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A particle X of massm and initial velocity u collide with another particle Y of mass `(3m)/(4)` which is at rest, The collision is head on and perfectly elastic. The ratio of de-Broglie wavelengths `lambda_(Y)` and `lambda_(X)` after the collision is

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To solve the problem step by step, we will analyze the elastic collision between the two particles and then calculate the de-Broglie wavelengths to find the desired ratio. ### Step 1: Understand the initial conditions - Particle X has mass \( m \) and initial velocity \( u \). - Particle Y has mass \( \frac{3m}{4} \) and is initially at rest (velocity = 0). ### Step 2: Apply conservation of momentum The total momentum before the collision must equal the total momentum after the collision. Initial momentum: \[ p_{\text{initial}} = m \cdot u + \frac{3m}{4} \cdot 0 = mu \] Let \( v_x \) be the final velocity of particle X and \( v_y \) be the final velocity of particle Y after the collision. The final momentum is: \[ p_{\text{final}} = m \cdot v_x + \frac{3m}{4} \cdot v_y \] Setting initial momentum equal to final momentum: \[ mu = mv_x + \frac{3m}{4}v_y \] Dividing through by \( m \): \[ u = v_x + \frac{3}{4}v_y \quad \text{(Equation 1)} \] ### Step 3: Apply conservation of kinetic energy In a perfectly elastic collision, the total kinetic energy before the collision equals the total kinetic energy after the collision. Initial kinetic energy: \[ KE_{\text{initial}} = \frac{1}{2} m u^2 + 0 = \frac{1}{2} m u^2 \] Final kinetic energy: \[ KE_{\text{final}} = \frac{1}{2} m v_x^2 + \frac{1}{2} \cdot \frac{3m}{4} v_y^2 \] Setting initial kinetic energy equal to final kinetic energy: \[ \frac{1}{2} m u^2 = \frac{1}{2} m v_x^2 + \frac{3m}{8} v_y^2 \] Dividing through by \( \frac{1}{2} m \): \[ u^2 = v_x^2 + \frac{3}{4} v_y^2 \quad \text{(Equation 2)} \] ### Step 4: Solve the equations simultaneously From Equation 1: \[ v_x = u - \frac{3}{4}v_y \] Substituting \( v_x \) into Equation 2: \[ u^2 = \left(u - \frac{3}{4}v_y\right)^2 + \frac{3}{4}v_y^2 \] Expanding the left side: \[ u^2 = u^2 - \frac{3}{2}uv_y + \frac{9}{16}v_y^2 + \frac{3}{4}v_y^2 \] Combining the terms: \[ u^2 = u^2 - \frac{3}{2}uv_y + \frac{9}{16}v_y^2 + \frac{12}{16}v_y^2 \] \[ u^2 = u^2 - \frac{3}{2}uv_y + \frac{21}{16}v_y^2 \] Cancelling \( u^2 \) from both sides: \[ 0 = -\frac{3}{2}uv_y + \frac{21}{16}v_y^2 \] Factoring out \( v_y \): \[ v_y \left(-\frac{3}{2}u + \frac{21}{16}v_y\right) = 0 \] Thus, either \( v_y = 0 \) (not possible since Y is moving after collision) or: \[ -\frac{3}{2}u + \frac{21}{16}v_y = 0 \] \[ v_y = \frac{3}{2}u \cdot \frac{16}{21} = \frac{24u}{21} = \frac{8u}{7} \] Substituting \( v_y \) back to find \( v_x \): \[ v_x = u - \frac{3}{4} \cdot \frac{8u}{7} = u - \frac{6u}{7} = \frac{1u}{7} = \frac{u}{7} \] ### Step 5: Calculate de-Broglie wavelengths The de-Broglie wavelength \( \lambda \) is given by: \[ \lambda = \frac{h}{mv} \] For particle Y: \[ \lambda_Y = \frac{h}{\frac{3m}{4} \cdot \frac{8u}{7}} = \frac{h \cdot 4 \cdot 7}{3m \cdot 8u} = \frac{28h}{24mu} = \frac{7h}{6mu} \] For particle X: \[ \lambda_X = \frac{h}{m \cdot \frac{u}{7}} = \frac{7h}{mu} \] ### Step 6: Find the ratio \( \frac{\lambda_Y}{\lambda_X} \) \[ \frac{\lambda_Y}{\lambda_X} = \frac{\frac{7h}{6mu}}{\frac{7h}{mu}} = \frac{1}{6} \] Thus, the ratio of the de-Broglie wavelengths \( \lambda_Y : \lambda_X \) is: \[ \boxed{1:6} \]
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