This is a graduate seminar that uses general relativity as a working language for cosmology, treating Einstein's equations less as a finished theory and more as a flexible framework you can stretch — into FLRW spacetimes, inflation, and modified gravity like f(R). You'll review the geometric machinery (Killing vectors, the gravitational action, the energy-momentum tensor), then spend most of the term building and solving cosmological models, with regular homework and two midterms keeping the calculations honest. It sits at the interface where differential geometry, PDE symmetry methods, and observational cosmology meet, and is the natural launching point if you want to do research in gravitation or theoretical cosmology.
→ STARS müfredatı (resmi syllabus)
İlk dosyayı sen atarsan — not, slayt, geçmiş sınav, çözüm, cheat-sheet, ne varsa — defter ekibi öğrenci paylaşımlarından bu dersin notlarını yazar. Drive linki / PDF / ZIP, hepsi olur.
Course Learning Outcomes: Course Learning Outcome Assessment Identify and classify the symmetries of differential equations Midterm:Essay/written Final:Essay/written Homework Apply symmetries to produce solutions of partial differential equations Midterm:Essay/written Final:Essay/written Homework Analyze and interpret the group invariant solutions of the partial differential equations Midterm:Essay/written Final:Essay/written Homework