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Clusters in Nuclei, Volume 3 pp 95–145Cite as

From Light to Hyper-heavy Molecules and Neutron-Star Crusts in a Dynamical Mean-Field Approach

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Part of the book series: Lecture Notes in Physics ((LNP,volume 875))

Abstract

The richness of phenomena occurring in heavy-ion collisions calls for microscopic approaches where the motion of each nucleon is treated quantum mechanically. The most popular microscopic approach for low-energy collisions between atomic nuclei is the time-dependent Hartree-Fock (TDHF) theory, providing a quantum mean-field dynamics of the system. The TDHF approach and some of its extensions are used to predict the evolution of out-of-equilibrium nuclear systems. The formation of di-nuclear systems with a structure close to molecular states is investigated. In particular, lifetimes and exit channels are described. The formation of light molecules and the dynamics of α-clustering are discussed. Di-nuclear systems formed in transfer, deep-inelastic, and quasi-fission reactions, as well as hyper-heavy molecules produced in reactions between actinides are also investigated. The formation and stability of structures in neutron star crusts are finally discussed.

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Acknowledgements

Long term theoretical collaborations with D. Lacroix, Ph. Chomaz, and B. Avez are acknowledged. Some of the calculations have been performed in collaboration with B. Avez, C. Golabek, D.J. Kedziora, D. Lebhertz, and A. Wakhle. The redaction of this chapter would not have been possible without numerous scientific exchanges with theoreticians and experimentalists. In particular, discussions with E. Ackad, G. Adamian, N. Antonenko, Ch. Beck, M. Bender, K. Bennaceur, S. Courtin, M. Dasgupta, T. Duguet, M. Evers, W. Greiner, F. Gulminelli, F. Haas, D.J. Hinde, D. Jacquet, D.H. Luong, J. Meyer, J.A. Maruhn, M. Morjean, V. de la Mota, M.-G. Porquet, R. du Rietz, N. Rowley, M.-D. Salsac, P. Schuck, F. Sébille, E. Suraud, and S. Umar are acknowledged. E. Ackad, N. Chamel, M. Evers, J.A. Maruhn, V. de la Mota, W. Newton, F. Sébille, and S. Umar are warmly thanked for providing figures of their own works. The calculations with the tdhf3d code were performed on the Centre de Calcul Recherche et Technologie of the Commissariat à l’Énergie Atomique, France, and on the NCI National Facility in Canberra, Australia, which is supported by the Australian Commonwealth Government. Some of the works presented in this chapter were performed with the support from ARC grants DP0879679, DP110102858, DP110102879, and FT120100760.

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    Cédric Simenel

  2. Department of Nuclear Physics, RSPE, Australian National University, Canberra, ACT, 0200, Australia

    Cédric Simenel

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Simenel, C. (2014). From Light to Hyper-heavy Molecules and Neutron-Star Crusts in a Dynamical Mean-Field Approach. In: Beck, C. (eds) Clusters in Nuclei, Volume 3. Lecture Notes in Physics, vol 875. Springer, Cham. https://doi.org/10.1007/978-3-319-01077-9_4

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