Introduction to Big Bang Cosmology - ETH Z ... in shape and intensity. T = 2.736 K RW metric â€œexplainsâ€‌ Documents

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ΤΙΤΛΟΣ ΒΙΒΛΙΟΥ: Το κορίτσι απ’ τη Σαµψούντα ΣΥΓΓΡΑΦΕΑΣ: Σόφη Θεοδωρίδου ΕΠΙΜΕΛΕΙΑ – ∆ΙΟΡΘΩΣΗ…

Lecture 14: Cosmology Olbers’ Paradoxtjp/ItA/ita14.pdf · The Hot Big Bang model If the universe is expanding, then it follows that by going back in time, we move towards a moment Documents

1 Lecture 14: Cosmology •  Olbers’ paradox •  Redshift and the expansion of the Universe •  The Cosmological Principle •  Ω0 and the curvature of space…

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