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Question: Three identical balls A,B and C each of mass m = 3kg are connected by strings AB and BC as shown in ...

Three identical balls A,B and C each of mass m = 3kg are connected by strings AB and BC as shown in the figure. The whole system is placed on a smooth horizontal surface.

Now the ball B is given an initial velocity v0=3v_0 = \sqrt{3} m/s, perpendicular to the string and along the horizontal surface. Find the tension (in newton) in the string just before the balls A and C collide.

Answer

2.5

Explanation

Solution

The initial configuration of the system is three balls A, B, and C of mass m=3m=3 kg, connected by strings AB and BC of length L=1L=1 m each, arranged in a line on a smooth horizontal surface. Ball B is given an initial velocity v0=3v_0 = \sqrt{3} m/s perpendicular to the string. Let the initial line of balls be the x-axis, with B at the origin (0,0), A at (-1,0), and C at (1,0). The initial velocity of B is along the y-axis, vB(0)=(0,v0)\vec{v}_B(0) = (0, v_0). The initial velocities of A and C are zero.

Due to symmetry, the motion will be symmetric with respect to the y-axis. Ball B will move along the y-axis, so its x-coordinate remains 0. Balls A and C will move symmetrically with respect to the y-axis, so their x-coordinates are opposite, and their y-coordinates are equal. Let the coordinates at time t be A(x,y)A(-x, y), B(0,yB)B(0, y_B), and C(x,y)C(x, y). The lengths of the strings are constant: AB2=(0(x))2+(yBy)2=x2+(yBy)2=L2=1|AB|^2 = (0 - (-x))^2 + (y_B - y)^2 = x^2 + (y_B - y)^2 = L^2 = 1 BC2=(x0)2+(yyB)2=x2+(yyB)2=L2=1|BC|^2 = (x - 0)^2 + (y - y_B)^2 = x^2 + (y - y_B)^2 = L^2 = 1

Balls A and C collide when their x-coordinates are equal, i.e., x=x-x = x, which implies x=0x=0.

Conservation of momentum in the y-direction: Initial y-momentum = mv0m v_0. At time t, y-momentum = mvAy+mvBy+mvCym v_{Ay} + m v_{By} + m v_{Cy}. Since yA=yC=yy_A = y_C = y, vAy=vCy=y˙v_{Ay} = v_{Cy} = \dot{y}. Let vBy=y˙Bv_{By} = \dot{y}_B. my˙+my˙B+my˙=mv0m \dot{y} + m \dot{y}_B + m \dot{y} = m v_0, so 2y˙+y˙B=v02 \dot{y} + \dot{y}_B = v_0.

Conservation of energy: Initial kinetic energy = 12mv02\frac{1}{2} m v_0^2. Initial potential energy = 0. At time t, kinetic energy = 12m(vAx2+vAy2)+12m(vBx2+vBy2)+12m(vCx2+vCy2)\frac{1}{2} m (v_{Ax}^2 + v_{Ay}^2) + \frac{1}{2} m (v_{Bx}^2 + v_{By}^2) + \frac{1}{2} m (v_{Cx}^2 + v_{Cy}^2). vAx=x˙v_{Ax} = -\dot{x}, vAy=y˙v_{Ay} = \dot{y}, vBx=0v_{Bx} = 0, vBy=y˙Bv_{By} = \dot{y}_B, vCx=x˙v_{Cx} = \dot{x}, vCy=y˙v_{Cy} = \dot{y}. 12m((x˙)2+y˙2)+12m(02+y˙B2)+12m(x˙2+y˙2)=12mv02\frac{1}{2} m ((-\dot{x})^2 + \dot{y}^2) + \frac{1}{2} m (0^2 + \dot{y}_B^2) + \frac{1}{2} m (\dot{x}^2 + \dot{y}^2) = \frac{1}{2} m v_0^2. mx˙2+my˙2+12my˙B2+12my˙2=12mv02m \dot{x}^2 + m \dot{y}^2 + \frac{1}{2} m \dot{y}_B^2 + \frac{1}{2} m \dot{y}^2 = \frac{1}{2} m v_0^2. 2x˙2+3y˙2+y˙B2=v022 \dot{x}^2 + 3 \dot{y}^2 + \dot{y}_B^2 = v_0^2.

