Step 1: The de-Broglie wavelength of a particle is given by: \[ \lambda = \frac{h}{mv} \] where \( h \) is Planck's constant and \( m \) is the mass of the particle, and \( v \) is its velocity. For the electron, we have: \[ \lambda_{{electron}} = \frac{h}{m_{{e}} \cdot \frac{c}{3}} \] where \( m_{{e}} \) is the mass of the electron.
Step 2: For the photon, the wavelength is related to its energy by: \[ E_{{photon}} = \frac{hc}{\lambda_{{photon}}} \] Since the wavelengths of the electron and the photon are equal, we can equate their expressions: \[ \frac{h}{m_{{e}} \cdot \frac{c}{3}} = \frac{hc}{E_{{photon}}} \] This leads to the energy of the photon: \[ E_{{photon}} = \frac{3m_{{e}} c^2}{2} \]
Step 3: The kinetic energy of the electron is given by: \[ E_{{electron}} = \frac{1}{2} m_{{e}} v^2 = \frac{1}{2} m_{{e}} \left( \frac{c}{3} \right)^2 = \frac{1}{2} m_{{e}} \cdot \frac{c^2}{9} \]
Step 4: The ratio of the kinetic energies of the electron and the photon is: \[ {Ratio} = \frac{E_{{electron}}}{E_{{photon}}} = \frac{\frac{1}{2} m_{{e}} \cdot \frac{c^2}{9}}{\frac{3m_{{e}} c^2}{2}} = \frac{1}{3} \]
Step 5: Hence, the ratio of the kinetic energies is \( 1 : 3 \).
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: