Part 2 Evolution to Black Hole of a Large Gas Ball

Here we look at the experience of a human-scale observer inside a ball of gas which may be quite dilute but is large enough to form a black hole.

Again the key quantity that we consider is the red shift for signals between and within parts of the observer and we shall refer to the formula for gravitational red shift per meter that we obtain in Lemma 2

Leave a Reply

Your email address will not be published.