HI cosmology:: Expectations at z>6

被引:0
|
作者
Cen, Renyue
机构
关键词
cosmology; intergalactic medium; reionization; star formation;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
One would not have expected just a few years ago that we could observationally start probing the reionization process in the redshift range 6-15. This is indeed extremely exciting, because we are in a completely uncharted water. I will review some of the latest developments on cosmological reionization and what is being done on the theoretical side to make detailed predictions of reionization signatures in the high-z universe with respect to the evolution of neutral intergalactic medium.
引用
收藏
页码:10 / 16
页数:7
相关论文
共 50 条
  • [31] Impenetrable barriers for positrons in neighbourhood of superheavy nuclei with Z>118
    Neznamov, V. P.
    XVII WORKSHOP ON HIGH ENERGY SPIN PHYSICS (DSPIN-2017), 2018, 938
  • [32] Stars and stellar systems at z>5:: Implications for structure formation and nucleosynthesis
    Rees, MJ
    SPACE SCIENCE REVIEWS, 1998, 84 (1-2) : 43 - 53
  • [33] The second APM UKST colour survey for z>4 quasars
    Storrie-Lombardi, LJ
    Irwin, MJ
    McMahon, RG
    Hook, IM
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2001, 322 (04) : 933 - 944
  • [34] F stars, metallicity, and the ages of red galaxies at z>1
    Nolan, LA
    OBSERVED HR DIAGRAMS AND STELLAR EVOLUTION: THE INTERPLAY BETWEEN OBSERVATIONAL CONSTRAINTS AND THEORY, 2002, 274 : 416 - 420
  • [35] The Z>4 quasar population observed by Chandra and XMM-Newton
    Vignali, C
    Brandt, WN
    Schneider, DP
    MULTIWAVELENGTH AGN SURVEYS, 2004, : 287 - 290
  • [36] Fusion-fission of nuclei with Z>100 at low excitation energies
    Itkis, MG
    Oganessian, YT
    Kozulin, EM
    Kondratiev, NA
    Krupa, L
    Pokrovsky, IV
    Polyakov, AN
    Ponomarenko, VA
    Prokhorova, EV
    Pustylnik, BI
    Rusanov, AY
    Vakatov, VI
    NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA A-NUCLEI PARTICLES AND FIELDS, 1998, 111 (6-7): : 783 - 790
  • [37] Host galaxies and cluster environment of BL Lac objects at z>0.5
    Heidt, J
    Fried, J
    Hopp, U
    Jäger, K
    Nilsson, K
    Sutorius, E
    QSO HOSTS AND THEIR ENVIRONMENTS, 2001, : 39 - 44
  • [38] The universe at z>5:: When and how did the "dark age" end?
    Rees, MJ
    PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 1998, 95 (01) : 47 - 52
  • [39] PG 1002+506:: A Be star apparently at z>+10 kiloparsecs
    Ringwald, FA
    Rolleston, WRJ
    Saffer, RA
    Thorstensen, JR
    ASTROPHYSICAL JOURNAL, 1998, 497 (02): : 717 - 720
  • [40] FeII/Mg II emission-line ratios of QSOs.: II.: z>6 objects
    Iwamuro, F
    Kimura, M
    Eto, S
    Maihara, T
    Motohara, K
    Yoshii, Y
    Doi, M
    ASTROPHYSICAL JOURNAL, 2004, 614 (01): : 69 - 74