https://doi.org/10.1140/epjc/s10052-024-12942-z
Regular Article – Theoretical Physics
-Dirac stars
1
School of Physical Science and Technology, Lanzhou University, 730000, Lanzhou, China
2
Lanzhou Center for Theoretical Physics, Key Laboratory of Theoretical Physics of Gansu Province, and Key Laboratory of Quantum Theory and Applications of MoE, Lanzhou University, 730000, Lanzhou, China
3
Institute of Theoretical Physics and Research Center of Gravitation, Lanzhou University, 730000, Lanzhou, China
4
School of Physics and Technology, Nantong University, 226019, Nantong, China
Received:
25
April
2024
Accepted:
22
May
2024
Published online:
15
July
2024
In this paper, we construct a Dirac star model composed of pairs of spinor fields. The azimuthal harmonic indices m of these spinor fields are half-integers, and they satisfy . When , it corresponds to the conventional Dirac star model, formed by two spinor fields with and . When , among these pairs of spinor fields, there exist spinor fields with azimuthal harmonic indices , and all spinor fields still conform to the same Dirac field equation. Different families of solutions are distinguished by the value of , so we named these solutions -Dirac stars. We obtain solutions for by using numerical methods. Additionally, we compute their ADM mass M, Noether charge Q, and binding energy E, and illustrate how these quantities change with the spinor field’s frequency for different . We observe significant differences between solutions for and the case. Furthermore, we provide the energy density distribution of the Dirac stars, wherein for scenarios, the Dirac stars exhibit a spherical shell-like structure. Moreover, we employ three-dimensional diagrams to intuitively depict how influences the combination of spinor fields to form a spherically symmetric configuration.
© The Author(s) 2024
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