Absorption of Fermionic Dark Matter in the PICO-60 C$_{3}$F$_{8}$ Bubble Chamber
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arXiv
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2025
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| author | Adams, E. Ali, B. Anderson-Dornan, R. Arnquist, I. J. Bai, M. Baxter, D. Behnke, E. Broerman, B. Chen, C. J. Clark, K. Collar, J. I. Cooper, P. S. Cranshaw, D. Cripe, C. Crisler, M. Dahl, C. E. Das, M. Das, S. Fallows, S. Farine, J. Filgas, R. García-Viltres, A. Giroux, G. Harris, O. Hawley-Herrera, H. Hillier, T. Hoppe, E. W. Jackson, C. M. Jin, M. Krauss, C. B. Laurin, M. Lawson, I. Leblanc, A. Leng, H. Levine, I. Licciardi, C. Lippincott, W. H. Malin, Q. Mitra, P. Monette, V. Moore, C. Neilson, R. Noble, A. J. Nozard, H. Pal, S. Piro, M. -C. Priya, S. Rethmeier, C. Robert, M. Robinson, A. E. Savoie, J. Sekula, S. J. Sonnenschein, A. Starinski, N. Štekl, I. Tripathi, M. Vázquez-Jáuregui, E. Wichoski, U. Woodley, William Zacek, V. Zhang, J. |
| author_facet | Adams, E. Ali, B. Anderson-Dornan, R. Arnquist, I. J. Bai, M. Baxter, D. Behnke, E. Broerman, B. Chen, C. J. Clark, K. Collar, J. I. Cooper, P. S. Cranshaw, D. Cripe, C. Crisler, M. Dahl, C. E. Das, M. Das, S. Fallows, S. Farine, J. Filgas, R. García-Viltres, A. Giroux, G. Harris, O. Hawley-Herrera, H. Hillier, T. Hoppe, E. W. Jackson, C. M. Jin, M. Krauss, C. B. Laurin, M. Lawson, I. Leblanc, A. Leng, H. Levine, I. Licciardi, C. Lippincott, W. H. Malin, Q. Mitra, P. Monette, V. Moore, C. Neilson, R. Noble, A. J. Nozard, H. Pal, S. Piro, M. -C. Priya, S. Rethmeier, C. Robert, M. Robinson, A. E. Savoie, J. Sekula, S. J. Sonnenschein, A. Starinski, N. Štekl, I. Tripathi, M. Vázquez-Jáuregui, E. Wichoski, U. Woodley, William Zacek, V. Zhang, J. |
| contents | 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2504_13089 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Absorption of Fermionic Dark Matter in the PICO-60 C$_{3}$F$_{8}$ Bubble Chamber Adams, E. Ali, B. Anderson-Dornan, R. Arnquist, I. J. Bai, M. Baxter, D. Behnke, E. Broerman, B. Chen, C. J. Clark, K. Collar, J. I. Cooper, P. S. Cranshaw, D. Cripe, C. Crisler, M. Dahl, C. E. Das, M. Das, S. Fallows, S. Farine, J. Filgas, R. García-Viltres, A. Giroux, G. Harris, O. Hawley-Herrera, H. Hillier, T. Hoppe, E. W. Jackson, C. M. Jin, M. Krauss, C. B. Laurin, M. Lawson, I. Leblanc, A. Leng, H. Levine, I. Licciardi, C. Lippincott, W. H. Malin, Q. Mitra, P. Monette, V. Moore, C. Neilson, R. Noble, A. J. Nozard, H. Pal, S. Piro, M. -C. Priya, S. Rethmeier, C. Robert, M. Robinson, A. E. Savoie, J. Sekula, S. J. Sonnenschein, A. Starinski, N. Štekl, I. Tripathi, M. Vázquez-Jáuregui, E. Wichoski, U. Woodley, William Zacek, V. Zhang, J. High Energy Physics - Experiment High Energy Physics - Phenomenology 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. |
| title | Absorption of Fermionic Dark Matter in the PICO-60 C$_{3}$F$_{8}$ Bubble Chamber |
| topic | High Energy Physics - Experiment High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2504.13089 |