A chain of plasmoids is created on the equatorial plane along the current sheet, where the particle density (left part) is higher. Here, magnetic reconnection takes place, accelerating particles to very high energies (right). Particles also reach relativistic speeds along the spin axis and eventually form the jet, powered by the Blandford–Znajek mechanism. Gray: Magnetic field lines. Image: Meringolo, Camilloni, Rezzolla (2025)
A chain of plasmoids is created on the equatorial plane along the current sheet, where the particle density (left part) is higher. Here, magnetic reconnection takes place, accelerating particles to very high energies (right). Particles also reach relativistic speeds along the spin axis and eventually form the jet, powered by the Blandford–Znajek mechanism. Gray: Magnetic field lines. Image: Meringolo, Camilloni, Rezzolla (2025)

Galactic engines revealed: The supercomputer quest to unveil how black holes ignite cosmic jets

Within the vast, silent expanse of the universe, black holes remain concealed yet omnipresent. Despite their invisibility, their gravitational influence is undeniable, as they consume matter and distort the fabric of spacetime. Paradoxically, these celestial entities also fuel some of the universe's most remarkable phenomena: relativistic jets, powerful beams of matter and energy that propagate outwards at speeds approaching the speed of light. The mechanisms driving these cosmic jets have long been a subject of intense investigation within the physics community. Now, a research team at Goethe University Frankfurt posits a breakthrough in understanding this phenomenon, employing supercomputing technology rather than traditional telescopes to unravel the mystery.

A Century-Old Mystery, Revisited

The galaxy Messier 87 (M87) has long captivated astronomers. At its heart lies a supermassive black hole, M87*, estimated to weigh six and a half billion Suns. From this inky core, a jet erupts, carrying plasma outward across thousands of light-years. Despite decades of observation, the precise mechanism by which a black hole converts its rotational energy into a directed, powerful jet has remained elusive.

The Frankfurt team, led by Professor Luciano Rezzolla, has developed a new computational framework—the FPIC (Frankfurt particle-in-cell) code—that simulates the interaction of charged particles, electromagnetic fields, and gravity near a spinning black hole in extreme detail. Their findings point to a two-fold mechanism: the well-known Blandford–Znajek process, which extracts energy via magnetic fields anchored in the black hole’s spin, and a newly highlighted role for magnetic reconnection. In this latter process, magnetic field lines break and rejoin, releasing energy, accelerating particles, and feeding into the jet itself.

Supercomputers as Modern Alchemists

Simulating these scenes—where gravity, electromagnetism, and plasma physics converge—demands computational power of immense scale. The Goethe team leveraged the "Goethe" supercomputer and Stuttgart's "Hawk," consuming millions of CPU hours to execute their models. The code simultaneously solves Maxwell's equations (governing electromagnetic fields), the equations of motion for electrons and positrons, and aspects of general relativity, all within a curved spacetime. It creates a virtual environment where plasmoids (bubbles of plasma) emerge on the equatorial plane, are propelled outward, and ultimately funnel into jets aligned with the black hole's rotational axis.

The simulations' remarkable accuracy in mirroring observational data—matching temperature estimates, densities, magnetic field strengths, and even radio emissions—bolsters confidence in both the computational method and the physical model it elucidates.

A New Narrative for Jet Power

This work's most inspirational aspect is its expansion of our theoretical toolkit. While the Blandford–Znajek mechanism has long been the leading explanation for how rotating black holes launch jets, the Frankfurt simulations suggest that magnetic reconnection plays a significant, and perhaps indispensable, supporting role. Plasmoids created by reconnection may tap into the black hole’s energy reservoir, spawn regions of negative energy, and seed the jet structure itself. This layered mechanism helps explain how jets maintain their power over thousands of light-years and remain stable, even in the chaotic environment near a black hole. It paints black holes not as mere consumers of matter, but as cosmic engines—engines that convert spin into focused, blazing outflows.

Inspiration from Codes and Crystals of Light

Beyond the physics itself lies a deeper message: the universe responds to our curiosity, if only we dare to ask with enough fidelity and boldness. These simulations don’t just approximate reality; they become mini-universes, where fields, particles, and forces dance under our command (at least in code). Supercomputers serve as the telescopes of the theoretical world. It is no small feat to translate equations into digital matter, to make each photon, electron, and magnetic line part of a symphony. The researchers behind FPIC have demonstrated the extent of human ingenuity, building tools that convert abstract mathematics into images and predictions that reflect the real cosmos.