From x2+(yBy)2=1x^2 + (y_B - y)^2 = 1, differentiating with respect to time: 2xx˙+2(yBy)(y˙By˙)=02x \dot{x} + 2(y_B - y)(\dot{y}_B - \dot{y}) = 0, so xx˙+(yBy)(y˙By˙)=0x \dot{x} + (y_B - y)(\dot{y}_B - \dot{y}) = 0.

Just before collision, x0x \to 0. The equation becomes (yBy)(y˙By˙)=0(y_B - y)(\dot{y}_B - \dot{y}) = 0. Since x2+(yBy)2=1x^2 + (y_B - y)^2 = 1, as x0x \to 0, (yBy)21(y_B - y)^2 \to 1, so yBy1|y_B - y| \to 1. Thus, yBy0y_B - y \neq 0. Therefore, we must have y˙By˙=0\dot{y}_B - \dot{y} = 0, which means y˙B=y˙\dot{y}_B = \dot{y}. So, just before collision, the y-velocities of A, B, and C are equal: vAy=vBy=vCy=y˙v_{Ay} = v_{By} = v_{Cy} = \dot{y}. From the conservation of y-momentum: 2y˙+y˙=v02 \dot{y} + \dot{y} = v_0, so 3y˙=v03 \dot{y} = v_0, y˙=v0/3\dot{y} = v_0/3. Just before collision, vAy=vBy=vCy=v0/3v_{Ay} = v_{By} = v_{Cy} = v_0/3.

From the energy conservation equation: 2x˙2+3y˙2+y˙B2=v022 \dot{x}^2 + 3 \dot{y}^2 + \dot{y}_B^2 = v_0^2. Substitute y˙=y˙B=v0/3\dot{y} = \dot{y}_B = v_0/3: 2x˙2+3(v0/3)2+(v0/3)2=v022 \dot{x}^2 + 3 (v_0/3)^2 + (v_0/3)^2 = v_0^2. 2x˙2+3(v02/9)+v02/9=v022 \dot{x}^2 + 3 (v_0^2/9) + v_0^2/9 = v_0^2. 2x˙2+v02/3+v02/9=v022 \dot{x}^2 + v_0^2/3 + v_0^2/9 = v_0^2. 2x˙2=v02v02/3v02/9=v02(11/31/9)=v02(9319)=v02(59)2 \dot{x}^2 = v_0^2 - v_0^2/3 - v_0^2/9 = v_0^2 (1 - 1/3 - 1/9) = v_0^2 (\frac{9 - 3 - 1}{9}) = v_0^2 (\frac{5}{9}). x˙2=5v0218\dot{x}^2 = \frac{5 v_0^2}{18}. Just before collision, A and C are moving towards the y-axis, so x˙=518v0\dot{x} = -\sqrt{\frac{5}{18}} v_0. vAx=x˙=518v0v_{Ax} = -\dot{x} = \sqrt{\frac{5}{18}} v_0 and vCx=x˙=518v0v_{Cx} = \dot{x} = -\sqrt{\frac{5}{18}} v_0.

At the moment just before collision, A and C are at (0,y)(0, y), and B is at (0,y±1)(0, y \pm 1). The strings are along the y-axis. The velocity of A is vA=(518v0,v0/3)\vec{v}_A = (\sqrt{\frac{5}{18}} v_0, v_0/3). The velocity of B is vB=(0,v0/3)\vec{v}_B = (0, v_0/3). The velocity of C is vC=(518v0,v0/3)\vec{v}_C = (-\sqrt{\frac{5}{18}} v_0, v_0/3).

