Unsettling Physics in the Quantum-Corrected Schwarzschild Black Hole
We study a quantum-corrected Schwarzschild black hole proposed recently in Loop Quantum Gravity. Prompted by the fact that corrections to the innermost stable circular orbit of Schwarzschild diverge, we investigate time-like and null radial geodesics. Massive particles moving radially outwards are c...
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MDPI AG
2020-08-01
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Series: | Symmetry |
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Online Access: | https://www.mdpi.com/2073-8994/12/8/1264 |
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author | Valerio Faraoni Andrea Giusti |
author_facet | Valerio Faraoni Andrea Giusti |
author_sort | Valerio Faraoni |
collection | DOAJ |
description | We study a quantum-corrected Schwarzschild black hole proposed recently in Loop Quantum Gravity. Prompted by the fact that corrections to the innermost stable circular orbit of Schwarzschild diverge, we investigate time-like and null radial geodesics. Massive particles moving radially outwards are confined, while photons make it to infinity with infinite redshift. This unsettling physics, which deviates radically from both Schwarzschild (near the horizon) and Minkowski (at infinity) is due to repulsion by the negative quantum energy density that makes the quasilocal mass vanish as one approaches spatial infinity. |
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institution | Directory Open Access Journal |
issn | 2073-8994 |
language | English |
last_indexed | 2024-03-10T18:03:04Z |
publishDate | 2020-08-01 |
publisher | MDPI AG |
record_format | Article |
series | Symmetry |
spelling | doaj.art-5771e5cec50b4f8bb9a5a29a8df600302023-11-20T08:44:39ZengMDPI AGSymmetry2073-89942020-08-01128126410.3390/sym12081264Unsettling Physics in the Quantum-Corrected Schwarzschild Black HoleValerio Faraoni0Andrea Giusti1Department of Physics & Astronomy, Bishop’s University, 2600 College Street, Sherbrooke, QC J1M 1Z7, CanadaDepartment of Physics & Astronomy, Bishop’s University, 2600 College Street, Sherbrooke, QC J1M 1Z7, CanadaWe study a quantum-corrected Schwarzschild black hole proposed recently in Loop Quantum Gravity. Prompted by the fact that corrections to the innermost stable circular orbit of Schwarzschild diverge, we investigate time-like and null radial geodesics. Massive particles moving radially outwards are confined, while photons make it to infinity with infinite redshift. This unsettling physics, which deviates radically from both Schwarzschild (near the horizon) and Minkowski (at infinity) is due to repulsion by the negative quantum energy density that makes the quasilocal mass vanish as one approaches spatial infinity.https://www.mdpi.com/2073-8994/12/8/1264quantum-corrected black holeLoop Quantum Gravitypseudo-Newtonian potential |
spellingShingle | Valerio Faraoni Andrea Giusti Unsettling Physics in the Quantum-Corrected Schwarzschild Black Hole Symmetry quantum-corrected black hole Loop Quantum Gravity pseudo-Newtonian potential |
title | Unsettling Physics in the Quantum-Corrected Schwarzschild Black Hole |
title_full | Unsettling Physics in the Quantum-Corrected Schwarzschild Black Hole |
title_fullStr | Unsettling Physics in the Quantum-Corrected Schwarzschild Black Hole |
title_full_unstemmed | Unsettling Physics in the Quantum-Corrected Schwarzschild Black Hole |
title_short | Unsettling Physics in the Quantum-Corrected Schwarzschild Black Hole |
title_sort | unsettling physics in the quantum corrected schwarzschild black hole |
topic | quantum-corrected black hole Loop Quantum Gravity pseudo-Newtonian potential |
url | https://www.mdpi.com/2073-8994/12/8/1264 |
work_keys_str_mv | AT valeriofaraoni unsettlingphysicsinthequantumcorrectedschwarzschildblackhole AT andreagiusti unsettlingphysicsinthequantumcorrectedschwarzschildblackhole |