Relativistic Corrections to the CBF Effective Nuclear Hamiltonian
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arXiv
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| Format: | Preprint |
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2024
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| _version_ | 1866929612377817088 |
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| author | Sabatucci, Andrea Benhar, Omar Lovato, Alessandro |
| author_facet | Sabatucci, Andrea Benhar, Omar Lovato, Alessandro |
| contents | We discuss the inclusion of relativistic boost corrections into the CBF effective nuclear Hamiltonian, derived from a realistic model of two- and three-nucleon interactions using the formalism of correlated basis functions and the cluster expansion technique. Different procedures to take into account the effects of boost interactions are compared on the basis of the ability to reproduce the nuclear matter equation of state obtained from accurate many-body calculations. The results of our study show that the repulsive contribution of the boost interaction significantly depends on the underlying model of the non relativistic potential. On the other hand, the dominant relativistic correction turns out to be the corresponding reduction of the strength of repulsive three-nucleon interactions, leading to a significant softening of the equation of state at supranuclear densities. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2406_05732 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Relativistic Corrections to the CBF Effective Nuclear Hamiltonian Sabatucci, Andrea Benhar, Omar Lovato, Alessandro Nuclear Theory General Relativity and Quantum Cosmology We discuss the inclusion of relativistic boost corrections into the CBF effective nuclear Hamiltonian, derived from a realistic model of two- and three-nucleon interactions using the formalism of correlated basis functions and the cluster expansion technique. Different procedures to take into account the effects of boost interactions are compared on the basis of the ability to reproduce the nuclear matter equation of state obtained from accurate many-body calculations. The results of our study show that the repulsive contribution of the boost interaction significantly depends on the underlying model of the non relativistic potential. On the other hand, the dominant relativistic correction turns out to be the corresponding reduction of the strength of repulsive three-nucleon interactions, leading to a significant softening of the equation of state at supranuclear densities. |
| title | Relativistic Corrections to the CBF Effective Nuclear Hamiltonian |
| topic | Nuclear Theory General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2406.05732 |