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Scientists have discovered a unique link between ferroelectric domain walls and superconductivity in two-dimensional van der Waals materials. This breakthrough, credited to research by Gaurav Chaudhary from the University of Cambridge and Ivar Martin from Argonne National Laboratory, sheds light on how specific structural features in these materials enable strong electron interactions. The findings are expected to pave the way for new superconducting devices and innovative applications in the field of condensed matter physics.

Sliding Ferroelectricity and Polarisation Reversal

According to reports by phys.org, sliding ferroelectricity in certain 2D van der Waals materials, including boron nitride and transition metal dichalcogenides (TMDs), facilitates polarisation reversal under moderate electric fields. This phenomenon allows for large-scale manipulation of layer stacking, significantly impacting the material’s electronic properties. Researchers noted that domain walls—boundaries separating regions with differing orientations of ferroelectric polarisation—exhibit unique characteristics that enhance electron-phonon coupling.

Superconductivity Observed at Domain Walls

The study revealed that in materials like molybdenum ditelluride (MoTe₂), superconductivity is transiently enhanced near ferroelectric reversal transitions. This enhancement occurs within hysteresis loops where domains of varying polarisation coexist. The dynamic fluctuations in domain walls were identified as the driving mechanism for the pairing interactions required for superconductivity. It was highlighted that these conditions are exclusive to 2D TMDs, which support interlayer ferroelectricity while remaining conductive within their planes.

Future Research and Applications

Chaudhary and Martin indicated to phys.org that their findings hold potential for developing highly controllable superconducting devices. Efforts are underway to explore the systematic design of new superconductors by layering polar materials and leveraging domain wall networks in moiré systems. They also emphasised the need for further investigations to validate their theoretical models using advanced microscopic simulations.
The study has generated interest among scientists aiming to uncover unconventional mechanisms of superconductivity, marking an important step forward in understanding and utilising the properties of 2D materials.

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Newly Confirmed Super-Earth HD 20794 d May Support Life in Habitable Zone

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Newly Confirmed Super-Earth HD 20794 d May Support Life in Habitable Zone

A super-Earth has been confirmed in the habitable zone of a nearby star, raising possibilities for future studies on potentially life-supporting planets. The discovery follows over two decades of observations and has been credited to a team of international researchers. Initially detected two years ago, the planet, named HD 20794 d, is situated 20 light years from Earth and has a mass six times that of Earth. Scientists suggest its orbit places it at an optimal distance from its star to sustain liquid water, a key factor for habitability.

Observational Data Confirms Planet’s Existence

According to a study published in Astronomy & Astrophysics, HD 20794 d was first identified as a possible exoplanet by Dr. Michael Cretignier from the University of Oxford in 2022. Data from the HARPS (High Accuracy Radial Velocity Planet Searcher) spectrograph at the La Silla Observatory in Chile indicated periodic shifts in the light spectrum of the host star, suggesting gravitational influence from an orbiting planet. However, initial findings lacked definitive confirmation due to the faintness of the signal, which led to doubts over whether the anomaly was planetary, instrumental, or caused by stellar activity.

To validate the discovery, data spanning over 20 years from both HARPS and ESPRESSO, an advanced spectrograph also based in Chile, were analysed. As reported by phys.org, Dr. Cretignier said that they have worked on data analysis for years and are gradually analysing and eliminating all possible sources of contamination. The confirmation required advanced processing techniques to separate the planetary signal from background interference.

Implications for Future Space Missions

Dr. Cretignier expressed both excitement and relief upon confirmation of the planet. He stated that great joy was naturally felt when the planet’s existence could be confirmed. Relief was also experienced, as the original signal had been at the edge of the spectrograph’s detection limit, making it difficult at that time to be completely convinced of the signal’s authenticity. He further stated that HD 20794 d’s proximity to Earth makes it a prime candidate for future missions aiming to capture direct images of exoplanets.

Despite its placement in the habitable zone, the planet’s elliptical orbit raises questions about its suitability for life. Its changing distance from the star moves it between the inner and outer edges of the habitable zone, potentially subjecting it to extreme temperature variations.

Potential for Further Study

HD 20794 d is expected to be a focal point for upcoming projects like the Extremely Large Telescope, the Habitable Worlds Observatory, and the Large Interferometer For Exoplanets (LIFE). These instruments aim to study exoplanet atmospheres in search of biosignatures that could indicate life.

