Tag: dark energy

  • Einstein’s theories tested on the largest scale ever – he was right

    Einstein’s theories tested on the largest scale ever – he was right

    [ad_1]

    The DESI instrument observing the sky from the Nicholas U. Mayall Telescope during a meteor shower

    KPNO/NOIRLab/NSF/AURA/R. Sparks

    Albert Einstein’s theory of general relativity has been proven right on the largest scale yet. An analysis of millions of galaxies shows that the way they have evolved and clustered over billions of years is consistent with his predictions.

    Ever since Einstein put forward his theory of gravity more than a century ago, researchers have been trying to find scenarios where it doesn’t hold up. But there had not been such a test at the level of the largest distances in the universe until now, says Mustapha Ishak-Boushaki at the University of Texas at Dallas. He and his colleagues used data from the Dark Energy Spectroscopic Instrument (DESI) in Arizona to conduct one.

    Details of cosmic structure and how it has changed over time are a potent test of how well we understand gravity because it was this force that shaped galaxies as they evolved out of the small variations in the distribution of matter in the early universe.

    DESI has so far collected data on how nearly 6 million galaxies clustered over the course of the past 11 billion years. Ishak-Boushaki and his colleagues combined this with results from several other large surveys, such as those mapping the cosmic microwave background radiation and supernovae. Then, they compared this with predictions from a theory of gravity that encompassed both Einstein’s ideas and more contemporary competing theories of modified gravity. They found no deviation from Einstein’s gravity. Ishak-Boushaki says that even though there are some uncertainties in the measurements, there is still no strong evidence that any theory that deviates from Einstein’s would capture the state of the universe more accurately.

    Itamar Allali at Brown University in Rhode Island says that while general relativity has been shown to hold in extremely precise tests conducted in laboratories, it is important to be able to test it at all scales, including across the entire cosmos. This helps eliminate the possibility that Einstein made correct predictions for objects of one size but not another, he says.

    The new analysis also offers hints for how dark energy, a mysterious force thought to be responsible for the accelerating expansion of the universe, fits within our theories of gravity, says Nathalie Palanque-Delabrouille at Lawrence Berkeley National Laboratory in California. Einstein’s earliest formulations of general relativity included a cosmological constant – a kind of anti-gravitational force that played the same role as dark energy – but previous DESI results have suggested that dark energy isn’t constant. It may have changed as the universe aged, says Palanque-Delabrouille.

    “The fact that we see agreement with [general relativity] and still see this departure from the cosmological constant really open the Pandora’s box of what the data could actually be telling us,” says Ishak-Boushaki.

    DESI will keep collecting data for several more years and ultimately record the positions and properties of 40 million galaxies, which the three scientists all say will bring clarity on how to correctly marry general relativity and theories of dark energy. This new analysis only used one year of DESI’s data, but in March 2025 the team will share takeaways from the instrument’s first three years of observations.

    Allali says he is anticipating these results to be consequential in several important ways, such as pinpointing shifts in the Hubble constant, which is a measure of the rate of the universe’s expansion, narrowing down the mass of elusive particles called neutrinos and even searching for new cosmic ingredients like “dark radiation”.

    “This analysis will weigh in on a lot more than gravity, it will weigh in on all of cosmology,” he says.

    Topics:

    [ad_2]

    Source link

  • First breathtaking images from Euclid telescope’s map of the universe

    First breathtaking images from Euclid telescope’s map of the universe

    [ad_1]

    New Scientist. Science news and long reads from expert journalists, covering developments in science, technology, health and the environment on the website and the magazine.

    The interaction between two distant galaxies, captured by Euclid

    ESA

    A mosaic of images from the European Space Agency’s Euclid space telescope captures more than 14 million galaxies, offering a first glimpse of a “cosmic atlas”. The mapping project could add to our understanding of the role dark matter and dark energy play in the structure of the universe.

    “The scale is utterly incomprehensible,” Carole Mundell, the director of science at the ESA, said at a meeting of the International Astronautical Congress in Italy on 15 October. Representing the image at full resolution would require more than 16,000 4K TV screens, she said.

    New Scientist. Science news and long reads from expert journalists, covering developments in science, technology, health and the environment on the website and the magazine.

    Euclid’s first mosaic image represents only 1 per cent of the final map

    ESA

    The mosaic of 260 images is the first glimpse into Euclid’s project to create the largest and most accurate map of the universe yet. The vast number of galaxies was captured during a two-week survey in April and represents only 1 per cent of the final map. The image covers an area of the southern sky about 500 times the size of the full moon.

