scholarly journals Nonlinear Hamiltonian analysis of new quadratic torsion theories: Cases with curvature-free constraints

2021 ◽  
Vol 104 (8) ◽  
Author(s):  
W. E. V. Barker ◽  
A. N. Lasenby ◽  
M. P. Hobson ◽  
W. J. Handley
PCI Journal ◽  
1985 ◽  
Vol 30 (5) ◽  
pp. 96-127 ◽  
Author(s):  
Arthur E. McMullen ◽  
Wael M. EI-Degwy

1994 ◽  
Vol 49 (2) ◽  
pp. 1603-1609 ◽  
Author(s):  
D. Farina ◽  
F. Casagrande ◽  
U. Colombo ◽  
R. Pozzoli

2013 ◽  
Vol 41 (9) ◽  
pp. 3224-3240
Author(s):  
Mohsen Asgharzadeh ◽  
Massoud Tousi
Keyword(s):  

2011 ◽  
Vol 2011 (1) ◽  
Author(s):  
M. Blagojević ◽  
B. Cvetković

2011 ◽  
Vol 696 (4) ◽  
pp. 426-431 ◽  
Author(s):  
Seoktae Koh ◽  
Sunyoung Shin
Keyword(s):  

2015 ◽  
Vol 219 (8) ◽  
pp. 3629-3676 ◽  
Author(s):  
Tomas Everaert ◽  
Marino Gran
Keyword(s):  

2018 ◽  
Vol 33 (27) ◽  
pp. 1850159 ◽  
Author(s):  
Shad Ali ◽  
Xin-Yang Wang ◽  
Wen-Biao Liu

Christodoulou and Rovelli have shown that the interior volume of a Schwarzschild black hole grows linearly with time. The entropy of a scalar field in this interior volume of a Schwarzschild black hole has been calculated and shown to increase linearly with the advanced time too. In this paper, considering Hawking radiation from a d-dimensional charged black hole, we investigate the proportional relation between the entropy of the scalar field in the interior volume and the Bekenstein–Hawking entropy using the method of our previous work. We also derive this proportionality relation using Hamiltonian analysis and find a consistent result. We then investigate the proportionality coefficient with respect to d and find that it gradually decreases as the dimension of space–time increases.


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