Electrodynamics for nuclear matter in bulk

被引:24
|
作者
Ruffini, Remo
Rotondo, Michael
Xue, She-Sheng
机构
[1] Univ Roma La Sapienza, ICRANet, I-00185 Rome, Italy
[2] Univ Roma La Sapienza, Dept Phys, I-00185 Rome, Italy
来源
关键词
neutron stars; Thomas-Fermi equation; critical electric field; THOMAS-FERMI THEORY; EQUATION; FIELDS; ATOMS; STARS; MODEL;
D O I
10.1142/S021827180700922X
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an approach to analyze the electrodynamics of nuclear matter in bulk using the relativistic Thomas - Fermi equation. We generalize to the case of N similar or equal to (m(Planck)/ mn)(3) nucleons of mass mn an approach well tested in very heavy nuclei (Z similar or equal to 10(6)). Particular attention is given to implement the condition of charge neutrality globally on the entire configuration, versus the one usually adopted on a microscopic scale. As the limit N similar to (mPlanck/ mn) 3 is approached the penetration of electrons inside the core increases and a relatively small tail of electrons persists leading to a significant electron density outside the core. Within a region of 10(2) electron Compton wavelength near the core, surface electric fields close to the critical value for pair creation by vacuum polarization effect develop. These results can have important consequences on the understanding of physical process in neutron star structures as well as on the initial conditions leading to the process of gravitational collapse to a black hole.
引用
收藏
页码:1 / 9
页数:9
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