Cosmogenic Muon Background Characterization for the Colorado Underground Research Institute (CURIE)
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arXiv
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| Format: | Preprint |
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2024
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| author | Keblbeck, Dakota K. Mayotte, Eric Greife, Uwe Leach, Kyle G. Van De Pontseele, Wouter |
| author_facet | Keblbeck, Dakota K. Mayotte, Eric Greife, Uwe Leach, Kyle G. Van De Pontseele, Wouter |
| contents | We present the characterization of cosmogenic muon backgrounds for the Colorado Underground Research Institute (CURIE), located in the Edgar Experimental Mine (EEM) in Idaho Springs, Colorado. The CURIE facility at the EEM offers a versatile shallow underground environment, with accessible horizontal tunnel access and stable rock formations ideal for low-background physics experiments. We have measured the total underground muon flux in two locations, Site 0 and Site 1, yielding values of $ϕ$ = 0.246 $\pm$ 0.020$_{sys.}$ $\pm$ 0.012$_{stat.}$ and 0.239 $\pm$ 0.025$_{sys.}$ $\pm$ 0.010$_{stat.}$ $μ\text{/}m^{2}\text{/}s$, respectively. We have utilized GEANT4 and PROPOSAL Monte Carlo simulations with Daemonflux and MUTE to model the muon flux at both sites, as well as an additional future location. We find good agreement between measurement and simulations, demonstrating the first instance of this computational framework being successfully used for depths $<$ 1 km.w.e. The measured underground flux corresponds to a factor of 700 reduction compared to the sea level flux. Additionally, we present a new depth-intensity relationship to normalize the mountain overburden to an equivalent flat depth, enabling direct comparison with other underground facilities. We report an average equivalent vertical depth of 0.415 $\pm$ 0.027 km.w.e. Based on our measurements, this work highlights the facility's capability for hosting low-background experiments, addressing the demand for shallow underground research spaces. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2411_01626 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Cosmogenic Muon Background Characterization for the Colorado Underground Research Institute (CURIE) Keblbeck, Dakota K. Mayotte, Eric Greife, Uwe Leach, Kyle G. Van De Pontseele, Wouter Instrumentation and Detectors High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics High Energy Physics - Experiment Nuclear Experiment We present the characterization of cosmogenic muon backgrounds for the Colorado Underground Research Institute (CURIE), located in the Edgar Experimental Mine (EEM) in Idaho Springs, Colorado. The CURIE facility at the EEM offers a versatile shallow underground environment, with accessible horizontal tunnel access and stable rock formations ideal for low-background physics experiments. We have measured the total underground muon flux in two locations, Site 0 and Site 1, yielding values of $ϕ$ = 0.246 $\pm$ 0.020$_{sys.}$ $\pm$ 0.012$_{stat.}$ and 0.239 $\pm$ 0.025$_{sys.}$ $\pm$ 0.010$_{stat.}$ $μ\text{/}m^{2}\text{/}s$, respectively. We have utilized GEANT4 and PROPOSAL Monte Carlo simulations with Daemonflux and MUTE to model the muon flux at both sites, as well as an additional future location. We find good agreement between measurement and simulations, demonstrating the first instance of this computational framework being successfully used for depths $<$ 1 km.w.e. The measured underground flux corresponds to a factor of 700 reduction compared to the sea level flux. Additionally, we present a new depth-intensity relationship to normalize the mountain overburden to an equivalent flat depth, enabling direct comparison with other underground facilities. We report an average equivalent vertical depth of 0.415 $\pm$ 0.027 km.w.e. Based on our measurements, this work highlights the facility's capability for hosting low-background experiments, addressing the demand for shallow underground research spaces. |
| title | Cosmogenic Muon Background Characterization for the Colorado Underground Research Institute (CURIE) |
| topic | Instrumentation and Detectors High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics High Energy Physics - Experiment Nuclear Experiment |
| url | https://arxiv.org/abs/2411.01626 |