Distant Metals reveal the Universe's evolution

When did the first sources of light bombard the universe's gas, tearing electrons from atoms in a period known as reionization? A new study uses the metal-filled gas surrounding galaxies to learn more about the important transition.

The study was published in the recent journal of American Astronomical Society.

After the universe's birth in the hot Big Bang, expansion and cooling allowed the soup of electrons and protons that pervaded space to recombine into neutral hydrogen atoms. But sometime within the first billion years after the Big Bang, these atoms were again ionized by high-energy radiation from the first sources of light in the universe.

How and when, exactly, did this period of reionization occur? One way we can seek to answer these questions is by studying the gas that lies both between and immediately around galaxies.

While the broadly dispersed intergalactic medium (IGM) consists largely of hydrogen gas, the circumgalactic medium (CGM) immediately around galaxies is a little more complicated: it's enriched with elements heavier than helium -- "metals" -- that have been produced by the galaxy's stars and flung into the surrounding matter.

Because this distant gas is diffuse and dim, we can't easily study its emission. Instead, we explore these clouds of gas by looking at how they absorb light from bright background sources.

In a new study led by George Becker (University of California, Riverside), a team of scientists has examined the spectra of nearly 200 background quasars -- bright, active galaxies -- with redshifts up to z = 6.6, corresponding to a time when the universe was less than a billion years old. Their goal: to explore the absorption by clouds of metal-enriched CGM that lie between us and the quasars.

Becker and collaborators looked for the signatures of several metals in these clouds, including neutral oxygen. From their sample, the authors were able to infer how absorbing clouds containing neutral oxygen are distributed over cosmic time between redshifts of 3.