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dc.contributor.advisorIain Stewart.en_US
dc.contributor.authorProuty. Jeffrey Cen_US
dc.contributor.otherMassachusetts Institute of Technology. Department of Physics.en_US
dc.date.accessioned2015-01-05T20:06:48Z
dc.date.available2015-01-05T20:06:48Z
dc.date.copyright2014en_US
dc.date.issued2014en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/92695
dc.descriptionThesis: S.B., Massachusetts Institute of Technology, Department of Physics, 2014.en_US
dc.descriptionCataloged from PDF version of thesis.en_US
dc.descriptionIncludes bibliographical references (pages 51-53).en_US
dc.description.abstractWe continue the work of Abbate et al. in [1], in which a factorization formula for the thrust distribution in electron-positron collisions was developed in the framework of soft-collinear effective theory. We extend the analysis of thrust to the peak region of the distribution, in which a nonperturbative soft function encoding the effects of large-angle soft gluon radiation plays a significant role. We write the soft function as an infinite sum of basis functions and use a truncated version in our calculations, allowing us to fit for the basis coefficients ci with all available thrust data from center-of-mass energies Q = 35 to 207 GeV. To characterize the soft function independently of a particular parameterization, we present fit results for its cumulant moments, denoted [Omega]1, up to i = 4. We compute experimental uncertainties from the fits and theory uncertainties using a random scan in the space of the undetermined parameters of the theory. Our approach significantly improves the fit in the peak region, reducing the minimum X2/d.o.f. value from to 5.29 using the best fit form the tail region without fitting basis functions, to 1.23 using five basis functions. We find [Omega]1 = 0.387 ± (0.003)exp ±(0.026)pert GeV, indicating that the peak region determines [Omega] with considerably more precision than the tail. For the second cumulant moment, we find [Omega]'2 = 0.032 ± (0.002)exp ± (0.011)pert GeV2 . We also estimate the third and fourth cumulant moments, obtaining [Omega]'3 = [3.5 ± (0.7)expt ±(2.3)pert] x 10- GeV 3 and [Omega]'4 = [-0.7 ± (3 .8)exp ± (11.9)pert] X 10-4 GeV4.en_US
dc.description.statementofresponsibilityby Jeffrey C. Prouty.en_US
dc.format.extent53 pagesen_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsM.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectPhysics.en_US
dc.titleRigorous fit to the peak region of the thrust distributionen_US
dc.typeThesisen_US
dc.description.degreeS.B.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.identifier.oclc898331977en_US


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