scholarly journals The Computational Limit to Quantum Determinism and the Black Hole Information Loss Paradox

2015 ◽  
Vol 7 (2) ◽  
pp. 107-113
Author(s):  
Arkady Bolotin
Keyword(s):  
Black Hole ◽  
Information Loss ◽  
Information Loss Paradox ◽  
Black Hole Information

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.

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.

A new length scale for quantum gravity: A resolution of the black hole information loss paradox

2017 ◽  
Vol 26 (12) ◽  
pp. 1743015 ◽  
Author(s):  
Tejinder P. Singh
Keyword(s):  
Black Hole ◽  
Information Loss ◽  
Einstein Equations ◽  
Dirac Field ◽  
Length Scale ◽  
Compton Wavelength ◽  
Information Loss Paradox ◽  
Torsion Field ◽  
Black Hole Information ◽  
Schwarzschild Radius

We show why and how Compton wavelength and Schwarzschild radius should be combined into one single new length scale, which we call the Compton–Schwarzschild length. Doing so offers a resolution of the black hole information loss paradox, and suggests Planck mass remnant black holes as candidates for dark matter. It also compels us to introduce torsion, and identify the Dirac field with a complex torsion field. Dirac equation and Einstein equations, are shown to be mutually dual limiting cases of an underlying gravitation theory which involves the Compton–Schwarzschild length scale, and includes a complex torsion field.

scholarly journals INFORMATION-PRESERVING BLACK HOLES STILL DO NOT PRESERVE BARYON NUMBER AND OTHER EFFECTIVE GLOBAL QUANTUM NUMBERS

2005 ◽  
Vol 14 (12) ◽  
pp. 2293-2300 ◽  
Author(s):  
DEJAN STOJKOVIC ◽  
GLENN D. STARKMAN ◽  
FRED C. ADAMS
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Quantum Number ◽  
Baryon Number ◽  
Information Loss ◽  
Quantum States ◽  
Literature Information ◽  
Information Loss Paradox ◽  
Quantum Numbers ◽  
Black Hole Information

It has been claimed recently that the black hole information-loss paradox has been resolved: the evolution of quantum states in the presence of a black hole is unitary and information preserving. We point out that, contrary to some claims in literature, information-preserving black holes still violate the baryon number and any other quantum number which follows from an effective (and thus approximate) or anomalous symmetry.

scholarly journals Binary Black Hole Information Loss Paradox & Future Prospects

2020 ◽  
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 pseudo-density operator. This approach has successfully dealt 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.

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