Showing posts with label science. Show all posts
Showing posts with label science. Show all posts

Houston We Have a Podcast

Mike's Notes

I just discovered this very interesting NASA podcast. As of today, it has 442 episodes. I'm sharing episode 437: Chris Williams and Neil deGrasse Tyson.

Definitely a podcast to follow. 😎

Resources

References

  • Reference

Repository

  • Home > Ajabbi Research > Library >
  • Home > Handbook > 

Last Updated

27/10/2026

Houston We Have a Podcast

By: 
NASA: 27/10/2026

...

Houston We Have a Podcast is the official weekly podcast of the NASA Johnson Space Center in Houston, Texas. Launched in July 2017 and hosted primarily by Public Affairs Officer Gary Jordan, the show brings listeners into the world of human spaceflight, covering everything from Low Earth orbit to missions heading to the Moon and Mars.

From Earth orbit to the Moon and Mars, explore the world of human spaceflight with NASA each week on the official podcast of the Johnson Space Center in Houston, Texas. Listen to in-depth conversations with the astronauts, scientists and engineers who make it possible.


Cosmic Perspectives with Neil deGrasse Tyson

On episode 437, NASA astronaut Chris Williams and astrophysicist Neil deGrasse Tyson explore human spaceflight, astrophysics, and the wonder of the universe.  This episode was recorded September 1, 2026.

On Being a Scientist: A Guide to the Responsible and Ethical Conduct of Research: Fourth Edition 2026

Mike's Notes

Useful for future reference. The guide can be read freely online.

Resources

References

  • National Academies of Sciences, Engineering, and Medicine. 2026. On Being a Scientist: A Guide to the Responsible and Ethical Conduct of Research: Fourth Edition. Washington, DC: The National Academies Press. https://doi.org/10.17226/29488. 2026. On Being a Scientist: A Guide to the Responsible and Ethical Conduct of Research: Fourth Edition. Washington, DC: The National Academies Press.

Repository

  • Home > Ajabbi Research > Library >
  • Home > Handbook > 

Last Updated

22/10/2026

On Being a Scientist: A Guide to the Responsible and Ethical Conduct of Research: Fourth Edition 2026

By: Megan Lowry
The National Academies of Sciences, Engineering, and Medicine: 17/09/2026

Megan Lowry: Megan Lowry is Manager, Media Relations, of the Office of News and Public Information at the National Academies of Sciences, Engineering, and Medicine.

...

WASHINGTON — The National Academies of Sciences, Engineering, and Medicine today released an update of On Being a Scientist: A Guide to the Responsible and Ethical Conduct of Research. This fourth edition is organized into online, thematic modules, and reflects the evolution of the scientific enterprise since the last version in 2009 by including new topics such as research security and responsible collaboration.

On Being a Scientist introduces students and early-career researchers across disciplines and sectors to the fundamental values that guide responsible research — such as objectivity, honesty, and openness — and explores the increasingly complex research contexts in which they need to be applied. The report was mandated by Congress.

“The research enterprise has changed immensely in recent years because of increasing collaboration, growing global competition, and emerging technologies like AI and CRISPR; these changes offer exciting opportunities for the advancement of science but also raise new ethical questions,” said Michele Masucci, vice chancellor for research and economic development for the University System of Maryland, and co-chair of the committee that developed the guide. “On Being a Scientist is meant to help students and early-career researchers navigate this evolving landscape. We hope the guide will also serve as a framework for responsible research practices for the entire scientific community.”

This guide’s release as online modules rather than as a printed book reflects how users typically access the guide and will make it easier to update going forward. The new edition follows previous printed versions published in 2009, 1995, and 1989.

While directed primarily toward undergraduate and graduate students, postdocs, and early-career researchers, the guide is also useful for faculty who teach research ethics and for established researchers who mentor people in research activities across range of settings — academic institutions, government agencies and laboratories, and industry.

“The dynamic, ever-shifting research environment makes the basic tenets of responsible science — including rigor, integrity, and transparency — even more critical to the effective functioning of the research enterprise and to maintaining public trust,” said National Academy of Sciences President Neil H. Shubin, who co-authored a preface to the new edition with Tsu-Jae Liu and Monica Bertagnolli, the current presidents of the National Academy of Engineering and National Academy of Medicine, along with the immediate past presidents of the NAS and NAM. “This guide is an essential resource to help set norms for ethical conduct and encourage practices that promote the use of science for societal benefit.”

The guide includes an introduction that offers an overview of responsible research and scientific values, together with the following four modules:

  • Collaborating Responsibly provides guidance on collaborating productively across disciplines and institutions, which is increasingly important as the scale and complexity of science grows. This module explores how to enter collaborations intentionally, structure them, manage challenges, and learn from experience.
  • Earning and Maintaining Trust focuses on the daily practices and professional commitments that establish trustworthiness; the institutional structures — including policies, cultures, and accountability measures — that support trustworthy science; and trustworthy communication with the public.
  • Openness and Security offers guidance on navigating the “productive tension” between openness about methods, materials, and data — which is important to evaluating findings and advancing science — and research security, which protects research from misuse, theft, or unintended harm.
  • Responsible Conduct and Stewardship of the Research Process covers the norms and practices of responsible science, such as the judicious use of resources, appropriate oversight and protections for research participants and subjects, prevention of mistakes and negligence, and adherence to norms of ethics and integrity.

“No single resource can fully cover the wide range of situations researchers encounter in their work,” said committee co-chair Alan Leshner, chief executive officer emeritus of the American Association for the Advancement of Science. “On Being a Scientist offers an introduction to these issues and ways to think about them. The goal is to help researchers recognize the relevant considerations when they arise, ask the right questions, and know where to look for further guidance.”

The project — undertaken by the Committee on On Being a Scientist: An Online and Updated Guide to the Responsible and Ethical Conduct of Research — was sponsored by the National Science Foundation, the U.S. Department of Energy, and the Alfred P. Sloan Foundation.

The National Academies of Sciences, Engineering, and Medicine are private, nonprofit institutions that provide independent, objective analysis and advice to the nation to solve complex problems and inform public policy decisions related to science, engineering, and medicine. They operate under an 1863 congressional charter to the National Academy of Sciences, signed by President Lincoln.

Contact:

Megan Lowry
Manager, Media Relations
Office of News and Public Information
202-334-2138; email news@nas.edu

The Martians

Mike's Notes

The Martians is the working title for a long-term publishing and associated screen project currently in Development.

