The fate of Reissner-Nortstr\"{o}m black hole in the Einstein-Yang-Mills-Higgs system
Takashi Tamaki, Kei-ichi Maeda
TL;DR
This paper investigates the evaporation process of black holes within the Einstein-Yang-Mills-Higgs framework, comparing monopole black holes and Reissner-Nordström black holes to understand their differing evaporation rates.
Contribution
It provides the first detailed comparison of evaporation rates between monopole black holes and Reissner-Nordström black holes in the Einstein-Yang-Mills-Higgs system.
Findings
Monopole black holes evaporate at different rates than RN black holes.
The scalar field considered does not couple with gauge or Higgs fields.
Differences in evaporation dynamics are highlighted between the two black hole types.
Abstract
We study about an evaporating process of black holes in SO(3) Einstein-Yang-Mills-Higgs system. We consider a massless scalar field which couple neither with the Yang-Mills field nor with the Higgs field surrounding the black hole. We discuss differences in evaporating rate between a monopole black hole and a Reissner-Nortstr\"{o}m (RN) black hole.
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