Tanelorn said:
Thanks Marcus for clarifying the distinction, I was not aware of that. Both the collapse leading to rebound (to a new U?) and Smolin's theory have a certain elegance, not that that means anything of course.
I would be very interested in learning how well this, and other speculative theories are accepted. Perhaps some kind of a ratings system amongst Cosmologists would help part timers know which one theories to take more seriously?
If I were a professional cosmologist, doing research, I would take those theories seriously which were relevant to my specialty, and had not been disproven. If I was not studying the very start of expansion and how we can learn about it, I would not bother to make a serious evaluation.
I would not be interested in
answering the "big questions" I would focus on ideas that had a bearing on my research specialty.
So, for researchers with a legitimate interest in
bounce cosmology or in NONSINGULAR cosmology generally (where there is something besides a "singularity" at the start of expansion) there are special sessions at the international conferences where they can get together and present their papers and discuss, and there are REVIEW articles that survey the different models and approaches to modeling the start of expansion (and the conditions preceding and around that).
I don't think I can give you any guidance about what YOU PERSONALLY should "take seriously" or not. If you were doing research in some type of bounce cosmology, you could publish in peer review professional journals on the same basis as other mainstream research--i.e if the quality met standards.
You could deliver your papers at mainstream international conferences, at the appropriate parallel sessions, on the same basis as other--i.e if your research was up to standard. You could find other bounce cosmology specialists to argue with, about your various different approaches, and so on.
But if you are not already involved I don't see any basis on which I could advise you. Why should anybody be more interested in this line of cosmology research than in, say inflation theories, or CmB interpretation, or galaxy-redshift counts as a key to structure, or dark matter distribution, or galaxy formation(!), or ages of star populations,...?
Personally I find the mainstream research classified as "quantum cosmology" (which for the most part is quantum bounce cosmology) intensely fascinating--so I follow it with fairly close attention even though I have no career interest (I'm retired.)
I'll get you a link to the QC papers since 2009, ranked by number of citation (a rough measure of importance in the QC category) to satisfy any curiosity, you can read the titles of the papers and sample abstracts here and there if you wish.
But I cannot advise you. It would be extremely pretentious of someone to say "do be interested" or "don't be interested", fatuous even.
You are or you aren't. If someone is, and is able to read the technical literature, I can suggest papers.
I'll get that QC link. It is to the Stanford-SLAC research data base, using keyword "quantum cosmology"
This is "quantum cosmology" since 2009, Inspire search:
http://inspirehep.net/search?ln=en&ln=en&p= "quantum cosmology" and NOT d 1900->2008&of=hb&action_search=Search&sf=&so=d&rm=citation&rg=25&sc=0 (750 found as of 30 Nov 2014)
You can see the QC research output is on the order of 10 papers per month, roughly 120 per year.
I checked and roughly half are in the Loop QG approach and the other half are in various other approaches to quantum gravity and quantum cosmology. And I see no compelling reason to take such details (of rates and percentages) seriously as if they indicated something with longterm validity or relevance. Before year 2000 the Loop QG annual share was roughly zero, now it is 50%, other approaches percentage shares have changed as well during that time.. Research emphasis changes.
Researcher interest shifts.