Perfect Cosmological Principle

The Perfect Cosmological Principle states that the Universe is homogeneous and isotropic in space and time. In this view the universe looks the same everywhere (on the large scale), the same as it always has and always will. It is the principle underpinning steady-state theory and emerging from Chaotic inflation theory.[1][2][3]

The Perfect Cosmological Principle is an extension of the Cosmological Principle, which asserts that the universe changes its gross feature with time, but not across space.

See also

References

  1. ↑ Aguirre, Anthony & Gratton, Steven (2003). "Inflation without a beginning: A null boundary proposal". Phys. Rev. D. 67. arXiv:gr-qc/0301042Freely accessible. Bibcode:2003PhRvD..67h3515A. doi:10.1103/PhysRevD.67.083515.
  2. ↑ Aguirre, Anthony & Gratton, Steven (2002). "Steady-State Eternal Inflation". Phys. Rev. D. 65. arXiv:astro-ph/0111191Freely accessible. Bibcode:2002PhRvD..65h3507A. doi:10.1103/PhysRevD.65.083507.
  3. ↑ Gribbin, John. "Inflation for Beginners".


This article is issued from Wikipedia - version of the 3/7/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.