The discussion focuses on the Schwarzschild metric in the context of a particle falling radially into a black hole. It emphasizes the importance of understanding the metric's implications for proper time, detailing how a particle's movement in spherical coordinates can be described mathematically. The equation provided illustrates the relationship between changes in proper time and the coordinates of the particle as it approaches the black hole. This foundational knowledge is crucial for grasping the dynamics of particles in strong gravitational fields. Mastery of this concept is essential for academic success in the course.
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Cythermax
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New poster has been reminded to show their work on schoolwork problems
Homework Statement
Attached it below
Relevant Equations
Not sure which equations necessary here.
I've been stuck starting anywhere with this. I need to finish this class for graduation and i'd like a safety net of a passing grade with this.
Well, do you know what the Schwarzschild metric is? In Schwarzschild (spherical) coordinates, if a particle starts at the point ##r, \theta, \phi## at time ##t## and travels a small distance to the point ##r+\delta r, \theta + \delta \theta, \phi + \delta \phi## by time ##t+\delta t##, then the the change in proper time ##\delta \tau## satisfies:
for d), I am a bit confused. I have two trains of thoughts here
any thoughts on which answer is correct, and why the other one is incorrect? Both seem like valid solutions to me. Or is the question ambiguous?
thanks