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El Capitan Is Now the Fastest Supercomputer on the Planet

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El Capitan Is Now the Fastest Supercomputer on the Planet

The world’s most powerful supercomputer, El Capitan, has been officially launched at the Lawrence Livermore National Laboratory (LLNL) in California. Built at a cost of $600 million, the system has been designed to manage highly classified national security tasks. The primary objective of the supercomputer is to ensure the security and reliability of the U.S. nuclear stockpile in the absence of underground testing, which has been prohibited since 1992. Research in high-energy-density physics, material discovery, nuclear data analysis, and weapons design will be conducted, along with other classified operations.

Performance and Capabilities

According to reports, El Capitan became the fastest supercomputer globally after achieving 1.742 exaFLOPS in the High-Performance Linpack (HPL) benchmark. The system has a peak performance of 2.746 exaFLOPS, making it the third machine ever to reach exascale computing speeds. The measurement, taken in floating-point operations per second (FLOPS), represents the ability of the supercomputer to perform one quintillion (10^18) calculations per second.

As reported by space.com, the second-fastest supercomputer, Frontier, located at Oak Ridge National Laboratory in Illinois, has recorded a standard performance of 1.353 exaFLOPS, with a peak of 2.056 exaFLOPS. El Capitan’s significant advancement marks a leap in computational capabilities within high-performance computing.

Technical Specifications

As reported by The Next Platform, El Capitan is powered by over 11 million processing and graphics cores distributed across 44,544 AMD MI300A accelerated processing units. These units incorporate AMD EPYC Genoa CPUs, AMD CDNA3 GPUs, and shared computing memory. Each processing unit includes 128 gigabytes of high-bandwidth memory, designed to optimise computational efficiency while minimising power consumption.

Development and Commissioning

Reports indicate that construction of El Capitan began in May 2023, with the system going online in November 2024. The official dedication took place on January 9, 2025. The supercomputer was commissioned by the U.S. Department of Energy’s CORAL-2 program as a successor to the Sierra supercomputer, which was deployed in 2018 and currently ranks 14th in the latest Top500 list of most powerful supercomputers.

With El Capitan’s full-scale deployment, advancements in national security research and computational science are expected to reach unprecedented levels.

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ISRO Dismisses Glitch Reports in SpaDeX Docking, Confirms Mission Progress

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ISRO Dismisses Glitch Reports in SpaDeX Docking, Confirms Mission Progress

The Indian Space Research Organisation (ISRO) has dismissed reports suggesting issues in its maiden space docking mission, SpaDeX. On February 8, ISRO Chairman and Secretary, Department of Space, V Narayanan, clarified that no technical faults had been encountered in the docking process. He stated that the mission was progressing systematically and that further experiments were planned. His remarks were made during the 15th Biennial Edition of the Aero India International Seminar in Bengaluru, scheduled from February 10 to 14. The docking of satellites under SpaDeX was carried out successfully on January 16, with post-docking control enabling the satellites to function as a single entity.

Successful Docking and Mission Details

As reported by The Indian Express, according to ISRO, SpaDeX achieved a significant milestone by docking two satellites in orbit, with docking precision confirmed through manoeuvres. The agency reported that post-docking stability was achieved, with the satellites operating as a unified structure. The mission also involved injecting the NVS-02 navigation satellite into a Geosynchronous Transfer Orbit (GTO).

ISRO detailed the docking procedure, stating in a post on X (formerly Twitter) that the satellites were manoeuvred from a 15-metre distance to a 3-metre hold point before initiating capture. The docking process was completed with retraction and rigidisation for structural stability. With this development, India became the fourth country globally to achieve space docking.

Challenges in Orbit Raising Operations

Despite the successful docking, ISRO issued an update on February 2 indicating that attempts to raise the satellite’s orbit had encountered difficulties. The agency explained that the oxidiser valves, crucial for thruster ignition, had failed to open, preventing orbital repositioning. The issue remains under analysis as ISRO assesses possible solutions.

The SpaDeX mission was launched on December 30, 2024, using the PSLV C60 rocket, which deployed two small satellites, SDX01 and SDX02, into a 475-kilometre orbit. The mission serves as a demonstration of in-space docking capabilities, aiming to advance cost-effective space technology for future applications.

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