论文标题

深色能源宇宙学的宇宙学方法:使用超新星,类星体和伽马射线爆发的哈勃图表的新约束

Cosmography approach to dark energy cosmologies: new constrains using the Hubble diagrams of supernovae, quasars and gamma-ray bursts

论文作者

Rezaei, Mehdi, Ojaghi, Saeed Pour, Malekjani, Mohammad

论文摘要

在宇宙学方法的上下文中,并使用哈勃图的数据进行超新星,类星体和伽马射线爆发,我们研究了一些参数化以及一致性$λ$ CDM宇宙。 Using the different combinations of data sample including ({\it i}) supernovae (Pantheon), ({\it ii}) Pantheon + quasars and ({\it iii}) Pantheon + quasars + gamma-ray bursts and applying the minimization of $χ^2$ function of distance modulus of data samples in the context of Markov Chain Monte Carlo method, we first obtain the constrained values模型独立宇宙学方案中的cosmogrogron参数。然后,我们研究我们的分析,对于不同的一致性$λ$ CDM宇宙学,$ W $ CDM,CPL和PADE参数化。将对于DE方案获得的cosmographic参数的数值与模型独立方法的数值进行比较时,我们表明,当我们涉及类星体和伽马射线时,一致性$λ$ CDM模型在我们的分析中会出现严重的张力。虽然高红移类星体和伽马射线爆发可以伪造一致性模型,但我们的宇宙学方法的结果表明,其他DE参数化仍然与这些观察结果一致。

In the context of cosmography approach and using the data of Hubble diagram for supernovae, quasars and gamma-ray bursts, we study some DE parametrizations and also the concordance $Λ$CDM universe. Using the different combinations of data sample including ({\it i}) supernovae (Pantheon), ({\it ii}) Pantheon + quasars and ({\it iii}) Pantheon + quasars + gamma-ray bursts and applying the minimization of $χ^2$ function of distance modulus of data samples in the context of Markov Chain Monte Carlo method, we first obtain the constrained values of the cosmographic parameters in model independent cosmography scenario. We then investigate our analysis, for different concordance $Λ$CDM cosmology, $w$CDM, CPL and Pade parametrizations. Comparing the numerical values of the cosmographic parameters obtained for DE scenarios with those of the model independent method, we show that the concordance $Λ$CDM model has a serious tension when we involve the quasars and gamma-ray bursts data in our analysis. While the high redshift quasars and gamma-ray bursts can falsify the concordance model, our results of cosmography approach indicate that the other DE parametrizations are still consistent with these observations.

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