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The Character of Physical Law (Messenger Lectures) →0/7
1

The Law of Gravitation, an Example of Physical Law

55:26
2

The Relation of Mathematics to Physics

55:28
3

The Great Conservation Principles

55:54
4

Symmetry in Physical Law

56:51
5

The Distinction of Past and Future

46:11
6

Probability and Uncertainty: The Quantum Mechanical View of Nature

56:09
7

Seeking New Laws: Theory, Prediction, and Observation

57:53

The Distinction of Past and Future

Richard FeynmanNobel LaureateCornell University

Nobel Laureate in Physics

46:11·2018·introductory level

Traces how microscopic time-reversible dynamical laws give rise to macroscopic irreversibility, thermodynamic entropy growth, and a cosmological low-entropy boundary condition.

MathematicsPhysicsProbability & Information TheoryRichard P. FeynmanPhysics

Richard P. Feynman Lecture Cornell University 1964

Source: Mark Stump via YouTubeWatch on YouTube
LecturerAll lecturers →
Richard FeynmanNobel Laureate

Nobel Prize in Physics (1965)

Nobel Laureate in Physics renowned for quantum electrodynamics, path-integral formulation, and The Feynman Lectures on Physics.

1 course · 9 lecturesCanon
Previous · Lecture 4

Symmetry in Physical Law

Next · Lecture 6

Probability and Uncertainty: The Quantum Mechanical View of Nature

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