Results from the LUX dark matter experiment

Horn, Markus; Akerib, D. S.; Araújo, H. M.; Bai, X.; Bailey, A. J.; Balajthy, J.; Bernard, E.; Bernstein, A.; Bradley, A.; Byram, D.; Cahn, S. B.; Carmona-Benitez, M. C.; Chan, C.; Chapman, J. J.; Chiller, A. A.; Chiller, C.; Currie, A.; de Viveiros, L.; Dobi, A.; Dobson, J.; Druszkiewicz, E.; Edwards, B.; Faham, C. H.; Fiorucci, S.; Flores, C.; Gaitskell, R. J.; Gehman, V. M.; Ghag, C.; Gibson, K. R.; Gilchriese, M. G.D.; Hall, C.; Hanhardt, M.; Haselschwardt, S.; Hertel, S. A.; Huang, D. Q.; Ihm, M.; Jacobsen, R. G.; Kazkaz, K.; Knoche, R.; Larsen, N. A.; Lee, C.; Lenardo, B.; Lesko, K. T.; Lindote, A.; Lopes, M. I.; Malling, D. C.; Mannino, R.; McKinsey, D. N.; Mei, D. -M.; Mock, J.; Moongweluwan, M.; Morad, J.; Murphy, A. St.J.; Nehrkorn, C.; Nelson, H.; Neves, F.; Ott, R. A.; Pangilinan, M.; Parker, P. D.; Pease, E. K.; Pech, K.; Phelps, P.; Reichhart, L.; Shutt, T.; Silva, C.; Solovov, V. N.; Sorensen, P.; O׳Sullivan, K.; Sumner, T. J.; Szydagis, M.; Taylor, D.; Tennyson, B.; Tiedt, D. R.; Tripathi, M.; Uvarov, S.; Verbus, J. R.; Walsh, N.; Webb, R.; White, J. T.; Witherell, M. S.; Wolfs, F. L.H.; Woods, M.; Zhang, C.

doi:10.1016/j.nima.2014.11.033

Title: Results from the LUX dark matter experiment

Abstract

The LUX (Large Underground Xenon) experiment aims at the direct detection of dark matter particles via their collisions with xenon nuclei. The 370 kg two-phase liquid xenon time projection chamber measures simultaneously the scintillation and ionization from interactions in the target. The ratio of these two signals provides very good discrimination between potential nuclear recoil and electronic recoil signals to search for WIMP-nucleon scattering. The LUX detector operates at the Sanford Underground Research Facility (Lead, South Dakota, USA) since February 2013. Of note, first results were presented in late 2013 setting the world's most stringent limits on WIMP-nucleon scattering cross-sections over a wide range of WIMP masses. A 300 day run beginning in 2014 will further improve the sensitivity and new calibration techniques will reduce systematics for the WIMP signal search.

Authors:: Horn, Markus; Akerib, D. S.; Araújo, H. M.; Bai, X.; Bailey, A. J.; Balajthy, J.; Bernard, E.; Bernstein, A.; Bradley, A.; Byram, D.; Cahn, S. B.; Carmona-Benitez, M. C.; Chan, C.; Chapman, J. J.; Chiller, A. A.; Chiller, C.; Currie, A.; de Viveiros, L.; Dobi, A.; Dobson, J. more »« less

Publication Date:: Tue Nov 18 00:00:00 EST 2014

Research Org.:: Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)

Sponsoring Org.:: USDOE National Nuclear Security Administration (NNSA)

Contributing Org.:: LUX Collaboration

OSTI Identifier:: 1872290

Alternate Identifier(s):: OSTI ID: 1246238

Report Number(s):: LLNL-JRNL-833907
Journal ID: ISSN 0168-9002; 1052226; TRN: US2306861

Grant/Contract Number:: AC52-07NA27344; FG02-08ER41549; FG02-91ER40688; FG02-95ER40917; FG02-91ER40674; NA0000979; FG02-11ER41738; SC0006605; AC02-05CH11231; FG01-91ER40618; FG02- 08ER41549

Resource Type:: Accepted Manuscript

Journal Name:: Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment

Additional Journal Information:: Journal Volume: 784; Journal ID: ISSN 0168-9002

Publisher:: Elsevier

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; dark matter; WIMP; liquid xenon; time projection chamber

