#4#4#4
So let’s get to the speculation. If we observe what we call a big bang arena, the one we are in and part of, can any reasonable and responsible speculation about preconditions be drawn from that observation?
How about speculation that our arena is not the only one? If one big bang arena can exist why would we think that it has to be the only one? The speculation up for discussion is this:
Is it reasonable to speculate that there might be other arenas within the landscape of the greater universe? Answer: Of course it is reasonable.
Thought starter: What preconditions would be consistent with the existence of other arenas?
Here is a Google link to “alternative cosmology”:
http://www.google.com/#hl=en&cp=21&....,cf.osb&fp=4d00a8c03c934068&biw=1280&bih=582
Here is the Wiki page that comes up. You can see that the topic has some content for review:
http://en.wikipedia.org/wiki/Non-standard_cosmology
“Non-standard cosmologies can be grouped according to the assumptions or the features of the big bang universe which they contradict.
[edit] Alternative metric cosmologies
The Friedmann-Robertson-Walker metric that is necessary for the Big Bang and steady state models emerged in the decade after the development of Einstein's general relativity and was accepted as a model for the universe after Edwin Hubble's discovery of his eponymous law. It was not clear early on how to find a "universe solution" to Einstein's equations that allowed for a universe that was infinite, unending, and immutable (scientists of the time assumed for philosophical reasons the universe should have such a character). Even after the development of expanding universe theories, people would engage in this exercise from time to time when looking for a replacement for general relativity. Any alternative theory of gravity would imply immediately an alternative cosmological theory since current modeling is dependent on general relativity as a framework assumption. What is included are a number of models based on alternative gravitational scenarios as well as early attempts to derive cosmological solutions from relativity.
[edit] Newtonian cosmology
Main article: Friedmann-Lemaître-Robertson-Walker metric#Newtonian approximation
While not seriously advocated by anyone after Einstein's development of relativity, Newtonian gravity can be used to model the universe and non-rigorously derive the Friedmann equations that are used in the big bang universe. This non-standard cosmology is mostly used as an elementary exercise for astronomy and physics students and doesn't represent a serious alternative proposal.
[edit] Lorentzian universes
Main article: Milne model
Before the complete development of general relativity, Arthur Milne offered a cosmology based on Lorentz transformations which had the feature of being applicable to a universe of any scale. It relied on a rejection of the curvature of space and so contradicted predictions from general relativity about the shape of the universe caused by the mass it contains. Milne's universe is still used today as a model of a hypothetical "empty universe".
[edit] Early general relativity based cosmologies
See also: static universe and De Sitter universe
Before the present general relativistic cosmological model was developed, Albert Einstein proposed a way to dynamically stabilize a cosmological scenario that would necessarily collapse in on itself due to the gravitational attraction[citation needed] of the matter constituents in the universe. Such a universe would need a source of "anti-gravity" to balance out the mutual attraction[citation needed], a scalar term in Einstein's equations that would come to be known as the cosmological constant. Einstein's first attempt at modeling relied on a cosmological constant that was finely tuned to exactly balance out matter curvature and provide a framework for an infinite and unchanging spacetime metric in which the objects of the universe were embedded. This happens to be the same as a special case of the current cosmological model where the cosmic scale factor is unchanging and the density seen in the Friedman equations is equally divided between the cosmological constant and matter.
Willem de Sitter would later generalize Einstein's scalar potential model to a universe model that would expand exponentially. As the early development of the Big Bang theory began, DeSitter would be falsely credited for inventing the expanding universe metric because of this. In reality, it was the work of Alexander Friedman and Georges Lemaitre who established the metric that would come to be the most accepted for cosmology. Nevertheless, DeSitter's model appears in two places today: in the discussion of cosmic inflation and in the discussion of dark energy dominated universes.
[edit] Machian universe
See also: Mach's principle and Brans-Dicke theory
Ernst Mach developed a kind of extension to general relativity which proposed that inertia was due to gravitational effects of the mass distribution of the universe. This led naturally to speculation about the cosmological implications for such a proposal. Carl Brans and Robert Dicke were able to successfully incorporate Mach's principle into general relativity which admitted for cosmological solutions that would imply a variable mass. The homogeneously distributed mass of the universe would result in a roughly scalar field that permeated the universe and would serve as a source for Newton's gravitational constant; creating a theory of quantum gravity.
[edit] Gödel's universe
Main article: Gödel metric
Partly as a counter-example to Mach's principle, Kurt Gödel found a solution to the Einstein field equations describing a universe with a non-zero angular momentum. This cosmology contained closed timelike curves; a signal or object starting from an event in such a universe could return to the same event. Einstein was unsatisfied with the implications of this and abandoned his hope for incorporating Mach's Principle into general relativity. Because of this effect, astronomers can in principle put limits on the rotation rate of the universe which today is measured to be close enough to zero that no cosmological implications should be expected.
[edit] MOND
Main article: Modified Newtonian Dynamics
Modified Newtonian Dynamics (MOND) is a relatively modern proposal to explain the galaxy rotation problem based on a variation of Newton's Second Law of Dynamics at low accelerations. This would produce a large-scale variation of Newton's universal theory of gravity. A modification of Newton's theory would also imply a modification of general relativistic cosmology in as much as Newtonian cosmology is the limit of Friedman cosmology. While almost all astrophysicists today reject MOND in favor of dark matter, a small number of researchers continue to enhance it, recently incorporating Brans-Dicke theories into treatments that attempt to account for cosmological observations.
