对五维Myers-Perry黑洞隧穿辐射的研究
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摘要
霍金辐射是黑洞物理学最重要的成就之一。自从霍金在理论上证明了黑洞具有热辐射以来,霍金辐射就受到国内外学者们的广泛关注。隧穿辐射的研究方法有很多,最近Anghben-Nadalini-Vanzo-Zerbini(ANVZ)提出协变量的方法来研究霍金辐射,值得强调的是该方法给出了协变量的结果。采用ANVZ协变量的方法研究了一个非零角动量的高维轴对称的Myers-Perry黑洞的隧穿辐射,目的是将ANVZ协变量的方法推广到高维情形,最终得出了Myers-Perry黑洞的隧穿率及霍金温度,其结论与其他方法得到的结果一致。
The Hawking radiation is one of the most important achievements in black hole physics.Since Hawking proved the thermal radiation of black holes in theory,Hawking radiation is widely concerned by scholars.There are many ways to study the Hawking radiation,and AnghbenNadalini-Vanzo-Zerbini(ANVZ)proposed covariance method to study Hawking radiation recently.It is important to emphasize that the method give the covariance of results.Based on the ANVZ covariance method,we investigate the Hawking radiation from the high-dimensional axisymmetric Myers-Perry black hole with a single non-zero angular momentum.Our aim is to extend the ANVZ covariance method to study high-dimensional tunneling radiation of black holes.Eventually,we get the tunneling rate and Hawking temperature of the Myers-Perry black hole,which is accord well with the results by other methods.
The Hawking radiation is one of the most important achievements in black hole physics.Since Hawking proved the thermal radiation of black holes in theory,Hawking radiation is widely concerned by scholars.There are many ways to study the Hawking radiation,and AnghbenNadalini-Vanzo-Zerbini(ANVZ)proposed covariance method to study Hawking radiation recently.It is important to emphasize that the method give the covariance of results.Based on the ANVZ covariance method,we investigate the Hawking radiation from the high-dimensional axisymmetric Myers-Perry black hole with a single non-zero angular momentum.Our aim is to extend the ANVZ covariance method to study high-dimensional tunneling radiation of black holes.Eventually,we get the tunneling rate and Hawking temperature of the Myers-Perry black hole,which is accord well with the results by other methods.
引文
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[6]SALEH M,THOMAS B B,KOFANE T C.Hawking radiation from a five dimension-al Lovelock black hole[J].Front Phys,2015,10(5):100401-100405.
[7]LI H L,HUANG T,GAO P.Fermion tunneling from the 5dimensional Kerr-Gdel black hole[J].EPL,2009,86(6):60001-60004.
[8]YANG S Z,CHEN D Y.A new method to study Hawking radiation of charged partical from stationary axisymmetric sen black hole[J].Chin Phys Lett,2007,24(1):39-41.
[9]NADALINI M,VANZO L,ZERBIN S.Hawking radiation as tunneling:the D-dimensional rotating case[J].Jourmal of Physics A:Mathematical and Theoretical,2006,39(21):6601-6608.
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[11]LI H L,LIN R,ZHOU T J.Hawking radiation as tunneling with back-reaction for the kerr anti de sitter black hole[J].Theoretical and Mathematical Physics,2009,161(1):1438-1444.
[2]HAWKING S W.Hawking S Breakdown of predictability in gravitational collapse[J].Phys Rev D,1976,14(10):2460-2473.
[3]VANZO L.Radiation of extreme black holes[J].Phys Rev D,1997,55(4):2192-2201.
[4]DAMOUR T,RUFFINI R.Black hole evaporation in the Klein Sauter Heisenberg ulerformalism[J].Phys Rev D,1976,14(2):332-334.
[5]PARIKH M K,WILCZEK F.Hawking radiation as tunneling[J].Phys Rev Lett,2008,85(24):5042-5045.
[6]SALEH M,THOMAS B B,KOFANE T C.Hawking radiation from a five dimension-al Lovelock black hole[J].Front Phys,2015,10(5):100401-100405.
[7]LI H L,HUANG T,GAO P.Fermion tunneling from the 5dimensional Kerr-Gdel black hole[J].EPL,2009,86(6):60001-60004.
[8]YANG S Z,CHEN D Y.A new method to study Hawking radiation of charged partical from stationary axisymmetric sen black hole[J].Chin Phys Lett,2007,24(1):39-41.
[9]NADALINI M,VANZO L,ZERBIN S.Hawking radiation as tunneling:the D-dimensional rotating case[J].Jourmal of Physics A:Mathematical and Theoretical,2006,39(21):6601-6608.
[10]MYERS R C,PERRY M J.Black hole in higher dimensional space-times[J].Annals of Physics,1986,172(2):304-347.
[11]LI H L,LIN R,ZHOU T J.Hawking radiation as tunneling with back-reaction for the kerr anti de sitter black hole[J].Theoretical and Mathematical Physics,2009,161(1):1438-1444.