共查询到20条相似文献,搜索用时 15 毫秒
1.
In the paper [R.-G. Cai, L.-M. Cao, Y.-P. Hu, arXiv: 0809.1554], the scalar particles' Hawking radiation from the apparent horizon of Friedmann–Robertson–Walker (FRW) universe was investigated by using the tunneling formalism. They obtained the Hawking temperature associated with the apparent horizon, which was extensively applied in investigating the relationship between the first law of thermodynamics and Friedmann equations. In this Letter, we calculate fermions' Hawking radiation from the apparent horizon of FRW universe via tunneling formalism. Applying WKB approximation to the general covariant Dirac equation in FRW spacetime background, the radiation spectrum and Hawking temperature of apparent horizon are correctly recovered, which supports the arguments presented in the paper [R.-G. Cai, L.-M. Cao, Y.-P. Hu, arXiv: 0809.1554]. 相似文献
2.
We investigate the validity of the generalized second law of gravitational thermodynamics on the dynamical apparent horizon
in a non-flat FRW universe containing the interacting new agegraphic dark energy with dark matter. We show that for this model,
the equation of state parameter can cross the phantom divide line. We also present that for the selected model under thermal
equilibrium with the Hawking radiation, the generalized second law is always satisfied throughout the history of the universe.
Whereas, the evolution of the entropy of the universe and dynamical apparent horizon, separately, depends on the equation
of state parameter of the interacting new agegraphic dark energy model. 相似文献
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4.
Ke-Xia Jiang Tsun Feng Dan-Tao Peng 《International Journal of Theoretical Physics》2009,48(7):2112-2121
An analysis of Hawking radiation about apparent horizon in a FRW universe is performed by using the method developed in the
paper (Banerjee, Majhi in JHEP 06:095 2008), in which the Hawking radiation of a black hole is treated as the quantum tunneling
by Hamilton-Jacobi method beyond semiclassical approximation and then all the higher order quantum corrections can be given
out. In our analysis, the Kodama vector instead of the Killing vector to define the energy of the particle plays a key role.
We present our analysis under the Friedmann-Robertson-Walker like coordinate system and the much-like to Painlevé coordinate
system respectively. The result show that the formulized procedure can be extended to fully analyse the Hawking radiation
of a dynamical system. 相似文献
5.
Recently, Banerjee and Kulkarni (R. Banerjee, S. Kulkarni, arXiv: 0707. 2449 [hep-th]) suggested that it is conceptually clean
and economical to use only the covariant anomaly to derive Hawking radiation from a black hole. Based upon this simplified
formalism, we apply the covariant anomaly cancellation method to investigate Hawking radiation from a modified Schwarzschild
black hole in the theory of rainbow gravity. Hawking temperature of the gravity’s rainbow black hole is derived from the energy-momentum
flux by requiring it to cancel the covariant gravitational anomaly at the horizon. We stress that this temperature is exactly
the same as that calculated by the method of cancelling the consistent anomaly. 相似文献
6.
Using the gravitational anomaly method proposed by Robinson and Wilczek, Hawking radiation from the apparent horizon of a
Vaidya black hole is calculated. The thermodynamics can be built successfully on the apparent horizon. In the meantime, when
a time-dependent perturbation is given to the apparent horizon, the first law of thermodynamics can also be constructed successfully
at a new supersurface near the apparent horizon. The expressions of the characteristic position and temperature are consistent
with the previous result where the viewpoint is that the thermodynamics should be built on the event horizon. Based on the
results, the thermodynamics should be constructed on the apparent horizon exactly while the event horizon thermodynamics is
just one of the perturbations near the apparent horizon. 相似文献
7.
We investigate the corrected entropy and Hawking temperature of the BTZ black hole which obtained from (2 + 1) dimensional black hole. Besides, we generalize our analysis of black holes to the case of Friedmann-Robertson-Walker (FRW) universe. The corrections to the Hawking temperature and entropy of apparent horizon for FRW universe are also obtained. Comparing the results with the high energy black hole demonstrates how the semi-classic approximation affects the thermodynamics of the BTZ black hole, corrected terms, classical action and the entropy. 相似文献
8.
In this paper, Hawking radiation from the Kerr Newman de Sitter black hole is studied via gauge anomaly and gravitational anomaly. The obtained results of Hawking radiation from the event horizon and the cosmological horizon accord with those by other methods. 相似文献
9.
Robinson–Wilczek's recent work shows that, the energy–momentum tensor flux required to cancel gravitational anomaly at the event horizon of a Schwarzschild-type black hole has an equivalent form to that of a (1+1)-dimensional blackbody radiation at the Hawking temperature. Motivated by their work, Hawking radiation from the cosmological horizons of the general Schwarzschild–de Sitter and Kerr–de Sitter black holes, has been studied by the method of anomaly cancellation. The result shows that the absorbing gauge current and energy momentum tensor fluxes required to cancel gauge and gravitational anomalies at the cosmological horizon are precisely equal to those of Hawking radiation from it. It should be emphasized that the effective field theory for generic black holes in de Sitter spaces should be formulated within the region between the event horizon (EH) and the cosmological horizon (CH), to integrate out the classically irrelevant ingoing modes at the EH and the classically irrelevant outgoing modes at the CH, respectively. 相似文献
10.
Hawking radiation from the with a global monopole via Schwarzschild black hole gravitational anomaly 下载免费PDF全文
This paper derives the Hawking flux from the Schwarzschild black hole with a global monopole by using Robinson and Wilczek's method. Adopting a dimensional reduction technique, it can describe the effective quantum field in the (3 + 1)-dimensional global monopole background by an infinite collection of the (1 + 1)-dimensional massless fields if neglecting the ingoing modes near the horizon, where the gravitational anomaly can be cancelled by the (1 + 1)- dimensional black body radiation at the Hawking temperature. 相似文献
11.