Into the Future: Open Questions & Wider Horizons

While the Frankfurt simulation marks a significant step, it's not the final answer. Real black holes are fed by complex accretion disks that experience magnetic turbulence, instabilities, and misalignments. How do these local environments—warped disks, feeding flows, and external field structures—influence jet morphology and stability across galactic scales?

The team aims to expand FPIC to more realistic scenarios, including varied spin rates, tilted disks, and uneven magnetic environments. They also plan to directly compare their findings with upcoming high-resolution observations, such as those from next-generation radio interferometers.

One thing is certain: when minds, mathematics, and machines align, the universe reveals itself to us in beautiful, unexpected ways. From the silent entropy of black holes to the blazing pillars of relativistic jets, we are learning that even the darkest regions can shine when viewed through the lens of human curiosity and supercomputing power.

In a data center, supercomputers hum. In their memory, replicas of black hole environments evolve. Magnetic fields twist, plasmas erupt, jets hurtle outward. And in our world, these simulations bring us closer to understanding how the universe’s deadliest monsters light up the cosmos. If that isn't inspiring, what is?

A new world emerges in our cosmic backyard

Astronomers have revealed exciting new evidence of a Saturn-mass planet orbiting Alpha Centauri A, the nearest Sun-like star to Earth, thanks to the advanced capabilities of NASA's James Webb Space Telescope and the analytical prowess of supercomputer simulations.

The planet candidate, concealed amidst the brilliance of two glowing suns, was detected using Webb's Mid-Infrared Instrument (MIRI) with a coronagraphic mask to block out starlight. Researchers then painstakingly extracted the planet's signal through advanced image processing and modeling. However, capturing the light is just part of the story, supercomputers provided the essential support.

Simulations: Illuminating an Invisible World

After Webb’s initial observation identified a source more than 10,000 times fainter than Alpha Centauri A, subsequent images were unable to recreate the detection. To understand why, scientists turned to high-powered simulations, digital models that trace hypothetical orbits, analyze light behavior around bright stars, and interpret the optical signatures left by a planet that is too faint to be seen clearly.

These simulations, conducted on supercomputers designed to handle massive datasets, enabled researchers to rule out artifacts, confirm that the signal was consistent with that of a planet, and explain why it might disappear from view in subsequent observations. Such modeling is critical; by virtually recreating the interplay of light, shadow, and movement around the star, researchers could confidently support their candidate's existence.

The Promise of What Lies Ahead

This combination of Webb’s observational power and supercomputer modeling expands our horizons. If confirmed, this gas giant orbiting within the habitable zone of one of our nearest stellar neighbors would represent a significant advancement, achieved through the synergy of cutting-edge engineering and computational capabilities.

As Caltech graduate student Aniket Sanghi notes, confirming this discovery would signify “a new milestone for exoplanet imaging,” driven not only by Webb’s observations but also by the powerful computational tools that bring clarity to complex data.

In an era where every pixel presents a puzzle and every faint dot may represent a new world, it is the collaboration between telescopes and supercomputers that lights our path forward.

Supermicro's sales increased by 7%, but profits fell due to rising costs

Concerns Mount Despite Strong AI Demand and Revenue Growth

Super Micro Computer, Inc. has reported a 7% increase in revenue, exceeding $5.8 billion in Q4 FY25 and achieving an impressive $22 billion for the full year. However, underlying this growth are several cautionary signs that have investors and analysts concerned.

Despite a substantial 47% year-over-year sales increase, net income fell to $195 million in Q4, a sharp decline from $297 million in the same quarter last year. Diluted earnings per share dropped over 32%, landing at just $0.31. For a company positioned for growth in the AI infrastructure boom, these decreasing profits are raising eyebrows.

In its earnings release, Supermicro credited strong demand from neoclouds, cloud service providers, sovereign entities, and enterprise customers as key revenue drivers. The company’s Datacenter Building Block Solutions (DCBBS) have been particularly well received for their plug-and-play efficiency in AI-ready environments.

However, the financial details reveal that growth has come at a cost. Operating expenses soared to $1.18 billion for the year, up from $851 million in FY24. Stock-based compensation increased over 35% year-over-year to $314 million, and interest expenses tripled to nearly $60 million, largely due to the company's aggressive financing strategy, which included the issuance of $3 billion in new convertible notes.

