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AI agents search 1.9 billion protein clusters, discover a new biological system
AI agents search 1.9 billion protein clusters, discover a new biological system
AI’s trillion dollar compute race hits a hard limit: There isn’t enough power
AI’s trillion dollar compute race hits a hard limit: There isn’t enough power
Supercomputing turns dark-matter waves into a testable prediction
Supercomputing turns dark-matter waves into a testable prediction
Alibaba’s superintelligence ambition puts supercomputing at the center of the AI race
Alibaba’s superintelligence ambition puts supercomputing at the center of the AI race
Japanese supercomputer recreates the birth of the Universe’s monster black holes
Japanese supercomputer recreates the birth of the Universe’s monster black holes
China’s supercomputing push meets a harder problem: Teaching computers to keep asteroids honest
China’s supercomputing push meets a harder problem: Teaching computers to keep asteroids honest
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AI agents search 1.9 billion protein clusters, discover a new biological system
Featured

AI agents search 1.9 billion protein clusters, discover a new biological system

Tyler O'Neal, Staff Editor September 25, 2026, 1:00 pm

Autonomous scientific computing turns genome mining into an adaptive HPC workload, using 949 agent sessions, 60 CPU cores, GPU-accelerated structure prediction, and more than 215 million tokens to uncover a previously unknown family of reverse transcriptases.

For decades, a central challenge in computational biology has been deceptively simple to articulate: the volume of biological data far exceeds the capacity for human analysis. While modern metagenomic databases contain billions of uncharacterized protein sequences, conventional computational pipelines remain limited by their reliance on predefined search criteria, effectively restricting discovery to what researchers already know how to describe.

Recent research from Anthropic proposes an alternative paradigm. By moving beyond fixed analytical pipelines, the researchers developed an autonomous system wherein AI agents can search, analyze, self-critique, and initiate iterative computational tasks to investigate unexpected observations. In this study, the system surveyed approximately 1.9 billion protein clusters, ultimately identifying a novel family of reverse transcriptases associated with tandem DNA repeat arrays, which the team has termed array-associated reverse transcriptases (ART).

While this discovery is biologically significant, the underlying computing architecture offers a compelling advancement for high-performance computing (HPC). Rather than a singular AI model addressing a solitary query, the system functioned as an orchestrated scientific workload. Over 21.5 hours of wall-clock time, the campaign executed 119 research tasks and 949 agent sessions, totaling 215.6 million tokens, all without human intervention. The infrastructure utilized 58 concurrent sessions within a sandbox environment featuring 60 CPU cores and 192 GiB of memory, while offloading specialized structure prediction tasks to NVIDIA A100 and L4 GPUs. This experiment illustrates a shift in HPC workloads, moving from conventional batch processing toward dynamic, exploratory scientific computing.

From fixed pipelines to computational exploration

Traditional genome mining is extraordinarily powerful.

Researchers can construct profile hidden Markov models, search enormous sequence databases, cluster homologous proteins, build phylogenetic trees, and examine genomic neighborhoods. These operations are highly amenable to parallel computing.

But there is a fundamental limitation.

A conventional pipeline has to be told what constitutes an interesting result.

If the software is searching for a particular protein family, genomic architecture or sequence motif, the pipeline is optimized around those expectations. Anything that falls outside the predefined feature set may simply be classified as noise.

The researchers behind the study describe this as a novelty problem.

A human scientist looking at a sequence can notice something that was not part of the original search specification: an unusual repeat, a strange genomic neighborhood or an unexpected combination of molecular components.

The question was whether an AI-driven computational system could perform some of that exploratory work at database scale.

The answer, in this experiment, was yes, but with important qualifications.

The system did not simply unleash a language model on 1.9 billion sequences.

It constructed a hierarchy of computational agents.

A launch agent converted the research brief into stages. Worker agents performed individual analyses. Supervisor agents reviewed their plans and results. Curator agents placed findings into a shared knowledge base. Editor agents reviewed reports.

Most importantly, observations could generate new work.

Of the 119 tasks in the campaign, agents proposed 98 follow-up tasks. Those tasks entered a triage queue, where the research harness could release or reject them.

That creates a very different computational model from a conventional workflow.

Instead of: input → fixed pipeline → output the architecture becomes: input → analysis → observation → new task → analysis → new observation → new task

The compute graph can therefore change as the science develops.

For HPC architects, that distinction is crucial.

1.94 billion protein clusters become a compute problem

The initial search was enormous.

The agents assembled reverse-transcriptase profile HMMs and searched approximately 1.94 billion protein clusters.

That produced approximately 198,290 RT clusters after filtering, which were classified into nine RT classes.

The system then examined approximately 10,983 RT loci and evaluated 3,564 recurring protein families in their genomic neighborhoods as potential partner genes.

Sixteen candidate families passed the initial criteria and were assigned dedicated investigations.

An additional candidate emerged from follow-up work.

The campaign ultimately produced 19 reports, including reports on candidate partner families and three newly identified RT lineages.

Only three of the 17 candidate partner families survived as previously unreported RT associations.

That rejection rate is important.