With help from Google Search AI Mode, here is some historical background on some of the main characters (some of whom appeared in Christopher Nolan's film Oppenheimer). This project will be self-funded by the future Ajabbi Foundation.

This project exists because Pipi uses much of the maths and science these people developed.

I read Ananyo Bhattacharya's excellent book, The Man from the Future: The Visionary Life of John von Neumann, last month while researching Hilbert Spaces to add to Pipi in a future release.

The top secret sneaky plan

As part of the forthcoming Pipi documentation going on the Ajabbi websites, these scientists and mathematicians will be featured alongside their insights, including references to read, embedded video, and Jupyter Notebooks. This will happen early on.

As resources allow, this effort will expand to include other scientists of the period, including Einstein, Boltzmann, Planck, Noether, etc., historical reenactments with actors, and the factual historical factors at play.

This science communication resource will be made freely available to all, and can also be used for teaching, exhibitions, documentaries and historical drama for TV, etc.

Redworks

This project is well underway. Redworks will be an initial development vehicle once we quickly sort out some minor legal and tax issues. Initially, the focus will be on "world-building", leading into production design. Scripts will come later.

Update 25/10/2026

The Martians will use the Workspaces for Screen. It will be a good dogfooding test of its capabilities and drive additional useful features.

Update 27/10/2026

Include Euler, Gauss, and Riemann from The Martians' perspective to show how these personalities and continuity shaped the development of maths and physics and the emergence of The Martians.

Euler–Riemann Zeta Function

"If Euler was the master of manipulating infinite series, algebra, and the properties of real numbers, Riemann was the architect who took those exact same equations and projected them into multi-dimensional, complex space." - Wikipedia

Leonard Euler (15 April 1707 – 18 September 1783) was the greatest mathematician who has ever lived and was revered throughout Europe at the time. Bernhard Riemann (17 September 1826 – 20 July 1866) was a student of Carl Gauss, who was deeply influenced by Euler.

Resources

References

  • The Man from the Future: The Visionary Life of John von Neumann by Ananyo Bhattacharya. Penguin (2022).
  • Macrae, Norman (1992). John von Neumann: The Scientific Genius Who Pioneered the Modern Computer, Game Theory, Nuclear Deterrence, and Much More. Pantheon Press. p. 33. ISBN 0-679-41308-1.
  • Marx, George (2001). The Voice of the Martians: Hungarian Scientists Who Shaped the 20th Century in the West. Budapest: Akadémiai Kiadó. ISBN 963-05-7830-1. OCLC 48621487.

Repository

  • Home > Ajabbi Research > Library > Subject > Mathematics
  • Home > Handbook > 

Last Updated

25/10/2026

The Martians

By: Mike Peters
Redworks: 13/10/2026

Mike Peters: Mike invented and designed Pipi and founded Ajabbi.

...

The Martians is a working title for a publishing and associated screen project under development. It is about how a group of Hungarian Jews revolutionised mathematics and physics between the French Revolution and WW2. After the revolutions of 1848, the slow decay of the Austro-Hungarian Empire led to WWI, then to the Russian Revolution, the Stalinist counter-revolution, anti-semitism and the rise of Hitler. The project ends with the start of World War II.

The sudden explosion of genius from late 19th and early 20th-century Budapest is one of the greatest intellectual mysteries of modern history. Historians generally agree that it wasn't a coincidence, but rather the result of a highly specific "perfect storm" of political, educational, and cultural factors unique to the Austro-Hungarian Empire.

Here are the primary reasons why this specific environment bred such extraordinary minds:

1. The Legendary High Schools (Gimnáziums)

The Hungarian secondary education system at the time is widely considered one of the best in human history. Following reforms in the late 19th century, the state established gimnáziums (high schools) modelled after the rigorous German classical system, but with a heavier emphasis on mathematics and hard sciences.

  • Elite Teachers: Because university positions were limited, many world-class scientists and mathematicians taught at the high school level.
  • The "Fasori" Phenomenon: Schools like the Fasori Evangélikus Gimnázium produced John von Neumann and Eugene Wigner in the exact same generation.

2. A Hyper-Competitive Culture of Math

Hungary turned mathematics into a highly prestigious, nationwide competitive sport.

  • The KöMaL Journal: Founded in 1894, this monthly high school mathematics and physics journal published incredibly difficult, creative problems. Students from all over the country mailed in their solutions, which were graded and published. This created a national, collaborative network of young geniuses who pushed each other to their absolute limits before ever reaching university.

  • The Kürschák Competition: This annual, blind-graded mathematics competition identified the country's top talent, turning young mathematicians into national celebrities within academic circles.

3. Jewish Emancipation and the "Golden Age" of Budapest

Following the Austro-Hungarian Compromise of 1867, Jews in the empire were granted full civil rights. This triggered a massive wave of urbanisation, and Budapest quickly grew into a booming, wealthy metropolis.

  • The New Middle Class: Barred from traditional aristocratic roles like landownership or politics, the newly emancipated Jewish population poured their wealth and energy into education, medicine, science, and industry. Most of the "Martians" came from this highly driven, affluent Budapest Jewish bourgeoisie, where intellectual achievement was viewed as the ultimate status symbol.

4. The "Budapest Coffee House" Culture

Much like Vienna, Budapest developed a vibrant coffee house culture. Intellectuals, writers, artists, and scientists did not lock themselves in laboratories; they spent their afternoons in cafes like the New York Café or Café Centrál. Ideas from physics, psychology, literature, and economics were fiercely debated across disciplines, fostering lateral thinking, intense debate, and intellectual agility.

5. A State of Creative Anxiety

The "Martians" grew up in a world of profound instability. They witnessed the collapse of the Austro-Hungarian Empire, a communist revolution, a Stalinist counter-revolution, hyperinflation, and the rapid rise of virulent anti-Semitism and Fascism.

Vienna in the 1930s. The sign, belonging to a gambling parlour, reads: “Don’t let luck pass you by.” A horseshoe and chimney sweep, superstitious symbols of good fortune, appear above it. (Photograph: Roman Vishniac)

  • This created what Eugene Wigner called a "feeling of extreme insecurity" and an awareness that everything they owned could be taken away—except what was inside their minds.
  • This background forced them to be adaptable, highly driven, and comfortable with chaos, traits that proved invaluable when they later had to solve unprecedented problems in wartime America.

"The Martians" (Hungarian: A marslakók) was a nickname for a group of exceptionally brilliant Hungarian physicists and mathematicians who emigrated to the United States in the early 20th century. Most were secular Jewish refugees fleeing Nazi expansion and rising anti-Semitism in Europe.

