
| To determine the longitudinal strain in the wire, we first calculate the tension caused by the two connected masses, \(m_1=2\,\text{kg}\) and \(m_2=4\,\text{kg}\), assuming an acceleration \(a\). The forces acting on each mass are described by: |
| \[ T - m_1g = m_1a \] |
| \[ m_2g - T = m_2a \] |
| Summing these equations cancels out \(T\): |
| \[ m_2g - m_1g = (m_1 + m_2)a \] |
| The acceleration is found to be: |
| \[ a = \frac{(m_2 - m_1)g}{m_1 + m_2} = \frac{(4 - 2) \times 10}{6} = \frac{20}{6} = \frac{10}{3} \, \text{m/s}^2 \] |
| Substituting \(a\) back into \(T = m_1(g + a)\) yields the tension: |
| \[ T = 2 \times \left(10 + \frac{10}{3}\right) = 2 \times \frac{40}{3} = \frac{80}{3} \text{N} \] |
| The longitudinal strain \(\epsilon\) is defined as: |
| \[ \epsilon = \frac{\text{Stress}}{\text{Young's Modulus}} = \frac{T}{A \cdot Y} \] |
| The wire's cross-sectional area \(A\) is calculated as: |
| \[ A = \pi r^2 = \pi \times (4.0 \times 10^{-5})^2 = 16\pi \times 10^{-10} \, \text{m}^2 \] |
| Consequently, the strain is: |
| \[ \epsilon = \frac{\frac{80}{3}}{16\pi \times 10^{-10} \times 2 \times 10^{11}} \] |
| \[ = \frac{80}{3 \times 32\pi } \times 10^{-11} \times 5 \] |
| \[ = \frac{1}{12\pi} \] |
| The calculated strain is \(\frac{1}{12\pi}\). This implies \(\alpha = 12\), which falls within the expected range of [12,12]. Therefore, \(\alpha = 12\). |

The Young's modulus of a steel wire of length \(6 m\) and cross-sectional area \(3 \,mm ^2\), is \(2 \times 10^{11}\) \(N / m ^2\). The wire is suspended from its support on a given planet A block of mass \(4 kg\) is attached to the free end of the wire. The acceleration due to gravity on the planet is \(\frac{1}{4}\) of its value on the earth The elongation of wire is (Take \(g\) on the earth \(=10\, m / s ^2\)) :