Citation Formats


                    Horn, Markus, Akerib, D. S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Bernard, E., Bernstein, A., Bradley, A., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., de Viveiros, L., Dobi, A., Dobson, J., Druszkiewicz, E., Edwards, B., Faham, C. H., Fiorucci, S., Flores, C., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G.D., Hall, C., Hanhardt, M., Haselschwardt, S., Hertel, S. A., Huang, D. Q., Ihm, M., Jacobsen, R. G., Kazkaz, K., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Mannino, R., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J., Murphy, A. St.J., Nehrkorn, C., Nelson, H., Neves, F., Ott, R. A., Pangilinan, M., Parker, P. D., Pease, E. K., Pech, K., Phelps, P., Reichhart, L., Shutt, T., Silva, C., Solovov, V. N., Sorensen, P., O׳Sullivan, K., Sumner, T. J., Szydagis, M., Taylor, D., Tennyson, B., Tiedt, D. R., Tripathi, M., Uvarov, S., Verbus, J. R., Walsh, N., Webb, R., White, J. T., Witherell, M. S., Wolfs, F. L.H., Woods, M., and Zhang, C. Results from the LUX dark matter experiment.  United States: N. p., 2014. 
Web.  doi:10.1016/j.nima.2014.11.033.

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                    Horn, Markus, Akerib, D. S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Bernard, E., Bernstein, A., Bradley, A., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., de Viveiros, L., Dobi, A., Dobson, J., Druszkiewicz, E., Edwards, B., Faham, C. H., Fiorucci, S., Flores, C., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G.D., Hall, C., Hanhardt, M., Haselschwardt, S., Hertel, S. A., Huang, D. Q., Ihm, M., Jacobsen, R. G., Kazkaz, K., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Mannino, R., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J., Murphy, A. St.J., Nehrkorn, C., Nelson, H., Neves, F., Ott, R. A., Pangilinan, M., Parker, P. D., Pease, E. K., Pech, K., Phelps, P., Reichhart, L., Shutt, T., Silva, C., Solovov, V. N., Sorensen, P., O׳Sullivan, K., Sumner, T. J., Szydagis, M., Taylor, D., Tennyson, B., Tiedt, D. R., Tripathi, M., Uvarov, S., Verbus, J. R., Walsh, N., Webb, R., White, J. T., Witherell, M. S., Wolfs, F. L.H., Woods, M., & Zhang, C. Results from the LUX dark matter experiment.  United States.  https://doi.org/10.1016/j.nima.2014.11.033

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                    Horn, Markus, Akerib, D. S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Bernard, E., Bernstein, A., Bradley, A., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., de Viveiros, L., Dobi, A., Dobson, J., Druszkiewicz, E., Edwards, B., Faham, C. H., Fiorucci, S., Flores, C., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G.D., Hall, C., Hanhardt, M., Haselschwardt, S., Hertel, S. A., Huang, D. Q., Ihm, M., Jacobsen, R. G., Kazkaz, K., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Mannino, R., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J., Murphy, A. St.J., Nehrkorn, C., Nelson, H., Neves, F., Ott, R. A., Pangilinan, M., Parker, P. D., Pease, E. K., Pech, K., Phelps, P., Reichhart, L., Shutt, T., Silva, C., Solovov, V. N., Sorensen, P., O׳Sullivan, K., Sumner, T. J., Szydagis, M., Taylor, D., Tennyson, B., Tiedt, D. R., Tripathi, M., Uvarov, S., Verbus, J. R., Walsh, N., Webb, R., White, J. T., Witherell, M. S., Wolfs, F. L.H., Woods, M., and Zhang, C. Tue .  
"Results from the LUX dark matter experiment".  United States.  https://doi.org/10.1016/j.nima.2014.11.033.  https://www.osti.gov/servlets/purl/1872290.