    The wispy blue band across the image is dust and gas in the nearby Milky Way, known as “galactic cirrus”, said Mundell. Zooming in reveals swirling galaxies interacting hundreds of millions of light years away, some with a supermassive black hole at their centre that can produce gravitational waves measurable on Earth.

    Over the next six years, the telescope will autonomously scan about a third of the night sky. The researchers anticipate the final map will show around 8 billion galaxies, each with billions of stars, stretching across 10 billion years of cosmic history.


    By observing clusters of galaxies and other phenomena, such as how gravity bends light, “Euclid will measure the cosmic web – the distribution of matter in space and time”, said the ESA’s Valeria Pettorino at the meeting. Because dark energy and dark matter affect the formation of voids between clusters of galaxies, measuring these voids could help us understand the characteristics of these elusive substances, she said.

    “We’re testing the fundamental laws of physics at the extreme scales of the cosmos,” said Mundell.

    Topics:

    [ad_2]

    Source link

  • Gravitational waves: We are about to hear echoes in the fabric of space for the first time

    Gravitational waves: We are about to hear echoes in the fabric of space for the first time

    [ad_1]

    New Scientist Default Image

    Did  you hear the one about the star that died twice? In 2014, astronomers saw the explosion of the Refsdal supernova. Then, 360 days later, it went bang again.

    This bizarre sequence of events was down to a phenomenon called gravitational lensing, in which massive objects warp the fabric of space enough to cause light to bend. The path of the flash from the supernova was changed in this way on its journey to us, so that portions of it took different routes and arrived at different times – almost a year apart in this extreme case.

    As that story shows, gravitational lensing has been around for a while, but now it is about to enter a compelling new chapter. Scientists know it isn’t just light that can be lensed, but gravitational waves too. It is a mind-bending concept: ripples in space-time themselves being distorted by the curvature of space. It is also a deeply important phenomenon that could illuminate the secret interiors of neutron stars, settle a mystery about the power of dark energy and test gravity itself more keenly than ever. And here is the best part: we may be on the cusp of spotting our first lensed gravitational wave.

    No one is under any illusions that this will be anything other than fiendishly difficult. Still, there is a sense it will happen sooner or later – and there are tricks we can pull to expedite the discovery. “It’s exciting, and it’s going to happen,” says Simon Birrer at Stony Brook University in New York. “There’s…

    [ad_2]

    Source link

  • Invisible ‘dark radiation’ may explain a big problem with dark energy

    Invisible ‘dark radiation’ may explain a big problem with dark energy

    [ad_1]

    A slice through the largest 3D map of our universe to date

    A slice through the largest 3D map of our universe to date

    laire Lamman/DESI collaboration

    There are hints that the universe may be behaving unexpectedly, and astrophysicists are racing to explain why. Their ideas to account for the surprising result include allowing dark matter and dark energy to interact, and arguing for the existence of strange “dark radiation” that is similar in nature to regular light but invisible.

    In April, researchers using the Dark Energy Spectroscopic Instrument (DESI) in Arizona released the biggest 3D map of the universe ever created, and it hinted…

    [ad_2]

    Source link

  • The Mysterious ‘Dark’ Energy That Permeates the Universe Is Slowly Eroding

    The Mysterious ‘Dark’ Energy That Permeates the Universe Is Slowly Eroding

    [ad_1]

    Beyond DESI, a slew of new instruments are coming online in the coming years, including the 8.4-meter Vera Rubin Observatory in Chile, NASA’s Nancy Grace Roman Space Telescope, and the European Space Agency’s Euclid mission.

    “Our data in cosmology has made enormous leaps over the last 25 years, and it’s about to make bigger leaps,” Frieman said.

    As they amass new observations, researchers may continue to find that dark energy appears as constant as it has for a generation. Or, if the trend continues in the direction suggested by DESI’s results, it could change everything.

    New Physics

    If dark energy is weakening, it can’t be a cosmological constant. Instead, it may be the same sort of field that many cosmologists think sparked a moment of exponential expansion during the universe’s birth. This kind of “scalar field” could fill space with an amount of energy that looks constant at first—like the cosmological constant—but eventually starts to slip over time.

    “The idea that dark energy is varying is very natural,” said Paul Steinhardt, a cosmologist at Princeton University. Otherwise, he continued, “it would be the only form of energy we know which is absolutely constant in space and time.”

    But that variability would bring about a profound paradigm shift: We would not be living in a vacuum, which is defined as the lowest-energy state of the universe. Instead, we would inhabit an energized state that’s slowly sliding toward a true vacuum. “We’re used to thinking that we’re living in the vacuum,” Steinhardt said, “but no one promised you that.”

