Spallation in Dual-Shock Quark Nova: A Robust Nucleosynthetic Process
atmire.migration.oldid | 1363 | |
dc.contributor.advisor | Ouyed, Rachid | |
dc.contributor.advisor | Leahy, Denis | |
dc.contributor.author | Ouyed Hernandez, Amir Hassan | |
dc.date.accessioned | 2013-09-13T17:20:03Z | |
dc.date.available | 2013-11-12T08:00:17Z | |
dc.date.issued | 2013-09-13 | |
dc.date.submitted | 2013 | en |
dc.description.abstract | This thesis presents an alternate, spallation, nucleosynthesis mechanism in the context of the dual-shock Quark Nova (dsQN). The dsQN is an evolutionary channel where a core collapse supernova is followed by the detonation of its neutron star - an event that generates nuclear spallation reactions. Spallation produces new, daughter isotopes, by the fragmentation of larger nuclei - in contrast to conventional nucleosynthesis models which are based on the accretion of smaller nuclei and particles into larger nuclei. This spallation nucleosynthesis model is fairly extensive - it can produce abundant isotopes in the A < 130 mass range and therefore solve some of the issues faced by conventional r-process models. Furthermore, the specificities of dsQN spallation might be the key to explain the peculiarities of 44Ti production in the universe. Finally, dsQN spallation nucleosynthesis is fairly robust in relation to the universe’s age and the chemical composition of core-collapse supernovae. | en_US |
dc.identifier.citation | Ouyed Hernandez, A. H. (2013). Spallation in Dual-Shock Quark Nova: A Robust Nucleosynthetic Process (Master's thesis, University of Calgary, Calgary, Canada). Retrieved from https://prism.ucalgary.ca. doi:10.11575/PRISM/27841 | en_US |
dc.identifier.doi | http://dx.doi.org/10.11575/PRISM/27841 | |
dc.identifier.uri | http://hdl.handle.net/11023/945 | |
dc.language.iso | eng | |
dc.publisher.faculty | Graduate Studies | |
dc.publisher.institution | University of Calgary | en |
dc.publisher.place | Calgary | en |
dc.rights | University of Calgary graduate students retain copyright ownership and moral rights for their thesis. You may use this material in any way that is permitted by the Copyright Act or through licensing that has been assigned to the document. For uses that are not allowable under copyright legislation or licensing, you are required to seek permission. | |
dc.subject | Nuclear | |
dc.subject | Astronomy and | |
dc.subject | Elementary Particles and High Energy | |
dc.subject | Nuclear | |
dc.subject | Nuclear | |
dc.subject.classification | Supernova | en_US |
dc.subject.classification | Nucleosynthesis | en_US |
dc.subject.classification | strange matter | en_US |
dc.subject.classification | quarks | en_US |
dc.subject.classification | spallation | en_US |
dc.title | Spallation in Dual-Shock Quark Nova: A Robust Nucleosynthetic Process | |
dc.type | master thesis | |
thesis.degree.discipline | Physics and Astronomy | |
thesis.degree.grantor | University of Calgary | |
thesis.degree.name | Master of Science (MSc) | |
ucalgary.item.requestcopy | true |