宇宙理論研究室ガイダンス
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- あつとし わたぬき
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2 60 S.L.Glashow Glashow : Interaction Warner Books
3
4 CMB CMB
5 /
6
7 The universe in a nutshell
8 A
9 H He C, O Ne, Mg Si Fe
10
11 Sphere(0.1 cylinder (0. slab (0. Cylinder hole (0. Spherical hole (0.
12 20 CMB CMB
13 = CDM Ωtotal
14 21 20
15 Expanding the expanding universe 0th order 1st order 2nd order 3rd order 4th order L-th order M-th order N-th order
16 Zooming in the simulated structure 75h -1 Mpc 5h -1 Mpc 20h -1 Mpc SPH simulations in LCDM (Yoshikawa, Taruya, Jing & Suto 2001)
17 ~ 5x10 12 M sun ~ 5x10 13 M sun ~ 3x10 14 M sun Jing & Suto (2000)
18 Slices from SDSS spectroscopic galaxy samples Clustering of galaxies on the light-cone! (although the light-cone effect is not important) 9971 galaxies (r <17) in in SDSS EDR (Early Data Release) Classification of of early and late -types using the concentration index (Doi, Fukugita & Okamura 1993) by Nakamura, Fukugita et et al. (2001) slice early late total A B
19 SDSS Morphology dependent correlation functions of SDSS galaxies N-body Mock samples and the model predictions SDSS early-type SDSS late-type type average SDSS データ解析 : Kayo, Nakamura Fukugita, Suto et al (2002) redshift space Redshift-space distortion real space 理論モデル :Hamana, Colombi & Suto(2000)
20 Morphology-dependent galaxy bias from SDSS data b( s) ξ( s; galaxies)/ ξ( s; ΛCDM) early-type late-type type assumed fluctuation amplitude and pair-wise velocity dispersion [km/s] average CDM (+ σ 8,, σ p ) assumed. clear morphology dependence on clustering amplitude. early -types are positively biased relative to to mass, while late -types are antibiased. galaxy bias is is fairly scale-independent. Kayo et al., in preparation
21
22 Are we alone?
23 (Wolszczan & Frail) (Mayor & Quelos) (Butler, Marcy & Fisher) (Charbonneau et al., Henry et al.)
24 3m/s
25 (Charbonneau et al. 2000, Henry et al. 2000) (Charbonneau et al. 2001)
26 characterization habitable planets? search for life CO 2 O 3 H 2 O
27
28 S.L.Shapiro and S.Teukolsky Black Holes, White Dwarfs and Neutron Stars
29
太陽系外惑星探査
http://hubblesite.org/newscenter/archive/2001/38/ Terra MODIS http://modarch.gsfc.nasa.gov/ http://www.nasa.gov/home/index.html / 2 Are we alone? Origins Where are they? (Fermi 1950) 3 4 0.5 arcsec 10pc
More informationdark matter density profiles
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http://hubblesite.org/newscenter/archive/2001/38/ 2004 9 30 1781 1846 1930 50 2 3 radial velocity HDS 5m/s HD209458 HD209458+I 2 cell Subaru/HDS 4 (Mayor & Queloz 1995) 4.2 5 2 1.5% HST 4 orbits Brown
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