Projected sensitivity of the SuperCDMS SNOLAB experiment
Abstract
SuperCDMS SNOLAB will be a next-generation experiment aimed at directly detecting low-mass (< 10 GeV/c$^2$) particles that may constitute dark matter by using cryogenic detectors of two types (HV and iZIP) and two target materials (germanium and silicon). The experiment is being designed with an initial sensitivity to nuclear recoil cross sections ~ 1 x 10$$^{-43}$$ cm$^2$ for a dark matter particle mass of 1 GeV/c$^2$, and with capacity to continue exploration to both smaller masses and better sensitivities. The phonon sensitivity of the HV detectors will be sufficient to detect nuclear recoils from sub-GeV dark matter. A detailed calibration of the detector response to low energy recoils will be needed to optimize running conditions of the HV detectors and to interpret their data for dark matter searches. Low-activity shielding, and the depth of SNOLAB, will reduce most backgrounds, but cosmogenically produced $$^{3}$$H and naturally occurring $$^{32}$$Si will be present in the detectors at some level. Even if these backgrounds are x10 higher than expected, the science reach of the HV detectors would be over three orders of magnitude beyond current results for a dark matter mass of 1 GeV/c$^2$. The iZIP detectors are relatively insensitive to variations in detector response and backgrounds, and will provide better sensitivity for dark matter particle masses (> 5 GeV/c$^2$). The mix of detector types (HV and iZIP), and targets (germanium and silicon), planned for the experiment, as well as flexibility in how the detectors are operated, will allow us to maximize the low-mass reach, and understand the backgrounds that the experiment will encounter. Upgrades to the experiment, perhaps with a variety of ultra-low-background cryogenic detectors, will extend dark matter sensitivity down to the "neutrino floor", where coherent scatters of solar neutrinos become a limiting background.
- Authors:
- more »
- Publication Date:
- Research Org.:
- Pacific Northwest National Laboratory (PNNL), Richland, WA (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Univ. of South Dakota, Vermillion, SD (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- Contributing Org.:
- SuperCDMS Collaboration; SuperCDMS
- OSTI Identifier:
- 1389551
- Alternate Identifier(s):
- OSTI ID: 1350517; OSTI ID: 1350792; OSTI ID: 1458490; OSTI ID: 1598297
- Report Number(s):
- arXiv:1610.00006; FERMILAB-PUB-16-467-AE; PNNL-SA-128797
Journal ID: ISSN 2470-0010; PRVDAQ
- Grant/Contract Number:
- AC02-76SF00515; AC02-07CH11359; AC05-76RL01830; AC02-05CH11231; SC0015657
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review D
- Additional Journal Information:
- Journal Volume: 95; Journal Issue: 8; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; dark matter; particle astrophysics; particle dark matter; weakly interacting massive particles
Citation Formats
Agnese, R., Anderson, A. J., Aramaki, T., Arnquist, I., Baker, W., Barker, D., Basu Thakur, R., Bauer, D. A., Borgland, A., Bowles, M. A., Brink, P. L., Bunker, R., Cabrera, B., Caldwell, D. O., Calkins, R., Cartaro, C., Cerdeño, D. G., Chagani, H., Chen, Y., Cooley, J., Cornell, B., Cushman, P., Daal, M., Di Stefano, P. C. F., Doughty, T., Esteban, L., Fallows, S., Figueroa-Feliciano, E., Fritts, M., Gerbier, G., Ghaith, M., Godfrey, G. L., Golwala, S. R., Hall, J., Harris, H. R., Hofer, T., Holmgren, D., Hong, Z., Hoppe, E., Hsu, L., Huber, M. E., Iyer, V., Jardin, D., Jastram, A., Kelsey, M. H., Kennedy, A., Kubik, A., Kurinsky, N. A., Leder, A., Loer, B., Lopez Asamar, E., Lukens, P., Mahapatra, R., Mandic, V., Mast, N., Mirabolfathi, N., Moffatt, R. A., Morales Mendoza, J. D., Orrell, J. L., Oser, S. M., Page, K., Page, W. A., Partridge, R., Pepin, M., Phipps, A., Poudel, S., Pyle, M., Qiu, H., Rau, W., Redl, P., Reisetter, A., Roberts, A., Robinson, A. E., Rogers, H. E., Saab, T., Sadoulet, B., Sander, J., Schneck, K., Schnee, R. W., Serfass, B., Speller, D., Stein, M., Street, J., Tanaka, H. A., Toback, D., Underwood, R., Villano, A. N., von Krosigk, B., Welliver, B., Wilson, J. S., Wright, D. H., Yellin, S., Yen, J. J., Young, B. A., Zhang, X., and Zhao, X. Projected sensitivity of the SuperCDMS SNOLAB experiment. United States: N. p., 2017.
Web. doi:10.1103/PhysRevD.95.082002.
