physics 133: extragalactic astronomy ad cosmology lecture 5; january 22 2014
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Physics 133: Extragalactic Astronomy ad Cosmology
Lecture 5; January 22 2014
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Previously
• The universe is a 4 dimensional manifold as in General Relativity
• The universe is homogeneous and isotropic• This implies that space and time can be “separated” so that
we can define a cosmic time t• There are only three possible geometries for the universe.
Their metric is the Robertson-Walker metric• In the RW non-static universe redshift is a measure of
distance.• The dynamics of the Universe is described by Friedmann
Equation; Newtonian analog.
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Outline:
Dynamics of the Universe:– Friedmann Equation– Fluid Equation– Acceleration Equation– Equation of State– Cosmological Constant
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Dynamics of the Universe. Friedmann Equation
• Limitations of Newtonian analog:
– Newtonian– What’s outside the
sphere?– Inhomogeneous. Isotropic
• Friedmann Equation (1922) is the correct form with energy instead of mass and curvature instead of internal energy [Blackboard]
1888 - 1925
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Dynamics of the Universe. “Fluid” equation
• We have 1 equation and two functions a(t) and ε(t)
• What is the connection between the two?
• Adiabatic expansion• [Black board]
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Dynamics of the Universe. Acceleration equation
• Another convenient form (not independent) is the equation of motion with the second derivative
• [Black board]• Examples of
Equation of state [blackboard]
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Fate of the universe in curvature + mass models
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The cosmological constant
• Soon after the completion of general relativity (1916) people used it to describe the universe.
• However, with only matter there was no way to obtain a static solution, which at that time was the prejudice.
• Einstein added the cosmological constant to his equations to find a static solution…
• [Blackboard]
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The cosmological constant
• Unfortunately the static solution is unstable
• And, when Hubble announced his discovery of the expansion, unnecessary
• So the cosmological constant remained on the outskirts of cosmology for a long time…
• Now it’s back!
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Cosmological constant or dark energy?
• Nowadays people prefer to talk in terms of dark energy, instead of cosmological constant.
• The classic cosmological constant is a modification of Einstein’s equation [Black board]
• Dark energy is interpreted as something with negative pressure filling space
• Is it some sort of vacuum energy?
• We really don’t know…
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Dynamics of the Universe. Summary
• Friedmann Equation describes the evolution of a(t) depending on content and geometry of the universe.
• Fluid equations describe the evolution of the content of the universe with a(t).
• The cosmological constant or dark energy is an extra term in Friedmann Equation and can induce acceleration. Currently supported by observations.
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The End
See you on monday!