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Nucleus A decays to B with decay constan...

Nucleus `A` decays to `B` with decay constant `lambda_(1)` and `B` decays to `C` with decay constant `lambda_(2)`. Initially at `t=0` number of nuclei of `A` and `B` are `2N_(0)` and `N_(0)` respectively. At `t=t_(o)`, no. of nuclei of `B` is `(3N_(0))/(2)` and nuclei of `B` stop changing. Find `t_(0)`?

A

the value of `t_(0)"is"(1)/(lambda_(1))ln.(4)/(3)(lambda_(1))/(lambda_(2))`

B

the value of `t_(0)"is"(1)/(lambda_(2))ln.(4)/(3)(lambda_(1))/(lambda_(2))`

C

the value of `N_(A)` at `t_(0)"is""(3N_(0))/(2)(lambda_(2))/(lambda_(1))`

D

the value of `N_(A)` at `t_(0)"is""(2N_(0))/(3)(lambda_(2))/(lambda_(1))`

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To solve the problem step by step, we will analyze the decay of nuclei A to B and B to C using the given information. ### Step 1: Understand the decay process Nucleus A decays to nucleus B with decay constant \( \lambda_1 \), and nucleus B decays to nucleus C with decay constant \( \lambda_2 \). Initially, at \( t = 0 \): - Number of nuclei of A, \( N_A(0) = 2N_0 \) - Number of nuclei of B, \( N_B(0) = N_0 \) ### Step 2: Write the differential equation for B The change in the number of nuclei of B over time can be expressed as: \[ \frac{dN_B}{dt} = \lambda_1 N_A - \lambda_2 N_B \] Substituting \( N_A \) in terms of time: \[ N_A(t) = N_A(0) e^{-\lambda_1 t} = 2N_0 e^{-\lambda_1 t} \] So the equation becomes: \[ \frac{dN_B}{dt} = \lambda_1 (2N_0 e^{-\lambda_1 t}) - \lambda_2 N_B \] ### Step 3: Evaluate at \( t = t_0 \) At time \( t = t_0 \), it is given that the number of nuclei of B is \( N_B(t_0) = \frac{3N_0}{2} \). At this point, the rate of change of \( N_B \) becomes zero: \[ \frac{dN_B}{dt} \bigg|_{t=t_0} = 0 \] So we set up the equation: \[ 0 = \lambda_1 (2N_0 e^{-\lambda_1 t_0}) - \lambda_2 \left(\frac{3N_0}{2}\right) \] ### Step 4: Rearranging the equation Rearranging the above equation gives: \[ \lambda_1 (2N_0 e^{-\lambda_1 t_0}) = \frac{3}{2} \lambda_2 N_0 \] Dividing both sides by \( N_0 \) (assuming \( N_0 \neq 0 \)): \[ 2 \lambda_1 e^{-\lambda_1 t_0} = \frac{3}{2} \lambda_2 \] ### Step 5: Solve for \( e^{-\lambda_1 t_0} \) Rearranging gives: \[ e^{-\lambda_1 t_0} = \frac{3 \lambda_2}{4 \lambda_1} \] ### Step 6: Taking the natural logarithm Taking the natural logarithm of both sides: \[ -\lambda_1 t_0 = \ln\left(\frac{3 \lambda_2}{4 \lambda_1}\right) \] Thus, \[ t_0 = -\frac{1}{\lambda_1} \ln\left(\frac{3 \lambda_2}{4 \lambda_1}\right) \] ### Final Result The time \( t_0 \) when the number of nuclei of B becomes \( \frac{3N_0}{2} \) and stops changing is given by: \[ t_0 = \frac{1}{\lambda_1} \ln\left(\frac{4 \lambda_1}{3 \lambda_2}\right) \]
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