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dc.contributor.advisorDenis Dujmic and Gabriella Sciolla.en_US
dc.contributor.authorSahin, Timur Cemalen_US
dc.contributor.otherMassachusetts Institute of Technology. Dept. of Physics.en_US
dc.date.accessioned2011-08-30T15:46:57Z
dc.date.available2011-08-30T15:46:57Z
dc.date.copyright2011en_US
dc.date.issued2011en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/65532
dc.descriptionThesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2011.en_US
dc.descriptionCataloged from PDF version of thesis.en_US
dc.descriptionIncludes bibliographical references (p. 43).en_US
dc.description.abstractDark matter makes up approximately 22% of the energy density of the universe and as much as 83% of its matter composition. Despite its ubiquitous nature, it remains incredibly difficult to detect due to the weakness of its interaction with the regular matter. The Dark Matter Time Projection Chamber (DMTPC) is an experiment that searches for traces of ionization created by Weakly Interacting Massive Particles (WIMP's). The detector uses a charge coupled device (CCD) camera to image the ionization signal created in the detector gas. The CCD chip itself is also sensitive to interactions with the WIMP's and the background radiation. In this thesis I explore the contributions these interactions may have on the DMTPC experiment. First, I develop an algorithm that filters out the electronic noise in the CCD chip such that the remaining images contain true ionization events in the chip. Second, I study insidious effects of neutron interaction with the CCD chip. I develop a GEANT4 based Monte Carlo simulation and set up an experiment that uses a neutron source with a known energy and measure the energy deposition in the chip. The energy spectrum agrees with the prediction based on the elastic scattering kinematics and the silicon ionization rate thus providing an energy calibration. Finally, I measure the level of background in the CCD chip coming from the inside of the camera, I set up an experiment in which outside neutrons are shielded with layers of plastic material and x-rays are suppressed with lead bricks surrounding the camera. Cosmic muons create particle showers that can also interact with the CCD chip so I build an active shield using a pair of scintillating paddles. I find that background interactions with silicon produce CCD signals that are small enough to be eliminated by existing DMTPC cuts on interaction range.en_US
dc.description.statementofresponsibilityby Timur Cemal Sahin.en_US
dc.format.extent43 p.en_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.titleInteractions of neutrons with silicon CCD chipsen_US
dc.title.alternativeInteractions of neutrons with silicon charge coupled device chipsen_US
dc.typeThesisen_US
dc.description.degreeS.B.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.identifier.oclc746898889en_US


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