scholarly journals Holographic complexity in charged Vaidya black hole

Author(s):  
Jie Jiang
Keyword(s):  
2018 ◽  
Vol 57 (7) ◽  
pp. 2145-2150 ◽  
Author(s):  
Hao Tang ◽  
Bin Wu ◽  
Cheng-yi Sun ◽  
Yu Song ◽  
Rui-hong Yue

2000 ◽  
Vol 62 (10) ◽  
Author(s):  
Li Xiang ◽  
Zhao Zheng
Keyword(s):  

2007 ◽  
Vol 312 (3-4) ◽  
pp. 315-319 ◽  
Author(s):  
Yongping Zhang ◽  
Wenbiao Liu

2006 ◽  
Vol 23 (5) ◽  
pp. 1099-1102 ◽  
Author(s):  
Zhang Jing-Yi ◽  
Zhao Zheng
Keyword(s):  

2010 ◽  
Vol 25 (01) ◽  
pp. 145-153 ◽  
Author(s):  
HARYANTO M. SIAHAAN ◽  
TRIYANTA

We derive the general form of Hawking temperature for Vaidya black hole in the tunneling pictures. This type of black hole is regarded as the description of a more realistic one compared to static case such as Schwarzschild's solution. The black hole mass in Vaidya solution is time dependent and decreasing due to evaporation process. Clearly, the temperature would be time dependent as our findings show. We use the semiclassical methods, namely radial null geodesic and complex paths methods. Both methods are found to give the same results. Then, we discuss the possible form of the corresponding entropy.


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