Slipping shoelace

A shoelace of length l = 60 cm l = 60 \, \text{cm} and mass m = 8 g m = 8 \, \text{g} lies on the edge of a table with an overhanging part of lenght x cm x\text{ cm} . At time t = 0 , t = 0, the initial overhang is x 0 = 4.7 cm x_0 = 4.7 \, \text{cm} and the shoelace is at rest ( ( initial velocity v 0 = 0 ) . v_0 = 0).

Now, the overhanging part of the lace is accelerated by gravity so that the lace gradually slips over the edge.

Find the time t = T t = T when the shoelace completely slips off the table and is in free fall ( i.e. x ( T ) = l ) . \big(\text{i.e. }x (T) = l\big).

We assume that the tabletop is perfectly smooth and that there is no friction. The shoelace has a homogeneous mass distribution and its diameter is negligible. The gravitational acceleration is g 9.81 m / s 2 g \approx 9.81 \, \text{m} / \text{s}^2 .

T 0.3 s T \approx 0.3 \,\text{s} T 0.8 s T \approx 0.8 \,\text{s} T 1.2 s T \approx 1.2 \,\text{s} T 2 s T \approx 2 \,\text{s}

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1 solution

We consider the potential energy U U of the lace. In doing so, we divide the shoelace into the sub-masses m m x m - m_x and m x = x l m m_x = \frac{x}{l} m , which respectively lie on the table top or overhang at the edge. While the mass m m x m - m_x is at the height h 0 h_0 (height of the table), the height of the mass m x m_x can be determined by the position of its center of gravity at h x = h 0 1 2 x h_x = h_0 - \frac{1}{2} x . The potential is thus U ( x ) = ( m m x ) g h 0 + m x g h x = m g [ l x l h 0 + x l ( h 0 x 2 ) ] = m g 2 l x 2 + const \begin{aligned} U(x) &= (m - m_x) g h_0 + m_x g h_x \\ &= m g \left[ \frac{l - x}{l} h_0 + \frac{x}{l} \left(h_0 - \frac{x}{2} \right) \right] \\ &= - \frac{m g}{2 l} x^2 + \text{const} \end{aligned} The force on the shoelace results m x ¨ = F = U ( x ) = m g l x m \ddot x = F = - U'(x) = \frac{m g}{l} x This differential equation can be solved with an expotential function x ( t ) = A e + λ t + B e λ t x ¨ ( t ) = λ 2 A e + λ t + λ 2 B e λ t = λ 2 x ( t ) \begin{aligned} x(t) &= A \cdot e^{+ \lambda t} + B \cdot e^{- \lambda t} \\ \Rightarrow \quad \ddot x(t) &= \lambda^2 A \cdot e^{+ \lambda t} + \lambda^2 B \cdot e^{- \lambda t} = \lambda^2 \cdot x(t) \end{aligned} with the exponent λ = g / l \lambda = \sqrt{g/l} and two coefficients A A and B B , that are fixed by the initial conditions: x ( t = 0 ) = A + B = ! x 0 x ˙ ( t = 0 ) = λ A λ B = ! 0 \begin{aligned} x(t = 0) &= A + B \stackrel{!}{=} x_0 \\ \dot x(t= 0) &= \lambda A - \lambda B \stackrel{!}{=} 0 \end{aligned} Therefore, A = B = 1 2 x 0 A = B = \frac{1}{2}x_0 and we get the result x ( t ) = x 0 2 [ e + λ t + e λ t ] = x 0 cosh ( λ t ) x(t) = \frac{x_0}{2} \left[e^{+ \lambda t} + e^{- \lambda t} \right] = x_0 \cosh(\lambda t) Finally, the equation x ( T ) = l x(T) = l can be solved by the time T T : T = l g arccosh ( l x 0 ) 0.8 s T = \sqrt{\frac{l}{g}} \cdot \text{arccosh}\left(\frac{l}{x_0}\right) \approx 0.8 \,\text{s}

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Ols Muka - 3 years, 2 months ago

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