Figure 1.Experiments at the NPL studied many reactions of the type A(a,b)B (or A+a → B+b) in which a fragment x is transferred between the target nucleus A and the projectile a. Niels Bohr discussed only those nuclear reactions that occur via formation of a compound nucleus (CN) which subsequently breaks up into a final nucleus B and an ejectile b, as shown in Fig. 1. Because the compound nucleus lives long enough to "forget" how it was formed, the CN mechanism results in the c.m. angular distribution of b having a symmetrical U-shaped form, as shown in Fig. 2.
Figure 2.However, the success of models introduced by Serber [SER47] in 1947 (see Fig. 3) and Butler [BUT51] in 1951 showed that at higher energies some transfer reactions can occur "directly" in one step, without formation of a compound nucleus. The simplest direct transfer reactions are (d,p) "stripping" and (p,d) "pickup", in which it is a neutron that is transferred.
Many more direct transfer reactions were identified at the NPL as well as other laboratories. Diagrams showing the simplest direct mechanisms for generalized stripping and pickup reactions are shown in Figs. 4 and 5. In these diagrams the horizontal dashed lines symbolize the effect of elastic scattering of a and A (or b and B) through the appropriate optical potential Ua (or Ub). These diagrams correspond to what is called the Distorted-Waves Born Approximation (DWBA) [AUS70] for the transition amplitude. DWBA treats the iterated interaction that binds x and a (or x and b) as a perturbation; this is found to be a successful first approximation, even though strong interactions are involved.
Figure 3.In Figs. 3 and 4 the vertices involving a, b, and x can be described quite well for our purposes from knowledge of the structure of the fairly simple particles a, b, and x. In contrast, the nuclear vertices involving A, B, and x depend on the structure of the nuclei A and B under investigation. The nuclear vertex (and hence the transition amplitude) is proportional to a certain spectroscopic matrix element:
For pickup, transition amplitude
For stripping, transition amplitude
Here ΦAiis the initial state of the target and ΦBf is the state in which the final nucleus is detected. The operator a↑N ljm is the creation operator for fragment x in a single-particle state with radial quantum number n, orbital angular momentum l, and total angular momentum jm, while its Hermitian conjugate aNljm is the corresponding destruction operator. The cross sections dσ/dΩ are proportional to spectroscopic factors Sfinljm, which are the absolute squares of the spectroscopic matrix elements:
For pickup,
For stripping,
Figure 4.
Figure 5.
It follows that, provided the direct reaction mechanism is valid, it is possible to use transfer reactions to measure spectroscopic factors. Because the cross section is proportional to the spectroscopic factor, an equation of the type
is used for practical analysis of experiments, with
calculated by DWBA. A particularly important quantity is l, the orbital angular
momentum of the transferred particle. The angular distribution of the
cross section depends on the value of l. This can be seen from
a simple version of the plane-wave Butler theory, in which the reaction
is assumed to occur only at the surface of the target nucleus, which is
taken as a sphere of radius R. This gives for the angular distribution
Figure 6.Here jl(qR) is a spherical Bessel function, pa and p b are the momenta of the projectile and the ejectile, respectively, and θ is the scattering angle. A more physical explanation of the l dependence is given on page 353 of the book [COH71] by B. L. Cohen. The l dependence of the angular distribution can be used to determine l, as illustrated in Fig. 7.
Spectroscopic factors give information that is very useful in determining the structure of individual nuclear states. As a simple example, consider the stripping reaction 16O(d,p)17O beginning with the target nucleus 16 O in its ground state. Suppose that (as specified by the simplest version of the shell model) the ground state of 17 O consists of an 16 O ground state core with a neutron in an N = 2, l = 2, j = 5/2 state orbiting around it. Then the corresponding spectroscopic factor should be exactly 1, and measurements of the stripping cross section (combined with calculations of the DWBA cross section) should confirm this. If, however, the ground state of 17 O contains appreciable components in which the 16 O core is not in its ground state, the spectroscopic factor will be appreciably less than 1, and the measurements should be able to reveal this. As always happens in nuclear physics with strongly interacting probes, there are uncertainties in the reaction mechanism and in the optical potentials that should be used in the DWBA calculations, so care must be exercised in analyzing the results of experiments.
Figure 7.