Recognizing the First Radiation Sources Through Their 21-cm Signature
arXiv:astro-ph/0605511 · doi:10.1086/507626
Abstract
At the beginning of the reionization epoch, radiation sources produce fluctuations in the redshifted 21-cm background. We show that different types of sources (such as miniquasars, Pop II and III stars, supernovae, etc.) produce distinct signatures in the 21-cm signal radial profiles and statistical fluctuations, through which they can be identified. Further, we show that the 21-cm signal from X-ray emitting sources is much easier to observe than was expected, due to a previously neglected pumping mechanism.
4 pages, 4 figures, accepted by ApJL
Cited by in corpus (37)
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- 21 cm fluctuations from inhomogeneous X-ray heating before reionization
- Evolution of the 21 cm signal throughout cosmic history
- Constraining the unexplored period between reionization and the dark ages with observations of the global 21 cm signal
- What does the first highly-redshifted 21-cm detection tell us about early galaxies?
- The Global 21-cm Signal in the Context of the High-z Galaxy Luminosity Function
- The Effects of Dark Matter Decay and Annihilation on the High-Redshift 21 cm Background
- The Epoch of Reionization
- Secondary ionization and heating by fast electrons
- 21 cm signal from cosmic dawn: Imprints of spin temperature fluctuations and peculiar velocities
- The Physics and Early History of the Intergalactic Medium
- Decoding the X-ray Properties of Pre-Reionization Era Sources
- Time-evolution of ionization and heating around first stars and miniquasars
- Spin Exchange Rates in Electron-Hydrogen Collisions
- Imaging the redshifted 21-cm pattern around the first sources during the cosmic dawn using the SKA
- Unique Signatures of Population III Stars in the Global 21-cm Signal
- Current models of the observable consequences of cosmic reionization and their detectability
- Influence of primordial magnetic fields on 21 cm emission
- Heating of the Intergalactic Medium by Primordial Miniquasars
- Spin Exchange Rates in Proton-Hydrogen Collisions
- Impact of Dark Matter Annihilation on the High-Redshift Intergalactic Medium
- Spatially Extended 21 cm Signal from Strongly Clustered UV and X-Ray Sources in the Early Universe
- Detecting Early Galaxies Through Their 21-cm Signature
- Radiative Transfer Effect on Ultraviolet Pumping of the 21cm Line in the High Redshift Universe
- On the spin-temperature evolution during the epoch of reionization
- Time evolution of Wouthuysen-Field coupling
- Enhanced Detectability of Pre-reionization 21-cm Structure
- A WENO algorithm for radiative transfer with resonant scattering: the time scale of the Wouthuysen-Field Coupling
- Probing the growth of supermassive black holes at z>6 with LOFAR
- 21 cm Signals from Early Ionizing Sources
- A practical theorem on using interferometry to measure the global 21-cm signal
- Lensing of 21cm Absorption "Halos" of 20-30 First Galaxies
- The Infancy of Cosmic Reionization
- Luminosity Bias (II): The Cosmic Web of the First Stars