Non-Singular Quantum Geometry of the Schwarzschild Black Hole Interior

Ashtekar, Abhay; Bojowald, Martin

アイテム詳細

登録内容を編集ファイル形式で保存

一時保存へ追加

タグ情報を表示リリース履歴を表示詳細要約

公開

学術論文

Non-Singular Quantum Geometry of the Schwarzschild Black Hole Interior

MPS-Authors

Bojowald, Martin
Quantum Gravity & Unified Theories, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

External Resource

There are no locators available

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

フルテキスト (公開)

0509075.pdf
(プレプリント), 323KB

付随資料 (公開)

There is no public supplementary material available

引用

Ashtekar, A., & Bojowald, M. (2006). Non-Singular Quantum Geometry of the Schwarzschild Black Hole Interior. Classical and Quantum Gravity, 23(2), 391-412.

引用: https://hdl.handle.net/11858/00-001M-0000-0013-4B39-6

要旨

In homogeneous cosmologies, quantum geometry effects lead to a resolution of the classical singularity without having to invoke special boundary conditions at the singularity or introduce ad-hoc elements such as unphysical matter. The same effects are shown to lead to a resolution of the Schwarzschild singularity. The resulting quantum extension of space-time is likely to have significant implications to the black hole evaporation process. Similarities and differences with the situation in quantum geometrodynamics are pointed out.