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COURSE CATALOGUE
Course Catalogue. The core sequence of six Theoretical Minimum courses covers Classical Mechanics through Statistical Mechanics and Cosmology. The core sequence is currently being repeated, so the six courses below are a mix of the old and new sequence. Earlier versions of the repeated courses can be found under the Archived Courses tab.LEONARD SUSSKIND
Leonard Susskind is the Felix Bloch Professor of Theoretical Physics at Stanford University, and Director of the Stanford Institute for Theoretical Physics. His research interests include string theory, quantum field theory, quantum statistical mechanics and quantum cosmology. He is a member of the National Academy of Sciences, and theAmerican
SUPPLEMENTAL COURSES| THE THEORETICAL MINIMUM The Theoretical Minimum courses include a core sequence of six courses, plus a set of supplemental courses that teach additional related material. The core sequence is currently being repeated with Statistical Mechanics being taught during Spring quarter, 2013. ENTROPY AND CONSERVATION OF INFORMATION In this sense, the conservation of information is more fundamental that other physical quantities such as temperature or energy. Professor Susskind then moves on to continuous systems and phase space, and Liouville's theorem. The lecture concludes with the presentation of formulas for computing entropy, and some examples. EINSTEIN FIELD EQUATIONS November 26, 2012. Professor Susskind derives the Einstein field equations of general relativity. Beginning with Newtonian gravitational fields, an analogy with the four-current, and the continuity equation, he develops the stress-energy tensor (also known as the energy momentum tensor). Putting these concepts together andgeneralizing the
SPECIAL RELATIVITY AND ELECTRODYNAMICS (SPRING, 2012 Spring, 2012. In 1905, while only twenty-six years old, Albert Einstein published "On the Electrodynamics of Moving Bodies" and effectively extended classical laws of relativity to all laws of physics, even electrodynamics. In this course, we will take a close look at the special theory of relativity and also at classical fieldtheory.
ENTANGLEMENT AND THE NATURE OF REALITY February 20, 2012. This lecture takes a deeper look at entanglement. Professor Susskind begins by discussing the wave function, which is the inner product of the system's state vector with the set of basis vectors, and how it contains probability amplitudes for the various states. He relates these probability amplitudes to the expectation RENORMALIZATION CONCEPTS, AND DIMENSIONAL ANALYSIS March 29, 2010. In the first lecture of the series Professor Susskind introduces the concept of renormalization, which allows elimination of as yet unknown physics at very tiny scales or high energies from our calculations of physics at accessible scales. He also connects dimensional analysis to the set of possible Lagrangians for ourtheories.
PRESSURE OF AN IDEAL GAS AND FLUCTUATIONS Professor Susskind derives the formula for the pressure of an ideal gas. He begins by introducing the Helmholtz free energy, and the concept of adiabatic processes. These concepts lead to the definition of pressure as the change of energy with volume at a fixed entropy, and then to the famous equation of state for an ideal gas: pV = NkT. THE THEORETICAL MINIMUMHOMECOURSESBIOGRAPHYABOUTREFERENCESLOG IN The Theoretical Minimum. A number of years ago I became aware of the large number of physics enthusiasts out there who have no venue to learn modern physics and cosmology. Fat advanced textbooks are not suitable to people who have no teacher to ask questions of, and the popular literature does not go deeply enough to satisfy these curiouspeople.
COURSE CATALOGUE
Course Catalogue. The core sequence of six Theoretical Minimum courses covers Classical Mechanics through Statistical Mechanics and Cosmology. The core sequence is currently being repeated, so the six courses below are a mix of the old and new sequence. Earlier versions of the repeated courses can be found under the Archived Courses tab.LEONARD SUSSKIND
Leonard Susskind is the Felix Bloch Professor of Theoretical Physics at Stanford University, and Director of the Stanford Institute for Theoretical Physics. His research interests include string theory, quantum field theory, quantum statistical mechanics and quantum cosmology. He is a member of the National Academy of Sciences, and theAmerican
SUPPLEMENTAL COURSES| THE THEORETICAL MINIMUM The Theoretical Minimum courses include a core sequence of six courses, plus a set of supplemental courses that teach additional related material. The core sequence is currently being repeated with Statistical Mechanics being taught during Spring quarter, 2013. ENTROPY AND CONSERVATION OF INFORMATION In this sense, the conservation of information is more fundamental that other physical quantities such as temperature or energy. Professor Susskind then moves on to continuous systems and phase space, and Liouville's theorem. The lecture concludes with the presentation of formulas for computing entropy, and some examples. EINSTEIN FIELD EQUATIONS November 26, 2012. Professor Susskind derives the Einstein field equations of general relativity. Beginning with Newtonian gravitational fields, an analogy with the four-current, and the continuity equation, he develops the stress-energy tensor (also known as the energy momentum tensor). Putting these concepts together andgeneralizing the
SPECIAL RELATIVITY AND ELECTRODYNAMICS (SPRING, 2012 Spring, 2012. In 1905, while only twenty-six years old, Albert Einstein published "On the Electrodynamics of Moving Bodies" and effectively extended classical laws of relativity to all laws of physics, even electrodynamics. In this course, we will take a close look at the special theory of relativity and also at classical fieldtheory.
