8 286 le ture 9 o tober 10 2018 dynamics of homogeneous
play

8.286 Leture 9 Otober 10, 2018 DYNAMICS OF HOMOGENEOUS - PowerPoint PPT Presentation

8.286 Leture 9 Otober 10, 2018 DYNAMICS OF HOMOGENEOUS EXPANSION, PART IV Summary of Leture 8 Age of a Flat Matter-Dominated Universe: 2 2 = 3 1 a ( t ) / = ) = t t H 3 1 1 F or = 67 : 7 0 : 5


  1. 8.286 Le ture 9 O tober 10, 2018 DYNAMICS OF HOMOGENEOUS EXPANSION, PART IV

  2. Summary of Le ture 8 Age of a Flat Matter-Dominated Universe: 2 2 = 3 � 1 a ( t ) / = ) = t t H 3 � 1 � 1 F or = 67 : 7 � 0 : 5 km-s -Mp , age = 9.56 { 9.70 billion H y ears | but stars are older. Con lusion: our univ erse is nearly �at, but not matter-dominated. a (0) = 0, with in�nite densit y , is a The Big Bang Singularity: feature of our mo del, but not ne essarily the real univ erse. Alan Guth Massa husetts Institute of T e hnology {1{ 8.286 Le ture 9, O tober 10, 2018

  3. Summary of Le ture 8 Age of a Flat Matter-Dominated Universe: 2 2 = 3 � 1 a ( t ) / = ) = t t H 3 � 1 � 1 F or = 67 : 7 � 0 : 5 km-s -Mp , age = 9.56 { 9.70 billion H y ears | but stars are older. Con lusion: our univ erse is nearly �at, but not matter-dominated. a (0) = 0, with in�nite densit y , is a The Big Bang Singularity: feature of our mo del, but not ne essarily the real univ erse. Alan Guth Massa husetts Institute of T e hnology {1{ 8.286 Le ture 9, O tober 10, 2018

  4. the presen t distan e of the furthest parti les Horizon Distan e: from whi h ligh t has had time to rea h us. t Z 0 ( t ) = a ( t ) d t ` : ys ; horizon ph a ( t ) 0 0 2 = 3 � 1 a ( t ) / = ) = 3 t = 2 H t ` : ys ; horizon ph Alan Guth Massa husetts Institute of T e hnology {2{ 8.286 Le ture 9, O tober 10, 2018

  5. Equations for a Matter-Dominated Universe (\Matter-dominated" = dominated b y nonrelativist i matter.) F riedmann equations: 2 2 a _ 8 � k 8 9 = G� ; � > > : ; a 3 a 2 4 � � a = G� ( t ) a : � 3 Matter onserv ation: 3 1 � a ( t ) � 1 � ( t ) ; or � ( t ) = � ( t ) for an y t . / 1 1 a 3 ( t ) a ( t ) An y t w o of the ab o v e equations an allo w us to �nd the third. Alan Guth Massa husetts Institute of T e hnology {3{ 8.286 Le ture 9, O tober 10, 2018

  6. Evolution of a Closed Universe 2 2 � a _ � 8 � k 3 = G� ; � ( t ) a ( t ) = onstan t ; k > 0 : � a 3 a 2 2 Re all [ a ( t )℄ = meter/not h, [ k ℄ = 1/not h . De�ne new v ariables: a ( t ) ~ a ( t ) ~ ; t t (b oth with units of distan e) p � � k 2 2 Multiplyi ng F riedmann eq b y a = ( k ): 2 2 1 � da � 8 � G�a = 1 : � k dt 3 k 2 2 Alan Guth Massa husetts Institute of T e hnology {4{ 8.286 Le ture 9, O tober 10, 2018

  7. 2 2 1 � da � 8 � G�a = 1 � k 2 dt 3 k 2 (4 : 15) p 3 8 � G�a k = 1 : � 3 = 2 3 k 2 a Rewrite as 2 � d ~ a � 2 � = 1 ; � ~ a ~ d t where 3 4 � G� ~ a � : � 3 2 2 [ � ℄ = meter. � is onstan t, sin e �a is onstan t. Alan Guth Massa husetts Institute of T e hnology {5{ 8.286 Le ture 9, O tober 10, 2018

  8. 2 � � ~ 2 � ~ ~ d a a d a ~ p = � 1 = ) = d t : ~ ~ a d t 2 2 � ~ � ~ a a Then ~ t a ~ ~ ~ Z Z a d a f f ~ ~ p = = t d t ; f 2 2 � ~ � ~ a a 0 0 ~ where is an arbitrary hoi e for a \�nal time" for the al ulation, t f ~ and ~ is the v alue of ~ at time . a a t f f Alan Guth Massa husetts Institute of T e hnology {6{ 8.286 Le ture 9, O tober 10, 2018

  9. Evolution of a Closed Universe = � ( � � sin ) t � ; a p = � (1 � os ) � : k p p � � � � � 2 � � 1 2 � � 1 = ar sin � � t : 3 = 2 2 j H j (� � 1) � � Alan Guth Massa husetts Institute of T e hnology {7{ 8.286 Le ture 9, O tober 10, 2018

  10. {8{

  11. Evolution of a Closed Universe = � ( � � sin ) t � ; a p = � (1 � os ) � : k p p � � � � � 2 � � 1 2 � � 1 = ar sin � � t : 3 = 2 2 j H j (� � 1) � � Alan Guth Massa husetts Institute of T e hnology {9{ 8.286 Le ture 9, O tober 10, 2018

  12. Evolution of a Closed Universe = � ( � � sin ) t � ; a p = � (1 � os ) � : k p p � � � � � 2 � � 1 2 � � 1 = ar sin � � t : 3 = 2 2 j H j (� � 1) � � Alan Guth Massa husetts Institute of T e hnology {9{ 8.286 Le ture 9, O tober 10, 2018

  13. p p � � � � � 2 � � 1 2 � � 1 = ar sin � � t : 3 = 2 2 j H j (� � 1) � � � 1 Quadran t Phase � Sign Choi e sin () � 1 Expanding 1 to 2 Upp er 0 to 2 � 2 Expanding 2 to 1 Upp er to � 2 3 � 3 Con tra ting 1 to 2 Lo w er to � 2 3 � 4 Con tra ting 2 to 1 Lo w er to 2 � 2 Alan Guth Massa husetts Institute of T e hnology {10{ 8.286 Le ture 9, O tober 10, 2018

  14. Alan Guth Massa husetts Institute of T e hnology {11{ 8.286 Le ture 9, O tober 10, 2018

  15. Alan Guth Massa husetts Institute of T e hnology {12{ 8.286 Le ture 9, O tober 10, 2018

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend