Scaling dark energy

被引:11
作者
Capozziello, S
Melchiorri, A
Schirone, A
机构
[1] Univ Salerno, Dipartimento Fis ER Caianiello, I-84081 Baronissi, Salerno, Italy
[2] Ist Nazl Fis Nucl, Sez Napoli, Grp Coll Salerno, I-84081 Baronissi, Salerno, Italy
[3] Univ Roma La Sapienza, Dipartimento Fis G Marconi, I-00185 Rome, Italy
[4] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy
来源
PHYSICAL REVIEW D | 2004年 / 70卷 / 10期
关键词
D O I
10.1103/PhysRevD.70.101301
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the possibility that dark energy is scaling with epochs. A phenomenological model is introduced whose energy density depends on the redshift z in such a way that a smooth transition among the three dominant phases of the Universe evolution (radiation era, matter domination, asymptotic de Sitter state) is achieved. We use the Wilkinson Microwave Anisotropy Probe cosmic microwave background data and the luminosity distances of Type Ia Supernovae to test whether the model is in agreement with astrophysical observations.
引用
收藏
页码:101301 / 1
页数:5
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