Affiche Modern Physics for Non-Scientists
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A series of 24 lectures, explaining complex physics to the laymen.


Saisons & épisodes Les résumés de tous les épisodes de Modern Physics for Non-Scientists

S01E01 Time Travel, Tunneling, Tennis, and Tea 00/00/0000 What are the two big ideas of modern physics? How can nonscientists gain a handle on these ideas and the radical changes they bring to our philosophical thinking about the physical world?
S01E02 Heaven and Earth, Place and Motion 00/00/0000 Understanding motion is the key to understanding space and time. Is there a "natural" state of motion? Learn why the ancients gave different answers to this question, and how Copernicus, Kepler, and Galileo laid the foundation for a new approach.
S01E03 The Clockwork Universe 00/00/0000 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.
S01E04 Let There Be Light 00/00/0000 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.
S01E05 Speed c Relative to What 00/00/0000 In mechanics (the branch of physics that studies motion), the principle of Galilean relativity holds. Meaning that the laws of mechanics are the same for anything in uniform motion. Is the same true for the laws of electromagnetism?
S01E06 Earth and the Ether-A Crisis in Physics 00/00/0000 In the 1880s, Albert Michelson and Edward Morley conducted an experiment to determine the motion of Earth relative to the ether. You'll learn about their experiment, its shocking result, and the resulting theoretical crisis.
S01E07 Einstein to the Rescue 00/00/0000 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.
S01E08 Uncommon Sense-Stretching Time 00/00/0000 Why does the simple statement of relativity - that the laws of physics are the same for all observers in uniform motion - lead directly to absurd-seeming situations that violate our commonsense notions of space and time?
S01E09 Muons and Time-Traveling Twins 00/00/0000 As a dramatic example of what relativity implies, you will consider a thought experiment involving a pair of twins, one of whom goes on a journey to the stars and returns to Earth younger than her sister!
S01E10 Escaping Contradiction-Simultaneity Is Relative 00/00/0000 If, as relativity implies, "moving clocks run slow," who's to say which clock is moving?
S01E11 Faster than Light-Past, Future, and Elsewhere 00/00/0000 Relativity implies that the time order of events can be different in different reference frames. Does this wreak havoc with cause and effect? Finally, why is it that nothing can go faster than light?
S01E12 What about E=mc2 and Is Everything Relative 00/00/0000 Shortly after publishing his 1905 paper on special relativity, Einstein realized that his theory required a fundamental equivalence between mass and energy, which he expressed in the equation E=mc2. Among other things, this famous formula means that the energy contained in a single raisin could power a large city for an entire day.
S01E13 A Problem of Gravity 00/00/0000 Historically, the path to general relativity followed Einstein's attempt to incorporate gravity into relativity theory, which led to his understanding of gravity not as a force, but as a local manifestation of geometry in curved spacetime.
S01E14 Curved Spacetime 00/00/0000 What causes spacetime to curve? Einstein's theory of relativity offers an answer, but for decades after he published it, there were only a few, very subtle tests of its validity. How has modern astrophysics changed all that?
S01E15 Black Holes 00/00/0000 General relativity is similar to Newtonian gravitation except in the case of very dense objects such as collapsed stars. Learn why they are called black holes.
S01E16 Into the Heart of Matter 00/00/0000 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.
S01E17 Enter the Quantum 00/00/0000 The "stuff" of the universe, matter and energy, is not continuously subdividable but comes in discrete "chunks". This fundamental graininess of the universe has profound implications for the behavior of matter and energy at the smallest scales.
S01E18 Wave or Particle? 00/00/0000 Einstein's resolution of the photoelectric effect problem suggests that light consists of particles (photons). But how can this be reconciled with the understanding of light as an electromagnetic wave?
S01E19 Quantum Uncertainty-Farewell to Determinism 00/00/0000 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?
S01E20 Particle or Wave? 00/00/0000 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.
S01E21 Quantum Weirdness and Schrodinger's Cat 00/00/0000 Wave-particle duality gives rise to strange phenomena, some of which are explored in Schrödinger's famous "cat in the box" example. Philosophical debate on Schrödinger's cat still rages.
S01E22 The Particle Zoo 00/00/0000 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?
S01E23 Cosmic Connections 00/00/0000 Why does physicist Freeman Dyson think that intelligence may persist into the infinite future, even as the universe evolves through an unimaginable richness of new forms and structures?
S01E24 Toward a Theory of Everything 00/00/0000 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.

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