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相关论文: Cosmogenic production of $^{39}$Ar and $^{37}$Ar i…

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Underground argon (UAr) with lower cosmogenic activities of $^{39}Ar$ and $^{42}Ar$ has been planned as a detector in detecting scintillation light and charge collection using time projection chambers for dark matter searches and as a veto…

仪器与探测器 · 物理学 2022-06-08 Chao Zhang , Dongming Mei

Radioactive decays from ^{42}Ar and its progeny ^{42}K are potential background sources in large-scale liquid-argon-based neutrino and dark matter experiments. In the atmosphere, ^{42}Ar is produced primarily by cosmogenic activation on…

仪器与探测器 · 物理学 2023-09-29 Sagar S. Poudel , Ben Loer , Richard Saldanha , Brianne R. Hackett , Henning O. Back

In this paper, we demonstrate the use of physical models to evaluate the production of $^{39}$Ar and $^{40}$Ar underground. Considering both cosmogenic $^{39}$Ar production and radiogenic $^{40}$Ar production in situ and from external…

核实验 · 物理学 2010-05-25 D. -M. Mei , Z. -B. Yin , J. Spaans , M. Koppang , A. Hime , C. Keller , V. M. Gehman

The cosmogenic $^{39}$Ar(t$_{1/2}$= 268 years) isotope of argon is used for geophysical dating and tracing owing to its appropriate half-life and chemical inertness as a noble gas; $^{39}$Ar serves also in nuclear weapon test monitoring. We…

Accurate understanding of the subsurface production rate of the radionuclide $^{39}$Ar is necessary for argon dating techniques and noble gas geochemistry of the shallow and the deep Earth, and is also of interest to the WIMP dark matter…

We estimate the amount of $^{37}$Ar produced in natural xenon via cosmic ray-induced spallation, an inevitable consequence of the transportation and storage of xenon on the Earth's surface. We then calculate the resulting $^{37}$Ar…

高能物理 - 实验 · 物理学 2022-05-11 J. Aalbers , D. S. Akerib , A. K. Al Musalhi , F. Alder , S. K. Alsum , C. S. Amarasinghe , A. Ames , T. J. Anderson , N. Angelides , H. M. Araújo , J. E. Armstrong , M. Arthurs , X. Bai , A. Baker , J. Balajthy , S. Balashov , J. Bang , J. W. Bargemann , D. Bauer , A. Baxter , K. Beattie , E. P. Bernard , A. Bhatti , A. Biekert , T. P. Biesiadzinski , H. J. Birch , G. M. Blockinger , E. Bodnia , B. Boxer , C. A. J. Brew , P. Brás , S. Burdin , J. K. Busenitz , M. Buuck , R. Cabrita , M. C. Carmona-Benitez , M. Cascella , C. Chan , A. Chawla , H. Chen , N. I. Chott , A. Cole , M. V. Converse , A. Cottle , G. Cox , O. Creaner , J. E. Cutter , C. E. Dahl , A. David , L. de Viveiros , J. E. Y. Dobson , E. Druszkiewicz , S. R. Eriksen , A. Fan , S. Fayer , N. M. Fearon , S. Fiorucci , H. Flaecher , E. D. Fraser , T. Fruth , R. J. Gaitskell , J. Genovesi , C. Ghag , E. Gibson , M. G. D. Gilchriese , S. Gokhale , M. G. D. van der Grinten , C. B. Gwilliam , C. R. Hall , S. J. Haselschwardt , S. A. Hertel , M. Horn , D. Q. Huang , D. Hunt , C. M. Ignarra , O. Jahangir , R. S. James , W. Ji , J. Johnson , A. C. Kaboth , A. C. Kamaha , K. Kamdin , D. Khaitan , A. Khazov , I. Khurana , D. Kodroff , L. Korley , E. V. Korolkova , H. Kraus , S. Kravitz , L. Kreczko , V. A. Kudryavtsev , E. A. Leason , D. S. Leonard , K. T. Lesko , C. Levy , J. Lee , J. Lin , A. Lindote , R. Linehan , W. H. Lippincott , X. Liu , M. I. Lopes , E. Lopez Asamar , B. Lopez-Paredes , W. Lorenzon , S. Luitz , P. A. Majewski , A. Manalaysay , L. Manenti , R. L. Mannino , N. Marangou , M. E. McCarthy , D. N. McKinsey , J. McLaughlin , E. H. Miller , E. Mizrachi , A. Monte , M. E. Monzani , J. A. Morad , J. D. Morales Mendoza , E. Morrison , B. J. Mount , A. St. J. Murphy , D. Naim , A. Naylor , C. Nedlik , H. N. Nelson , F. Neves , J. A. Nikoleyczik , A. Nilima , I. Olcina , K. Oliver-Mallory , S. Pal , K. J. Palladino , J. Palmer , N. Parveen , S. J. Patton , E. K. Pease , B. Penning , G. Pereira , E. Perry , J. Pershing , A. Piepke , D. Porzio , Y. Qie , J. Reichenbacher , C. A. Rhyne , A. Richards , Q. Riffard , %Q. Riffard , G. R. C. Rischbieter , R. Rosero , P. Rossiter , T. Rushton , D. Santone , A. B. M. R. Sazzad , R. W. Schnee , P. R. Scovell , S. Shaw , T. A. Shutt , J. J. Silk , C. Silva , G. Sinev , R. Smith , M. Solmaz , V. N. Solovov , P. Sorensen , J. Soria , I. Stancu , A. Stevens , K. Stifter , B. Suerfu , T. J. Sumner , N. Swanson , M. Szydagis , W. C. Taylor , R. Taylor , D. J. Temples , P. A. Terman , D. R. Tiedt , M. Timalsina , W. H. To , Z. Tong , D. R. Tovey , M. Trask , M. Tripathi , D. R. Tronstad , W. Turner , U. Utku , A. Vaitkus , B. Wang , Y. Wang , J. J. Wang , W. Wang , J. R. Watson , R. C. Webb , R. G. White , T. J. Whitis , M. Williams , F. L. H. Wolfs , S. Woodford , D. Woodward , C. J. Wright , Q. Xia , X. Xiang , J. Xu , M. Yeh

