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òòò½ÍøJoins Global Scientific Network, GNOME, to Search for Dark Matter

We are proud to share that òòò½Íøhas joined the Global Network of Optical Magnetometers for Exotic physics (GNOME), facilitated by Q.InC. GNOME is a prestigious international collaboration of 15 research stations at some of the world’s leading institutions, dedicated to detecting signals of dark matter and other exotic physics phenomena.

Dark matter detection stands at the forefront of modern physics, as it remains one of the greatest scientific mysteries. Together with dark energy, it is theorised to constitute 95% of the universe, yet its nature remains elusive – driving global efforts to unlock its secrets.

Dark matter interacts gravitationally but does not couple to electromagnetic radiation (e.g. light), which makes it “dark” and renders direct detection extremely challenging. However, some theories suggest that it may exert subtle, magnetic field-like influences on atoms, offering an alternative pathway for detection through precise quantum magnetometry.

GNOME collaborators continuously analyse magnetic field signals detected by highly sensitive quantum sensors. By analysing correlated data across the network, scientists aim to identify potential global “domain walls” moving through Earth – hypothetical structures that could be linked to dark matter. This innovative approach may provide groundbreaking insights into the fundamental nature of dark matter, bringing us closer to uncovering its mysteries.

Visualisation of a dark matter domain-wall crossing. Image from Nat. Phys. 17, 1396–1401 (2021), licensed under CC BY 4.0. [1]

Synergistic Partnership in Search of Dark Matter

The òòò½ÍøGNOME station will be hosted at the òòò½Íø, Technology and Research (A*STAR), with contributions from the Centre for Quantum Technologies (CQT), the National University of òòò½Íø(NUS), and Nanyang Technological University, òòò½Íø(NTU Singapore).  Research teams in òòò½Íøbring together advanced sensing capabilities and technologies, working collaboratively on a carefully coordinated multi-messenger approach to detecting dark matter.

A*STAR - Advanced quantum magnetometers [2, 3]

CQT - [4] and [5]

AWS -  Enhanced with and

This precise quantum magnetometer at A*STAR will be used to detect pseudomagnetic fields potentially caused by dark matter, indicating its presence. Photo by Dr. Wang Tao.


Strengthening Capabilities for Broader Applications

Through GNOME, òòò½Íøwill foster deeper collaborations with exceptional scientists worldwide. In line with its scientific mission, Q.InC aims to leverage the power of this global network to progress and deepen quantum research whilst delivering real-world impact. The shared knowledge, expertise and innovations from the initiative will accelerate the development of hyper-accurate, hyper-sensitive sensing (and related) technologies, with transformative applications in:

  • Smart City Infrastructure and Urban Planning Enabled by Sensor Networks
  • Biomedical imaging and precision diagnostics
  • Positioning, navigation, and timing (PNT) systems
  • Mineral exploration and geophysical mapping
  • Defence and security

The team at Q.InC share an ambitious vision of contributing to a quantum-ready Singapore. Read the full article for more on the significance and potential of this partnership, as well as comments from A*STAR’s Chief Quantum Scientist, Professor Lam Ping Koy, and Senior Quantum Scientist, Dr Wang Tao, who previously operated and optimised two other GNOME stations at the University of California, Berkeley.

Q.InC GNOME-òòò½Íøteam members (from left to right): V Vijendran, Vincent Lau, Joel K. Jose, Vishwanath Singh, and Wang Tao

Q.Inc Advisory Panel member and an original co-founder of GNOME, Prof. Dmitry Budker (second from the right) (UC Berkeley and JGU Mainz), visited the Q.Inc Quantum Magnetometer for GNOME.

 

[1] Afach S, etc. Search for topological defect dark matter with a global network of optical magnetometers. Nature Physics. 17(12):1396-401 (2021)

[2] Wang T, etc. Pulsed vector atomic magnetometer using an alternating fast-rotating field. Nature Communications. 16(1):1374 (2025)

[3] Wang T, etc. Application of spin-exchange relaxation-free magnetometry to the cosmic axion spin precession experiment. Physics of the dark universe. 1;19:27-35 (2018)

[4] Zhiqiang Z, etc. 176Lu+ clock comparison at the 10− 18 level via correlation spectroscopy. Science Advances. 9, eadg1971 (2023).

[5] Shettell N, etc. Geophysical survey based on hybrid gravimetry using relative measurements and an atomic gravimeter as an absolute reference. Scientific Reports. 18;14(1):6511 (2024)