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
近代物理研究所 [33]
紫金山天文台 [4]
上海应用物理研究所 [3]
理论物理研究所 [2]
数学与系统科学研究院 [2]
高能物理研究所 [2]
更多
采集方式
OAI收割 [53]
iSwitch采集 [1]
内容类型
期刊论文 [53]
会议论文 [1]
发表日期
2021 [1]
2020 [2]
2019 [2]
2016 [1]
2015 [2]
2014 [2]
更多
学科主题
Astronomy ... [3]
Physics [3]
天文学 [2]
Chemistry,... [1]
地球科学 [1]
地球科学::空间物理... [1]
更多
筛选
浏览/检索结果:
共54条,第1-10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
发表日期升序
发表日期降序
提交时间升序
提交时间降序
作者升序
作者降序
On the Terrestrial Gamma Ray Flashes Preceding Narrow Bipolar Events
期刊论文
OAI收割
Geophysical Research Letters, 2021, 卷号: 48, 页码: e92160
作者:
HXMT
  |  
收藏
  |  
浏览/下载:32/0
  |  
提交时间:2022/02/08
low frequency magnetic sferics
narrow bipolar events (NBEs)
relativistic feedback mechanism
Terrestrial Gamma ray Flashes (TGFs)
Abstract: Narrow bipolar events (NBEs) are occasionally reported to occur within a few ms after Terrestrial Gamma ray Flashes (TGFs), while the formation mechanism remains mysterious partially due to the lack of sufficient observations. Here, nine more TGFs of this scenario are reported with concurrent LF sferics and lightning location data. The gamma ray production in these TGFs preceded the occurrence of NBEs by a minimum of 60 µs up to 13.5 ms, and no other fast leader discharge was found within 20 ms before the TGF. The TGF preceded positive NBEs occurred at altitudes of 8.6-11 km in thunderstorms, likely in the high electric field (E field) region of lightning initiation. The analyses show that the NBE preceding TGFs bear harder energy spectrum with larger proportion of high energy photons than EIP related TGFs produced in association with lightning leader. Our findings support the relativistic feedback mechanism of gamma ray generation in the large scale thunderstorm E field.
Verification of Radiative Transfer Schemes for the EHT
期刊论文
OAI收割
The Astrophysical Journal, 2020, 卷号: 897, 期号: 2, 页码: 21
作者:
Gold, Roman
;
Broderick, Avery E.
;
Younsi, Ziri
;
Fromm, Christian M.
;
Gammie, Charles F.
  |  
收藏
  |  
浏览/下载:79/0
  |  
提交时间:2020/08/24
black hole physics
High energy astrophysics
Radiative transfer
Relativity
General relativity
Relativistic disks
Very long baseline interferometry
Radio astronomy
Event horizons
No pulsed radio emission during a bursting phase of a Galactic magnetar
期刊论文
OAI收割
Nature, 2020, 卷号: 587, 页码: 63-65
作者:
HXMT
  |  
收藏
  |  
浏览/下载:51/0
  |  
提交时间:2022/02/08
Astrophysics - High Energy Astrophysical Phenomena
Abstract: Fast radio bursts (FRBs) are millisecond-duration radio transients of unknown physical origin observed at extragalactic distances
1-3
. It has long been speculated that magnetars are the engine powering repeating bursts from FRB sources
4-13
, but no convincing evidence has been collected so far
14
. Recently, the Galactic magnetar SRG 1935+2154 entered an active phase by emitting intense soft íray bursts
15
. One FRB-like event with two peaks (FRB 200428) and a luminosity slightly lower than the faintest extragalactic FRBs was detected from the source, in association with a soft íray/hard-X-ray flare
18-21
. Here we report an eight-hour targeted radio observational campaign comprising four sessions and assisted by multi-wavelength (optical and hard-X-ray) data. During the third session, 29 soft-íray repeater (SGR) bursts were detected in íray energies. Throughout the observing period, we detected no single dispersed pulsed emission coincident with the arrivals of SGR bursts, but unfortunately we were not observing when the FRB was detected. The non-detection places a fluence upper limit that is eight orders of magnitude lower than the fluence of FRB 200428. Our results suggest that FRB-SGR burst associations are rare. FRBs may be highly relativistic and geometrically beamed, or FRB-like events associated with SGR bursts may have narrow spectra and characteristic frequencies outside the observed band. It is also possible that the physical conditions required to achieve coherent radiation in SGR bursts are difficult to satisfy, and that only under extreme conditions could an FRB be associated with an SGR burst.