ENTANGLEMENT AND THE NATURE OF REALITY February 20, 2012. This lecture takes a deeper look at entanglement. Professor Susskind begins by discussing the wave function, which is the inner product of the system's state vector with the set of basis vectors, and how it contains probability amplitudes for the various states. He relates these probability amplitudes to the expectation RENORMALIZATION CONCEPTS, AND DIMENSIONAL ANALYSIS March 29, 2010. In the first lecture of the series Professor Susskind introduces the concept of renormalization, which allows elimination of as yet unknown physics at very tiny scales or high energies from our calculations of physics at accessible scales. He also connects dimensional analysis to the set of possible Lagrangians for ourtheories.
PRESSURE OF AN IDEAL GAS AND FLUCTUATIONS Professor Susskind derives the formula for the pressure of an ideal gas. He begins by introducing the Helmholtz free energy, and the concept of adiabatic processes. These concepts lead to the definition of pressure as the change of energy with volume at a fixed entropy, and then to the famous equation of state for an ideal gas: pV = NkT. THE THEORETICAL MINIMUM The Theoretical Minimum is a series of Stanford Continuing Studies courses taught by world renowned physicist Leonard Susskind. These courses collectively teach everything required to gain a basic understanding of each area of modern physics including all of the fundamental mathematics. The sequence begins with the modernformulations of
LEONARD SUSSKIND
Leonard Susskind is the Felix Bloch Professor of Theoretical Physics at Stanford University, and Director of the Stanford Institute for Theoretical Physics. His research interests include string theory, quantum field theory, quantum statistical mechanics and quantum cosmology. He is a member of the National Academy of Sciences, and theAmerican
REFERENCES | THE THEORETICAL MINIMUM Books. Quantum Computer Science: An Introduction by N. David Mermin. It's About Time: Understanding Einstein's Relativity by N. David Mermin. Spacetime and Geometry: An Introduction to General Relativity by Sean Carroll. Quantum Physics: A Fundamental Approach to Modern Physics by John S. Townsend. The Inflationary Universe by Alan H.Guth.
COURSE ARCHIVE
This course of the Theoretical Minimum series will concentrate on cosmology, the science of the origin and development of the universe. Along the way, students will take a close look at the Big Bang, the geometry of space-time, inflationary cosmology, cosmic microwave background, dark matter, dark SUPPLEMENTAL COURSES| THE THEORETICAL MINIMUM The Theoretical Minimum courses include a core sequence of six courses, plus a set of supplemental courses that teach additional related material. The core sequence is currently being repeated with Statistical Mechanics being taught during Spring quarter, 2013. GENERAL RELATIVITY (FALL, 2012) General relativity is the geometric theory of gravitation published by Albert Einstein in 1916 and the current description of gravitation in modern physics. General relativity generalises special relativity and Newton's law of universal gravitation, providing a unified description of gravity as a geometric property of space and time, or spacetime. GEODESICS AND GRAVITY A geodesic is a path that is locally as straight as possible, which means that the derivative of the tangent vector is equal to zero at every point. Professor Susskind then moves on to relate the mathematics of Riemannian geometry (which we have been studying so far) to spacetime. Spacetime is represented by Minkowski space, whichhas a
UNCERTAINTY, UNITARY EVOLUTION, AND THE SCHRÖDINGER Professor Susskind then demonstrates how to solve the Schrödinger equation for a general quantum mechanical system. This solution is the origin of the connection between the energy of a system and oscillations of the wave function. This is the Heisenberg matrix formulation of quantum mechanics. The lecture concludes by solving apractical
COSMOLOGY AND BLACK HOLES (WINTER, 2011) Winter, 2011. In the last of course of this series, Leonard Susskind continues his exploration of string theory that attempts to reconcile quantum mechanics and general relativity. In particular, the course focuses on string theory with regard to important issues in contemporary physics. Topics include: 1) the impact of string theoryon the
CLASSICAL FIELD THEORY Professor Susskind moves on from relativity to introduce classical field theory. The most commonly studied classical field is the electromagnetic field; however, we will start with a less complex field - one in which the field values only depends on time - not on any spatial dimensions. THE THEORETICAL MINIMUMHOMECOURSESBIOGRAPHYABOUTREFERENCESLOG IN The Theoretical Minimum. A number of years ago I became aware of the large number of physics enthusiasts out there who have no venue to learn modern physics and cosmology. Fat advanced textbooks are not suitable to people who have no teacher to ask questions of, and the popular literature does not go deeply enough to satisfy these curiouspeople.
