김성구
양종만
김성원
2017-08-29T02:34:55Z
2017-08-29T02:34:55Z
1990
0369-3554
OAK-13121
http://dspace.ewha.ac.kr/handle/2015.oak/229155
The attempt of nonstationary black-hole thermodynamics is made for the case of radiation mode of Vaidya metric. Calculating the modified temperature from the wave equation, entropy is defined by the apparent horizon, as the local quantity whose state is a proper fiducial equilibrium state. In those thermodynamic quantities we try to see what the mass-varying effects play the role of. So it is a kind of quasi-equilibrium thermodynamic theory on the two points of view for mass-varying processes, rather than a complete nonequilibrium thermodynamics. © 1990 Società Italiana di Fisica.
English
Società Italiana di Fisica
Black-hole thermodynamics for the nonstationary case
Article
8-9
105
SCOPUS
857
865
Il Nuovo Cimento B Series 11
10.1007/BF02741553
2-s2.0-51649153936
Klm S.-W.
Kim S.K.
Yang J.
김성구(22967145800;18836103200)
양종만(15039320200)
김성원(55862533800)
20180104081001