The system was not simply programmed to turn every unusual observation into a discovery. It had to eliminate annotation artifacts, previously characterized systems and proteins that merely happened to occur nearby.

That is where the computational workflow begins to look increasingly like an HPC-enabled scientific laboratory.

The infrastructure behind the agents

The study’s autonomous research harness was built around Claude Code instances configured with Claude Mythos 5.

The computational environment permitted up to 58 concurrent sessions.

The sandbox itself contained:

  • 60 CPU cores
  • 192 GiB of memory
  • No GPU

The absence of GPUs in the main sandbox is itself revealing.

The dominant workload was not neural-network training or large-scale inference performed locally on an accelerator. Much of the work consisted of conventional scientific computing: sequence searches, data manipulation, clustering, alignment, phylogenetic analysis, scripting, file processing and database queries.

The agents could execute software including HMMER, MMseqs2, BLAST+, MAFFT, FastTree, SeqKit, skani, geNomad, Infernal, ViennaRNA and other computational biology tools.

For structural analysis, the workflow could dispatch jobs to external GPU resources.

The researchers report 19 GPU jobs on NVIDIA A100 and L4 GPUs, using ESMFold or ColabFold with AlphaFold2-based models.

That is a classic heterogeneous HPC pattern.

CPU resources handled broad exploration and data analysis.

GPU resources were brought into the workflow when the problem demanded computationally expensive protein-structure prediction.

The AI agents effectively became a workload-management layer sitting above a collection of scientific-computing tools.

The numbers tell the HPC story

The campaign generated:

119 research tasks

949 agent sessions

77 agent-hours

215.6 million tokens

21.5 hours of wall-clock time

7,578 shell commands

696 database queries

131 literature searches

61 web requests

That workload is fundamentally different from a traditional supercomputing simulation.

There is no single enormous MPI job running for several hours across thousands of nodes.

Instead, the workload consists of many relatively independent, heterogeneous and dynamically generated tasks.

Some are computational.

Some are database operations.

Some involve text and literature.

Some involve sequence analysis.

Some invoke GPUs.

Some produce additional work.

And some terminate because the hypothesis is rejected.

This looks less like a conventional batch queue and more like a scientific task graph whose topology is discovered during execution.

That could become an important class of HPC workload.

Then the AI noticed something it wasn’t specifically looking for

The most consequential observation emerged from an investigation that was not originally designed to find the ART system.

The research campaign was primarily looking for previously unknown associations between reverse transcriptases and partner protein-coding genes.

One RT lineage, however, contained an unusual feature in the noncoding DNA upstream of the RT.

An agent retrieved the actual DNA sequence.

And instead of merely processing a predefined annotation, the agent examined the sequence directly.

It noticed a repeating pattern.

The worker identified tandem repeats approximately 16–17 nucleotides long, separated by spacers roughly 100–200 nucleotides long.

One locus contained 14 copies of a 16-nucleotide repeat.

The pattern looked sufficiently unusual that the agent began comparing it with known systems, including CRISPR-like arrays, retron-related architectures and other repeat-associated mechanisms.

It then performed a novelty investigation.

The repeat architecture did not match previously reported features.

That observation became the starting point for the ART discovery.

This is perhaps the most interesting computational moment in the entire study.

The system found something that the original research specification had not explicitly asked it to find.

The discovery emerged from looking at the data, rather than merely matching the data against a predefined list of expected features.

Why context mattered

The researchers subsequently tested whether the AI models could recognize the unusual repeat arrays when given different amounts of information and different tools.

The results expose an important limitation, and an important opportunity.

The strongest models could recognize the ART array when the DNA sequence itself was placed directly into their context.

But giving the model more tools did not automatically make it better at recognizing the repeat architecture.

In some benchmark conditions, performance actually declined.

The researchers found that a major factor was whether the model actually read enough DNA sequence.

When at least 200 nucleotides of contiguous DNA were read into context, repeat recognition increased substantially.

For the pooled group of four most capable models, recognition increased as progressively larger amounts of DNA were brought into context, reaching as high as 76% of attempts in the reported bins and as high as 96% for Mythos 5 in the largest-context condition.

The implication is striking for scientific AI infrastructure.

Giving an agent access to a tool is not the same thing as giving it the information contained in the tool’s output.

A filesystem can contain thousands of nucleotides, millions of rows, or gigabytes of scientific data. The agent still has to decide what to inspect.

That makes data movement, context construction, and intelligent I/O part of the computational problem.

For future scientific AI systems, the bottleneck may not always be FLOPS.

It may be what information the agent chooses to bring into its working context.

From sequence anomaly to biological system

Once the unusual architecture was identified, the researchers expanded the computational investigation.

The ART systems turned out to occur primarily in jumbo phages and to contain three recurring components: an RT protein, a tandem repeat array, and a partner gene.

The researchers examined 95 ART members and additional phage loci.

Computational analysis showed that the repeat arrays were not simply random sequence repetitions. Their spacing, conservation and organization distinguished them from shuffled controls.

Phylogenetic analyses placed the ART proteins in a distinct family.

The researchers also identified three major partner-protein types.

Type I systems were associated with a protein of roughly 600 amino acids containing two tandem GNAT-like folds.

