Not so fine tuned after all? A response to Steven Weinberg's objection to the design argument from cosmic fine tuning
This paper discusses one particular objection to the design argument from cosmic fine-tuning: the objection which says that the universe is not so fine tuned after all. It looks at a specific version of this objection, made by professor Steven Weinberg.
This paper is longer and more technical than most on this site. There really isn’t any way to get to the argument without the technicalities. However, if you just want to see the conclusion, you can get this by reading the last few paragraphs. A slightly longer version of the paper - including some extended quotations from the original sources - is also available here as a pdf file.
Your body is made from organic chemicals – complicated chemicals containing carbon. The only place carbon atoms are made is inside stars. You are made of star dust.
Carbon, mass number 12, is made inside stars by the fusion of three helium nuclei, mass number 4. (Helium nuclei are also called alpha particles, α.) Along the way to producing carbon, two helium nuclei combine together to make a nucleus of beryllium, mass number 8.
Beryllium is pretty unstable – a beryllium nucleus will break down again into two helium nuclei in a tiny fraction of a second, unless a third helium nucleus is added before this happens.
The problem is that this reaction shouldn’t happen, because the beryllium nucleus and helium nucleus together have more energy than a carbon nucleus. The amount of carbon produced in stars should be very small – and this means you and I shouldn’t be here at all.
In the 1950s, the astronomer and physicist Fred Hoyle was working on how the elements are made inside stars. He couldn’t account for the production of carbon, because of the problem described above.
Because the universe contains astronomers and physicists, and other complicated things made from carbon atoms, Hoyle reasoned that there must be something that made the carbon reaction go faster than expected. He predicted the existence of an excited energy state (called a resonance) in the carbon 12 nucleus, at just the right energy level – just above the combined energies of the 8Be and 4He nuclei. This would allow the reaction making carbon to go ahead much more quickly.
So Hoyle predicted the existence of a resonant energy level at about 7.68 MeV in 12C. Researchers looked for this energy level, and found it just where he said it should be.
To make the picture a bit more complicated, oxygen is made by adding another helium nucleus to carbon. If this reaction had a resonance, all the carbon would be converted to oxygen, which would also be bad for the existence of complicated things made from carbon. Fortunately, the appropriate energy level in oxygen is just below the combined energy of carbon and helium, and the reaction cannot be resonant.
If these energy levels were not exactly as they are, either very little carbon would be produced, or all the carbon that is produced would be turned into oxygen. Our existence depends on the universe having significant amounts of both carbon and oxygen.
To Hoyle, the presence of this energy level in carbon seemed to be a case of remarkable fine-tuning. Hoyle – an out-and-out atheist - would later say that nothing had shaken his atheism as much as this discovery. He said:
‘A common sense interpretation of the facts suggests that a superintellect has monkeyed with physics, as well as with chemistry and biology, and that there are no blind forces worth speaking about in nature. The numbers one calculates from the facts seem to me so overwhelming as to put this conclusion almost beyond question.’
‘I do not believe that any scientist who examines the evidence would fail to draw the inference that the laws of nuclear physics have been deliberately designed with regard to the consequences they produce inside stars. If this is so, then my apparently random quirks have become part of a deep-laid scheme. If not, then we are back again at a monstrous sequence of accidents.’
So much for the physics and the original fine-tuning argument. What of the objection?
In April 1999, Professor Steven Weinberg gave a lecture to the ‘Cosmic Design’ conference of the American Association for the Advancement of Science, His lecture was called ‘Designer Universe?’
(Weinberg won the Nobel Prize in Physics in 1979. He is the author of ‘The First Three Minutes,’ which is one of the best popular accounts of the physics of the Big Bang. He is also a well-known atheist.)
In his talk, he claimed that the placing of the energy level in carbon 12 is not much of a case for cosmic fine-tuning, because it does not have to be especially precisely adjusted after all.
Although it looks as if the energy has to be very finely tuned with relation to the ground state of carbon 12 (within about 1%), the critical issue is really how it relates to the combined energies of the beryllium and helium nuclei. Looked at like this, it only has to be ‘fine-tuned’ to within about 20% - which is nowhere near so precise. (See the extended quotation from Weinberg’s talk in the longer version of this article.)
In discussion with John Polkinghorne, Weinberg said:
[I] am not terribly impressed by the examples of fine-tuning of constants of nature that have been presented. To be a little bit more precise about the case of carbon, the energy levels of carbon, which is the most notorious example that’s always cited, there is an energy level that is 7.65 MeV above the ground state of carbon. If it was .06 of an MeV higher, then carbon production would be greatly diminished and there would be much less chance of life forming. That looks like a 1% fine-tuning of the constants of nature ... However, as has been realized subsequently after this ‘fine-tuning’ was pointed out, you should really measure the energy level not above the ground state of carbon but above the state of the nucleus Beryllium 8 (8Be) plus a helium nucleus ... In other words, the fine-tuning is not 1% but it’s something like 25%. So, it’s not very impressive fine-tuning at all.
