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Can we constrain the evolution of HI bias using configuration entropy?

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dc.contributor.author Pandey, Biswajit
dc.contributor.author Das, Biswajit
dc.date.accessioned 2021-05-27T11:05:02Z
dc.date.available 2021-05-27T11:05:02Z
dc.date.issued 2020
dc.identifier.uri https://vbudspace.lsdiscovery.in/xmlui/handle/123456789/68
dc.description.abstract We study the evolution of the configuration entropy of HI distribution in the post-reionization era assuming different time evolution of HI bias. We describe time evolution of linear bias of HI distribution using a simple form b(a) = b0a n with different index n. The derivative of the configuration entropy rate is known to exhibit a peak at the scale factor corresponding to the Λ-matter equality in the unbiased ΛCDM model. We show that in the ΛCDM model with time-dependent linear bias, the peak shifts to smaller scale factors for negative values of n. This is related to the fact that the growth of structures in the HI density field can significantly slow down even before the onset of Λ domination in the presence of a strong time evolution of the HI bias. We find that the shift is linearly related to the index n. We obtain the best fit relation between these two parameters and propose that identifying the location of this peak from observations would allow us to constrain the time evolution of HI bias within the framework of the ΛCDM model en_US
dc.language.iso en en_US
dc.publisher CAS and IOP Publishing en_US
dc.relation.ispartofseries RAA 2021 Vol. 21 No. 2, 35(7pp);
dc.subject methods: analytical — cosmology: theory — large scale structure of the universe en_US
dc.title Can we constrain the evolution of HI bias using configuration entropy? en_US
dc.title.alternative Research in Astronomy and Astrophysics en_US
dc.type Article en_US


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