The effects of a depleted Maxwellian tail on thermonuclear reactions, pressure, and solar neutrinos

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dc.contributor.advisorClayton, Donald W.en_US
dc.creatorDwek, Elien_US
dc.date.accessioned2018-12-18T21:16:53Zen_US
dc.date.available2018-12-18T21:16:53Zen_US
dc.date.issued1975en_US
dc.descriptionText includes handwritten formulasen_US
dc.description.abstractNuclear reaction rates and pressure are calculated using a Maxwellian distribution function which is depleted at its high energy tail. The results are applied to nuclear reactions occuring within the solar interior, showing that the neutrino counting rate can be significantly reduced.en_US
dc.format.digitalOriginreformatted digitalen_US
dc.format.extent58 ppen_US
dc.identifier.callnoThesis Sp. Sci. 1975 Dweken_US
dc.identifier.citationDwek, Eli. "The effects of a depleted Maxwellian tail on thermonuclear reactions, pressure, and solar neutrinos." (1975) Master’s Thesis, Rice University. <a href="https://hdl.handle.net/1911/104061">https://hdl.handle.net/1911/104061</a>.en_US
dc.identifier.digitalRICE1687en_US
dc.identifier.urihttps://hdl.handle.net/1911/104061en_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.titleThe effects of a depleted Maxwellian tail on thermonuclear reactions, pressure, and solar neutrinosen_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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