The name originated as a joke among colleagues like Enrico Fermi and Leo Szilárd. When discussing the Fermi Paradox—asking why there is no evidence of intelligent extraterrestrial life—Szilárd quipped that aliens were already here, but they simply disguised themselves as Hungarians. The moniker stuck because these scientists possessed seemingly superhuman intellects, all grew up within walking distance of each other in Budapest, and spoke English with a thick, matching accent.

Core Members of "The Martians"

While the wider group included up to 23 thinkers, the core group of five distinct "Martians" reshaped modern physics, defence, and computing:

  • John von Neumann (1903–1957): Widely considered one of the greatest mathematicians of the 20th century.
  • Leo Szilárd (1898–1964): The visionary physicist who conceived the nuclear chain reaction.
  • Edward Teller (1908–2003): Theoretical physicist known historically as the "father of the hydrogen bomb".
  • Eugene Wigner (1902–1995): Theoretical physicist who won the Nobel Prize in Physics in 1963.
  • Theodore von Kármán (1881–1963): A pioneer in aerodynamics and mathematics.
Others included:
  • Denis Gabor: A physicist who won the 1971 Nobel Prize in Physics for inventing holography.
  • John G. Kemeny: A mathematician and computer scientist who co-developed the BASIC programming language.
  • George Pólya: Mathematician
  • Paul Erdős: One of the most prolific mathematicians in human history, known for his eccentric lifestyle and work in combinatorics and number theory.
  • Cornelius Lanczos:
  • Egon Orowan:
  • Franz Alexander:
  • George de Hevesy:
  • George Olah:
  • John Harsanyi:
  • John Polanyi:
  • Paul Halmos:
  • Paul Neményi:
  • Peter Carl Goldmark:
  • Peter Lax:
  • Valentine Telegdi:

Inside Café Josephinum, the convening place of the Vienna Circle

Impact on Science and Mathematics

The Martians did not just contribute to their fields; they laid the bedrock for the technology, national security, and computational infrastructure of the modern world.

  • The Von Neumann Architecture: John von Neumann designed the framework for modern digital computers. He pioneered the system in which data and program instructions are stored in the same memory space—a fundamental structure that nearly all desktop computers, smartphones, and servers still use.
  • Cellular Automata: Von Neumann created the concept of cellular automata, modelling self-reproducing systems on computer screens before the biological role of DNA was even fully understood.
  • The Nuclear Chain Reaction: In 1933, Leo Szilárd conceived the idea of a neutron-driven nuclear chain reaction and patented it.
  • The Manhattan Project: Recognising the threat of Nazi Germany, Szilárd drafted the famous Einstein–Szilárd letter to President Franklin D. Roosevelt, which sparked the creation of the Manhattan Project. Von Neumann, Wigner, and Teller all performed core calculations that made the atomic bomb a reality.
  • Thermonuclear Weapons: Post-WWII, Edward Teller drove the physics and design behind the first hydrogen bomb, fundamentally changing Cold War geopolitics.
  • Aviation & Space Flight: Theodore von Kármán provided the mathematical and scientific foundation for modern aerodynamics. He discovered the Kármán vortex street (fluid dynamics) and helped establish the U.S. Air Force’s research wing.
  • JPL Founding: Von Kármán later co-founded NASA's legendary Jet Propulsion Laboratory (JPL).
  • Game Theory: John von Neumann co-created mathematical Game Theory, publishing Theory of Games and Economic Behaviour. This framework mathematically analyses strategy, risk, and decision-making, transforming modern economics, evolutionary biology, and military strategy.
  • Quantum Mechanics: Eugene Wigner introduced Group Theory into quantum mechanics. His work on the symmetries of atomic nuclei earned him a Nobel Prize.
  • Heuristics and Education: George Pólya wrote How to Solve It, a foundational text that systematically defined how to approach and teach mathematical problem-solving.

Sizing Up the Ghosts in the Machines

Mike's Notes

Very true.

Resources

References

  • Reference

Repository

  • Home > Ajabbi Research > Library > Subscriptions > Santa Fe Institute
  • Home > Handbook > 

Last Updated

15/09/2026

Sizing Up the Ghosts in the Machines

By: David Krakauer
Santa Fe Institute: 01/09/2026

David Krakauer: David Krakauer, President of the Santa Fe Institute.

...

A BEYOND BORDERS column by David Krakauer, President of the Santa Fe Institute.

...


Diagram of the Human Mind , Robert Fludd, 1617, via Public Domain Review

All of science is in the business of exorcism. When philosopher Gilbert Ryle coined “the ghost in the machine” in The Concept of Mind (1949), he was identifying an unnecessary explanatory entity in Cartesian dualism and expelling it. Descartes had posited a res cogitans, a thinking substance categorically distinct from the mechanical body. Ryle diagnosed this as a “category mistake,” and explained it away in the manner an Oxford professor does any superstition: like being shown the colleges, library, and playing fields of the university, and still asking the benighted question, “But where is the University?”

What Ryle did for mind, other sciences have done for their own spectral inhabitants. But the ghosts differ in kind, and so do their rites of exorcism. Physics exorcises supernumerary particles — unnecessary free parameters in pursuit of universality. Biology exorcises redundant processes — divine or teleological agencies. And the sciences of intelligence exorcise imposed patterns — transcendent sources of cognition. Each tradition seeks minimality, yet each means something profoundly different by it.

The deepest ambition of physics has always been to reduce the number of independent facts the universe requires us to accept. Theoretical physicist Eugene Wigner observed that symmetry and invariance principles act as filters on possible theories, eliminating free parameters with a scandalous efficiency. And Einstein’s general relativity derived gravitation from the minimal geometric postulate that spacetime curvature is gravity, eliminating Newton’s action-at-a-distance.

Biology’s ghost was never a free parameter but an agent. Before Darwin, the complexity of organisms demanded an intelligent designer the way a watch implied a watchmaker. On the Origin of Species (1859) performed an exorcism on the demiurge itself and replaced a transcendent creative process with a mechanical one. The ghost to be exorcised is the unnecessary rule, an act of God or Lamarckian inheritance. What remains after exorcism is not the universal parameterization of physics, but a universal mechanism (selection) that operates locally and iteratively.

