CRYSTALLINE-STRUCTURE OF THE MIXED CONFINED-DECONFINED PHASE IN NEUTRON-STARS

被引：60

作者：

GLENDENNING, NK ^{[1
]}

PEI, S ^{[1
]}

机构：

[1] BEIJING NORMAL UNIV, DEPT PHYS, BEIJING 100875, PEOPLES R CHINA

来源：

PHYSICAL REVIEW C | 1995年 / 52卷 / 04期

关键词：

D O I：

10.1103/PhysRevC.52.2250

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

We calculate that the geometrical structure of the crystalline solid mixed phase of confined-deconfined hadronic matter in neutron stars-its form, size, spacing, and location in the star-is highly individualistic according to small changes in the stellar mass. This suggests a possible connection with the wide range of glitch behavior observed in different pulsars, since glitches are almost certainly associated with solid regions.

引用

页码：2250 / 2253

页数：4

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