The electrostatic force between the electron and nucleus is described by:
\[ F = \frac{K(Ze)(e)}{r^2} = \frac{mv^2}{r} \]
The electron's kinetic energy (KE) is calculated as:
\[ \text{KE} = \frac{1}{2}mv^2 = \frac{1}{2} \frac{K(Ze)(e)}{r} \]
Potential energy (PE) is defined as:
\[ \text{PE} = -\frac{K(Ze)(e)}{r} \]
Total energy (TE) is the sum of KE and PE:
\[ \text{TE} = \text{KE} + \text{PE} = \frac{K(Ze)(e)}{2r} + \left( -\frac{K(Ze)(e)}{r} \right) = -\frac{K(Ze)(e)}{2r} \]
Consequently, the relationship between total energy and potential energy is:
\[ 2 \times \text{TE} = \text{PE} \]
This simplifies to \( 2E = U \), aligning with Option (4).