Home > Research > Publications & Outputs > Study on cosmogenic activation above ground for...

Associated organisational unit

Electronic data

  • 2301.12970

    Accepted author manuscript, 1.66 MB, PDF document

    Available under license: CC BY: Creative Commons Attribution 4.0 International License

Links

Text available via DOI:

View graph of relations

Study on cosmogenic activation above ground for the DarkSide-20k project

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

Study on cosmogenic activation above ground for the DarkSide-20k project. / The Darkside Collaboration; Elersich, A.; Franchini, Paolo et al.
In: Astroparticle Physics, Vol. 152, 102878, 31.10.2023.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

APA

Vancouver

The Darkside Collaboration, Elersich A, Franchini P, Nowak J. Study on cosmogenic activation above ground for the DarkSide-20k project. Astroparticle Physics. 2023 Oct 31;152:102878. Epub 2023 Jul 10. doi: 10.1016/j.astropartphys.2023.102878

Author

The Darkside Collaboration ; Elersich, A. ; Franchini, Paolo et al. / Study on cosmogenic activation above ground for the DarkSide-20k project. In: Astroparticle Physics. 2023 ; Vol. 152.

Bibtex

@article{3a75bbbe5fe140cf9122aa555b7e5d99,
title = "Study on cosmogenic activation above ground for the DarkSide-20k project",
abstract = " The activation of materials due to the exposure to cosmic rays may become an important background source for experiments investigating rare event phenomena. DarkSide-20k is a direct detection experiment for galactic dark matter particles, using a two-phase liquid argon time projection chamber filled with 49.7 tonnes (active mass) of Underground Argon (UAr) depleted in 39Ar. Here, the cosmogenic activity of relevant long-lived radioisotopes induced in the argon and other massive components of the set-up has been estimated; production of 120 t of radiopure UAr is foreseen. The expected exposure above ground and production rates, either measured or calculated, have been considered. From the simulated counting rates in the detector due to cosmogenic isotopes, it is concluded that activation in copper and stainless steel is not problematic. Activation of titanium, considered in early designs but not used in the final design, is discussed. The activity of 39Ar induced during extraction, purification and transport on surface, in baseline conditions, is evaluated to be 2.8% of the activity measured in UAr from the same source, and thus considered acceptable. Other products in the UAr such as 37Ar and 3H are shown to not be relevant due to short half-life and assumed purification methods. ",
keywords = "astro-ph.IM, hep-ex, physics.ins-det",
author = "{The Darkside Collaboration} and A. Elersich and Paolo Franchini and Jaroslaw Nowak",
year = "2023",
month = oct,
day = "31",
doi = "10.1016/j.astropartphys.2023.102878",
language = "English",
volume = "152",
journal = "Astroparticle Physics",
issn = "0927-6505",
publisher = "Elsevier",

}

RIS

TY - JOUR

T1 - Study on cosmogenic activation above ground for the DarkSide-20k project

AU - The Darkside Collaboration

AU - Elersich, A.

AU - Franchini, Paolo

AU - Nowak, Jaroslaw

PY - 2023/10/31

Y1 - 2023/10/31

N2 - The activation of materials due to the exposure to cosmic rays may become an important background source for experiments investigating rare event phenomena. DarkSide-20k is a direct detection experiment for galactic dark matter particles, using a two-phase liquid argon time projection chamber filled with 49.7 tonnes (active mass) of Underground Argon (UAr) depleted in 39Ar. Here, the cosmogenic activity of relevant long-lived radioisotopes induced in the argon and other massive components of the set-up has been estimated; production of 120 t of radiopure UAr is foreseen. The expected exposure above ground and production rates, either measured or calculated, have been considered. From the simulated counting rates in the detector due to cosmogenic isotopes, it is concluded that activation in copper and stainless steel is not problematic. Activation of titanium, considered in early designs but not used in the final design, is discussed. The activity of 39Ar induced during extraction, purification and transport on surface, in baseline conditions, is evaluated to be 2.8% of the activity measured in UAr from the same source, and thus considered acceptable. Other products in the UAr such as 37Ar and 3H are shown to not be relevant due to short half-life and assumed purification methods.

AB - The activation of materials due to the exposure to cosmic rays may become an important background source for experiments investigating rare event phenomena. DarkSide-20k is a direct detection experiment for galactic dark matter particles, using a two-phase liquid argon time projection chamber filled with 49.7 tonnes (active mass) of Underground Argon (UAr) depleted in 39Ar. Here, the cosmogenic activity of relevant long-lived radioisotopes induced in the argon and other massive components of the set-up has been estimated; production of 120 t of radiopure UAr is foreseen. The expected exposure above ground and production rates, either measured or calculated, have been considered. From the simulated counting rates in the detector due to cosmogenic isotopes, it is concluded that activation in copper and stainless steel is not problematic. Activation of titanium, considered in early designs but not used in the final design, is discussed. The activity of 39Ar induced during extraction, purification and transport on surface, in baseline conditions, is evaluated to be 2.8% of the activity measured in UAr from the same source, and thus considered acceptable. Other products in the UAr such as 37Ar and 3H are shown to not be relevant due to short half-life and assumed purification methods.

KW - astro-ph.IM

KW - hep-ex

KW - physics.ins-det

U2 - 10.1016/j.astropartphys.2023.102878

DO - 10.1016/j.astropartphys.2023.102878

M3 - Journal article

VL - 152

JO - Astroparticle Physics

JF - Astroparticle Physics

SN - 0927-6505

M1 - 102878

ER -