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Title: Cosmic reionization on computers. Mean and fluctuating redshifted 21 CM signal

Journal Article · · The Astrophysical Journal (Online)
ORCiD logo [1];  [2]
  1. Univ. of Chicago, Chicago, IL (United States)
  2. Univ. of Chicago, Chicago, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

We explore the mean and fluctuating redshifted 21 cm signal in numerical simulations from the Cosmic Reionization On Computers project. We find that the mean signal varies between about ±25 mK. Most significantly, we find that the negative pre-reionization dip at z ~ 10–15 only extends to $$\langle {\rm{\Delta }}{T}_{B}\rangle \sim -25\,{\rm{mK}}$$, requiring substantially higher sensitivity from global signal experiments that operate in this redshift range (EDGES-II, LEDA, SCI-HI, and DARE) than has often been assumed previously. We also explore the role of dense substructure (filaments and embedded galaxies) in the formation of the 21 cm power spectrum. We find that by neglecting the semi-neutral substructure inside ionized bubbles, the power spectrum can be misestimated by 25%–50% at scales k ~ 0.1–1h Mpc–1. Furthermore, this scale range is of particular interest, because the upcoming 21 cm experiments (Murchison Widefield Array, Precision Array for Probing the Epoch of Reionization, Hydrogen Epoch of Reionization Array) are expected to be most sensitive within it.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
AC02-07CH11359
OSTI ID:
1275509
Report Number(s):
FERMILAB-PUB-15-493-A; arXiv:1510.08767; 1401347
Journal Information:
The Astrophysical Journal (Online), Vol. 824, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 5 works
Citation information provided by
Web of Science

References (32)

PAPER-64 CONSTRAINTS ON REIONIZATION: THE 21 cm POWER SPECTRUM AT z = 8.4 journal August 2015
EMMA: an adaptive mesh refinement cosmological simulation code with radiative transfer journal September 2015
Science with the Murchison Widefield Array journal January 2013
A lower limit of Δz > 0.06 for the duration of the reionization epoch journal December 2010
Probing the first stars and black holes in the early Universe with the Dark Ages Radio Explorer (DARE) journal February 2012
BRIGHT SOURCE SUBTRACTION REQUIREMENTS FOR REDSHIFTED 21 cm MEASUREMENTS journal November 2010
Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data journal January 2014
Empirical covariance modeling for 21 cm power spectrum estimation: A method demonstration and new limits from early Murchison Widefield Array 128-tile data journal June 2015
Low-mass galaxy formation and the ionizing photon budget during reionization journal August 2014
The Growth of H ii Regions During Reionization journal September 2004
Cosmic Reionization on Computers. i. Design and Calibration of Simulations journal September 2014
Cosmic Reionization on Computers. ii. Reionization History and its Back-Reaction on Early Galaxies journal September 2014
Redshifted 21 Centimeter Emission from the Pre‐Reionization Era. I. Mean Signal and Linear Fluctuations journal June 2004
MULTIREDSHIFT LIMITS ON THE 21 cm POWER SPECTRUM FROM PAPER journal March 2015
Cosmic Reionization on Computers. iii. the Clumping Factor journal September 2015
Starburst99: Synthesis Models for Galaxies with Active Star Formation
  • Leitherer, Claus; Schaerer, Daniel; Goldader, Jeffrey D.
  • The Astrophysical Journal Supplement Series, Vol. 123, Issue 1 https://doi.org/10.1086/313233
journal July 1999
Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array journal June 2008
THE IMPACT OF THE SUPERSONIC BARYON-DARK MATTER VELOCITY DIFFERENCE ON THE z ∼ 20 21 cm BACKGROUND journal October 2012
21cmfast: a fast, seminumerical simulation of the high-redshift 21-cm signal: 21cmfast journal November 2010
Reionization of the Inhomogeneous Universe journal February 2000
Probing the Ultraviolet Luminosity Function of the Earliest Galaxies with the Renaissance Simulations journal June 2015
NEW LIMITS ON 21 cm EPOCH OF REIONIZATION FROM PAPER-32 CONSISTENT WITH AN X-RAY HEATED INTERGALACTIC MEDIUM AT z = 7.7 journal May 2014
SARAS: a precision system for measurement of the cosmic radio background and signatures from the epoch of reionization journal April 2013
Saras Measurement of the Radio Background at long Wavelengths journal March 2015
PAPER-64 CONSTRAINTS ON REIONIZATION. II. THE TEMPERATURE OF THE z = 8.4 INTERGALACTIC MEDIUM journal August 2015
WHAT NEXT-GENERATION 21 cm POWER SPECTRUM MEASUREMENTS CAN TEACH US ABOUT THE EPOCH OF REIONIZATION journal January 2014
Evolution of the 21 cm signal throughout cosmic history journal November 2008
21 cm cosmology in the 21st century journal July 2012
BIGHORNS - Broadband Instrument for Global HydrOgen ReioNisation Signal journal January 2015
The Evolution of Lyman Limit Absorption Systems to Redshift six journal September 2010
THE IMPACT OF POINT-SOURCE SUBTRACTION RESIDUALS ON 21 cm EPOCH OF REIONIZATION ESTIMATION journal September 2012
PROBING THE DARK AGES AT z ∼ 20: THE SCI-HI 21 cm ALL-SKY SPECTRUM EXPERIMENT journal January 2014

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