What Does the Central Limit Theorem Have to Say About General Relativity?
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This Laplacian can be solved to get an expression for the magnitude of the linear
radial gravitational field:
g(r) = −
− →
∇ Φ (r)
= −
2Kc 2 Mc 2
(4πσ )
3 r 2
exp
−
σ 2
2r 2
(21)
which reduces to the Newton description for large r values.
The gravitational potential can be obtained, if Eq. (21) is integrated:
Φ(r) =
r
0
g(r)dr =
2Kc 2 Mc 2
(4πσ )
3
√
π
√
2σ
erf c
σ
√
2r
= Φ erf c (r)
(22)
where the integration limits, from 0 to r, are consistent, according to Eq. (14), with
integration from r = ∞ to 0 in the corresponding flat space representation, which
leads to an erfc potential. In other words, in a flat space, the gravitational potential
is fixed to zero at r = ∞ and the Minkowskian metric is recovered under this
condition. But when the flat model is projected into a curved space, according to
the inverse relationship (14) between r and
r , Eq. (22) predicts a constant potential
at r = infinity. This is the particular feature of an erfc potential which leads to an
original description of the space-time surrounding a massive object as previously
published [7, 8]. Eq. (22) also converges toward the Newton limit, if the constant
term included in the erfc function is arbitrarily subtracted, which leads to an erf
potential that tends toward a 1/r behavior at large r values.
3 Conclusion
Under the paradigm of a self-organizing universe, the laws of physics should emerge
from the space-time and matter-energy distribution. From a global perspective,
the analogical and speculative approach presented in this paper can be seen as a
heuristic strategy to mathematically take into account Mach’s principle [9]. On top
of Einstein’s arguments [14], Eq. (3) provides a rationale based on a fundamental
law of probabilities, the Bayes’s law [15]. Applying this interdependence principle
and the Central Limit Theorem, we have pinpointed a possible explanation for the
emergence of a weighted Newton’s law of gravitation in such a system. One key
feature of the present theory [16] is that it is based on the existence of an intrinsic
star-specific physical constant, the parameter σ 2 , which automatically emerges from
a convergence process described by the Central Limit Theorem. As reported in [7,
8], the new erfc potential once incorporated into a spherically symmetric metric,
describes various features of the resulting modified Schwarzschild geometry. For
example, computing the systematic errors that emerge when the effect of σ is
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