Introduction to Black Holes
Μεταφορτώθηκε στις 29 Σεπ 2008
Frontiers/Controversies in Astrophysics (ASTR 160)
The
second half of the course begins, focusing on black holes and
relativity. In introducing black holes, Professor Bailyn offers a
definition, talks about how their existence is detected, and explains
why (unlike in the case with exoplanets where Newtonian physics was
applied) Einstein's Theory of Relativity is now required when studying
black holes. The concepts of escape and circular velocity are
introduced. A number of problems are worked out and students learn how
to calculate an object's escape velocity. A historical overview is
offered of our understanding and discovery of black holes in the context
of stellar evolution.
00:00 - Chapter 1. Introduction
02:38 - Chapter 2. Escape Velocity
12:12 - Chapter 3. Defining Black Holes and the Schwarzschild Radius
18:50 - Chapter 4. Gravity and Pressure in the Evolution of Stars
28:06 - Chapter 5. From Electron Degeneracy Pressure to the Chandrasekhar Limit
37:59 - Chapter 6. Neutron Stars
42:38 - Chapter 7. Conclusion
Complete course materials are available at the Open Yale Courses website: http://open.yale.edu/courses
This course was recorded in Spring 2007.
The
second half of the course begins, focusing on black holes and
relativity. In introducing black holes, Professor Bailyn offers a
definition, talks about how their existence is detected, and explains
why (unlike in the case with exoplanets where Newtonian physics was
applied) Einstein's Theory of Relativity is now required when studying
black holes. The concepts of escape and circular velocity are
introduced. A number of problems are worked out and students learn how
to calculate an object's escape velocity. A historical overview is
offered of our understanding and discovery of black holes in the context
of stellar evolution.
00:00 - Chapter 1. Introduction
02:38 - Chapter 2. Escape Velocity
12:12 - Chapter 3. Defining Black Holes and the Schwarzschild Radius
18:50 - Chapter 4. Gravity and Pressure in the Evolution of Stars
28:06 - Chapter 5. From Electron Degeneracy Pressure to the Chandrasekhar Limit
37:59 - Chapter 6. Neutron Stars
42:38 - Chapter 7. Conclusion
Complete course materials are available at the Open Yale Courses website: http://open.yale.edu/courses
This course was recorded in Spring 2007.
ANAΡΤΗΣΗ ΑΠΟ ΤΟ YOUTUBE 20/3/2014
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