A Lagrangian formulation of a theory of a scalar field superfluid dark matter

dc.contributor.advisorLarena, Julien
dc.contributor.advisorOsano, Bob
dc.contributor.authorTema, Seturumane
dc.date.accessioned2023-03-13T09:54:33Z
dc.date.available2023-03-13T09:54:33Z
dc.date.issued2022
dc.date.updated2023-02-21T07:23:02Z
dc.description.abstractIn this thesis we discuss the dynamics of the relativistic Lagrangian of the theory of dark matter superfluidity. The second and third chapters of the thesis are a review. In the fourth chapter we show that a complex scalar field whose dynamics are dictated by such a Lagrangian, models dust in the background universe on cosmological scale. Prior to our calculations, the theory was shown to model dust on cosmological scale and a superfluid on galactic scale in the non-relativistic case [1]. This project, extends the non-relativistic theory, to include the relativistic background. We continued, using the relativistic Lagrangian, to investigate how perturbations of such a theory grow in a perturbed universe, and found that the density contrast (of the theory) is constant when the complex scalar field is not coupled to baryons in the weak-field limit.
dc.identifier.apacitationTema, S. (2022). <i>A Lagrangian formulation of a theory of a scalar field superfluid dark matter</i>. (). ,Faculty of Science ,Department of Mathematics and Applied Mathematics. Retrieved from http://hdl.handle.net/11427/37371en_ZA
dc.identifier.chicagocitationTema, Seturumane. <i>"A Lagrangian formulation of a theory of a scalar field superfluid dark matter."</i> ., ,Faculty of Science ,Department of Mathematics and Applied Mathematics, 2022. http://hdl.handle.net/11427/37371en_ZA
dc.identifier.citationTema, S. 2022. A Lagrangian formulation of a theory of a scalar field superfluid dark matter. . ,Faculty of Science ,Department of Mathematics and Applied Mathematics. http://hdl.handle.net/11427/37371en_ZA
dc.identifier.ris TY - Master Thesis AU - Tema, Seturumane AB - In this thesis we discuss the dynamics of the relativistic Lagrangian of the theory of dark matter superfluidity. The second and third chapters of the thesis are a review. In the fourth chapter we show that a complex scalar field whose dynamics are dictated by such a Lagrangian, models dust in the background universe on cosmological scale. Prior to our calculations, the theory was shown to model dust on cosmological scale and a superfluid on galactic scale in the non-relativistic case [1]. This project, extends the non-relativistic theory, to include the relativistic background. We continued, using the relativistic Lagrangian, to investigate how perturbations of such a theory grow in a perturbed universe, and found that the density contrast (of the theory) is constant when the complex scalar field is not coupled to baryons in the weak-field limit. DA - 2022_ DB - OpenUCT DP - University of Cape Town KW - Maths and Applied Mathematics LK - https://open.uct.ac.za PY - 2022 T1 - A Lagrangian formulation of a theory of a scalar field superfluid dark matter TI - A Lagrangian formulation of a theory of a scalar field superfluid dark matter UR - http://hdl.handle.net/11427/37371 ER - en_ZA
dc.identifier.urihttp://hdl.handle.net/11427/37371
dc.identifier.vancouvercitationTema S. A Lagrangian formulation of a theory of a scalar field superfluid dark matter. []. ,Faculty of Science ,Department of Mathematics and Applied Mathematics, 2022 [cited yyyy month dd]. Available from: http://hdl.handle.net/11427/37371en_ZA
dc.language.rfc3066eng
dc.publisher.departmentDepartment of Mathematics and Applied Mathematics
dc.publisher.facultyFaculty of Science
dc.subjectMaths and Applied Mathematics
dc.titleA Lagrangian formulation of a theory of a scalar field superfluid dark matter
dc.typeMaster Thesis
dc.type.qualificationlevelMasters
dc.type.qualificationlevelMSc
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