scholarly journals DIRAC MONOPOLES AND HAWKING RADIATION IN KOTTLER SPACETIME

2002 ◽  
Vol 17 (32) ◽  
pp. 4947-4957
Author(s):  
A. A. BYTSENKO ◽  
YU. P. GONCHAROV
Keyword(s):  
Black Hole ◽  
Scalar Field ◽  
Energy Density ◽  
Hawking Radiation ◽  
Natural Extension ◽  
Schwarzschild Black Hole ◽  
Complex Scalar ◽  
Radiation Process ◽  
Complex Scalar Field ◽  
The Given

The natural extension of Schwarzschild metric to the case of nonzero cosmological constant Λ known as the Kottler metric is considered and it is discussed under what circumstances the given metric could describe the Schwarzschild black hole immersed in a medium with nonzero energy density. Under the latter situation such an object might carry topologically inequivalent configurations of various fields. The given possibility is analyzed for complex scalar field and it is shown that the mentioned configurations might be tied with natural presence of Dirac monopoles on black hole under consideration. In turn, this could markedly modify the Hawking radiation process.

INCREASE OF HAWKING RADIATION FROM BLACK HOLES BY DIRAC MONOPOLES

1996 ◽  
Vol 05 (04) ◽  
pp. 419-432 ◽  
Author(s):  
YU. P. GONCHAROV ◽  
N.E. FIRSOVA
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Scalar Field ◽  
Hawking Radiation ◽  
Schwarzschild Black Hole ◽  
Complex Scalar ◽  
Total Luminosity ◽  
Complex Scalar Field

We study a mechanism of increasing Hawking radiation from a black hole by using the example of twisted topologically inequivalent configurations (TICs) of a complex scalar field on the Schwarzschild black hole. Physically this increase is tied with the natural presence of Dirac monopoles on black holes. We satisfy both analytical and numerical considerations and find that twisted TICs give the contribution of order 17% to the total luminosity (summed up over all the TICs) of a black hole.

scholarly journals On the pattern of black hole information release

2014 ◽  
Vol 29 (09) ◽  
pp. 1450047 ◽  
Author(s):  
I. Y. Park ◽  
F. James
Keyword(s):  
Black Hole ◽  
Scalar Field ◽  
Scattering Amplitudes ◽  
Cross Section ◽  
Schwarzschild Black Hole ◽  
Complex Scalar ◽  
Mass Growth ◽  
Complex Scalar Field ◽  
Black Hole Information ◽  
Flux Loss

We propose a step towards a resolution to black hole information paradox by analyzing scattering amplitudes of a complex scalar field around a Schwarzschild black hole. The scattering cross-section reveals much information on the incoming state but exhibits flux loss at the same time. The flux loss should be temporary, and indicate mass growth of the black hole. The black hole should Hawking-radiate subsequently, thereby, compensating for the flux loss. By examining the purity issue, we comment on the possibility that information bleaching may be the key to the paradox.

scholarly journals Wave Function for the Reissner–Nordström Black Hole

1997 ◽  
Vol 12 (20) ◽  
pp. 1491-1505 ◽  
Author(s):  
P. V. Moniz
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Wave Function ◽  
Scalar Field ◽  
Hawking Radiation ◽  
Apparent Horizon ◽  
Complex Scalar ◽  
Charge Rate ◽  
Quantum Behavior ◽  
Complex Scalar Field

We study the quantum behavior of Reissner–Nordström (RN) black holes interacting with a complex scalar field. A Maxwell field is also present. Our analysis is based on M. Pollock's1 method and is characterized by solving a Wheeler–DeWitt equation in the proximity of an apparent horizon of the RN space–time. Subsequently, we obtain a wave function Ψ RN [M,Q] representing the RN black hole when its charge, |Q|, is small in comparison with its mass, M. We then compare quantum-mechanically the cases of (i) Q=0 and (ii) M≥|Q|≠0. A special emphasis is given to the evolution of the mass-charge rate affected by Hawking radiation.

