Soft gamma rays from low accreting supermassive black holes and connection to energetic neutrinos
The origins of the soft gamma-ray and high-energy neutrino backgrounds remain unknown. Here, the authors show radiatively inefficient accretion flows of low-luminosity active galactic nuclei can produce the soft gamma ray and high energy neutrino backgrounds simultaneously.
Guardado en:
Autores principales: | Shigeo S. Kimura, Kohta Murase, Péter Mészáros |
---|---|
Formato: | article |
Lenguaje: | EN |
Publicado: |
Nature Portfolio
2021
|
Materias: | |
Acceso en línea: | https://doaj.org/article/4cedad3099ac4b3fa1b6b641cb29f4db |
Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
-
X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary
por: Xinwen Shu, et al.
Publicado: (2020) -
Observational appearances of a f(R) global monopole black hole illuminated by various accretions
por: Guo-Ping Li, et al.
Publicado: (2021) -
Accretion onto a quintessence contaminated rotating black hole: violating the lower limit for eta over s
por: Ritabrata Biswas, et al.
Publicado: (2021) -
Polarized image of a Schwarzschild black hole with a thin accretion disk as photon couples to Weyl tensor
por: Zelin Zhang, et al.
Publicado: (2021) -
Sterile Neutrinos with Neutrino Telescopes
por: Carlos A. Argüelles, et al.
Publicado: (2021)