scholarly journals Corrected Hawking Radiation of Dirac Particles from a General Static Riemann Black Hole

2013 ◽  
Vol 2013 ◽  
pp. 1-6 ◽  
Author(s):  
Ge-Rui Chen ◽  
Yong-Chang Huang
Keyword(s):  
Black Hole ◽  
Quantum Theory ◽  
Hawking Radiation ◽  
Radiation Spectrum ◽  
Direct Consequence ◽  
Information Loss ◽  
Back Reaction ◽  
Information Loss Paradox ◽  
Dirac Particles ◽  
Black Hole Information

Considering energy conservation and the back reaction of radiating particles to the spacetime, we investigate the massive Dirac particles' Hawking radiation from a general static Riemann black hole using improved Damour-Ruffini method. A direct consequence is that the radiation spectrum is not strictly thermal. The correction to the thermal spectrum is consistent with an underlying unitary quantum theory and this may have profound implications for the black hole information loss paradox.

scholarly journals A SECRET TUNNEL THROUGH THE HORIZON

2004 ◽  
Vol 13 (10) ◽  
pp. 2351-2354 ◽  
Author(s):  
MAULIK PARIKH
Keyword(s):  
Black Hole ◽  
Quantum Theory ◽  
Energy Conservation ◽  
Hawking Radiation ◽  
Radiation Spectrum ◽  
Direct Consequence ◽  
Thermal Spectrum ◽  
Black Hole Information

Hawking radiation is often intuitively visualized as particles that have tunneled across the horizon. Yet, at first sight, it is not apparent where the barrier is. Here I show that the barrier depends on the tunneling particle itself. The key is to implement energy conservation, so that the black hole contracts during the process of radiation. A direct consequence is that the radiation spectrum cannot be strictly thermal. The correction to the thermal spectrum is of precisely the form that one would expect from an underlying unitary quantum theory. This may have profound implications for the black hole information puzzle.

MODIFIED HAWKING RADIATION FROM A KERR–NEWMAN BLACK HOLE DUE TO BACK-REACTION

2008 ◽  
Vol 23 (04) ◽  
pp. 281-287 ◽  
Author(s):  
BO LIU ◽  
GANG WANG ◽  
WENBIAO LIU
Keyword(s):  
Black Hole ◽  
Angular Momentum ◽  
Hawking Radiation ◽  
Energy Charge ◽  
Information Loss ◽  
Back Reaction ◽  
Information Loss Paradox ◽  
Newman Black Hole

Hawking radiation from a general Kerr–Newman black hole is investigated using Damour–Ruffini's method. Considering the back-reaction of particle's energy, charge and angular momentum to the spacetime, we obtain a modified nonthermal spectrum. Maybe the information loss paradox can be explained, furthermore, the result is also consistent with the result obtained using Parikh and Wilczek's method.

scholarly journals Binary Black Hole Information Loss Paradox and Future Prospects

Entropy ◽  
2020 ◽  
Vol 22 (12) ◽  
pp. 1387
Author(s):  
Ayan Mitra ◽  
Pritam Chattopadhyay ◽  
Goutam Paul ◽  
Vasilios Zarikas
Keyword(s):  
Black Hole ◽  
Information Loss ◽  
Complete Agreement ◽  
Future Prospects ◽  
Information Loss Paradox ◽  
Binary Black Hole ◽  
Proposed Model ◽  
Qubit System ◽  
Input Source ◽  
Black Hole Information

Various techniques to tackle the black hole information paradox have been proposed. A new way out to tackle the paradox is via the use of a pseudo-density operator. This approach has successfully dealt with the problem with a two-qubit entangle system for a single black hole. In this paper, we present the interaction with a binary black hole system by using an arrangement of the three-qubit system of Greenberger–Horne–Zeilinger (GHZ) state. We show that our results are in excellent agreement with the theoretical value. We have also studied the interaction between the two black holes by considering the correlation between the qubits in the binary black hole system. The results depict a complete agreement with the proposed model. In addition to the verification, we also propose how modern detection of gravitational waves can be used on our optical setup as an input source, thus bridging the gap with the gravitational wave’s observational resources in terms of studying black hole properties with respect to quantum information and entanglement.

scholarly journals Non-Monogamy of Spatio-Temporal Correlations and the Black Hole Information Loss Paradox

