期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 511, 期 2, 页码 1637-1646出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stac201
关键词
dark energy; cosmological parameters; cosmology: observations
资金
- Ministry of Human Resource and Development, Government of India via Institute fellowship at IISER Bhopal
The cosmological models with tracker properties are important for understanding dark energy. This paper focuses on the oscillatory tracker model and uses observational data to constrain its parameters. The results show that the oscillatory tracker dark energy model has noticeable differences from the usual ΛCDM predictions, but there is still a high level of agreement between the two.
The cosmological models exhibiting tracker properties have great significance in the context of dark energy as they can reach the present value of dark energy density from a wide range of initial conditions, thereby alleviating both the fine-tuning and the cosmic coincidence problem. The alpha-attractors, which are originally discussed in the context of inflation, can exhibit the properties of dark energy as they can behave like cosmological trackers at early times and show the late-time behaviour of a cosmological constant. In this paper, we study the oscillatory tracker model (OTM), which belongs to the family of alpha-attractor dark energy models. Using the current observational data sets like cosmic microwave background (CMB), baryon acoustic oscillation, and type la supernova data (Pantheon compilation), we constrain the parameters of the model and estimate both the mean and best-fitting values. Although the OTM contains a larger set of parameters than the usual lambda cold dark matter (LCDM) model, the common set of parameters of both agree within 1 sigma error limits. Our observations using both high redshift and low redshift data support Hubble parameter value H-0 = 67.4 Km s(-1) Mpc(-1). We study the effect of the OTM on the CMB temperature and polarization power spectra, matter power spectrum and f sigma(8). Our analysis of the CMB power spectrum and matter power spectrum suggests that the oscillatory tracker dark energy model has noticeable differences from usual LCDM predictions. Yet, in most cases, the agreement is very close.
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