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Concepts Of Physics MCQ Edition [Volume 2]
Exam
Concepts Of Physics MCQ Edition [Volume 2]
Subject
Physics
Chapter
The Nucleus

Concepts Of Physics MCQ Edition [Volume 2] · Physics · The Nucleus

A point source emitting alpha particles is situated at a distance...

A point source emitting alpha particles is situated at a distance of 1 m1 \text{ m} from a counter that registers any alpha particle striking its 1 cm21 \text{ cm}^2 window. Given that the source has 6.0×10166.0 \times 10^{16} active nuclei and the counter registers a rate of 50000 counts/second50000 \text{ counts/second}, determine the decay constant. Assume the source radiates alpha particles uniformly in all directions and that the alpha particles strike the window nearly normally.

Options

  1. A8.33×10−9 s−18.33 \times 10^{-9} \text{ s}^{-1}
  2. B4.19×10−7 s−14.19 \times 10^{-7} \text{ s}^{-1}
  3. C1.05×10−7 s−11.05 \times 10^{-7} \text{ s}^{-1}
  4. D2.09×10−7 s−12.09 \times 10^{-7} \text{ s}^{-1}

Correct answer

C. 1.05×10−7 s−11.05 \times 10^{-7} \text{ s}^{-1}

Step-by-step solution

The total activity of the source is given by A0=λNA_0 = \lambda N, where λ\lambda is the decay constant and NN is the number of active nuclei.

Since the alpha particles are emitted uniformly in all directions, the fraction of particles hitting the window is the ratio of the area of the window to the total surface area of a sphere of radius rr.

Fraction of particles registered =A4πr2= \dfrac{A}{4\pi r^2}

The count rate CC is the number of alpha particles striking the window per second:

C=A0×A4πr2=λNA4πr2C = A_0 \times \dfrac{A}{4\pi r^2} = \lambda N \dfrac{A}{4\pi r^2}

Rearranging for the decay constant λ\lambda:

λ=C×4πr2N×A\lambda = \dfrac{C \times 4\pi r^2}{N \times A}

Substituting the given values C=50000 s−1C = 50000 \text{ s}^{-1}, r=1 m=100 cmr = 1 \text{ m} = 100 \text{ cm}, A=1 cm2A = 1 \text{ cm}^2, and N=6.0×1016N = 6.0 \times 10^{16}:

λ=50000×4π×(100)26.0×1016×1\lambda = \dfrac{50000 \times 4\pi \times (100)^2}{6.0 \times 10^{16} \times 1}

λ=5×104×4π×1046.0×1016\lambda = \dfrac{5 \times 10^4 \times 4\pi \times 10^4}{6.0 \times 10^{16}}

λ=20π×1086.0×1016\lambda = \dfrac{20\pi \times 10^8}{6.0 \times 10^{16}}

λ=10π3×10−8 s−1\lambda = \dfrac{10\pi}{3} \times 10^{-8} \text{ s}^{-1}

λ≈10.47×10−8 s−1=1.047×10−7 s−1\lambda \approx 10.47 \times 10^{-8} \text{ s}^{-1} = 1.047 \times 10^{-7} \text{ s}^{-1}

Rounding to three significant figures, we get 1.05×10−7 s−11.05 \times 10^{-7} \text{ s}^{-1}.
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