Alan Turing showed in 1936 that a device of absurd simplicity consisting of a tape, a head, and a finite set of states could compute anything computable. Warren McCulloch and Walter Pitts demonstrated in 1943 that networks of binary threshold neurons could instantiate logical operations. Both of these exorcisms expelled patterns of architectural extravagance that Descartes and his followers had imposed on the mind. David Marr, in his 1969 model of cerebellar cortex, proposed a single, repeating architecture consisting of Purkinje cells trained by climbing-fiber error signals, that could learn arbitrary input–output mappings. Computation of near arbitrary complication could be solved through scale.

Computer scientists build architectures that seek to be spirit-proof. When physicists criticize biology for having too many parameters, they are applying parametric parsimony where processual parsimony is the goal. And when biologists accuse neuroscience of ignoring evolutionary constraint, they are importing processual parsimony into a domain governed by architectural parsimony. Each field is haunted by a different ghost, exists in a different intellectual bardo, each governed by its own rituals.

The old disciplinary ghosts aspired to be ontological, frightening entities posited to occupy ordered states of reality, from which ensuing and more skeptical generations banished them. We now have epistemic ghosts, patterns in large datasets, manifesting as regularities, correlations, and structures, that no human theorist seems to have previously named or noticed. LLMs suggest that we have been haunted by vast domains of regularity, in language, protein folding, weather, and genomics, that are simply too high-dimensional for human intuition to observe but not too complex for a sufficiently scaled statistical model to discern.

The ghosts are multiplying, many of them hallucinations, and scientific exorcists must learn new rites.

— David Krakauer

President, Santa Fe Institute

From the Summer 2026 edition of the SFI Parallax newsletter. Subscribe for our monthly e-Parallax, or email “news at santafe.edu” to request quarterly home delivery in print.

10 Pioneers Who Changed Our Understanding of Nature

Mike's Notes

I agree, it's not your formal qualifications that matter; it's your contributions. Many self-taught people, or "amateurs," have made great discoveries. I discovered this article via a Knowable Magazine article about Narwhal tusks and who was figuring them out. In this case, a dentist with a side passion.

Resources

References

  • Reference

Repository

  • Home > Ajabbi Research > Library > Subscriptions > Knowable Magazine
  • Home > Handbook > 

Last Updated

26/08/2026

10 Pioneers Who Changed Our Understanding of Nature

By: .
Narwhal Research: 06/02/2025

Nweeia, whose dental surgery practice is based in Sharon, Connecticut, lectures at Harvard’s School of Dental Medicine and holds a global fellow position at the Polar Institute at the Wilson Center. He is also a research associate at the Arctic Studies Center of the Smithsonian Institution and at the Canadian Museum of Nature, and a member of the Zoonomia Consortium of Harvard/MIT.

...

Great Amateurs in Science

Dr. Nweeia joins a pantheon of discoverers, many of whom had no formal scientific training, who have made extraordinary scientific contributions. 

Often overlooked by the experts in their fields, they made contributions recognized sometimes long after they were gone. Who are they? They are amateur scientists who excel in other fields — people like Thomas Jefferson, Michael Faraday, and Arthur C. Clarke— whose groundbreaking work occasionally leaves their professional counterparts envious. Against the odds, they’ve carved out a remarkable legacy in the history of science.

1. Gregor Johann Mendel

Regarded as the father of genetics, Gregor Mendel, an Austrian monk, conducted groundbreaking experiments on pea plants, discovering the fundamental laws of inheritance. Despite publishing his work in 1865, his findings remained unnoticed for decades. Mendel’s meticulous research laid the foundation for modern genetics, influencing evolutionary biology and agriculture.

2. David Levy

David Levy, a Canadian amateur astronomer, is renowned for co-discovering the comet Shoemaker-Levy 9, which dramatically collided with Jupiter in 1994. With no formal training in astronomy, Levy’s passion for stargazing led to the discovery of multiple comets, establishing his place in celestial history alongside the Shoemaker team.

3. Henrietta Swan Leavitt

Henrietta Leavitt, an American astronomer, unlocked the key to measuring cosmic distances by discovering the relationship between a Cepheid star’s brightness and its pulsation period. Her groundbreaking work allowed astronomers to determine the scale of the universe, leading to Edwin Hubble’s later discovery of galaxies beyond the Milky Way.

4. Joseph Priestley

Joseph Priestley, an 18th-century English polymath, is best known for discovering oxygen. His scientific contributions spanned chemistry, electricity, and photosynthesis, yet he was also a prominent theologian and political thinker. His work in chemistry laid foundational knowledge for future discoveries, including modern gas chemistry and the invention of soda water.

5. Michael Faraday

Michael Faraday, an English scientist, revolutionized the fields of electromagnetism and electrochemistry. Despite limited formal education, his discovery of electromagnetic induction led to the invention of the electric generator. Faraday’s pioneering experiments and contributions to the understanding of electricity earned him recognition as one of history’s greatest experimentalists.

6. Grote Reber

Grote Reber, an American radio engineer, built the world’s first radio telescope in his backyard in 1937. His innovative work in radio astronomy revealed radio emissions from the Milky Way, transforming the field. Reber’s telescope and research paved the way for large-scale radio observatories, advancing our understanding of the universe.

7. Arthur C. Clarke

Arthur C. Clarke, a visionary science-fiction writer and futurist, revolutionized global communication by proposing the concept of geostationary satellites in 1945. Best known for his science fiction, including 2001: A Space Odyssey, Clarke’s contributions to satellite technology transformed broadcasting and laid the groundwork for modern telecommunications.

8. Thomas Jefferson

Thomas Jefferson, third U.S. president and principal author of the Declaration of Independence, was also a pioneering archaeologist. In 1784, his methodical excavation of an Indian burial mound introduced modern archaeological techniques. Jefferson’s interdisciplinary genius spanned architecture, zoology, and botany, and he remains a towering figure in American history.

9. Susan Hendrickson

Susan Hendrickson, an American paleontologist and self-taught explorer, unearthed the largest and most complete Tyrannosaurus rex skeleton in South Dakota in 1990. Known as "Sue," this extraordinary find is a centerpiece at Chicago’s Field Museum. Hendrickson’s discoveries, spanning fossils and marine life, have left a lasting impact on paleontology.

10. Felix d'Herelle

Felix d’Herelle, a French-Canadian bacteriologist, discovered bacteriophages—viruses that attack bacteria—while researching dysentery in 1916. His work in phage therapy offered potential solutions for bacterial diseases, influencing genetic research and DNA studies. D’Herelle’s discovery paved the way for modern virology, particularly as antibiotic resistance becomes an increasing concern.

I have been very lucky

Mike's Notes

A curious mix of chance and trying hard; who would have thought? I am very grateful to all those who helped me along the way.

