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 \( 1 : 3 \).
Consider a rope fixed at both ends under tension so that it is horizontal (i.e. assume the rope is along x-axis, with gravity acting along z-axis). Now the right end is continually oscillated at high frequency n (say n=100 Hz) horizontally and in a direction along the rope; amplitude of oscillation is negligible. The oscillation travells along the rope and is reflected at the left end.
Let the total length of rope be l, total mass be m and the acceleration due to gravity be g.
After initial phase (say a mintue or so), the rope has __(BLANK-1)__ wave, which is __(BLANK-2)__ in nature. It results from superposition of left travelling and right travelling __(BLANK-3)__ waves. This resulting wave has a frequency __ (BLANK-4)_ that of oscillation frequency nu. Simple dimensional analysis indicates that the frequency of can be of the form: ___(BLANK-5)__ .
In the given cycle ABCDA, the heat required for an ideal monoatomic gas will be:
Evaluate the following limit: $ \lim_{n \to \infty} \prod_{r=3}^n \frac{r^3 - 8}{r^3 + 8} $.