Hydrogen in strong magnetic fields in neutron star surfaces

被引：3
|
作者：
Salpeter, EE [1 ]
机构：
[1] Cornell Univ, Ithaca, NY 14853 USA
来源：
JOURNAL OF PHYSICS-CONDENSED MATTER | 1998年 / 10卷 / 49期
关键词：
D O I：
10.1088/0953-8984/10/49/017
中图分类号：
O469 [凝聚态物理学];
学科分类号：
070205 ;
摘要：
In magnetic fields of very much more than 2 x 10(9) G, polyatomic hydrogen molecules, in the form of long chains, are stable. in neutron star surfaces, fields of 10(13) G are commonplace and 10(15) G has been reported. Liquid hydrogen can form at the higher field with a zero-pressure density of about 10(6) g cm(-3). At these densities, hydrogen can burn to helium by pycnonuclear reactions even at low temperatures-the 'real cold fusion'.
引用
收藏
页码：11285 / 11288
页数：4
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