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IP Characterization Measuring the Boost Vector. Matt Weaver PEP Meeting May 15, 2006. Motivation. Measure parameters contributing to luminosity to quantitatively verify that we’re generating all we can. Machine behavior in collision may have surprises that we can benefit from understanding.
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IP Characterization Measuring the Boost Vector Matt Weaver PEP Meeting May 15, 2006
Motivation • Measure parameters contributing to luminosity to quantitatively verify that we’re generating all we can. • Machine behavior in collision may have surprises that we can benefit from understanding.
Boost Trajectory Measurement e+ e- m- m+ Measure collision point {x,y,z} and trajectories of mm pair {x’,y’} z mean, spread, distribution x,y mean, spread, correlation with z x’,y’ mean, spread, correlation with z correlation with x,y z resolution ~ 60 mm x,y resolution ~ 30 mm x’,y’ resolution ~ 0.6 mrad
Boost Vector Properties Near the waist (z << b*), x and x’ are uncorrelated x z this 9 times greater than Expect that X measurements behave like this (z << b*X) Boost X’ spread largely reflects HER X’ angular spread
Move to half-integer x-tune Luminous X-size (mm) dynamic b HER X’-spread (mrad) dynamic b + ?
Boost Vector Properties Far from the waist (z >> b*), x and x’ are highly correlated x z Bunch lengths are small compared to b*X and comparable to b*Y, so we never see these relations fully. However, the transition must develop on a z-scale of b*, so the z-dependence of these msmts must be a measure of b*
Boost Vector Z-Dependence (luminosity-weighted)
Monte Carlo Validation dy’/dy 14mm b* 14mm b* sy’ mrad mrad-cm 5 fit parameters bY* y-waist z offset eH eL s2YY’ detector error z (cm) z (cm) 10mm b* 10mm b* Fit c2 is a simple sum of the two c2s No s2{sy’ dy’/dy} covariance terms included 6mm b* 6mm b* ~ 1 week data
Example measurement of angular spread Non-zero slope is reminiscent of lumi X-size measurements. Implies X-waist offset. “Width” is measure of b*. “Height” is measure of e/b*. Value at z-centroid is well-determined. Limit for z>>b* not reached.
Example measurement of collision position-boost angle correlation “Z >0” “Z <0”
Run5 Fit Results lumi centroid waist z (mm) b* (mm) eL (nm) eH (nm)
SY (mm) SY derived from combined-fit results shows good anti-correlation with specific luminosity Specific Luminosity
2.5 2 1 SX derived from Y measurements “SX” X sizes (mm) sXL SX / sXL Ratio of beam x-sizes
Fit Results b* (mm) waist z (mm) lumi centroid waist eL (nm) eH (nm)
Plans Separately determine HER, LER b*Y and y-waist locations Estimate impact of coupling, dispersion {hY, hY’} Make a measure of coupling y’B(x), x’B(y) What to do with x? 3 measurements { sX,sX’,x’B(x)}, at least 4 parms Make quantitative comparisons to beam-beam simulation versus bunch current, tune?
Boost Trajectory Measurement e+e-m+m- • mmomenta poorly measured • trajectories well measured • reconstruct mm decay plane normal n n n l y n z m- f x U m+ tanl = - x’Bcosf – y’Bsinf ≈l x’(or y’)B = EH x’H – EL x’L EH - EL
Y-Y’ Correlation in Run5 Data Y distribution Less S-shape y’ (mrad) Shift in mean Y-mean depends upon f More work to do here y’ vs y in various z-bins y (cm) y (cm) y’ vs y in various z-bins dy’/dy versus z dy’/dy z (cm)
Slope of x’ angular spread Move to half-integer x-tune d sx’H / dz (mrad/cm) Need to know emittances and beta*s to convert into a waist shift
From x-x’ correlation measurement assuming common waist X-waist offset (cm) Move to half-integer x-tune
generated value Monte Carlo Fit Results b* (mm) waist z (mm) eL (nm) eH (nm) sy’(z) fit only combinedfit
Toy Monte Carlo Tests dy’/dy bH*= bL*=10mm zH=zL=0 bH*= bL*=10mm zH=zL=0 sy’ mrad mrad-cm 7 fit parameters b*H, b*L y-waist z offsets (H,L) eH, eL s2YY’ detector error z (cm) z (cm) bH*= bL*=10mm zH=+4mm zL=-4mm bH*= bL*=10mm zH=+4mm zL=-4mm Correlated detector errors are not modeled bH*= 8.23mm bL*=13.72mm zH=zL=0 bH*= 8.23mm bL*=13.72mm zH=zL=0 ≤ 1 week data
generated value Toy Fit Results b*L (mm) b*H (mm) zL (mm) zH (mm)
Fit Results b* (mm) waist z (mm) eL (nm) eH (nm)
SY (mm) SY derived from combined-fit results shows good anti-correlation with specific luminosity Specific Luminosity