Entropy ◽  
2020 ◽  
Vol 22 (2) ◽  
pp. 228 ◽  
Author(s):  
Chiara Marletto ◽  
Vlatko Vedral ◽  
Salvatore Virzì ◽  
Enrico Rebufello ◽  
Alessio Avella ◽  
...  
Keyword(s):  
Black Hole ◽  
Physical Phenomenon ◽  
Quantum Correlations ◽  
Information Loss ◽  
Experimental Demonstration ◽  
Information Loss Paradox ◽  
Temporal Correlations ◽  
Black Hole Information ◽  
Spatio Temporal ◽  
Theoretical Proposal

Pseudo-density matrices are a generalisation of quantum states and do not obey monogamy of quantum correlations. Could this be the solution to the paradox of information loss during the evaporation of a black hole? In this paper we discuss this possibility, providing a theoretical proposal to extend quantum theory with these pseudo-states to describe the statistics arising in black-hole evaporation. We also provide an experimental demonstration of this theoretical proposal, using a simulation in optical regime, that tomographically reproduces the correlations of the pseudo-density matrix describing this physical phenomenon.

Black-hole Information Loss Problem: Past, Present, and Future

2020 ◽  
Vol 29 (11) ◽  
pp. 17-25
Author(s):  
Sang-Heon YI ◽  
Dong-han YEOM
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Quantum Mechanics ◽  
Quantum Information ◽  
Hawking Radiation ◽  
Recent Progress ◽  
Information Loss ◽  
Future Perspectives ◽  
Black Hole Information ◽  
Information Loss Problem

In this article, we discuss the information loss problem of black holes and critically review candidate resolutions of the problem. As a black hole evaporates via Hawking radiation, it seems to lose original quantum information; this indicates that the unitarity of time evolution in quantum mechanics and the fundamental predictability of physics are lost. We categorized candidate resolutions by asking (1) where information is and (2) which principle of physics is changed. We also briefly comment on the recent progress in the string theory community. Finally, we present several remarks for future perspectives.

Hawking Radiation of Charged Particles as Tunneling from Kim Black Hole

2012 ◽  
Vol 538-541 ◽  
pp. 2169-2174
Author(s):  
Qing Quan Jiang
Keyword(s):  
Black Hole ◽  
Hawking Radiation ◽  
Quantum Tunneling ◽  
Radiation Spectrum ◽  
Charged Particles ◽  
Information Loss ◽  
Unitary Theory ◽  
Conservation Of Energy ◽  
Black Hole Evaporation ◽  
Tunneling Method

In this paper, when considering the conservation of energy, electric charge and angular momentum, we develop the Parikh-Wilczek’s quantum tunneling method to study the Hawking radiation of charged particles via tunneling from the event horizon of Kim black hole. The result shows the exact radiation spectrum deviates from the precisely thermal one, but satisfies an underlying unitary theory, which provides a possible solution to the information loss during the black hole evaporation.

scholarly journals INFORMATION CONSERVATION IS FUNDAMENTAL: RECOVERING THE LOST INFORMATION IN HAWKING RADIATION

2013 ◽  
Vol 22 (12) ◽  
pp. 1341014 ◽  
Author(s):  
BAOCHENG ZHANG ◽  
QING-YU CAI ◽  
MING-SHENG ZHAN ◽  
LI YOU
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Hawking Radiation ◽  
Energy Charge ◽  
Fundamental Principle ◽  
Information Loss ◽  
Information Loss Paradox ◽  
Information Conservation ◽  
World Information ◽  
Conservation Laws Of Energy

In both classical and quantum world, information cannot appear or disappear. This fundamental principle, however, is questioned for a black hole, by the acclaimed "information loss paradox." Based on the conservation laws of energy, charge, and angular momentum, we recently show the total information encoded in the correlations among Hawking radiations equals exactly to the same amount previously considered lost, assuming the nonthermal spectrum of Parikh and Wilczek. Thus the information loss paradox can be falsified through experiments by detecting correlations, for instance, through measuring the covariances of Hawking radiations from black holes, such as the manmade ones speculated to appear in LHC experiments. The affirmation of information conservation in Hawking radiation will shine new light on the unification of gravity with quantum mechanics.

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