Based on the anomaly cancellation method, initiated by Robinson and Wilczek, we investigate Hawking radiation from the event horizon and cosmological horizon of the higher dimensional Reissner–Nordström–de Sitter black hole via covariant gauge and gravitational anomalies. Unlike in black hole space-time, to describe the observable physics, the effective field theory here is constructed between the event horizon and cosmological horizon. Our result shows that to restore the underlying gauge covariance and diffeomorphism covariance at the quantum level, the covariant compensating fluxes of gauge and energy–momentum tensor, which are shown to equal to those of Hawking radiation, should be radiated from the event horizon and absorbed from the cosmological horizon, respectively. 相似文献
12.
Li-Chun Zhang Huai-Fan Li Yue-Qin Wu Ren Zhao 《International Journal of Theoretical Physics》2010,49(7):1587-1594
Taking the reaction of the radiation to the spacetime into consideration, we discuss Hawking radiation spectrum and Bekenstein-Hawking
entropy correction in Friedmann-Robertson-Walker (FRW) universe by the analytical continuation method. We derive the radiation
spectrum that satisfies the unitary principle and the logarithmic correction term of entropy in FRW universe. 相似文献
13.
M.R. Setare 《The European Physical Journal C - Particles and Fields》2007,49(3):865-868
In this paper we obtain the flux of Hawking radiation from rotating BTZ black holes from the gauge and gravitational anomalies
point of view. Then we show that the gauge and gravitational anomaly in BTZ spacetime is cancelled by the total flux of a
2-dimensional blackbody at the Hawking temperature of the spacetime. 相似文献
14.
Ritabrata Biswas Nairwita Mazumder Subenoy Chakraborty 《International Journal of Theoretical Physics》2012,51(1):101-109
The paper deals with anisotropic spherically symmetric Lemaitre-Tolman-Bondi model of the universe bounded by the apparent
horizon. Using Hamilton-Jacobi method for both massive and massless test particles, we are able to show that the temperature
associated with the apparent horizon due to Hawking radiation is the usual Hawking Temperature. Also the usual Lemaitre-Tolman-Bondi
model and the transformed r-gauge Lemaitre-Tolman-Bondi model are shown to be equivalent. Finally, the results of Tunneling
approach agree with the Hamiltonian-Jacobi method. 相似文献
15.
Xian-Ming Liu Su-Jun Cheng Wen-Biao Liu 《International Journal of Theoretical Physics》2012,51(2):518-525
Under the extended dynamical tortoise coordinate transformation, Damour-Ruffini method has been applied to calculate the charged
particles’ Hawking radiation from the apparent horizon of a dynamical Kerr-Newman black hole. It is shown that Hawking radiation
is still purely thermal black body spectrum. Moreover, the temperature of Hawking radiation is corresponding to the apparent
horizon surface gravity and the first law of thermodynamics can also be constructed successfully on the apparent horizon in
the dynamical Kerr-Newman black hole. 相似文献
16.
Hawking tunneling radiation of spin ? 1/2 particles from the event horizon of the Reissner–Nordström black hole is studied. We introduce the Dirac equation of the charged particles. We further consider the gravitational interaction and back reaction of the emitted spin particles in the dynamical background space–time. The result shows that when the energy conservation and charge conservation are taken into account, the actual radiation spectrum of fermions also derivates from the thermal one and the tunneling rate is related to the change of Bekenstein–Hawking entropy. 相似文献
17.
Hawking radiation from the cylindrical symmetric black hole, which is asymptotically anti-de Sitter not only in the transverse
direction but also in the string or membrane direction, is discussed from the anomaly point of view. We implement the covariant
anomaly cancellation method, the more refined formalism that was proposed by Banerjee and Kulkarni recently than the initial
work of Robinson et al., to discuss the near-horizon gauge and gravitational anomalies. Our result shows that Hawking radiation
from the cylindrical configurations with horizons also can be reproduced by the anomaly cancellation method. 相似文献
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19.
In this paper, we mainly investigate the anomalous effective action of the rotating Taub-NUT black hole and show that the
flux of Hawking radiation can be determined by anomaly cancellation conditions and regularity requirement at the event horizon.
With the method of a dimensional reduction technique, that is, the (1+1) dimensional quantum anomalies equation, we successfully
obtain the simplified metric near the horizon. In addition, the covariant energy-momentum tensor that is related with Hawking
temperature are calculated in this black hole. 相似文献
20.
Xiao-Xiong Zeng Kai Lin Shu-Zheng Yang 《International Journal of Theoretical Physics》2008,47(10):2533-2542
Very recently, a conceptually clean and economical anomaly cancellation method, based on the initial work of Robinson and
Wilczek, on Hawking radiation was proposed. On the basis of this formalism, we investigate Hawking radiation from the higher
dimensional Schwarzschild de Sitter and Anti-de Sitter black holes. To describe the observable physics in de Sitter space,
we construct the effective field theory between the event horizon and cosmological horizon. Our result shows that when the
underlying diffeomorphism symmetries are saved at the quantum level, Hawking radiation, from not only the event horizon but
also the cosmological horizon in the higher dimensional space time, can be determined by the covariant compensating fluxes
of energy momentum tensor. Meanwhile, we also discuss the exact radiation spectrum by incorporating the self-gravitational
interaction and back reaction of the outgoing modes. 相似文献