COURSE CATALOGUE
Course Catalogue. The core sequence of six Theoretical Minimum courses covers Classical Mechanics through Statistical Mechanics and Cosmology. The core sequence is currently being repeated, so the six courses below are a mix of the old and new sequence. Earlier versions of the repeated courses can be found under the Archived Courses tab. THE THEORETICAL MINIMUM The Theoretical Minimum is a series of Stanford Continuing Studies courses taught by world renowned physicist Leonard Susskind. These courses collectively teach everything required to gain a basic understanding of each area of modern physics including all of the fundamental mathematics. The sequence begins with the modernformulations of
LEONARD SUSSKIND
Leonard Susskind is the Felix Bloch Professor of Theoretical Physics at Stanford University, and Director of the Stanford Institute for Theoretical Physics. His research interests include string theory, quantum field theory, quantum statistical mechanics and quantum cosmology. He is a member of the National Academy of Sciences, and theAmerican
SUPPLEMENTAL COURSES| THE THEORETICAL MINIMUM The Theoretical Minimum courses include a core sequence of six courses, plus a set of supplemental courses that teach additional related material. The core sequence is currently being repeated with Statistical Mechanics being taught during Spring quarter, 2013. GENERAL RELATIVITY (FALL, 2012) General relativity is the geometric theory of gravitation published by Albert Einstein in 1916 and the current description of gravitation in modern physics. General relativity generalises special relativity and Newton's law of universal gravitation, providing a unified description of gravity as a geometric property of space and time, or spacetime. EINSTEIN FIELD EQUATIONS November 26, 2012. Professor Susskind derives the Einstein field equations of general relativity. Beginning with Newtonian gravitational fields, an analogy with the four-current, and the continuity equation, he develops the stress-energy tensor (also known as the energy momentum tensor). Putting these concepts together andgeneralizing the
MOTION IN AN ELECTROMAGNETIC FIELD According to Liouville's theorem, a system evolving according to Hamilton's equations conserves the volume of phase space. Information is conserved. The Principle of Least Action underlies Lagrangian and Hamiltonian methods. Investigate motion in an electromagnetic field. Demonstrate gauge invariance. Link time invariance and energyconservation.
ENTROPY AND CONSERVATION OF INFORMATION In this sense, the conservation of information is more fundamental that other physical quantities such as temperature or energy. Professor Susskind then moves on to continuous systems and phase space, and Liouville's theorem. The lecture concludes with the presentation of formulas for computing entropy, and some examples. CLASSICAL FIELD THEORY Professor Susskind moves on from relativity to introduce classical field theory. The most commonly studied classical field is the electromagnetic field; however, we will start with a less complex field - one in which the field values only depends on time - not on any spatial dimensions. THE THEORETICAL MINIMUMHOMECOURSESBIOGRAPHYABOUTREFERENCESLOG IN The Theoretical Minimum. A number of years ago I became aware of the large number of physics enthusiasts out there who have no venue to learn modern physics and cosmology. Fat advanced textbooks are not suitable to people who have no teacher to ask questions of, and the popular literature does not go deeply enough to satisfy these curiouspeople.