I learn by the seat of my pants, making lots of mistakes, never repeating them. Being self-educated is great. So is listening, asking questions, reading print books, learning to use tools to make things, challenging every assumption, "strong opinions, weakly held", subject to change as factual evidence emerges via robust Science. We are all capable of doing this.

We are all smarter than we give ourselves credit for.

Resources

References

  • Reference

Repository

  • Home > Ajabbi Research > Library >
  • Home > Handbook > 

Last Updated

09/08/2026

I have been very lucky

By: Mike Peters
On a Sandy Beach: 27/07/2026

Mike is the inventor and architect of Pipi and the founder of Ajabbi.

I have been very lucky. I have had a lot of people in my life who were a good influence on me. (I get rid of anyone who sabotages or is a bad influence)

My grandmother Bessie showered me with attention and love, gave me endless things to pull apart to see how they worked, and took me to meet very clever people in a small-minded backwater town.

Family holidays in wild New Zealand, next to rivers, beaches, forests and mountains, which ignited a lifelong obsession with the patterns of nature, the why in my life.

My best friend right through school; he was the brightest kid in NZ.

My remedial "Cabbage Maths" teacher, Mrs Campbell, who took me from the bottom of a class to the top of the school with 98% by teaching me maths visually. That's when I learned the problem was not me; it was the way I was being taught, so from then on, I taught myself everything by reading 20 books a week, drawing notes, and having a go.

My high school science teacher, Mr Morgan, let me play in the chemistry lab, doing experiments after school unsupervised for several years, and taught me the scientific method on my very last day at school, the most important thing I learned in 12 wasted years.

The wise old tradesmen took a skinny kid from sweeping the floor to being able to make anything by learning on the job, trying hard, and having my butt kicked when I deserved it.

Nelson Mandela taught me to have the courage of my convictions and never give up.

The sculptor Neil Dawson and the set designer Tony Geddes taught me how to work authentically and in the flow.

My blind friend Grant, who made and gave away $60 M NZD, taught me, while he was cutting down bushes with a chainsaw, determination, quiet courage and human decency.

The magnificent 50,000 working people of South Christchurch, who trusted me to lead a volunteer residents' army doing recovery work for 3 years after the Christchurch Earthquake, teaching me humility, what honour is, and valuable leadership skills gained by trial and error in the moment.

My beloved Tracy, the bravest woman I have ever met, the only paraplegic to do the Coast-to-Coast Iron Man, who married an undomesticated autistic male and made me a much better man. Her unwavering devotion, encouragement and loyalty made all this possible.

They all shaped me; I can't thank them enough. May their memories be a blessing.

No posts for a wee while

Mike's Notes

I was on holiday for the last few weeks and am back now. There will be no blog posts, newsletters or meetings until Pipi Core is back up and running.

Update 27/05/2026

Lots of surprises. Making rapid progress. The peace and quiet are bliss.

Update 31/05/2026

The problem and solution are how things are named. Pipi auto-generates thousands of code names using multiple pattern languages, and all the naming conventions require many minor fixes for several unexpected reasons after migrating from a developer laptop to a production server environment. Everything else is absolutely fine.

Other naming problems are also being solved now, including:

  • The rapid development of Boxlang by Ortus has brought forward another challenge. Pipi 10 will be migrated to run on top of Boxlang in 2027 to support multiple languages, including C++, CFML, COBOL, Go, Java, JavaScript, PHP, Python, Rust, etc.
  • Future integration with cloud-based LLMs.
  • Future integrations with Office365, Google Workspace, Zoho, LibreOffice, etc.

The common solution is to create standardised naming systems that are simple, stable, robust, schema-based, versioned, self-documenting, and extensible to meet unanticipated future needs.

This is done by replacing code-based naming rules with database-driven ones that can be easily edited in the future via an admin UI.

90% of these names are internal, hidden in the closed core, and how they work and what they are will not be discussed here. The rest will be publicly and fully documented as part of the open-source workspaces for developers to work with.

Update 02/06/2026

I'm changing the disclosure boundary between the Pipi closed-core and open-source workspaces. Previously, "disclose everything unless there is a security reason not to". This is now changed to "disclose on the basis of need to know".

Closed-core accounts for 90% and open-source workspaces for 10% of lines of code, databases, etc.

This will reduce the documentation burden, given Pipi's vast scale. So, the open-source workspaces will be fully shared and documented on GitHub, etc, without restriction. This includes;

  • Standards schema
  • Ontologies
  • Parameters
  • Laws of physics
  • HTML + CSS
  • Algorithms
  • Module DDD models
  • Workflow diagrams
  • Documentation
  • API schema
  • UI code
  • etc

This also means some existing technical documentation about the closed-core will become hidden and only available internally.

Update 07/06/2026

Pipi Core is the IDE used to edit Pipi Core (AKA: which came first, the chicken or the egg?). Temporary UIs have been created and are being used across multiple engines to edit the names in use. This is much faster than directly editing data, which had to be done initially. The next step will be turning auto-generation back on. Once that's done, temporary UIs will be used to build permanent UIs. More automation will then be enabled via the UIs, and so on, as Pipi Core builds itself with a human in the loop.

Update 08/06/2026

The list of code cases available to use now for auto-generated naming, I/O translation, etc with examples, includes;

  • camelCase: userProfilePicture
  • kebab-case: user-profile-picture
  • PascalCase: UserProfilePicture
  • snake_case: user_profile_picture
  • SCREAMING_SNAKE_CASE: USER_PROFILE_PICTURE
  • Train-Case: User-Profile-Picture
  • flatcase: userprofilepicture
  • UPPER-CASE-KEBAB-CASE: USER-PROFILE-PICTURE
  • Sentence case: User profile picture
  • Title Case: User Profile Picture
  • middot·case: user·profile·picture
  • dot.case: user.profile.picture
  • UPPER CASE: USER PROFILE PICTURE
  • lowercase: user profile picture

Update 12/06/20026

Checking that these changes to variable names and internal messaging do not clash with the Gödel Machine.

Update 17/06/2026

The DevOps Engine (dvp) has unexpectedly proven to be critical to solving this puzzle. Mostly fixed last night. Watching the rather excellent live Google talk, Beyond the GPU: Maximising goodput with self-healing AI infrastructure, this morning has given me valuable insights into how to fix the remaining issues by reviewing Google HPC YAML files. 😎😎 Sometimes insights come from the strangest places.

Update 01/07/2026

The main work now is rapidly configuring Pipi for production and full autonomous automation. Using Google Search AI Mode (Gemini) and then Grammarly Pro makes the work easier and 100x faster.

