- Title题目 Search for axion-like particle as dark matter candidate with nuclear magnetic resonance (利用核磁共振寻找暗物质类轴子粒子)
- Speaker报告人 张宇哲 (约翰内斯·谷登堡-美因茨大学)
- Date日期 2022年9月7日 16:00
- Venue地点 线上,腾讯会议地址 https://meeting.tencent.com/dm/Z1NAVCIInIeD
Axion originated from a solution to the strong-CP problem[1, 2]. During the past decade, axion and other light pseudoscalar bosons (< 1 eV/c^2) which are collectively referred to as axion-like particles or ALPs have become well-motivated dark matter (DM) candidates. The cosmic axion spin precession experiment (CASPEr)[3] aims at probing axion and ALPs with nuclear magnetic resonance (NMR) technique. CASPEr-Gradient in Mainz searches for the coupling of nuclear spins to the gradient of the ALP field[4]. The experimental apparatus was designed to scan ALP Compton frequency from 100 Hz to 600 MHz, corresponding to ALP mass range of approximately 10^-13 to 10^-6 eV. The detection system has been commissioned for this research. We performed a 10-hr measurement with thermally-polarized liquid methanol sample with a 25 ppm homogeneity at the 317 G leading field, which corresponds to searching for an ALP field at 1.349533 MHz with 33 Hz bandwidth. Noise of the setup and ALP coupling constant exclusion have been analyzed for the measurement.
References:
[1] Peccei, R., and Quinn, H.: Constraints imposed by CP conservation in the presence of pseudoparticles. Phys. Rev. D 16, 1791 (1977).
[2] Peccei, R., and Quinn, H.: CP conservation in the presence of pseudoparticles. Phys. Rev. Lett. 38, 1440 (1977).
[3] Derek F. Jackson Kimball et al. “Overview of the Cosmic Axion Spin Precession Experiment (CASPEr)”. In: Microwave Cavities and Detectors for Axion Research. Ed. by Gianpaolo Carosi and Gray Rybka. Cham: Springer International Publishing, 2020, pp. 105–121. isbn: 978-3-030-43761-9.
[4] Peter W. Graham and Surjeet Rajendran. “New observables for direct detection of axion dark matter”. In: Phys. Rev. D 88 (3 Aug. 2013), p. 035023. doi: 10.1103/PhysRevD.88.035023. url: https://link.aps.org/doi/10.1103/PhysRevD.88.035023.