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@article{osti_1872290,

  title        = {Results from the LUX dark matter experiment},

  author       = {Horn, Markus and Akerib, D. S. and Araújo, H. M. and Bai, X. and Bailey, A. J. and Balajthy, J. and Bernard, E. and Bernstein, A. and Bradley, A. and Byram, D. and Cahn, S. B. and Carmona-Benitez, M. C. and Chan, C. and Chapman, J. J. and Chiller, A. A. and Chiller, C. and Currie, A. and de Viveiros, L. and Dobi, A. and Dobson, J. and Druszkiewicz, E. and Edwards, B. and Faham, C. H. and Fiorucci, S. and Flores, C. and Gaitskell, R. J. and Gehman, V. M. and Ghag, C. and Gibson, K. R. and Gilchriese, M. G.D. and Hall, C. and Hanhardt, M. and Haselschwardt, S. and Hertel, S. A. and Huang, D. Q. and Ihm, M. and Jacobsen, R. G. and Kazkaz, K. and Knoche, R. and Larsen, N. A. and Lee, C. and Lenardo, B. and Lesko, K. T. and Lindote, A. and Lopes, M. I. and Malling, D. C. and Mannino, R. and McKinsey, D. N. and Mei, D. -M. and Mock, J. and Moongweluwan, M. and Morad, J. and Murphy, A. St.J. and Nehrkorn, C. and Nelson, H. and Neves, F. and Ott, R. A. and Pangilinan, M. and Parker, P. D. and Pease, E. K. and Pech, K. and Phelps, P. and Reichhart, L. and Shutt, T. and Silva, C. and Solovov, V. N. and Sorensen, P. and O׳Sullivan, K. and Sumner, T. J. and Szydagis, M. and Taylor, D. and Tennyson, B. and Tiedt, D. R. and Tripathi, M. and Uvarov, S. and Verbus, J. R. and Walsh, N. and Webb, R. and White, J. T. and Witherell, M. S. and Wolfs, F. L.H. and Woods, M. and Zhang, C.},

  abstractNote = {The LUX (Large Underground Xenon) experiment aims at the direct detection of dark matter particles via their collisions with xenon nuclei. The 370 kg two-phase liquid xenon time projection chamber measures simultaneously the scintillation and ionization from interactions in the target. The ratio of these two signals provides very good discrimination between potential nuclear recoil and electronic recoil signals to search for WIMP-nucleon scattering. The LUX detector operates at the Sanford Underground Research Facility (Lead, South Dakota, USA) since February 2013. Of note, first results were presented in late 2013 setting the world's most stringent limits on WIMP-nucleon scattering cross-sections over a wide range of WIMP masses. A 300 day run beginning in 2014 will further improve the sensitivity and new calibration techniques will reduce systematics for the WIMP signal search.},

  doi          = {10.1016/j.nima.2014.11.033},

  journal      = {Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment},

  number       = ,

  volume       = 784,

  place        = {United States},

  year         = {Tue Nov 18 00:00:00 EST 2014},

  month        = {Tue Nov 18 00:00:00 EST 2014}

}

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Works referencing / citing this record:

Twin Higgs WIMP Dark Matter
text, January 2015

García, Isabel García; Lasenby, Robert; March-Russell, John
arXiv
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Testing gravity with cold atom interferometry: results and prospects
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Tino, Guglielmo M.
Quantum Science and Technology, Vol. 6, Issue 2
DOI: 10.1088/2058-9565/abd83e

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Title: Results from the LUX dark matter experiment

Abstract

Citation Formats

First Results from the LUX Dark Matter Experiment at the Sanford Underground Research Facility journal, March 2014

WIMP-nucleon cross-section results from the second science run of ZEPLIN-III journal, March 2012

Dark Matter Search Results from the CDMS II Experiment journal, March 2010

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First Dark Matter Results from the XENON100 Experiment journal, September 2010

CoGeNT: A search for low-mass dark matter using p -type point contact germanium detectors journal, July 2013

Review of Particle Physics journal, July 2012

First results from DAMA/LIBRA and the combined results with DAMA/NaI journal, August 2008

A simple high-sensitivity technique for purity analysis of xenon gas journal, September 2010

Technical results from the surface run of the LUX dark matter experiment journal, May 2013

An ultra-low background PMT for liquid xenon detectors journal, March 2013

Liquid xenon detectors for particle physics and astrophysics journal, July 2010

Dark Matter Results from 225 Live Days of XENON100 Data journal, November 2012

The Large Underground Xenon (LUX) experiment journal, March 2013

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Silicon Detector Dark Matter Results from the Final Exposure of CDMS II journal, December 2013

Twin Higgs WIMP Dark Matter text, January 2015

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First Results from the LUX Dark Matter Experiment at the Sanford Underground Research Facility
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Dark Matter Search Results from the CDMS II Experiment
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Final results of the EDELWEISS-II WIMP search using a 4-kg array of cryogenic germanium detectors with interleaved electrodes
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First Dark Matter Results from the XENON100 Experiment
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