Something isn't quite right in the universe. At least based on everything physicists know so far. Stars, galaxies, black holes and all the other celestial objects are hurtling away from each other ever faster over time. Past measurements in our local neighborhood of the universe find that the universe is exploding outward faster than it was in the beginning. That shouldn't be the case, based on scientists' best descriptor of the universe.
If their measurements of a value known as the Hubble Constant are correct, it means that the current model is missing crucial new physics, such as unaccounted-for fundamental particles, or something strange going on with the mysterious substance known as dark energy.[5 Elusive Particles Beyond the Higgs | Quantum Physics]
Now, in a new study, published Jan. 22 in the journal Monthly Notices of the Royal Astronomical Society, scientists have measured the Hubble Constant in an entirely new way, confirming that, indeed, the universe is expanding faster now than it was in its early days.
"Something interesting going on"
To explain how the universe went from a tiny, hot, dense speck of soupy plasma to the vast expanse we see today, scientists have proposed what's known as the Lambda Cold Dark Matter (LCDM) model. The model puts constraints on the properties of dark matter, a kind of matter that exerts gravitational pull but emits no light, and dark energy, which seems to oppose gravity. LCDM can successfully reproduce the structure of galaxies and the cosmic microwave background — the universe's first light — as well as the amount of hydrogen and helium in the universe. But it can't explain why the universe is expanding faster now than it did early on. [Big Bang to Civilization: 10 Amazing Origin Events]
That means that either the LCDM model is wrong or the measurements of expansion rate are.
The new method aims to finally settle the expansion-rate debate, Simon Birrer, a researcher at the University of California, Los Angeles, and lead author on the new study, told Live Science. So far, the new, independent measurements confirm the discrepancy, suggesting new physics may be needed.
To nail down Hubble's Constant, scientists had previously used several different methods. Some used supernovas in the local universe (the nearby part of the universe), and others have relied on Cepheids, or types of stars that pulsate and regularly flicker in brightness. Still others have studied the cosmic background radiation.
The new research used a technique that involves light from quasars — extremely bright galaxies powered by massive black holes — in an effort to break the tie.
"No matter how careful an experiment is, there can always be some effect that is built into the kinds of tools that they're using to make that measurement. So when a group comes along like this and uses a completely different set of tools… and gets the same answer, then you can pretty quickly conclude that that answer is not a result of some serious effect in the techniques," said Adam Riess, a Nobel laureate and researcher at the Space Telescope Science Institute and at Johns Hopkins University. "I think that our confidence is growing that there's something really interesting going on," Riess, who was not involved in the study, told Live Science.
Here's how the technique worked: When light from a quasar passes an intervening galaxy, gravity from the galaxy causes that light to "gravitationally bend" before hitting Earth. The galaxy acted like a lens to distort the quasar's light into multiple copies — most commonly two or four depending on the alignment of the quasars in relation to the galaxy. Each of those copies traveled a slightly different path around the galaxy.
Quasars don't usually shine steadily like many stars. On account of material falling into their central black holes, they change in brightness on scales of hours to millions of years. Thus, when a quasar's image is lensed into multiple copies with unequal light paths, any change in the brightness of the quasar will result in a subtle flickering between the copies, as light from certain copies takes a touch longer to reach Earth.
From this discrepancy, scientists could precisely determine how far we are from both the quasar and the intermediary galaxy. To calculate the Hubble Constant, astronomers then compared that distance to the object's redshift, or the shift in wavelengths of light toward the red end of the spectrum (which shows how much the object's light has stretched as the universe expands).
Studying light from systems that create four images, or copies, of a quasar has been done in the past. But, in the new paper, Birrer and his collaborators successfully demonstrated that it is possible to measure the Hubble Constant from systems that create just a double image of the quasar. This dramatically increases the number of systems that can be studied, which ultimately will allow the Hubble Constant to be measured more precisely.
"Images of quasars that appear four times are very rare — there are maybe only 50 to 100 across the whole sky, and not all are bright enough to be measured," Birrer told Live Science. "Doubly- lensed systems, however, are more frequent by about a factor of five."
The new results from a doubly-lensed system, combined with three other previously measured quadruple-lensed systems, put the value for the Hubble Constant at 72.5 kilometers per second per megaparsec; that's in agreement with other local universe measurements, but still around 8 percent higher than measurements from the distant universe (the older, or early, universe). As the new technique is applied to more systems, researchers will be able to home in on the exact difference between distant (or early) universe and local (more recent) universe measurements.
"The key is to go from a point where we're saying, yeah, these things don't agree, to having a very precise measure of the level to which they don't agree, because ultimately that will be the clue that allows theory to say what is going on," Riess told Live Science.
Accurately measuring the Hubble Constant helps scientists understand more than just how fast the universe is flying apart. The value is imperative in determining the age of the universe and the physical size of distant galaxies. It also gives astronomers clues as to the amount of dark matter, and dark energy, out there.
As for explaining what possibly exotic physics might explain their mismatch in expansion-rate measurements, that's way down the line.
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Originally published on Live Science.
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Mara Johnson-Groh is a contributing writer for Live Science. She writes about everything under the sun, and even things beyond it, for a variety of publications including Discover, Science News, Scientific American, Eos and more, and is also a science writer for NASA. Mara has a bachelor's degree in physics and Scandinavian studies from Gustavus Adolphus College in Minnesota and a master's degree in astronomy from the University of Victoria in Canada.