Consider the motion of ball A relative to ball B. The relative velocity is vA/B=vAvB=(518v0,0)\vec{v}_{A/B} = \vec{v}_A - \vec{v}_B = (\sqrt{\frac{5}{18}} v_0, 0). Just before collision, A is at (0,y)(0, y) and B is at (0,y±1)(0, y \pm 1). The vector from B to A is (0,y)(0,y±1)=(0,1)(0, y) - (0, y \pm 1) = (0, \mp 1). The radial velocity of A with respect to B is the component of vA/B\vec{v}_{A/B} along the vector from B to A. If B is at (0,y+1)(0, y+1), the vector from B to A is (0,1)(0, -1). Radial velocity = vA/B(0,1)=(518v0,0)(0,1)=0\vec{v}_{A/B} \cdot (0, -1) = (\sqrt{\frac{5}{18}} v_0, 0) \cdot (0, -1) = 0. If B is at (0,y1)(0, y-1), the vector from B to A is (0,1)(0, 1). Radial velocity = vA/B(0,1)=(518v0,0)(0,1)=0\vec{v}_{A/B} \cdot (0, 1) = (\sqrt{\frac{5}{18}} v_0, 0) \cdot (0, 1) = 0. In both cases, the radial velocity is 0. This means the length of the string is not changing at this instant, which is consistent with the constraint.

Consider the motion of A relative to B. The string AB is of length L=1L=1. The motion of A relative to B is such that A is moving in a circle of radius 1 centered at B, or the distance between A and B is always 1. At the moment just before collision, A is at (0,y)(0,y) and B is at (0,y±1)(0,y \pm 1). The string AB is along the y-axis. The tension T in the string AB acts along the string. For ball A, the net force in the direction towards B (along the string) provides the centripetal acceleration. Let's assume B is at (0,yB)(0, y_B) and A is at (xA,yA)(x_A, y_A). The string AB is along the vector from B to A. The velocity of A relative to B is vA/B=vAvB\vec{v}_{A/B} = \vec{v}_A - \vec{v}_B. The component of vA/B\vec{v}_{A/B} perpendicular to the string is the tangential velocity. The component of vA/B\vec{v}_{A/B} along the string is the radial velocity. Just before collision, A is at (0,y)(0,y) and B is at (0,yB)(0, y_B). The vector from B to A is (0,yyB)(0, y-y_B). The length is yyB=1|y-y_B| = 1. Let's assume yB=y+1y_B = y+1. Then the vector from B to A is (0,1)(0, -1). The string is along the negative y-axis relative to B. vA=(518v0,v0/3)\vec{v}_A = (\sqrt{\frac{5}{18}} v_0, v_0/3), vB=(0,v0/3)\vec{v}_B = (0, v_0/3). vA/B=(518v0,0)\vec{v}_{A/B} = (\sqrt{\frac{5}{18}} v_0, 0). The radial velocity is vA/B(0,1)=0\vec{v}_{A/B} \cdot (0, -1) = 0. The tangential velocity magnitude is the magnitude of the component of vA/B\vec{v}_{A/B} perpendicular to the vector from B to A. The direction perpendicular to (0,1)(0, -1) is (±1,0)(\pm 1, 0). The tangential velocity is vA/B(vA/Br^)r^\vec{v}_{A/B} - (\vec{v}_{A/B} \cdot \hat{r}) \hat{r}, where r^\hat{r} is the unit vector from B to A, which is (0,1)(0, -1). Tangential velocity vector = (518v0,0)((518v0,0)(0,1))(0,1)=(518v0,0)0=(518v0,0)(\sqrt{\frac{5}{18}} v_0, 0) - ((\sqrt{\frac{5}{18}} v_0, 0) \cdot (0, -1)) (0, -1) = (\sqrt{\frac{5}{18}} v_0, 0) - 0 = (\sqrt{\frac{5}{18}} v_0, 0). The magnitude of the tangential velocity is vtan=(518v0)2+02=518v0v_{tan} = \sqrt{(\sqrt{\frac{5}{18}} v_0)^2 + 0^2} = \sqrt{\frac{5}{18}} v_0. The centripetal acceleration of A towards B is arad=vtan2L=(518v0)21=5v0218a_{rad} = \frac{v_{tan}^2}{L} = \frac{(\sqrt{\frac{5}{18}} v_0)^2}{1} = \frac{5 v_0^2}{18}. The net force on A along the string is the tension T. This force provides the centripetal acceleration. So, T=marad=m5v0218T = m a_{rad} = m \frac{5 v_0^2}{18}.

