CAJ | 학술논문

Parikh-Wilzcek把四维Schwarzshild和Reissner—Nordstrom黑洞的Hawking辐射认为是半经典隧穿行为的结果，在考虑到粒子间自引力的作用下，所得的辐射谱不再是纯热谱．本文运用此方法研究了高维Reissner—Nordstrom黑洞的隧穿辐射，得到了修正的辐射谱，它与黑洞的Bekenstein—Hawking熵变有关，不再是纯热谱，并指出Pafikh-Wilzcek的工作只局限于可逆过程．
Parikh-Wilzcek파사유Schwarzshild화Reissner—Nordstrom흑동적Hawking복사인위시반경전수천행위적결과，재고필도입자간자인력적작용하，소득적복사보불재시순열보．본문운용차방법연구료고유Reissner—Nordstrom흑동적수천복사，득도료수정적복사보，타여흑동적Bekenstein—Hawking적변유관，불재시순열보，병지출Pafikh-Wilzcek적공작지국한우가역과정．
Parikh-Wilzeek's recent work, which treats the Hawking radiation as semi-classical tunneling process from the event horizon of four dimensional Schwarzshild and Reissner-ordstrom black hole, indicates that the derived radiant spectrum is no longer precisely thermal after taking the self-gravitation action into account. This paper applies the method to studying the tunneling radiation of arbitrary dimensional Reissner-Nordstrom black holes, and finds that the modified spectrum is related to the change of Bekenstein-Hawking entropy, and is no longer the pure thermal one. Finally, it points out that the Parikh-Wilzcek's tunneling framework is only limited to the reversible process.