The Fermi-Dirac distribution is given by:
\[ f(E) = \frac{1}{1 + \exp\left(\frac{E - E_F}{k_B T}\right)} \]
We are given \( f(E) = 0.2 \), so we need to solve for \( E \).
Taking the reciprocal of both sides:
\[ \frac{1}{f(E)} = 1 + \exp\left(\frac{E - E_F}{k_B T}\right) \]
Subtracting 1 from both sides:
\[ \frac{1}{f(E)} - 1 = \exp\left(\frac{E - E_F}{k_B T}\right) \]
Taking the natural logarithm on both sides:
\[ \ln \left(\frac{1}{f(E)} - 1\right) = \frac{E - E_F}{k_B T} \]
Solving for \( E \):
\[ E = E_F + k_B T \ln \left(\frac{1}{f(E)} - 1\right) \]
Substituting \( f(E) = 0.2 \), \( E_F = 5.5 \) eV, \( k_B = 8.62 \times 10^{-5} \) eV/K, and \( T = 500K \):
\[ E = 5.5 + (8.62 \times 10^{-5} \times 500) \ln \left(\frac{1}{0.2} - 1\right) \]
\[ E = 5.5 + (8.62 \times 10^{-5} \times 500) \ln(4) \]
\[ E = 5.5 + (0.0431) \times 1.386 \]
\[ E = 5.5 + 0.0598 \]
\[ E \approx 5.56 \text{ eV} \]
The energy of the level is approximately 5.56 eV.
The motion of a particle in the XY plane is given by \( x(t) = 25 + 6t^2 \, \text{m} \); \( y(t) = -50 - 20t + 8t^2 \, \text{m} \). The magnitude of the initial velocity of the particle, \( v_0 \), is given by:
At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/mΒ³, which is dimensionally incorrect for a spectral density. The correct unit J/(mΒ³Β·Hz) or JΒ·s/mΒ³ is used here for the solution.)