Evaporating black-to-white hole

التفاصيل البيبلوغرافية
العنوان: Evaporating black-to-white hole
المؤلفون: Martin-Dussaud, Pierre, Rovelli, Carlo
المساهمون: 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)
المصدر: https://hal.science/hal-02148273Test ; 2024.
بيانات النشر: HAL CCSD
سنة النشر: 2024
المجموعة: Université de Toulon: HAL
مصطلحات موضوعية: space-time: geometry, radiation: Hawking, back reaction, black hole: evaporation, effect: quantum, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
الوصف: 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.
نوع الوثيقة: report
اللغة: English
العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/1905.07251; hal-02148273; https://hal.science/hal-02148273Test; https://hal.science/hal-02148273/documentTest; https://hal.science/hal-02148273/file/1905.07251.pdfTest; ARXIV: 1905.07251; INSPIRE: 1735402
DOI: 10.1088/1361-6382/ab5097
الإتاحة: https://doi.org/10.1088/1361-6382/ab5097Test
https://hal.science/hal-02148273Test
https://hal.science/hal-02148273/documentTest
https://hal.science/hal-02148273/file/1905.07251.pdfTest
حقوق: info:eu-repo/semantics/OpenAccess
رقم الانضمام: edsbas.A1988EC9
قاعدة البيانات: BASE