Positron survival in type II supernovae

dc.contributor.advisorClayton, Donald D.en_US
dc.creatorSturner, Steven J.en_US
dc.date.accessioned2009-06-04T00:21:44Zen_US
dc.date.available2009-06-04T00:21:44Zen_US
dc.date.issued1990en_US
dc.description.abstractIn this work I investigate the possibility of Type II supernovae being the origin for positrons producing observed annihilation radiation observed toward the Galactic center. It was my contention that the decay of $\sp{56}$Co coupled with falling densities would allow for the production and extended existence of positrons in the supernova outflow. Supernova 1987A has prompted many people to construct models of supernova outflow. I use the results of two existing models as the initial conditions in my models. I have created both an analytic and a computer model for the survival of positrons. These models show that while Type II supernovae fall short of the needed production of surviving positrons, the lower densities existing in Type I supernovae may be a more promising source.en_US
dc.format.extent64 p.en_US
dc.format.mimetypeapplication/pdfen_US
dc.identifier.callnoThesis Sp. Sci. 1990 Sturneren_US
dc.identifier.citationSturner, Steven J.. "Positron survival in type II supernovae." (1990) Master’s Thesis, Rice University. <a href="https://hdl.handle.net/1911/13475">https://hdl.handle.net/1911/13475</a>.en_US
dc.identifier.urihttps://hdl.handle.net/1911/13475en_US
dc.language.isoengen_US
dc.rightsCopyright is held by the author, unless otherwise indicated. Permission to reuse, publish, or reproduce the work beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.en_US
dc.subjectAstronomyen_US
dc.subjectAstrophysicsen_US
dc.titlePositron survival in type II supernovaeen_US
dc.typeThesisen_US
dc.type.materialTexten_US
thesis.degree.departmentSpace Scienceen_US
thesis.degree.disciplineNatural Sciencesen_US
thesis.degree.grantorRice Universityen_US
thesis.degree.levelMastersen_US
thesis.degree.nameMaster of Scienceen_US
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