The production of $^{3}$H, $^{7}$Be, and $^{22}$Na by interactions of cosmic-ray particles with silicon can produce radioactive backgrounds in detectors used to search for rare events. Through controlled irradiation of silicon CCDs and…

The direct detection of dark matter particles requires ultra-low background conditions at energies below a few tens of keV. Radioactive isotopes are produced via cosmogenic activation in detectors and other materials and those isotopes…

The production of long-lived radioactive isotopes in materials due to the exposure to cosmic rays on Earth surface can be an hazard for experiments demanding ultra-low background conditions, typically performed deep underground. Production…

The production of long-lived radioactive isotopes due to the exposure to cosmic rays on the Earth's surface is an hazard for experiments searching for rare events like the direct detection of galactic dark matter particles. The use of large…

天体物理仪器与方法 · 物理学 2024-02-06 S. Cebrian

The $^{36}$Ar$(n,\gamma)^{37}$Ar ($t_{1/2}$ = 35 d) and $^{38}$Ar$(n,\gamma)^{39}$Ar (269 y) reactions were studied for the first time with a quasi-Maxwellian ($kT \sim 47$ keV) neutron flux for Maxwellian Average Cross Section (MACS)…

Neutrons produced in nuclear interactions initiated by cosmic-ray muons present an irreducible background to many rare-event searches, even in detectors located deep underground. Models for the production of these neutrons have been tested…

