How Do I Calculate Coulomb's Law for Fractional Electrical Charges?

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To calculate Coulomb's Law for fractional electrical charges, the fractional value can be directly used in the formula F = K * (qa * qb / r^2). If the charge is +2/3, it should be plugged in as 2/3 in the q's spot. The unit of charge is Coulombs, and for two charges of +2/3 C, the calculation would be F = (8.98e9)(2/3)^2 / r^2. Understanding the relationship between fractional charges and their representation in Coulombs is crucial for accurate calculations.
robertroman10
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The law I am talking about is F=K* (qa*qb / r2) I know the values of all but I have a question on the q's which represent the electrical charges...
If the charge is +2/3 do I plug in the fraction 2/3 in the q's spot? is this the numerical number I use? PLEASE HELP!
 
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robertroman10 said:
The law I am talking about is F=K* (qa*qb / r2) I know the values of all but I have a question on the q's which represent the electrical charges...
If the charge is +2/3 do I plug in the fraction 2/3 in the q's spot? is this the numerical number I use? PLEASE HELP!
Are you trying to find the coulomb force between two charges of +2e/3?

AM
 
Yess
 
OK, so what unit is charge measured in? How much is e in those units? So how much then is 2/3e?
 
robertroman10 said:
The law I am talking about is F=K* (qa*qb / r2) I know the values of all but I have a question on the q's which represent the electrical charges...
If the charge is +2/3 do I plug in the fraction 2/3 in the q's spot? is this the numerical number I use? PLEASE HELP!

If both of the charges are +2/3 C, then you just plug in the charges for q

F = KQQ / R^2
F = (8.98e9)(2/3)^2 / R^2

The units for charge are Coulombs.
 
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ok thanks
 
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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