EF04 Topical Group Conversation

US/Eastern
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Meeting ID: 955 4136 9778

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Jakob Beyer / Jenny List - Beam polarization for EWK precision
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two advantages:
direct access to chiral interactions (shown for future colliders)
isolating systematic effects (still open question)

looking at EWK fit in different scenarios:
both beam polarized (ILC-like)
only e- polarized (CLIC-like)
no-polarized scenario not yet investigated

2/ab and 10/ab scenarios
in fit, polarization and luminosity (the uncertainties?) are free parameters

look at e+e- -> Z/G* -> mu+mu-
return-to-Z events, and high sqrt(s)
polarization-weighed distributions -> toy-fluctuated distributions -> combined log-likelihood fit

6 fit parameters
physical parameters (3):
total chiral cross section; initial/final fermion chiral asymmetry
correction parameters (3):
interference correction
radiative correction factors (L and R separately)

fit results
uncertainty drops by factor 2 in high-lumi case
about 20% reduction when adding e+ polarization?

Ae (the electron - i.e., initial - chiral asymmetry) decreases a lot (factor 4?) when positron beam polarized
results on polarization (nuisance parameter) and Ae shows importance of redundancy offered by knowing e+ polarization

systematic effects
flipping polarization, get different physics, in same detector -> unique global signatures of systematic effects, can be decoupled and reduce their effect

looked at some of them: first tested (looked at LEP papers) is muon acceptance
(ALEPH, L3, OPAL: muon acceptance was among dominant)
used two parameters to describe acceptance: dC and dW (C is acceptance, W is cos\theta\*)
acceptance modeled as a box (center, width - C and W)

ILD: could be able to ID muons up to 7deg from beamline

in fit, dC and dW (size of box) are determined very well
beam polarization: uncertainty on C and W halved
for this setup, only two parameters affected by letting dC and dW free: KL and KR
see that effect is very small, and there is no additional advantage from e+ polarization (mu acceptance is well determined)

question: is model too simplified? what is case with unpolarized beams?

direct access to chiral part of interactions makes EWK measurements much easier: decouples them from other physical or systematic effects that do not depend on 
polarization

Ayres: Ae determined much less precisely than Af; Af is from AFB, which, at Z pole, is proportional to product of Ae and Af: why one much more precisely than the other?
JB: we have access to polarized AFB, and that is directly proportional to Af
Ayres: then, would not you need to know polarization well? 
JB: shall check interpretation of results; all improvement in Ae, Pe-, Pe+ is from redundancy, need to think about that

Ayres: what about e+e- -> e+e-? Af becomes Ae, one could do combined fit of the two processes... would that make advantage of positron polarization less important? (one 
can get Ae from final state)
JB: issue is extra term from t-channel, interpretation less direct (but can be done)

Ayres: all quantities improve, but need also to keep in mind that polarization comes at price of luminosity

in parameterization (slide 5), it is linear in cos\theta; summing the two to get unpolarized cross section, get term proportional to Ae*Af

Junping: this is single channel w/ muon, Ae should be better at end if looking at all fermion pairs
JB: indeed

question is why Ae precision much worse than Af; then, adding all channels, difference goes away?

Alberto: unpolarized scenarios?
JB: parameter like Ae cannot be determined, fit does not converge, cannot get uncertainty
planning to add constraints to parameters that cannot be determined

Junping: Ae and Af can be decoupled if one integrates out cos\theta distribution (Af disappears), and Ae is just count of events; is that why Ae limited by knowledge of 
polarization, while Af is from asymmetry?
Ayres: one could go to double-AFB (initial and forward); this depends on Af, but again affected by polarization uncertainties

Junping: on systematic uncertainties; how are C and W fixed from data? cut on angular distribution in cos\theta?
JB: determining w/ MC what is the influence of cut on C and W (and variations of these cuts) on the differential distributions, then parameterize the bin variations (when 
varying the cuts on C and W)
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