kerr black hole 中文意思是什麼
kerr black hole
解釋
克而黑洞-
Particle energy levels in the spacetime of a non - kerr black hole
一個非克爾黑洞時空中的粒子能級 -
After that, both the equilibrium and the non - equilibrium fluctuations of thermodynamical quantities in schwarzschild black hole, reissner - nordstrom black hole, charged dilaton black hole, and kerr - newman black hole are calculated
在第三章中，我們嚴格地計算了schwarzschild黑洞、 reissner - nordstrm黑洞、靜態帶電伸縮子黑洞（ cdbh ）和kerr - newman黑洞等穩態黑洞的平衡漲落和非平衡漲落。 -
We find ( 1 ) the second order phase transitions do n ' t occur in schwarzschild black hole and in charged dilaton black hole when a = 1 ; ( 2 ) the second order phase transitions take place at the points where the heat capacities are diverged in the reissner - nordstrom black hole, charged dilaton black hole when a 1, and kerr - newman black hole
結果表明： （ 1 ） schwarzschild黑洞和= 1時的靜態帶電伸縮子黑洞（ cdbh ）沒有二級相變發生。 （ 2 ） reissner - nordstrm黑洞、 1時的靜態帶電伸縮子黑洞和kerr - newman黑洞等穩態黑洞，在熱容量發散的地方發生了二級相變。 -
Quantum area spectrum of kerr black hole and the smallest mass of micro - black hole
黑洞的量子面積譜及微黑洞的最小質量 -
The brown - york quasilocal energies of some black holes in string theory are calculated and martinez ' s conjecture, originally proposed for the kerr black hole in general relativity, is explored in string theory
本文用brown - york準定域能定義對弦理論中的一些黑洞的能量進行了計算，並探討了源於廣義相對論中kerr黑洞的martinez猜測在弦理論中的適用性。 -
Metric of the second order infinitesimal neighborhood nearby the horizon pole of a kerr - newman black hole
黑洞視界極點處二級無限小鄰域的度規 -
In particular, we find that martinez ' s conjecture is also applicable to the kerr - sen black hole. this is different from bose - naing ' s result that the quasilocal energy of the kerr - sen black hole does not yield martinez ' s conjecture
特別是，我們還發現martinez猜測對kerr - sen時空也成立，這不同於bose - naing最近得出的martinez猜測對kerr - sen時空不成立的結論。
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