run 8 polarization measurements from star bbc andrew gordon september 12, 2008
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Run 8 Polarization measurements from STAR BBC
Andrew GordonSeptember 12, 2008
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} {East-West Coincidence
Bunch Crossing (7-bits){
Hank’s Scaler Boards
}
24-bit word is histogrammed every clock cycle
Inner tiles of BBC accumulated every clock cycle
Discriminated phototube outputs
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Requirements:
Outer left and right phototubes of small tiles have no hits.
Left Hit=Hit in 2 or 3 AND no hit in 5 and 6
Right Hit=Hit in 5 or 6 AND no hit in 2 and 3
Polarization:
p
NL NR
up down
NR NL
up down
-
NL NR
up down
NR NL
up down
+=
For effective analyzing power use final Run 6 polarizations and Run 6
BBC data:Yellow Polarization (%)=p(East)/(6.9±0.1(stat))x10-5
Blue Polarization (%)=p(West)/(7.1±0.1(stat))x10-5
See also J. Kiryluk (STAR) ArXiv:hep-ex/0501072v1, 28 Jan 2005
and C.A.Whitten (STAR), Proceedings PSTP 2007, p. 390.
Effective Analyzing PowerBBC Polarimeter
• Analysis from available run-6 data more complete analysis still to do
• Event data suggests BBC very similar year to year assume same effective analyzing power for run 8
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Example: Rates for start of Fill 9949East-West Coincidence Rates for each crossing
100 Yellow
filled & Blue
filled crossings
7 Yellow Empty
& Blue Filled
bunches
7 Yellow Filled &
Blue Empty bunches
Yellow Background ~ 0.1%
Blue Background ~ 0.2%
<Instantaneous BBC Rate>
~0.5 MHz
Star preliminary
6
Background level from abort gaps low
Yellow filled & Blue empty
Yellow empty & Blue empty
Yellow empty & Blue filled
Yellow filled & Blue filled
<Blue Empty & Yellow Filled>
<Blue Filled & Yellow Filled>
Yellow beam Background fraction
=
<Blue Filled & Yellow Empty>
<Blue Filled & Yellow Filled>
Blue beam Background fraction
=
Star preliminary
Example: Background for Fills 9949 and 9951
Note change
of scale on y-
axis
Background
fractions low and
relatively stable,
except for event in
blue beam at around
3 hours.
Time=midpoint of run relative to start of fill, <run time> ~ 10 minutes Star preliminary
Example: Multiplicity for Fills 9949 and 9951
Average number of
BBC phototubes with
hits is relatively
stable. (Event in blue
beam 9949 not
detectable.)
East BBC
West BBC
Star preliminary
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Sample polarization time dependenceDecline visible in fill 9949, but 9951 more stable.
Time=midpoint of run relative to start of fill, <run time> ~ 10 minutes Star preliminary
Flat line fits shown Flat line fits shown
10Polarization dependence not always smooth decay
Star preliminary
11Polarization dependence not always smooth decay
Star preliminary
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Effective decay rates of polarization vs Fill
Polarization of each fill fitted to
P = A e-t
separately for each beam.
Yellow beam decay rate more consistently non-zero than blue beam.
Star preliminary
Comparing to Whitten PSTP 2007, roughly same rates as for Run 6.
Polarization in units of percent. The values for are the y-axis values divided by 100.
<100>=1.7±0.1
<100>=0.7±0.1
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Fill averaged polarizationsRun 6 calibration of BBC asymmetries applied to Run 8 data.
Star preliminary
Comparison of Polarization to CNI results
For each fill calculate
STAR/pC
Error bars are uncorrelated errors only.
pC data from Sasha, September 12, 2008. Uncertainties dominated by pC uncertainty estimates.
Mean=1.026±0.023
Mean=0.929±0.012
15Conclusions
Absolute polarization can be derived from Run 6 calibration.
Polarization shows dependence on time.
•Some fills show a step downward in middle of fill
•Stronger for the yellow beam
STAR can measure polarization at relatively small time steps.