The focus on dark matter search has expanded to include low-mass particles such as axions or axion-like particles, and novel theoretical schemes extending the phenomenological landscape, within QCD and beyond, also garnered additional interest in recent decades. Assuming dark matter is composed of axions, in presence of a solenoidal magnetic field, they induce a displacement current that gives rise to a toroidal magnetic field. The Weakly Interacting Slender Particle detection with LC circuit (WISPLC) is a precision direct detection experiment that will search for light dark matter candidates such as axion-like particles in parts of the parameter space previously unexplored. We present two detection schemes of the signal in a pickup loop capturing the flux of this toroidal magnetic field. WISPLC operates in a broadband and a resonant scheme where a LC circuit is used to enhance the signal with an expected Q factor $\sim 10^4$. Taking into account the irreducible flux noise of the detector, we estimate the sensitivity of the experiment in the axion mass range between $10^{-11}$ eV and $10^{-6}$ eV to reach a detectable axion-photon coupling of $g_{aγγ}\approx 10^{-15}~\mathrm{GeV}^{-1}$, making it possible to probe mass ranges corresponding to ultralight axions motivated by string theory. The WISPLC experiment is fully funded and currently in the construction phase.
Search for QCD axion dark matter with transmon qubits and quantum circuit
Kyoto University（京都大学）；The University of Tokyo（东京大学）；International Center for Elementary Particle Physics (ICEPP), The University of Tokyo（东京大学 elementary particle physics 国际中心）；KEK（高能加速器研究机构）
Cavity, lumped-circuit, and spin-based detection of axion dark matter: differences and similarities
Bilkent University（比尔肯特大学）；Johannes Gutenberg-Universität Mainz（美因茨约翰内斯·古腾堡大学）；Helmholtz Institute Mainz（美因茨亥姆霍兹研究所）；GSI Helmholtzzentrum für Schwerionenforschung GmbH（德国重离子研究中心有限公司）；Department of Physics, University of California, Berkeley（加州大学伯克利分校物理系）；School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University（北京大学物理学院及核物理与核技术国家重点实验室）；Department of Physics and Astronomy, University of Mississippi（密西西比大学物理与天文学系）；University of Washington（华盛顿大学）；Department of Physics, California State University - East Bay（加州州立大学东湾分校物理系）
Quantum-enhanced Search for Galactic Dark Photons Using Cat-State Cavities
School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University（北京大学物理学院和核物理与技术国家重点实验室）；Center for High Energy Physics, Peking University（北京大学高能物理中心）；International Quantum Academy, Shenzhen（深圳国际量子学院）；Southern University of Science and Technology, Shenzhen（南方科技大学）；Beijing Laser Acceleration Innovation Center, Huairou, Beijing（北京怀柔激光加速创新中心）；School of Physics, Korea Institute for Advanced Study, Seoul（韩国高等研究院物理学院）；Shenzhen Branch, Hefei National Laboratory, Shenzhen（合肥国家实验室深圳分部）
Dark Matter Haloscope with a Disordered Dielectric Absorber
Research Laboratory of Electronics, Massachusetts Institute of Technology（麻省理工学院电子研究实验室）；Perimeter Institute for Theoretical Physics（理论物理前沿研究所）；Department of Physics and Astronomy, York University（约克大学物理与天文学系）；Department of Physics, University of Washington（华盛顿大学物理系）
Solid-state nuclear magnetic resonance search for axion-like dark matter with broadband SQUID magnetometry
Johns Hopkins University（约翰斯·霍普金斯大学）；Boston University（波士顿大学）；IQM Quantum Computers（IQM量子计算机公司）；Bilkent University（比尔肯特大学）；Johannes Gutenberg-Universität Mainz（美因茨约翰内斯·古腾堡大学）；Helmholtz Institute Mainz（美因茨亥姆霍兹研究所）；GSI Helmholtzzentrum für Schwerionenforschung GmbH（GSI重离子研究中心有限公司）；University of California, Berkeley（加州大学伯克利分校）；California State University - East Bay（加州州立大学东湾分校）
Search for low-mass electron-recoil dark matter using a single-charge sensitive SuperCDMS-HVeV Detector
University of British Columbia（不列颠哥伦比亚大学）；TRIUMF（特里姆夫实验室）；University of Toronto（多伦多大学）；Universidad Autónoma de Madrid（马德里自治大学）；Instituto de Física Teórica UAM-CSIC（UAM-CSIC理论物理研究所）；SLAC National Accelerator Laboratory（斯坦福直线加速器中心）；Kavli Institute for Particle Astrophysics and Cosmology（卡弗里粒子天体物理与宇宙学研究所）；Northeastern University（东北大学）；Texas A&M University（德克萨斯农工大学）；University of Florida（佛罗里达大学）