Type II systems occurred in a Staphylococcus phage lineage and encoded an approximately 270-residue all-helical protein.

Type III systems encoded a smaller, approximately 170-residue helical protein in one environmental lineage.

The three partner families showed no obvious sequence or predicted-structure similarity to one another.

That suggests the RT family may have been paired with unrelated partner proteins multiple times during evolution.

Again, much of this characterization depended on computational infrastructure.

Sequence clustering and homology searches narrowed the candidate universe.

Multiple sequence alignment and phylogenetic tools established evolutionary relationships.

Structure-prediction systems provided additional evidence about protein architecture and possible RT-partner interfaces.

The CPU and GPU workloads were therefore not competing alternatives.

They were complementary stages of the same scientific pipeline.

The GPU was not the discovery engine, it was part of the investigation

This distinction is worth emphasizing.

It would be easy to describe the work as an AI supercomputer discovering a new molecular system.

That would obscure how the computation actually worked.

The initial genome-scale search relied heavily on sequence analysis tools and CPU resources.

The GPU resources were used for specialized structural prediction.

That division is representative of the emerging architecture of scientific AI.

The future supercomputing system may not be dominated by a single accelerator type.

Instead, a scientific workload could move repeatedly between: CPU search → database → agent reasoning → CPU analysis → GPU prediction → CPU comparison → agent interpretation → new task

The scheduler becomes more important because the application itself determines what it needs next.

The workload is no longer completely known before execution begins.

The shared knowledge base becomes a new kind of scientific memory

Another important architectural feature was the shared knowledge base.

After each task, a curator agent reviewed the work and entered findings into a common record.

Later agents received relevant entries in their prompts.

Plans, results, reviews, and scripts were also maintained in a version-controlled record accessible to the agents.

This effectively created a persistent computational memory for the research campaign.

In HPC terms, it resembles a combination of workflow state, provenance database, experiment log and shared scientific scratch space, but with the contents actively influencing future computation.

That is potentially a major architectural direction for agentic science.

A traditional HPC workflow generally has explicit inputs and outputs.

An agentic workflow needs something more.

It needs to remember:

  • what has already been tested;
  • which hypotheses failed;
  • which datasets produced useful evidence;
  • which computational tools were successful; 
  • which observations deserve follow-up;
  • what another agent has already learned.

Without that shared state, dozens or hundreds of agents would simply duplicate each other’s work.

The database therefore becomes part of the intelligence of the system.

A supercomputer that changes the question

Perhaps the most inspiring aspect of the study is not that AI found another protein family.

It is that the computational system changed the question being asked.

The original mission focused on RT partner genes.

The important discovery emerged from noncoding DNA.

An agent saw a pattern that existed outside the original feature specification and created a new investigative path.

That is a subtle but potentially profound change in scientific computing.

For generations, supercomputers have excelled at executing questions defined by humans.

Scientists formulate a model.

They construct the equations.

They select the parameters.

They define the search space.

The machine explores that space at extraordinary speed.

Agentic scientific computing suggests another model: the machine can help explore what the search space should have been.

That does not mean the machine becomes the scientist.

It means the computational system can participate in identifying anomalies that deserve human attention.

And that distinction matters.

The discovery still requires science beyond the computer

The study should not be interpreted as proof that an AI independently solved the biological function of ART.

The computational evidence is substantial, but the biological mechanism remains incompletely understood.

The researchers observed that ART arrays produce discrete RNAs and that these RNAs can be highly expressed during phage infection. They also observed corresponding RNA production when ART systems were expressed in E. coli.

Those observations support the hypothesis that the arrays generate a repertoire of RNA molecules.

But the exact biological function of the ART system remains an open question.

The researchers have not established the complete biochemical mechanism by computational analysis alone.

That is where laboratory experimentation remains essential.

This is an important boundary for autonomous scientific computing.

AI can search.

AI can classify.

AI can notice anomalies.

AI can generate hypotheses.

AI can design follow-up analyses.

But the distinction between a compelling computational hypothesis and an experimentally established biological mechanism remains fundamental.

The next HPC workload may be adaptive

For supercomputing centers, the ART study points toward a workload category that could become increasingly common.

Scientific computing has traditionally been organized around relatively predictable workloads.

A researcher submits a simulation.

A scheduler allocates resources.

The computation runs.

Results are returned.

Agentic science introduces a feedback loop.

A computation produces an observation.

The observation changes the next computation.

The next computation may require a different resource.

A CPU-intensive search might trigger a GPU structure prediction.

The structure prediction might trigger another sequence search.

That result might launch a literature search.

The literature search might trigger a new biological hypothesis.

The hypothesis might generate dozens of additional jobs.

The workload becomes adaptive rather than predetermined.

That creates difficult problems for HPC infrastructure.

Schedulers will need to deal with bursts of short-lived tasks alongside traditional large jobs.

Resource managers may need to coordinate CPU, GPU, memory, and storage allocations dynamically.

Workflow systems will need robust checkpointing and provenance.

Data-management systems will need to move information rapidly between persistent databases, compute nodes and AI context windows.

