In this Winter course, we will continue an exploration of string theory with Leonard Susskind, the physicist who first developed this important theory that attempts to reconcile quantum mechanics and general relativity. He begins with the mathematical equations of a damped harmonic oscillator, and relates that simple system to... Geometries of space: flat, spherical, hyperbolic, Dark matter and allocation of energy density.
Professor Susskind introduces the topic of modern Cosmology, which started with the discovery of cosmic microwave background radiation in 1964. Professor Susskind examines the temperature history of our universe. Recorded April 14, 2008 at Stanford University.
Recorded April 14, 2008 at Stanford University.\r\rThis Stanford Continuing Studies course is the third of a six-quarter sequence of classes exploring the essential theoretical foundations of modern physics.
Professor Susskind opens the lecture with one of the fundamental questions in cosmology: why are there more protons than anti-protons in the universe today?
(Image credit: ESO/MPE/Marc Schartmann). In particular, the course will focus on string theory with regard to important issues in contemporary physics. Try Susskind’s ‘Advanced Quantum Mechanics’ which follows this first course and is equivalent to an upper division course on QM. Lecture 1 of Leonard Susskind's Modern Physics course concentrating on Special Relativity. 1. Beginning with the... After reviewing the basic equation for an expanding universe, Professor Susskind solves the equation explicitly for a zero energy universe, and then extends the derivation to universes with non-zero energy. Lecture 1 of Leonard Susskind's Modern Physics course concentrating on Quantum Mechanics. He has won both the Pregel Award from the New York Academy of Science and the J.J. Sakurai Prize in theoretical particle physics.
Recorded January 14, 2008 at Stanford University.\r\rThis Stanford Continuing Studies course is the second of a six-quarter sequence of classes exploring the essential theoretical foundations of modern physics.
The expanding (Newtonian) universe. The answer lies in theory of baryogenesis in the very early universe. The time-time component of Einstein's field equations for general relativity relate energy density to the geometry of space.
Professor Susskind introduces the topic of modern Cosmology, which started with the discovery of cosmic microwave background radiation in 1964. Leonard Susskind is the Felix Bloch Professor of Physics at Stanford University.\r\rComplete playlist for the course:\rhttp://youtube.com/view_play_list?p=189C0DCE90CB6D81\r\rStanford Continuing Studies: http://continuingstudies.stanford.edu/\r\rAbout Leonard Susskind: http://www.stanford.edu/dept/physics/people/faculty/susskind_leonard.html\r\rStanford University channel on YouTube:\rhttp://www.youtube.com/stanforduniversity
However, this lecture focuses on the classical or Newtonian view of … All Rights Reserved. Lecture 1 of Leonard Susskind's Modern Physics course concentrating on Quantum Mechanics. Recorded January 14, 2008 at Stanford University. For the past decade, Leonard Susskind, one of America's pre-eminent physicists, has taught a series of six courses in Stanford's Continuing Studies program. He was the first to introduce the idea of the string theory landscape in 2003. Professor Susskind develops the energy density allocation equation, and describes the historical progress of the effort to find the correct values for the terms in this equation. The series “explores the essential theoretical foundations of modern physics," helping lifelong learners (like you) attain the “theoretical minimum” for thinking intelligently about modern physics.
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