Authors: Claude Latourre
For more than a century, the equations of general relativity have evolved according to the observations of the universe. These changes are expressed through the cosmological constant (Λ), which was first added on the space-time part to account for a stationary universe, then removed when the expansion of the universe was observed. More recently, the constant reappeared on the energy-momentum part to describe an accelerated expansion of the universe. However, their contractions can express exactly the value of the cosmological constant: Λ = -1/4 (R + κ T) and fully define the equations of General Relativity: (Rµ√ -1/4 gµ√ R) = κ (Tµ√ -1/4 gµ√ T) without using other concepts: Dark energy, Quintessence...
Comments: 5 Pages. En français
Unique-IP document downloads: 216 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.