论文标题
幻影封闭宇宙学模型的关键测试
A crucial test of the phantom closed cosmological model
论文作者
论文摘要
我们建议进行至关重要的直接观察测试，以测量标准$λ$ CDM模型和最近提出的幻影深曲率曲率宇宙学模型之间的区别。该测试基于一般弗里德曼模型的基本距离 - 频率 - 红移关系。它不取决于CMBR数据，大规模结构增长模型以及哈勃常数$ H_0 $的值。我们的关键测试可以通过Theseus空间任务的未来伽马射线爆发观测来进行，并通过现代高级Ligo-Virgo和即将出现的Lisa探测器使用引力波标准的警笛观测。
We suggest a crucial direct-observational test for measuring distinction between the standard $Λ$CDM model and recently proposed phantom dark energy positive curvature cosmological model. The test is based on the fundamental distance--flux--redshift relation for general Friedmann models. It does not depend on the CMBR data, on the large-scale structure growth models, and also on the value of the Hubble constant $H_0$. Our crucial test can be performed by future gamma-ray burst observations with THESEUS space mission and by using gravitational-wave standard siren observations with modern advanced LIGO--Virgo and also forthcoming LISA detectors.
