Poster presentation at SI2026 in Fuji Yoshida
Presented a poster on two-component pseudo-Nambu-Goldstone boson dark matter at the 30th International Summer Institute on Phenomenology of Elementary Particle Physics and Cosmology.

PhD Researcher
Theory of Elementary Particles Lab
Kyushu University Fukuoka, Japan
PhD Physics
Kyushu University, Japan
2024 – Present
MSc Physics
Banaras Hindu University, India
2020 – 2022
BSc Physics
Cotton University, India
2016 – 2019
Dark matter makes up about 26% of the energy density of the universe, yet everything we know about it comes from its gravity. My research asks what it is, what keeps it stable, how much of it the early universe left behind, and how it interacts with ordinary matter, however faintly. It could be a single particle or a whole family of hidden particles. Underground detectors have not yet seen a confirmed signal, which narrows the possibilities and points to signals these searches were not designed to look for.
Much of my work uses symmetry to build models of dark matter. In one family of models, called pseudo-Nambu-Goldstone boson (pNGB) dark matter, symmetry makes dark matter bump into ordinary atoms only very rarely, which would explain why detectors have missed it, while still letting the early universe end up with the right amount of it. I have also proposed a reason this protection holds, based on a recently studied kind of symmetry rule. Some of these models contain more than one kind of dark particle, and in some, part of the dark matter ends up moving much faster than the rest. I have studied whether large neutrino detectors could see this fast-moving part. Other models have a slightly heavier version of the dark matter particle that can survive from the early universe until today. When this heavier version hits an atom in a detector, it can drop to the lighter state and give the atom an extra kick, which could explain an unusually energetic event recently reported by the underground LZ experiment.
I also work on less conventional ways to measure dark matter. Even without electric charge, dark matter could still respond weakly to electric and magnetic fields. Its collisions would leave microscopic damage tracks in minerals, and rocks keep these tracks for up to a billion years, so paleo-detection in a small sample can record far more collisions than a laboratory detector running for a few years. On the cosmological side, I study where the cosmic magnetic fields seen in galaxies, and possibly in the near-empty space between them, come from. One possibility I am exploring is that an oscillating field from a hidden force strengthened them.
hep-ph
A non-invertible selection rule forbids the terms that give pNGB dark matter its mass at tree level. They appear only at one loop, which keeps direct-detection signals small but predictable.
hep-ph
Two nearly identical dark matter particles, one of which drops to the lighter state when it hits a nucleus and gives it an extra kick. We use this to interpret LZ's high-energy event at 248 keV.
hep-ph
A dark sector with two stable pNGB dark matter particles, where the heavier one converts into the lighter one and produces fast-moving “boosted” dark matter.
Presented a poster on two-component pseudo-Nambu-Goldstone boson dark matter at the 30th International Summer Institute on Phenomenology of Elementary Particle Physics and Cosmology.
Working on paleo-detection of dark matter.
Awarded a 2026 research encouragement grant from Fujukai (風樹会) in support of my research on methods to probe pseudo-Nambu-Goldstone dark matter.
Awarded the 2026 Sasakawa Scientific Research Grant from The Japan Science Society for a project on methods to probe pseudo-Nambu-Goldstone dark matter.
Presented an invited seminar on ways to probe pseudo-Nambu-Goldstone boson dark matter at Jilin University’s Young Scientist Forum.
Delivered my first physics presentation in Japanese on ways to probe pseudo-Nambu-Goldstone boson dark matter at the 131st JPS Kyushu Branch Meeting.
Completed Kyushu University’s Preparing Future Faculty Program and earned certification in Course Design in Higher Education (CDHE).
A hands-on walk-through of scanning the real singlet scalar dark matter model with micrOMEGAs, from the model that ships with micrOMEGAs to the relic-density curve.