Q1. Attempt all questions. Symbols have their usual meanings. The marks for each question are indicated against it.
- a)) A muon decays spontaneously into an electron and two neutrinos. If the number of muons at t = 0 is No and the number at time t is N where N is given by the expression N = Noe¯t/t . The mean lifetime of the muon is t = 2.20µs. If the muons are travelling with a speed of 0.95c, calculate the observed lifetime of the muons and the number of muons which remain after travelling a distance of 3.0 km. (200 words)
- b)) Two rockets of rest length Lo are approaching the earth from opposite directions with velocities of ±c/3. How long would one of them appear to the other? (200 words)
- c)) How fast and in what direction must a galaxy S be moving, if an absorbtion line observed at a wavelength of 550 nm for a stationary galaxy is shifted to 430 nm for S. (200 words)
- d)) Electrons in a television set are accelerated through a potential difference of 40 kV. Assuming that the electrons start from rest, calculate their velocity using the relativistic equation for the kinetic energy. (200 words)
- e)) A particle of mass M, initially at rest, decays into two particles with rest masses m₁ and m2 respectively. Show that the total energy of the mass m₁ is: E₁ = c² [M² + m² - m²] / 2M (200 words)
- Time dilation: Moving clocks run slower, observed lifetime τ = γτ₀.
- Length contraction: Moving objects appear shorter, observed length L = L₀/γ.
- Relativistic Doppler Effect: Wavelength shift indicates relative speed and direction.
- Relativistic Kinetic Energy: K.E. = (γ-1)mc² for particles near light speed.
Answer: This question delves into several fundamental concepts of Modern Physics, primarily Special Relativity, applying its principles to real-world phenomena like particle decay, interstellar travel, and astronomical observations. It covers time dilation, length contraction, the relativistic Doppler effect, relativistic kinetic energy, and the conservation laws in particle decay. Understanding the Lorentz factor (γ) and the interrelation between energy, momentum, and mass is crucial for solving these ...