Showing posts with label Big Bang. Show all posts
Showing posts with label Big Bang. Show all posts

Friday, May 24, 2019

3253. New Research Suggests that the Big Bang Occurred 12.5 Billion Years Ago

By Corey S. Powell, NBC News, May 18, 2019

A ground-based telescope's view of the Large Magellanic Cloud


Studies of star clusters in a neighboring galaxy (inset) add to the evidence that the universe is younger and faster-expanding than expected.Space Telescope Science Institute Office of Public Outreach / NASA, ESA, A. Reiss (STScI/JHU)
We've all lost track of time at one point or another, but astronomers really go all in. Recent studies show they may have overestimated the age of the universe by more than a billion years — a surprising realization that is forcing them to rethink key parts of the scientific story of how we got from the Big Bang to today.

The lost time is especially vexing because, in a universe full of mysteries, its age has been viewed as one of the few near-certainties. By 2013, the European Planck space telescope's detailed measurements of cosmic radiation seemed to have yielded the final answer: 13.8 billion years old. All that was left to do was to verify that number using independent observations of bright stars in other galaxies.

Then came an unexpected turn of events.

A few teams, including one led by Nobel laureate Adam Riess of the Space Telescope Science Institute in Baltimore, set out to make those observations. Instead of confirming Planck's measurements, they started getting a distinctly different result.

"It was getting to the point where we say, 'Wait a second, we're not passing this test — we're failing the test!'" says Riess, co-author of a new paper about the research to be published in Astrophysical Journal.

He estimates that his results, taken at face value, indicate a universe that is only 12.5 billion to 13 billion years old.


At first, the common assumption was that Riess and the other galaxy-watchers had made a mistake. But as their observations continued to come in, the results didn't budge.

Reanalysis of the Planck data didn't show any problems, either.

If all the numbers are correct, then the problem must run deeper. It must lie in our interpretation of those numbers — that is, in our fundamental models of how the universe works. "The discrepancy suggests that there's something in the cosmological model that we're not understanding right," Riess says. What that something could be, nobody knows.

Discovery of the dawn of time


The current discrepancy traces its origin way back to 1929, when astronomer Edwin Hubble discovered that galaxies are fleeing from Earth in all directions. More shocking, Hubble found that the farther away the galaxies are, the faster they're moving apart. That pattern means they're all fleeing from each other as well. "The only way all of this can be true is if space is expanding," Riess says.

If the idea of an expanding universe seems bizarre to you, welcome to the club.
"It's still bizarre to me, too," Riess says. "But that's what all of the data show, and that's what our theory predicts." Even Hubble never fully accepted the implications of his own work.
An expanding universe implies that the universe has a definite age, because you can retrace the action back to a time when everything in the cosmos was crammed together in an extremely dense, hot state: what we call the Big Bang.



"This is another hard concept for people to get their heads around," University of Chicago cosmologist Wendy Freedman said, adding that the Big Bang didn't go off like a kind of bomb. "The Big Bang is an explosion of space, not into space," she said.

In other words, galaxies are not flying away from each other through space. Space itself is stretching between them, and it has been ever since the Big Bang. So it's meaningless to ask where the Big Bang occurred. It occurred everywhere. As Freedman puts it, "There is no center or edge to the explosion."

But in the expanding universe, there is a beginning of time — at least, time as we know it. 

By measuring the rate at which galaxies are moving apart, astronomers realized, they could figure out the moment when the cosmos blinked into existence. All they had to do is figure out how to get their galactic measurements exactly right.

Clocking the cosmos


Freedman has been working on that problem for more than three decades, far longer than she ever expected. "This is an incredible challenge," she says. "Imagine making measurements out to hundreds of millions of light years to 1-percent accuracy!"

Hubble himself flubbed the test. His original calculations implied a universe younger than Earth, because he had drastically underestimated the distances to other galaxies.

The difficulty of making direct observations of other galaxies is one of the reasons why scientists created the Planck space telescope. It was designed to detect radiation left over from the Big Bang. The pattern of that radiation indicates the exact physical state of the early universe, if you know how to decode it. In principle, then, the Planck readings should tell us everything we want to know about what the universe is made of, and how old it is.