COURSE CATALOGUE
Course Catalogue. The core sequence of six Theoretical Minimum courses covers Classical Mechanics through Statistical Mechanics and Cosmology. The core sequence is currently being repeated, so the six courses below are a mix of the old and new sequence. Earlier versions of the repeated courses can be found under the Archived Courses tab. THE THEORETICAL MINIMUM The Theoretical Minimum is a series of Stanford Continuing Studies courses taught by world renowned physicist Leonard Susskind. These courses collectively teach everything required to gain a basic understanding of each area of modern physics including all of the fundamental mathematics. The sequence begins with the modernformulations of
LEONARD SUSSKIND
Leonard Susskind is the Felix Bloch Professor of Theoretical Physics at Stanford University, and Director of the Stanford Institute for Theoretical Physics. His research interests include string theory, quantum field theory, quantum statistical mechanics and quantum cosmology. He is a member of the National Academy of Sciences, and theAmerican
SUPPLEMENTAL COURSES| THE THEORETICAL MINIMUM The Theoretical Minimum courses include a core sequence of six courses, plus a set of supplemental courses that teach additional related material. The core sequence is currently being repeated with Statistical Mechanics being taught during Spring quarter, 2013. GENERAL RELATIVITY (FALL, 2012) General relativity is the geometric theory of gravitation published by Albert Einstein in 1916 and the current description of gravitation in modern physics. General relativity generalises special relativity and Newton's law of universal gravitation, providing a unified description of gravity as a geometric property of space and time, or spacetime. EINSTEIN FIELD EQUATIONS November 26, 2012. Professor Susskind derives the Einstein field equations of general relativity. Beginning with Newtonian gravitational fields, an analogy with the four-current, and the continuity equation, he develops the stress-energy tensor (also known as the energy momentum tensor). Putting these concepts together andgeneralizing the
MOTION IN AN ELECTROMAGNETIC FIELD According to Liouville's theorem, a system evolving according to Hamilton's equations conserves the volume of phase space. Information is conserved. The Principle of Least Action underlies Lagrangian and Hamiltonian methods. Investigate motion in an electromagnetic field. Demonstrate gauge invariance. Link time invariance and energyconservation.
ENTROPY AND CONSERVATION OF INFORMATION In this sense, the conservation of information is more fundamental that other physical quantities such as temperature or energy. Professor Susskind then moves on to continuous systems and phase space, and Liouville's theorem. The lecture concludes with the presentation of formulas for computing entropy, and some examples. CLASSICAL FIELD THEORY Professor Susskind moves on from relativity to introduce classical field theory. The most commonly studied classical field is the electromagnetic field; however, we will start with a less complex field - one in which the field values only depends on time - not on any spatial dimensions. REFERENCES | THE THEORETICAL MINIMUM Books. Quantum Computer Science: An Introduction by N. David Mermin. It's About Time: Understanding Einstein's Relativity by N. David Mermin. Spacetime and Geometry: An Introduction to General Relativity by Sean Carroll. Quantum Physics: A Fundamental Approach to Modern Physics by John S. Townsend. The Inflationary Universe by Alan H.Guth.
COURSE ARCHIVE
This course of the Theoretical Minimum series will concentrate on cosmology, the science of the origin and development of the universe. Along the way, students will take a close look at the Big Bang, the geometry of space-time, inflationary cosmology, cosmic microwave background, dark matter, dark COSMOLOGY (WINTER, 2013) This course of the Theoretical Minimum series will concentrate on cosmology, the science of the origin and development of the universe. Along the way, students will take a close look at the Big Bang, the geometry of space-time, inflationary cosmology, cosmic microwave background, dark matter, dark energy, the anthropic principle, and the string theory landscape. QUANTUM MECHANICS (WINTER, 2012) Winter, 2012. Quantum theory governs the universe at its most basic level. In the first half of the 20th century physics was turned on its head by the radical discoveries of Max Planck, Albert Einstein, Niels Bohr, Werner Heisenberg, and Erwin Schroedinger. An entire new logical and mathematical foundation—quantum mechanics—eventually GENERAL RELATIVITY (FALL, 2008) General Relativity. Fall, 2008. General relativity, or the general theory of relativity, is the geometric theory of gravitation published by Albert Einstein in 1916 and the current description of gravitation in modern physics. General relativity generalises special relativity and Newton's law of universal gravitation, providing a unified SPECIAL RELATIVITY AND ELECTRODYNAMICS (SPRING, 2012 Spring, 2012. In 1905, while only twenty-six years old, Albert Einstein published "On the Electrodynamics of Moving Bodies" and effectively extended classical laws of relativity to all laws of physics, even electrodynamics. In this course, we will take a close look at the special theory of relativity and also at classical fieldtheory.
