Although the spectra of many light hypernuclei have been studied,
there are only a few experiments on hypernuclear systems
beyond the
-shell.
Most of these later data were obtained using the
reaction,
which strongly populates deeply-bound,
high-spin states due to the large momentum transfer in this reaction.
The BNL-AGS experiments surveyed the single particle nature of
hypernuclei
up to
Y, and observed peaks corresponding to the major
shell structure [1]. The KEK E140a experiment
made an intensive
spectroscopic study using the SKS spectrometer, and observed the major
shell structure of
the single particle
orbits up to
Pb [2,10].
These spectra, shown in Fig. 1 were interpreted
in terms of a
bound in a Woods-Saxon, density-dependent potential.
However, the spectra are of poor quality as seen in the spectra,
and the peak positions of the various shell structures were not well determined.
Resolutions varied from 1.5 to 4 MeV FWHM from the light to heavy systems.
The best hypernuclear spectrum in the medium-heavy
mass region was taken
for the Y by the
reaction having an energy resolution of 1.7 MeV (FWHM).
This spectrum is shown in Fig. 2 [11].
In addition to the major shell structure, the figure clearly shows
the splitting of the higher shell orbitals, e.g. the
orbit. The
origin of this splitting is under intensive discussion, and may be
related to the hypernuclear
splitting.
The progress
reaction spectroscopy has largely been driven by the
superconducting kaon spectrometer (SKS), which has momentum
resolution of 0.1 %, and a large solid angle of 100 msr
[12,13].
Using this spectrometer as a microscope, an intensive spectroscopic
study of
hypernuclei has been undertaken at KEK.
Binding energies of a
within nuclei
as heavy as Pb have been extracted from the spectra, and the
central part of the
hyperon potential has been experimentally
investigated .
For -shell
hypernuclei,
high quality hypernuclear spectra have been derived again by the
reaction at KEK PS
and the structure information on light
hypernuclei
were obtained [3].
The spectra yielded information on the hypernuclear structure such as core excited states
and also on spin-dependent
N interaction.
A sample spectrum for the
C(
,K
) reaction is shown
in Fig. 3.
Other recent progress in hypernuclear spectroscopy involves the observation of
transitions between hypernuclear states which are excited by
pion or kaon production reactions. The
rays are observed
by Germanium and NaI detectors in coincidence with the production of
bound hypernuclear levels. Because
the splitting of the hypernuclear states
by spin-dependent interactions (spin-spin and spin-orbit) is small,
high precision
ray spectroscopy is the only technique available which can directly
measure these splittings. Of course identifying hypernuclear as
opposed to nuclear gammas is difficulty and is presently limited to
states in light
hypernuclei in the low excitation region.
Previously observation of the
Li E2 and M1 transition
gave crucial information on the spin-spin interaction, and the structure change of
the nucleus when a
is added to the system [15].
The observation of the E1 gamma transition between the p
excited
and the s
ground states of
C [17]
and the determination of the splitting between 5/2
and 3/2
spin-orbit
partners in
Be [16] confirmed the smallness of the
N
spin-orbit splitting.
Both reaction and the ray spectroscopy
have greatly advanced in the past few years, but
spin splittings are too small to be observed by reaction spectroscopy.
The best energy resolution achievable by the
reaction spectroscopy
is 1.5 MeV (FWHM), and is mainly dependent on beam quality and target
thickness. Thus until improved kaon and pion beams of much higher
intensity become available, this resolution cannot be improved.
In summary, the present issues in hypernuclear spectroscopy are as follows.
Although the spin-dependent interaction is best intensively studied in
the -shell by the
-ray spectroscopy, complementary information from higher mass
nuclei and higher excitation energies will be important. However the
single particle nature of the
hyperon embedded in nuclear
matter must be studied by the spectroscopy of heavy hypernuclei,
and this is the key motivation of this proposal.