Planck has been a resounding success, pinning hard numbers onto the soft riddles of the cosmos. It indicated that 26 percent of the universe consists of dark matter, invisible material that helps hold galaxies together. It also confirmed the surprise discovery that the universe is dominated by dark energy, an unknown force that permeates all of empty space. (The detection of dark energy is what earned Riess a shared 2011 Nobel Prize.)

The likely implication of these findings is that the universe will keep expanding forever, faster and faster, into an ever-deeper darkness. It's an uncomfortable thought, one that Riess would rather not dwell on: "The scale of time is so beyond that of humanity, I don't think of it in human terms."
Most satisfying, perhaps, Planck finally completed the job that Hubble began, determining how quickly the universe is expanding and how long it has been around. Or so it seemed.

Something big is missing


Fortunately, Freedman and Riess and their colleagues didn't give up on their alternate approach to determining the age of the universe. They kept improving their observations, and are now getting close to that ambitious target of 1 percent accuracy. Which brings us to the current dispute — what the scientists politely refer to as "the tension."

The latest galaxy studies indicate an expansion rate about 9 percent faster than the answer from Planck. That might not sound like much of a disagreement, but over cosmic history it adds up to that full billion years of lost time.

Given the stakes, everyone involved is checking and rechecking their results for possible sources of error. Increasingly, though, it looks like the problem lies not with the observations but with the theories of cosmology that underpin them. If those theories are wrong or incomplete, the interpretation of the Planck readings will be flawed, too.

"There's currently no consistent story that works for all our cosmological data," says Princeton University astrophysicist Jo Dunkley, who has extensively analyzed the Planck results. "That means there is fascinating work to be done, to see if there is something out there that can explain all of it."

The "tension" reminds scientists of just how much they still don't understand about the underlying laws of nature. Dunkley points to the ghostly particles known as neutrinos, which are extremely abundant throughout space. "We measure neutrinos in the lab and put them in our cosmological model assuming that they are behaving just as we expect them to, but we simply don't know if that's true," she says. "I wouldn't find it surprising if dark matter turned out to be more complicated than we think, too."

Then there's the enigma of dark energy. "We have no good ideas for what it is. Perhaps there are also elements completely missing from the model side, still to be discovered," Freedman says. Theorists have no shortage of ideas: new types of dark energy, new fields, new particles.
Figuring out which explanation is correct — if any — will require another vast improvement in how we measure what the universe is actually doing. Freedman isn't coy about the magnitude of our ignorance: "The question is, what do we have yet to learn? I'd love to come back in a hundred or a thousand years and find out!"

Wednesday, February 18, 2015

1740. Unlocking the Mystery of the First Billion Years of the Universe

By Steven Tingay, The Conversation, February 17, 2015

More than 100 million years has been wiped off the age of the first stars but there is still the question of what happened in the first billion years of the universe.
Earlier this month the European Space Agency’s Planck mission team announced that the first stars formed some 560 million years after the Big Bang.
This is approximately 140 million years later than previously thought. It is an interesting result because it helps us to understand how structures such as stars and galaxies formed and evolved after the Big Bang.
The Planck team were studying the Cosmic Microwave Background (CMB), the radiation left over from the Big Bang, the origin of our universe. The CMB can be traced to events that occurred only approximately 380,000 years after the Big Bang.


Polarisation of the Cosmic Microwave Background across the sky, the latest data from the ESA Planck mission. ESA and the Planck CollaborationCC BY
Click to enlarge

Since the CMB discovery about 50 years ago, astrophysicists have been analysing it to better understand the early evolution of our universe, accurately measure its age (approximately 13.8 billion years) and help us realise that the laws of physics do not properly describe approximately 95% of the universe that we live in.
A short time after the Big Bang, almost all the ordinary matter created took the form of protons and electrons that, after 380,000 years, settled into hydrogen atoms (each atom is one proton and one electron bound together). Hydrogen is the simplest atom possible and the basic building block for everything we humans can see and touch in the universe (ordinary matter).
The Planck result means that over the first 560 million years, under the influence of gravity, this hydrogen gas collapsed into stars.
Inside stars, hydrogen atoms get combined into helium, oxygen, nitrogen, carbon and other elements. These elements end up in new stars, planets, oceans, DNA, iron ore deposits and so on. Quite useful stuff for humans. Stars really are the engines of life.

What happened next?