And scientific users will need ways to reproduce an agent’s decisions, not simply reproduce the final executable.

From FLOPS to scientific decisions

For years, supercomputing performance has been measured in familiar units: FLOPS, bandwidth, latency, memory capacity and energy efficiency.

Those metrics remain essential.

But autonomous scientific computing introduces another dimension.

How efficiently can a machine decide what computation should happen next?

That is a very different performance question.

The ART campaign processed nearly two billion protein clusters, but the important computational achievement was not brute-force enumeration alone.

It was the ability to progressively reduce that enormous search space while retaining the possibility of following an unexpected clue.

The system moved from approximately 1.94 billion clusters to roughly 198,000 RT clusters, then to approximately 11,000 loci, thousands of candidate partner families, and ultimately a much smaller set of biological systems worthy of deep investigation.

The computational hierarchy became a scientific funnel.

At every stage, compute reduced uncertainty.

And occasionally, an unexpected observation widened the funnel again.

That is precisely what makes the workload interesting for HPC.

The beginning of autonomous discovery infrastructure

The study regarding array-associated reverse transcriptases (ART) does not signify the obsolescence of conventional supercomputing; rather, it represents a pivotal transition toward a new paradigm of scientific machinery. The supercomputer of the future may evolve beyond merely accelerating simulations to orchestrating thousands of heterogeneous computational operations. Such a system would maintain a collective memory of scientific evidence, determine the necessity of further computation, and dynamically route tasks to the optimal hardware.

In this model, CPU cores would manage genome searches, GPUs would facilitate molecular structure prediction, and specialized storage and networking would handle vast sequence repositories and intermediate datasets. AI agents would serve as the decision-making layer, identifying which investigations warrant further resources, while human scientists remain at the forefront to validate emerging discoveries. The ART discovery offers a preliminary look at this architecture, demonstrating how a vast database can be transformed into an active search space and how a suite of diverse tools can function as a unified scientific instrument. Ultimately, the next generation of supercomputing will likely transcend simple calculation, increasingly assisting researchers in discerning which scientific questions are truly worth pursuing.

AI’s trillion dollar compute race hits a hard limit: There isn’t enough power
Featured

AI’s trillion dollar compute race hits a hard limit: There isn’t enough power

Tyler O'Neal, Staff Editor September 24, 2026, 10:00 am

For years, the artificial intelligence industry has focused on a deceptively simple question: how many GPUs can be integrated into a single data center? However, an increasingly critical challenge has emerged that can no longer be ignored: securing the electricity required to power these systems. This question is now fundamentally shaping the future of supercomputing.

The urgency of this issue is highlighted by Oracle’s Project Jupiter in New Mexico, a cornerstone of the collaborative Stargate infrastructure initiative involving Oracle, OpenAI, and SoftBank. Oracle has issued a force-majeure notice to the project’s developer, a unit of Blue Owl Capital, citing potential delays in securing sufficient power. While this notice provides contractual flexibility should the 2028 operational target be missed, Oracle maintains that the project remains on schedule.

The implications for the broader supercomputing industry extend far beyond a single facility or financing arrangement. This situation reveals a fundamental systemic risk within the current AI infrastructure boom: it is becoming significantly easier to acquire computational capacity than to secure the physical infrastructure necessary to power it.

The supercomputer is no longer just a computer

Traditional supercomputing discussions tend to revolve around familiar metrics: FLOPS, accelerator count, memory bandwidth, network bandwidth, storage throughput, and application performance.

Those metrics remain critical.

But an AI supercomputer also has another specification that is becoming just as important: Megawatts.

Modern AI clusters are effectively enormous distributed computing systems. Thousands of accelerators must operate simultaneously, connected by extremely high-bandwidth networks and supported by storage, cooling, and power-conversion infrastructure.

The result is a system whose computational performance is inseparable from its physical infrastructure.

A facility may have the latest accelerators available.

It may have the network fabric.

It may have the cooling system.

It may even have customers waiting for compute capacity.

But if the electrical infrastructure is not ready, the supercomputer does not exist in any meaningful operational sense.

It is simply an expensive collection of hardware waiting for electrons.

Project Jupiter Makes the Problem Concrete

Project Jupiter illustrates the scale of the challenge.

The New Mexico campus is designed as a massive AI computing facility. Recent reporting puts its planned power requirement at roughly 2.45 gigawatts, with the current design centered on Bloom Energy fuel cells operating as an onsite microgrid. 

That is not a conventional data-center power requirement.

It is an industrial-scale energy system attached to a computing system.

And the power infrastructure itself has become a critical-path component.

A natural-gas pipeline intended to supply the facility has faced regulatory setbacks and a delay. TechCrunch reports that the pipeline schedule has moved to February 2027, while a separate air-quality permit for the fuel-cell system remains pending. 

Oracle’s own June description of the revised design says the company moved away from the previously planned gas-turbine and diesel-generator configuration toward Bloom Energy fuel-cell technology. Oracle says the revised system is intended to reduce water consumption and nitrogen-oxide emissions while providing reliable onsite power. 

That engineering evolution is important.

