Zeeman splitting E 1 =E 0 -μ B H, E 2 =E 0 + μ B H, μ B =eћ/(2m e c), μ B =9.3*10 -21 erg/G

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Magnetic field estimations near BH horizon in AGNs and GBHCs (Zakharov, Kardashev, Lukash, Repin, MNRAS, 342,1325, (2003)). Zeeman splitting E 1 =E 0 -μ B H, E 2 =E 0 + μ B H, μ B =eћ/(2m e c), μ B =9.3*10 -21 erg/G Figure1 Figure2 Figure3 Figure4 Figure5 Figure6 ASCAdata. - PowerPoint PPT Presentation

Transcript of Zeeman splitting E 1 =E 0 -μ B H, E 2 =E 0 + μ B H, μ B =eћ/(2m e c), μ B =9.3*10 -21 erg/G

Page 1: Zeeman splitting E 1 =E 0 -μ B H, E 2 =E 0 + μ B H, μ B =eћ/(2m e c), μ B =9.3*10 -21 erg/G
Page 2: Zeeman splitting E 1 =E 0 -μ B H, E 2 =E 0 + μ B H, μ B =eћ/(2m e c), μ B =9.3*10 -21 erg/G

Magnetic field estimations near BH horizon in AGNs and GBHCs

(Zakharov, Kardashev, Lukash, Repin, MNRAS, 342,1325, (2003))

• Zeeman splitting E1=E0-μBH, E2=E0+ μBH, μB=eћ/(2mec), μB=9.3*10-21 erg/G

• Figure1• Figure2• Figure3• Figure4• Figure5• Figure6• ASCAdata

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Mirages around Kerr black holes and retro-gravitational lenses

• Let us consider an illumination of black holes. Then retro-photons form caustics around black holes or mirages around black holes or boundaries around shadows.

• (Zakharov, Nucita, DePaolis, Ingrosso,• New Astronomy 10 (2005) (479-489); astro-

ph/0411511)

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