Given m=3m=3 kg and v0=3v_0 = \sqrt{3} m/s. T=3×5(3)218=3×5×318=3×1518=3×56=52=2.5T = 3 \times \frac{5 (\sqrt{3})^2}{18} = 3 \times \frac{5 \times 3}{18} = 3 \times \frac{15}{18} = 3 \times \frac{5}{6} = \frac{5}{2} = 2.5 N.

Let's verify this from the perspective of ball B. The forces on B are tension T from AB downwards and tension T from BC downwards. The net force on B is 2T2T downwards (assuming B is above A and C). The acceleration of B is aB=(0,y¨B)\vec{a}_B = (0, \ddot{y}_B). The equation of motion for B in the y-direction is 2T=my¨B-2T = m \ddot{y}_B.

Let's consider the equation of motion for A in the x-direction. The tension T has a component along the x-direction. Let θ\theta be the angle between AB and the y-axis. Then the x-component of tension is Tsinθ-T \sin \theta. Equation of motion for A in x-direction: Tsinθ=maAx=mx¨A=m(x¨)-T \sin \theta = m a_{Ax} = m \ddot{x}_A = m (-\ddot{x}). So Tsinθ=mx¨T \sin \theta = m \ddot{x}. Equation of motion for A in y-direction: Tcosθ=maAy=my¨A=my¨T \cos \theta = m a_{Ay} = m \ddot{y}_A = m \ddot{y}.

Just before collision, x0x \to 0, so sinθ0\sin \theta \to 0 and cosθ1\cos \theta \to 1. As x0x \to 0, Tsinθ=mx¨T \sin \theta = m \ddot{x}. If T is finite, then x¨0\ddot{x} \to 0. Tcosθ=my¨T \cos \theta = m \ddot{y}. As θ0\theta \to 0, T=my¨T = m \ddot{y}.

From x2+(yBy)2=1x^2 + (y_B - y)^2 = 1, differentiating twice: 2x˙2+2xx¨+2(y˙By˙)2+2(yBy)(y¨By¨)=02 \dot{x}^2 + 2x \ddot{x} + 2(\dot{y}_B - \dot{y})^2 + 2(y_B - y)(\ddot{y}_B - \ddot{y}) = 0. Just before collision, x=0x=0, y˙B=y˙\dot{y}_B = \dot{y}, yBy=1|y_B - y| = 1. 2x˙2+0+0+2(yBy)(y¨By¨)=02 \dot{x}^2 + 0 + 0 + 2(y_B - y)(\ddot{y}_B - \ddot{y}) = 0. 2x˙2+2(yBy)(y¨By¨)=02 \dot{x}^2 + 2(y_B - y)(\ddot{y}_B - \ddot{y}) = 0. x˙2+(yBy)(y¨By¨)=0\dot{x}^2 + (y_B - y)(\ddot{y}_B - \ddot{y}) = 0. We found x˙2=5v0218\dot{x}^2 = \frac{5 v_0^2}{18}. 5v0218+(yBy)(y¨By¨)=0\frac{5 v_0^2}{18} + (y_B - y)(\ddot{y}_B - \ddot{y}) = 0.

From 2y˙+y˙B=v02 \dot{y} + \dot{y}_B = v_0, differentiating: 2y¨+y¨B=02 \ddot{y} + \ddot{y}_B = 0. So y¨B=2y¨\ddot{y}_B = -2 \ddot{y}. Substitute into the equation above: 5v0218+(yBy)(2y¨y¨)=0\frac{5 v_0^2}{18} + (y_B - y)(-2 \ddot{y} - \ddot{y}) = 0. 5v0218+(yBy)(3y¨)=0\frac{5 v_0^2}{18} + (y_B - y)(-3 \ddot{y}) = 0. 5v02183(yBy)y¨=0\frac{5 v_0^2}{18} - 3 (y_B - y) \ddot{y} = 0.

