For the p=1/2 Einstein-Maxwell power-Yang-Mills black hole, increasing the hair parameter Q_YM shrinks the horizon, photon sphere, ISCO, shadow, and photon ring, an effect equivalent to a mass shift in Reissner-Nordström.
New Variables for Classical and Quantum Gravity in all Dimensions III. Quantum Theory
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
abstract
We quantise the new connection formulation of D+1 dimensional General Relativity developed in our companion papers by Loop Quantum Gravity (LQG) methods. It turns out that all the tools prepared for LQG straightforwardly generalise to the new connection formulation in higher dimensions. The only new challenge is the simplicity constraint. While its "diagonal" components acting at edges of spin network functions are easily solved, its "off-diagonal" components acting at vertices are non trivial and require a more elaborate treatment.
citation-role summary
background 1
citation-polarity summary
fields
gr-qc 1years
2025 1verdicts
REJECT 1roles
background 1polarities
unclear 1representative citing papers
citing papers explorer
-
Testing Einstein Maxwell Power-Yang-Mills Hair via Black Hole Photon Rings
For the p=1/2 Einstein-Maxwell power-Yang-Mills black hole, increasing the hair parameter Q_YM shrinks the horizon, photon sphere, ISCO, shadow, and photon ring, an effect equivalent to a mass shift in Reissner-Nordström.