Bubble Nucleation and Eternal Inflation - cosmo 06

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Slow-Roll Eternal Inflation Driven by large V or small V’: Condition for eternal inflation: V m 2 pV ′2/3 > 1 Jump in a Hubble volume over a Hubble time: (Coarse-graining) δφ = H 2π
Slow-Roll Eternal Inflation Concentrate on large V: V f V i
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Bubble Nucleation and Eternal Infla
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nton is cut along the surface denot
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to the hypersurface indicated in th
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Page 15 and 16: Vacuum Bubbles 3 Ingredients for Cl
Page 17 and 18: Schwarzschild-de Sitter Future null
Page 19 and 20: Schwarzschild-de Sitter Continues f
Page 21 and 22: Require metric continuity across bo
Page 23 and 24: Allowed Spacetimes II II II'' r BH
Page 25 and 26: Allowed Spacetimes II II II'' r BH
Page 27 and 28: orals - p.14/41 Got Tunneling Got T
Page 29 and 30: =0 C r III’’ III I C III’’
Page 31 and 32: =0 Zero Mass Limit: III IV L Geomet
Page 33 and 34: Zero Mass Limit: FIG. 11: Tunneling
Page 35 and 36: Zero Mass Limit: FIG. 11: Tunneling
Page 37 and 38: dS to Bubble Spacetime IV IV’’
Page 39 and 40: dS to Bubble Spacetime IV IV’’
Page 41 and 42: Tunneling There are many possible t
Page 47 and 48: would be a ple, if the fact forbidw
Page 49 and 50: Nucleation Probability Zero mass li
Page 51 and 52: Nucleation Probability CDL Bubbles
Page 53 and 54: Measures for Eternal Inflation We n
Page 55 and 56: Comoving Volume Weighting • Weigh
Page 57 and 58: Comoving Volume Weighting • Weigh
Page 59 and 60: L+R Geometries
Page 61 and 62: L+R Geometries Behind the wormhole.
Page 63 and 64: L+R Geometries Behind the wormhole.
Page 65: Adjusted Measure • Initial comovi
Page 69 and 70: Slow-Roll Eternal Inflation Concent
Page 71: Conclusions • There are a variety
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Bubble Nucleation and Eternal Inflation - cosmo 06

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