If B is above A and C, yBy=1y_B - y = 1. Then 5v02183(1)y¨=0\frac{5 v_0^2}{18} - 3 (1) \ddot{y} = 0, so y¨=5v0254\ddot{y} = \frac{5 v_0^2}{54}. If B is below A and C, yBy=1y_B - y = -1. Then 5v02183(1)y¨=0\frac{5 v_0^2}{18} - 3 (-1) \ddot{y} = 0, so 5v0218+3y¨=0\frac{5 v_0^2}{18} + 3 \ddot{y} = 0, y¨=5v0254\ddot{y} = -\frac{5 v_0^2}{54}.

From the equation of motion for A in y-direction, just before collision, T=my¨T = m \ddot{y}. If y¨=5v0254\ddot{y} = \frac{5 v_0^2}{54}, then T=m5v0254T = m \frac{5 v_0^2}{54}. If y¨=5v0254\ddot{y} = -\frac{5 v_0^2}{54}, then T=m5v0254T = -m \frac{5 v_0^2}{54}. Tension must be positive, so this case is not possible unless the string is slack.

Let's reconsider the geometry. When B is given initial velocity upwards, it moves upwards, and A and C move upwards and inwards. When A and C collide at the y-axis, they are at the same y-coordinate. B is at a different y-coordinate. Since the strings have length 1, B must be 1 unit away from A and C along the y-axis. Since B started at the origin and moved upwards, its y-coordinate is greater than the initial y-coordinate of A and C (which is 0). As A and C move upwards, their y-coordinate increases. Consider the initial setup where A, B, C are on the x-axis. B is at (0,0), A at (-1,0), C at (1,0). B is given velocity (0,v0)(0, v_0). So B moves to (0,yB)(0, y_B) with yB>0y_B > 0. A moves to (x,y)(-x, y) and C moves to (x,y)(x, y), with xx decreasing and yy increasing. When A and C collide, x=0x=0. So A and C are at (0,y)(0, y). Since the string length is 1, the distance between B and A (or B and C) is 1. So (00)2+(yBy)2=1\sqrt{(0-0)^2 + (y_B - y)^2} = 1, yBy=1|y_B - y| = 1. Since B moved upwards and A and C also moved upwards, and B started between A and C in the initial line, it is likely that B is above A and C when they collide. So yB>yy_B > y. Thus yBy=1y_B - y = 1.

So, y¨=5v0254\ddot{y} = \frac{5 v_0^2}{54}. Then T=my¨=m5v0254=3×5(3)254=3×5×354=3×1554=3×518=56T = m \ddot{y} = m \frac{5 v_0^2}{54} = 3 \times \frac{5 (\sqrt{3})^2}{54} = 3 \times \frac{5 \times 3}{54} = 3 \times \frac{15}{54} = 3 \times \frac{5}{18} = \frac{5}{6} N.

Let's check the centripetal acceleration approach again. The relative velocity of A with respect to B is vA/B=vAvB\vec{v}_{A/B} = \vec{v}_A - \vec{v}_B. The radial direction is along the line AB. The tension provides the force in this direction. The component of vA/B\vec{v}_{A/B} along AB is the radial velocity. The component perpendicular to AB is the tangential velocity. The centripetal acceleration of A towards B is vtan2L\frac{v_{tan}^2}{L}. The force in the radial direction is T. So T=mvtan2LT = m \frac{v_{tan}^2}{L}. Just before collision, A is at (0,y)(0,y), B is at (0,yB)(0,y_B), with yBy=1|y_B - y| = 1. Let's assume yB>yy_B > y, so B is above A. The vector from B to A is (0,yyB)=(0,1)(0, y-y_B) = (0, -1). The unit vector from B to A is r^=(0,1)\hat{r} = (0, -1). vA=(518v0,v0/3)\vec{v}_A = (\sqrt{\frac{5}{18}} v_0, v_0/3), vB=(0,v0/3)\vec{v}_B = (0, v_0/3). vA/B=(518v0,0)\vec{v}_{A/B} = (\sqrt{\frac{5}{18}} v_0, 0). Radial velocity vrad=vA/Br^=(518v0,0)(0,1)=0v_{rad} = \vec{v}_{A/B} \cdot \hat{r} = (\sqrt{\frac{5}{18}} v_0, 0) \cdot (0, -1) = 0. Tangential velocity vector vtan=vA/Bvradr^=(518v0,0)0=(518v0,0)\vec{v}_{tan} = \vec{v}_{A/B} - v_{rad} \hat{r} = (\sqrt{\frac{5}{18}} v_0, 0) - 0 = (\sqrt{\frac{5}{18}} v_0, 0). Magnitude of tangential velocity vtan=518v0v_{tan} = \sqrt{\frac{5}{18}} v_0. Centripetal acceleration arad=vtan2L=(518v0)21=5v0218a_{rad} = \frac{v_{tan}^2}{L} = \frac{(\sqrt{\frac{5}{18}} v_0)^2}{1} = \frac{5 v_0^2}{18}. Tension T=marad=m5v0218=3×5(3)218=3×5×318=3×1518=3×56=52=2.5T = m a_{rad} = m \frac{5 v_0^2}{18} = 3 \times \frac{5 (\sqrt{3})^2}{18} = 3 \times \frac{5 \times 3}{18} = 3 \times \frac{15}{18} = 3 \times \frac{5}{6} = \frac{5}{2} = 2.5 N.

