Zhong-Wen Feng

Dr. Zhong-Wen Feng


Research Focus & Metrics

Academic Career Length

13Years (2014-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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16 April 2016 in The European Physical Journal C
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Journal Article
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ZFZhong-Wen Feng
Zhong-Wen Feng
HLH. L. Li
H. L. Li
XZXiaotao Zu
Xiaotao Zu
SYS. Z. Yang
S. Z. Yang
We investigate the thermodynamics of Schwarzschild–Tangherlini black hole in the context of the generalized uncertainty principle (GUP). The correcti

1 May 2017 in Physics Letters B
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Journal Article
Open access
ZFZhong-Wen Feng
Zhong-Wen Feng
SYShu-Zheng Yang
Shu-Zheng Yang
HLHui-Ling Li
Hui-Ling Li
XZXiao-Tao Zu
Xiao-Tao Zu
In this letter, we show that the dimensionless parameter in the generalized uncertainty principle (GUP) can be constrained by the gravitational wave event GW150914, which was discovered by the LIGO Scientific and Virgo Collaborations. Firstly, according to the Heisenberg uncertainty principle (HUP) and the data of gravitational wave event GW150914, we derive the standard energy-momentum dispersion relation and calculate the difference between the propagation speed of gravitons and the speed of light, i.e., $\Delta \upsilon$. Next, using two proposals regarding the GUP, we also generalize our study to the quantum gravity case and obtain the modified speed of gravitons. Finally, based on the modified speed of gravitons and $\Delta \upsilon$, the improved upper bounds on the GUP parameters are obtained. The results show that the upper limits of the GUP parameters $\beta_0$ and $\alpha_0$ are $2.3 \times 10^ {60}$ and $1.8 \times 10^{20}$.Comment: 8 pages, 2 Table

1 September 2017 in Physics Letters B
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Journal Article
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ZFZhong-Wen Feng
Zhong-Wen Feng
SYShu-Zheng Yang
Shu-Zheng Yang
In this letter, using the rainbow functions that were proposed by Magueijo and Smolin, we investigate the thermodynamics and the phase transition of rainbow Schwarzschild black hole. First, we calculate the rainbow gravity corrected Hawking temperature. From this modification, we then derive the local temperature, free energy, and other thermodynamic quantities in an isothermal cavity. Finally, we analyze the critical behavior, thermodynamic stability, and phase transition of the rainbow Schwarzschild black hole. The results show that the rainbow gravity can stop the Hawking radiation in the final stages of black holes' evolution and lead to the remnants of black holes. Furthermore, one can observe that the rainbow Schwarzschild black hole has one first-order phase transition, two second-order phase transitions, and three Hawking-Page-type phase transitions in the framework of rainbow gravity theory.Comment: 7 pages, 3 figures, accepted for publication in Physical Letter B. arXiv admin note: substantial text overlap with arXiv:1608.0682

27 May 2019 in The European Physical Journal C
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Journal Article
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ZFZhong-Wen Feng
Zhong-Wen Feng
QDQunchao Ding
Qunchao Ding
SYShuZheng Yang
ShuZheng Yang
The tunneling behavior of fermions with half-integral spin from a higher dimensional charged anti-de Sitter (AdS) black hole in de Rham, Gabadadze and Toll

15 September 2015 in Astrophysics and Space Science
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ZFZhong-Wen Feng
Zhong-Wen Feng
YCYang Chen
Yang Chen
XZXiaotao Zu
Xiaotao Zu

24 September 2018 in The European Physical Journal C
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HLHui-Ling Li
Hui-Ling Li
ZFZhong-Wen Feng
Zhong-Wen Feng
SYShuZheng Yang
ShuZheng Yang
XZXiaotao Zu
Xiaotao Zu
In this paper, taking into account a black hole solution of Finsler theory, we study the remnant and its phase transition close to the Planck scale. Based