Prospects for probing the dark energy via supernova distance measurements

被引：358

作者：

Huterer, D ^{[1
]}

Turner, MS

机构：

[1] Univ Chicago, Enrico Fermi Inst, Dept Phys, Chicago, IL 60637 USA

[2] Univ Chicago, Enrico Fermi Inst, Dept Astron & Astrophys, Chicago, IL 60637 USA

[3] Fermi Natl Accelerator Lab, NASA, Fermilab Astrophys Ctr, Batavia, IL 60510 USA

来源：

PHYSICAL REVIEW D | 1999年 / 60卷 / 08期

关键词：

D O I：

10.1103/PhysRevD.60.081301

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Distance measurements to type Ia supernovae (SNe Ia) indicate that the Universe is accelerating and that two-thirds of the critical energy density exists in a dark-energy component with negative pressure. Distance measurements to SNe Ia can be used to distinguish between different possibilities for the dark energy, and if it is an evolving scalar field, to reconstruct the scalar-field potential. We derive the reconstruction equations and address the feasibility of this approach by Monte Carlo simulation. [S0556-2821(99)50118-5].

引用

页数：5

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