Talk:Loop quantum cosmology

Boasty style

 * LQC has led to many successes, including the emergence of a possible mechanism for cosmic inflation, resolution of gravitational singularities as well as development of effective, semi-classical Hamiltonians.

What kind of "resolution" of gravitational singularities? Why is the emergence of a possible mechanism for X a success? What does Hamiltonians have to do with cosmology, and why is semi-classical Hamiltonians a success compared to classical Hamiltonians? Etc. etc.. The text needs explanations. It currently only makes boasts about things it can do, if those things are really good... ... said: Rursus ( m bork³ ) 22:31, 5 October 2009 (UTC)

LQC has no infinite density, no infinite curvature - no big bang a la GR. Singularity resolved - physics never encounters one. Semi-classical hamiltonians are vital to incorporate quantum effects, and Hamiltonian cosmology is a well established way of expressing classical GR cosmology. 71.58.102.7 (talk) 02:49, 9 February 2010 (UTC)

'loop quantum cosmology' should be merged with 'loop quantum gravity' because they are almost the same thing Qtom.masters (talk) 06:17, 13 December 2011 (UTC)

External links modified
Hello fellow Wikipedians,

I have just modified one external link on Loop quantum cosmology. Please take a moment to review my edit. If you have any questions, or need the bot to ignore the links, or the page altogether, please visit this simple FaQ for additional information. I made the following changes:
 * Added archive https://web.archive.org/web/20070629122851/http://hermes.aei.mpg.de/lrr/2005/11/article.xhtml to http://hermes.aei.mpg.de/lrr/2005/11/article.xhtml

When you have finished reviewing my changes, you may follow the instructions on the template below to fix any issues with the URLs.

Cheers.— InternetArchiveBot  (Report bug) 02:16, 6 January 2018 (UTC)