When the mass leaves the contact from the hemisphere, then R = 0, so, mgcos
=
.
cos
=
 —– (i)
We draw a perpendicular QS on PO. Therefore, SO = h = rcos
.
Using conservation of energy at point P and Q we get,
+ mg(PS) = 
Or,
 + mg(r- rcos
) = 
Or,
 =
+ 2gr(1- cos
)
u = 
Putting the value of u in equation (i) we get, cos
=
Â
Or, cos
=
+ 2 – 2cos
Or, 3cos
 =
 + 2 Â
=
.