Overall a factor 10 loss in luminosity w.r.t. full compressed bunches (with all the other parameters the same)

Page 29: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Second way to decrease the ‘Long Range Beam Beam’ is to apply the travel focus idea, but now has to be applied in the transverse plane since x and z are swapped.

Vertical waist position in z is a function of x: Zy_waist(x)=x/2Crabbed waist All components of the beam collide at a

minimum y => - the ‘hour glass’ is reduced - the geometric luminosity is higher - the bb effects are reduced

y blowup at the equilibrium less than a factor 2

Page 30: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Vertical waist has to be a function of x:

Z=0 for particles at –x (- x/2 at low current)

Z= x/ for particles at + x (x/2 at low current)

2Sz

2Sx

z

x

2Sx/

2Sz*

e-e+Y

Page 31: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Emittance blowup due to the crossing angle Colliding with no crossing angle and

x=100m, z=100m:

y (single pass)=4*10-4 L=2.1*1027

Colliding with crossing angle=2*25mrad and

x=2.67um, z=4mm (z*=100um, x/=104um):

y =4*10-3 (single pass) L=2.14*1027

Same geometric luminosity but 10 times more emittance blowup Adding the “Crab-waist”, Zy_waist(x)=x/2:

y =1.5*10-3 (single pass) L=2.29*1027

- the ‘hour glass’ is reduced, the geometric luminosity is higher: small effect about 5% more luminosity - the main effect: blowup due the the beam-beam is reduced,

about a factor 2.4 less y (3.8 times the nocross)

Page 32: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Colliding with an angle requires just the ILC DR and the ILC FF.

No compression needed

Crabbed ywaist is achieved by placing a sextupole upstream the IP (and symmetrically downstream) in a place in phase with the IP in X and at /2 in Y (much easier than the longitudinal travel focus).

Only natural energy spread in the beams Angular divergences about 150rad in both planes Crossing angle so large makes the IR (and the FF)

design very easy Low energy spread makes the FF very easy Beam currents around 1.9Amps, possible better trade

off currentdamping time

Page 33: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Collisions with uncompressed beamsCrossing angle = 2*25mradRelative Emittance growth per collision about 1.5*10-3

yout/yin=1.0015

Horizontal Plane Vertical Plane

Page 34: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Y bb_scan

Page 35: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Y bb_scan with 40um horizontal separationY field linear and much smaller kick:1.5rad instead of 150rad

No X separation y-scan

Page 36: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Ring Collider Uncompressed Bunches

Crab focus on in vertical plane Xcrossing_angle=2*25mrad

z=6mm e=6MeV e_Luminosity=9MeV

x=0.8nm y=0.002nm z=8.0m Collision_frequency=600MHz Lmultiturn=1.0*1036 (Lsingleturn=1.2*1036) with Np=2.3*1010

Vertical tune shift like in PEP!!! (similar currents,100 times more luminosity, 100 times smaller betay) Projected Sigmax=Sigmaz*Cross_angle=100m, like in PEP! Possible to further increase the luminosity with: - more current: L=1.8*1036 with Np=4*1010 - further simultaneuos x and y squeeze

- z shortening

Page 37: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Vertical beam size vs crab focusK2=sextupole strength

Luminosity vs crab focusK2=sextupole strength

With k2=8 the vertical emittance blowup is < 20% Luminosity gain about 70%Vertical size rms reduction about a factor 2.5, large tails reduction

Luminosity in excess of 1e36 is achievable

Ohmi simulations

Page 38: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Beam-Beam Tails (D.N. Shatilov)

Without Crab Focus With Crab Focus

Page 39: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Tune shift and luminosity with crossing angle

Very small:

z*=100m

=25mrad

x=9mm

Page 40: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

X-Z Coupling smaller then KeK:z*=100m=25mradx=9mm

Kicks that a particle receives while passing through the other beam

Page 41: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Multiturn simulations for uncompressed beams6Km ring, 12000 bunchesColl_freq=600MHz

Bunch_charge=2*1010 e=4mm, Xcrossing=2*25mrad

y0=2pm x0=400pm

Page 42: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

IPFF FF

ILC ring & ILC FF

Simplified layout in the Small Disruption Regime Collisions every TurnUncompressed bunchesCrossing angle = 2*25 mradCrabbed Y-Waist

Page 43: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi
Page 44: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

35m long FF

A.Seryi

Page 45: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Conclusions (1):- Rapid progress in the optimization of the

SuperB parameters and layout- First workable parameters set requires: - ILC damping ring, - ILC bunch compressor, - ILC Final Focus - No energy acceleration- Same parameters set but with increased

collision rate and reduced beam current gives more and more luminosity

- The optimal collision rate is every turn.

Page 46: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Solution with ILC DR + ILC FF and no compression seems extremely promising:

- Crossing angle of about 25mrad - Requires virtually no extra R&D - Uses all the work done for ILC - Ring and FF layouts virtually done, 6km (down to 2km should be

possible) circunference rings - 100% Synergy with ILC - IR extremely simplified - Beam stay clear about 20sigmas supposing 1cm radius beam pipe - Beam Currents around 2.0Amps - Background should be better than PEP and KEKB - Possibly to operate at the energy with L=1035

- Total cost less than half of the ILC e+ DRs (2 e+ 6km rings in ILC) - Power around 40MW, further optimization possible - Possible to reuse PEP RF system, power supplies, Vacuum pumps,

etc., further reducing the overall cost - Needs the standard injector system, probably a C-band 7GeV linac like

in KEKB upgrade (around 100ME)

Conclusions (2)

Page 47: Status on SuperB effort Daresbury, April 26, 2006 P. Raimondi

Conclusions (3)

• Possible fall back on the existing factories

• The crabbed waist potentially beneficial also for the current factories

• Possibility to simultaneously boost the performances of the existing machines and do SuperB R&D