STRING THEORY (FALL, 2010) String Theory. Fall, 2010. In this set of lectures Professor Susskind gives an introduction to String Theory, which he describes as a mathematical framework for theories that unify all the forces of nature, including gravity. In string theory, fundamental objects are no longer point particles; instead they are strings or higherdimensional
RELATIVITY (SPRING, 2007) Spring, 2007. This course takes a deeper look at relativity. Most of the course focuses on Einstein's special theory of relativity. General relativity is introduced in the last few lectures. (Image credit: KIPAC at Stanford University) iTunes Playlist. YouTube Playlist. CLASSICAL MECHANICS (FALL, 2011) Classical Mechanics. Fall, 2011. Our exploration of the theoretical underpinnings of modern physics begins with classical mechanics, the mathematical physics worked out by Isaac Newton (1642--1727) and later by Joseph Lagrange (1736--1813) and William Rowan Hamilton (1805--1865). We will start with a discussion of the allowable laws ofphysics
RENORMALIZATION CONCEPTS, AND DIMENSIONAL ANALYSIS March 29, 2010. In the first lecture of the series Professor Susskind introduces the concept of renormalization, which allows elimination of as yet unknown physics at very tiny scales or high energies from our calculations of physics at accessible scales. He also connects dimensional analysis to the set of possible Lagrangians for ourtheories.
THE THEORETICAL MINIMUMHOMECOURSESBIOGRAPHYABOUTREFERENCESLOG IN The Theoretical Minimum. A number of years ago I became aware of the large number of physics enthusiasts out there who have no venue to learn modern physics and cosmology. Fat advanced textbooks are not suitable to people who have no teacher to ask questions of, and the popular literature does not go deeply enough to satisfy these curiouspeople.
COURSE CATALOGUE
Course Catalogue. The core sequence of six Theoretical Minimum courses covers Classical Mechanics through Statistical Mechanics and Cosmology. The core sequence is currently being repeated, so the six courses below are a mix of the old and new sequence. Earlier versions of the repeated courses can be found under the Archived Courses tab. THE THEORETICAL MINIMUM The Theoretical Minimum is a series of Stanford Continuing Studies courses taught by world renowned physicist Leonard Susskind. These courses collectively teach everything required to gain a basic understanding of each area of modern physics including all of the fundamental mathematics. The sequence begins with the modernformulations of
LEONARD SUSSKIND
Leonard Susskind is the Felix Bloch Professor of Theoretical Physics at Stanford University, and Director of the Stanford Institute for Theoretical Physics. His research interests include string theory, quantum field theory, quantum statistical mechanics and quantum cosmology. He is a member of the National Academy of Sciences, and theAmerican
SUPPLEMENTAL COURSES| THE THEORETICAL MINIMUM The Theoretical Minimum courses include a core sequence of six courses, plus a set of supplemental courses that teach additional related material. The core sequence is currently being repeated with Statistical Mechanics being taught during Spring quarter, 2013. GENERAL RELATIVITY (FALL, 2012) General relativity is the geometric theory of gravitation published by Albert Einstein in 1916 and the current description of gravitation in modern physics. General relativity generalises special relativity and Newton's law of universal gravitation, providing a unified description of gravity as a geometric property of space and time, or spacetime. EINSTEIN FIELD EQUATIONS November 26, 2012. Professor Susskind derives the Einstein field equations of general relativity. Beginning with Newtonian gravitational fields, an analogy with the four-current, and the continuity equation, he develops the stress-energy tensor (also known as the energy momentum tensor). Putting these concepts together andgeneralizing the
MOTION IN AN ELECTROMAGNETIC FIELD According to Liouville's theorem, a system evolving according to Hamilton's equations conserves the volume of phase space. Information is conserved. The Principle of Least Action underlies Lagrangian and Hamiltonian methods. Investigate motion in an electromagnetic field. Demonstrate gauge invariance. Link time invariance and energyconservation.
ENTROPY AND CONSERVATION OF INFORMATION In this sense, the conservation of information is more fundamental that other physical quantities such as temperature or energy. Professor Susskind then moves on to continuous systems and phase space, and Liouville's theorem. The lecture concludes with the presentation of formulas for computing entropy, and some examples. CLASSICAL FIELD THEORY Professor Susskind moves on from relativity to introduce classical field theory. The most commonly studied classical field is the electromagnetic field; however, we will start with a less complex field - one in which the field values only depends on time - not on any spatial dimensions. THE THEORETICAL MINIMUMHOMECOURSESBIOGRAPHYABOUTREFERENCESLOG IN The Theoretical Minimum. A number of years ago I became aware of the large number of physics enthusiasts out there who have no venue to learn modern physics and cosmology. Fat advanced textbooks are not suitable to people who have no teacher to ask questions of, and the popular literature does not go deeply enough to satisfy these curiouspeople.
