Brilliant Beams of Quasars Provide a Light Map to Trace Growth and Evolution of the Universe

 

          

 

Astronomers have found a possible way to map the spread and structure of the universe, guided by the light of quasars. The technique, combined with the expected discovery of millions more far-away quasars over the next decade, could yield an unprecedented look back to a time shortly after the Big Bang, when the universe was a fraction the size it is today.

Researchers found the key while analyzing the visible light from a small group of quasars. Patterns of light variation over time were consistent from one quasar to another when corrected for the quasar's redshift. This redshift occurs because an expanding universe carries the quasars away from us, thus making the light from them appear redder (hence the term), and also making the time variations appear to occur more slowly.

Turning this around, by measuring the rate at which a quasar's light appears to vary and comparing this rate to the standard rate at which quasars sampled actually vary, the researchers were able to infer the redshift of the quasar.

Knowing the quasar redshift enables the scientists to calculate the relative size of the universe when the light was emitted, compared to today. "It appears we may have a useful tool for mapping out the expansion history of the universe," said Glenn Starkman, a physics professor at Case Western Reserve and an author of the study, published this summer in Physical Review Letters.

"If we could measure the redshifts of millions of quasars, we could use them to map the structures in the universe out to a large redshift." The larger the redshift, the farther and older the light source. The group plans to seek larger samples of quasars, to confirm the patterns are consistent and can be used to calculate their redshifts everywhere across the universe. The work was led by De-Chang Dai, who earned his PhD working with Starkman and was most recently a member of the Astrophysics, Cosmology and Gravity Centre, University of Cape Town.

The scientists graphed the amount of light from 14 quasars recorded by the Massive Compact Halo Objects project, which sought evidence of dark matter in and around the Milky Way. Light from each quasar was measured repeatedly over hundreds of days. Graphing revealed phases during which the amount of light would either increase or decrease in a linear fashion over an extended period of time. Although other properties varied, the rate at which the measurable light changed was nearly identical among all 14 quasars, once scientists corrected for the effects of the universe's expansion.

"It's as if there was a dimmer switch on them with someone turning it to the left then the right," Starkman said. "The overall trend was surprisingly consistent." This consistency of patterns enabled the scientists to accurately calculate the cosmological redshift of one quasar from another. The researchers tested this capability in two ways. They fit segments of the light curves, that is, the measured light over time, to straight lines. The slopes of the lines were consistent and appeared to be directly related to the quasars' redshifts. By comparing corresponding slopes of 13 quasars with a known redshift value to the slopes of one other quasar, the researchers could calculate the redshift of the lone quasar within two percentage points.

In a second approach, the researchers took large sections of the light curves of two quasars and concentrated on the segments that matched most closely. By varying the ratio of the redshifts of the two quasars to try to get the best possible match of the two light curves, they were able to determine the ratio of the quasars' redshifts to within 1.5 percentage points.

Astronomers have used the bright light of supernovae with redshifts up to about 1.7 to measure the accelerating expansion of the universe. A star with a redshift of 1.7 would have been emitting that light when the universe was 2.7 times smaller than today. Quasars are older and farther away and have been measured with redshifts of up to 7.1, which means they emitted the light we are seeing when the universe was as small as one-eighth the size it is today. If this method of determining quasar redshifts proves applicable to higher redshift quasars, scientists could have millions of markers to trace the growth and evolution of structure and the expansion of the universe out to large distances and early times.

"This could help us learn about how gravity has assembled structure in the universe." Starkman said. "And, the rate of structure growth can help us determine whether dark energy or modified laws of gravity drive the accelerated expansion of the universe."

Journal reference: Physical Review Letters.

The Daily Galaxy via Case Western Reserve University.

Comments

[yas hart]

Draw 2 diagonal lines to divide 4 spaces, at such a way so, space A in reverse to B, and space C in reverse to D.
I want a bet, all extremely highest redshift quasars only exist at space A and B, whilst at space C & D only contain moderate redshift quasars. All quasars at space C & D will head for space A and B. At space A they are distributed at around 1 small post, while at space B, they are distributed at around 2 large areas.
If your cosmological observation shows to be like that, we can talk. If not, just forget me.

[Suc Iyant]

Yas Hart, on above comment, has made mistakes.
Cosmos must look like this: Watched from MW, all quasars at entire cosmos redshift, under condition:

1. There is region at cosmos where highest redshift quasars, scattering around that region, vanish. That event happens repeatedly. Name center of that region N. Before they vanish, those quasars get closer to one another.

2. We will observe highest redshift quasars, scattering at entire cosmos (excluded region around N), vanish or construct galaxies. That event happens repeatedly. Before they vanish or construct galaxies, those quasars recede from one another.

3. We at MW will frequently watch a unique event. Scattered at ball surface with diameter MW-N, quasars occur from emptiness, and then each quasar splits into 2 quasars. Then, the 2 quasars recede from one another. Throughout cosmos, that phenomenon only occurs at above ball surface, except at MW & around N.