Quantum condensation of particles is one of the most amazing phenomena exhibited by many-body systems. Familiar yet striking examples known for many decades include superconductivity of metals at low temperatures and superfluidity of liquid 4He. More recently the realization of Bose-Einstein condensation of ultracold atoms in traps has created an exciting new field of quantum many-body physics. Also, atomic nuclei and neutron stars can experience quantum condensation of fermion pairs and display superfluid properties. However, in nuclear physics the most tightly bound light cluster is not a pair but a quartet, namely the alpha particle. Can we then expect α-particle condensation in nuclei? Before pursuing to this question, let us make some general remarks. It is a fact that quartetting is more pronounced in nuclei than in most other Fermi systems. And the dominance of quartetting can be traced to the fact that nucleons can exist in four different internal states: proton and neutron, each with spin up or down, all attracting each other. Therefore, a shell model picture in which the α-particle is the first doubly magic nucleus, with a filled 0S–level, is valid (see below, Fig. 2). Moreover, the α-particle is especially stiff, with its first excited state lying quite high, at ∼ 20 MeV. The search is now on for quartets in systems other than nuclei.
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