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Talk53 min

Cosmological fluctuations and conservation laws

Steven Weinberg · CERN

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About

In order to use observations of the anisotropy and polarization of the cosmic microwave background to learn about inflation, it is necessary to rely on conservation laws that apply outside the horizon. The general conservation law for both scalar and tensor modes is derived as a version of Goldstone's theorem. The damping of tensor modes after they re-enter the horizon is calculated..

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The talk

  1. Cosmological fluctuations and conservation laws 2003-09-15 · 53 min · CERN's player

Credits and licence

Institution
CERN
Department
CERN Miscellaneous Lectures
Speaker
Steven Weinberg
Year
2003
Language
English
Source
CERN
Licence
CERN, as CERN states it. CERN's terms
Attribution
© CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
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