Quasar Absorption-Line Number Density in a Closed, Λ-Dominated Universe

被引:0
作者
J. M. Overduin
W. Priester
机构
[1] Stanford University,Gravity Probe B, Hansen Experimental Physics Laboratory
[2] Universität Bonn,Institut für Astrophysik und Extraterrestrische Forschung
来源
Astrophysics and Space Science | 2006年 / 305卷
关键词
Quasars; absorption lines; cosmology; cosmological parameters;
D O I
暂无
中图分类号
学科分类号
摘要
We investigate the dependence of the line number density in the Lyman α forest on cosmological and evolutionary parameters. Recent data from eight high-redshift quasars obtained with VLT/UVES imply that either there is very strong evolution in the absorber population, or we live in a “nearly flat” closed universe which is more heavily vacuum-dominated than standard ΛCDM models.
引用
收藏
页码:159 / 163
页数:4
相关论文
共 19 条
[1]  
Carroll S.M.(1992)undefined Ann. Rev. Astron. Astrophys 30 499-undefined
[2]  
Press W.H.(1990)undefined Nature 348 705-undefined
[3]  
Turner E.L.(1986)undefined Rev. Mod. Phys 58 689-undefined
[4]  
Efstathiou G.(1991)undefined Comments Astrophys 15 127-undefined
[5]  
Sutherland W.J.(2003)undefined Astrophys. J 598 102-undefined
[6]  
Maddox S.J.(1992)undefined Astron. Astrophys 261 377-undefined
[7]  
Felten J.E.(2004)undefined Astrophys. J 611 26-undefined
[8]  
Isaacman R.(1998)undefined Naturwissenschaften 85 524-undefined
[9]  
Hoell J.(1998)undefined Ann. Rev. Astron. Astrophys 36 301-undefined
[10]  
Priester W.(2003)undefined Astrophys. J 594 1-undefined