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Category: cosmology – Page 24

Bridging the gap between the cosmic microwave background and the first galaxies

One of the Holy Grails in cosmology is a look back at the earliest epochs of cosmic history. Unfortunately, the universe’s first few hundred thousand years are shrouded in an impenetrable fog. So far, nobody’s been able to see past it to the Big Bang. As it turns out, astronomers are chipping away at that cosmic fog by using data from the Atacama Cosmology Telescope (ACT) in Chile.

ACT measured light first emitted in the baby some 380,000 years after the Big Bang. According to the Consortium director Suzanne Staggs, that measurement opened the window to a time when the first cosmic structures were starting to assemble. “We are seeing the first steps towards making the earliest stars and galaxies,” she said. “And we’re not just seeing light and dark, we’re seeing the in high resolution. That is a defining factor distinguishing ACT from Planck and other, earlier telescopes.”

The clearer data and images from ACT are also helping scientists understand just when and where the first galaxies began to form. If the ACT data are confirmed, they represent the earliest baby picture of the universe, showing scientists what the seeds of galaxies looked like only a few hundred thousand years after the Big Bang.

Astronomers unveil ‘baby pictures’ of the first stars and galaxies

The clearest and most precise images yet of the universe in its infancy—the earliest cosmic time accessible to humans—have been produced by an international team of astronomers.

Measuring light, known as the (CMB), that traveled for more than 13 billion years to reach a telescope high in the Chilean Andes, the new images reveal the universe when it was about 380,000 years old—the equivalent of hours-old baby pictures of a now middle-aged cosmos.

The research, by the Atacama Cosmology Telescope (ACT) collaboration, shows both the intensity and polarization of the earliest light after the Big Bang with unprecedented clarity, revealing the formation of ancient, consolidating clouds of hydrogen and helium that later developed into the first stars and galaxies.

Webb telescope sees galaxy in mysteriously clearing fog of early universe

Astronomers have identified a bright hydrogen emission from a galaxy in the very early universe. The surprise finding is challenging researchers to explain how this light could have pierced the thick fog of neutral hydrogen that filled space at that time.

A key goal of the NASA/ESA/CSA James Webb Space Telescope has been to see further than ever before into the distant past of our universe, when the first galaxies were forming after the Big Bang, a period known as cosmic dawn.

Researchers studying one of those very early galaxies have now made a discovery in the spectrum of its light, that challenges our established understanding of the universe’s early history. Their results are reported in the journal Nature.

X-ray observations reveal dynamic features of galaxy cluster PLCKG287

Using NASA’s Chandra X-ray observatory, astronomers have observed a massive and hot galaxy cluster known as PLCKG287.0+32.9 (or PLCKG287 for short). Results of the observational campaign, presented March 17 on the arXiv pre-print server, deliver important insights into the morphological and thermodynamical properties of this cluster.

Galaxy clusters contain up to thousands of galaxies bound together by gravity. They generally form as a result of mergers and grow by accreting sub-clusters. These processes provide an excellent opportunity to study matter in conditions that cannot be explored in laboratories on Earth. In particular, merging could help us better understand the physics of shock and cold fronts seen in the diffuse intra-cluster medium, the cosmic ray acceleration in clusters, and the self-interaction properties of dark matter.

PLCKG287, also known as PSZ2 G286.98+32.90, is a galaxy cluster at a redshift of 0.38, with a mass of about 1.37 quadrillion solar masses and a temperature of 13 keV. The cluster has an X-ray luminosity in the 2–10 keV band at a level of 1.7 quattuordecillion erg/s.

A new piece in the matter–antimatter puzzle: A fundamental asymmetry in the behavior of baryons

On March 24, at the annual Rencontres de Moriond conference taking place in La Thuile, Italy, the LHCb collaboration at CERN reported a new milestone in our understanding of the subtle yet profound differences between matter and antimatter.

In its analysis of large quantities of data produced by the Large Hadron Collider (LHC), the international team found overwhelming evidence that particles known as baryons, such as the protons and neutrons that make up , are subject to a mirror-like asymmetry in nature’s fundamental laws that causes matter and antimatter to behave differently.

The discovery provides new ways to address why the that make up matter fall into the neat patterns described by the Standard Model of particle physics, and to explore why matter apparently prevailed over antimatter after the Big Bang. The paper is available on the arXiv preprint server.

Beyond the Observable

There remain many questions — how precisely to test prime resonance coupling in the lab, how to formalize “consciousness” in a rigorous physical sense, and how to harness these insights for breakthrough technologies.

Yet the potential is vast. Non-local communication, quantum AI, and a bold reinterpretation of black holes as ultimate observers challenge us to delve deeper and rethink old assumptions.

The journey forward will require experiments that push the boundaries of quantum measurement, investigate subtle anomalies in tunneling and interference, and refine our understanding of how consciousness might operate as an entropic conductor.

“Space tornadoes” discovered at the center of our galaxy

Deep in the galaxy’s central molecular zone (CMZ), surrounding the supermassive black hole at the Milky Way’s center, clouds of dust and gas swirl amid energetic shock waves.

Now, a collaboration of international astronomers – using the Atacama Large Millimeter/submillimeter Array (ALMA) – has greatly sharpened our view of these processes by a factor of 100.

The team has uncovered an unexpected class of long, narrow filaments within this turbulent region, giving fresh insight into the cyclical formation and destruction of material in the CMZ.

Time Travel? Powerful Atacama Cosmology Telescope Peers Over 99.99% of the Way Back in Time

A pair of studies describing the findings also confirm the standard model of cosmology and offer compelling findings regarding the cosmological conundrum known as the Hubble Tension. The researchers also spotted light from several other sources, resulting in a virtual cosmic road map from the present to the beginning of time.

“We can see right back through cosmic history,” said Jo Dunkley, the Joseph Henry Professor of Physics and Astrophysical Sciences at Princeton University and the ACT analysis leader, in an announcement, “from our own Milky Way, out past distant galaxies hosting vast black holes, and huge galaxy clusters, all the way to that time of infancy.”

The new data from the ACT builds on several previous studies, including a time-traveling video from NASA’s James Webb Space Telescope, examining the early universe after the Big Bang when time reportedly moved five times slower than today. One study even proposed a second event called a “dark Big Bang” to explain lingering cosmic mysteries.

Theories and Engineering Possibilities for Time Travel

Time travel has long fascinated scientists and theorists, prompting questions about whether the future can send visitors into its own past and whether individuals could move forward in time in ways that bypass the normal flows of daily life. The general idea of time as a fourth dimension, comparable to spatial dimensions, gained traction when Hermann Minkowski famously stated that “space by itself, and time by itself, are doomed to fade away into mere shadows” (Minkowski, 1908, p. 75). This integrated view of spacetime underlies many physics-based theories of how a traveler might move along the temporal axis.

In relativity, closed timelike curves (CTCs) theoretically allow a path through spacetime that loops back to its origin in time. As Kip Thorne put it, “wormhole physics is at the very forefront of our understanding of the Universe” (Thorne, 1994, pp. 496–497). A wormhole with suitable geometry might permit travel from one point in time to another. However, such scenarios raise paradoxes. One common example is the “grandfather paradox,” which asks how a traveler could exist if they venture into the past and eliminate their own ancestor. David Deutsch offered one possible resolution by suggesting that “quantum mechanics may remove or soften the paradoxes conventionally associated with time travel” (Deutsch, 1991, p. 3198). His reasoning rests on the idea that quantum behavior might allow timelines to branch or otherwise circumvent contradictions.