Entropy in a d-dimensional charged black hole

2018 ◽  
Vol 33 (27) ◽  
pp. 1850159 ◽  
Author(s):  
Shad Ali ◽  
Xin-Yang Wang ◽  
Wen-Biao Liu
Keyword(s):  
Black Hole ◽  
Scalar Field ◽  
Hawking Radiation ◽  
Space Time ◽  
Charged Black Hole ◽  
Schwarzschild Black Hole ◽  
Proportionality Coefficient ◽  
Proportional Relation ◽  
Hamiltonian Analysis ◽  
Interior Volume

Christodoulou and Rovelli have shown that the interior volume of a Schwarzschild black hole grows linearly with time. The entropy of a scalar field in this interior volume of a Schwarzschild black hole has been calculated and shown to increase linearly with the advanced time too. In this paper, considering Hawking radiation from a d-dimensional charged black hole, we investigate the proportional relation between the entropy of the scalar field in the interior volume and the Bekenstein–Hawking entropy using the method of our previous work. We also derive this proportionality relation using Hamiltonian analysis and find a consistent result. We then investigate the proportionality coefficient with respect to d and find that it gradually decreases as the dimension of space–time increases.

S-MATRICES FOR QUANTUM CHARGED MASSIVE SCALAR PARTICLES ON KERR BLACK HOLES

2001 ◽  
Vol 16 (22) ◽  
pp. 1465-1477 ◽  
Author(s):  
N. E. FIRSOVA
Keyword(s):  
Black Holes ◽  
Scalar Field ◽  
Hawking Radiation ◽  
Massive Scalar ◽  
Numerical Computations ◽  
Scattering Problems ◽  
Complex Scalar ◽  
Scalar Particles ◽  
Complex Scalar Field ◽  
Kerr Black Holes

The results obtained recently on the scattering problems connected with the contribution of the topologically inequivalent configurations of the massless complex scalar field on Kerr black holes to the Hawking radiation are extended to include the massive case as well. The corresponding S-matrices are examined and presented in the form convenient for numerical computations.

COMPLEX LINE BUNDLES OVER TWO-SPHERE AND BLACK HOLE PHYSICS

1994 ◽  
Vol 09 (34) ◽  
pp. 3175-3183 ◽  
Author(s):  
YU. P. GONCHAROV ◽  
J.V. YAREVSKAYA
Keyword(s):  
Black Hole ◽  
Black Hole Physics ◽  
Dimensional Space ◽  
Line Bundles ◽  
Complex Line ◽  
Schwarzschild Black Hole ◽  
Complex Scalar ◽  
Complex Scalar Field ◽  
Standing Problem ◽  
Complex Line Bundles

We discuss a long-standing problem of the global topological non-trivial properties of the four-dimensional space-times underlying black hole physics and observe that the standard space-time topology of the ℝ2×S2 form for black hole physics admits topologically inequivalent configurations of a complex scalar field on black hole by virtue of the availability of non-trivial complex line bundles over S2. Each configuration can be labeled by its Chern number n∈ℤ. For the Schwarzschild black hole we formulate an appropriate wave equation for these configurations in massless case and describe its solutions as a first step to study quantum effects for the above configurations within the framework of black hole physics.

scholarly journals Complex Scalar Field Reheating and Primordial Black Hole production

2021 ◽  
Vol 2021 (07) ◽  
pp. 001
Author(s):  
Karim Carrion ◽  
Juan Carlos Hidalgo ◽  
Ariadna Montiel ◽  
Luis E. Padilla
Keyword(s):  
Black Hole ◽  
Scalar Field ◽  
Primordial Black Hole ◽  
Complex Scalar ◽  
Complex Scalar Field

scholarly journals ON GENERALIZED MONOPOLE SPHERICAL HARMONICS AND THE WAVE EQUATION OF A CHARGED MASSIVE KERR BLACK HOLE

2010 ◽  
Vol 25 (38) ◽  
pp. 3191-3200
Author(s):  
SHABNAM BEHESHTI ◽  
FLOYD L. WILLIAMS
Keyword(s):  
Black Hole ◽  
Wave Equation ◽  
Scalar Field ◽  
Spherical Harmonics ◽  
Spherical Harmonic ◽  
Kerr Black Hole ◽  
Complex Scalar ◽  
Linearly Independent ◽  
Complex Scalar Field

We find linearly independent solutions of the Goncharov–Firsova equation in the case of a massive complex scalar field on a Kerr black hole. The solutions generalize, in some sense, the classical monopole spherical harmonic solutions previously studied in the massless cases.

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