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OPPORTUNITIES IN NUCLEAR SCIENCE A Long-Range Plan for ...

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THE <strong>SCIENCE</strong> • ATOMIC NUCLEI: STRUCTURE AND STABILITY<br />

nuclear properties with increasing excitation energy provides<br />

a fascinating quantum analog to the general problem of transitions<br />

from ordered to chaotic motion. Very neutron-rich<br />

nuclei, far from the common isotopes found in nature, open<br />

the door to investigations of the often-unusual properties of<br />

weakly bound quantum systems. For instance, such nuclei<br />

can include regions characterized by entirely new <strong>for</strong>ms of<br />

low-density, spatially extended, nearly pure neutron matter<br />

akin to that on the surfaces of neutron stars.<br />

Recent advances in understanding the nucleus. Major<br />

conceptual and technical advances have revolutionized the<br />

study of nuclear structure over the past ten years, and<br />

nuclear structure studies have flourished with measurements<br />

and calculations aimed at nuclei both near and far<br />

from the valley of stability. Recent significant advances in<br />

several areas can be briefly summarized:<br />

• Shell structure in exotic nuclei. Investigations of<br />

nuclear shell structure far from stability are fundamental<br />

to our understanding of nuclei and their synthesis<br />

within the cosmos. Recent landmark experiments<br />

include the observation of the doubly-magic unstable<br />

nuclei 48 Ni (Z = 28, N = 20) and 78 Ni (Z = 28, N = 50).<br />

In lighter neutron-rich nuclei, spectroscopic studies<br />

have demonstrated clear evidence <strong>for</strong> a reordering of<br />

nucleonic shells; <strong>for</strong> a weakening of the familiar shell<br />

closures around N = 8, 20, and 28; and <strong>for</strong> the emergence<br />

of a new shell gap at N = 16 in the most neutronrich<br />

nuclei. These studies provide the first indications<br />

that our models of nuclear structure, developed near<br />

beta stability, are not adequate <strong>for</strong> nuclei with large<br />

neutron excesses. In the most proton-rich nuclei,<br />

where, counterintuitively, a strong Coulomb <strong>for</strong>ce<br />

inhibits charged-particle emission, proton decay has<br />

rapidly evolved from an exotic phenomenon to a powerful<br />

spectroscopic tool. First signatures of a new<br />

<strong>for</strong>m of pairing have been seen in nuclei with equal<br />

numbers of protons and neutrons, and a new decay<br />

mode, nonsequential two-proton radioactivity, has<br />

been discovered.<br />

• Collective excitations. We gain insight into the properties<br />

of nuclei by establishing and studying their<br />

basic modes of excitation. Recent advances include<br />

the discovery of the first candidates <strong>for</strong> the new collective<br />

modes of chiral rotation and wobbling motion<br />

in triaxial nuclei. Dynamical symmetries of the<br />

nuclear Hamiltonian have been explored, and the<br />

properties of nuclei with very elongated (superde<strong>for</strong>med)<br />

shapes have been elucidated. In particular,<br />

light superde<strong>for</strong>med nuclei have been discovered.<br />

They provide a unique opportunity to study the<br />

underlying microscopic structure of collective rotations.<br />

Definitive excitation energies and quantum<br />

numbers have been determined <strong>for</strong> the first time in<br />

the key superde<strong>for</strong>med nuclei 152 Dy and 194 Hg.<br />

• Synthesis, structure, and chemistry of the heaviest<br />

elements. The discovery and investigation of the<br />

heaviest nuclei test our understanding of which combinations<br />

of neutrons and protons can give rise to<br />

long-lived superheavy nuclei, and extends the periodic<br />

table, fundamental to all of chemistry.<br />

Significant achievements within the last several years<br />

include the synthesis of new superheavy elements;<br />

the first chemical studies of seaborgium (Z = 106),<br />

bohrium (Z = 107), and hassium (Z = 108); and the<br />

first in-beam gamma-ray spectroscopy of the transfermium<br />

nucleus nobelium (Z = 102).<br />

• Nuclear structure theory. Enormous progress has<br />

been made in the microscopic description of nuclei,<br />

including ab initio calculations <strong>for</strong> light nuclei and<br />

advances in the shell model and mean-field theory to<br />

include improved effective interactions and coupling<br />

to the continuum <strong>for</strong> studies of weakly bound systems.<br />

These advances enabled theorists to make<br />

detailed quantitative predictions of structure and<br />

reaction aspects of nuclei.<br />

Looking ahead: A concise roadmap. Current progress in<br />

understanding the properties of nuclei is impressive, and the<br />

field is poised <strong>for</strong> significant breakthroughs over the next<br />

decade. A deeper understanding of the atomic nucleus will be<br />

achieved by ef<strong>for</strong>ts in both nuclear structure theory and<br />

experiment, where each discipline takes its inspiration from<br />

the other. But the impetus in both areas lies increasingly with<br />

studies of nuclei under extreme conditions, especially those<br />

with extreme proton-to-neutron ratios. In the near and intermediate-term<br />

future, complementary studies both near and<br />

far from stability will be pursued at stable-beam accelerators,<br />

such as those at Argonne and Berkeley Lab and at a number<br />

of universities, as well as at existing dedicated exotic-beam<br />

facilities, especially HRIBF at Oak Ridge and the new projectile<br />

fragmentation facility of the NSCL at Michigan State. In<br />

the longer term, the properties of the new and currently inaccessible<br />

rare isotopes that inhabit the very boundaries of the<br />

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