Zobrazeno 1 - 10
of 5 622
pro vyhledávání: '"Shao, Yong"'
Autor:
Shi, Yi, Tian, Xu-Peng, Wang, Yun-Kai, Zhang, Tie-Yi, Yao, Bin, Wang, Hui, Shao, Yong, Wang, Cen-Cen, Zeng, Rong, Zhan, De-Chuan
Automated sperm morphology analysis plays a crucial role in the assessment of male fertility, yet its efficacy is often compromised by the challenges in accurately segmenting sperm images. Existing segmentation techniques, including the Segment Anyth
Externí odkaz:
http://arxiv.org/abs/2407.03772
Galactic double white dwarfs are predominant sources of gravitational waves in the millihertz frequencies accessible to space-borne gravitational wave detectors. With advances in multi-messenger astronomy, an increasing number of double white dwarf s
Externí odkaz:
http://arxiv.org/abs/2406.16474
The spins of binary black holes (BBHs) measured from gravitational waves carry notable information of the formation pathways. Here we propose a quantity "dimensionless net spin" ($\chi_{\rm N}$), which is related to the sum of angular momentum of com
Externí odkaz:
http://arxiv.org/abs/2406.03257
Neutron star$-$white dwarf (NSWD) binaries are one of the most abundant sources of gravitational waves (GW) in the Milky Way. These GW sources are the evolutionary products of primordial binaries that experienced many processes of binary interaction.
Externí odkaz:
http://arxiv.org/abs/2403.04983
The detection of gravitational wave events has stimulated theoretical modeling of the formation and evolution of double compact objects (DCOs). However, even for the most studied isolated binary evolution channel, there exist large uncertainties in t
Externí odkaz:
http://arxiv.org/abs/2402.04658
It is widely accepted that quite a number of double compact objects (DCOs) in the Milky Way can be identified by future space-based gravitational wave (GW) detectors, while systematic investigations on the detection of the GW sources in nearby galaxi
Externí odkaz:
http://arxiv.org/abs/2307.07955
We evaluate the prospects for radio follow-up of the double neutron stars (DNSs) in the Galactic disk that could be detected through future space-borne gravitational wave (GW) detectors. We first simulate the DNS population in the Galactic disk that
Externí odkaz:
http://arxiv.org/abs/2305.05202
Autor:
Hu, Rui-Chong, Zhu, Jin-Ping, Qin, Ying, Shao, Yong, Zhang, Bing, Yu, Yun-Wei, Liang, En-Wei, Liu, Liang-Duan, Wang, Bo, Shu, Xin-Wen, Liu, Jian-Feng
Extreme stripped-envelope supernovae (SESNe), including Type Ic superluminous supernovae (SLSNe), broad-line Type Ic SNe (SNe Ic-BL), and fast blue optical transients (FBOTs), are widely believed to harbor a newborn fast-spinning highly-magnetized ne
Externí odkaz:
http://arxiv.org/abs/2301.06402
Autor:
Zheng, Ling-Lin, Sun, Mouyuan, Gu, Wei-Min, Yi, Tuan, Zhang, Zhi-Xiang, Wang, Pei, Wang, Junfeng, Wu, Jianfeng, Wang, Song, Zhang, Jia, Li, Chun-Qian, Shi, Jian-Rong, Shao, Yong, Li, Xiang-Dong, Fu, Jin-Bo, Yang, Fan, Bai, Zhongrui, Bai, Yu, Zhang, Haotong, Liu, Jifeng
Recent studies have revealed the global deposition on Earth of radioactive elements (e.g., $^{60}$Fe) resulting from the metal-enriched ejecta of nearby (within $\sim 100$ pc) supernova explosions. The majority of neutron stars in our Solar neighborh
Externí odkaz:
http://arxiv.org/abs/2210.04685
Autor:
Shao, Yong
Mass distribution of black holes in low-mass X-ray binaries previously suggested the existence of a $ \sim 2-5M_{\odot} $ mass gap between the most massive neutron stars and the least massive black holes, while some recent evidence appears to support
Externí odkaz:
http://arxiv.org/abs/2210.00425