Grant: Subatomic Physics Envelope - Project

The Standard Model of Particles and Interactions summarizes our current understanding of the fundamental particles in nature, and the interactions they undergo. There are four forces in nature: the gravitational force, the electromagnetic force and the weak and strong nuclear forces. Some fundamental particles include electrons and the quarks that make up protons and neutrons. The strength with which these particles interact via a particular force depends on the size of the ?charge? for that force. The weak and electromagnetic forces have been unified and it is a goal of subatomic theorists to unify the other two forces as well. The discovery of the Higgs boson at CERN validates the Standard Model to a certain extent, but there are still things we do not know. Dark matter and dark energy, for example, are not yet included in the Standard Model. Therefore testing the Standard Model has a high priority within the subatomic physics community. The MOLLER collaboration will measure the parity-violating asymmetry in polarized electron-electron (Moller) scattering. In the Standard Model, this asymmetry is due to the interference between the electromagnetic and the weak forces, the latter being mediated by the Z0 boson. The asymmetry is predicted to be ~35 parts per billion (ppb) at the kinematics of the MOLLER experiment. The goal is to measure its value to a precision of 0.73 ppb. The result will yield a measurement of the weak charge of the electron to a fractional accuracy of 2.3% at an average Q2 of 0.0056 GeV^2. The measurement will be carried out in Hall A at Jefferson Laboratory, where an 11 GeV longitudinally polarized electron beam will be incident on a 1.5 m liquid hydrogen target. Moller electrons (beam electrons scattering off target electrons) in the full range of the azimuth and spanning the polar angular range 5 - 19 mrad, will be separated from background and brought to a ring focus ~ 30 m downstream of the target by a spectrometer system consisting of a pair of toroidal magnet assemblies and precision collimators. The Moller ring will be intercepted by a system of quartz detectors; the resulting Cherenkov light would provide a relative measure of the scattered flux. Simultaneously with data collection, beam properties such as position, angle and energy will be monitored, the polarization of the beam will be measured, and auxiliary detectors will measure backgrounds. Special runs will be used to measure the mean scattering angle. MOLLER is sensitive to the interference of the electromagnetic amplitude with new neutral current amplitudes as weak as ~10^-3 G_F from as yet undiscovered high energy dynamics. Such a level of sensitivity is unlikely to be matched by any experiment measuring a flavor- and CP-conserving process over the next decade, and results in a unique window to new physics at the multi-TeV scale in a manner complementary to direct searches at high energy colliders. MOLLER will be sensitive to physics beyond the Standard Model, including supersymmetry and some ""dark"" particles. In the Standard Model, the measurement of the weak charge of the electron yields a determination of the weak mixing angle with an uncertainty of +/- 0.00026 (stat) +/- 0.00013 (syst), similar to the accuracy of the single best such determination from high energy colliders. Thus, our result will influence the central value of this fundamental electroweak parameter, a critical input to deciphering signals of any physics beyond the Standard Model that might be observed at the Large Hadron Collider (LHC). If MOLLER measures a value of the weak mixing angle that differs from the Standard Model prediction, then there must be a new, as-yet-undiscovered particle that could have a mass of 7.5 TeV or higher.