The structural formation and baryonic fluctutations being presented initially come from an article by Chechin as to perturbation growth in the early universe. Due to a set of notes as written up by Sahoo, and Misra the author has reviewed what would be the consequences of adding in strange quark matter, cosmic strings and also domain walls, which change the nature of the initial baryonic model perturbations. The conclusion which jumps out, via what is the consequences for domain walls and galaxy formation , after the electro weak, is that the initial perturbations are heavily influenced by domain wall tension. I.e. almost as a free parameter, which is troubling since there is no experimental way to quantify what sort of domain wall tension is suitable at/ before the electro-weak regime.
Comments: 6 pages, addition of a useful reference, 5, plus elaborations
Unique-IP document downloads: 54 times
Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.