Status and development of the large angle beamstrahlung monitor for superkekb
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Status and development of the Large Angle Beamstrahlung Monitor for SuperKEKB. Giovanni Bonvicini. Collaboration: Hawaii (G. Varner) KEK (J. Flanagan, Y. Funakoshi, K. Kanazawa, N. Ohuchi) Luther College (T. Pedlar) PNNL ( D. Asner et al.)

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Status and development of the large angle beamstrahlung monitor for superkekb

Status and development of the Large Angle Beamstrahlung Monitor for SuperKEKB

Giovanni Bonvicini


Collaboration: Monitor for SuperKEKB

Hawaii (G. Varner)

KEK (J. Flanagan, Y. Funakoshi, K. Kanazawa, N. Ohuchi)

Luther College (T. Pedlar)

PNNL ( D. Asner et al.)

Wayne State Univ. (G. Bonvicini, H. Farhat, R. Gillard)

Outline:

Experimental method

CESR device and results

SuperKEKB design

Possibilities for SuperKEKB


What is beamstrahlung
What is beamstrahlung Monitor for SuperKEKB

  • The radiation of the particles of one beam due to the bending force of the EM field of the other beam

  • Used to monitor the beam-beam interaction already at SLC (in the gamma ray part of the spectrum), it produced fundamental information about the beam conditions.

  • Produced at SuperKEKB, 1.3kW for LER and 5.4 kW for the HER at nominal conditions

  • Many similarities with SR but

  • Also some substantial differences due to very short “magnet” (L=z/2√2=2mm). Short magnets produce a much broader angular distribution


Major efforts in diagnosing luminosity degradation already at KEKB - BMST Monitor improves instrumentation. L=(I+I-)Xspec. Lum.


Beam beam interaction limits the achievable luminosity and has many d o f 7 in the transverse plane
Beam-beam interaction limits the achievable luminosity and has many d.o.f. (7 in the transverse plane)


Methods to measure the beam beam interaction

A very difficult experimental problem - few measurements, many degrees of freedom

Gamma ray part of the Beamstrahlung spectrum used with great success at SLC

Beam-beam scanning and scattering also very successful at SLC (two quantities)

Frequency locked vertical oscillation successful at CESR (one quantity)

Other methods indirect

Methods to measure the Beam-Beam Interaction


Properties of large angle radiation
Properties of large angle radiation many degrees of freedom

  • It corresponds to the near backward direction in electron rest frame (5 degrees at CESR, 2-4 degrees at KEKB)

  • Lorentz boost of EM field produces a 8-fold pattern, unpolarized as a whole, but locally up to 100% polarized according to cos2(2), sin2(2)

  • Polarization carries information about the direction of the forces in the beam-beam interaction. It is easily measured in the infrared or visible.



From diagrams to asymmetries
From diagrams to asymmetries (collinear beams case)

  • Derive asymmetry parameter from diagram and plot versus waste parameter (w=1-L/L0 ), or (w=1-S/S0 ), S the specific luminosity

  • Apply correction based on measured asymmetry

  • The whole collinear beams analysis depends on two parameters, L0 and U0


Multiple pathologies (collinear case) showed complete convergence of the correction processand 6 out of 7 transverse degrees of freedom measured from diagram and its derivatives


Large angle beamstrahlung power
Large angle beamstrahlung power convergence of the correction process

  • Energy for collinear collision by beam 1 is: P0=0.112re3mc2N1N22/(x2z)

  • Wider angular distribution (compared to quadrupole SR) provides main background separation

  • CESR regime: exponent is about 4.5

  • SuperKEKB: exponent is 0.13 to 0.62


Large angle detector concept
Large Angle Detector Concept convergence of the correction process

  • Radiated power for

    horizontal and vertical polarizations

  • Two optic ports are reserved for each direction (E and W)

  • IR PMT for signal, VIS PMT for background


Cesr location
CESR location convergence of the correction process


Set up principal scheme
¼ Set-up principal scheme convergence of the correction process

  • Transverse view

  • Optic channel

  • Mirrors

  • PBS

  • Chromatic mirrors

  • PMT numeration


Detector parameters of interest
Detector parameters of interest convergence of the correction process

  • Diffraction limit is 0.1 mrad (0.15-0.3mrad at SuperKEKB). Sharp cutoff can be assumed

  • Optics is double collimator. Has triangular acceptance with max width of 1.7mrad

  • At IP, accepted spot is about 1cm (0.4cm at SuperKEKB)


Set up general view
Set-up general view convergence of the correction process

  • East side of CLEO

  • Mirrors and optic port ~6m apart from I.P.

  • Optic channel with wide band mirrors


On the top of set up
On the top of set-up convergence of the correction process

  • Input optics channel

  • Radiation profile scanner

  • Optics path extension volume


The detector
The ¼ detector convergence of the correction process

  • Input channel

  • Polarizing Beam Splitter

  • Dichroic filters

  • PMT’s assembly

  • Cooling…


Check for alignment @ 4 2gev
Check for alignment @ 4.2GeV convergence of the correction process


Directionality
Directionality convergence of the correction process

  • Scanning is routinely done to reconfirm the centroid of the luminous spot.


