The monopole and quadrupole moments of the Epoch of Reionization (EoR) 21-cm bispectrum

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Autori principali: Gill, Sukhdeep Singh, Pramanick, Suman, Bharadwaj, Somnath, Shaw, Abinash Kumar, Majumdar, Suman
Natura: Preprint
Pubblicazione: 2023
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author Gill, Sukhdeep Singh
Pramanick, Suman
Bharadwaj, Somnath
Shaw, Abinash Kumar
Majumdar, Suman
author_facet Gill, Sukhdeep Singh
Pramanick, Suman
Bharadwaj, Somnath
Shaw, Abinash Kumar
Majumdar, Suman
contents We study the monopole ($\bar{B}^0_0$) and quadrupole ($\bar{B}^0_2$) moments of the 21-cm bispectrum (BS) from EoR simulations and present results for squeezed and stretched triangles. Both $\bar{B}^0_0$ and $\bar{B}^0_2$ are positive at the early stage of EoR where the mean neutral hydrogen (HI) density fraction $\bar{x}_{\rm HI} \approx 0.99$. The subsequent evolution of $\bar{B}^0_0$ and $\bar{B}^0_2$ at large and intermediate scales $(k=0.29$ and $0.56 \, {\rm Mpc}^{-1}$ respectively) is punctuated by two sign changes which mark transitions in the HI distribution. The first sign flip where $\bar{B}^0_0$ becomes negative occurs in the intermediate stages of EoR $(\bar{x}_{\rm HI} > 0.5)$, at large scale first followed by the intermediate scale. This marks the emergence of distinct ionized bubbles in the neutral background. $\bar{B}^0_2$ is relatively less affected by this transition, and it mostly remains positive even when $\bar{B}^0_0$ becomes negative. The second sign flip, which affects both $\bar{B}^0_0$ and $\bar{B}^0_2$, occurs at the late stage of EoR $(\bar{x}_{\rm HI} < 0.5)$. This marks a transition in the topology of the HI distribution, after which we have distinct HI islands in an ionized background. This causes $\bar{B}^0_0$ to become positive. The negative $\bar{B}^0_2$ is a definite indication that the HI islands survive only in under-dense regions.
format Preprint
id arxiv_https___arxiv_org_abs_2310_15579
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle The monopole and quadrupole moments of the Epoch of Reionization (EoR) 21-cm bispectrum
Gill, Sukhdeep Singh
Pramanick, Suman
Bharadwaj, Somnath
Shaw, Abinash Kumar
Majumdar, Suman
Cosmology and Nongalactic Astrophysics
We study the monopole ($\bar{B}^0_0$) and quadrupole ($\bar{B}^0_2$) moments of the 21-cm bispectrum (BS) from EoR simulations and present results for squeezed and stretched triangles. Both $\bar{B}^0_0$ and $\bar{B}^0_2$ are positive at the early stage of EoR where the mean neutral hydrogen (HI) density fraction $\bar{x}_{\rm HI} \approx 0.99$. The subsequent evolution of $\bar{B}^0_0$ and $\bar{B}^0_2$ at large and intermediate scales $(k=0.29$ and $0.56 \, {\rm Mpc}^{-1}$ respectively) is punctuated by two sign changes which mark transitions in the HI distribution. The first sign flip where $\bar{B}^0_0$ becomes negative occurs in the intermediate stages of EoR $(\bar{x}_{\rm HI} > 0.5)$, at large scale first followed by the intermediate scale. This marks the emergence of distinct ionized bubbles in the neutral background. $\bar{B}^0_2$ is relatively less affected by this transition, and it mostly remains positive even when $\bar{B}^0_0$ becomes negative. The second sign flip, which affects both $\bar{B}^0_0$ and $\bar{B}^0_2$, occurs at the late stage of EoR $(\bar{x}_{\rm HI} < 0.5)$. This marks a transition in the topology of the HI distribution, after which we have distinct HI islands in an ionized background. This causes $\bar{B}^0_0$ to become positive. The negative $\bar{B}^0_2$ is a definite indication that the HI islands survive only in under-dense regions.
title The monopole and quadrupole moments of the Epoch of Reionization (EoR) 21-cm bispectrum
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2310.15579