User:
Pass:
Remember Me
Forgot Pass Register

Our educational work is entirely supported by people like you. Your donations directly add new exhibits and new features to the website, and even helps us open the Prehistoria Natural History Center!




eXTReMe Tracker

Schools / M.I.T. / 8.224 Exploring Black Holes: General Relativity and Astrophysics / Lecture 3: Einstein's Field Equations







Lecture 3: Einstein's Field Equations
  • Currently 2.72/5
  • 1
  • 2
  • 3
  • 4
  • 5
Rating: 2.7 / 5 (1032 votes)
Click Here For More Lectures In This Course
Loading the player...

Lecture 3: Einstein's Field Equations
In this lecture Edmund Bertschinger tackles Einstein's Field Equations, revealing the history of our understanding of curved spacetime and the mathematical and physical implications of this discovery.

Additional Information:


Posted by nova on June 19, 2011 at 4:47 pm
Hits: 5945 | Comments: 0
Send to a Friend

More Free Lectures

Lecture 1: Introduction to Astrobiology
Lecture 1: Introduction to Astrobiology
Type: Stanford University
Lecture 12: Hematology I
Lecture 12: Hematology I
Type: Berkeley
Lecture 37: Endocrine System
Lecture 37: Endocrine System
Type: Berkeley
Lecture 26: Peripheral Nerves
Lecture 26: Peripheral Nerves
Type: Berkeley
Lecture 5: Fermions & Energy Conservation
Lecture 5: Fermions & Energy Conservation
Type: Stanford University
Lecture 4: From Orson Welles To The Dead
Lecture 4: From Orson Welles To The Dead
Type: M.I.T.
Lecture 3: The Search for Other Earths and Life in the Universe
Lecture 3: The Search for Other Earths and Life in the Universe
Type: Stanford University
Lecture 38: Female Reproductive System
Lecture 38: Female Reproductive System
Type: Berkeley
Lecture 8: Dirac Equation & Particle Spin
Lecture 8: Dirac Equation & Particle Spin
Type: Stanford University
Lecture 28: Motor Pathways & The Forebrain
Lecture 28: Motor Pathways & The Forebrain
Type: Berkeley
Lecture 07: Skeletal System VI
Lecture 07: Skeletal System VI
Type: Berkeley
Lecture 10: Path Integral Formulation
Lecture 10: Path Integral Formulation
Type: Stanford University
Lecture 6: Cosmic Structure Formation, From Inflation to Galaxies
Lecture 6: Cosmic Structure Formation, From Inflation to Galaxies
Type: M.I.T.
Lecture 8: Catastrophic Impacts in Earth's History
Lecture 8: Catastrophic Impacts in Earth's History
Type: Stanford University
Lecture 2: From Astrochemistry to Astrobiology
Lecture 2: From Astrochemistry to Astrobiology
Type: Stanford University

Comments

There are no comments on this item.
User: Pass: Remember Me

To comment on this item, please login or register.