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Category: cosmology

ALMA reveals hidden structures in the first galaxies of the universe

Astronomers have used the Atacama Large Millimeter/submillimeter Array (ALMA) to peer into the early universe and uncover the building blocks of galaxies during their formative years. The CRISTAL survey—short for [CII] Resolved ISM in STar-forming galaxies with ALMA—reveals cold gas, dust, and clumpy star formation in galaxies observed as they appeared just 1 billion years after the Big Bang.

“Thanks to ALMA’s unique sensitivity and resolution, we can resolve the internal structure of these early in ways never possible before,” said Rodrigo Herrera-Camus, principal investigator of the CRISTAL survey, professor at Universidad de Concepción, and Director of the Millennium Nucleus for Galaxy Formation (MINGAL) in Chile. “CRISTAL is showing us how the first galactic disks formed, how stars emerged in giant clumps, and how gas shaped the galaxies we see today.”

CRISTAL, an ALMA Large Program, observed 39 typical star-forming galaxies selected to represent the main population of galaxies in the early universe. Using [CII] line emission, a specific type of light emitted by ionized in cold interstellar gas, as a tracer of and dust, and combining it with near-infrared images from the James Webb and Hubble Space Telescopes, researchers created a detailed map of the interstellar medium in each system.

Star-Shredding Spectacle: NASA Reveals Brightest Black Hole Blasts Since the Big Bang

Supermassive black holes usually lurk unseen, but when an unlucky star drifts too close they ignite titanic outbursts brighter than 100 supernovae. By mixing NASA, ESA, and ground-based data, astronomers caught three of these rare “extreme nuclear transients,” including the cheekily named “Barbie

Supernova remnant SNR J0450.4−7050 investigated in detail

An international team of astronomers has employed various satellites and ground-based telescopes to perform multiwavelength observations of a supernova remnant known as SNR J0450.4−7050. Results of the observational campaign, published June 18 on the pre-print server arXiv, yield new insights into the properties of this remnant, finding that it is much larger than previously thought.

Supernova remnants (SNRs) are diffuse, expanding structures resulting from a supernova explosion, which usually last several hundred thousand years before dispersing into the (ISM). Observations show that SNRs contain ejected material expanding from the explosion and other interstellar material that has been swept up by the passage of the shockwave from the exploded star.

Studies of SNRs beyond the Milky Way are crucial for understanding their feedback in different evolutionary phases and gaining insights into their local ISM. The Large Magellanic Cloud (LMC) is one of the galaxies that has its SNR population explored in detail.

A magnetically levitated particle enables researchers to search for ultralight dark matter

Dark matter, although not visible, is believed to make up most of the total mass of the universe. One theory suggests that ultralight dark matter behaves like a continuous wave, which could exert rhythmic forces that are detectable only with ultra-sensitive quantum instrumentation.

New research published in Physical Review Letters and led by Rice University physicist Christopher Tunnell and postdoctoral researcher Dorian Amaral, the study’s first author and lead analyst, sees the first direct search for ultralight using a magnetically levitated particle.

In collaboration with physicists from Leiden University, the team suspended a microscopic neodymium magnet inside a superconducting enclosure cooled to near absolute zero. The setup was designed to detect subtle oscillations believed to be caused by dark matter waves moving through Earth.

New theoretical framework reveals hidden complexity in black hole ringdown signals

In a recently published paper in Physical Review Letters, scientists propose a comprehensive theoretical framework indicating that gravitational wave signals from black hole mergers are more complex than earlier anticipated.

When two black holes merge in the cosmos, the cataclysmic event doesn’t end with a simple collision. The newly formed black hole continues to vibrate like a struck bell, producing gravitational waves in what scientists call the “ringdown” phase.

Researchers found that the cosmic reverberations involve sophisticated quadratic mode couplings—secondary oscillations that develop when primary modes interact with each other. This nonlinear behavior had been predicted in Einstein’s theory of , but has never been fully characterized until now.

“We’re Rewiring the Future”: MIT’s Superconducting Chip Breakthrough Could Unlock the True Power of Quantum Computing

IN A NUTSHELL 🔬 MIT researchers have developed a superconducting diode-based rectifier that converts AC to DC on a single chip. 💡 This innovation could streamline power delivery in ultra-cold quantum systems, reducing electromagnetic noise and interference. 🔍 The technology is crucial for enhancing qubit stability and could significantly impact dark matter detection circuits at