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- URN zum Zitieren dieses Dokuments:
- urn:nbn:de:bvb:355-epub-455699
- DOI zum Zitieren dieses Dokuments:
- 10.5283/epub.45569
Zusammenfassung
In the past years, black holes and the fate of their singularity have been heavily studied within loop quantum gravity. Effective spacetime descriptions incorporating quantum geometry corrections are provided by the so-called polymer models. Despite the technical differences, the main common feature shared by these models is that the classical singularity is resolved by a black-to-white hole ...
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