Physics & Astronomy

Illustration of photon-photon scattering in the laboratory.
Physics & Astronomy

Oxford Physicists Unveil Extreme Quantum Vacuum Effects

Using advanced computational modelling, a research team led by the University of Oxford, working in partnership with the Instituto Superior Técnico in the University of Lisbon, has achieved the first-ever real-time, three-dimensional simulations of how intense laser beams alter the ‘quantum vacuum’—a state once assumed to be empty, but which quantum physics predicts is full of virtual electron-positron pairs. Excitingly, these simulations recreate a bizarre phenomenon predicted by quantum physics, known as vacuum four-wave mixing. This states that the combined…

TOI-6894b Exoplanet
Physics & Astronomy

Giant Planet Around Tiny Star: A New Challenge to Formation Theories

An international team of astronomers, including researchers from the University of Liège and collaborators in UK, Chile, the USA, and Europe, has discovered a giant planet orbiting the smallest known star to host such a companion The host star, TOI-6894, is a red dwarf with only 20% the mass of the Sun, typical of the most common stars in our galaxy. Until now, such low-mass stars were not thought capable of forming or retaining giant planets. But as published today…

Artistic concept of the early WASP-121 disc, the birthplace of WASP-121b
Physics & Astronomy

Webb Uncovers Origins of Ultra-Hot Exoplanet WASP-121b

The detection of atmospheric methane and silicon monoxide suggests that it originated in a region analogous to the Solar System’s domain of gas and ice giants. Observations with the James Webb Space Telescope (JWST) have provided new clues about how the exoplanet WASP-121b has formed and where it might have originated in the disc of gas and dust around its star. These insights stem from the detection of multiple key molecules: water vapour, carbon monoxide, silicon monoxide, and methane. With…

Physics & Astronomy

MISTRAL: Transforming SRT Observations with Innovative Insights

MISTRAL is a new generation receiver installed on the Sardinia Radio Telescope (SRT) and built by the Sapienza University of Rome for the National Institute for Astrophysics (INAF) as part of the upgrade of the radio telescope for the study of the Universe at high frequencies, funded by a PON (National Operational Program) project, concluded in 2023 and now providing its first significant scientific results. MISTRAL stands for “MIllimetric Sardinia radio Telescope Receiver based on Array of Lumped elements kids”….

Super massive black holes
Physics & Astronomy

Decoding the Origins of Mysterious Radiation Phenomena

Could black holes help explain high-energy cosmic radiation? The universe is full of different types of radiation and particles that can be observed here on Earth. This includes photons across the entire range of the electromagnetic spectrum, from the lowest radio frequencies all the way to the highest-energy gamma rays. It also includes other particles such as neutrinos and cosmic rays, which race through the universe at close to the speed of light. Curiously, “cosmic rays” are not actually rays…

The Plasma Micro-accelerator
Physics & Astronomy

Tabletop Proton Accelerator Powered by University Lasers

Laser Ion acceleration uses intense laser flashes to heat electrons of a solid to enormous temperatures and propel these charged particles to extreme speeds. These have recently gained traction for applications in selectively destroying cancerous tumor cells, in processing semiconductor materials, and due to their excellent properties – for imaging and fusion relevant conditions. Massive laser systems with several Joules of light energy are needed to irradiate solids for the purpose. This produces a flash of ions which are accelerated…

Galaxy & Turbulence Simulation Composite
Physics & Astronomy

Scientists Simulate Unpredictable Galactic Turbulence

Turbulence on the Galactic Scales From the ocean’s rolling swells to the bumpy ride of a jetliner, turbulence is everywhere. It breaks large waves into smaller ones, cascading energy across scales. It is ubitquitous throughout our Galaxy and the broader Universe, shaping the behavior of plasma, stars, and magnetic fields. Yet despite its ubiquity, turbulence remains one of the greatest unsolved problems in physics. Now, by developing the world’s largest-ever simulations of magnetized turbulence, an international team of scientists has measured —…

Figure 1
Physics & Astronomy

Squid Galaxy Elevates Neutrino Game with New Advances

An international team of researchers, including the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), has used a mismatch between elementary particles and gamma rays from NGC 1068 to propose a new route by which neutrinos can be produced. Antarctic ice has eyes that can see elementary particles called neutrinos, and what they’ve observed is puzzling scientists: a remarkably strong neutrino signal accompanied by a surprisingly weak gamma ray emission in the galaxy NGC 1068,…

Singular and non singular
Physics & Astronomy

Exploring Black Holes: Insights Beyond the Singularity

Can we do away with the troublesome singularity at the heart of black holes? A new paper in JCAP reimagines these extreme objects in light of current knowledge. “Hic sunt leones,” remarks Stefano Liberati, one of the authors of the paper and director of IFPU. The phrase refers to the hypothetical singularity predicted at the center of standard black holes — those described by solutions to Einstein’s field equations. To understand what this means, a brief historical recap is helpful….