These rising costs and tightening gross margins (down to 9.5% GAAP in Q4 from 10.2% a year ago) have triggered concern among financial observers.

Stock Market Reaction

According to a CNBC report on August 6, investors responded with caution. While shares initially surged during trading hours, enthusiasm waned after the earnings call revealed narrowing profitability and increasing debt obligations. The stock had skyrocketed over 200% in the past year due to the promise of AI-driven growth, but investors are now questioning whether Supermicro can sustain both rapid expansion and profitable earnings.

Supermicro anticipates Q1 FY26 net sales between $6.0 billion and $7.0 billion, with diluted GAAP earnings per share possibly as low as $0.30. While top-line growth may persist, the expected EPS range suggests continued pressure on profitability.

The company currently carries $4.8 billion in convertible debt—almost equal to its cash reserves of $5.2 billion. Although Supermicro insists this is part of a strategic expansion to meet global demand, it also exposes the company to risks in a volatile macroeconomic environment characterized by fluctuating interest rates and inflation.

The Bigger Picture

Supermicro is making a significant bet on hyperscale demand for AI, cloud, and edge computing. CEO Charles Liang remains optimistic, stating that the company is “on track to grow its large-scale datacenter customers from four in FY25 to six to eight in FY26.”

However, the numbers illustrate a story of razor-thin profitability amid a quest for aggressive growth. The company's Adjusted EBITDA margin declined to just 5.9% in Q4, down from 7.2% the previous year—a troubling trend given its ambitious growth plans.

As the AI gold rush continues, Supermicro has positioned itself at the forefront of next-gen computing infrastructure. The pressing question for investors is how long the company can maintain this rapid pace of growth before profit erosion undermines its potential rewards.

Bottom Line

Supermicro’s results indicate a company thriving on revenue growth but burdened by rising costs, shrinking margins, and increasing debt. While its investment in AI scale seems to be paying off in sales for now, unless profit metrics improve, Wall Street's patience may wear thin despite its optimism.

CrowdStrike launches Signal: AI technology unveils hidden threats

This week at Black Hat USA 2025, CrowdStrike introduced Signal, a groundbreaking self-learning detection engine that represents a significant advancement in AI-driven cybersecurity. Positioned to transform how organizations identify sophisticated threats, Signal aims to detect stealthy intrusions long before they escalate, generating considerable excitement within security circles.

Understanding Signal: Learning normal behavior and spotting subtle anomalies

At the core of Signal is a series of statistical time-series models that continuously learn the normal behavior of each user, host, and process over time and across systems. Rather than relying on static rules, Signal adapts in real-time by detecting even the slightest deviations that could indicate malicious activity.

By correlating these low-signal events over time, Signal generates high-confidence leads grouped into sequences of suspicious actions that cut through the noise of regular activity. This capability enhances the speed of investigation and response, significantly reducing alert fatigue for security teams.

Identifying the invisible: Connecting the dots

While traditional tools may interpret isolated benign behaviors, Signal makes connections among them. It identifies the use of living-off-the-land tools, unusual process executions, or atypical temporary directory activity—activities that may appear harmless in isolation but form part of a larger, more concerning pattern over hours or days.

This layered, temporal intelligence transforms fragmented events into actionable threat leads, enabling defenders to act early, often well before any compromise becomes apparent.

CrowdStrike's cloud-native strength

Signal is integrated into the Falcon platform and supported by the CrowdStrike Security Cloud. It operates at an immense scale, analyzing billions of events in each customer environment daily, yet distills this information into a few high-fidelity leads that can be acted upon.

CrowdStrike’s AI-native architecture allows for swift deployment and effective detection from day one without the need for heavy agents or complex setups.

The role of supercomputing: Enhancing AI detection at scale

While Signal utilizes distributed cloud infrastructure, the development and ongoing refinement of these advanced behavioral models rely heavily on modern high-performance computing (HPC). Research indicates that cutting-edge AI systems—particularly those focused on anomaly detection and time-series learning—benefit immensely from being trained at scale on supercomputers equipped with tens of thousands of cores and GPU clusters.

In fields like gravitational-wave research and anomaly detection, AI models are trained on supercomputing resources utilizing thousands of GPUs, later optimized for swift inference across large datasets using specialized tools like NVIDIA TensorRT.

