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Astonomy 62 Lecture #37t 0≡ NOWr(t) = radius of theexpanding sphericalshellv(t) = expansion velocity ofthe shell(t) = density of mattercontained inside theshellExpandingShellmrv

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Astonomy 62 Lecture #37t 0≡ NOWr(t) = radius of theexpanding sphericalshellv(t) = expansion velocity ofthe shell(t) = density of mattercontained inside theshellExpandingShellmrv

Density Energy Dynamics GeometryE = 0(Criticallybound)Expandsforeverwithv 0E < 0(Bound)Eventuallyre-collapsesE > 0(Unbound)Expandsforeverwithv 0

Page 1 and 2: Astonomy 62 Lecture #37Last TimeAct
Page 3: Astonomy 62 Lecture #37Cosmological
Page 7 and 8: Density Energy Dynamics Geometry=1E
Page 9 and 10: Astonomy 62 Lecture #37Closed1Flat=
Page 11 and 12: Data from Type Ia High-Redshift Sup
Page 13 and 14: =0 empty

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