The Truth about Science and Religion. Fraser Fleming

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The Truth about Science and Religion - Fraser Fleming

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understanding creation, see the first chapter of Genesis as having a poetic form not suited to a literal interpretation.

      In fact, this is nothing new. Theologians since the third century have identified problems with a literal interpretation, such as there being an end to the first day without a sun or earth. A non-literal interpretation of “day” overcomes the otherwise problematic issue of God’s work schedule. If God created light instantaneously, what did he do for the rest of the day? The focus in Genesis, it is suggested, is not how God made the world, but that God made the world as the stage for the drama of life.

      In the 1920s Edwin Hubble’s telescopic images demonstrated that the universe was continuously expanding. Prominent among the proponents of this idea was the Catholic priest and physicist, Georges Lemaître, who saw no problem harmonizing God and cosmological theory. Galaxies moving apart at the speed of light means that, playing the tape backward, there was a beginning from which all creation came. The space between galaxies is stretching with space continuing to grow, but exactly what is the universe expanding into? Like the question of what happened before the universe existed, this particular question is better suited to philosophical answers than scientific ones.

      Harmonizing scriptures with new scientific discoveries is a continuous process. In a sense, the resilience of Genesis to reinterpretation as science advances shows either God’s providence or people’s stubborn belief in God. Harmonizing the truths of science and religion is ultimately only valuable if the result is a richer, purposeful, and more consistent life.

      A Finely-Tuned Universe

      Whether experiencing nature’s web in a pristine mountain glade or peering at the wonders of a working cell, evidence of an intricately functional universe is everywhere. The beautiful and elegant descriptions used of nature are exactly those used by cosmologists to describe the equations for the expansion of the universe. Equally surprising is that the mathematical equations that describe the universe’s development are few and simple, the kind of equations whose discovery earns Nobel prizes.

      The universe not only has a beautiful mathematical structure but the equations and values are very finely tuned. Just four basic forces affected the first particles during the initial stages of the Big Bang: gravity, electromagnetism, the strong nuclear force, and the weak nuclear force. The balance between these forces is extremely precise in two ways: first the physical constants of the universe have very specific values, and second, the initial “boundary” conditions for the universe are tightly specified. Boundary conditions refer to the starting or developing nature of the universe, such as the delicate poise between expansion and collapse, and the fluctuations that form galaxies without forming black holes. Cosmologists like to say that the universe seems quite finely balanced between the outward energy of expansion and the inward pull of gravitation. Like shooting hoops, the force and trajectory must work together.

      Fine tuning is nicely illustrated in the life of a star. Stars get their energy by burning hydrogen to form helium. When all the hydrogen is consumed, the core of the star pulls together under extreme gravity to form beryllium. Beryllium is a toxic element lacking the right bonding properties for most living organisms but is very efficiently converted to carbon (~100 percent), because there is just the right relationship between the electromagnetic and nuclear forces of beryllium and carbon. The energy for the conversion of beryllium into carbon is very closely matched so that if the conversion were only 4 percent higher or 0.5 percent lower, virtually no carbon would form. Carbon, once formed, can be consumed through a carbon-helium collision whose energy is similarly highly controlled; a deviation of only half a percent would lead all the carbon to be converted to oxygen. Carbon is slowly converted to oxygen, gradually enough to allow carbon to build up, but at a rate sufficient to produce oxygen for life. A series of delicately poised transformations provides a way for carbon to be produced from stars to provide “the building block for life.”

      If the value of the gravitational constant was slightly larger, then the stars’ lifetimes would be much shorter with much less time for planets, and life, to evolve. Alternatively, weak gravity would mean that the stars could not generate enough heat to grow and explode to liberate the heavy atoms needed for life. How finely balanced is the force of gravity? Estimates for the allowable variation are in the range of 1 part in 100,000,000,000,000 (one hundred thousand billion).

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