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1 Introduction - Caltech High Energy Physics - California Institute of ...

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10 <strong>Introduction</strong><br />

Measuring γ<br />

Table 1-6 lists two expected statistical errors on the measurement <strong>of</strong> γ with 10 ab −1 . The more conservative<br />

error estimate <strong>of</strong> 2 ◦ − 3 ◦ is obtained employing only methods and decay modes that have already been<br />

observed and used in γ-related measurements. These are B ± → DK ± with D 0 → K − π + , D 0 → CP -<br />

eigenstates, and D 0 → KSπ + π − .The sensitivities are estimated from the quoted experimental references.<br />

The range in the estimates is due to current uncertainties in the ratio between the interfering b → u and<br />

b → c amplitudes, taken to be between 0.1 and 0.2. The mode D 0 → KSπ + π − is especially important in<br />

that it reduces the 8-fold asymmetry to a 2-fold asymmetry.<br />

The less conservative estimate <strong>of</strong> 1.2 ◦ − 2 ◦ is based on cautious assumptions about the sensitivities that<br />

could be obtained with modes that have yet to be fully explored experimentally. One category <strong>of</strong> such<br />

modes is additional multi-body D decays to final states such as π + π − π 0 , K + K − π 0 , KSK + K − , KSK + π − ,<br />

KSπ + π − π 0 , K + π − π 0 ,andK + π − π + π − . The second category is B 0 → DK (∗)0 , with a time-dependentand<br />

time-independentanalysis. The third category is B → D + KSπ − decays [16], which also requires a timedependent<br />

analysis.<br />

It should be noted that there are additional modes and methods, not included in the γ sensitivity estimates <strong>of</strong><br />

Table 1-6, that can be used to measure γ. These methods presently suffer from difficulties in obtaining a clean<br />

extraction <strong>of</strong> γ, which will likely be resolved in the future. Examples include sin(2β + γ) inB → D (∗)+ π − ,<br />

B → D (∗)+ ρ − , where BABAR has already published measurements <strong>of</strong> CP asymmetries and constraints on γ. It<br />

is not clear, however, whether the ratio between the interfering b → u and b → c amplitudes can be measured<br />

with sufficient precision for these measurements to be competitive with the B → DK measurements at high<br />

luminosity. The estimates also exclude the possible contribution <strong>of</strong> B ± → DK ± π 0 , where experimental<br />

issues are yet to be resolved and the level <strong>of</strong> interference is not yet known.<br />

1.2.3 <strong>Physics</strong> Performance Projections<br />

Various benchmark physics measurements, discussed in Sections 1.2.1 and 1.2.2, have been used to illustrate<br />

the physics reach <strong>of</strong> a Super B Factory on the basis <strong>of</strong> integrated samples. In some cases, comparisons with<br />

hadronic experiments are also possible. A set <strong>of</strong> assumptions has been made concerning the pace at which<br />

these projects reach their design luminosity goals, as summarized in Table 1-7. These assumptions then form<br />

the basis for time varying projections <strong>of</strong> effective tagged samples in a number <strong>of</strong> important channels (observed<br />

yield weighted by effective tagging efficiency). Finally, the effective tagged sample sizes, when combined with<br />

measured or simulated single event sensitivities can be used to project the errors on benchmark observables.<br />

In the case <strong>of</strong> the e + e − collider options the samples are assumed to be continuations <strong>of</strong> the event samples<br />

obtained at PEP-II through the end <strong>of</strong> the already planned program. In all cases, PEP-II is assumed to<br />

cease operations at the point when installation <strong>of</strong> the upgraded collider must begin. Integrated luminosities<br />

in these periods are taken from the published PEP-II plan.<br />

Figure 1-3 shows the time evolution <strong>of</strong> the error on the sine coefficient for time-dependent CP violation in<br />

various b → s Penguin modes. In this case the error reaches below 0.04 in most case within two years, which<br />

is the regime that is relevant for definitive demonstration <strong>of</strong> potential New <strong>Physics</strong> in such modes. Figure 1-7<br />

shows the error evolution for the electromagnetic Penguin mode B 0 → K 0 Sπ 0 γ.<br />

Figure 1-4 shows the effective tagged sample accumulations and expected evolution <strong>of</strong> the error on the<br />

sine amplitude in time-dependent CP asymmetries for B 0 → π + π − . In this case both LHCb and BTEV<br />

are capable <strong>of</strong> measurements, as well as a Super B Factory. However, only a Super B Factory is capable<br />

<strong>of</strong> doing the complete isospin analysis <strong>of</strong> the two-body modes in order to obtain the correction from the<br />

determination <strong>of</strong> αeff in the CP asymmetry from the charged mode to the unitarity angle α. The evolution<br />

<strong>of</strong> this correction as a function <strong>of</strong> time is shown in Figure 1-5. The error on sin 2α falls below 0.05 within<br />

two years <strong>of</strong> startup for the Super B Factory.<br />

The Discovery Potential <strong>of</strong> a Super B Factory

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