Contrast the stated motivations of Bondi and Gold on the one hand, and Hoyle on the other, for developing the "Steady State" cosmological model. | [2] |
Note that the question says "Contrast", so you are looking for differences.
Bondi and Gold base their argument explicitly on the argument that observed physics laws have only been tested against the background of the currently observed universe, and that changes in the parameters of the "background" universe, e.g. higher average density, might result in changes in physical constants or laws (e.g. a change in G. Therefore, they argue that the only logically consistent theory of cosmology is one in which the reference universe does not change, i.e. a "Steady State" universe, and they set out to investigate whether such a model is tenable. [Their exact words are "We do not claim that this principle must be true, but we say that if it does not hold, one's choice of the variability of physical laws becomes so wide that cosmology is no longer a science."] Hoyle, on the other hand, has a rather more concrete motivation: he points out that, with the then accepted value of H, the universe should be only 1.3 Gyr old, or at least should have been in an ultra-dense state 1.3 Gyr ago, whereas astrophysical arguments suggest that this has not been the case for at least 5 Gyr, and the Earth itself is at least 2 Gyr old. This is an absolutely valid Popperian/Kuhnian motivation for proposing an alternative model: the existing model is falsified by this observation (Popper), or at least is suffering from a serious anomaly (Kuhn). Therefore, we see that Bondi and Gold do not have any practical objections to the existing Friedmann-Lemaître models - the problem is that they do not believe that we can justify applying the physical laws we observe in our present universe to a universe with very different physical conditions. Hoyle, on the other hand, does raise a practical objection: he notes, correctly, that the then accepted value of the Hubble constant produces too young a universe in the Friedmann-Lemaître models, and he provides reasoned arguments against the use of a cosmological constant to solve the problem. (He does not consider the correct resolution, namely the radical revision of H, but nobody else at the time did either, so that isn't his fault!) [Hoyle does also refer to "aesthetic objections to the creation of the universe in the remote past". Although he emphasises the practical aspects much more in his paper, it would seem that this more "philosophical" or emotional objection better reflects his real feelings, since if he were motivated purely by pragmatic considerations, he would not have clung to the Steady State model long after unbiased observers felt that it had been conclusively disproved. This is why the question specifies the stated motivations!] |
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What are the testable predictions of the Steady State model? Explain how developments in observational cosmology through the 1960s effectively disproved the Steady State model. | [4] |
Note that the question asks for testable predictions. The prediction of continuous
creation of matter is not testable, because the predicted rate is unobservably
small, and therefore does not count.
The basic feature of the Steady State model is that it is a Steady State model: its properties should not change with time. Note that this does not mean that it is static - just that the density, rate of expansion, radius of curvature, stellar populations, etc., should not change with time. Given the finite speed of light, this is equivalent to saying that the properties of the universe should not change with redshift - i.e., that the high redshift universe should look essentially identical, on a large enough scale, to the local universe. Therefore, the testable predictions of the Steady State model are:
The 1960s observational evidence contradicting these predictions was:
It may be seen that objections can be raised to any one piece of contrary evidence (some of the objections being less credible than others). However, the combination of evidence is devastating: you are comparing natural expectations on the one hand (in the Big Bang model evolution of populations is to be expected, so more radio sources and quasars at high redshift is perfectly reasonable though not a prediction, while the existence of a relic blackbody background at a few kelvin is a prediction) with not one but three ad hoc after-the-fact rationalisations on the other. At this point there is no contest! |
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Discuss the observational evidence for and against the "classical" (i.e. not inflationary) Big Bang model as it stood around 1980. Hence, briefly explain what motivated Alan Guth to propose the idea of inflation in 1981. | [4] |
Note that you are looking specifically for evidence for the Big Bang. Observations
which are consistent with the Big Bang but equally consistent with competing models,
such as the expansion of the universe, therefore don't count.
The first two points against constitute Guth's motivation for inflation. Introducing a brief period of exponential expansion in the very early universe (long before BBN, let alone the CMB emission) can ensure that our entire visible universe originates inside a single causally connected domain (thus solving the horizon problem), and the expansion dilutes away any initial curvature (thus solving the flatness problem). [Inflation does not address the last problem, which is solved by the introduction of dark energy - which increases the age of the universe - and dark matter - which provides an additional contribution to Ω which does not contribute to nucleosynthesis.] |
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