COURSE CATALOGUE
Course Catalogue. The core sequence of six Theoretical Minimum courses covers Classical Mechanics through Statistical Mechanics and Cosmology. The core sequence is currently being repeated, so the six courses below are a mix of the old and new sequence. Earlier versions of the repeated courses can be found under the Archived Courses tab. THE THEORETICAL MINIMUM The Theoretical Minimum is a series of Stanford Continuing Studies courses taught by world renowned physicist Leonard Susskind. These courses collectively teach everything required to gain a basic understanding of each area of modern physics including all of the fundamental mathematics. The sequence begins with the modernformulations of
LEONARD SUSSKIND
Leonard Susskind is the Felix Bloch Professor of Theoretical Physics at Stanford University, and Director of the Stanford Institute for Theoretical Physics. His research interests include string theory, quantum field theory, quantum statistical mechanics and quantum cosmology. He is a member of the National Academy of Sciences, and theAmerican
SUPPLEMENTAL COURSES| THE THEORETICAL MINIMUM The Theoretical Minimum courses include a core sequence of six courses, plus a set of supplemental courses that teach additional related material. The core sequence is currently being repeated with Statistical Mechanics being taught during Spring quarter, 2013. GENERAL RELATIVITY (FALL, 2012) General relativity is the geometric theory of gravitation published by Albert Einstein in 1916 and the current description of gravitation in modern physics. General relativity generalises special relativity and Newton's law of universal gravitation, providing a unified description of gravity as a geometric property of space and time, or spacetime. EINSTEIN FIELD EQUATIONS November 26, 2012. Professor Susskind derives the Einstein field equations of general relativity. Beginning with Newtonian gravitational fields, an analogy with the four-current, and the continuity equation, he develops the stress-energy tensor (also known as the energy momentum tensor). Putting these concepts together andgeneralizing the
MOTION IN AN ELECTROMAGNETIC FIELD According to Liouville's theorem, a system evolving according to Hamilton's equations conserves the volume of phase space. Information is conserved. The Principle of Least Action underlies Lagrangian and Hamiltonian methods. Investigate motion in an electromagnetic field. Demonstrate gauge invariance. Link time invariance and energyconservation.
ENTROPY AND CONSERVATION OF INFORMATION In this sense, the conservation of information is more fundamental that other physical quantities such as temperature or energy. Professor Susskind then moves on to continuous systems and phase space, and Liouville's theorem. The lecture concludes with the presentation of formulas for computing entropy, and some examples. CLASSICAL FIELD THEORY Professor Susskind moves on from relativity to introduce classical field theory. The most commonly studied classical field is the electromagnetic field; however, we will start with a less complex field - one in which the field values only depends on time - not on any spatial dimensions. REFERENCES | THE THEORETICAL MINIMUM Books. Quantum Computer Science: An Introduction by N. David Mermin. It's About Time: Understanding Einstein's Relativity by N. David Mermin. Spacetime and Geometry: An Introduction to General Relativity by Sean Carroll. Quantum Physics: A Fundamental Approach to Modern Physics by John S. Townsend. The Inflationary Universe by Alan H.Guth.
COURSE ARCHIVE
This course of the Theoretical Minimum series will concentrate on cosmology, the science of the origin and development of the universe. Along the way, students will take a close look at the Big Bang, the geometry of space-time, inflationary cosmology, cosmic microwave background, dark matter, dark COSMOLOGY (WINTER, 2013) This course of the Theoretical Minimum series will concentrate on cosmology, the science of the origin and development of the universe. Along the way, students will take a close look at the Big Bang, the geometry of space-time, inflationary cosmology, cosmic microwave background, dark matter, dark energy, the anthropic principle, and the string theory landscape. QUANTUM MECHANICS (WINTER, 2012) Winter, 2012. Quantum theory governs the universe at its most basic level. In the first half of the 20th century physics was turned on its head by the radical discoveries of Max Planck, Albert Einstein, Niels Bohr, Werner Heisenberg, and Erwin Schroedinger. An entire new logical and mathematical foundation—quantum mechanics—eventually GENERAL RELATIVITY (FALL, 2008) General Relativity. Fall, 2008. General relativity, or the general theory of relativity, is the geometric theory of gravitation published by Albert Einstein in 1916 and the current description of gravitation in modern physics. General relativity generalises special relativity and Newton's law of universal gravitation, providing a unified SPECIAL RELATIVITY AND ELECTRODYNAMICS (SPRING, 2012 Spring, 2012. In 1905, while only twenty-six years old, Albert Einstein published "On the Electrodynamics of Moving Bodies" and effectively extended classical laws of relativity to all laws of physics, even electrodynamics. In this course, we will take a close look at the special theory of relativity and also at classical fieldtheory.
