|
Part 6 - Selfproof (cont) |
SELFPROOF 0206 - FLATNESS
PROBLEM
CURRENT COSMOLOGY MODEL
The
flatness problem is a cosmological fine-tuning problem within the Big
Bang model of the Universe. The parameter which appears fine-tuned is
the density of matter and energy in the Universe. This value affects
the curvature of spacetime, with a very specific critical value being
required for a flat Universe. The current density of the Universe is
observed to be very close to this critical value. Since the total
density departs rapidly from the critical value over cosmic time, the
early Universe must have had a density even closer to the critical
density, departing from it by one part in 1062
or less. This leads cosmologists to question how the initial density
came to be so closely fine-tuned to this 'special' value. The most
commonly accepted solution among cosmologists is cosmic inflation,
the idea that the Universe went through a brief period of extremely
rapid expansion in the first fraction of a second after the Big Bang.
(Wikipedia 12 Oct 2011)
MALTA COSMOLOGY TEMPLATE
- The property measures of the Universe are the sum of the property measures of its teels and teelpairs. (see ARGUMENT 0121)
- Thus the mass of the Universe is the sum of the mass of the teels it contains.
- Thus the energy of the Universe is the sum of the kineticenergy, the potentialenergy, and the latentenergy of its teelpairs.
- Thus the matter of the Universe is its mass modified by its energy.
- The Universe has a measure of mass and a measure of energy.
- The measure of the Universe's mass is not "balanced" or "fine-tuned" against the measure of its energy.
- A "universe" can have any measure of mass and energy.
- Its measures of mass and energy at any specified moment will depend on its prior history.
- What happens after a specified moment will depend upon its measures of mass and energy at that specified moment.
COMMENTARY
-
The
Flatness Problem is founded in the belief that the Universe is a
selfcontained unit with nothing outside it.
- Depending on the
energy/matter density of the early Universe, the Current Cosmology
Model universe can either be open, flat, or closed.
- The density
seems to have been exactly right to make the Universe flat.
- Such
fine tuning is difficult to believe in without there being a very
good reason for it.
- There
is no Flatness Problem in the Malta Cosmology Template.
- Its
Universe is not a selfcontained unit.
- It is currently expanding
within the uberuniverse.
- The terms open, flat, or closed, as used
in the Current Cosmology Model do not apply to the Universe of the Malta Cosmology Template.
|
|
|