It also demonstrates the uncomfortable reality of AI infrastructure: The power system can become as complicated as the computer system.

When megawatts become a computing specification

Consider what happens inside a large AI cluster.

An accelerator performing a computation consumes electrical power.

Thousands of accelerators multiply that requirement.

Then add CPUs, memory systems, high-speed networking, storage, power-conversion losses, cooling equipment and facility overhead.

The electricity requirement becomes enormous.

And unlike purchasing additional GPUs, increasing electrical capacity is not simply a matter of placing another order.

Power infrastructure requires physical construction.

Transmission capacity may have to be expanded. Substations must be built. Generation resources have to be secured. Fuel infrastructure may be required. Permits have to be obtained. Cooling systems must be engineered. Communities and regulators may have to approve the development.

Those processes operate on very different timescales from the semiconductor industry.

A new accelerator generation can arrive in months.

A major power project can take years.

That mismatch is becoming one of the central infrastructure problems of the AI era.

The GPU supply chain may not be the only bottleneck

The technology industry has spent enormous resources expanding accelerator production.

That effort has created another race: the race to build facilities capable of deploying those accelerators at scale.

This changes the economics of supercomputing.

If a company can acquire 100,000 accelerators but cannot energize the corresponding computing facility, those accelerators do not produce useful AI capacity.

The limiting resource has shifted from silicon alone to the entire infrastructure stack.

Compute availability = accelerators + memory + networking + storage + cooling + power + facility.

Remove any one of those components and the system’s theoretical performance becomes irrelevant.

For AI infrastructure developers, this creates a dangerous possibility: billions of dollars can be committed to computational capacity before the physical infrastructure necessary to operate that capacity is fully secured.

Project Jupiter demonstrates precisely why that matters.

The financing problem follows the power problem

There is another layer to this story.

The AI infrastructure boom is being financed at a scale rarely seen in computing.

Project Jupiter reportedly has approximately $18 billion in loans tied to its development, while Blue Owl has committed roughly $3 billion in equity to the New Mexico project, according to reporting from The Information. 

Reuters reported last week that the $18 billion in loans had come under pressure, with portions quoted around 89 to 91 cents on the dollar amid concerns about the project’s regulatory and infrastructure challenges. 

That does not mean the project has failed.

It does, however, demonstrate how the physical risks of AI infrastructure can become financial risks.

If a supercomputer takes longer than expected to come online, capital remains tied up.

If power infrastructure is delayed, the facility cannot generate the expected computing capacity.

If construction costs rise, financing requirements increase.

If customer commitments depend upon a particular operational date, delays can ripple through the entire AI infrastructure ecosystem.

The computer may be digital.

The risk is not.

The AI factory has become an energy factory

There is a conceptual shift taking place in the industry.

The next generation of AI facilities should perhaps no longer be thought of simply as data centers.

They are AI factories.

They convert electricity into computation.

Electricity enters the facility.

Accelerators transform that energy into mathematical operations.

Networks move data between processors.

Memory systems feed the calculations.

Storage provides the datasets.

Cooling removes the resulting heat.

The output is computational capacity.

From that perspective, electricity is not merely an operating expense.

It is one of the fundamental raw materials of AI.

That makes the availability of electricity a direct determinant of how much AI computation a company can actually deliver.

Efficiency suddenly matters more

This also changes the meaning of performance optimization.

Historically, HPC engineers have pursued better performance for familiar reasons: finish the simulation sooner, increase throughput, reduce queue times or solve larger problems.

AI adds another dimension: How much computation can be produced per megawatt?

That question could increasingly influence processor architecture, cooling technology, interconnect design, scheduling software, and even algorithms.

A cluster that delivers more useful work per watt can effectively provide more computational capacity without requiring proportional increases in generation and transmission infrastructure.

This is where traditional HPC engineering becomes particularly relevant.

Techniques developed to maximize utilization of supercomputers, workload scheduling, accelerator efficiency, communication optimization, memory locality, precision reduction, and application-specific optimization, suddenly have an infrastructure-level economic consequence.

Every percentage point of efficiency can represent substantial avoided power consumption when multiplied across hundreds of megawatts.

The hidden supercomputer bottleneck

The industry has become accustomed to thinking about AI bottlenecks in terms of GPUs.

Then came high-bandwidth memory.

Then networking.

Then advanced packaging.

Now another bottleneck is becoming increasingly visible: The grid.

Project Jupiter is not proof that the AI industry has run out of electricity.

It is evidence that obtaining enough reliable power, in the right location and on the required schedule, is becoming a major engineering and infrastructure challenge for hyperscale AI.

That distinction matters.

Oracle maintains that Project Jupiter remains on schedule, and the company has invested heavily in a revised onsite power strategy. Oracle also says it will fund the project’s energy infrastructure and electricity costs rather than shifting those costs to local residents. 

But the fact that power availability has become important enough to appear in a force majeure notice should get the attention of anyone planning the next generation of AI supercomputers.

The Clock Is Running

There is an uncomfortable mismatch at the heart of the AI boom.

The semiconductor industry is accelerating.

AI models are growing.

Demand for inference is expanding.

Training clusters are becoming larger.

