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Introduction

Much of our knowledge of nuclear physics comes from the study of nuclear reactions. We consider nuclear reactions resulting from a collision between two nuclei. As a result, we can have a rearrangement of the nucleons so that the final state differs from the intial state. We consider mainly final states in which there are one or two nuclei.

Nuclear reactions are thus a transition between an initial state and a final state.

Binary reactions with a two-body final state may generally be denoted as

displaymath1779

where a is a projectile, A a target nucleus, b an ejectile and B a residual nucleus. This is often represented as

displaymath1780

Many important reactions are of this type.

Some examples of reactions (note also the notation) are

Elastic scattering
tex2html_wrap_inline1811 -- no change in the internal energy of the constituents.
Inelastic scattering
tex2html_wrap_inline1813 -- there is a change in the internal energy of the tex2html_wrap_inline1815 , and hence in the energy of the outgoing alpha (hence the prime).
Pickup reaction
tex2html_wrap_inline1817 . A proton is ``picked up'' from the target nucleus. This is a typical rearrangement collision.

The final states that are accessible in a collision are governed by the conservation laws. For the reaction above, conservation of baryon number and charge results in tex2html_wrap_inline2379 and tex2html_wrap_inline2381 . As long as we are not dealing with beta decays, the number of protons and neutrons in a reaction are separately conserved.



Physics Department
Wed Nov 6 08:30:28 GMT+0200 1996