Let's check the case where B is below A and C, yB<yy_B < y, so yBy=1y_B - y = -1. The vector from B to A is (0,1)(0, 1). The unit vector is r^=(0,1)\hat{r} = (0, 1). Radial velocity vrad=vA/Br^=(518v0,0)(0,1)=0v_{rad} = \vec{v}_{A/B} \cdot \hat{r} = (\sqrt{\frac{5}{18}} v_0, 0) \cdot (0, 1) = 0. Tangential velocity magnitude is the same, vtan=518v0v_{tan} = \sqrt{\frac{5}{18}} v_0. Centripetal acceleration is the same, arad=5v0218a_{rad} = \frac{5 v_0^2}{18}. Tension T=marad=2.5T = m a_{rad} = 2.5 N.

The direction of centripetal acceleration of A relative to B is towards B. If B is above A, the direction is upwards. If B is below A, the direction is downwards. Tension acts from A towards B. If B is above A, tension on A is upwards. If B is below A, tension on A is downwards. The force equation for A in the direction from A to B is T. The acceleration of A relative to B in this direction is the radial acceleration. Acceleration of A is aA=(x¨A,y¨A)=(x¨,y¨)\vec{a}_A = (\ddot{x}_A, \ddot{y}_A) = (-\ddot{x}, \ddot{y}). Acceleration of B is aB=(0,y¨B)\vec{a}_B = (0, \ddot{y}_B). Relative acceleration aA/B=aAaB=(x¨,y¨y¨B)\vec{a}_{A/B} = \vec{a}_A - \vec{a}_B = (-\ddot{x}, \ddot{y} - \ddot{y}_B). The radial acceleration is the component of aA/B\vec{a}_{A/B} along the vector from B to A. If B is above A, vector from B to A is (0,1)(0, -1). Radial acceleration = aA/B(0,1)=(x¨,y¨y¨B)(0,1)=(y¨y¨B)=y¨By¨\vec{a}_{A/B} \cdot (0, -1) = (-\ddot{x}, \ddot{y} - \ddot{y}_B) \cdot (0, -1) = -(\ddot{y} - \ddot{y}_B) = \ddot{y}_B - \ddot{y}. This radial acceleration is equal to vtan2L-\frac{v_{tan}^2}{L} because it is towards the center B. So, y¨By¨=vtan2L=5v0218\ddot{y}_B - \ddot{y} = -\frac{v_{tan}^2}{L} = -\frac{5 v_0^2}{18}. From 2y¨+y¨B=02 \ddot{y} + \ddot{y}_B = 0, y¨B=2y¨\ddot{y}_B = -2 \ddot{y}. 2y¨y¨=5v0218-2 \ddot{y} - \ddot{y} = -\frac{5 v_0^2}{18}, so 3y¨=5v0218-3 \ddot{y} = -\frac{5 v_0^2}{18}, y¨=5v0254\ddot{y} = \frac{5 v_0^2}{54}. y¨B=2y¨=10v0254=5v0227\ddot{y}_B = -2 \ddot{y} = -\frac{10 v_0^2}{54} = -\frac{5 v_0^2}{27}. The net force on A in the y-direction is the tension T (since the string is vertical). So T=maAy=my¨=3×5v0254=3×5×354=56T = m a_{Ay} = m \ddot{y} = 3 \times \frac{5 v_0^2}{54} = 3 \times \frac{5 \times 3}{54} = \frac{5}{6} N. This is not matching the centripetal force calculation.

