Titlebook: Black Hole Physics; Venzo Sabbata,Zhenjiu Zhang Book 1992 Kluwer Academic Publishers 1992 Cosmology.Gravity.Relativity.Universe.general re

palliative

書目名稱Black Hole Physics影響因子(影響力)




書目名稱Black Hole Physics影響因子(影響力)學(xué)科排名




書目名稱Black Hole Physics網(wǎng)絡(luò)公開度




書目名稱Black Hole Physics網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Black Hole Physics被引頻次




書目名稱Black Hole Physics被引頻次學(xué)科排名




書目名稱Black Hole Physics年度引用




書目名稱Black Hole Physics年度引用學(xué)科排名




書目名稱Black Hole Physics讀者反饋




書目名稱Black Hole Physics讀者反饋學(xué)科排名

北京人起源

Thermodynamics and Black Holes,with the question of thermodynamic stability of such systems when in contact with normal systems (§6). The non-extensivity of black hole entropy leads to further problems and two toy models are used to consider them. This leads to the consideration of superadditivity, concavity and homogeneity of th

充氣女

String Quantum Gravity and Black Holes, accelerated observers, Hawking radiation and its consequences, the Wheeler-De Witt equation and the “wave function of the universe”…) (ii) grand unification (the unification of all interactions including gravity from the particle physics point of view, in which, gravity is considered as a massless

泥瓦匠

constitutional

Marcello M. Veiga,John A. Meechreviewed. We conclude that it appears that the laws of black hole thermodynamics . the ordinary laws of thermodynamics applied to a system containing a black hole, and that A/4 represents the physical entropy of a black hole. Many puzzles remain, however. For example, ergodic behavior underlies the

有雜色

王得到

Evocative

1389-2185 r of broad areas related to different branches of physics. In fact have been widely treated not only classical aspects, thermodynamics, entropy, internal dynami978-94-010-5067-8978-94-011-2420-1Series ISSN 1389-2185

線

Marcello M. Veiga,John A. Meechly, deep) relationship between laws of black hole physics and the ordinary laws of thermodynamics. These lectures are devoted to a review of this relationship. We derive some fundamental properties of black holes in classical general relativity — in particular, the area theorem and the “first law” —

車床

Sara Hoover,Ryan Hill,Tom Watsonstellar systems and to arrive at minimum masses needed for black-hole formation under various conditions(§§2–3). Black hole parameters are introduced, including temperature and entropy, and the magnitude of these is elucidated (§4). It is shown that the work done in changing the mass and charge of a