Relativistic HPIC-LBM and its application in large temporal-spatial turbulent magnetic reconnection. Part II. Role of turbulence in the flux rope interaction
期刊论文
OAI收割
Applied Mathematical Modelling, 2019
作者:
Zhu BJ(朱伯靖)
;
Yan, Hui
;
Zhong, Ying
;
Chen, Jingkun
;
Du, Yunfei
  |  
收藏
  |  
浏览/下载:79/0
  |  
提交时间:2019/05/31
Relativistic Hpic-lbm
3d Ltstmr
Oblique Instability
Turbulent Acceleration Mechanism
Slipping Magnetic Reconnection (1 St Type Mr)
Magnetic Field Line Break-rejoin Magnetic Reconnection (2nd Type Mr)
Magnetic Energy Conversion
Event-Shape Engineering for the D-meson elliptic flow in mid-central Pb-Pb collisions at sNN=5.02 TeV
期刊论文
OAI收割
JOURNAL OF HIGH ENERGY PHYSICS, 2019, 期号: 2, 页码: —
作者:
Acharya, S
;
Acosta, FT
;
Adamova, D
;
Adler, A
;
Adolfsson, J
  |  
收藏
  |  
浏览/下载:68/0
  |  
提交时间:2019/12/30
RELATIVISTIC NUCLEAR COLLISIONS
HEAVY-ION COLLISIONS
FLAVOR HADRON DECAYS
QUARK COALESCENCE
ANISOTROPIC FLOW
ENERGY-LOSS
CHARM
THE RELATIVISTIC VLASOV-MAXWELL-BOLTZMANN SYSTEM FOR SHORT RANGE INTERACTION
期刊论文
OAI收割
KINETIC AND RELATED MODELS, 2016, 卷号: 9, 期号: 3, 页码: 515-550
作者:
Liu, Shuangqian
;
Xiao, Qinghua
收藏
  |  
浏览/下载:38/0
  |  
提交时间:2016/07/12
Relativistic Vlasov-Maxwell-Boltzmann system
large time stability
coercivity
time-velocity weighted energy method
optimal temporal decay
The Electron Fraction and the Fermi Energy of Relativistic Electrons in a Neutron Star
期刊论文
OAI收割
Publications of The Korean Astronomical Society, 2015, 卷号: 30, 页码: 569-572
作者:
Li, X. D.
;
Wang, N.
;
Peng, Q. H.
;
Gao, Z. F.
  |  
收藏
  |  
浏览/下载:20/0
  |  
提交时间:2017/06/11
Neutron Star
Weak-magnetic Field Approximation
Generate And Relativistic Electrons
Electron Fermi Energy
The evaporation residue in the fission state of barium nuclei within relativistic mean-field theory
期刊论文
OAI收割
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 2015, 卷号: 42, 期号: 1, 页码: 15105
作者:
Bhuyan, M
;
Patra, SK
;
Gupta, RK
收藏
  |  
浏览/下载:21/0
  |  
提交时间:2016/11/21
relativistic mean field theory
binding energy
potential energy surface
nuclear fission state
On the possible mechanism of the first ground level enhancement in cosmic ray intensity of solar cycle 24
期刊论文
OAI收割
ASTROPHYSICS AND SPACE SCIENCE, 2014, 卷号: 350, 期号: 1, 页码: 21-32
作者:
Firoz, Kazi A.
;
Gan, W. Q.
;
Li, Y. P.
;
Rodriguez-Pacheco, J.
收藏
  |  
浏览/下载:25/0
  |  
提交时间:2014/11/20
Cosmic rays
Ground level enhancement
Solar flare
CME-driven shock
Solar radio burst
Solar flux density
Relativistic energy
Particle release time
Breaking the EOS-gravity degeneracy with masses and pulsating frequencies of neutron stars
期刊论文
OAI收割
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 2014, 卷号: 41, 期号: 7
Lin, WK
;
Li, BA
;
Chen, LW
;
Wen, DH
;
Xu, J
收藏
  |  
浏览/下载:29/0
  |  
提交时间:2015/03/13
RELATIVISTIC STELLAR MODELS
EQUATION-OF-STATE
NUCLEAR SYMMETRY ENERGY
NON-RADIAL PULSATION
HEAVY-ION REACTIONS
INVERSE-SQUARE LAW
NONRADIAL PULSATION
GRAVITATIONAL-WAVES
ANALYTIC ANALYSIS
DARK-MATTER