The Science of Discworld II

The Science of Discworld II Read Online Free PDF Page A

Book: The Science of Discworld II Read Online Free PDF
Author: Terry Pratchett
(Jules Verne suggested) we could get there in a hollowed-out cylinder fired by a giant gun, located in Florida. Finally, in the 1960s, we found the right kind of swan (liquid oxygen and hydrogen) and the right kind of chariot (several million tons of metal) and we flew to the Moon. In a hollowed-out cylinder, launched from Florida. It wasn’t exactly a gun. Well, actually it was in a basic physical sense; the rocket was the gun and it went along for the ride, firing burnt fuel in place of a bullet.
    If we’d not told ourselves stories about the Moon, there would have been no point in going there at all. An interesting view, maybe … but we ‘knew’ about the view only because we had told ourselves scientific stories about images sent back by space probes. Why did we go? Because we’d been telling ourselves that we would, one day, for several hundred years. Because we’d made it inevitable and introduced it into the ‘future story’ of a great many people. Because it satisfied our curiosity, and because the Moon was waiting. The Moon was a story waiting to be finished (‘First human lands on the Moon!’), and we went there because the story demanded it.
    When Mind evolved on Earth, a kind of narrativium evolved alongside it. Unlike the Discworld variety of narrativium, which on the Disc is just as real as iron or copper or praseodymium, our variety is purely mental. It is an imperative, but the imperative has not been reified into a thing. However, we have the sort of mind, that respond to imperatives, and to many other non-things. And so it feels to us as if our universe runs on narrativium.
    There is a curious resonance here, and ‘resonance’ is definitely the word. Physicists tell a story about how carbon forms in the universe. In certain stars there is a particular nuclear reaction, a ‘resonance’ between nearby energy levels, which gives nature a stepping-stone from lighter elements to carbon. Without that resonance, so the story goes, carbon could not have formed. Now, the laws of physics as wecurrently understand them involve several ‘fundamental constants’, such as the speed of light, Planck’s constant in quantum theory, and the charge on an electron. These numbers determine the quantitative implications of the physical laws, but any choice of constants sets up a potential universe. The way that a universe behaves depends on the actual numbers that are used in its laws. As it happens, carbon is an essential constituent of all known life. All of which leads up to a clever little story called the Anthropic Principle: that it’s silly for us to ask why we live in a universe whose physical constants make that nuclear resonance possible – because if we didn’t, there’d be no carbon, hence no us to ask about it.
    The story of the carbon resonance can be found in many science books, because it creates a powerful impression of hidden order in the universe, and it seems to explain so much. But if we look a little more closely at this story, we find that it is a beautiful illustration of the seductive power of a compelling but false narrative. When a story seems to hang together, even consciously self-critical scientists can fail to ask the question that makes it fall apart.
    Here’s how the story goes. Carbon is created in red giant stars by a rather delicate process of nuclear synthesis, called the triple-alpha process. This involves the fusion of three helium nuclei. 5 A helium nucleus contains two protons and two neutrons. If you fuse three helium nuclei together, you get six protons and six neutrons. That, as it happens, is a carbon nucleus.
    All very well, but the odds on such a triple collision occurring inside a star are very small. Collisions of two helium nuclei are much more common, though still relatively rare. It is extremely rare for a third helium nucleus to crash into two that are just colliding. It’s like
Read Online Free Pdf

Similar Books

Shadow Creatures

Andrew Lane

Always

Lynsay Sands

Addicted

Ray Gordon

The Doctors' Baby

Marion Lennox

Homeward Bound

Harry Turtledove

He Loves My Curves

Stephanie Harley