中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
机构
理论物理研究所 [2]
高能物理研究所 [2]
采集方式
OAI收割 [4]
内容类型
期刊论文 [4]
发表日期
2020 [1]
2018 [1]
2014 [1]
2013 [1]
学科主题
Physics [3]
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Introducing a special collection of papers in the Journal of High Energy Astrophysics on the Early Results of China's 1st X-ray Astronomy Satellite: Insight-HXMT
期刊论文
OAI收割
Journal of High Energy Astrophysics, 2020, 卷号: 27, 页码: 51-52
作者:
HXMT
  |  
收藏
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浏览/下载:51/0
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提交时间:2022/02/08
Astrophysics - High Energy Astrophysical Phenomena
Abstract: Insight-HXMT is the first Chinese X-ray astronomical mission, launched successfully on June 15, 2017, from China's Jiuquan Satellite Launch Center. Insight-HXMT was designed to have a broad energy coverage in X-rays, from 1-250 keV, with excellent timing and adequate energy resolution at soft X-rays, and the largest effective area at hard X-rays. This allows, in particular, to observe bright sources like X-ray binaries (XRBs) in their bright/outburst states with high cadence and high statistics at hard and soft X-rays at once. It was then expected that the Insight-HXMT mission will bring us new insights regarding the characteristics of several source classes. Examples include characterizing High-Mass X-ray Binaries (HMXBs) and the outburst evolution of Low-Mass X-ray Binaries (LMXBs). For instance, in HMXB systems, the region around their Alfven radius that is responsible to determine whether accretion or propeller occurs, or the region around the NS magnetic pole where the intense X-rays are supposed to be produced are specially appealing targets of study. For the LMXBs, the evolution the outburst and the properties of the compact objects themselves are obvious priority targets for Insight-HXMT. Due to the broad coverage in energy, Insight-HXMT is specially well suited to study the influence of thermonuclear (type-I) X-ray bursts upon the surrounding environment.
Solving the muon g-2 anomaly in CMSSM extension with non-universal gaugino masses
期刊论文
OAI收割
JOURNAL OF HIGH ENERGY PHYSICS, 2018, 期号: 12, 页码: 41
作者:
Wang, F
;
Wang, K
;
Yang, JM
;
Zhu, JY
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收藏
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浏览/下载:33/0
  |  
提交时间:2019/07/19
HIGGS-BOSON MASS
SUPERSYMMETRIC STANDARD MODEL
GENERAL RENORMALIZABLE THEORY
HIGH-PRECISION PREDICTIONS
SCALAR SELF-ENERGIES
MAGNETIC-MOMENT
DARK-MATTER
2-LOOP CORRECTIONS
POLE MASSES
MSSM
Cosmological parameter estimation from CMB and X-ray cluster after Planck
期刊论文
OAI收割
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2014, 期号: 5, 页码: 20
作者:
Hu, JW
;
Cai, RG
;
Guo, ZK
;
Hu, B
收藏
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浏览/下载:44/0
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提交时间:2015/06/03
MICROWAVE BACKGROUND ANISOTROPIES
BARYON ACOUSTIC-OSCILLATIONS
MASS-TEMPERATURE RELATION
SOUTH-POLE TELESCOPE
SPT-SZ SURVEY
GALAXY CLUSTERS
HUBBLE CONSTANT
POWER SPECTRUM
CHANDRA SAMPLE
DAMPING TAIL
Measurement of masses in the t(t)over-tilde system by kinematic endpoints in pp collisions at root s=7 TeV
期刊论文
OAI收割
EUROPEAN PHYSICAL JOURNAL C, 2013, 卷号: 73, 期号: 7
作者:
CMS Collaboration
收藏
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浏览/下载:18/0
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提交时间:2015/12/02
TOP-QUARK
STANDARD MODEL
HIGGS-BOSON
POLE MASS
PARTICLE