[edit] TeVeS
Main article: TeVeS
Tensor-vector-scalar gravity (TeVeS) is a proposed relativistic theory that is equivalent to Modified Newtonian dynamics (MOND) in the non-relativistic limit, which purports to explain the galaxy rotation problem without invoking dark matter. Originated by Jacob Bekenstein in 2004, it incorporates various dynamical and non-dynamical tensor fields, vector fields and scalar fields.
The break-through of TeVeS over MOND is that it can explain the phenomenon of gravitational lensing, a cosmic optical illusion in which matter bends light, which has been confirmed many times. A recent preliminary finding is that it can explain structure formation without CDM, but requiring a ~2eV massive neutrino (They are also required to fit some Clusters of galaxies, including Bullet Cluster) [1] and [2]. However, other authors (see Slosar, Melchiorri and Silk [3]) claim that TeVeS can't explain cosmic microwave background anisotropies and structure formation at the same time, i.e. ruling out those models at high significance.
[edit] Steady state theories
Main article: Steady-state theory
The Steady state theory was proposed in 1948 by Fred Hoyle, Thomas Gold, Hermann Bondi and others as an alternative to the Big Bang theory that modified the homogeneity assumption of the cosmological principle to reflect a homogeneity in time as well as in space. This "perfect cosmological principle" as it would come to be called predicted a universe that expanded but did not change its density. In order to accomplish this, steady state cosmology had to posit a "matter-creation field" (the so called C-field) that would insert matter into the universe in order to maintain a constant density.
The idea was almost immediately attacked by proponents of the Big Bang who described the C-field as contradictory to a consistent understanding of physics. Hoyle, one of the most vocal proponents of the steady state model, and a committed materialist, believed that the competing, older model was forced as it violated fundamental philosophical principles regarding the infinite nature of existence. Hoyle explicitly warned that the Big Bang was being promoted as a first cause dogma in line with Western theology rather than science. To attack the connection, Hoyle began a public campaign to discredit the Big Bang theory and wound up coining the term "Big Bang" which remains stuck to the standard cosmological theory today, though the descriptive quality of the name has heavily been criticized as being misleading.[2]
The debate between the Big Bang and the Steady State models would happen for 15 years with camps roughly evenly divided until the discovery of the cosmic microwave background radiation. This radiation is a natural feature of the Big Bang model which demands a "time of last scattering" where photons decouple with baryonic matter. The Steady State model proposed that this radiation could be accounted for by so-called "integrated starlight" which was a background caused in part by Olbers' paradox in an infinite universe. In order to account for the uniformity of the background, steady state proponents posited a fog effect associated with microscopic iron particles that would scatter radio waves in such a manner as to produce an isotropic CMB. The proposed phenomena was whimsically named "cosmic iron whiskers" and served as the thermalization mechanism. The Steady State theory did not have the horizon problem of the Big Bang because it assumed an infinite amount of time was available for thermalizing the background.
As more cosmological data began to be collected, cosmologists began to realize that the Big Bang correctly predicted the abundance of light elements observed in the cosmos. What was a coincidental ratio of hydrogen to deuterium and helium in the steady state model was a feature of the Big Bang model. Additionally, detailed measurements of the CMB beginning in the 1990s indicated that the spectrum of the background was closer to a blackbody than any other source in nature. The best integrated starlight models could predict was a thermalization to the level of 10% while the COBE satellite measured the deviation at one part in 105. After this dramatic discovery, the majority of cosmologists became convinced that the steady state theory could not explain the cosmological observations as well as the Big Bang. Since that time, detailed observations of WMAP have isolated a standard Lambda-CDM model which relates the anisotropies in the CMB to features in the universe such as large-scale structure, the detailed nature of Hubble's Law, and even bizarre features such as inflation, dark energy, and cold dark matter.
Although the original steady state model is now considered to be contrary to observations even by its one-time supporters, a modification of the steady state model has been proposed, which envisions the universe as originating through many little bangs rather than one big bang. It supposes that the Universe goes through periodic expansion and contraction phases, with a soft "rebound" in place of the Big Bang. Thus the redshift is explained by the fact that the Universe is currently in an expansion phase. A handful of remaining steady state theorists (most famously Jayant V. Narlikar) continue to insist that the intergalactic medium contains cosmic iron whiskers. However, there is still no corroborating observational evidence for the existence of these iron particles.
[End of Wiki quote]
Strangely enough, none of the alternatives seem to have a footing that would make then candidates to overtake the existing Big Bang Theory consensus. And preconditions are missing accept for steady state cosmologies, but the Steady-state Theory described above in the main article is not the only possibility for a steady state model and in fact has some pretty obvious flaws as pointed out. The other stead state version I call Iron Whiskers is a cyclical stead state which also has flaws, one of which is that each cycle will inevitably emit energy that cannot be recalled for the following crunch/bang, and as a result it will eventually not be able to recall enough energy to bang at all.
If you agree that there were preconditions to our big bang, are you willing to specify some particulars about the preconditions that would characterize a model that you would consider to replace Big Bang Theory?