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Neutron star motion in the disk galaxy

The neutron star motions are based on the undisturbed finitely thick galactic disk gravitational potential model. Two initial conditions, i.e. the locations and velocities, are considered. The Monte Carlo method is employed to separate rich diversities of the orbits of neutron stars into several sor... Full description

Journal Title: Chinese Physics Letters 2010, Vol.27(11), p.119801 (4pp)
Main Author: Wei, Ying-Chun
Other Authors: Taani, A. , Pan, Yuan-Yue , Wang, Jing , Cai, Yan , Liu, Gao-Chao , Luo, A-Li , Zhang, Hong-Bo , Zhao, Yong-Heng
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: ISSN: 0256-307X ; E-ISSN: 1741-3540 ; DOI: 10.1088/0256-307X/27/11/119801
Link: http://dx.doi.org/10.1088/0256-307X/27/11/119801
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recordid: iop10.1088/0256-307X/27/11/119801
title: Neutron star motion in the disk galaxy
format: Article
creator:
  • Wei, Ying-Chun
  • Taani, A.
  • Pan, Yuan-Yue
  • Wang, Jing
  • Cai, Yan
  • Liu, Gao-Chao
  • Luo, A-Li
  • Zhang, Hong-Bo
  • Zhao, Yong-Heng
subjects:
  • 不规则运动
  • 中子星
  • 银河系
  • 地球重力场模型
  • 磁盘
  • 蒙特卡罗方法
  • 大肠杆菌
  • 多样性
ispartof: Chinese Physics Letters, 2010, Vol.27(11), p.119801 (4pp)
description: The neutron star motions are based on the undisturbed finitely thick galactic disk gravitational potential model. Two initial conditions, i.e. the locations and velocities, are considered. The Monte Carlo method is employed to separate rich diversities of the orbits of neutron stars into several sorts. The Poincaré section has the potential to play an important role in the diagnosis of the neutron star motion. It has been observed that the increasing ratio of the motion range vertical to the galactic plane to that parallel to the galactic plane results in the irregularity of neutron star motion.
language: eng
source:
identifier: ISSN: 0256-307X ; E-ISSN: 1741-3540 ; DOI: 10.1088/0256-307X/27/11/119801
fulltext: fulltext
issn:
  • 0256-307X
  • 1741-3540
  • 0256307X
  • 17413540
url: Link


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ispartofChinese Physics Letters, 2010, Vol.27(11), p.119801 (4pp)
identifier
descriptionThe neutron star motions are based on the undisturbed finitely thick galactic disk gravitational potential model. Two initial conditions, i.e. the locations and velocities, are considered. The Monte Carlo method is employed to separate rich diversities of the orbits of neutron stars into several sorts. The Poincaré section has the potential to play an important role in the diagnosis of the neutron star motion. It has been observed that the increasing ratio of the motion range vertical to the galactic plane to that parallel to the galactic plane results in the irregularity of neutron star motion.
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subject不规则运动 ; 中子星 ; 银河系 ; 地球重力场模型 ; 磁盘 ; 蒙特卡罗方法 ; 大肠杆菌 ; 多样性;
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titleNeutron Star Motion in the Disk Galaxy
descriptionThe neutron star motions are based on the undisturbed finitely thick galactic disk gravitational potential model. Two initial conditions, i.e. the locations and velocities, are considered. The Monte Carlo method is employed to separate rich diversities of the orbits of neutron stars into several sorts. The Poincaré section has the potential to play an important role in the diagnosis of the neutron star motion. It has been observed that the increasing ratio of the motion range vertical to the galactic plane to that parallel to the galactic plane results in the irregularity of neutron star motion.
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abstractThe neutron star motions are based on the undisturbed finitely thick galactic disk gravitational potential model. Two initial conditions, i.e. the locations and velocities, are considered. The Monte Carlo method is employed to separate rich diversities of the orbits of neutron stars into several sorts. The Poincaré section has the potential to play an important role in the diagnosis of the neutron star motion. It has been observed that the increasing ratio of the motion range vertical to the galactic plane to that parallel to the galactic plane results in the irregularity of neutron star motion.
doi10.1088/0256-307X/27/11/119801
date2010-11-01