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pro vyhledávání: '"Fan Xi"'
Autor:
Peng Caini, Peng Junyuan, Lyu Zhuoran, Dai Liguo, Wang Jingru, Zhang Jiayi, Liu Yinya, Fan Xi
Publikováno v:
Sichuan jingshen weisheng, Vol 37, Iss 2, Pp 150-155 (2024)
BackgroundPrevention and intervention of procrastination in college students are of great practical significance， and studies have illustrated a pairwise correlation among mindfulness， self-control， insecure attachment and procrastination， wh
Externí odkaz:
https://doaj.org/article/227189dde91e4305962ba636a48dcf59
Autor:
Wang, Ao-Bo, Pan, Chu-Cheng, Dong, Xiang, Sun, Yu-Chang, Hu, Yu-Xuan, Cheng, Ao-Yan, Cai, Hao, Fan, Xi-Long
Cosmic muon imaging technology is increasingly being applied in various fields. However, simulating cosmic muons typically requires the rapid generation of a large number of muons and tracking their complex trajectories through intricate structures.
Externí odkaz:
http://arxiv.org/abs/2410.06539
Autor:
Tang, Li, Fan, Xi-Long
The spin characteristics of black holes offer valuable insights into the evolutionary pathways of their progenitor stars, crucial for understanding the broader population properties of black holes. Traditional Hierarchical Bayesian inference techniqu
Externí odkaz:
http://arxiv.org/abs/2407.06781
Binary stars are as frequency as single stars in the Universe, and at least 70\% of the massive stars located in our Galaxy belong to a binary system. For the first time we produce the gravitational waveforms for the extreme mass ratio inspiral syste
Externí odkaz:
http://arxiv.org/abs/2405.07113
Publikováno v:
Phys Rev D 109, 084011 (2024)
General relativity predicts the existence of only two tensorial gravitational wave polarizations, while a generic metric theories of gravity can possess up to four additional polarizations, including two vector and two scalar ones. These vector/scala
Externí odkaz:
http://arxiv.org/abs/2401.03474
Publikováno v:
Phys. Rev. D 107, 123029, 2023
Resolving individual gravitational waves from tens of millions of double white dwarf (DWD) binaries in the Milky Way is a challenge for future space-based gravitational wave detection programs. By using previous data to define the priors for the next
Externí odkaz:
http://arxiv.org/abs/2309.06037
The gravitational waves (GW) from core-collapse supernovae (CCSN) have been proposed as a probe to investigate physical properties inside of the supernova. However, how to search and extract the GW signals from core-collapse supernovae remains an ope
Externí odkaz:
http://arxiv.org/abs/2309.06011
The Johannsen black hole (BH) is a generic rotating BH admitting three constants of motions (energy, angular momentum, and Carter constant) and is characterized by four deviation parameters besides mass and spin, which could be a model-independent pr
Externí odkaz:
http://arxiv.org/abs/2307.08953
The nature of the merger remnant of binary neutron star (BNS) remains an open question. From the theoretical point of view, one possible outcome is a supra-massive neutron star (SMNS), which is supported by rigid rotation and through its survival of
Externí odkaz:
http://arxiv.org/abs/2305.01364
Publikováno v:
MNRAS, 527, 3, 2024, 5616-5626
An enormous number of compact binary systems, spanning from stellar to supermassive levels, emit substantial gravitational waves during their final evolutionary stages, thereby creating a stochastic gravitational wave background (SGWB). We calculate
Externí odkaz:
http://arxiv.org/abs/2304.08333