LOYOLA COLLEGE (AUTONOMOUS), CHENNAI – 600 034
B.Sc. DEGREE EXAMINATION – PHYSICS
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FIFTH SEMESTER – November 2008
PH 5500 – ATOMIC & NUCLEAR PHYSICS
Date : 03-11-08 Dept. No. Max. : 100 Marks
Time : 9:00 – 12:00
PART – A
Answer ALL questions: (10×2=20 Marks)
- Why do the traces of parabola in Thomson’s method not pass through the origin?
- State the advantages of Aston’s mass spectrograph.
- The Kα line of molybdenum has a wavelength of 0.7078Å.Calculate the wavelength of the Kα line of copper. Atomic number of molybdenum is 42 and of copper is 29.
- The photoelectric threshold for a metal is 3000Å. Find the kinetic energy of an electron ejected from it by radiation of wavelength 1200 Å.
- What are isotones and isotopes?
- Calculate the binding energy in MeV of deutrons. Given, mass of 1H1=1.008145amu,
mass of 0n11.008987amu and mass of 1H2=2.014741amu.
- A reactor is developing energy at the rate of 32×106 How many atoms of U235 undergo fission per sec? Assume that on the average an energy of 200 MeV is released per fission.
- Distinguish between slow and fast neutrons.
- What are cosmic rays?
- What are particles and antiparticles? Give two examples.
PART – B
Answer any FOUR questions: (4×7.5=30 Marks)
- Explain the two types of coupling schemes between the orbital and spin angular momenta.
- Explain the different types of photoelectric cells and their action.
- a) Explain mass defect and binding energy. (3)
- b) Explain the variation of binding energy with mass number and discuss its salient
features. (4.5)
- a) What do you mean by chain reaction? (2.5)
- b) Explain controlled and uncontrolled chain reaction. (5)
- a) Explain the main features of shell model of a nucleus. (5)
- b) What are magic numbers? (2.5)
PART – C
Answer any FOUR questions: (4×12.5=50 Marks)
- a) Describe Stern-Gerlach experiment. Discuss its significance. (10)
- b) Why is an inhomogeneous magnetic field required in the experiment? (2.5)
- a) Explain Millikan’s experimental verification of Einstein’s photoelectric equation. (10)
- b) Photon of energy 1.02MeV undergoes Compton scattering through 180°. Calculate the
wavelength of scattered photon. (2.5)
- a) Give the origin of β -ray line and continuous spectra. (10)
- b) Find out the stable nucleus that has a radius half of Fe56. (2.5)
- Describe the construction and working of a nuclear reactor.
- Discuss the latitude,altitude and east-west effects of cosmic rays. Plot the concerned
graphs.