1.77k likes | 1.9k Views
Inflation, infinity, equilibrium and the observable Universe Andreas Albrecht UC Davis UCD Colloquium October 3, 2011. E. Cosmic Inflation: Great phenomenology, but
E N D
Inflation, infinity, equilibrium and the observable Universe Andreas Albrecht UC Davis UCD Colloquium October 3, 2011 A. Albrecht @ UCD 10/3/11
Cosmic Inflation: • Great phenomenology, but • Original goal of explaining why the cosmos is *likely* to take the form we observe has proven very difficult to realize. A. Albrecht @ UCD 10/3/11
Cosmic Inflation: • Great phenomenology, but • Original goal of explaining why the cosmos is *likely* to take the form we observe has proven very difficult to realize. This Talk A. Albrecht @ UCD 10/3/11
Cosmic Inflation: • Great phenomenology, but • Original goal of explaining why the cosmos is *likely* to take the form we observe has proven very difficult to realize. • OR: Just be happy we have equations to solve? A. Albrecht @ UCD 10/3/11
OUTLINE Big Bang & inflation basics Eternal inflation de Sitter Equilibrium cosmology Cosmic curvature from de Sitter Equilibrium cosmology A. Albrecht @ UCD 10/3/11
OUTLINE Big Bang & inflation basics Eternal inflation de Sitter Equilibrium cosmology Cosmic curvature from de Sitter Equilibrium cosmology A. Albrecht @ UCD 10/3/11
Friedmann Eqn. A. Albrecht @ UCD 10/3/11
Friedmann Eqn. Curvature A. Albrecht @ UCD 10/3/11
Friedmann Eqn. Curvature Relativistic Matter A. Albrecht @ UCD 10/3/11
Friedmann Eqn. Curvature Non-relativistic Matter Relativistic Matter A. Albrecht @ UCD 10/3/11
Friedmann Eqn. Dark Energy Curvature Non-relativistic Matter Relativistic Matter A. Albrecht @ UCD 10/3/11
The curvature feature/“problem” A. Albrecht @ UCD 10/3/11
The curvature feature/“problem” ! A. Albrecht @ UCD 10/3/11
The curvature feature/“problem” ! A. Albrecht @ UCD 10/3/11
The curvature feature/“problem” ! A. Albrecht @ UCD 10/3/11
The curvature feature/“problem” A. Albrecht @ UCD 10/3/11
The curvature feature/“problem” ! A. Albrecht @ UCD 10/3/11
The monopole “problem” A. Albrecht @ UCD 10/3/11
The monopole “problem” ! A. Albrecht @ UCD 10/3/11
Friedmann Eqn. Dark Energy Curvature Non-relativistic Matter Relativistic Matter A. Albrecht @ UCD 10/3/11
Now add cosmic inflation Friedmann Eqn. Dark Energy Inflaton Curvature Non-relativistic Matter Relativistic Matter A. Albrecht @ UCD 10/3/11
Now add cosmic inflation Friedmann Eqn. Dark Energy Inflaton Curvature Non-relativistic Matter Relativistic Matter A. Albrecht @ UCD 10/3/11
The inflaton: ~Homogeneous scalar field obeying Cosmic damping Coupling to ordinary matter All potentials have a “low roll” (overdamped) regime where A. Albrecht @ UCD 10/3/11
The inflaton: ~Homogeneous scalar field obeying Cosmic damping Coupling to ordinary matter All potentials have a “low roll” (overdamped) regime where A. Albrecht @ UCD 10/3/11
Add a period of Inflation: A. Albrecht @ UCD 10/3/11
With inflation, initially large curvature is OK: A. Albrecht @ UCD 10/3/11
With inflation, early production of large amounts of non-relativistic matter (monopoles) is ok : A. Albrecht @ UCD 10/3/11
Inflation detail: A. Albrecht @ UCD 10/3/11
Inflation detail: A. Albrecht @ UCD 10/3/11
Hubble Length A. Albrecht @ UCD 10/3/11
Hubble Length (aka ) A. Albrecht @ UCD 10/3/11
End of inflation A. Albrecht @ UCD 10/3/11
End of reheating A. Albrecht @ UCD 10/3/11