The Impact of SuperB on Flavor Physics
Author(s) -
B. Meadows,
Monika Blanke,
A. Stocchi,
A. Drutskoy,
A. Cervelli,
Michel Giorgi,
A. Lusiani,
A. Perez,
J. Walsh,
Tobias Hurth,
A. J. Bevan,
L. Silvestrini,
M. Ciuchini,
C. Tarantino
Publication year - 2012
Publication title -
osti oai (u.s. department of energy office of scientific and technical information)
Language(s) - English
Resource type - Reports
DOI - 10.2172/1035111
Subject(s) - physics beyond the standard model , physics , context (archaeology) , particle physics , observable , luminosity , collider , nuclear physics , quantum mechanics , paleontology , galaxy , biology
This report provides a succinct summary of the physics programme of SuperB, and describes that potential in the context of experiments making measurements in flavour physics over the next 10 to 20 years. Detailed comparisons are made with Belle II and LHCb, the other B physics experiments that will run in this decade. SuperB will play a crucial role in defining the landscape of flavour physics over the next 20 years. SuperB is an approved high luminosity e{sup +}e{sup -} collider intended to search for indirect and some direct signs of new physics (NP) at low energy, while at the same time, enabling precision tests of the Standard Model (SM). This experiment will be built at a new laboratory on the Tor Vergata campus near Rome, Italy named after Nicola Cabibbo. The project has been described in a Conceptual Design Report, and more recently by a set of three white papers on the accelerator, detector, and physics programme. The main focus of the physics programme rests in the study of so-called Golden Modes, these are decay channels that provide access to measurements of theoretically clean observables that can provide both stringent constraints on models of NP, and precision tests of the SM. A number of ancillary measurements that remain important include those with observables that may not be theoretically clean, and those that can be used to provide stringent constraints on the SM but are not sensitive to NP. The remainder of this section introduces SuperB before discussing the golden modes for SuperB, precision CKM measurement modes, and an outline of the rest of this report
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