What can a GNOME do? Search targets for the Global Network of Optical Magnetometers for Exotic physics searches

in: Annalen der Physik (2023)
Budker, Dmitry; Afach, Samer; Aybas Tumturk, Deniz; Bekker, Hendrik; Buchler, Ben C.; Cervantes, Kassandra; Derevianko, Andrei; Figueroa, Nataniel L.; Folman, Ron; Gavilan-Martin, Daniel; Givon, Menachem; Grujic, Zoran; Guo, Hong; Hamilton, Paul S.; Hedges, Morgan; Jackson Kimball, Derek F.; Khamis, Sami; Kim, Dongok; Klinger, Emmanuel; Kryemadhi, Abaz; Liu, Xiyu; Lukasiewicz, Grzegorz; Masia-Roig, Hector; Padniuk, Mikhail; Palm, Christopher A.; Park, Sun Yool; Pearson, Heather R.; Peng, Xiang; Pospelov, Maxim; Pustelny, Szymon; Rosenzweig, Yossi; Ruimi, Ophir M.; Scholtes, Theo; Segura, Perrin C.; Semertzidis, Yannis; Shin, Yun Chang; Smiga, Joseph A.; Stadnik, Yevgeny V.; Stalnaker, Jason E.; Sulai, Ibrahim; Tandon, Dhruv; Vu, Kenneth; Weis, Antoine; Wickenbrock, Arne; Wilson, Tatum; Wu, Teng; Xiao, Wei; Yang, Yucheng; Yu, Dongrui; Yu, Felix; Zhang, Jianwei; Zhao, Yixin
Numerous observations suggest that there exist undiscovered beyond-the-standard-model particles and fields. Because of their unknown nature, these exotic particles and fields could interact with standard model particles in many different ways and assume a variety of possible configurations. Here, an overview of the global network of optical magnetometers for exotic physics searches (GNOME), the ongoing experimental program designed to test a wide range of exotic physics scenarios, is presented. The GNOME experiment utilizes a worldwide network of shielded atomic magnetometers (and, more recently, comagnetometers) to search for spatially and temporally correlated signals due to torques on atomic spins from exotic fields of astrophysical origin. The temporal characteristics of a variety of possible signals currently under investigation such as those from topological defect dark matter (axion-like particle domain walls), axion-like particle stars, solitons of complex-valued scalar fields (Q-balls), stochastic fluctuations of bosonic dark matter fields, a solar axion-like particle halo, and bursts of ultralight bosonic fields produced by cataclysmic astrophysical events such as binary black hole mergers are surveyed.

Cookies & Skripte von Drittanbietern

Diese Website verwendet Cookies. Für eine optimale Performance, eine reibungslose Verwendung sozialer Medien und aus Werbezwecken empfiehlt es sich, der Verwendung von Cookies & Skripten durch Drittanbieter zuzustimmen. Dafür werden möglicherweise Informationen zu Ihrer Verwendung der Website von Drittanbietern für soziale Medien, Werbung und Analysen weitergegeben.
Weitere Informationen finden Sie unter Datenschutz und im Impressum.
Welchen Cookies & Skripten und der damit verbundenen Verarbeitung Ihrer persönlichen Daten stimmen Sie zu?

Sie können Ihre Einstellungen jederzeit unter Datenschutz ändern.