STRING THEORY (FALL, 2010) String Theory. Fall, 2010. In this set of lectures Professor Susskind gives an introduction to String Theory, which he describes as a mathematical framework for theories that unify all the forces of nature, including gravity. In string theory, fundamental objects are no longer point particles; instead they are strings or higherdimensional
RELATIVITY (SPRING, 2007) Spring, 2007. This course takes a deeper look at relativity. Most of the course focuses on Einstein's special theory of relativity. General relativity is introduced in the last few lectures. (Image credit: KIPAC at Stanford University) iTunes Playlist. YouTube Playlist. CLASSICAL MECHANICS (FALL, 2011) Classical Mechanics. Fall, 2011. Our exploration of the theoretical underpinnings of modern physics begins with classical mechanics, the mathematical physics worked out by Isaac Newton (1642--1727) and later by Joseph Lagrange (1736--1813) and William Rowan Hamilton (1805--1865). We will start with a discussion of the allowable laws ofphysics
RENORMALIZATION CONCEPTS, AND DIMENSIONAL ANALYSIS March 29, 2010. In the first lecture of the series Professor Susskind introduces the concept of renormalization, which allows elimination of as yet unknown physics at very tiny scales or high energies from our calculations of physics at accessible scales. He also connects dimensional analysis to the set of possible Lagrangians for ourtheories.
THE THEORETICAL MINIMUMHOMECOURSESBIOGRAPHYABOUTREFERENCESLOG IN A number of years ago I became aware of the large number of physics enthusiasts out there who have no venue to learn modern physics andcosmology.
COURSE CATALOGUE
The core sequence of six Theoretical Minimum courses covers Classical Mechanics through Statistical Mechanics and Cosmology. The core sequence is currently being repeated, so the six courses below are a mix of the old and new sequence. THE THEORETICAL MINIMUM The Theoretical Minimum is a series of Stanford Continuing Studies courses taught by world renowned physicist Leonard Susskind. These courses collectively teach everything required to gain a basic understanding of each area of modern physics including all of the fundamental mathematics.LEONARD SUSSKIND
Leonard Susskind is the Felix Bloch Professor of Theoretical Physics at Stanford University, and Director of the Stanford Institute for Theoretical Physics. SUPPLEMENTAL COURSES| THE THEORETICAL MINIMUM The Theoretical Minimum courses include a core sequence of six courses, plus a set of supplemental courses that teach additional related material. The core sequence is currently being repeated with Statistical Mechanics being taught during Spring quarter, 2013. GENERAL RELATIVITY (FALL, 2012) General relativity is the geometric theory of gravitation published by Albert Einstein in 1916 and the current description of gravitation inmodern physics.
EINSTEIN FIELD EQUATIONS Professor Susskind derives the Einstein field equations of general relativity. Beginning with Newtonian gravitational fields, an analogy with the four-current, and the continuity equation, he develops the stress-energy tensor (also known as the energy momentum tensor). ENTROPY AND CONSERVATION OF INFORMATION Professor Susskind introduces statistical mechanics as one of the most universal subjects in modern physics in terms of it's ability to explain and predict natural phenomena. CLASSICAL FIELD THEORY Professor Susskind moves on from relativity to introduce classical field theory. The most commonly studied classical field is the electromagnetic field; however, we will start with a less complex field - one in which the field values only depends on time - not on any spatial dimensions. MOTION IN AN ELECTROMAGNETIC FIELD According to Liouville's theorem, a system evolving according to Hamilton's equations conserves the volume of phase space. Informationis conserved.
THE THEORETICAL MINIMUMHOMECOURSESBIOGRAPHYABOUTREFERENCESLOG IN A number of years ago I became aware of the large number of physics enthusiasts out there who have no venue to learn modern physics andcosmology.
COURSE CATALOGUE
The core sequence of six Theoretical Minimum courses covers Classical Mechanics through Statistical Mechanics and Cosmology. The core sequence is currently being repeated, so the six courses below are a mix of the old and new sequence. THE THEORETICAL MINIMUM The Theoretical Minimum is a series of Stanford Continuing Studies courses taught by world renowned physicist Leonard Susskind. These courses collectively teach everything required to gain a basic understanding of each area of modern physics including all of the fundamental mathematics.LEONARD SUSSKIND
Leonard Susskind is the Felix Bloch Professor of Theoretical Physics at Stanford University, and Director of the Stanford Institute for Theoretical Physics. SUPPLEMENTAL COURSES| THE THEORETICAL MINIMUM The Theoretical Minimum courses include a core sequence of six courses, plus a set of supplemental courses that teach additional related material. The core sequence is currently being repeated with Statistical Mechanics being taught during Spring quarter, 2013. GENERAL RELATIVITY (FALL, 2012) General relativity is the geometric theory of gravitation published by Albert Einstein in 1916 and the current description of gravitation inmodern physics.
