Speaker
Description
The study of atomic nuclei presents a compelling example of the challenges involved in solving many-body systems. Understanding these complexities reveals one of the most intriguing mysteries of the Universe: the fundamental information of atomic nuclei. The first theoretical models of molecular states and nucleon clustering in atomic nuclei were proposed in the 1930s [1]. In this context, we employ the relativistic Hartree-Bogoliubov (RHB) framework to explore these phenomena, which naturally incorporates critical relativistic effects such as spin-orbit interactions and scalar and vector potentials [2]. This study utilizes the RHB method to investigate nucleon clustering in nuclei near the neutron drip line, particularly at extreme conditions [3, 4]. Key insights are drawn from parameters such as the density profile and nucleon-nucleon correlation functions.
References
J. A. Wheeler, Phys. Rev. 52, 1083 (1937)
D. Vretenar, A. V. Afanasjev, G. A. Lalazissis, and P. Ring, Phys. Repo. 409, 101 (2005).
A. L. Goodman, Nuclear Physics A 352, 30 (1981).
T. Nikšić, N. Paar, D. Vretenar, and P. Ring, Comput. Phys. Commun. 185, 1808 (2014).
