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Question

Question: Figure shows the variation of frequency of a characteristic X-ray and atomic number....

Figure shows the variation of frequency of a characteristic X-ray and atomic number.

A

The characteristic X-ray is KαK_{\alpha}

B

The characteristic X-ray is KβK_{\beta}

C

The energy of photon emitted when this X-ray is emitted by a metal having z = 101 is 204 keV

D

The energy of photon emitted when this X-ray is emitted by a metal having z = 101 is 102 keV

Answer

The characteristic X-ray is KαK_{\alpha}, The energy of photon emitted when this X-ray is emitted by a metal having z = 101 is 102 keV

Explanation

Solution

The graph shows the variation of frequency ν\nu of a characteristic X-ray with atomic number ZZ. According to Moseley's law, for a characteristic X-ray of a given series, the frequency is related to the atomic number by ν=a(Zb)\sqrt{\nu} = a(Z-b), where aa and bb are constants. Thus, ν=a2(Zb)2\nu = a^2 (Z-b)^2. For K-series X-rays, the screening constant bb is approximately 1. The graph shows that ν0\nu \approx 0 when Z=1Z=1, which is consistent with b=1b=1. So we can write ν=A(Z1)2\nu = A(Z-1)^2 for some constant AA.

The energy of the emitted photon is E=hν=hA(Z1)2E = h\nu = hA(Z-1)^2. Let E0=hAE_0 = hA. Then E=E0(Z1)2E = E_0 (Z-1)^2. The constant E0E_0 depends on the specific transition. For the K-series, the transitions are to the K shell (n1=1n_1=1).

For the KαK_{\alpha} line, the transition is from the L shell (n2=2n_2=2) to the K shell (n1=1n_1=1). The energy is given by EKα=Ry(Z1)2(112122)=Ry(Z1)234E_{K_{\alpha}} = R_y (Z-1)^2 (\frac{1}{1^2} - \frac{1}{2^2}) = R_y (Z-1)^2 \frac{3}{4}. So, E0=Ry34E_0 = R_y \frac{3}{4}, where RyR_y is the Rydberg constant for energy, approximately 13.6 eV. E013.6×34=10.2E_0 \approx 13.6 \times \frac{3}{4} = 10.2 eV. Thus, EKα10.2(Z1)2E_{K_{\alpha}} \approx 10.2 (Z-1)^2 eV.

For the KβK_{\beta} line, the transition is from the M shell (n2=3n_2=3) to the K shell (n1=1n_1=1). The energy is given by EKβ=Ry(Z1)2(112132)=Ry(Z1)289E_{K_{\beta}} = R_y (Z-1)^2 (\frac{1}{1^2} - \frac{1}{3^2}) = R_y (Z-1)^2 \frac{8}{9}. So, E0=Ry89E_0 = R_y \frac{8}{9}. E013.6×8912.09E_0 \approx 13.6 \times \frac{8}{9} \approx 12.09 eV. Thus, EKβ12.09(Z1)2E_{K_{\beta}} \approx 12.09 (Z-1)^2 eV.

Now let's evaluate the energy for Z=101Z=101. If the characteristic X-ray is KαK_{\alpha}, EKα(Z=101)10.2(1011)2=10.2×1002=10.2×10000=102000E_{K_{\alpha}}(Z=101) \approx 10.2 (101-1)^2 = 10.2 \times 100^2 = 10.2 \times 10000 = 102000 eV = 102 keV. If the characteristic X-ray is KβK_{\beta}, EKβ(Z=101)12.09(1011)2=12.09×10000=120900E_{K_{\beta}}(Z=101) \approx 12.09 (101-1)^2 = 12.09 \times 10000 = 120900 eV = 120.9 keV.

The calculated energy for KαK_{\alpha} at Z=101 is 102 keV, which matches the fourth option. This suggests that the characteristic X-ray is KαK_{\alpha}.