dark age
(dark ages)
(interval when the universe's hydrogen atoms were neutral)
In cosmology, the dark age is the time between recombination
(when ions and electrons formed neutral hydrogen atoms,
around 380,000 years after the Big Bang or a redshift of 1090)
and the formation of stars and galaxies (around redshift 20,
producing light),
a point in time sometimes called the cosmic dawn.
During the dark ages, atoms were neutral and space was transparent but
without stars, all was relatively dark.
The cosmic dawn was essentially the beginning of the epoch of reionization,
the latter when ionizing radiation from stars again
ionized hydrogen atoms in large numbers,
150 million years after the Big Bang, the ionization occurring from
redshift 20 to redshift 6.
(Big Bang,cosmology,hydrogen,ionization,early universe,recombination,EOR)
Further reading:
https://en.wikipedia.org/wiki/Chronology_of_the_universe#Dark_Ages
https://ui.adsabs.harvard.edu/abs/2003Sci...300.1904M/abstract
https://www.space.com/13368-universe-dark-ages-survival-cosmos-evolution.html
https://eeyore.astro.illinois.edu/~lwl/classes/astro122/spring06/Lectures/lecture28.pdf
Redshift | Parsecs /Distance | Lightyears /Lookback Years | | |
20 | 4.27Gpc | 13.91Gly | nearest | dark age |
1090 | 4.29Gpc | 13.98Gly | furthest | dark age |
|
Referenced by pages:
epoch of reionization (EOR)
FARSIDE
LEDA
OVRO-LWA
recombination
Index