Pmt rate correlations with beam currents
PMT rate correlations with beam currents convergence of the correction process


Natural variability of machine provided crucial evidence
Natural variability of machine provided crucial evidence convergence of the correction process

  • In July, relatively high e+ current and relatively low e- current. In December, currents are more balanced, providing a stronger expected BMST signal

  • In July, e- beam was smaller than e+. In December, the reverse was true. Differing polarizations expected


Main results page
Main results page convergence of the correction process

  • Signal(x) strongly correlated to I+I-2

  • Signal strongly polarized according to ratios of vertical sigmas

  • Total rates consistent with expectations at 10.3 mrad


Backgrounds
Backgrounds convergence of the correction process

  • At CESR, S/B~0.02-0.7

  • Signal per collision will increase by 2-400,000 at SuperKEKB (at equal angles), while backgrounds will remain approximately the same or decrease

  • Backgrounds are dominated by the beam tails. At CESR, beams were off center in the quadrupoles, and that further increased backgrounds


Superkekb parameters
SuperKEKB parameters convergence of the correction process

  • SuperKEKB simulations show large signals at 5mrad, high sensitivity to offsets, and unchanged sensitivity to y-mismatches.

  • High signals suggest the same optics used at CESR, double collimator with no focusing.

  • 1% systematics from asymmetries corresponds to about 1 nm sensitivity at SuperKEKB for offset, 2nm for y-bloating


Pmt array
PMT array convergence of the correction process

  • From VIS/IR at CESR to 4 bands at SuperKEKB

  • Useful for background determination, and also for bunch length direct measurement from different spectra in x- and y- PMTs


Beam pipe insert
Beam pipe insert convergence of the correction process

  • View port location at ±90 degrees minimizes backgrounds, polarization measurement errors, and provides redundancy against beam orbit errors

  • To be located anywhere between 5 and 10 mrad from the beam direction at the IP

  • Suggested mirror and window sizes: 2X2.8mm2 and 2.2X2.2 mm2 (we could go lower at 10 mrad). Mirror is collimator 1

  • Well measured distance between mirrors provides a constraint against beam pipe misalignments


Main optics box
Main Optics Box convergence of the correction process


Some results from current activities
Some results from current activities convergence of the correction process

The Test bench shows ratios of efficiencies that depend on rates. PMT response Characterization:

R=R0**(1+aR/K1)*(1+b/K2)


Rotation of pmts for online calibration
Rotation of PMTs for online calibration convergence of the correction process

PMT can can rotate to five different positions, -90 to +90 degrees step 45. There will be 40 measurements for 32 d.o.f., of which 16 will be measured also on the Test Bench.


Beam dump direct measurement of background
Beam Dump: direct measurement of background convergence of the correction process

  • When one beam is lost, the other beam goes from the colliding beam envelope to the single beam envelope over several damping times (50 msec or so)

  • Triggering on such an event, or storing and retrieving data, would measure backgrounds directly.


Design summary
Design Summary convergence of the correction process

  • Double, opposite mirrors minimize backgrounds and eliminate beam position systematics

  • Different possible locations of primary mirrors are dealt with by observing at different wavelengths

  • Small PMT and optics systematics are controlled by Test Bench measurements and online calibration

  • Box can be made as small as 25X25X40 cm3, and it can go anywhere from (0-3) meters from Pipe


Data analysis system
Data analysis system convergence of the correction process

  • Where algorithms are tried offline before they go in EPICS

  • One server (non-EPICS) with 50 TB of disk space (at 1kHz sampling, 2.5 years of data)

  • Substantial analysis platform by T. Pedlar (ROOT-based), including periodometer, advanced fitting and other statistical software, global data analysis

  • Event record of order 100 variables including all beam monitors (LABM, Interferometers, BPM, Luminosity Monitors, Ground Motion sensors)


Electronics
Electronics convergence of the correction process

  • Front end electronics from G. Varner, Hawaii

  • Some work needed about data packaging and algorithms to extract needed information from EPICS. PNNL, Luther College interested in this part


Some examples of potentially interesting special data taking
Some examples of potentially interesting special data taking convergence of the correction process

  • Bunch-to-bunch effects

  • Measurement of beam tails at IP during fill

  • Ground motion effects on IP Beam Spot

  • frequency-locked measurements at IP (1nm IP variations)

    ALL THESE ARE PASSIVE MEASUREMENTS EXCEPT FREQUENCY-LOCKED


Ground motion labm vs luminosity monitor
Ground motion: LABM vs luminosity monitor convergence of the correction process

  • A luminosity monitor does not pick out higher corrections. If luminosity decreases due to defocussing, and luminosity feedback is activated, the luminosity will decrease further

  • Even if the motion is purely offset-y, a luminosity monitor will not specify whether the correction is up or down

  • LABM can produce an asymmetry, Au-d=(Ru-Rd)/(Ru+Rd), which will specify the direction of deflection. For offset-y=1nm, =5mrad, and the UV PMTs, Au-d=0.04, recorded on two sides and two polarizations


Conclusions
Conclusions convergence of the correction process

  • This project is about making the study of the beam-beam interaction data-driven

  • The tools are a direct, precise monitor of the beam-beam interaction, global, ILC-type monitor analysis, and a flexible DAQ system

  • We hope that SuperKEKB scientists will use and be helped by the information this device can produce



If the angle can be considered large and constant
If the angle can be considered large and constant… convergence of the correction process

  • Assuming (atan(z/)+atan((L-z)/ ) as the field profile, one gets (u=s,c=cos,sin())


Ilc concept
ILC concept convergence of the correction process


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