Hyperscalers are announcing increasingly ambitious AI infrastructure programs.

But electrical infrastructure cannot necessarily move at the same speed.

The industry can announce a gigawatt-scale AI campus today.

That does not mean the electrons will be available tomorrow.

And without those electrons, the promised FLOPS remain theoretical.

This is why Project Jupiter deserves attention from the supercomputing community.

The story is not fundamentally about Oracle’s stock price, Blue Owl’s investment or one delayed pipeline.

It is about whether the physical infrastructure of the world’s computing systems can keep pace with the computational ambitions of the AI industry.

The next supercomputing race may be measured in megawatts

For decades, progress in supercomputing was primarily measured in FLOPS. Over time, the industry’s focus expanded to include memory bandwidth, interconnect performance, storage throughput, and energy efficiency. Currently, however, a critical new metric has emerged: available power. The next generation of supercomputing facilities may be constrained not by the density of processors, but by the volume of megawatts that can be reliably delivered to the site. This introduces a significant uncertainty into the trillion-dollar AI infrastructure race. 

While the industry may possess sufficient chips, capital, customers, and data, these assets remain dormant without the necessary electricity to power them. Ultimately, the future of artificial intelligence may depend on a fundamental infrastructure challenge: whether we can scale power generation in alignment with our computational ambitions.

Artist's impression illustrating how wave-like density patterns produced by ultralight dark matter could warp space and alter the path of light from a distant source. As the light travels past the lensing object on its way to Earth, it follows a distorted path shaped by the surrounding mass distribution. The reflective sphere symbolizes the still-unknown nature of dark matter. The image was created using 3D computer graphics software. Credit: Amruth Alfred
Artist's impression illustrating how wave-like density patterns produced by ultralight dark matter could warp space and alter the path of light from a distant source. As the light travels past the lensing object on its way to Earth, it follows a distorted path shaped by the surrounding mass distribution. The reflective sphere symbolizes the still-unknown nature of dark matter. The image was created using 3D computer graphics software. Credit: Amruth Alfred
Featured

Supercomputing turns dark-matter waves into a testable prediction

Deckard, Staff Editor September 23, 2026, 9:00 am

Direct Schrödinger–Poisson simulations generate 1,000 three-dimensional fuzzy-dark-matter halos and demonstrate how high-performance computing can turn an exotic particle hypothesis into an observational test

Determining the nature of dark matter, specifically whether it consists of conventional cold, massive particles or ultralight quantum waves, remains one of the most formidable and computationally intensive challenges in modern cosmology. 

A recent study published in The Astrophysical Journal Letters (https://iopscience.iop.org/article/10.3847/2041-8213/ae9a9e) demonstrates how high-performance numerical simulations can transition this inquiry from theoretical speculation to an observationally testable framework. Jiajun Zhou and his collaborators conducted the first calculations of gravitationally lensed images derived directly from three-dimensional fuzzy-dark-matter (FDM) density fields, evolved via the Schrödinger–Poisson equations. By computationally evolving the dark-matter wave field rather than relying on statistical approximations, the researchers were able to predict how these quantum structures perturb the images of distant, gravitationally lensed quasars. 

This work marks a significant computational milestone, as it effectively tests whether the intricate structures generated by quantum wave evolution persist through numerical processing to produce observable consequences that align with astronomical measurements. While these findings provide encouraging support for the fuzzy-dark-matter hypothesis, the authors emphasize that further research is essential to fully validate these results.

From particles to waves

Fuzzy dark matter, also called wave dark matter, proposes that dark matter is composed of extremely light particles whose quantum-mechanical de Broglie wavelengths can become comparable to astrophysical scales.

For a particle mass of 10⁻²² electronvolts, the characteristic de Broglie wavelength in the simulated galaxy-scale system is roughly 100 parsecs. That is an extraordinary scale for a quantum effect: roughly hundreds of light-years.

At these scales, the dark-matter halo cannot be treated simply as a collection of classical particles.

It must be treated as a coherent wave field.

That changes the computational problem fundamentally.

The researchers solve the coupled Schrödinger–Poisson equations, in which the complex wave function describes the FDM field while the gravitational potential is obtained from the density generated by that field.

The density is proportional to the squared magnitude of the wave function:

[
\rho = M|\psi|^2.
]

The gravitational field generated by that density then feeds back into the evolution of the wave itself.

This creates a nonlinear, self-gravitating wave problem.

It is precisely the kind of problem for which numerical resolution and algorithmic efficiency become inseparable from the scientific result.

A 512³ computational grid

The researchers employ a global Fourier pseudospectral method.

The choice is important from an HPC perspective.

Pseudospectral methods represent the field in Fourier space and can achieve high spectral accuracy for smooth wave fields while reducing numerical diffusion. The paper states that this approach is particularly suitable for the galaxy-scale lensing problem being investigated.

The production calculations use a 512³ grid, equivalent to more than 134 million spatial cells.

The simulation volume is a cube approximately 40 kiloparsecs on a side, and each realization is evolved for approximately 3.3 billion years of physical evolution time. The simulations use a total dark-matter mass of approximately 4 × 10¹¹ solar masses and investigate particle masses of 10⁻²² and 10⁻²³ eV.

