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שיעור 11 מבוא לקוסמולוגיה
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Observational facts Density contrast at small scales
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Anisotropy at small scales
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Homogeneity and isotropy at large scales Homogeneity and isotropy at large scales
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Olbers’ paradox Why the sky is dark ? Olbers’ paradox Why the sky is dark ?
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Hubble expansion 1929 redshift
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1996
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Expanding space
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Distance: coordinates and proper distances Distance: coordinates and proper distances
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Lookback time
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Looking into past Looking into past
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Curvature
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Cosmological resdshift Cosmological resdshift
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Cosmological change of angular size Cosmological change of angular size
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Horizons
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Test particle
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Friedmann’s equations
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Deceleration parameter and critical density Deceleration parameter and critical density
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How parameters depend on a ?
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