Cosmology Lecture 10
Δημοσιεύτηκε στις 5 Απρ 2013
(March 18, 2013) Leonard Susskind
discusses the inhomogeneities in the cosmic microwave background, and
derives the current theory whereby these inhomogeneities are created by
quantum fluctuations in the inflaton field of the early universe. These
fluctuations lead to variations in energy density that ultimately
result in the formation of galaxies.
Originally presented in the Stanford Continuing Studies Program.
Stanford University:
http://www.stanford.edu/
Continuing Studies Program:
http://csp.stanford.edu/
Stanford University Channel on YouTube:
http://www.youtube.com/stanford
discusses the inhomogeneities in the cosmic microwave background, and
derives the current theory whereby these inhomogeneities are created by
quantum fluctuations in the inflaton field of the early universe. These
fluctuations lead to variations in energy density that ultimately
result in the formation of galaxies.
Originally presented in the Stanford Continuing Studies Program.
Stanford University:
http://www.stanford.edu/
Continuing Studies Program:
http://csp.stanford.edu/
Stanford University Channel on YouTube:
http://www.youtube.com/stanford
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