Stephen Hawking
Stephen Hawking has been hailed as one of the most brilliant theoretical physicists since Albert Einstein. Hawking was born on January 8, 1942, which as he likes to point out is the 300th anniversary of Galileo's death. Hawking originally studied at Oxford University in England studying physics even though he would have preferred math. He moved onto Cambridge University to work on his PhD in cosmology. Hawking's career has focused upon the cosmic entities known as black holes, and has extended to specialized areas such as quantum gravity, particle physics, and supersymmetry. A field of study that Stephen Hawking is known for is cosmology. Cosmology is the metaphysical study of the origin and nature of the universe. A brief synopsis of Hawking indicates that, according to Hawking, "there is 'no place for a creator', that God does not exist." In his quantum cosmology, he indicates, "there would be no singularities at which the laws of science broke down and no edge of space-time at which one would have to appeal to God or some new law to set the boundary conditions for space-time . . . The universe would be completely self-contained and not affected by anything outside itself. It would neither be created nor destroyed. It would just BE . . . What place, then, for a creator?"(Smith 2005)Theists have argued against this position, specifically, "that even if Hawking's physical laws are true, that fact does not entail that the God of classical theism does not exist or even disconfirm the classical theistic hypothesis." It would appear that Hawking did not inhibit himself to simply one theory when asking the question where did we come from and why. Rather, he points out that "if we do discover a complete theory, it should in time be understandable in broad principle by everyone, not just a few scientists. Then we shall all, philosophers, scientists, and just ordinary people, be able to take part in the discussion of the question of why it is that we and the
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Hawking, S. (1998). Public Lecture: The beginning of Time. Retrieved from
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