MCS5280
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Homework Statement
a. The first part of this problem was to derive the escape speed (Vesc) for a star of mass M and radius R.
b. The second part is where I am having trouble. It says to equate the Vesc calculated above and derive a formula for Planck length in terms of c, G, and h_bar.
Homework Equations
This is from the Heisenberg uncertainty section for position and momentum so:
\DeltaX * \DeltaP = h_bar/2
E = mc2
The Attempt at a Solution
The escape velocity I calculated from part a was Vesc = \sqrt{2GM/R}
Equating Vesc to C gives:
C = \sqrt{2GM/R}
Am I supposed to assume that \Deltap = Mc and solve for \Deltax using the Heisenberg uncertainty principle?
I have tried a couple of different methods and I can't get this to simplify down to the form I need. I am pretty sure this is an easy problem, I just am not seeing the trick.