    The fate of the cosmos would depend on how quickly the number previously known as the cosmological constant declines, and how far it might go. If it reaches zero, cosmic acceleration would stop. If it dips far enough below zero, the expansion of space would turn to a slow contraction—the sort of reversal required for cyclic theories of cosmology, such as those developed by Steinhardt.

    String theorists share a similar outlook. With their proposal that everything boils down to the vibration of strings, they can weave together universes with different numbers of dimensions and all manner of exotic particles and forces. But they can’t easily construct a universe that permanently maintains a stable positive energy, as our universe has seemed to. Instead, in string theory, the energy must either gently fall over the course of billions of years or violently drop to zero or a negative value. “Essentially, all string theorists believe that it’s one or the other. We do not know which one,” said Cumrun Vafa of Harvard University.

    Observational evidence for a gradual decline of dark energy would be a boon for the gentle-fall scenario. “That would be amazing. It would be the most important discovery since the discovery of dark energy itself,” Vafa said.

    But for now, any such speculations are rooted in the DESI analysis in only the loosest of ways. Cosmologists will have to observe many millions more galaxies before seriously entertaining thoughts of revolution.

    “If this holds up, it could light the way to a new, potentially deeper understanding of the universe,” Riess said. “The next few years should be very revealing.”


    Original story reprinted with permission from Quanta Magazine, an editorially independent publication of the Simons Foundation whose mission is to enhance public understanding of science by covering research developments and trends in mathematics and the physical and life sciences.

    [ad_2]

    Source link

  • There are hints that dark energy may be getting weaker

    There are hints that dark energy may be getting weaker

    [ad_1]

    A slice of the largest 3D map of the universe showing the underlying structure of matter

    laire Lamman/DESI collaboration; custom colormap package by cmastro

    The largest 3D map of the universe ever created is providing hints about the evolution of the cosmos, and they suggest that we may be wrong about the behaviour of dark energy, which makes up most of the universe. It seems that this mysterious force may be weakening over time.

    “If it holds up, this is a very big deal,” says Adam Riess at Johns Hopkins University in Maryland, who found the first evidence for dark energy 25 years ago. That is because the standard model of cosmology, called lambda-CDM, suggests that the strength of dark energy should be static over time.

    Dark energy is thought to cause the accelerating expansion of the cosmos – if it is not static, that could also have huge implications for our ideas about the beginning of the universe, its size and its ultimate fate. Reiss, who was not involved in the new work, says the implications could mean “we will have to do some serious soul-searching regarding [our understanding of] gravity and fields”.

    The strange findings come from the Dark Energy Spectroscopic Instrument (DESI) in Arizona – and even DESI collaborators are not quite sure what to make of the fact that their data suggests dark energy may have recently gotten weaker. “It’s all we’ve been talking in the collaboration about for months… whether this is interesting or not,” says DESI spokesperson Kyle Dawson at the University of Utah.

    DESI researchers examined the strength of dark energy by measuring the large-scale structure and distribution of galaxies in the cosmos, which illuminates how the universe has expanded over time. The researchers then combined this information with three sets of data on supernovae, which act as so-called “standard candles” to determine the distances to cosmic objects thanks to their predictable brightnesses.

    Surprisingly, each of the three samples of supernovae yielded a different answer to the change in the universe’s rate of expansion over time. All three suggested that the effects of dark energy may have decreased in recent aeons, but the strength of these suggestions varied, so researchers are not quite sure how to interpret the data.

    “Two of the supernova samples disagree with each other, and they’re very, very similar samples,” says Dawson. “I don’t know which one’s right, it’s possible that the truth lies in between, but it really looks like the differences lie in the way [the supernova researchers] evaluated the data.”

    Discrepancies in models are denoted by a factor called sigma, which measures the likelihood that a similar clash could have happened by chance if the models did disagree with one another. “About 3-sigma is the level we usually sit up and pay attention and call an ‘indication’ of something,” says Riess. Anything lower than that would not generally be particularly exciting to researchers – it would be too likely to be a simple coincidence.

    The discrepancies between lambda-CDM and the combination of supernova and DESI measurements ranged from 2.5-sigma to 3.9-sigma. “Both statements are true: it is sufficient tension, it’s interesting; and it’s not sufficient tension to say that anything is definitely there,” says Dawson.

    Dark energy makes up nearly 70 per cent of the universe, so any error in our understanding of its nature could have widespread impacts on physics. Proving whether that error is really there, though, will take more precise measurements in the coming years.

    “If [this is] true, it would be the first real clue we have gotten about the nature of dark energy in 25 years,” says Riess.

    Topics:

    [ad_2]

    Source link