  • I have decided to have Pipi re-render the many Ajabbi draft public websites with the new and missing developer information. (20K pages)
  • The website's .robot.txt file will then be unlocked to enable search engines.
  • The HTML will be updated to make it easier for AI to read.
  • This blog will be imported into Pipi, cleaned up, re-exported from Pipi, and published to Blogger via the API.
  • The new posts created in Pipi will return to A Sandy Beach to discuss something already built rather than being built.

Update 02/07/2026

The DevOps and IaC engines are getting rapid data model overhauls. The IaC engine is a great test for the variable names. I'm building a capability into Pipi to autonomously and automatically run OpenTofu and Ansible, initially targeting the Pipi Data Centre, then GCP and AWS for deployments. It's going very well and making rapid progress.

Update 05/07/2026

Pipi will initially run the open-source enterprise applications on Google Cloud Run and Google Cloud Storage (GCS). The code is complete and will be very low-cost to run, giving Ajabbi, a bootstrapping-purpose startup, a very long runway.

Update 18/07/2026

The job has now shifted to configuring, networking and deploying many physical servers. Installing software, including Pipi, labelling cables and rack gear, throwing out junk, tidying, etc., leaving nothing to chance. Shipping delays are holding up part deliveries.

Update 28/07/2026

Most of the equipment has arrived, and the small data centre setup is coming together. More deliveries later this week. It's already running a lot better and is much more productive.

Update 31/07/2026

Work on Pipi has reached a tipping point or system phase change as Pipi takes over tasks using autonomous automation. Pipi now has deadlines, not me. Soon it will set the deadlines. It's now a downhill run; daily posts from me resume tomorrow, and much more will come.

In hindsight. This whole project has been systematic trial and error, spending 10 years learning how to crack a hard problem.

Resources

References

  • Reference

Repository

  • Home > Ajabbi Research > Library >
  • Home > Handbook > 

Last Updated

31/07/2026

No posts for a wee while

By: Mike Peters
On a Sandy Beach: 15/05/2026

Mike is the inventor and architect of Pipi and the founder of Ajabbi.

I was on a no-coding holiday for the last few weeks to clear my mind, and it has been great. I am back on the job today.

Suspended

Until the closed-source Pipi Core is back up and running 100% on autopilot, 10x faster, the following are suspended.

  • New posts "On a Sandy Beach
  • All newsletters, including the weekly Friday Report and the monthly Ajabbi Research Newsletter.
  • The fortnightly online Open R&D meeting.

Rapid refocus

  • A new developer area with five coding screens, designed to be more productive for hypervisual learners.
  • A better library has been set up for my A4 drawings in ring binders, the many reference books I use, and more bookshelves are on the way.
  • The server rack has been moved to a better location.
  • The light levels have been adjusted.
  • A big office tidy is almost done. An office-work-only desk has yet to be set up with a cat bed included.
  • A separate area with no screens for the happy cat, coffee, music, reading and drawing.

Less is more

Minimise screen time to be more productive at work. The new setup is also much less tiring.

Get the job done

The good thing is that, with a holiday and lots of drawing, I now have mental clarity about what needs fixing and how to fix it. Mainly, quite delicate changes here and there, organised into a list of steps. Now, I need to concentrate on one thing only: go as fast as possible, without meetings, post-deadlines, phone calls, or other distractions.

How

1. Use an AI workforce

Be the architect, and AI fills in the dots to make it happen.

Use Google Search AI mode (Gemini) to generate 99% of the code in one-page chunks (including references) to copy and paste, then manually change the variable names and SQL. Careful, test everything, resulting in 100x faster progress. Know how everything works and rapidly raise personal skill level.

2. Then build a cathedral

Make a wooden scale model of a cathedral for the builders. Google Search AI mode (Gemini) makes each brick, and Pipi Core assembles the bricks into floors, arches, walls, and vaults...

Speed is king

With the 100x coding productivity gains from Google Search AI mode (Gemini), plus the 10x10x10x speedup of Pipi Core currently underway over the next few months, what previously took a year will be done in hours and better.

Phase transitions

Once these initial migration issues from laptop to server are resolved, further transitions can be anticipated as the number of engines rapidly increases beyond 20. Increasing the number of engines slowly changes the whole system's behaviour from deterministic to probabilistic and adaptive.

Here is a partial list of transitions expected as the number of engines increases from 0 to 200. The actual numbers are a bit of a guess.

  • 20 engines enable Pipi 9 Core in a simple, deterministic structure.
  • 40 engines enable a workspace with a UI for administering Pipi Core.
  • 60 engines enable self-generation of user documentation.
  • 80 engines enable REPL and IAC (infrastructure-as-code).
  • 100 engines enable Workspaces for different user accounts.
  • Different Pipi 9 editions are made with the same engines, which recombine differently in response to the external environment.
  • And so on until...
  • 200 engines self-organise into a multi-layered complex fluid structure with probabilistic behaviour and emergent properties, as engines also act as agents.
  • 200+ engines enable Pipi 10 to interact with externally cloud-hosted LLMs, combining the very different strengths of both.

Live 4K video of Earth and space: 24/7 Livestream of Earth by Sen’s 4K video cameras on the ISS

Mike's Notes

Just beautiful.

Resources

References

  • Reference

Repository

  • Home > Ajabbi Research > Library >
  • Home > Handbook > 

Last Updated

25/04/2026

Live 4K video of Earth and space: 24/7 Livestream of Earth by Sen’s 4K video cameras on the ISS

By: Sen
Sen: 25/04/2026

Sen’s vision is to democratise space through video to inform, educate, inspire, and benefit all of humanity. Sen’s mission is to stream real-time video from space to billions of people, gathering news and information about Earth and space and making the data universally accessible and useful.

Watch Earth Live and in 4K from Sen's video cameras on the International Space Station, downlinked via NASA. This is the world’s first continuous 4K livestream from space, empowering you to see our planet like astronauts do.

How to Accelerate Protein Structure Prediction at Proteome-Scale

Mike's Notes

Impressive and socially useful. The original article has many links.

Resources

References

  • Reference

Repository

  • Home > Ajabbi Research > Library > Subscriptions > NVIDEA Developer
  • Home > Handbook > 

Last Updated

19/04/2026

How to Accelerate Protein Structure Prediction at Proteome-Scale

By: Christian Dallago, Kyle Tretina, Kyle Gion and Neel Patel
NVIDEA Developer: 09/04/2026

Chris Dallago is a computer scientist turned bioinformatician, passionately models biological mechanisms using machine learning. He's advanced bio-sequence representation learning, contributing to its establishment, notably in transformer models. Chris is dedicated to solving scarce data problems, such as designing proteins for therapeutic and industrial applications.