But we currently know little about what happened after the first stars formed. If we fast forward the universe 500 million years, we know that galaxies were forming, because we can see a few of them, such as UDFy-38135539, at the limits of powerful telescopes such as the Hubble Space Telescope.
If we fast forward again, another few billion years, the universe looks a lot like it does now, 13.8 billion years after the Big Bang.
So how exactly did the universe go from hydrogen, to stars, to galaxies and to life?


A Spitzer Space Telescope image of Messier 81, a spiral galaxy something like what our galaxy, the Milky Way, might look like if seen from the outside. Such a galaxy would contain billions of stars. NASA/JPL-Caltech/S. Willner (Harvard-Smithsonian Center for Astrophysics)
Click to enlarge

Planck has narrowed things down for us with an exciting result – no stars before about 560 million years, and the universe is starting to look vaguely familiar roughly 500 million years after that.
But those first billion years remain the last great unexplored period in the evolution of our universe (aside from the future of the universe).
So how do we go about uncovering these mystery years of the early universe? Even powerful telescopes such as Hubble cannot examine the formation of the first stars as they are too distant and faint, and stars do not produce visible light until they turn on.

Radio astronomy holds the key to the early universe

Happily, astronomers have a different and powerful set of tools to crack this nut. Atoms of hydrogen emit radio waves with a specific wavelength of 21cm (similar wavelength to what your mobile phone uses).
The hydrogen formed in the early universe produced these radio waves. By the time the radio waves travel all the way to us on Earth, through an expanding universe, they change their wavelength from 21cm to several metres (similar wavelength to what your FM radio uses).
If we can “tune in” to the radio waves, we can watch what the hydrogen gas is doing in the early universe, 100 million, 200 million, 500 million or a billion years after the Big Bang.
We can watch how the hydrogen gas forms into stars, how the stars are distributed, how long they take to form, how much energy they produce, and how galaxies start to form.
As the stars turn on, their radiation breaks apart the surrounding hydrogen atoms, leaving a “Swiss cheese” pattern (see below) in the radio emitting gas for astronomers to detect and analyse.


The Big Bang is at the left of this diagram. We live in a galaxy at the right of the diagram, 13.8 billion years after the Big Bang. NASA/CXC/SAO
Click to enlarge

Facilities in Australia are at the forefront

This is a challenge that astronomers are now embracing, by building massive telescopes capable of collecting these radio waves, such as the Murchison Widefield Array (MWA).
The MWA is located in the middle of Murchison Shire in Western Australia, well away from sources of human-made radio wave interference (mobile phones, microwave ovens, FM radio stations and cars) where we can pick up these faint radio whispers from the early universe.
Over the past two years, we have used the MWA to collect 4 petabytes of data (the equivalent of over 5,700 hours of full HD video) and have produced more than 50 scientific papers from the data already.


Part of the Murchison Widefield Array radio telescope, Western Australia. Curtin University
Click to enlarge

Our data are stored at the Pawsey supercomputer centre in Perth and we are sifting carefully through them using millions of supercomputer hours to obtain the first hints of the formation of the first stars and galaxies.
Competition to make the first detection of these radio signals comes from other telescopes in the USThe Netherlands and South Africa. So unlocking the mysteries of the first billion years of the universe is a big scientific prize.
But the MWA is only the first step needed to fill the gaps that Planck has so elegantly defined. A much larger radio telescope is needed, and that’s where the Square Kilometre Array (SKA) comes in.
The MWA is a A$50-million science and engineering precursor for the SKA, specifically the low frequency SKA, which will be approximately 100 times bigger than the MWA.
The SKA, when it’s switched on sometime in the next decade, will fill in the first billion year gap in detail and help us understand how the universe transformed from hydrogen gas into us. The MWA is designed to light the trail for the SKA.


Part of what the low frequency SKA may look like in the future. Hundreds of thousands of simple low frequency antennas spread over 10s of kilometres of the Western Australian outback.SKA/Curtin University/LFAA consortium/Swinburne University of Technology
Click to enlarge

The great news for Australia is that this much bigger SKA facility will be built on the same site as the MWA, in Western Australia, learning from our solid and hard won experience, placing Australian science and engineering on page one of the next exciting multi-decade chapter in the unfolding story of cosmic discovery

Steven Tingay is professor of Radio Astronomy at Curtin University, Australia.