Authors: Joseph F. Messina
Recent astronomical observations have revealed important new clues regarding dark matter's behavior. However, the fact remains that all experimental efforts to detect dark matter directly, in a laboratory setting, have failed. A natural explanation for these failed efforts may be possible by postulating that dark matter's behavior is governed by a non-Planckian "action." It is pointed out, as a preliminary to advancing this possibility, that no purely dark matter measurement of Planck's constant exists. The resulting hypothesis advocates the existence of a new, experimentally verifiable, dark matter candidate. An extension of this hypothesis to the cosmological realm suggests that dark matter may have come into existence 10 to the minus 44 seconds after the big bang; an order of magnitude prior to the Planck era.
Comments: 4 Pages. Updated to match version submitted to "Papers in Physics"
Unique-IP document downloads: 209 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.