Kyle Tretina is a product marketing leader at NVIDIA, focused on advancing AI for digital biology and drug discovery. He drives the strategy and storytelling behind BioNeMo and our work with BioPharma, shaping how next-generation foundation models and GPU-accelerated microservices transform molecular and protein design. With a PhD in molecular microbiology and immunology, Kyle bridges science and strategy, translating breakthroughs in AI, chemistry, and biology into platforms that accelerate discovery for researchers, startups, and pharmaceutical companies worldwide.

Kyle Gion is a product manager for Research at NVIDIA, where he translates R&D in digital biology and molecular science into impactful products. He focuses on guiding research that applies computational biology, computational chemistry, and AI to life sciences, drawing on experience that spans both building scientific software and developing cystic fibrosis therapies. Kyle earned his bachelor's and master's degrees in Chemical Engineering from Brown University.

Neel Patel is a drug discovery scientist at NVIDIA, focusing on cheminformatics and computational structural biology. Before joining NVIDIA, Neel was a computational chemist in big pharma, where he worked on structure-based drug design. He holds a Ph.D. from the University of Southern California. He lives in San Diego with his family and enjoys hiking and traveling.

Proteins rarely function in isolation as individual monomers. Most biological processes are governed by proteins interacting with other proteins, forming protein complexes whose structures are described in the hierarchy of protein structure as the quaternary representation. 

This represents one level of complexity up from tertiary representations, the 3D structure of monomers, which are commonly known since the emergence of AlphaFold2 and the creation of the Protein Data Bank.

Structural information for the vast majority of complexes remains unavailable. While the AlphaFold Protein Structure Database (AFDB), jointly developed by Google DeepMind and EMBL’s European Bioinformatics Institute (EMBL-EBI), transformed access to monomeric protein structures, interaction-aware structural biology at the proteome scale has remained a bottleneck with unique challenges:

  • Massive combinatorial interaction space
  • High computational cost for multiple sequence alignment (MSA) generation and protein folding
  • Inference scaling across millions of complexes
  • Confidence calibration and benchmarking
  • Dataset consistency and biological interpretability

In recent work, we extended the AFDB with large-scale predictions of homomeric protein complexes generated by a high-throughput pipeline based on AlphaFold-Multimer—made possible by NVIDIA accelerated computing. Additionally, we predicted heteromeric complexes to compare the accuracy of different complex prediction modalities.

In particular, for the predictions of these datasets, we leveraged kernel-level accelerations from MMseqs2-GPU for MSA generation, and NVIDIA TensorRT and NVIDIA cuEquivariance for deep-learning-based protein folding. We then mapped the workload to HPC-scale inference by maximizing the utilization of all available GPUs, including scale-out to multiple clusters.

This blog describes the major principles we adopted to increase protein folding throughput, from adopting libraries and SDKs to optimizations to reduce the computational complexity of the workload. These principles can help you set up a similar pipeline yourself by borrowing from the techniques we used to create this new dataset.

So, if you are a:

  • Computational biologist scaling structure prediction pipelines
  • AI researcher training generative protein models
  • HPC engineer optimizing GPU workloads
  • Bioinformatician team building structural resources

You will learn how to:

  • Design a proteome-scale complex prediction strategy
  • Separate MSA generation from structure inference for efficiency
  • Scale AlphaFold-Multimer workflows across GPU clusters

Prerequisites

  • Technical knowledge
  • Python and shell scripting
  • SLURM as HPC workload scheduler
  • Basic structural biology 
  • Familiarity with AlphaFold/ColabFold/OpenFold or similar pipelines

Infrastructure

We describe scaling on a multi-GPU and multi-node NVIDIA DGX H100 Superpod cluster

This cluster includes high-speed storage to store MSAs and intermediate outputs

Software

  • Access to MMseqs2-GPU
  • Familiarity with TensorRT

If not using a model with integrated cuEquivariance, knowledge about triangular attention and multiplication operations 

Procedure/Steps

1. Define the dataset you’d like to compute

Begin by defining the scope of prediction. Because predicting protein complexes can become a combinatorial problem, it’s useful to understand what may be most interesting. In some cases, if your proteomes are small enough, an all-against-all (dimeric) complex prediction might be tractable; however, this could change if you want to predict large datasets of proteomes.

Here’s how we decided to go about it:

  • Homomeric complexes: We selected all proteomes represented in the AFDB and sorted them by perceived importance (e.g., proteomes of human concern or commonly accessed). This allowed us to rank proteomes for computation in a particular order, making execution more manageable.
  • Heteromeric complexes: This is where things can get complicated, fast. For our heteromeric runs, we decided to focus on complexes originating from several reference proteomes and proteomes included in the WHO list of important proteomes. As there’s an intractable number of combinations of complexes that can be derived from these proteomes, for our runs, we focused on dimers (complexes of two proteins), within the same proteome (no inter-proteome complexes) that had “physical” interaction evidence in STRING. As we sought coverage, we decided to consider all interactions reported in STRING for these proteomes, rather than further filtering. Evidence in the literature suggests that filtering for STRING scores >700 can further reduce the number of inputs while increasing the likelihood of well-predicted complexes.

2. Decoupling MSA generation from structure prediction

MSA generation and structure inference are both compute-intensive but scale differently, as we recently presented in a white paper. We thus approached these computations as separate steps and implemented separate SLURM pipelines. In general, for optimal use of a node, we set up MSA generation and structure prediction this way.

MSA generation

We generated MSAs using colabfold_search with the MMseqs2-GPU backend. While MMSeqs2-GPU scales across GPUs on a node natively, we chose to spawn one MMseqs2-GPU server process per GPU on a node for easier process management. In colabfold_search, the GPUs are only used for the ungappedfilter stages and not the subsequent alignment stages (which are multithreaded CPU processes).

Therefore, we can stack colabfold_search calls and start the next one once the GPU is no longer used by the previous one, by monitoring the colabfold_search output, to reduce GPU idle time.

Although this approach oversubscribes CPU resources, in practice, we found that on a DGX H100 node, up to 25% of the overall increase in throughput can be achieved with three staggered colabfold_search processes, at the expense of slower processing of individual input chunks. 

