4.5.5. Black Holes
... ingoing particle will be redshifted by an increasing amount as the particle approaches the event horizon. Physically, one possible way to form black holes is through the collapse of stars or cluster of stars [see S.W.Hawkins, G.F.R.Ellis, “The Large-Scale Structure of Spacetime”, Cambridge Univ. Pre ...
... ingoing particle will be redshifted by an increasing amount as the particle approaches the event horizon. Physically, one possible way to form black holes is through the collapse of stars or cluster of stars [see S.W.Hawkins, G.F.R.Ellis, “The Large-Scale Structure of Spacetime”, Cambridge Univ. Pre ...
Ch.8 Rotational Equilibrium and Rotational Dynamics.
... Moment of Inertia For a point object: The moment of inertia is: I = mr2 m is the object mass and r is the distance to the axis of rotation. For a rigid body made up of more than one point, we need to add up the moments of inertia for each point. I = miri2 ...
... Moment of Inertia For a point object: The moment of inertia is: I = mr2 m is the object mass and r is the distance to the axis of rotation. For a rigid body made up of more than one point, we need to add up the moments of inertia for each point. I = miri2 ...
formation2
... • This over dense region is not uniform, but has within it other, smaller regions of high density. • As the over density begins to be drawn together by gravity, it fragments into smaller pockets of gas which go on to form individual stars. • The result is a star cluster. The more massive pockets fro ...
... • This over dense region is not uniform, but has within it other, smaller regions of high density. • As the over density begins to be drawn together by gravity, it fragments into smaller pockets of gas which go on to form individual stars. • The result is a star cluster. The more massive pockets fro ...
