Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7220
Title: Analytic Formulation of 21cm Signal from Cosmic Dawn: Lyα Fluctuations
Authors: Raste, Janakee
Sethi, S.K.
Keywords: cosmology
theory – dark ages
reionization
first stars
Issue Date: 1-May-2019
Publisher: IOP Sciences for The American Astronomical Society
Citation: Astrophysical Journal, 2019, Vol. 876, p17
Abstract: We present an analytic formalism to compute the fluctuating component of the H i signal and extend it to take into account the effects of partial Lyα coupling during the era of cosmic dawn. We use excursion set formalism to calculate the size distribution of randomly distributed self-ionized regions. These ionization bubbles are surrounded by partially heated and Lyα coupled regions, which create spin temperature T S fluctuations. We use the ratio of number of Lyα to ionizing photons (f L ) and number of X-ray photons emitted per stellar baryon (N heat) as modeling parameters. Using our formalism, we compute the global H i signal, its autocorrelation, and its power spectrum in the redshift range 10 ≤ z ≤ 30 for the ΛCDM model. We check the validity of this formalism for various limits and simplified cases. Our results agree reasonably well with existing results from N-body simulations, in spite of following a different approach and requiring orders of magnitude less computation power and time. We further apply our formalism to study the fluctuating component corresponding to the recent observation by the Experiment to Detect the Global Epoch of reionization Signature (EDGES) that shows an unexpectedly deep absorption trough in the global H i signal in the redshift range 15 < z < 19. We show that, generically, the EDGES observation predicts a larger signal in this redshift range but a smaller signal at higher redshifts. We also explore the possibility of negative real-space autocorrelation of spin temperature and show that it can be achieved for partial Lyα coupling in many cases corresponding to simplified models and a complete model without density perturbations.
Description: Open Access.
URI: http://hdl.handle.net/2289/7220
ISSN: 0004-637X
Alternative Location: https://ui.adsabs.harvard.edu/abs/2019ApJ...876...56R/abstract
https://arxiv.org/abs/1810.12746
https://doi.org/10.3847/1538-4357/ab13a6
Copyright: 2019, The American Astronomical Society
Appears in Collections:Research Papers (A&A)

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