The Felsenkeller shallow-underground laboratory for nuclear astrophysics.

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Title: The Felsenkeller shallow-underground laboratory for nuclear astrophysics.
Authors: Bemmerer, Daniel1 (AUTHOR) d.bemmerer@hzdr.de, Boeltzig, Axel1 (AUTHOR), Grieger, Marcel1 (AUTHOR), Gudat, Katharina1 (AUTHOR), Hensel, Thomas1,2 (AUTHOR), Masha, Eliana1 (AUTHOR), Osswald, Max1,2 (AUTHOR), Poser, Bruno1,2 (AUTHOR), Rümmler, Simon1,2 (AUTHOR), Schmidt, Konrad1 (AUTHOR), Taín, José Luis3 (AUTHOR), Tarifeño-Saldivia, Ariel3,4 (AUTHOR), Turkat, Steffen2 (AUTHOR), Yadav, Anup1,2 (AUTHOR), Zuber, Kai2 (AUTHOR)
Source: European Physical Journal A -- Hadrons & Nuclei. Jan2025, Vol. 61 Issue 1, p1-15. 15p.
Subjects: Cosmic ray muons, Ion accelerators, Background radiation, Physical sciences, Muons
Abstract: In the Felsenkeller shallow-underground site, protected from cosmic muons by a 45 m thick rock overburden, a research laboratory including a 5 MV Pelletron ion accelerator and a number of radioactivity-measurement setups is located. The laboratory and its installations are described in detail. The background radiation has been studied, finding suppression factors of 40 for cosmic-ray muons, 200 for ambient neutrons, and 100 for the background in germanium γ -ray detectors. Using an additional active muon veto, typically the background is just twice as high as in very deep underground laboratories. The properties of the accelerator including its external and internal ion sources and beam line are given. For the radioactivity counting setup, detection limits in the 10 - 4 Bq range have been obtained. Practical aspects for the usage of the laboratory by outside scientific users are discussed. [ABSTRACT FROM AUTHOR]
Copyright of European Physical Journal A -- Hadrons & Nuclei is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: The Felsenkeller shallow-underground laboratory for nuclear astrophysics.
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  Data: <searchLink fieldCode="AR" term="%22Bemmerer%2C+Daniel%22">Bemmerer, Daniel</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> d.bemmerer@hzdr.de</i><br /><searchLink fieldCode="AR" term="%22Boeltzig%2C+Axel%22">Boeltzig, Axel</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Grieger%2C+Marcel%22">Grieger, Marcel</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Gudat%2C+Katharina%22">Gudat, Katharina</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Hensel%2C+Thomas%22">Hensel, Thomas</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Masha%2C+Eliana%22">Masha, Eliana</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Osswald%2C+Max%22">Osswald, Max</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Poser%2C+Bruno%22">Poser, Bruno</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Rümmler%2C+Simon%22">Rümmler, Simon</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Schmidt%2C+Konrad%22">Schmidt, Konrad</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Taín%2C+José+Luis%22">Taín, José Luis</searchLink><relatesTo>3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Tarifeño-Saldivia%2C+Ariel%22">Tarifeño-Saldivia, Ariel</searchLink><relatesTo>3,4</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Turkat%2C+Steffen%22">Turkat, Steffen</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Yadav%2C+Anup%22">Yadav, Anup</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Zuber%2C+Kai%22">Zuber, Kai</searchLink><relatesTo>2</relatesTo> (AUTHOR)
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  Data: <searchLink fieldCode="JN" term="%22European+Physical+Journal+A+--+Hadrons+%26+Nuclei%22">European Physical Journal A -- Hadrons & Nuclei</searchLink>. Jan2025, Vol. 61 Issue 1, p1-15. 15p.
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  Data: <searchLink fieldCode="DE" term="%22Cosmic+ray+muons%22">Cosmic ray muons</searchLink><br /><searchLink fieldCode="DE" term="%22Ion+accelerators%22">Ion accelerators</searchLink><br /><searchLink fieldCode="DE" term="%22Background+radiation%22">Background radiation</searchLink><br /><searchLink fieldCode="DE" term="%22Physical+sciences%22">Physical sciences</searchLink><br /><searchLink fieldCode="DE" term="%22Muons%22">Muons</searchLink>
– Name: Abstract
  Label: Abstract
  Group: Ab
  Data: In the Felsenkeller shallow-underground site, protected from cosmic muons by a 45 m thick rock overburden, a research laboratory including a 5 MV Pelletron ion accelerator and a number of radioactivity-measurement setups is located. The laboratory and its installations are described in detail. The background radiation has been studied, finding suppression factors of 40 for cosmic-ray muons, 200 for ambient neutrons, and 100 for the background in germanium γ -ray detectors. Using an additional active muon veto, typically the background is just twice as high as in very deep underground laboratories. The properties of the accelerator including its external and internal ion sources and beam line are given. For the radioactivity counting setup, detection limits in the 10 - 4 Bq range have been obtained. Practical aspects for the usage of the laboratory by outside scientific users are discussed. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
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  Data: <i>Copyright of European Physical Journal A -- Hadrons & Nuclei is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1140/epja/s10050-025-01490-z
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      – Code: eng
        Text: English
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      – SubjectFull: Cosmic ray muons
        Type: general
      – SubjectFull: Ion accelerators
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      – SubjectFull: Background radiation
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      – SubjectFull: Physical sciences
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      – SubjectFull: Muons
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      – TitleFull: The Felsenkeller shallow-underground laboratory for nuclear astrophysics.
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              Text: Jan2025
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