The Lowest ℓ = 0 Proton Resonance in Si-26 and Its Implications for the Stellar Nucleosynthesis of Al-26.
Determining the stellar production site of 26Al is an exciting problem that spans experimental and theoretical nuclear physics, astrophysics, and observational astronomy. This thesis details an experiment to measure the 25Al(d,n)26Si single proton transfer reaction, which can provide information on...
Other Authors: | |
---|---|
Format: | Others |
Language: | English English |
Published: |
Florida State University
|
Subjects: | |
Online Access: | http://purl.flvc.org/fsu/fd/FSU_migr_etd-2032 |
id |
ndltd-fsu.edu-oai-fsu.digital.flvc.org-fsu_180280 |
---|---|
record_format |
oai_dc |
spelling |
ndltd-fsu.edu-oai-fsu.digital.flvc.org-fsu_1802802020-06-09T03:08:56Z The Lowest ℓ = 0 Proton Resonance in Si-26 and Its Implications for the Stellar Nucleosynthesis of Al-26. Peplowski, Patrick N. (Patrick Nelson), 1981- (authoraut) Wiedenhöver, Ingo (professor directing dissertation) Fuelberg, Henry (outside committee member) Volya, Alexander (committee member) Rogachev, Grigory (committee member) Höflich, Peter (committee member) Department of Physics (degree granting department) Florida State University (degree granting institution) Text text Florida State University Florida State University English eng 1 online resource computer application/pdf Determining the stellar production site of 26Al is an exciting problem that spans experimental and theoretical nuclear physics, astrophysics, and observational astronomy. This thesis details an experiment to measure the 25Al(d,n)26Si single proton transfer reaction, which can provide information on the astrophysically significant 25Al(p,gamma)26Si reaction. The first 3+ state in 26Si, which is predicted to dominate the stellar nucleosynthesis rate, was observed and characterized. The implications for stellar nucleosynthesis are discussed for potential stellar production sites. A Dissertation Submitted to the Department of Physics in Partial FulfiLlment of the Requirements for the Degree of Doctor of Philosophy. Spring Semester, 2009. March 3, 2009. Nuclear Physics, 26Al, Al-26, 26Si, Si-26, Galactic Al-26 Distribution, Radioactive Ion Beam, Al-25, 25Al, Rapid Proton Process, rp-process, Classical Nova, Core Collapse Supernova, Nova, Supernova Includes bibliographical references. Ingo Wiedenhöver, Professor Directing Dissertation; Henry Fuelberg, Outside Committee Member; Alexander Volya, Committee Member; Grigory Rogachev, Committee Member; Peter Höflich, Committee Member. Physics FSU_migr_etd-2032 http://purl.flvc.org/fsu/fd/FSU_migr_etd-2032 This Item is protected by copyright and/or related rights. You are free to use this Item in any way that is permitted by the copyright and related rights legislation that applies to your use. For other uses you need to obtain permission from the rights-holder(s). The copyright in theses and dissertations completed at Florida State University is held by the students who author them. http://diginole.lib.fsu.edu/islandora/object/fsu%3A180280/datastream/TN/view/Lowest%20%E2%84%93%20%3D%200%20Proton%20Resonance%20in%20Si-26%20and%20Its%20Implications%20for%20the%20Stellar%20Nucleosynthesis%20of%20Al-26..jpg |
collection |
NDLTD |
language |
English English |
format |
Others
|
sources |
NDLTD |
topic |
Physics |
spellingShingle |
Physics The Lowest ℓ = 0 Proton Resonance in Si-26 and Its Implications for the Stellar Nucleosynthesis of Al-26. |
description |
Determining the stellar production site of 26Al is an exciting problem that spans experimental and theoretical nuclear physics, astrophysics, and observational astronomy. This thesis details an experiment to measure the 25Al(d,n)26Si single proton transfer reaction, which can provide information on the astrophysically significant 25Al(p,gamma)26Si reaction. The first 3+ state in 26Si, which is predicted to dominate the stellar nucleosynthesis rate, was observed and characterized. The implications for stellar nucleosynthesis are discussed for potential stellar production sites. === A Dissertation Submitted to the Department of Physics in Partial FulfiLlment of the Requirements for the Degree of Doctor of Philosophy. === Spring Semester, 2009. === March 3, 2009. === Nuclear Physics, 26Al, Al-26, 26Si, Si-26, Galactic Al-26 Distribution, Radioactive Ion Beam, Al-25, 25Al, Rapid Proton Process, rp-process, Classical Nova, Core Collapse Supernova, Nova, Supernova === Includes bibliographical references. === Ingo Wiedenhöver, Professor Directing Dissertation; Henry Fuelberg, Outside Committee Member; Alexander Volya, Committee Member; Grigory Rogachev, Committee Member; Peter Höflich, Committee Member. |
author2 |
Peplowski, Patrick N. (Patrick Nelson), 1981- (authoraut) |
author_facet |
Peplowski, Patrick N. (Patrick Nelson), 1981- (authoraut) |
title |
The Lowest ℓ = 0 Proton Resonance in Si-26 and Its Implications for the Stellar Nucleosynthesis of Al-26. |
title_short |
The Lowest ℓ = 0 Proton Resonance in Si-26 and Its Implications for the Stellar Nucleosynthesis of Al-26. |
title_full |
The Lowest ℓ = 0 Proton Resonance in Si-26 and Its Implications for the Stellar Nucleosynthesis of Al-26. |
title_fullStr |
The Lowest ℓ = 0 Proton Resonance in Si-26 and Its Implications for the Stellar Nucleosynthesis of Al-26. |
title_full_unstemmed |
The Lowest ℓ = 0 Proton Resonance in Si-26 and Its Implications for the Stellar Nucleosynthesis of Al-26. |
title_sort |
lowest ℓ = 0 proton resonance in si-26 and its implications for the stellar nucleosynthesis of al-26. |
publisher |
Florida State University |
url |
http://purl.flvc.org/fsu/fd/FSU_migr_etd-2032 |
_version_ |
1719318271929352192 |