By developing and testing detection models on such powerful infrastructure, cybersecurity innovators can enhance engines like Signal to become faster, more accurate, and more adaptive, enabling them to manage billions of events in nearly real-time.

Why It Matters

The combination of AI and supercomputing creates a powerful feedback loop:

- Model Training at Scale: Utilizing HPC to identify subtle patterns and behaviors.

- Real-Time Inference at the Edge: Operating in production environments on lightweight Falcon agents, allowing for instant decision-making.

- Continuous Feedback: Models continuously update, learning new baselines as organizational environments evolve.

This synergy allows CrowdStrike to deliver a detection engine that is both intelligent and operationally efficient.

Looking forward: A safer cyber future

Signal represents a transformative step toward an AI-native, proactive defense strategy, one that anticipates stealthy threats rather than simply reacting to them. As adversaries employ increasingly sophisticated tactics to evade detection across time and systems, tools like Signal provide a promising defense, enabling security teams to recognize the early signs of an attack, piece together patterns, and respond rapidly.

In the future, continued progress in supercomputing and cloud AI will further empower detection engines to remain ahead of attackers, paving the way toward a future where cyber resilience is anchored in intelligence, scale, and speed.

ASU researchers uncover gigantic lightning

A decade-old thunderstorm that stretched across the Great Plains, from eastern Texas to nearly Kansas City—spanning 515 miles—has set a new world record for lightning, as discovered through an advanced global network of antennas located above Earth's surface.

In a recent study led by scientists at Arizona State University (ASU) and published in the Bulletin of the American Meteorological Society, the team re-examined satellite data from October 2017. They identified an astonishing megaflash extending 38 miles longer than the previous record set in April 2020.

From Antennas on Earth to Lightning Mappers in Orbit

Traditionally, lightning networks have relied on ground-based antenna arrays scattered across regions to locate strikes. However, this megaflash could only be fully mapped using space-based sensors. NOAA’s GOES-16 satellite, the first geostationary satellite equipped with a lightning mapper, joins similar instruments operated by Europe and China, enabling the detection of lightning from orbit.

These lightning mappers function like ultra-precise antennas in space. Each time a flash occurs, the sensors record its origin to the millisecond and trace its horizontal extent across continents.

Weaving Together Petabytes of Flash Data

The volume of data is staggering. GOES-16 detects about one million flashes each day, with each flash logged by time, location, and geographic extent. This massive stream of data must be continuously processed to identify the rare megaflashes, which are defined as exceeding approximately 100 kilometers (60 miles) in length.

Michael Peterson at Georgia Tech, the lead author of the published report, explains that modern data-processing techniques are essential. They sift through the vast number of ordinary lightning flashes, connecting fragmented pulses that belong to the same extended stroke. Only then can researchers reconstruct the full scale of these flashes, which can span hundreds of miles.

Networks of Antennas at Multiple Scales

Imagine dozens of satellite antennas, including GOES-16 in geostationary orbit and its counterparts operated by European and Chinese agencies. Together, they create a continuous, overlapping network of detection. Because these satellites cover most storm regions globally, even sprawling flashes can be captured in great detail.

While traditional ground networks are still useful for finer localization and cross-validation, the real breakthrough lies in the ability to measure continent-sized flashes from space.

Why It Matters—in Curiosity and Science

Fewer than 1% of thunderstorms produce megaflashes, which typically develop over more than 14 hours and cover areas the size of New Jersey. Capturing these rare phenomena allows scientists to explore storm dynamics and extreme weather from a new perspective.

Cerveny, a rapporteur for weather and climate extremes at the World Meteorological Organization, states, “It is likely that even greater extremes still exist.” As satellite systems advance and data archives grow, our ability to detect increasingly longer lightning events continues to improve.

In Summary

Satellites act as a network of space-based antennas, capturing lightning with millisecond precision and continental coverage. Advanced data-processing pipelines analyze millions of flash events each day, enabling the reconstruction of rare megaflashes that stretch across hundreds of miles. Ground networks still play a role, but the true advancement lies in the synergy of multiple satellites, assisting researchers in finding and analyzing the planet’s most extreme electrical events.

ASU’s work illustrates how innovations in detection and processing are redefining the limits of what we thought lightning could achieve—stretching across nations.