0.993
0.990
We can use the relativistic energy-momentum relation to find the speed of the electron. The total energy \( E \) of a particle is given by:
\[ E = \gamma m c^2 \]
where \( \gamma = \frac{1}{\sqrt{1 - v^2/c^2}} \) is the Lorentz factor, \( m \) is the rest mass, and \( v \) is the speed of the particle.
The total energy is the sum of the rest mass energy and the kinetic energy:
\[ E = m c^2 + \text{K.E.} \]
Substitute the given values:
Thus, the total energy is:
\[ E = 0.511 + 5.11 = 5.621 \, \text{MeV} \]
Using the formula \( E = \gamma m c^2 \), solve for \( \gamma \):
\[ \gamma = \frac{E}{m c^2} = \frac{5.621}{0.511} \approx 11 \]
From the Lorentz factor \( \gamma = \frac{1}{\sqrt{1 - v^2/c^2}} \), rearrange to find \( v \):
\[ v = c \sqrt{1 - \frac{1}{\gamma^2}} \]
Substitute \( \gamma = 11 \):
\[ v = c \sqrt{1 - \frac{1}{11^2}} = c \sqrt{1 - 0.00826} \approx c \sqrt{0.99174} \]
\[ v \approx 0.996c \]
Thus, the speed of the electron is closest to \( 0.996c \).
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/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)