The equilibrium equations of Boson-Fermi systems in the Newtonian approximation

The equilibrium equations of Boson-Fermi systems in the Newtonian approximation
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牛顿近似中玻色子-费米系统的平衡方程

DOI:
10.1002/asna.201913599
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发表时间:
2019-01
影响因子:
0.9
通讯作者:
H. Shan
H. Shan
中科院分区:
物理与天体物理4区
文献类型:
--
作者:
Z. F. Gao;D. L. Song;X. D. Li;H. Shan

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There is accumulating evidence that scalar fields may exist in nature. The gravitational collapse of a boson cloud leads to the formation of a boson star just like white dwarfs and neutron stars. In general, as one of the candidates of dark matter, a boson star holds a stable configuration and has deserved intensive attention and extensive research in the past 50years. At first, we analyze the ground state solutions for a Boson-Fermi system using the metric tensor in the Newtonian approximation, then analyze the configuration of a star composed of bosons and fermions. At last, for the purpose of investigating the equilibrium geometry of a Boson-Fermi system, we construct the virial equations of a boson-Fermi system with different orders. In our future work, we will explore the equilibrium configuration and the stability of a Boson-Fermi star and how a scalar field affects the pressure of the system using higher-order virial equations of fluid motions.
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