The grid resolution is not arbitrary.

The researchers require the computational cell size to be smaller than the de Broglie wavelength, with several cells needed across the wavelength to resolve the interference pattern.

The grid must also resolve the physical scale corresponding to the observed tens-of-milliarcsecond positional anomalies in the gravitationally lensed system.

This is a classic HPC constraint: the physics dictates the resolution, and the resolution dictates the computational cost.

Reducing the cell size increases the number of grid points in three dimensions rapidly. A modest increase in linear resolution therefore produces a much larger increase in memory requirements and computational work.

1,000 universes inside the computer

Perhaps the most revealing computational figure in the study is not 512³.

It is 1,000.

The researchers generated 1,000 independent initial conditions, each constructed from five randomly distributed three-dimensional Gaussian wave packets.

Every realization was then evolved through the full Schrödinger–Poisson calculation to produce an independent three-dimensional fuzzy-dark-matter halo.

This transforms the project from a single numerical experiment into a statistical computational campaign.

The objective is not merely to produce one halo that happens to resemble the observations.

Instead, the researchers ask how often the structures naturally generated by the underlying equations produce lensing configurations compatible with the observed system.

That distinction is important.

A single simulation can demonstrate possibility.

A large ensemble begins to address probability.

The computer must preserve the wave physics

Numerical integration becomes particularly important because the researchers are not simply tracking the motion of individual particles.

They are evolving a wave field whose phase and interference structure matter.

The simulations therefore use a split-step pseudospectral method. During each time step, the kinetic and gravitational-potential operators are applied separately. The time step is constrained by the fastest phase oscillations associated with the kinetic and gravitational terms, with a safety factor imposed to avoid phase aliasing.

That is an HPC issue as much as a physics issue.

A simulation can run faster by taking larger time steps or using lower spatial resolution.

But if those shortcuts erase physically relevant wave structure, the resulting gravitational lensing prediction can become numerically precise but physically wrong.

The researchers instead make the numerical resolution part of the physical model.

From a three-dimensional supercomputer field to a two-dimensional sky

The computational workflow does not end when the dark-matter halo has been evolved.

The researchers then have to turn the three-dimensional simulation into an observable lens.

For each simulated halo, they determine its principal axis and rotate the three-dimensional density field through representative viewing directions.

The density is projected along the line of sight to generate a two-dimensional convergence map, after which the gravitational lens equation is solved to generate simulated image positions. The open-source lenstronomy package performs the lensing calculations.

This creates a computational pipeline that can be summarized as: wave equation → gravitational potential → three-dimensional density field → viewing geometry → projected mass → lens equation → multiple images → statistical comparison with observations.

The researchers sample 103 representative viewing directions and 10⁴ source positions during the forward-modeling process.

At this point, the project begins to resemble a modern scientific computing workflow more than a conventional analytic astronomy calculation.

The supercomputer is effectively generating synthetic observations from first-principles numerical evolution.

Matching the geometry without fitting away the physics

The study introduces another computationally interesting element.

The researchers compare the simulated and observed four-image configurations using pairwise-distance invariants and Procrustes alignment.

This allows translations, rotations, and reflections that do not represent physical differences to be removed from the comparison.

For four images, the six pairwise distances provide a complete set of geometric invariants for the relative configuration. The researchers use these distances to identify the source position that best reproduces the observed geometry and then apply Procrustes alignment to quantify the remaining image-position anomaly.

That is an important numerical safeguard.

Without it, the calculation could incorrectly interpret a simple coordinate-frame difference as evidence that the dark-matter model is wrong.

The computational machinery therefore has to be careful not only about solving the equations, but also about comparing the output with observational data in a statistically meaningful way.

The result: wave simulations reproduce the observed lens

The target is HS 0810+2554, a quadruply lensed quasar system containing two compact radio sources.

High-resolution radio observations have measured eight lensed radio images with sufficient astrometric precision to expose discrepancies between the observations and smooth conventional lens models.

For fuzzy dark matter with a particle mass of 10⁻²² eV, the wave-evolved halos produce median image-position anomalies of approximately 12 and 6 milliarcseconds for the two radio components.

Some realizations produce anomalies below approximately 3 milliarcseconds, within the roughly 3σ observational uncertainty level used in the analysis.

The comparison is particularly interesting because the simulations are not tuned to force the halos into the observed configuration.

The halos evolve from randomly generated initial conditions.

The researchers report that the wave simulations can reproduce the observed image positions to within approximately 3σ without fitting the internal state of the simulated halo to the observations.

By comparison, the Gaussian-random-field approximation generally produces larger positional fluctuations, while the best-fit smooth NFW model produces substantially larger discrepancies for most of the observed images.

Particle mass becomes a computationally observable quantity

One of the most important results is the sensitivity to the assumed particle mass.

When the researchers reduce the FDM particle mass from 10⁻²² to 10⁻²³ eV, the de Broglie wavelength increases and the resulting density fluctuations occur on larger physical scales.

The simulated lensing position anomaly rises to a median of approximately 50 milliarcseconds, roughly four times the value produced in the 10⁻²²-eV case.

