Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Xue-Ling Mu"'
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 81, Iss 8, Pp 1-7 (2021)
Abstract The Jeans instability is regarded as an important tool for analyzing the dynamics of a self-gravitating system. However, this theory is challenging since astronomical observation data show some Bok globules, whose masses are less than the Je
Externí odkaz:
https://doaj.org/article/da7739dee9e740e5837278dd59b20f98
Publikováno v:
In Chinese Astronomy and Astrophysics July-September 2016 40(3):340-351
Publikováno v:
Chinese Physics C. 46:065104
In this study, we determine the influence of the nucleon-nucleon short range correlation (SRC) on static spherically symmetric neutron stars (NSs) from the perspectives of radial and nonradial oscillations for the first time. We revise the equation o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ce0a942e51d9409d78f324b3f4551c88
https://doi.org/10.1088/1674-1137/ac588d
https://doi.org/10.1088/1674-1137/ac588d
Autor:
Bin Hong, Xue-Ling Mu
Publikováno v:
Communications in Theoretical Physics. 74:065301
The implications of relativistic parameter sets established at saturation density on the tidal deformabilities and f-mode oscillations of neutron stars (NSs) are examined using constraints from the gravitational wave (GW) event GW170817 and NICER. Ac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0a8ed0aaf201514cc6a0fd1dfc2ea7c2
https://doi.org/10.1088/1572-9494/ac6803
https://doi.org/10.1088/1572-9494/ac6803
Publikováno v:
Communications in Theoretical Physics. 66:224-230
Adjusting the suitable coupling constants in relativistic mean Geld (RMF) theory and focusing on thermal effect of an entropy per baryon (S) from 0 to 3, we investigate the composition and structure of massive protoneutron stars corresponding PSR J16
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::84c1cb72218ff8384e8043a7a1b3ae46
https://doi.org/10.1088/0253-6102/66/2/224
https://doi.org/10.1088/0253-6102/66/2/224
Publikováno v:
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017).
Cosmic ray particles can be accelerated in the supernova. A protoneutron star is formed in a few seconds after the supernova explosion of a massive star. Neutron stars may be one of cosmic ray sources. Therefore, the study of structure of protoneutro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4dabfb024ea97edadf4149c52a9fa04b
https://doi.org/10.22323/1.301.0275
https://doi.org/10.22323/1.301.0275
Publikováno v:
2009 International Conference on Machine Learning and Cybernetics.
The authors establish the polynomial distribution lag model of GIC about the geomagnetic level change rate based on the geomagnetic data and GIC measuring data on the power systems. By testing, the model is reliable and the prediction result is more
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b17b620905af9f42239c9dd620525fe7
https://doi.org/10.1109/icmlc.2009.5212224
https://doi.org/10.1109/icmlc.2009.5212224
Publikováno v:
2008 International Workshop on Modelling, Simulation and Optimization.
Magnetic Storms are the earthpsilas magnetic field changes caused by solar activities, and can produce geomagnetically induced currents (GIC) in power systems, pipelines and other technological conductor systems on the ground. GIC have a great influe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::148b52924b626280f65b2255c5fd0a4b
https://doi.org/10.1109/wmso.2008.106
https://doi.org/10.1109/wmso.2008.106
Publikováno v:
2009 International Conference on Machine Learning & Cybernetics; 2009, p2091-2095, 5p
Publikováno v:
2008 International Workshop on Modelling, Simulation & Optimization; 2008, p3-6, 4p