Let's check the direction of tension. Tension on A is towards B. If B is above A, tension is upwards. If B is below A, tension is downwards. The centripetal acceleration of A relative to B is towards B. The force on A along the string is T. This force causes the radial acceleration. So, T=marad=mvtan2LT = m a_{rad} = m \frac{v_{tan}^2}{L}. This is correct. The issue might be in the application of the equation of motion T=my¨T = m \ddot{y}. This is only valid if the tension is the only force in the y-direction and the string is vertical.

Let's recheck the relative acceleration approach. The radial acceleration of A relative to B is aA/Br^\vec{a}_{A/B} \cdot \hat{r}. This is the acceleration along the line AB. The force on A along AB is T. So, T=m(aA/Br^)T = m (\vec{a}_{A/B} \cdot \hat{r}). Let's assume B is above A, so r^=(0,1)\hat{r} = (0, -1). T=m((x¨,y¨y¨B)(0,1))=m((y¨y¨B))=m(y¨By¨)T = m ((-\ddot{x}, \ddot{y} - \ddot{y}_B) \cdot (0, -1)) = m (-(\ddot{y} - \ddot{y}_B)) = m (\ddot{y}_B - \ddot{y}). We have y¨By¨=vtan2L=5v0218\ddot{y}_B - \ddot{y} = -\frac{v_{tan}^2}{L} = -\frac{5 v_0^2}{18}. So, T=m(5v0218)=m5v0218T = m (-\frac{5 v_0^2}{18}) = -m \frac{5 v_0^2}{18}. Tension cannot be negative.

Let's check the direction of radial acceleration. The radial acceleration of A relative to B is towards B. So, the component of aA/B\vec{a}_{A/B} along the vector from A to B should be equal to vtan2L\frac{v_{tan}^2}{L}. The vector from A to B is (0,yBy)(0, y_B - y). If yB>yy_B > y, this is (0,1)(0, 1). The unit vector is (0,1)(0, 1). Radial acceleration = aA/B(0,1)=(x¨,y¨y¨B)(0,1)=y¨y¨B\vec{a}_{A/B} \cdot (0, 1) = (-\ddot{x}, \ddot{y} - \ddot{y}_B) \cdot (0, 1) = \ddot{y} - \ddot{y}_B. So, y¨y¨B=vtan2L=5v0218\ddot{y} - \ddot{y}_B = \frac{v_{tan}^2}{L} = \frac{5 v_0^2}{18}. From 2y¨+y¨B=02 \ddot{y} + \ddot{y}_B = 0, y¨B=2y¨\ddot{y}_B = -2 \ddot{y}. y¨(2y¨)=5v0218\ddot{y} - (-2 \ddot{y}) = \frac{5 v_0^2}{18}, so 3y¨=5v02183 \ddot{y} = \frac{5 v_0^2}{18}, y¨=5v0254\ddot{y} = \frac{5 v_0^2}{54}. y¨B=2y¨=10v0254=5v0227\ddot{y}_B = -2 \ddot{y} = -\frac{10 v_0^2}{54} = -\frac{5 v_0^2}{27}. The force on A in the direction from A to B is T. So T=m(y¨y¨B)=m5v0218=3×5×318=2.5T = m (\ddot{y} - \ddot{y}_B) = m \frac{5 v_0^2}{18} = 3 \times \frac{5 \times 3}{18} = 2.5 N. This matches the centripetal force calculation. So, the tension is 2.5 N.