Active Galactic Nuclei=Black Hole Accretion Disk - PowerPoint PPT Presentation

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Active Galactic Nuclei=Black Hole Accretion Disk

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Title: Author: Ryoji Matsumoto Last modified by: Ryoji Matsumoto Created Date: 5/22/2000 1:55:02 PM Document presentation format – PowerPoint PPT presentation

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Title: Active Galactic Nuclei=Black Hole Accretion Disk


1
??????????????3??????????
  • ???? (????)

2
???????????
Active Galactic NucleiBlack Hole Accretion Disk
???????????
3
????????
????????????X????????????????????
4
???????????
Shibata et al. 1995
5
????????????????
  • ????????????????????????????????????
  • ?????????????????
  • ????????????????
  • a??????? trf aP
  • a 0.01-0.1 gtgt ????
  • ????
  • ???????????????
  • ??
  • a O(0.001) ?????
  • ????

??????????????????????
6
?????????????????X?????
GRS1915105?X???(?)?hard/soft?(?)?????(Belloni et
al. 1997)
Cyg X-1???X????? (Negoro et al. 1995)
7
?????????????????????????GRS1915105
VLA????????????????(Mirabel et al.1994)
Mirabel and Rodriguez (1998)
8
???????????????????????????????
Cyg X-1??????????????
???????(high state)????????????????????????
9
????????
  • ????????? (SADM)
  • ????????????????????

Qrad Qvis
  • ????????? (ADAF)

???? ??ADAF ??ADAF
Qadv Qvis
10
??????????
????????????????????
ADAF
??
Q gtQ-
ADAF
Q gtQ-
Q- gtQ
????????
????????
SADM
????
11
??????????(2)
Abramowicz et al. 1995
???
Slim
ADAF
SADM
???
??????
??????
12
???X-1?X?????
X??????????X?????????????????????(Negoro et al.
2001)
????
X?????
??
??
Cyg X-1???X????? (???1995)
?????????????X?????????(Manmoto et al. 1996)
13
QUESTIONS
  • ????????????????????a???????????????
  • ????????????X????????????????????????
  • ??????????????????(ADAF)??????????????
  • ?????????????
  • ???????????????

14
???????????? ??????
Angular momentum
Balbus and Hawley (1991)
15
?????????????????????????????
k//vA(15/16)1/2O????????(3/4)O
???
??
16
??????????????
Astrophysical Rotating Plasma Simulator (ARPS)
17
?????
18
????????3??MHD????(Newtonian)
Initial Condition
After 10 Rotation Period
b Pgas/Pmag100
20064240 grid points
Matsumoto 1999
??????? ????
19
????????????
ORBIT
20
???????????????
Machida et al. 2000
Magnetic Field Lines and Isosurface of Magnetic
Field Strength for a model Starting from ß1
21
??????????????X???????????
Cyg X-1?????(??)? ?????????????(??)
22
??????????????????????????????
Joule Heating Rate
Kawaguchi et al. 2000 PASJ 52, L1
Power Spectrum of Time Variation
23
????????????
??????J/????
???????????
(Kawaguchi et al 2000)
24
??????????????3??????????
Machida and Matsumoto (2002)
25
??????????
????????????? pseudo-Newtonian potential f -
GM/(r-rg)
rg ??????????
???? ????? R50rg???? ???/??? ß 100
???????? Rm 2000
r2rg???????
??????????????????????????? min 0.05, max
(J/?) vc2/Rm , 0.0
26
????
Zoom up Innermost Region
t 30630 -130rgltrlt130rg
27
??????????
( -0.5 lt log? lt 0)
3000 rg/c
? 50rg??Kepler?? ? 0.03 M/Mo
28
????ß(?????????)?????
????
Rm100 R lt 10Rg ??? (Machida et al. 2002)
ß10?????????!
????????500????
29
????????PSD
PSD
F(-1.5)
???????????????????10????????????????100Hz
?????Cyg X-1?PSD
???
30
????????????
???????????(rlt60)
?????????????(rlt10)
T30590
??????????10rg?????????????(BSS)??????????????????
???
31
Maxwell Stress?????? lt-BrBf/4pgt/ltPgt?????
??(4lt r lt 10 )
??(20 lt rlt 40 )
a0.1
a0.03
TIME
TIME
32
???????????????
????????????
?????????????t29000??31000?????????
33
????????
30570
30590
30610
30630
????? ????????????????????????
34
?????????????
???????
35
????
T30590
T30610
T30630
??????????????????????????????????????????????????
???????????????????????????????????
36
?????????????????
??????
T30590
????
???????
T30610
???
T30630
?????????????
time
37
X????????
????????? ? ???????
38
(No Transcript)
39
???
X-ray shot
???????????????????????
??????
??????????
????????? BSS???????
???????????(?????)??
40
?????????????? ????????
41
?????????????
Blandford and Payne 1982
Maruyama and Fujimoto 1987 Lovelace et al. 1991
42
Steady Model of Axisymmetric Jet(Kudoh and
Shibata 1997)
Along a Magnetic Field Line
43
?????????
44
?????????????? (Kuwabara et al. 2000
PASJ)
ideal
Mildly resistive
45
3D Structure
T0
T25
T33
T40
T0
T25
T33
T40
T0
T25
T33
T40
46
Works in progress Implementation of general
relativistic code
Study the time evolution of rotating black holes
with a rotating torus. Simulate how much energy
is extracted through magnetic fields.
Koide, Shibata, Kudoh, and Meier 2002, Science
47
??????MHD????(Koide et al. 1998,1999,2000)
V 0.93c (G2.7)
48
???
  • ??????????????3?????MHD?????????
  • Rlt10rg?????????????(BSS)??????1????????????
  • ??????????????????????BSS?????????????????????????
    ???????????
  • ??????????????????????Cyg X-1????????X????????????
    ???????????????????
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