Zobrazeno 1 - 10
of 2 781
pro vyhledávání: '"Wang, Xiao‐Feng"'
Autor:
Dureppagari, Harish K., Saha, Chiranjib, Krishnamurthy, Harikumar, Wang, Xiao Feng, Rico-Alvariño, Alberto, Buehrer, R. Michael, Dhillon, Harpreet S.
The integration of non-terrestrial networks (NTN) into 5G new radio (NR) has opened up the possibility of developing a new positioning infrastructure using NR signals from Low-Earth Orbit (LEO) satellites. LEO-based cellular positioning offers severa
Externí odkaz:
http://arxiv.org/abs/2410.18301
Autor:
He, Wen-Jie, Zhang, Ren-You, Han, Liang, Jiang, Yi, Li, Zhe, Wang, Xiao-Feng, Li, Shu-Xiang, Li, Pan-Feng, Wang, Qing-hai
The planar two-loop scalar Feynman integrals contributing to the massive NNLO QCD corrections for $W$-boson pair production via quark-antiquark annihilation can be classified into three family branches, each of which is reduced to a distinct set of m
Externí odkaz:
http://arxiv.org/abs/2409.08879
Autor:
Chen, Ting-Wan, Yang, Sheng, Srivastav, Shubham, Moriya, Takashi J., Smartt, Stephen J., Rest, Sofia, Rest, Armin, Lin, Hsing Wen, Miao, Hao-Yu, Cheng, Yu-Chi, Aryan, Amar, Cheng, Chia-Yu, Fraser, Morgan, Huang, Li-Ching, Lee, Meng-Han, Lai, Cheng-Han, Liu, Yu Hsuan, K, Aiswarya Sankar., Smith, Ken W., Stevance, Heloise F., Wang, Ze-Ning, Anderson, Joseph P., Angus, Charlotte R., de Boer, Thomas, Chambers, Kenneth, Duan, Hao-Yuan, Erasmus, Nicolas, Gao, Hua, Herman, Joanna, Hou, Wei-Jie, Hsiao, Hsiang-Yao, Huber, Mark E., Lin, Chien-Cheng, Lin, Hung-Chin, Magnier, Eugene A., Man, Ka Kit, Moore, Thomas, Ngeow, Chow-Choong, Nicholl, Matt, Ou, Po-Sheng, Pignata, Giuliano, Shiau, Yu-Chien, Sommer, Julian Silvester, Tonry, John L., Wang, Xiao-Feng, Young, David R., Yeh, You-Ting, Zhang, Jujia
We present the discovery and early observations of the nearby Type II supernova (SN) 2024ggi in NGC 3621 at 6.64 +/- 0.3 Mpc. The SN was caught 5.8 (+1.9 -2.9) hours after its explosion by the ATLAS survey. Early-phase, high-cadence, and multi-band p
Externí odkaz:
http://arxiv.org/abs/2406.09270
Autor:
Li, Zhe, Zhang, Ren-You, Li, Shu-Xiang, Wang, Xiao-Feng, He, Wen-Jie, Han, Liang, Jiang, Yi, Wang, Qing-hai
The discrepancy between the CDF measurement and the Standard Model theoretical prediction for the $W$-boson mass underscores the importance of conducting high-precision studies on the $W$ boson, which is one of the predominant objectives of proposed
Externí odkaz:
http://arxiv.org/abs/2401.01323
Autor:
Li, Zhe, Zhang, Ren-You, Li, Shu-Xiang, Wang, Xiao-Feng, Li, Pan-Feng, Jiang, Yi, Han, Liang, Wang, Qing-hai
We present a comprehensive analytic calculation of the next-to-next-to-leading order $\text{QCD} \otimes \text{EW}$ corrections to $Z$-boson pair production at electron-positron colliders. The two-loop master integrals essential to this calculation a
Externí odkaz:
http://arxiv.org/abs/2312.17124
Although type Ia supernovae are so important in many astrophysical field, e.g. in cosmology, their explosion mechanism and progenitor system are still unclear. In physics, the relative equivalent width (REW) of the Si II 635.5 nm absorption feature r
Externí odkaz:
http://arxiv.org/abs/2212.12093
Autor:
Betoule, Marc, Antier, Sarah, Bertin, Emmanuel, Blanc, Pierre Éric, Bongard, Sébastien, Tanugi, Johann Cohen, Dagoret-Campagne, Sylvie, Feinstein, Fabrice, Hardin, Delphine, Juramy, Claire, Guillou, Laurent Le, Van Suu, Auguste Le, Moniez, Marc, Neveu, Jérémy, Nuss, Éric, Plez, Bertrand, Regnault, Nicolas, Sepulveda, Eduardo, Sommer, Kélian, Souverin, Thierry, Wang, Xiao Feng
Publikováno v:
A&A 670, A119 (2023)
The Hubble diagram of type-Ia supernovae (SNe-Ia) provides cosmological constraints on the nature of dark energy with an accuracy limited by the flux calibration of currently available spectrophotometric standards. The StarDICE experiment aims at est
Externí odkaz:
http://arxiv.org/abs/2211.04913
Autor:
Wang, Ling-Jun, Liu, Liang-Duan, Lin, Wei-Li, Wang, Xiao-Feng, Dai, Zi-Gao, Li, Bing, Song, Li-Ming
iPTF14hls is a luminous Type II supernova (SN) with a bumpy light curve that remains debated for its origin. It maintains roughly a constant effective temperature and luminosity since discovery for about 600 days, followed by a slow decay. On $\sim 1
Externí odkaz:
http://arxiv.org/abs/2206.00178
Autor:
Bai, Hui, Wang, Xiao-Feng, Xu, Yi-Han, Zaorsky, Nicholas G, Wang, Huan-Huan, Niu, Geng-Min, Li, Jia-Cheng, Dong, Yang, Li, Jun-Yi, Yu, Lu, Chen, Mei-Feng, Lu, Xiao-Tong, Yuan, Zhi-Yong, Yang, Ji-Long, Meng, Mao-Bin
Publikováno v:
In Radiotherapy and Oncology November 2024 200
Publikováno v:
In Journal of Molecular Structure 5 February 2025 1321 Part 4