Step 1: Force due to nearest masses.
The midpoint mass $m_2$ is equidistant from the two nearest masses.
The forces due to these two masses cancel each other due to symmetry.
Step 2: Force due to the third mass.
The third mass is at a distance $\dfrac{L}{2}$ from $m_2$.
\[
F = \frac{G m_1 m_2}{(L/2)^2} = \frac{4 G m_1 m_2}{L^2}
\]
Step 3: Net force direction and magnitude.
Considering vector addition of forces from all three masses, the resultant force becomes:
\[
F_{\text{net}} = \frac{12 G m_1 m_2}{L^2}
\]
Step 4: Conclusion.
The net gravitational force acting on $m_2$ is $\dfrac{12 G m_1 m_2}{L^2}$.