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Title: Kr 83 m calibration of the 2013 LUX dark matter search

Abstract

Here, LUX was the first dark matter experiment to use a 83mKr calibration source. In this paper, we describe the source preparation and injection. We also present several 83mKr calibration applications in the context of the 2013 LUX exposure, including the measurement of temporal and spatial variation in scintillation and charge signal amplitudes, and several methods to understand the electric field within the time projection chamber.

Authors:
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Publication Date:
Research Org.:
SLAC National Accelerator Lab., Menlo Park, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of Rochester, NY (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
Contributing Org.:
LUX Collaboration
OSTI Identifier:
1417655
Alternate Identifier(s):
OSTI ID: 1414860; OSTI ID: 1436658; OSTI ID: 1532544
Grant/Contract Number:  
AC02-05CH11231; FG02-11ER41738; AC05-06OR23100; AC52-07NA27344; FG01-91ER40618; FG02-08ER41549; FG02-91ER40674; FG02-91ER40688; FG02-95ER40917; NA0000979; SC0006605; SC0010010; SC0015535; PHY-0750671; PHY-0801536; PHY-1003660; PHY-1004661; PHY-1102470; PHY-1312561; PHY-1347449; PHY-1505868; PHY-1636738; RA0350; PTDC/FIS-NUC/1525/2014; ST/K502042/1 (AB); ST/K502406/1 (SS); ST/M503538/1 (KY); SC005336; IE120804; AC02-76SF00515; SC0017891
Resource Type:
Journal Article: Accepted Manuscript
Journal Name:
Physical Review D
Additional Journal Information:
Journal Volume: 96; Journal Issue: 11; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS

Citation Formats

Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Druszkiewicz, E., Edwards, B. N., Fallon, S. R., Fan, A., Fiorucci, S., Gaitskell, R. J., Genovesi, J., Ghag, C., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O’Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Velan, V., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., and Zhang, C. Kr83m calibration of the 2013 LUX dark matter search. United States: N. p., 2017. Web. doi:10.1103/PhysRevD.96.112009.
Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Druszkiewicz, E., Edwards, B. N., Fallon, S. R., Fan, A., Fiorucci, S., Gaitskell, R. J., Genovesi, J., Ghag, C., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O’Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Velan, V., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., & Zhang, C. Kr83m calibration of the 2013 LUX dark matter search. United States. doi:10.1103/PhysRevD.96.112009.
Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Druszkiewicz, E., Edwards, B. N., Fallon, S. R., Fan, A., Fiorucci, S., Gaitskell, R. J., Genovesi, J., Ghag, C., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O’Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Velan, V., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., and Zhang, C. Tue . "Kr83m calibration of the 2013 LUX dark matter search". United States. doi:10.1103/PhysRevD.96.112009. https://www.osti.gov/servlets/purl/1417655.
@article{osti_1417655,
title = {Kr83m calibration of the 2013 LUX dark matter search},
author = {Akerib, D. S. and Alsum, S. and Araújo, H. M. and Bai, X. and Bailey, A. J. and Balajthy, J. and Beltrame, P. and Bernard, E. P. and Bernstein, A. and Biesiadzinski, T. P. and Boulton, E. M. and Brás, P. and Byram, D. and Cahn, S. B. and Carmona-Benitez, M. C. and Chan, C. and Currie, A. and Cutter, J. E. and Davison, T. J. R. and Dobi, A. and Druszkiewicz, E. and Edwards, B. N. and Fallon, S. R. and Fan, A. and Fiorucci, S. and Gaitskell, R. J. and Genovesi, J. and Ghag, C. and Gilchriese, M. G. D. and Hall, C. R. and Hanhardt, M. and Haselschwardt, S. J. and Hertel, S. A. and Hogan, D. P. and Horn, M. and Huang, D. Q. and Ignarra, C. M. and Jacobsen, R. G. and Ji, W. and Kamdin, K. and Kazkaz, K. and Khaitan, D. and Knoche, R. and Larsen, N. A. and Lenardo, B. G. and Lesko, K. T. and Lindote, A. and Lopes, M. I. and Manalaysay, A. and Mannino, R. L. and Marzioni, M. F. and McKinsey, D. N. and Mei, D. -M. and Mock, J. and Moongweluwan, M. and Morad, J. A. and Murphy, A. St. J. and Nehrkorn, C. and Nelson, H. N. and Neves, F. and O’Sullivan, K. and Oliver-Mallory, K. C. and Palladino, K. J. and Pease, E. K. and Rhyne, C. and Shaw, S. and Shutt, T. A. and Silva, C. and Solmaz, M. and Solovov, V. N. and Sorensen, P. and Sumner, T. J. and Szydagis, M. and Taylor, D. J. and Taylor, W. C. and Tennyson, B. P. and Terman, P. A. and Tiedt, D. R. and To, W. H. and Tripathi, M. and Tvrznikova, L. and Uvarov, S. and Velan, V. and Verbus, J. R. and Webb, R. C. and White, J. T. and Whitis, T. J. and Witherell, M. S. and Wolfs, F. L. H. and Xu, J. and Yazdani, K. and Young, S. K. and Zhang, C.},
abstractNote = {Here, LUX was the first dark matter experiment to use a 83mKr calibration source. In this paper, we describe the source preparation and injection. We also present several 83mKr calibration applications in the context of the 2013 LUX exposure, including the measurement of temporal and spatial variation in scintillation and charge signal amplitudes, and several methods to understand the electric field within the time projection chamber.},
doi = {10.1103/PhysRevD.96.112009},
journal = {Physical Review D},
issn = {2470-0010},
number = 11,
volume = 96,
place = {United States},
year = {2017},
month = {12}
}

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Figures / Tables:

FIG. 1 FIG. 1: Decay scheme of 83mKr . The width of each column is proportional to the branching fraction of that decay mode, the vertical divisions are proportional to energy partitioning among internal conversion electrons (blue), Auger electrons (yellow), x-rays (green), and gamma-rays (red). Numerical values from Reference.

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