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Uranium- 238 decays to thorium-234 with ...

Uranium- `238` decays to thorium-`234` with half-life `5xx10^(9) yr`. The resulting nucleus is in the excited state and hence further emits `gamma`-rays to come to the ground state. It emits `20 gamma`-rays per second. The emission rate will drop to `5 gamma`-rays per second in

A

(a)`.25xx10^(9)yr`

B

(b)`10^(10)yr`

C

(c)`10^(-8)yr`

D

(d)`1.25xx10^(-9)s`

Text Solution

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To solve the problem, we need to determine the time it takes for the emission rate of gamma rays from the excited state of Thorium-234 to drop from 20 gamma rays per second to 5 gamma rays per second. ### Step-by-step Solution: 1. **Understanding the decay process**: - Uranium-238 decays to Thorium-234, which is in an excited state and emits gamma rays to reach its ground state. - The initial emission rate of gamma rays is 20 gamma rays per second. 2. **Establishing the relationship**: - The emission rate of gamma rays is proportional to the number of excited nuclei present. - We denote the initial emission rate as \( N_0 = 20 \) gamma rays/second and the final emission rate as \( N = 5 \) gamma rays/second. 3. **Using the decay formula**: - The decay of the excited nuclei can be expressed as: \[ \frac{N}{N_0} = \frac{5}{20} = \frac{1}{4} \] - This means that after some time \( t \), the number of excited nuclei has decreased to one-fourth of its initial value. 4. **Applying the natural logarithm**: - We can use the relationship of decay: \[ \ln\left(\frac{N}{N_0}\right) = -\lambda t \] - Substituting the values we found: \[ \ln\left(\frac{1}{4}\right) = -\lambda t \] 5. **Finding the decay constant \( \lambda \)**: - The half-life \( T_{1/2} \) of Uranium-238 is given as \( 5 \times 10^9 \) years. - The decay constant \( \lambda \) is related to the half-life by: \[ \lambda = \frac{\ln(2)}{T_{1/2}} \] - Substituting the half-life: \[ \lambda = \frac{\ln(2)}{5 \times 10^9} \] 6. **Substituting \( \lambda \) into the decay equation**: - Now we can substitute \( \lambda \) back into the equation: \[ \ln\left(\frac{1}{4}\right) = -\left(\frac{\ln(2)}{5 \times 10^9}\right)t \] - Since \( \ln\left(\frac{1}{4}\right) = -2 \ln(2) \): \[ -2 \ln(2) = -\left(\frac{\ln(2)}{5 \times 10^9}\right)t \] 7. **Solving for \( t \)**: - Canceling \( \ln(2) \) from both sides: \[ 2 = \frac{t}{5 \times 10^9} \] - Rearranging gives: \[ t = 2 \times 5 \times 10^9 = 10 \times 10^9 = 10^{10} \text{ years} \] ### Final Answer: The emission rate will drop to 5 gamma rays per second in \( 10^{10} \) years.
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