So Weinberg’s argument is that the energy levels are not really as fine-tuned as Hoyle originally thought. Perhaps they are adjusted with an accuracy of only ±25%, rather than ±1%
Weinberg based his argument on some research published in 1989. A group of physicists modelled how the development of stars would change if the resonant energy level in carbon was different. They found that the energy level could be varied quite a bit without disastrously affecting the production of carbon. In fact, if the energy level is reduced slightly, much more carbon is produced.
From this they concluded that the tuning is not as precise as it at first appears, and therefore the ‘coincidence’ is not so significant.
Responding to the objection
So is Weinberg’s objection convincing? I don’t think so. Here are three reasons why:
(1) The fine tuning discovered by Hoyle isn’t just about a single energy level in carbon: it also involves the ‘coincidence’ that the energy level in oxygen is too low to allow resonance. If this level was a bit higher, all the carbon that is produced would be burned into oxygen. Of course, we need both carbon and oxygen, in roughly equal amounts. As Barrow and Tipler say:
‘Hoyle realized that this remarkable chain of coincidences – the unusual longevity of beryllium, the existence of an advantageous resonance level in C12 and the non-existence of a disadvantageous level in O16 – were necesssary, and remarkably fine-tuned, conditions for our own existence and indeed the existence of any carbon-based life in the Universe. ‘
The argument that by decreasing the energy of the resonant level a little bit, much more carbon could be produced, seems to miss this point: it is not just carbon, but also oxygen that we need.
(2) Weinberg is almost certainly mistaken about the fine tuning only needing to be 20 or 25%: The 1989 research varied the resonant energy level in carbon in an ad-hoc way, and investigated the effect on carbon formation. However, in a paper published in Science in 2000, three scientists investigated how the rate of production of carbon would be affected by small changes in the fundamental forces that lie behind the carbon resonance - the strong nuclear force and the electromagnetic force. Their conclusion was that a change of just 0.5% in the strong nuclear force or 4% in the electromagnetic force would reduce the production of carbon or oxygen by between 30 and 1000 times:
‘We conclude that a change of more than 0.5% in the strength of the strong interaction or more than 4% change in the strength of the Coulomb force would destroy either nearly all C or all O in every star. This implies that irrespective of stellar evolution the contribution of each star to the abundance of C or O in the ISM would be negligible. Therefore, for the above cases the creation of carbon based life in our universe would be strongly disfavored.’
So it looks as if there is still a strong case for fine tuning in the production of carbon and oxygen, looked at in terms of the strengths of the fundamental physical reactions involved.
(3) However, even if for the sake of argument we allow Weinberg’s central point – that the resonant energy level in carbon is only ‘fine-tuned’ to, say, 20%, rather than 1%, he has still not succeeded in his project of explaining away cosmic fine tuning:
The resonant energy level in carbon was one of the first, and one of the most specific cases of cosmic fine-tuning to be discovered. But it is only one example. Scientists now know of a number of other cases of cosmic fine-tuning. Some of these have to be much more precisely tuned than the carbon and oxygen energy levels.
To take just one example, the mathematical physicist Sir Roger Penrose says that the initial conditions of the Big Bang are so special that the odds of their coming about by chance are less than one part in 10 to the power of (10 to the power of 123). That is 1 in 1 followed by 10123 successive 0's. To give some idea of just how ridiculously small a number this is, there are only 1080 particles of any kind in the observable universe. As Penrose says,
‘... try to put one zero on every particle in the observable universe and you would be way short.’
‘There has got to be fine tuning. This is fine tuning, this is incredible precision in the organisation of the initial universe.’
There are several other examples of fine tuning besides the energy level in carbon. Some of these involve much more precise fine tuning. For Weinberg’s objection to carry through, he would have to explain away all of them, and he has not done that.
David Couchman MA, M.Sc, M.Min, May 2010
 Dunbar, D N F, Pixley, R E, Wenzel, W A and Whaling, W: ‘The 7.68 MeV State in C12,’ Physical Review vol. 29 Number 3, November 1st, 1953.
 Hoyle, F, ‘The Universe: Past and Present Reflections.’ in Engineering and Science, November, 1981. pp. 8–12
 Hoyle, F, in ‘Religion and the Scientists’ (1959) quoted in Barrow and Tipler p. 22
 Livio, M, Hollowell, D, Weiss, A & Truran, J W: ‘The anthropic significance of the existence of an excited state of 12C,’ Nature vol 340, No. 6231, 27 July 1989
 Barrow J D and Tipler F J: ‘The Anthropic Cosmological Principle’, 1986. pp 251 to 254
 Oberhummer, H, Csót, A, and Schlattl, H: ‘Stellar Production Rates of Carbon and Its Abundance in the Universe,’ Science, vol 289, p. 88-90 (2000);