Virtual Black Holes, Remnants and the Information Paradox
arXiv:1412.6270 · doi:10.1088/0264-9381/32/4/045007
Abstract
We revisit the question of the contributions of Planckian quantum black holes in general and of remnants in particular to low energy physics observables. As long as quantum gravity preserves the symmetries of the low energy effective field theory, we find that the bounds on the number of quantum black holes or remnants are very weak. Typically we rule out using data on the anomalous magnetic moment of the muon that there are more than quantum black holes coupled to the standard model particles gravitationally. Remnants thus remain a viable option as a solution to the information paradox of black holes.
arXiv comment8 pages
References in corpus (19)
- A Large Mass Hierarchy from a Small Extra Dimension
- The Hierarchy Problem and New Dimensions at a Millimeter
- New Dimensions at a Millimeter to a Fermi and Superstrings at a TeV
- Classical Black Hole Production in High-Energy Collisions
- Entropy Bounds and Black Hole Remnants
- Black Holes and Massive Remnants
- Minimum Length from Quantum Mechanics and Classical General Relativity
- Colorful quantum black holes at the LHC
- Quantum gravity at a TeV and the renormalization of Newton's constant
- Quantum Production of Black Holes
- Information locking in black holes
- Constraints on Black Hole Remnants
- Minimum Length from First Principles
- On the Status of Highly Entropic Objects
- Nonlocal and generalized uncertainty principle black holes
- Black Hole Masses are Quantized
- The anomalous magnetic moment of the muon and radiative lepton decays
- The flavor of quantum gravity
- On the Precision of a Length Measurement
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- Super-renormalizable or Finite Lee-Wick Quantum Gravity
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- Regular black holes from semi-classical down to Planckian size
- Non-Pertubative Quantum Corrections to a Born-Infeld Black Hole and its Information Geometry
- The horizon of the lightest black hole
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- Hawking Radiation of Mass Generating Particles From Dyonic Reissner Nordström Black Hole
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- ER= EPR and Non-Perturbative Action Integrals for Quantum Gravity