Answer:
[tex]T=3Mg[/tex]
Explanation:
Let's apply the conservation of energy between points A and B.
We just have gravitational potential energy at point A and just kinetic energy at point B.
[tex]MgL=\frac{1}{2}Mv^{2}[/tex] (1)
Now, let's apply force free-body diagram at point B, we have the tension upwards and weight downwards. Now using Newton's second law we have:
[tex]\sum F=Ma_{c}[/tex]
As we have circular motion, we use centripetal acceleration here (a(c)=v²/R). The forces acting are:
[tex]T-W_{bob}=Ma_{c}=M\frac{v^{2}}{L}[/tex], because the radius R is L.
So let's solve this equation for T.
[tex]T=W_{bob}+M\frac{v^{2}}{L}=Mg+M\frac{v^{2}}{L}[/tex] (2)
Using equation (1) we can find v².
[tex]v^{2}=2gL[/tex]
Finally let's put this value in the equation (2).
[tex]T=Mg+M\frac{2gL}{L}[/tex]
[tex]T=3Mg[/tex]
I hope it helps you!