高能物理 - 实验 · 物理学 2019-12-18 B. Aharmim , S. N. Ahmed , A. E. Anthony , N. Barros , E. W. Beier , A. Bellerive , B. Beltran , M. Bergevin , S. D. Biller , R. Bonventre , K. Boudjemline , M. G. Boulay , B. Cai , E. J. Callaghan , J. Caravaca , Y. D. Chan , D. Chauhan , M. Chen , B. T. Cleveland , G. A. Cox , R. Curley , X. Dai , H. Deng , F. B. Descamps , J. A. Detwiler , P. J. Doe , G. Doucas , P. -L. Drouin , M. Dunford , S. R. Elliott , H. C. Evans , G. T. Ewan , J. Farine , H. Fergani , F. Fleurot , R. J. Ford , J. A. Formaggio , N. Gagnon , K. Gilje , J. TM. Goon , K. Graham , E. Guillian , S. Habib , R. L. Hahn , A. L. Hallin , E. D. Hallman , P. J. Harvey , R. Hazama , W. J. Heintzelman , J. Heise , R. L. Helmer , A. Hime , C. Howard , M. Huang , P. Jagam , B. Jamieson , N. A. Jelley , M. Jerkins , C. Kéfélian , K. J. Keeter , J. R. Klein , L. L. Kormos , M. Kos , A. Kr\u , C. Kraus , C. B. Krauss , T. Kutter , C. C. M. Kyba , B. J. Land , R. Lange , J. Law , I. T. Lawson , K. T. Lesko , J. R. Leslie , I. Levine , J. C. Loach , R. MacLellan , S. Majerus , H. B. Mak , J. Maneira , R. D. Martin , A. Mastbaum , N. McCauley , A. B. McDonald , S. R. McGee , M. L. Miller , B. Monreal , J. Monroe , B. G. Nickel , A. J. Noble , H. M. O'Keeffe , N. S. Oblath , C. E. Okada , R. W. Ollerhead , G. D. Orebi Gann , S. M. Oser , R. A. Ott , S. J. M. Peeters , A. W. P. Poon , G. Prior , S. D. Reitzner , K. Rielage , B. C. Robertson , R. G. H. Robertson , M. H. Schwendener , J. A. Secrest , S. R. Seibert , O. Simard , D. Sinclair , P. Skensved , T. J. Sonley , L. C. Stonehill , G. Teš , N. Tolich , T. Tsui , R. Van Berg , B. A. VanDevender , C. J. Virtue , B. L. Wall , D. Waller , H. Wan Chan Tseung , D. L. Wark , J. Wendland , N. West , J. F. Wilkerson , J. R. Wilson , T. Winchester , A. Wright , M. Yeh , F. Zhang , K. Zuber

$^{37}$Ar is a promising candidate for complementing radioxenon isotopes as indicators of underground nuclear explosions. This study evaluates its potential anthropogenic background caused by emissions from commercial pressurised water…

仪器与探测器 · 物理学 2020-06-05 Gerald Kirchner , Franziska Gerfen , Anna Heise , Timo Schlüschen

The propagation of cosmic rays in the Earth's atmosphere is simulated. Calculations of the omnidirectional differential flux of neutrons for different solar activity levels are presented. The solar activity effect on the production rate of…

地球与行星天体物理 · 物理学 2012-10-22 A. V. Nesterenok , V. O. Naidenov

The production of radioactive isotopes by interactions of cosmic-ray particles with sodium iodide (NaI) crystals can produce radioactive backgrounds in detectors used to search for rare events. Through controlled irradiation of NaI crystals…

The activation of materials due to exposure to cosmic rays may become an important background source for experiments investigating rare event phenomena. DarkSide-20k, currently under construction at the Laboratori Nazionali del Gran Sasso,…

天体物理仪器与方法 · 物理学 2023-07-26 20k Collaboration

We measured the production of \nuc{57}{Co}, \nuc{54}{Mn}, \nuc{68}{Ge}, \nuc{65}{Zn}, and \nuc{60}{Co} in a sample of Ge enriched in isotope 76 due to high-energy neutron interactions. These isotopes, especially \nuc{68}{Ge}, are critical…

核实验 · 物理学 2010-12-02 S. R. Elliott , V. E. Guiseppe , R. A. Johnson , B. H. LaRoque , S. G. Mashnik

Experiments looking for rare events like the direct detection of dark matter particles, neutrino interactions or the nuclear double beta decay are operated deep underground to suppress the effect of cosmic rays. But the production of…

核实验 · 物理学 2017-08-25 Susana Cebrian

A physical model of Geant4-based simulation of galactic cosmic ray (GCR) particles interaction with the lunar surface matter has been developed to investigate the production rate of cosmogenic nuclei. In this model the GCRs, mainly very…

地球与行星天体物理 · 物理学 2013-09-10 Tie-Kuang Dong , Su-Jun Yun , Tao Ma , Jin Chang , Wu-Dong Dong , Xiao-Ping Zhang , Guo-Long Li , Zhong-Zhou Ren

The DarkSide-50 experiment demonstrated the ability to extract and purify argon from deep underground sources and showed that the concentration of $^{39}$Ar in that argon was greatly reduced from the level found in argon derived from the…

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