Neutron Stars and Black Holes Lecture - 14: Universe or Multiverse?!
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Universe or Multiverse?!
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What have we learn about our universe during last
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Our Universe is expanding
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The present expansion rate
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Age of the Universe
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The Universe is not only expanding,it is Accelerating!
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Geometry of the universe is Euclidean
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The geometry of the Universe
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Critical density
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The Energy-Density Budget of the Universe
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The Present Revolution in Astronomy
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A Singularity Theorem
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Some troubling things about our universe
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The "Horizon" problem
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Isotropy of the Cosmic Microwave Background
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At t~10-36 sec
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At Planck time =10-43 sec, the size of the universe exceeded the causality scale by 10 power 28
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The "Flatness" problem
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How to fix the Horizon Problem
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Why would the early universe expand exponentially?
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Inflationary Universe
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The "Heavy Nothing" or Vacuum Energy
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Matter & Radiation exert positive pressure
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Vacuum exerts negative pressure!
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Exponential Expansion
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An initial exponential expansion
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Ingredient of Inflation
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Unification of forces Cosmological Phase Transitions
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Symmetry Breaking and Phase Transitions
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Landau's theory of second order transition
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First order Phase Transition
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Supercooling and Superheating
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Nucleation during transition
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Cosmological Phase Transitions
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Symmetry Breaking and Phase Transitions
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Gauge Symmetry
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Gauge Theories of elementary particles
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Vacuum Driven Acceleration
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Exponential Expansion
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A curved surface expands by a factor of 3 in each panel.
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But there are problems!
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The initial hope was not to be!
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'New' Inflation
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Slow Roll Inflation
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New Inflation - a summary
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Inflation: underlying assumptions
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Chaotic Inflation
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Robertson-Walker Universe
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The essence of Chaotic Inflation
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Inflation is generic!
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Eternal Inflation
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Multiverses
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Was there a beginning?
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History in "Imaginary time"
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Cycles of time
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Wrap Up
Description:
Explore the fascinating realm of cosmology in this comprehensive lecture on the universe and multiverse theories. Delve into key concepts like the expanding universe, cosmic microwave background, and the age of the universe. Examine troubling aspects such as the horizon and flatness problems, and discover how inflationary theory attempts to resolve these issues. Learn about cosmological phase transitions, symmetry breaking, and gauge theories of elementary particles. Investigate various inflationary models, including chaotic and eternal inflation, and their implications for the multiverse concept. Contemplate profound questions about the beginning of the universe and alternative cosmological models like cyclic universes. Gain a deeper understanding of cutting-edge ideas in theoretical physics and cosmology through this engaging 2-hour lecture by G. Srinivasan from the Raman Research Institute.
Universe or Multiverse? - Neutron Stars and Black Holes Lecture 14