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There are two scientific theories that, taken together, explain the entire universe. The first, which describes the force of gravity, is widely known: Einstein’s General Theory of Relativity. But the theory that explains everything else—the Standard Model of Elementary Particles—is virtually unknown among the general public.
In The Theory of Almost Everything, Robert Oerter shows how what were once thought to be separate
...43) My brief history
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The physicist explores his life and intellectual evolution.
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Finish the course by surveying the many uses of radiation on Earth and beyond. Passive detectors identify radioactive contamination and clandestine nuclear bomb tests. Cosmic rays can be used to "X-ray" ancient buildings and learn the secrets of their construction. And, see why some scientists speculate that humans thrive on Earth thanks to an ancient bath of radiation from a supernova explosion.
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Discover that the values for work and heat in a given system depend on the path taken to get to a particular state. But note that the sum of work and heat does not depend on the path; it is a constant. This remarkable fact is the foundation of the first law of thermodynamics.
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Analyze the most central idea of thermodynamics: temperature. Investigate the origin of different temperature scales and the various methods for measuring temperature. See how the concept of temperature is a consequence of the zeroth law of thermodynamics, which deals with the nature of thermal equilibrium.
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The first inklings of a successful theory of everything will probably arise from symmetries and group theory. Prepare for this epochal moment by digging into these important mathematical ideas. Also, learn to approach proposed theories of everything with fascination, tinged with healthy skepticism.
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Thirty years after EPR, physicist John Bell dropped an even bigger bombshell, showing that a deterministic theory of quantum mechanics such as EPR violates the principle of locality - that particles in close interaction can't be instantaneously affected by events happening in another part of the universe.
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Understand how pressure, volume, and temperature are state functions related by a formula known as the ideal gas law. Contrast these variables with work and heat, learning why they are not state functions. See how the ideal gas law can be used to calculate the work done by a piston.
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The discovery of the neutron in 1932 led to the insight that neutrons can incite certain heavy elements to fission (break apart), releasing more neutrons and a prodigious amount of energy. In this lecture, lay the groundwork for understanding nuclear weapons and nuclear power by investigating nuclei that are prone to fission, how to initiate fission, and the "daughter nuclei" that result.
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Why can't we answer questions about what happened before the Big Bang, or what goes on at the center of a black hole? Can we manage the formidable task of combining quantum physics with general relativity? Physics may well be the most important subject in the universe, a theoretical realm that ranges from the infinitesimally small to the infinitely vast, its laws governing time, space, and the forces that created our world.
57) The Particle Zoo
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Are quarks, the particles that make up protons and neutrons, the truly elementary particles? What are the three fundamental forces that physicists identify as holding particles together? Are they manifestations of a single, universal force?
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See how hydrogen, helium, and a few other light nuclei were forged in the fiery aftermath of the Big Bang. Then, trace the formation of heavier nuclei in the interiors of stars, in supernova explosions, and in the collisions of neutron stars. Special attention is paid to the sequence of reactions and the required conditions that gave us the complete periodic table of elements.
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Investigate the properties of different materials as they change phase from solid to liquid to gas. Witness the surprising behavior of supercooled water, and discover that phase diagrams are an important tool for predicting how temperature and pressure determine when phase transitions occur.
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Quantization places severe limits on our ability to observe nature at the atomic scale because it implies that the act of observation disturbs that which is being observed. The result is Werner Heisenberg's famous Uncertainty Principle. What exactly does this principle say, and what are the philosophical implications?
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