Strange Power Inc — Albuquerque, NM

Fusion energy,
confined by dark matter

We are developing MQN Fusion — a compact fusion architecture grounded in over two decades of peer-reviewed research into Magnetized Quark Nugget dark matter.

Understand the science View publications
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What are MQNs?

The hypothesis, plainly stated

Roughly 85% of the mass of the universe is made of dark matter — something that exerts gravity but neither emits nor absorbs light. Its composition remains one of physics' central open questions.

Our research explores a specific dark matter candidate: Magnetized Quark Nuggets (MQNs). These are hypothetical objects composed of strange quark matter — a form of nuclear-density matter that may have formed in the first fractions of a second after the Big Bang.

The key property that distinguishes MQNs is their predicted ferromagnetism. Each MQN would behave as a single magnetic dipole — similar in structure to Earth's own magnetic field, but potentially up to 20 billion times stronger than any field we can generate on Earth today.

If MQNs exist, are stable, and can be collected, they would represent a fundamentally new class of engineerable material with direct implications for plasma confinement in fusion reactors.

This is a hypothesis under active scientific investigation. The publications below document the evidence that supports it and the experiments that could falsify it.

01

Cosmic origin

In the first ~65 microseconds after the Big Bang, quarks and gluons may have aggregated into large, stable clumps rather than dispersing into protons and neutrons. These clumps are quark nuggets.

02

Ferromagnetism at nuclear density

Theoretical models by physicist Tatsumi predict quark matter at nuclear density can be ferromagnetic — meaning quark nuggets would form a persistent magnetic dipole at extraordinary field strength.

03

MQNs as dark matter

Published models show MQNs could account for the observed dark matter density, survive to the present day, and produce detectable signatures when passing through planetary matter.

04

Detection and collection

MQNs interacting with matter would deposit energy and produce electromagnetic and acoustic signatures. Modeling suggests solar aerobraking could concentrate them in magnetite deposits, enabling extraction on Earth.


Peer-Reviewed Research

Seven published papers, 23 years of work

The scientific case for MQNs is documented in peer-reviewed literature. These publications establish the theoretical foundation, predict observable signatures, and report on detection campaigns — the full chain from hypothesis to experiment.


If MQNs Can Be Collected

Two long-range applications under development

MQN Fusion

MQN Fusion — Power Generation

Conventional fusion reactors require enormous superconducting coil systems to confine plasma. Our hypothesis is that an MQN could serve as an intrinsically stable, ultra-strong magnetic confinement structure — without large coil infrastructure.

This architecture, if achievable, could yield a substantially more compact and economically favorable fusion reactor than current tokamak or stellarator approaches.

Early-stage R&D
🛸

Dark Matter Drive

DMD — Deep-Space Propulsion

A speculative propulsion concept where MQNs serve as the power and impulse drivers for high-efficiency propulsion systems. The extreme magnetic moment of a collected MQN could enable propulsion regimes unavailable to conventional chemical or ion drives.

This remains a long-horizon concept contingent on MQN existence and collection, explored in parallel with the power generation program.

Conceptual exploration

Research Roadmap

A stepwise path from theory to application

Phase 1 — Complete

Theoretical foundation

Establish MQN formation models, mass distributions, magnetic field strengths, and compatibility with cosmological dark matter constraints. Seven papers published in peer-reviewed journals.

Phase 2 — Active

Detection campaigns

Design and deploy detection strategies using predicted electromagnetic, acoustic, and energy-deposition signatures. Search for MQN accumulation in iron ore and other materials. Refine flux limits from non-detection data.

Phase 3 — Future

Collection and characterization

If detection is confirmed, develop methods for concentrating and capturing MQNs from terrestrial sources. Characterize magnetic moment and nuclear mass density under laboratory conditions.

Phase 4 — Long-term

MQN Fusion prototype and energy systems

Design plasma confinement experiments using captured MQNs. Progress toward a fusion architecture that's economically advantageous, environmentally sustainable and carbon free.


About Strange Power Inc

Built from the MQN Collaboration

Strange Power Inc was founded from the MQN Collaboration — a global, virtual scientific network formed more than two decades ago to investigate whether Magnetized Quark Nuggets are a viable dark matter candidate.

We are headquartered in Albuquerque, New Mexico. Our team includes plasma physicists, experimentalists, and systems engineers with extensive backgrounds in nuclear technology and advanced sensing.

We approach this work with scientific rigor: the hypothesis could be falsified, and we design experiments accordingly.

Meet the team
23+
years of active research
7
peer-reviewed publications
20Bx
stronger than terrestrial magnets (predicted)
85%
of the mass of the universe is dark matter
Collaboration & Investment

Engaging partners who share a long horizon

We are currently engaging magnetite mining and processing companies, fusion power designers, utilities, industrial energy users, and forward‑looking capital partners who see MQN‑enabled fusion and propulsion as a strategic long‑term bet. If your mandate includes hedging against conventional fusion timelines or exploring new deep‑space mission architectures, we invite a conversation.