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High-velocity molecular clouds in M83 provide new insight into how galaxies evolve

A new result from the molecular gas survey in the Southern Pinwheel Galaxy M83 using the Atacama Large Millimeter/submillimeter Array (ALMA) Telescope reveals a discovery of 10 high-velocity clouds composed of molecular gas, moving at velocities significantly different from M83’s overall rotation, an indication that the influx of these gases—which help to form stars—are from outside the galaxy.

This survey is led by Jin Koda, professor in the Department of Physics and Astronomy in the College of Arts and Sciences at Stony Brook University, who collaborated with Maki Nagata and Fumi Egusa, of the University of Tokyo, as well as an international team of astrophysicists. Their findings are published in The Astrophysical Journal.

Galaxies are primarily composed of stars and gas, with gas serving as the material for forming new stars. Through this process of star formation, galaxies evolve by converting gas into stars. It is estimated that without a supply of gas from external sources, the existing gas in a galaxy would be consumed within about 1 billion years and star formation would cease. The team’s finding on the of M83 provides new insight into how galaxies may evolve over millions and billions of years.

Breaking Ohm’s law: Nonlinear currents emerge in symmetry-broken materials

In a review just published in Nature Materials, researchers take aim at the oldest principle in electronics: Ohm’s law.

Their article, “Nonlinear transport in non-centrosymmetric systems,” brings together rapidly growing evidence that, when a material lacks inversion symmetry, the familiar linear relation between current and voltage can break down, giving rise to striking quadratic responses.

The study was led by Manuel Suárez-Rodríguez—working under the guidance of Ikerbasque Professors Fèlix Casanova and Luis E. Hueso at CIC nanoGUNE, together with Prof. Marco Gobbi at the Materials Physics Center (CFM, CSIC-UPV/EHU).

Breaking the Rules of Magnetism: Unusual Crystal Surprises Physicists With Cooling Effect

The research team has identified atacamite as a material with magnetocaloric properties. Natural crystals have long captivated us with their vivid colors, flawless geometry, and striking symmetry. But for scientists, these beautiful formations offer more than just visual delight. Hidden within thei

Physicists Catch Light in ‘Imaginary Time’ in Scientific First

For the first time, researchers have seen how light behaves during a mysterious phenomenon called ‘imaginary time’

When you shine light through almost any transparent material, the gridlock of electromagnetic fields that make up the atomic alleys and side streets will add a significant amount of time to each photon’s commute.

This delay can tell physicists a lot about how light scatters, revealing details about the matrix of material the photons must navigate. Yet until now, one trick up the theorist’s sleeve for measuring light’s journey – invoking imaginary time – has not been fully understood in practical terms.

Tiny stars, many Earths: Potentially habitable worlds may be especially common around low-mass stars

According to the latest studies led by Heidelberg University astronomers, low-mass stars quite often host Earth-like planets. Data collected as part of the CARMENES project were the basis of this finding. By analyzing the data, an international research team succeeded in identifying four new exoplanets and determining their properties.

At the same time, the researchers were able to show that Earth-like planets are found quite frequently in the orbit of stars with less than a sixth of the mass of our sun. These findings could support the search for potentially life-sustaining worlds in our cosmic neighborhood. The work is published in the journal Astronomy & Astrophysics.

The CARMENES spectrograph system at the Calar Alto Observatory near Almería (Spain) was developed and built at the Königstuhl Observatory of Heidelberg University. It aids astronomers in the search for exoplanets that orbit so-called M-dwarfs. These stars have a mass of less than one-tenth to half the mass of our sun. M-dwarfs are the most abundant stars in our galaxy. They exhibit tiny periodic movements caused by the of orbiting planets, from which researchers can infer the existence of previously undiscovered worlds.

Researchers demonstrate giant photonic isolation and gyration

The original goal of the study was to get this asymmetry to a point of perfect isolation—that is, where there is zero interaction in one direction. They successfully achieved this goal by demonstrating a giant optical isolation effect, where the propagation of light in one direction was a million times easier than in the opposite direction.

But while exploring their test devices, the engineers encountered a surprise. Their approach was so efficient that they could even get past the isolation point to where the sign of the coupling simply flipped and the phase became direction dependent. This was something that had not been seen before in time modulated coupling and is an easy path to photonic gyration.

Going forward, the Illinois researchers will work to expand their findings. They are working with their partners specializing in condensed matter to explore how longer and more elaborate chains of resonators with this kind of tunable couplings could answer fundamental questions on topological physics. Simultaneously, from an engineering standpoint, they aim to create a pure gyrator which is a universal building block of many nonreciprocal devices.

Physicists Unravel Mystery of Mercury’s Bizarre Nuclear Fission

A five-dimensional model has successfully predicted the asymmetric fission of mercury isotopes, offering new insights into nuclear fission processes beyond the well-studied elements uranium and plutonium. A five-dimensional (5D) Langevin model developed by an international team of researchers, in

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