Latest findings from the South Pole Telescope bolster standard cosmological model

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A brand new research makes use of information collected by the South Pole Telescope, above, to deepen our understanding of how the universe was born and advanced. Credit score: Aman Chokshi

Roughly 400,000 years after the Large Bang, the universe cooled simply sufficient to permit photons to flee from the primordial cosmological soup. Over the subsequent 14 billion years, these historic photons—the universe’s first mild—continued touring. This relic mild is named the Cosmic Microwave Background.

In a brand new research, scientists used observational information of this primary mild—collected from the South Pole Telescope positioned on the Nationwide Science Basis’s Amundsen-Scott South Pole Station in Antarctica—to discover the theoretical underpinnings of the usual cosmological mannequin that describes the historical past of the universe over the previous 14 billion years.

The research was performed by UC Davis researchers and colleagues within the South Pole Telescope collaboration, which is led by the College of Chicago, and has been submitted to the journal Bodily Overview D. It’s at the moment accessible on the arXiv preprint server.

The research, based mostly on high-precision measurements of the cosmic microwave background and its polarized mild, provides additional assist to the veracity of the usual cosmological mannequin. It additionally makes a calculation of the Hubble fixed—how briskly the universe is increasing—with a brand new methodology, providing new perception on an ongoing scientific puzzle generally known as “the Hubble rigidity.”

“We now have a largely coherent, detailed, and profitable mannequin describing these 14 billion years of evolution,” mentioned Lloyd Knox, the Michael and Ester Vaida Endowed Chair in Cosmology and Astrophysics at UC Davis and one of many research’s co-authors. “However we do not know what truly generated the preliminary departures from full homogeneity that finally led to all of the constructions within the universe together with ourselves.”

“This result’s particularly thrilling, as a result of it represents the primary aggressive constraints on cosmology utilizing solely the polarization of the CMB, making it nearly 100% unbiased of earlier outcomes that relied totally on the overall depth,” mentioned research co-author and College of Chicago analysis professor Tom Crawford.

A polarizing and winding journey throughout the universe

Within the research, the researchers analyzed two years of polarized mild information collected by the South Pole Telescope in 2019 and 2020. The research’s observations cowl 1,500 sq. levels of sky and the collected information enabled the researchers to create a large-scale map of the mass within the universe.

Most pure mild is unpolarized, composed of a random assortment of sunshine waves, every oscillating (waving up and down) with no most well-liked route. However when mild is mirrored it might probably grow to be polarized—that means the sunshine oscillates in a most well-liked route.

This occurs when daylight displays off water, or the bottom, which explains polarized sun shades will be so useful for decreasing glare. It additionally occurred because the cosmic microwave background photons underwent their ultimate scattering occasions within the primordial plasma because it started to vanish 14 billion years in the past.

“The sunshine from the cosmic microwave background is partially polarized,” Knox mentioned. “We’re measuring at every location in our sky map the diploma to which it is polarized and the orientation of the polarization.”

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Researchers used the telescope information to create maps of the polarization of the cosmic microwave background mild—which can be utilized to tease out clues about what occurred within the very earliest years of the universe. The colours signify the quantity of polarization within the cosmic microwave background. Credit score: Ge et al

After that final scattering, the marginally polarized mild streamed throughout open house. Gravitational forces distort the paths of those mild rays. Mild from totally different areas can be distorted in another way, leading to a warped picture—an impact referred to as gravitational lensing.

To find each what the polarized picture would seem like within the absence of gravitational lensing and likewise the map of the mass inflicting the gravitational lensing, the workforce used computer systems on the Nationwide Power Analysis Scientific Computing Heart (NERSC) in Berkeley.

“What we primarily do at a very excessive stage is we have now this information and we ship it over to this supercomputer at NERSC,” mentioned Marius Millea, a venture scientist with Knox’s analysis group and the research’s second writer. “And the computer systems are testing this concept, “If this have been how the true universe appeared, would it not produce a map that appears like what we noticed?'”

“We now have the info, however we additionally must have a mannequin that produces or predicts these type of observables,” added Fei Ge, a graduate pupil with Knox’s analysis group and the research’s first writer.

The Hubble rigidity

The workforce’s analysis straight addresses a conundrum within the cosmological group generally known as “the Hubble rigidity.” In essence, scientists cannot come to an settlement on the speed of the enlargement of the universe, which varies relying on the methodology used to measure it.

In a single methodology, astronomers use the usual cosmological mannequin, mixed with observations of the cosmic microwave background, to foretell how quickly the universe is increasing at this time.

In one other methodology, they use observations of stars, and stellar explosions referred to as supernovae, to measure the enlargement fee extra straight. Measurements from this methodology have usually are available in greater—that’s, a sooner fee of enlargement—than the usual mannequin predictions. This is among the main puzzles in up to date cosmology; the origin of the discrepancy is unknown.

The workforce used their polarization information, mixed with the usual cosmological mannequin, to make a brand new prediction for the speed of enlargement. Their prediction is in step with the prediction made utilizing the cosmic microwave background depth maps measured by the Planck satellite tv for pc, a European House Company mission.

The workforce’s new prediction is exact sufficient to be discrepant with the supernovae measurements at very excessive statistical significance. It aligns extra with the speed of enlargement predicted by the usual cosmological mannequin and cosmic microwave background depth methodology, and represents yet one more hoop that any answer to the Hubble rigidity must leap by way of.

Extra info:
F. Ge et al, Cosmology From CMB Lensing and Delensed EE Energy Spectra Utilizing 2019-2020 SPT-3G Polarization Information, arXiv (2024). DOI: 10.48550/arxiv.2411.06000

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