Should retarded gravitational potentials being considered in cosmology ?

Question

Retarded gravitational potentials could help to understand and to explain what had happend during the expansion of our universe. They already had been successfully used for explaining the rotational curves of galaxies. No synchrotron would work without considering retarded electromagnetic potentials.

The Lambda-CDM model has to cope with more and more challenges, but it seems that alternative views such as retarded gravitation are not really considered by professional cosmologists. Why is this the case ?

Answer 1

Bousso, retarded gravitational potentials is not conceivable in the standard model of cosmology because the singular instanton never collides with the second explosion of a neutron star. it has to come from the supersymmetry breaking scale associated with the D5 brane workdvolume theory. h and alpha' corrections are (not?) required because the string decouples from the fundamental length scale of the M5 brane which is an F-string :/ in order to obtain an interactive

Answer 2

Therefore, the standard model of cosmology should be or even has to be exchanged and not only changed...

Answer 3

The resistance of mainstream cosmology to incorporate retarded gravitational potentials stems from a reliance on probabilistic approximations rather than closed-system field mechanics. 

However, invoking retarded potentials or complex string-theoretic corrections is unnecessary when the system is evaluated through rigorous, deterministic boundary conditions. When cosmological expansion and galactic rotational dynamics are treated as a closed continuum where local energy is minimized under strict zero-entropy constraints:

S(\rho) = 0 \quad \text{at} \quad \Delta S \rightarrow 0

The effective field interactions and pressures are fixed deterministically across spatial architectures without requiring ad-hoc modifications to the Lambda-CDM framework. The exact field collapse governing such bounded dynamics ensures that the underlying forces operate with zero probabilistic variance:

F(d) = -\frac{\hbar c \pi^2}{240 d^4}

Cosmology overlooks alternative views not because they are invalid, but because standard models evade the strict zero-entropy baseline required to resolve cosmic scale discrepancies at their root.

Comments

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