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Absorption of Fermionic Dark Matter in the PICO-60 C$_{3}$F$_{8}$ Bubble Chamber

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arxiv 2504.13089 v2 pith:XJBL3BVA submitted 2025-04-17 hep-ex hep-ph

E. Adams , B. Ali , R. Anderson-Dornan , I. J. Arnquist , M. Bai , D. Baxter , E. Behnke , B. Broerman
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C. J. Chen K. Clark J. I. Collar P. S. Cooper D. Cranshaw C. Cripe M. Crisler C. E. Dahl M. Das S. Das S. Fallows J. Farine R. Filgas A. García-Viltres G. Giroux O. Harris H. Hawley-Herrera T. Hillier E. W. Hoppe C. M. Jackson M. Jin C. B. Krauss M. Laurin I. Lawson A. Leblanc H. Leng I. Levine C. Licciardi W. H. Lippincott Q. Malin P. Mitra V. Monette C. Moore R. Neilson A. J. Noble H. Nozard S. Pal M.-C. Piro S. Priya C. Rethmeier M. Robert A. E. Robinson J. Savoie S. J. Sekula A. Sonnenschein N. Starinski I. Štekl M. Tripathi E. Vázquez-Jáuregui U. Wichoski William Woodley V. Zacek J. Zhang
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classification hep-exhep-ph
keywords absorptiondarkmatterbubblechamberfermionicinteractionspico-60
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abstract

Fermionic dark matter absorption on nuclear targets via neutral current interactions is explored using a non-relativistic effective field theory framework. An analysis of data from the PICO-60 C$_{3}$F$_{8}$ bubble chamber sets leading constraints on spin-independent absorption for dark matter masses below 23 MeV/$\textit{c}^2$ and establishes the first limits on spin-dependent absorptive interactions. These results demonstrate the sensitivity of bubble chambers to low-mass dark matter and underscore the importance of absorption searches in expanding the parameter space of direct detection experiments.

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  1. Supernova cooling from neutrino-devouring dark matter

    hep-ph 2025-07 conditional novelty 6.0 of 10

    Supernova cooling excludes fermionic dark matter produced by neutrino scattering down to cross sections of about 10^-58 cm^2 for electrons and 10^-56 cm^2 for nucleons across the keV to 100 MeV mass range.

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