EINSTEIN FIELD EQUATIONS Professor Susskind derives the Einstein field equations of general relativity. Beginning with Newtonian gravitational fields, an analogy with the four-current, and the continuity equation, he develops the stress-energy tensor (also known as the energy momentum tensor). ENTROPY AND CONSERVATION OF INFORMATION Professor Susskind introduces statistical mechanics as one of the most universal subjects in modern physics in terms of it's ability to explain and predict natural phenomena. CLASSICAL FIELD THEORY Professor Susskind moves on from relativity to introduce classical field theory. The most commonly studied classical field is the electromagnetic field; however, we will start with a less complex field - one in which the field values only depends on time - not on any spatial dimensions. MOTION IN AN ELECTROMAGNETIC FIELD According to Liouville's theorem, a system evolving according to Hamilton's equations conserves the volume of phase space. Informationis conserved.
REFERENCES | THE THEORETICAL MINIMUM Theoretical Minimum Books. The Theoretical Minimum: What You Need to Know to Start Doing Physics (with George Hrabovsky). Quantum Mechanics: The Theoretical Minimum (with Art Friedman). Other Books byLeonard Susskind
COURSE ARCHIVE
This course of the Theoretical Minimum series will concentrate on cosmology, the science of the origin and development of the universe. Along the way, students will take a close look at the Big Bang, the geometry of space-time, inflationary cosmology, cosmic microwave background, dark matter, dark COSMOLOGY (WINTER, 2013) This course of the Theoretical Minimum series will concentrate on cosmology, the science of the origin and development of the universe. Along the way, students will take a close look at the Big Bang, the geometry of space-time, inflationary cosmology, cosmic microwave background, dark matter, dark energy, the anthropic principle, and the string theory landscape. QUANTUM MECHANICS (WINTER, 2012) Quantum theory governs the universe at its most basic level. In the first half of the 20th century physics was turned on its head by the radical discoveries of Max Planck, Albert Einstein, Niels Bohr, Werner Heisenberg, and Erwin Schroedinger. CLASSICAL MECHANICS (FALL, 2011) Our exploration of the theoretical underpinnings of modern physics begins with classical mechanics, the mathematical physics worked out by Isaac Newton (1642--1727) and later by Joseph Lagrange (1736--1813) and William Rowan Hamilton (1805--1865). SPECIAL RELATIVITY AND ELECTRODYNAMICS (SPRING, 2012 In 1905, while only twenty-six years old, Albert Einstein published "On the Electrodynamics of Moving Bodies" and effectively extended classical laws of relativity to all laws of physics, evenelectrodynamics.
GENERAL RELATIVITY (FALL, 2008) General relativity, or the general theory of relativity, is the geometric theory of gravitation published by Albert Einstein in 1916 and the current description of gravitation in modern physics. STRING THEORY (FALL, 2010) In the first lecture of the series Professor Susskind explains the historical origins of string theory. Hadrons are observed to come in angular momentum sequences where a plot of angular momentum against mass squared is a straight line. RENORMALIZATION CONCEPTS, AND DIMENSIONAL ANALYSIS In the first lecture of the series Professor Susskind introduces the concept of renormalization, which allows elimination of as yet unknown physics at very tiny scales or high energies from our calculations of physics at accessible scales. RELATIVITY (SPRING, 2007) This course takes a deeper look at relativity. Most of the course focuses on Einstein's special theory of relativity. General relativity is introduced in the last few lectures.(Image credit: Skip to main content THE THEORETICAL MINIMUMSEARCH FORM
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> A number of years ago I became aware of the large number of physics > enthusiasts out there who have no venue to learn modern physics and > cosmology. Fat advanced textbooks are not suitable to people who > have no teacher to ask questions of, and the popular literature does > not go deeply enough to satisfy these curious people. So I started > a series of courses on modern physics at Stanford University where I > am a professor of physics. The courses are specifically aimed at > people who know, or once knew, a bit of algebra and calculus, but > are more or less beginners.HOME
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