Arşiv ve Dokümantasyon Merkezi
Dijital Arşivi

Solar axion production and detection mechanisms

Basit öğe kaydını göster

dc.contributor Graduate Program in Physics.
dc.contributor.advisor Arık, Metin.
dc.contributor.author Özuğurel, Umut Deniz.
dc.date.accessioned 2023-03-16T10:38:05Z
dc.date.available 2023-03-16T10:38:05Z
dc.date.issued 2009.
dc.identifier.other PHYS 2009 O88
dc.identifier.uri http://digitalarchive.boun.edu.tr/handle/123456789/13704
dc.description.abstract Production mechanisms of the axion particle in the Sun as well as the detection principle and the data analysis methods that the CAST experiment is based on are reviewed. It is shown that the solar axion production can be explained both by the Primako e ect with a reduced decay width due to plasma screening e ects and by the electromagnetic plasma excitations up to a momentum limit. The analysis of CAST data which results in an upper limit on the axion-photon coupling constant for a range of axion mass is explained in connection with the solar axion ux and the detection principle. Additionally, technical details about CAST is given. Finally, a survey on data collected during the rst part of the second phase of CAST is presented.
dc.format.extent 30cm.
dc.publisher Thesis (M.S.)-Bogazici University. Institute for Graduate Studies in Science and Engineering, 2009.
dc.relation Includes appendices.
dc.relation Includes appendices.
dc.subject.lcsh Axions.
dc.title Solar axion production and detection mechanisms
dc.format.pages xii, 53 leaves;


Bu öğenin dosyaları

Bu öğe aşağıdaki koleksiyon(lar)da görünmektedir.

Basit öğe kaydını göster

Dijital Arşivde Ara


Göz at

Hesabım