ehild said:
I think it significant. I tried but I failed.
OK. The objective is to get an estimate of the effect of the mg/2 portion of the tension in the lower rope on the radial component of tension in the upper rope. I'm going to start out by writing down the force balance equations on mass A, including the angulation effect of the two ropes (which was neglected in the previous development):
$$T'cosθ'-Tsinθ=ma_x $$
$$-T'sinθ'+Tcosθ-mg=ma_y$$
The first equation is the force balance in the horizontal direction, the second equation is the force balance in the vertical direction, the x-direction is to the left, the y-direction is upward, T' is the tension in the lower rope, and θ' is the angle that the lower rope makes with the horizontal. If we multiply the second equation by cosθ and the first equation by sinθ, and then subtract the first equation from the second equation, we obtain the component of the force balance in the radial direction:
$$-T'sin(θ+θ')+T-mg\cosθ=-ma_r=m\left[r\left(\frac{dθ}{dt}\right)^2-\frac{d^2r}{dt^2}\right]$$
The focus of the present analysis is the first term on the left hand side of this equation. Our first objective is to obtain an upper bound to the angle θ+θ' at the end of the collision, effectively at t =4τ, where t = (m/3C). If we integrate our equation for the x-velocity over this time interval, we obtain $$δx=v_0τ$$where δx is the x displacement during the time period. From this, it follows that the angle θ is given by:
$$θ=\frac{v_0τ}{l}$$
We can obtain an upper bound to the angle θ' by assuming that the mass A follows a circular arc, rather than also including the outward radial component of velocity along the upper rope. This will result in an upper bound to the predicted vertical displacement δ
y of mass A. So,
$$δ_y=l-lcosθ=l(1-cosθ)=l\frac{θ^2}{2}=\frac{(v_0τ)^2}{2l}$$
From this it follows that the angle θ' is given by:
$$θ'=\frac{(v_0τ)^2}{2ll'}$$
where l' is the horizontal distance between the lower pulley and mass A.
If we now sum the angles θ and θ', we obtain:
$$θ+θ'=\left(\frac{v_0τ}{l}\right)\left[1+\frac{v_0τ}{2l'}\right]$$
Note that, if the length l' is on the same order as l, the contribution of θ' to the sum of the two angles will be considerably smaller than the contribution of θ. If we substitute the equation ##v_0=\sqrt{gl}## into the the equation for θ+θ', we obtain:
$$θ+θ'=\sqrt{\frac{g}{l}}τ\left[1+\frac{\sqrt{gl}}{2l'}τ\right]≈\sqrt{\frac{g}{l}}τ$$
From this it follows that the contribution of the lower weight mg/2 to the radial component of tension on the upper rope is given by:
$$δT=\frac{mg}{2}\sqrt{\frac{g}{l}}τ$$
If the length l is 1 m, and the characteristic collision contact time is equal to ~0.001 sec, this equation predicts that δT≈0.0016 mg. This compares with the total tension of T=mg/18 = 0.055 mg calculated without accounting for the angulation of the ropes. With these values for the data, the contribution of the weight of the falling mass to the tension on mass B is on the order of a factor of about 35 lower than mg/18.
Chet