What is called innermost stable circular orbit radius?
10
What is the amount of precision compared to the Kepler problem in Newtonian theory?
11
Newtonian theory
12
What are the typical velocities in solar system?
13
Newtonian theory - Orbit is basically a conic section ellipse
14
Q&A
15
Analgesic equation
16
Light orbits
17
What is the effective potential?
18
Photon
19
Photon energies is lower than by L square by 2m
20
Q&A
21
Introduction of Karrdometric
22
What is the idea that fortune solution represents a static geometry?
23
Stationary; Axis symmetric
24
Coordinate system
25
What do you mean my gravitational radiation?
26
Q&A
Description:
Delve into the second lecture of an advanced course on general relativity, exploring effective equations for test particles, Newtonian theory, and relativistic orbits. Examine bound orbits, innermost stable circular orbits, and light trajectories in gravitational fields. Compare Newtonian and general relativistic approaches to orbital mechanics, discussing precision and typical velocities in the solar system. Investigate effective potentials, photon orbits, and the introduction of Kerr metric for stationary, axisymmetric spacetimes. Engage with concepts like gravitational radiation and static geometries through detailed explanations and Q&A sessions, enhancing understanding of advanced topics in general relativity.