Coincident $$f(\mathbb {Q})$$ gravity: black holes, regular black holes, and black bounces
نویسندگان
چکیده
Abstract In this paper, we will use the coincident gauge to investigate new solutions of $$f(\mathbb {Q})$$ f ( Q ) theory applied in context black holes, regular and black-bounce spacetime. For each these approaches, compute linear with constraint that non-metricity scalar is zero. We also analyze geodesics solution interpret whether spacetime extensible or not, find Kretschmann determine regularity along spacetime, holes black-bounce, calculate energy conditions. latter case realize null condition ( NEC ), specifically $$NEC_1=WEC_1=SEC_1\leftrightarrow \rho +p_{r}\ge 0$$ N E C 1 = W S ↔ ρ + p r ≥ 0 , satisfied outside event horizon.
منابع مشابه
Dilaton gravity black holes with regular interior
In a one parameter family of dilaton gravity theories which allow the coupling of the dilaton to gravity and to a U(1) gauge field to differ, we have found the existence of everywhere regular spacetimes describing black holes hiding expanding universes inside their horizon.
متن کاملRegular Black Holes and Black Universes
We give a comparative description of different types of regular static, spherically symmetric black holes (BHs) and discuss in more detail their particular type, which we suggest to call black universes. The latter have a Schwarzschild-like causal structure, but inside the horizon there is an expanding Kantowski-Sachs universe and a de Sitter infinity instead of a singularity. Thus a hypothetic...
متن کاملRegular Black Holes and Confinement
Properties of the rotating Kerr-Newman black hole solution allow to relate it with spinning particles. Singularity of black hole (BH) can be regularized by a metric deformation. In this case, as a consequence of the Einstein equations, a material source appears in the form of relativistically rotating superconducting disk which replaces the former singular region. We show a relation of the BH r...
متن کاملDirty Black Holes and Hairy Black Holes.
An approach based on considerations of the non-classical energy momentum tensor outside the event horizon of a black hole provides additional physical insight into the nature of discrete quantum hair on black holes and its effect on black hole temperature. Our analysis both extends previous work based on the Euclidean action techniques, and corrects an omission in that work. We also raise sever...
متن کاملNon-singular Gravity without Black Holes Non-singular Gravity without Black Holes
Canada " What are the everywhere regular solutions of these field equations? " Abstract A non-singular static spherically symmetric solution of the nonsymmetric gravita-tional and electromagnetic theory (NGET) field equations is derived, which depends on the four parameters m, ℓ 2 , Q and s, where m is the mass, Q is the electric charge, ℓ 2 is the NGT charge of a body and s is a dimensionless ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: European Physical Journal C
سال: 2023
ISSN: ['1434-6044', '1434-6052']
DOI: https://doi.org/10.1140/epjc/s10052-023-11660-2