Electron repulsion per unit volume

AI Thread Summary
To calculate the number of electrons needed to exert a pressure of 1 psi in a cubic centimeter, it's important to consider the collective repulsion among trillions of electrons. The challenge lies in accounting for the interactions, particularly for those electrons at the edges of the cube, as they experience different forces compared to those in the center. A suggested approach is to calculate the energy of a sphere with a given radius and total charge, then analyze how this energy changes with respect to radius to derive the necessary electron density. Additional references or resources may be required for more detailed calculations. Understanding these concepts is crucial for accurate modeling of electron behavior in confined spaces.
taylaron
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Hi, I am trying to calculate how many electrons I need to confine in one cubic centimeter to make the pressure on the "walls" 1psi. I've tried the equation for the repulsion of two charges, but we're talking about trillions of electrons here and they're all pushing on each other however slightly. Yes, the force exerted on the electrons toward the center of the cube will have neutral net repulsion but its the ones on the edge that stump my calculations.
Could anyone help me out here or suggest a reference?

Thanks in advance-

-Tay
 
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You can calculate the energy of a sphere (that's probably the easiest shape to start with) of radius R and total charge Q, and then look at dE/dr.
 
Sorry, the wrong topic
 
It may be shown from the equations of electromagnetism, by James Clerk Maxwell in the 1860’s, that the speed of light in the vacuum of free space is related to electric permittivity (ϵ) and magnetic permeability (μ) by the equation: c=1/√( μ ϵ ) . This value is a constant for the vacuum of free space and is independent of the motion of the observer. It was this fact, in part, that led Albert Einstein to Special Relativity.
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