Elsevier

Physics Reports

Volume 124, Issue 1, July 1985, Pages 1-68
Physics Reports

The nucleon-nucleon interaction and the nuclear many-body problem

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  • Cited by (174)

    • Chiral symmetry and effective field theories for hadronic, nuclear and stellar matter

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      In microscopic many-body perturbation theory, the optical model potential is identified with the nucleon self energy [127], a complex-valued quantity whose imaginary part in the context of nuclear scattering accounts for the strongly absorptive features of the nucleon–nucleus interaction. Numerous calculations of the optical potential have been carried out with realistic nuclear forces using a variety of many-body methods with differing degrees of reliability [128–134]. Here we review the recent calculations [135,100,136] that have been performed in the framework of chiral effective theory.

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      As students, Gerry told us on more than one occasion that his work with Tom Kuo in the 1960s deriving shell model Hamiltonians from the NN interaction [1,2] was his proudest achievement. Gerry was similarly fond of his work in the 1970s and 1980s with Babu, Bäckman, Niskanen, and others, where they used a combination of microscopic many-body theory and experimental constraints to derive the Fermi liquid parameters from the underlying NN interaction, see Ref. [3] for a review. Perhaps his sentimental attachment to both of these problems, and to many-body problems in general, stemmed from the fact that he fearlessly chose to work on them at a time when many of the leading physicists, whom he deeply admired, most notably Migdal and Wigner, told him he was crazy to work on problems that were, in their minds, almost completely intractable.

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    Work supported in part by U.S. Department of Energy Contract No. DE-ACo2-76ER13001.

    On leave from Department of Physics, Åbo Akademi, Porthansgatan 3, 20500 Åbo 50, Finland.

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