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Evaporating black-to-white hole

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اقرأ أكثر حفظ في قائمتي
  • معلومة اضافية
    • Contributors:
      Centre de Physique Théorique - UMR 7332 (CPT); Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS); ANR-11-IDEX-0001,Amidex,INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE(2011); ANR-11-LABX-0060,OCEVU,Origines, Constituants et EVolution de l'Univers(2011)
    • بيانات النشر:
      HAL CCSD
    • الموضوع:
      2024
    • Collection:
      Université de Toulon: HAL
    • نبذة مختصرة :
      International audience ; We construct and discuss the form of the (effective) spacetime geometry inside a black hole undergoing a quantum transition to a white hole, taking into account the back-reaction of the component of the Hawking radiation falling into the hole.
    • Relation:
      info:eu-repo/semantics/altIdentifier/arxiv/1905.07251; hal-02148273; https://hal.science/hal-02148273; https://hal.science/hal-02148273/document; https://hal.science/hal-02148273/file/1905.07251.pdf; ARXIV: 1905.07251; INSPIRE: 1735402
    • الرقم المعرف:
      10.1088/1361-6382/ab5097
    • الدخول الالكتروني :
      https://hal.science/hal-02148273
      https://hal.science/hal-02148273/document
      https://hal.science/hal-02148273/file/1905.07251.pdf
      https://doi.org/10.1088/1361-6382/ab5097
    • Rights:
      info:eu-repo/semantics/OpenAccess
    • الرقم المعرف:
      edsbas.A1988EC9