On determining reasonable input chunk sizes, there are two factors to consider. Smaller chunk sizes result in more chunks, which means more per-process overheads, such as database loading, which can take a couple of minutes each, even on fast storage. (Pre-staging the databases on the fastest storage available, such as the on-node SSD, helps with throughput as well.) On the other hand, larger chunks take more time to finish. On a SLURM cluster with a job time limit, this results in more unfinished chunks.

The sweet spot will depend on the cluster configuration, but for our DGX H100 node with a 4-hour wall time limit, the chunk size of 300 sequences seemed to work well with the staggering colabfold_search approach.

Structure prediction

In order to increase structure prediction throughput, we leveraged both optimizations in data handling for JAX-based folding through ColabFold, as well as accelerated tooling developed at NVIDIA, including TensorRT, and cuEquivariance for OpenFold-based folding.

Deep learning inference parameters

First, we selected inference parameters that struck a good balance between accuracy and speed. Protein inference setup for all deep learning inference pipelines (ColabFold and OpenFold), thus utilized:

  • Weights: 1x weights from AlphaFold Multimer (model_1_multimer_v3)
  • Four recycles (with early stopping)
  • No relaxation
  • MSAs: frozen MSAs generated through ColabFold-search (using MMseqs2-GPU), as described above

Accuracy validation

  Homodimer PDB set (125 proteins)
Model High Medium Accept Incorr Usable DockQ
DockQ >0.8 >0.6 >0.3 >0      
ColabFold 52 37 12 21 89 (72.95%) 0.637
OpenFold with TensorRT and cuEquivariance 53 39 10 20 92 (75.41%) 0.647

Table 1. A comparison of interface accuracy between ColabFold and OpenFold (accelerated by TensorRT and cuEquivariance) across a benchmark set of 125 homodimer proteins.

As we used different inference pipelines, we performed accuracy validation using a curated benchmark set of 125 X-ray resolved PDB homodimers released after AlphaFold2 was introduced, thus minimizing the potential for information leakage.

Predicted complexes for each deep learning implementation were compared against experimental reference structures using DockQ, which evaluates interface accuracy via the fraction of native contacts (Fnat), fraction of non-native contacts (Fnonnat), interface RMSD (iRMS), and ligand RMSD after receptor alignment (LRMS), and assigns standard CAPRI classifications of high, medium, acceptable, or incorrect.

Across the PDB homodimer benchmark, OpenFold accelerated through TensorRT and cuEquivariance reproduces ColabFold interface accuracy, achieving a similar fraction of “high” scoring predictions and comparable mean DockQ scores. This indicates that the accelerated implementations preserve interface-level structural accuracy relative to the ColabFold baseline.

MSA preparation and sequence packing

For ColabFold-based homodimer inferences, higher throughput can be achieved by packing homodimers of equal length into a batch for processing, sorted by their MSA depth in descending order. This reduces the number of JAX recompilations, thereby increasing end-to-end throughput. This trick, however, does not work when processing heterodimers, because the lengths of the individual chains differ.

For OpenFold, whether for homodimers or heterodimers, this packing strategy is not needed, as the method doesn’t require re-compilation. However, given a dependency between sequence length and execution time, reserving longer sequences for individual jobs may be beneficial if operating with specific SLURM runtimes. To further optimize the process, input featurizations (CPU-bound) were performed for the next input query alongside the inference step for the current query (GPU-bound).

Additionally, OpenFold’s throughput was enhanced through the integration of the NVIDIA cuEquivariance library and NVIDIA TensorRT SDK. These modular libraries and SDKs can be leveraged to accelerate operations common in protein structure AI and general inference AI workloads, respectively. We previously described how TensorRT can be leveraged to accelerate OpenFold inference.

3. Optimize GPU utilization with SLURM

As alluded to in the previous section, depending on the available hardware, you can increase throughput by “packing” GPUs and nodes. SLURM is a great orchestrator, and we divided the inference workflows in SLURM scripts to:

  • Pack multiple predictions per node
  • Match GPU memory to sequence length
  • Reduce idle time between jobs
  • Separate short vs long sequence queues

Our workload was mapped to a H100 DGX Superpod HPC system. We could thus deploy inference across NVIDIA H100 GPUs on multi-node clusters, leveraging exclusive execution on a single node, and packing each GPU with as many processes as saturated the GPU utilization for both MSA processing and deep learning inference.

Helpful tips:

  • Group jobs by total residue length
  • Monitor GPU memory fragmentation
  • Use asynchronous I/O to avoid disk bottlenecks

4. Making quality predictions accessible to the world

In partnership with EMBL-EBI, the Steineggerlab at Seoul National University, and Google DeepMind, we explored complex structure prediction analysis. We highlight that predicting these biological systems remains challenging. Unlike protein monomer prediction, where predicted Local Distance Difference Test (pLDDT) can inform overall prediction quality, yielding a balanced amount of plausible predictions, in the complex scenario, assessing interface plausibility is much harder. This has to do with the fact that assessing complexes involves global and per-chain confidence metrics, as well as local confidence metrics at the interface.

Simply put, is the interface between two monomers plausible, and is it predicted in the right pocket? These questions are much harder to answer than more “local” questions about monomer likelihood, given the very limited data available. Therefore, we make available a set of high-confidence structures through the AlphaFold Database, thereby enabling, for the first time, exploration of protein complexes. We intend to refine our approach further and expand the universe of available protein complexes in the AlphaFold Database.

Getting started

Proteome-scale quaternary structure prediction requires more than just running AlphaFold-Multimer at scale. Success depends on:

  • Evidence-driven interaction selection
  • Decoupled and optimized compute workflows
  • GPU-aware job orchestration
  • Confidence calibration and validation
  • Dataset health monitoring

By combining STRING-guided selection, MMseqs2-GPU acceleration, and NVIDIA H100-powered multimer inference, this work extends AFDB into a unified, interaction-aware structural resource.

This infrastructure enables:

  • Variant interpretation at interfaces
  • Systems-level structural biology
  • Drug target validation
  • Generative protein design benchmarking

Resources

Read more about the project here: https://research.nvidia.com/labs/dbr/assets/data/manuscripts/afdb.pdf 

Accelerated libraries and SDKs are available here:

  • MMseqs2-GPU
  • NVIDIA cuEquivariance
  • NVIDIA TensorRT

If you wish to deploy MSA search and protein folding easily, you can get accelerated inference pipelines through NVIDIA’s Inference Microservices (NIMs):

  • MSA Search NIM 
  • OpenFold2 NIM

The predictions from this effort are available through https://alphafold.com