Catalog Search Results
1) Arcadia
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"This play moves back and forth between 1809 and the present at the elegant estate owned by the Coverly family. The 1809 scenes reveal a household in transition. As the Arcadian landscape is being transformed into picturesque Gothic gardens, complete with a hermitage, thirteen-year-old Lady Thomasina and her tutor delve into intellectual and romantic issues. Present day scenes depict the Coverly descendants and two competing scholars who are researching...
2) Proof
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An enigmatic young woman. A manipulative sister. Their brilliant father. An unexpected suitor. One life-altering question. The search for the truth behind a mysterious mathematical proof is the perplexing problem in David Auburn's dynamic play. Starring Anne Heche and Jeremy Sisto, Proof is a winner of the 2001 Tony award for Best Play as well as the 2001 Pulitzer Prize for drama.
Includes an interview with Dr. Carrie Bearden, a Clinical Neuropsychologist
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Description
"No one would have believed in the last years of the nineteenth century that this world was being watched keenly and closely by intelligence greater than man's; that as men busied themselves about their various concerns they were scrutinized and studied. Yet across the gulf of space, intellects vast and cool and unsympathetic regarded this earth with envious eyes, and slowly and surely drew their plans against us. Then, late one night, in the middle...
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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? 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.
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Isaac Newton was born in 1642, the year that Galileo died. You'll learn how he built on the work of Galileo and Kepler, developing the three laws of motion and the concept of universal gravitation. You'll learn why Newton's laws suggest a universe that runs like a clock.
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With this lecture, you turn from relativity to explore the universe at the smallest scales. By the early 1900s, Ernest Rutherford and colleagues showed that atoms consist of a positively charged nucleus surrounded by negatively charged electrons whirling around it. But Rutherford's model could not explain all the observed phenomena.
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In 1905 a young Swiss patent clerk named Albert Einstein resolved the crisis that flowed from the Michelson-Morley result. When Einstein discarded the ether concept and asserted that the principle of relativity holds for all of physics, mechanics as well as electromagnetism, he was making a simple claim with almost unimaginably profound implications.
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In 1923, Louis de Broglie proposed that, like light photons, particles of matter might also display wave properties. The wave nature of smaller particles such as electrons is quite visible and leads to many unusual phenomena, including quantum tunneling mentioned in Lecture 1.
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The study of motion is not all there is to physics. By the 18th century, scientists were delving into the relationship between the two phenomena. Today, electromagnetism is known to be responsible for the chemical interactions of atoms and molecules and all of modern electronic technology.
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