Kerr Black Hole as a Pevatron at the Galaxy Center
Conventional general relativity supplies the notion of a vacuum tension and thus a maximum force <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>F</mi><mi>max</mi>&l...
Saved in:
| Main Authors: | Orlando Panella, Simone Pacetti, Giorgio Immirzi, Yogendra Srivastava |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
MDPI AG
2025-05-01
|
| Series: | Universe |
| Subjects: | |
| Online Access: | https://www.mdpi.com/2218-1997/11/5/160 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Image of the Kerr–Newman Black Hole Surrounded by a Thin Accretion Disk
by: Sen Guo, et al.
Published: (2024-01-01) -
Galactic Superaccreting X-Ray Binaries as Super-PeVatron Accelerators
by: Jieshuang Wang, et al.
Published: (2025-01-01) -
Cosmic ray contributions from rapidly rotating stellar mass black holes: cosmic Ray GeV to EeV proton and anti-proton sources
by: M. Allen, et al.
Published: (2024-12-01) -
Nonstandard Thermal History and Formation of Primordial Black Holes and SIGWs in Einstein–Gauss–Bonnet Gravity
by: Yogesh, et al.
Published: (2025-01-01) -
Assessing the Role of Intrinsic Variability in Black Hole Parameter Inference Using Multiepoch EHT Data
by: Dominic O. Chang, et al.
Published: (2025-01-01)