Galaxies M81 and M82. Image by rwittich, Envato.
Physics & Astronomy

Understanding Warm Galaxy Clusters and Giant Interstellar Structures

The XRISM science team, including members of Nagoya University, has explained how galaxy clusters maintain their heat despite emitting X-rays, which typically have a cooling effect on the hot gas. By observation of the Centaurus cluster of galaxies, the XRISM team discovered the existence of a fast-moving, high-temperature gas flow in the center of the cluster. Their findings, published by Nature, may solve the ‘cooling flow problem’, explaining why clusters of galaxies look like they do. Galaxy clusters are made…

A narrow-band image of the Sun at a wavelength of λ=588.9nm, that of a well known solar sodium line also known as the “NaD line.” The image was acquired during recent first light efforts with the VTF at the Inouye, and shows how precisely the structures within a sunspot are resolved. Each pixel in the original version of the image corresponds to 10 km (or 6.2 miles) on the Sun. Credit: © VTF/KIS/NSF/NSO/AURA
Physics & Astronomy

World’s Largest Solar Telescope Begins Operations

First Light! The spectro-polarimeter of the world’s largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany With a primary mirror diameter of four meters, the Inouye Solar Telescope is the largest in the world. Thanks to the optimal observational conditions on the Hawaiian volcano Haleakala and the use of sophisticated methods of image stabilization and reconstruction, the Inouye Solar Telescope has been providing breathtakingly detailed views of our star since…

The SwRI-led NASA New Horizons mission’s extensive observations of Lyman-alpha emissions have resulted in the first-ever map from the galaxy in Lyman-alpha light. This SwRI-developed Alice spectrograph map (in ecliptic coordinates, centered on the direction opposite the Sun) depicts the relatively uniform brightness of the Lyman-alpha background surrounding our heliosphere. The black dots represent approximately 90,000 known UV-bright stars in our galaxy. The north and south galactic poles are indicated (NGP & SGP, respectively), along with the flow direction of the interstellar medium through the solar system (both upstream and downstream). Credit: Southwest Research Institute
Physics & Astronomy

First Lyman-Alpha Map of Galaxy V from New Horizons

SwRI-led NASA spacecraft’s scans offer surprising view of galactic surroundings The NASA New Horizons spacecraft’s extensive observations of Lyman-alpha emissions have resulted in the first-ever map from the galaxy at this important ultraviolet wavelength, providing a new look at the galactic region surrounding our solar system. The findings are described in a new study authored by the SwRI-led New Horizons team. “Understanding the Lyman-alpha background helps shed light on nearby galactic structures and processes,” said SwRI’s Dr. Randy Gladstone, the…

Researechers are testing superconducting microwire single-photon detectors (SMSPDs) for use in future particle physics exepriments. The detectors, which were designed and fabricated at JPL and commissioned at the INQNET-Caltech labs, were recently tested at Fermilab. They have the ability to detect single parties at a time, and may improve the precision of measurements made in particle accelerator collisions. Credit: Cristián Peña, Fermilab
Physics & Astronomy

Quantum Sensors Set to Transform Particle Physics Experiments

New research shows that the specialized sensors can detect particles more precisely To learn more about the nature of matter, energy, space, and time, physicists smash high-energy particles together in large accelerator machines, creating sprays of millions of particles per second of a variety of masses and speeds. The collisions may also produce entirely new particles not predicted by the standard model, the prevailing theory of fundamental particles and forces in our universe. Plans are underway to create more powerful…

Ana Carolina de Souza-Feliciano is an associate professor at the Florida Space Institute. Her research focuses on characterizing the surface properties of small bodies in our solar system. (Photo by Antoine Hart) Credit: Photo by Antoine Hart
Physics & Astronomy

UCF Scientists Explore Solar System Origins with James Webb Telescope

A newly published study shows varying levels of methanol, a molecule that is an important component of pre-biotic chemistry, in a spectral analysis of small celestial objects beyond Neptune University of Central Florida (UCF) scientists and their collaborators discovered new insights into the formation of distant icy objects in space beyond Neptune, offering a deeper understanding of our solar system’s formation and growth. Using the James Webb Space Telescope (JWST), scientists analyzed far-away bodies — known as Trans-Neptunian Objects (TNOs)…

The Allen Telescope Array at Hat Creek Radio Observatory. Credit: Luigi Cruz
Physics & Astronomy

SETI Institute Launches ARISE Lab for Community Colleges

Bringing SETI science to community colleges SETI Institute Launches ARISE Lab, Bringing SETI and Radio Astronomy to Community Colleges The SETI Institute announced it will expand its pilot program funded through a grant from the Amateur Radio and Digital Communication (ARDC) Foundation now called ARISE Lab (arise.seti.org). This initiative brings SETI science to community colleges and provides hands-on training for community college instructors and students in astronomy, digital signal processing, and radio science. “Hands-on experiences are proven to improve student…

A team of Penn State researchers are developing solutions to some of the biggest problems currently facing satellite technology with the help of a Defense Advanced Research Projects Agency grant. Credit: Poornima Tomy/Penn State
Physics & Astronomy

The New Era of Space Exploration: A Shorter Race

Another race to space is on, but the competitors aren’t reaching for the moon. Instead, multiple national agencies and private companies across the world are aiming for the edge of Earth’s atmosphere. Launching satellites into this very low Earth orbit (VLEO) environment — the altitude between 60 and 280 miles above Earth — could solve spacecraft crowding in traditional orbits, according to Sven Bilén, Penn State professor of engineering design, of electrical engineering and of aerospace engineering. Bilén said satellites in traditional…

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