twin universe cosmology

En résumé (grâce à un LLM libre auto-hébergé)

  • The page explores the cosmology of twin universes and the associated physical equations.
  • It discusses the invariance of several fundamental equations such as those of Schrödinger, Boltzmann and Poisson.
  • The relationships between physical constants and cosmological quantities are analyzed.

twin universe cosmology Twin Universes cosmology (p 7)
The invariance of the Schrödinger equation is ensured if:
(56)

Equation 56

The Boltzmann equation is invariant if :

(57)

Equation 57

The Poisson equation for gravitation poses no particular problem and simply becomes (58)

From the Maxwell equations, we obtain :

(59)

Equation 59

(60)

Equation 60

which is consistent with the definition of an electric field due to an electric charge.

From the Einstein equation, as mentioned earlier, we obtain :

(61) G » c²

Otherwise, the equation is no longer divergenceless.

If the quantities :

(62) h , m , c , G, R , T

obey these relations, it will not be possible to evidence their variations in any laboratory experiment.

And then?

From (57), we obtain immediately :

(63)

Equation 63

which is nothing but the characteristic Schwarzschild length, so that :

(64) Rs » R

Let us now examine the Jeans length :

(65)

Equation 65

where :

(66)

Equation 66

(66b)

(66t)

(67)

Equation 67

Combining the equations (56) and (57), we obtain :

67b)

(68)

Equation 68

The Compton length varies like R :

(69)

Equation 69

The Planck length is :

(70)

Equation 70

(70b)

The Planck time is :

(71)

Equation 71

The Jeans time is :

(72)

Equation 72

Combining (61) and (63), we obtain :

(73)

Equation 73

The variation of the constants does not conserve the mass.

If we conserve the number of species, the mass density r is found to obey :

(74)

Equation 74

...same law for the contribution rr of the radiation to the density r. The conservation of the radiative energy gives :

(75) pr R³ = constant

Then :

(76)

Equation 76