Abstract
This paper reports a new 3D sub-quadratic Lorenz-like system and proves the existence of two pairs of heteroclinic orbits to two pairs of nontrivial equilibria and the origin, which are completely different from the existing ones to the unstable origin and a pair of stable nontrivial equilibria in the published literature. This motivates one to further explore it and dig out its other hidden dynamics: Hopf bifurcation, invariant algebraic surface, ultimate boundedness, singularly degenerate heteroclinic cycle and so on. Particularly, numerical simulation illustrates that the Lorenz-like chaotic attractors coexist with one saddle in the origin and two stable nontrivial equilibria, which are created through the broken infinitely many singularly degenerate heteroclinic cycles and explosions of normally hyperbolic stable foci \(E_{z}.\)
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Acknowledgements
This work was supported in part by the National Natural Science Foundation of China under Grant 12001489, in part by Natural Science Foundation of Zhejiang Guangsha Vocational and Technical University of construction under Grant 2022KYQD-KGY, in part by Zhejiang Public Welfare Technology Application Research Project of China Grant LGN21F020003, in part by Natural Science Foundation of Taizhou University under Grant T20210906033, and in part by NSF of Zhejiang Province under Grant LY20A020001, LQ18A010001. At the same time, the authors wish to express their sincere thanks to the anonymous editors and reviewers for their conscientious reading and numerous valuable comments which improved immensely the presentation of this paper.
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HW: conceptualization, software, writing—original draft, visualization, investigation. GK: supervision, software, methodology, investigation, visualization. JP: software, visualization, validation, writing—review and editing. FH: software, validation. HF: software, validation, writing—review and editing. QS: validation, writing—review and editing.
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Wang, H., Ke, G., Pan, J. et al. Two pairs of heteroclinic orbits coined in a new sub-quadratic Lorenz-like system. Eur. Phys. J. B 96, 28 (2023). https://doi.org/10.1140/epjb/s10051-023-00491-5
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DOI: https://doi.org/10.1140/epjb/s10051-023-00491-5