In my model, masses are concentrated at the nodes where columns and beams meet according to the tributary mass per node. I use rigid diaphragm constraint to each floor and each floor has three freedoms: UX, UY and RZ.
So I define mass as follow:
mass $node $m $m 0 0 0 0
Can opensees calculate the rotational inertia of the mass to the centre of the rigid diaphragm automatically? If it can’t, should I define the mass as:
mass $node $m $m 0 0 0 $m*d^2
d represent the distance between the mass and the centre of the rigid diaphragm.
thanks
rotational inertia of the mass
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