Erratum: Hawking radiation from dilatonic black holes via anomalies [Phys. Rev. D75, 064029 (2007)]

Abstract

Recently, Hawking radiation from a Schwarzschild-type black hole via gravitational anomaly at the horizon has been derived by Robinson and Wilczek. Their result shows that, in order to demand general coordinate covariance at the quantum level to hold in the effective theory, the flux of the energy momentum tensor required to cancel gravitational anomaly at the horizon of the black hole, is exactly equal to that of (1 + 1)-dimensional blackbody radiation at the Hawking temperature. In this paper, we attempt to apply the analysis to derive Hawking radiation from the event horizons of static, spherically symmetric dilatonic black holes with arbitrarily coupling constant α, and that from the rotating Kaluza-Klein (α = √ 3) as well as the Kerr-Sen (α = 1) black holes via an anomalous point of view. Our results support Robinson-Wilczek's opinion. In addition, the properties of the obtained physical quantities near the extreme limit are qualitatively discussed.

Mixing ofDs1(2460)andDs1(2536<

“…Similar mechanism has been studied in the a 0 (980)-f 0 (980) mixing in Ref. [10]. Determination of the mixing angle should be useful for understanding the property and internal structure of these two axial vector states.…”

“…(10). We adopt the following bare cs masses, m[ 22] GeV , it shows that the higher pole is stable and the lower one changes from 2.47 GeV to 2.44 GeV.…”

“…Intermediate states If all the particles involved are scalars or pseudoscalars, Fig. 1 will only represent sums of infinite geometric series and the resulting propagator matrix G becomes [10] …”

A Note on the Equivalence of Post-Newtonian Lagrangian and Hamiltonian Formulations

“…This result is useful to clarify the doubt on the absence of chaos in the 2PN ADM Hamiltonian approach [5,6] and the presence of chaos in the 2PN harmonic coordinate Lagrangian formulation [4]. As a point to illustrate, two other doubts about different chaotic indicators resulting in different dynamical behaviours of spinning compact binaries among references [12][13][14][15] and different descriptions of chaotic parameter spaces and chaotic regions between two articles [4,16] have been clarified in [17][18][19].…”

Covariant anomaly and Hawking radiation from the modified black hole in the rainbow gravity theory

“…The case of rotating black holes was investigated in [12][13][14], where the rotation acts as an induced U(1) Abelian gauge field. Subsequently considerable efforts [15][16][17][18][19][20][21][22][23][24][25][26][27][28][29] have been done to apply the method to various kinds of space-times. However all these researches are based upon the original RW's formalism [10,11] to derive Hawking radiation via the cancellation of consistent anomalies but to fix it by requiring the regularity of covariant anomaly at the horizon.…”