Newtonian Cosmology

dc.contributor.advisorÖvgün, Ali
dc.contributor.authorZebari, Hamza Saber Saeed
dc.date.accessioned2021-11-08T07:23:14Z
dc.date.available2021-11-08T07:23:14Z
dc.date.issued2020
dc.date.submitted2020-01
dc.departmentEastern Mediterranean University, Faculty of Arts and Sciences, Dept. of Physicsen_US
dc.descriptionMaster of Science in Physics. Thesis (M.S.)--Eastern Mediterranean University, Faculty of Arts and Sciences, Dept. of Physics, 2020. Supervisor: Assist. Prof. Dr. Ali Övgün.en_US
dc.description.abstractIn this work, we have used the Friedmann equation of general relativity with quantum correction terms to the Newtonian potential to obtain the modified Friedmann equation with quantum correction. The behavior of the solution is examined with a sign of the correction being put into consideration. With the correction, the singular and non-singular universe is clearly spelled out. The results reveal that the quantum correction effect depends on the sign in the correction. Applying cosmological constant to the modified Friedmann Equation, we found out that the scale factor of the universe is given by the first order in the expression of We also compare the Friedmann Equations with Loop Quantum Gravity (LQG) to the Friedmann Equation with quantum correction and found out that, for negative the critical density is not feasible but it is feasible for positive values . Keywords: Cosmology, quantum cosmology, Cosmological constant, Quantum bounce, Radiation universe, Dust universe.en_US
dc.description.abstractÖZ: Bu çalışmada, modifiye Friedmann denklemini kuantum düzeltmesi ile elde etmek için genel göreliliğin Friedmann denklemini kuantum düzeltme terimi ile Newton potansiyeline kullandık. Çözümün davranışı, dikkate alınan düzeltmenin işareti ile incelenir. Düzeltme ile, tekil ve tekil olmayan evren açıkça dile getirilir. Sonuçlar, kuantum düzeltme etkisinin düzeltme işaretine bağlı olduğunu göstermektedir. Modifiye edilmiş Friedmann Denklemine kozmolojik sabit uygulayarak, evrenin ölçek faktörünün τ ifadesinde ilk derece ϵ tarafından verildiğini öğrendik. Ayrıca, Döngü Kuantum Yerçekimi (LQG) ile Friedmann Denklemlerini kuantum düzeltmesi ile Friedmann Denklemi ile karşılaştırdık ve negatif için kritik yoğunluğun mümkün olmadığını, ancak pozitif değerler için mümkün olduğunu öğrendik . Anahtar Kelimeler: Kozmoloji, kuantum kozmolojisi, Kozmolojik sabit, Kuantum sıçraması, Radyasyon evreni, Toz evren.en_US
dc.identifier.citationZebari, Hamza Saber Saeed. (2020). Newtonian Cosmology. Thesis (M.S.), Eastern Mediterranean University, Institute of Graduate Studies and Research, Dept. of Physics, Famagusta: North Cyprus.en_US
dc.identifier.urihttps://hdl.handle.net/11129/5167
dc.language.isoen
dc.publisherEastern Mediterranean University (EMU) - Doğu Akdeniz Üniversitesi (DAÜ)en_US
dc.relation.publicationcategoryTez
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectPhysicsen_US
dc.subjectCosmologyen_US
dc.subjectCosmologyen_US
dc.subjectquantum cosmologyen_US
dc.subjectCosmological constanten_US
dc.subjectQuantum bounceen_US
dc.subjectRadiation universeen_US
dc.subjectDust universeen_US
dc.titleNewtonian Cosmologyen_US
dc.typeMaster Thesis

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