Observational constraint on the dark energy scalar field

• 作者: Ming-Jian Zhang Hong Li
• 来源期刊: 中国物理C（英文版）
• 年，卷（期）: 2021,（4）
• 所属期刊栏目: PARTICLE AND NUCLEAR ASTROPHYSICS AND COSMOLOGY
• 页码范围: 440-450
• 页数: 11页
• 语种: 英文
• DOI: 10.1088/1674-1137/abe0bf

摘要

In this paper,we study three scalar fields,namely the quintessence,phantom,and tachyon fields,to ex plore the source of dark energy via the Gaussian processes method from the background and perturbation growth rate data.The corresponding reconstructions suggest that the dark energy should be dynamical.Moreover,the quintom field,which is a combination of the quintessence and phantom fields,is powerfully favored by the reconstruction.The mean values indicate that the potential V(φ) in the quintessence field is a double exponential function,whereas V(φ) in the phantom field is a double Gaussian function.This reconstruction can provide an important reference for the scalar field study.The two types of data employed reveal that the tachyon field is disadvantageous for describing the cosmic acceleration.