2018/10/31 by Paul R. Anderson, Mathew J. Binkley, Jillian M. Bjerke +2 · 22 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Classical mechanics #Cosmology and Gravitation Theories #Gravitation #Horizon #Inflation (cosmology) #Mathematical physics #Mathematics #Physics #Pulsars and Gravitational Waves Research #Quantum #Quantum mechanics #Semiclassical physics #Sign (mathematics) #Theoretical physics #Zero (linguistics) #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.98.125011
published in Physical review. D/Physical review. D. 98(12) (American Physical Society) · References added, a brief discussion relating to pair creation of black holes added, sign of a higher derivative term corrected, minor changes and corrections, 20 pages, 3 figures
openalex publication_date 2018/12/18 · arxiv created 2019/01/26 · arxiv updated 2019/01/29 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
Zero temperature black hole solutions to the semiclassical backreaction equations are investigated. Evidence is provided that certain components of the stress-energy tensors for free quantum fields at the horizon only depend on the local geometry near the horizon. This allows the semiclassical backreaction equations to be solved near the horizon. It is found that macroscopic uncharged zero temperature black hole solutions to the equations may exist if the coefficient of one of the higher derivative terms in the gravitational Lagrangian is large enough and of the right sign for Starobinsky inflation to have occurred in the early Universe.