Emergence of Cluster Formation in Light Nuclei
Jos\'e Nicol\'as Orce, Manfred Jason Jaftha

TL;DR
This paper demonstrates that using experimentally derived deformation parameters within a specific coordinate transformation reveals the most probable nuclear shapes, elucidating cluster formation in light nuclei and providing insights into triaxiality.
Contribution
It introduces a method to identify the most probable nuclear shape from experimental data, explaining cluster emergence and triaxiality in light and deformed nuclei.
Findings
Cluster formation in light nuclei is spatially revealed.
Bowling-pin shapes of $^{10}$B and $^{20}$Ne are reproduced.
The approach captures superpositions of intrinsic configurations.
Abstract
Spherical harmonics form a complete orthonormal basis which allows any function on the sphere to be expanded. The nuclear shape of a given eigenstate can thus be described within Bohr's quasi-molecular model by a coordinate transformation from a randomly oriented ellipsoid in space to a coordinate system aligned with the ellipsoid's principal axes. This transformation (Eq. 4) is characterized by three Euler angles and two deformation parameters, (quadrupole) and (triaxiality), but does not uniquely define the nuclear shape; rotational averaging over equivalent orientations is expected to yield a diffuse nuclear shape. Rotational invariance under and is achieved using three transformation operators, which define a new coordinate system aligned with a single intrinsic configuration (Eq. 6). Here we show that the non-unique coordinate system of Eq. 4 with…
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