The problem of cosmological constant correlation between observation and QFT-measurement as a fixpoint-description
Description
Discussed is a trying to solve the obvious contradiction in discrepance between the measuring of
cosmological constant (CC) from GRT-description and its calculated prediction in classical QFT.
Either then the coupling of CC to theory is wrong or the physical and mathematical methods to
calculate CC by QFT in flat Minkowskispace-background are wrong. Tried is a fixpoint-method to
come to a calculated value of CC which better fits to observation. In this context the sum-rules for
1-loop/2-loop in BSM-QFT are solved, three new scalarons (“Stooges“) and two new heavy
fermione (“Tweedles“) are introduced to couple matter-field beyond SM to CC and to look at
discrepances between measuring and calculation in a more consistent way.
Files
Problem of Cosmological Constant.pdf
Files
(648.1 kB)
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Additional details
Additional titles
- Alternative title (English)
- Spectral self-adjustment of the cosmological constant from quantum vacuum structure
Dates
- Copyrighted
-
2026-04-24