中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页
机构
成果
学者
登录
注册
登陆
×
验证码:
换一张
忘记密码?
记住我
×
校外用户登录
CAS IR Grid
机构
理论物理研究所 [4]
高能物理研究所 [1]
中国科学院大学 [1]
软件研究所 [1]
采集方式
OAI收割 [6]
iSwitch采集 [1]
内容类型
期刊论文 [7]
发表日期
2022 [2]
2021 [1]
2020 [1]
2018 [1]
2009 [2]
学科主题
Physics [3]
Astronomy ... [1]
Computer S... [1]
Informatio... [1]
筛选
浏览/检索结果:
共7条,第1-7条
帮助
条数/页:
5
10
15
20
25
30
35
40
45
50
55
60
65
70
75
80
85
90
95
100
排序方式:
请选择
题名升序
题名降序
提交时间升序
提交时间降序
作者升序
作者降序
发表日期升序
发表日期降序
Search for the Gravitational-wave Background from Cosmic Strings with the Parkes Pulsar Timing Array Second Data Release
期刊论文
OAI收割
ASTROPHYSICAL JOURNAL, 2022, 卷号: 936, 期号: 1, 页码: 20
作者:
Chen, Zu-Cheng
;
Wu, Yu-Mei
;
Huang, Qing-Guo
  |  
收藏
  |  
浏览/下载:25/0
  |  
提交时间:2023/01/16
HOLE BINARY-SYSTEMS
SPIN NOISE
MODEL
RADIATION
LIMITS
PACKAGE
TEMPO2
Searching for isotropic stochastic gravitational-wave background in the international pulsar timing array second data release
期刊论文
OAI收割
COMMUNICATIONS IN THEORETICAL PHYSICS, 2022, 卷号: 74, 期号: 10, 页码: 105402
作者:
Chen, Zu-Cheng
;
Wu, Yu-Mei
;
Huang, Qing-Guo
  |  
收藏
  |  
浏览/下载:15/0
  |  
提交时间:2023/01/16
HOLE BINARY-SYSTEMS
RADIATION
PACKAGE
TEMPO2
LIMITS
PROBE
Non-tensorial gravitational wave background in NANOGrav 12.5-year data set
期刊论文
OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2021, 卷号: 64, 期号: 12, 页码: 120412
作者:
Chen, Zu-Cheng
;
Yuan, Chen
;
Huang, Qing-Guo
  |  
收藏
  |  
浏览/下载:7/0
  |  
提交时间:2023/01/16
PULSAR-TIMING PACKAGE
HOLE BINARY-SYSTEMS
ARRAY LIMITS
BLACK-HOLES
SEARCH
CONSTRAINTS
RADIATION
TEMPO2
PROBE
An underlying clock in the extreme flip-flop state transitions of the black hole transient Swift J1658.2-4242
期刊论文
OAI收割
Astronomy and Astrophysics, 2020, 卷号: 641, 页码: A101
作者:
HXMT
  |  
收藏
  |  
浏览/下载:58/0
  |  
提交时间:2022/02/08
accretion
accretion disks
black hole physics
X-rays: binaries
time
Astrophysics - High Energy Astrophysical Phenomena
Abstract:
Aims: Flip-flops are top-hat-like X-ray flux variations, which have been observed in some transient accreting black hole binary systems, and feature simultaneous changes in the spectral hardness and the power density spectrum (PDS). They occur at a crucial time in the evolution of these systems, when the accretion disc emission starts to dominate over coronal emission. Flip-flops remain a poorly understood phenomenon, so we aim to thoroughly investigate them in a system featuring several such transitions.
Methods: Within the multitude of observations of
Swift J1658.2-4242
during its outburst in early 2018, we detected 15 flip-flops, enabling a detailed analysis of their individual properties and the differences between them. We present observations by XMM-Newton, NuSTAR, Astrosat, Swift, Insight-HXMT, INTEGRAL, and ATCA. We analysed their light curves, searched for periodicities, computed their PDSs, and fitted their X-ray spectra, to investigate the source behaviour during flip-flop transitions and how the interval featuring flip-flops differs from the rest of the outburst.
Results: The flip-flops of Swift J1658.2-4242 are of an extreme variety, exhibiting flux differences of up to 77% within 100 s, which is much larger than what has been seen previously. We observed radical changes in the PDS simultaneous with the sharp flux variations, featuring transitions between the quasi-periodic oscillation types C and A, which have never been observed before. Changes in the PDS are delayed, but more rapid than changes in the light curve. Flip-flops occur in two intervals within the outburst, separated by about two weeks in which these phenomena were not seen. Transitions between the two flip-flop states occurred at random integer multiples of a fundamental period of 2.761 ks in the first interval and 2.61 ks in the second. Spectral analysis reveals the high and low flux flip-flop states to be very similar, but distinct from intervals lacking flip-flops. A change of the inner temperature of the accretion disc is responsible for most of the flux difference in the flip-flops. We also highlight the importance of correcting for the influence of the dust scattering halo on the X-ray spectra.
GWs from S-stars Revolving Around SMBH at Sgr A
期刊论文
OAI收割
COMMUNICATIONS IN THEORETICAL PHYSICS, 2018, 卷号: 70, 期号: 6, 页码: 735-748
作者:
Cai, RG
;
Liu, TB
;
Wang, SJ
  |  
收藏
  |  
浏览/下载:23/0
  |  
提交时间:2019/07/19
MASSIVE BLACK-HOLE
POST-NEWTONIAN MOTION
GRAVITATIONAL-RADIATION
BINARY-SYSTEMS
ASTROPHYSICS
EVOLUTION
POINT
SPACE
WAVES
A direct construction of polynomial-size obdd proof of pigeon hole problem
期刊论文
iSwitch采集
Information processing letters, 2009, 卷号: 109, 期号: 10, 页码: 472-477
作者:
Chen, Wei
;
Zhang, Wenhui
收藏
  |  
浏览/下载:32/0
  |  
提交时间:2019/05/10
Propositional proof systems
Binary decision diagrams
Pigeon hole problem
Proof complexity
Computational complexity
a direct construction of polynomial-size obdd proof of pigeon hole problem
期刊论文
OAI收割
INFORMATION PROCESSING LETTERS, 2009, 卷号: 109, 期号: 10, 页码: 472-477
Chen Wei
;
Zhang Wenhui
  |  
收藏
  |  
浏览/下载:23/0
  |  
提交时间:2011/03/18
Propositional proof systems
Binary decision diagrams
Pigeon hole problem
Proof complexity
Computational complexity