I’m a postdoctoral researcher at the UC Berkeley Leinweber Institute for Theoretical Physics.
Precision measurement technology is advancing rapidly, and my work focuses on using it to accelerate the discovery of physics beyond the Standard Model. To do this, I find novel laboratory signals of new fundamental particles, consistent with relativity and quantum mechanics, and work with experimentalists to develop effective “tabletop” detectors.
For instance, I have worked on searches for axion dark matter using superconducting cavities, now pursued in America, Europe, and China. I have also investigated infrared modifications of electromagnetism and gravity from continuous spin, new signals of axial vector dark matter, and the quantum effects of gravitational waves.
Previously, I got my PhD at Stanford in 2024, Master’s degrees at Cambridge and Oxford, and a Bachelor’s degree at MIT. During that time I spent a lot of energy on physics education, and I’m still always interested in hearing a good physics puzzle.
I can be reached at kzhou7@berkeley.edu, and a complete CV is available here.
Each paper comes with talk slides, which provide an illustrated introduction.
Intrinsically quantum effects of gravitational waves and dark matter carry extra powers of the weak coupling, relative to classical effects. This strong suppression can only be evaded using highly nonclassical detector states.
Conducting walls have a very small, but observable effect on measurements of electron $g-2$. We compute it from first principles with quantum field theory, and show how it can be accounted for in future measurements.
Intrinsically quantum effects of axion dark matter are always highly suppressed, and in practice undetectable. Thus, even though the axion may be in a nonclassical state, it can still be treated as a classical field.
The heterodyne approach to axion detection enhances the axion signal power. A prototype cavity was designed and tested, with a novel geometry that maximizes signal, suppresses noise, and allows a wide tuning range.
Light dark matter particles could couple directly to electron spin. Since the same is true for neutrons, existing neutron scattering data can accurately predict the signal rate of a dark matter experiment.
In Autumn 2022, I was the TA for Stanford’s introductory quantum field theory class, taught by Prof. Bernhard Mistlberger. We overhauled the course and made new problem sets, which strike a balance between traditional particle physics and connections to other fields. I gave weekly sections which laid out the big picture and trained problem solving skills.
From 2019 to 2024, I coached the US Physics Team and wrote many of its exam questions and solutions, while developing a comprehensive set of training material. These handouts are the result. They contain 1,000 tricky, solved problems covering a very wide range of ideas, along with hundreds of examples and remarks. For details, see the syllabus and FAQ. To see if you’re ready to start the handouts, try the preliminary problems (answers here).
I don’t currently write or run the USAPhO, and I don’t have time to tutor, but I do still update the handouts occasionally; feel free to reach out (at my personal address, kzhou7@gmail.com) if you find an issue or have a suggestion. For Russian translations, see Physics Hub.
These are my notes from learning physics at MIT, Cambridge’s Part III and Oxford’s MMathPhys. I use them for personal reference, but they’re terse, and not good to learn from. If you like the style, you can download a TeX template here.