This is precisely where HPC becomes scientifically powerful.

The computer is not merely illustrating a theory.

It is establishing a mapping: particle mass → wave scale → density structure → gravitational potential → image displacement.

That mapping gives astronomers a route toward constraining the mass of a hypothetical dark-matter particle through observations.

The paper concludes that future high-angular-resolution lensing observations could narrow the allowed FDM mass range.

Why Gaussian approximations are not enough

Previous FDM lensing calculations have often relied on Gaussian random fields because they are computationally efficient.

The approach can reproduce broad statistical characteristics of the fluctuations.

But it does not actually evolve the underlying three-dimensional wave system.

The distinction becomes important at higher precision.

The full Schrödinger–Poisson calculation naturally retains spatial correlations, mode coupling, and non-Gaussian higher-order structure generated during the evolution.

The researchers find that Gaussian random fields remain useful as efficient statistical approximations for moderate-precision calculations.

But for precision gravitational-lensing predictions, the direct wave calculation becomes increasingly important.

This is a familiar pattern in computational science.

Reduced-order models can provide enormous computational savings.

But as observational precision improves, the approximations that were once adequate can become the dominant source of error.

The HPC challenge is about to become larger

The authors explicitly acknowledge that full three-dimensional wave simulations are computationally expensive.

Future work will investigate larger simulation boxes and more efficient numerical approaches while preserving sufficient accuracy in the strong-lensing region.

That points directly toward the next generation of HPC requirements.

The current calculation uses a 512³ grid.

Moving toward larger physical volumes while maintaining comparable spatial resolution would increase the number of grid cells dramatically.

Increasing the resolution from 512³ to 1024³, for example, increases the number of spatial cells by a factor of eight.

Moving to 2048³ would increase it by another factor of eight.

And the problem is not simply memory.

Every time step requires large-scale numerical operations, including Fourier transforms and repeated evaluation of the gravitational potential. The long physical integration time compounds the workload.

An ensemble of thousands of realizations would turn the problem into a substantial distributed-computing campaign.

This is precisely where modern HPC architectures, large memory systems, high-bandwidth interconnects, accelerators, distributed FFT libraries and efficient parallel I/O, become critical.

China’s expanding computing ambitions

The scientific work is also part of a broader Chinese computational environment that is placing increasing emphasis on large-scale intelligent and scientific computing.

The research itself includes authors from Beijing Normal University and Tsinghua University, while the paper acknowledges support from China’s National Key Research and Development Program, the National Natural Science Foundation of China and the Strategic Priority Research Program of the Chinese Academy of Sciences.

That institutional investment exists alongside a much broader national effort to expand computing infrastructure.

In June 2026, China’s State Council called for accelerating breakthroughs in key AI technologies and specifically urged construction of ultra-large-scale intelligent computing clusters. 

In September, a separate State Council meeting emphasized that computing networks provide fundamental support for artificial intelligence and called for improved computing infrastructure, coordination between computing capacity and electricity supply, and integration of computing and communications networks. 

China’s information and communications development plan released this month sets a 2030 target of 9,800 EFLOPS of intelligent computing capacity and calls for continued development of a nationwide integrated computing-power network. 

Those targets concern AI and national computing infrastructure rather than the specific astrophysical simulations described in the paper. Nevertheless, they illustrate the scale of the computing environment China is attempting to develop.

For scientific HPC, that matters.

The same fundamental infrastructure required for enormous AI workloads, high-bandwidth memory, accelerators, high-speed networking, storage, and large-scale parallel computing, can also expand the computational envelope available to astronomy, cosmology and fundamental physics.

Supercomputing as an instrument for dark-matter physics

The significance of this work extends beyond the study of fuzzy dark matter, representing a pivotal shift in the field of computational astrophysics. As modern instrumentation provides observations of unprecedented precision, capable of distinguishing between physical models previously obscured by measurement uncertainty, simulations must evolve to achieve commensurate realism. In the context of fuzzy dark matter, this necessitates moving beyond statistical approximations in favor of the direct evolution of the underlying wave field.

In this framework, the supercomputer functions as a laboratory where candidate universes are constructed, simulated, and observed. The study by Zhou et al. illustrates a rigorous numerical pipeline: evolving three-dimensional dark-matter halos, applying varied viewing geometries, projecting these into gravitational lenses, and benchmarking the results against milliarcsecond-scale astronomical data. This approach underscores a fundamental reality of contemporary high-performance computing: scientific advancement increasingly relies not merely on scaling computational capacity, but on resolving governing equations with sufficient fidelity to generate observationally testable predictions. 

Because the universe does not permit direct experimental manipulation of dark-matter particles, researchers must instead construct numerical proxies to evaluate theoretical consequences. By demonstrating that wave-driven gravitational structures produce measurable shifts in quasar images, this research establishes a vital mapping between particle properties and observable phenomena. Future progress will require simulations that are not only larger in scale but also more robust, statistically comprehensive, and deeply integrated with observational data. Ultimately, the trajectory of dark-matter research may depend on the extent to which the current computational frontier can be expanded.

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