Match the nuclear processes given in Column I with the appropriate option(s) in Column II.Column IColumn II(A) Nuclear fusion(P) Absorption of thermal neutrons by (B) Fission in a nuclear reactor(Q) nucleus(C) β-decay(R) Energy production in stars via hydrogen conversion to helium(D) γ-ray emission (S) Heavy water (T) Neutrino emission.

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Nucleus and Nuclear Force

Mass Defect Q Value Binding Energy Stability of Nucleus and Nucleus and Nuclear Reactions

Question

Match the nuclear processes given in Column I with the appropriate option(s) in Column II.

Column I	Column II
(A) Nuclear fusion	(P) Absorption of thermal neutrons by $_{92}^{235} U$
(B) Fission in a nuclear reactor	(Q) $_{27}^{60} Co$ nucleus
(C) β-decay	(R) Energy production in stars via hydrogen conversion to helium
(D) γ-ray emission	(S) Heavy water
	(T) Neutrino emission.

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Nuclear fusion - Energy production in stars via hydrogen conversion to He.

- In nuclear fusion reaction emission of neutrinos is very common.

Nuclear fission - Involves absorption of thermal neutrons.

- Heavy water is used as moderator.

- In nuclear fission reaction emission of neutrinos is very common.

β-decay - Cobalt-60 is used as source of β-particle

- Neutrino's are also released with β-particle.

γ-ray emission - After absorpsion of thermal neutrons emission of γ-radiations may take place.

- Co⁶⁰ also involves γ-radiation.

- γ-emission is common in both fission and fusion reaction.