Agnese, R., Anderson, A. J., Aramaki, T., Arnquist, I., Baker, W., Barker, D., Basu Thakur, R., Bauer, D. A., Borgland, A., Bowles, M. A., Brink, P. L., Bunker, R., Cabrera, B., Caldwell, D. O., Calkins, R., Cartaro, C., Cerdeño, D. G., Chagani, H., Chen, Y., Cooley, J., Cornell, B., Cushman, P., Daal, M., Di Stefano, P. C. F., Doughty, T., Esteban, L., Fallows, S., Figueroa-Feliciano, E., Fritts, M., Gerbier, G., Ghaith, M., Godfrey, G. L., Golwala, S. R., Hall, J., Harris, H. R., Hofer, T., Holmgren, D., Hong, Z., Hoppe, E., Hsu, L., Huber, M. E., Iyer, V., Jardin, D., Jastram, A., Kelsey, M. H., Kennedy, A., Kubik, A., Kurinsky, N. A., Leder, A., Loer, B., Lopez Asamar, E., Lukens, P., Mahapatra, R., Mandic, V., Mast, N., Mirabolfathi, N., Moffatt, R. A., Morales Mendoza, J. D., Orrell, J. L., Oser, S. M., Page, K., Page, W. A., Partridge, R., Pepin, M., Phipps, A., Poudel, S., Pyle, M., Qiu, H., Rau, W., Redl, P., Reisetter, A., Roberts, A., Robinson, A. E., Rogers, H. E., Saab, T., Sadoulet, B., Sander, J., Schneck, K., Schnee, R. W., Serfass, B., Speller, D., Stein, M., Street, J., Tanaka, H. A., Toback, D., Underwood, R., Villano, A. N., von Krosigk, B., Welliver, B., Wilson, J. S., Wright, D. H., Yellin, S., Yen, J. J., Young, B. A., Zhang, X., & Zhao, X. Projected sensitivity of the SuperCDMS SNOLAB experiment. United States. https://doi.org/10.1103/PhysRevD.95.082002
Agnese, R., Anderson, A. J., Aramaki, T., Arnquist, I., Baker, W., Barker, D., Basu Thakur, R., Bauer, D. A., Borgland, A., Bowles, M. A., Brink, P. L., Bunker, R., Cabrera, B., Caldwell, D. O., Calkins, R., Cartaro, C., Cerdeño, D. G., Chagani, H., Chen, Y., Cooley, J., Cornell, B., Cushman, P., Daal, M., Di Stefano, P. C. F., Doughty, T., Esteban, L., Fallows, S., Figueroa-Feliciano, E., Fritts, M., Gerbier, G., Ghaith, M., Godfrey, G. L., Golwala, S. R., Hall, J., Harris, H. R., Hofer, T., Holmgren, D., Hong, Z., Hoppe, E., Hsu, L., Huber, M. E., Iyer, V., Jardin, D., Jastram, A., Kelsey, M. H., Kennedy, A., Kubik, A., Kurinsky, N. A., Leder, A., Loer, B., Lopez Asamar, E., Lukens, P., Mahapatra, R., Mandic, V., Mast, N., Mirabolfathi, N., Moffatt, R. A., Morales Mendoza, J. D., Orrell, J. L., Oser, S. M., Page, K., Page, W. A., Partridge, R., Pepin, M., Phipps, A., Poudel, S., Pyle, M., Qiu, H., Rau, W., Redl, P., Reisetter, A., Roberts, A., Robinson, A. E., Rogers, H. E., Saab, T., Sadoulet, B., Sander, J., Schneck, K., Schnee, R. W., Serfass, B., Speller, D., Stein, M., Street, J., Tanaka, H. A., Toback, D., Underwood, R., Villano, A. N., von Krosigk, B., Welliver, B., Wilson, J. S., Wright, D. H., Yellin, S., Yen, J. J., Young, B. A., Zhang, X., and Zhao, X. Fri .
"Projected sensitivity of the SuperCDMS SNOLAB experiment". United States. https://doi.org/10.1103/PhysRevD.95.082002. https://www.osti.gov/servlets/purl/1389551.
@article{osti_1389551,
title = {Projected sensitivity of the SuperCDMS SNOLAB experiment},
author = {Agnese, R. and Anderson, A. J. and Aramaki, T. and Arnquist, I. and Baker, W. and Barker, D. and Basu Thakur, R. and Bauer, D. A. and Borgland, A. and Bowles, M. A. and Brink, P. L. and Bunker, R. and Cabrera, B. and Caldwell, D. O. and Calkins, R. and Cartaro, C. and Cerdeño, D. G. and Chagani, H. and Chen, Y. and Cooley, J. and Cornell, B. and Cushman, P. and Daal, M. and Di Stefano, P. C. F. and Doughty, T. and Esteban, L. and Fallows, S. and Figueroa-Feliciano, E. and Fritts, M. and Gerbier, G. and Ghaith, M. and Godfrey, G. L. and Golwala, S. R. and Hall, J. and Harris, H. R. and Hofer, T. and Holmgren, D. and Hong, Z. and Hoppe, E. and Hsu, L. and Huber, M. E. and Iyer, V. and Jardin, D. and Jastram, A. and Kelsey, M. H. and Kennedy, A. and Kubik, A. and Kurinsky, N. A. and Leder, A. and Loer, B. and Lopez Asamar, E. and Lukens, P. and Mahapatra, R. and Mandic, V. and Mast, N. and Mirabolfathi, N. and Moffatt, R. A. and Morales Mendoza, J. D. and Orrell, J. L. and Oser, S. M. and Page, K. and Page, W. A. and Partridge, R. and Pepin, M. and Phipps, A. and Poudel, S. and Pyle, M. and Qiu, H. and Rau, W. and Redl, P. and Reisetter, A. and Roberts, A. and Robinson, A. E. and Rogers, H. E. and Saab, T. and Sadoulet, B. and Sander, J. and Schneck, K. and Schnee, R. W. and Serfass, B. and Speller, D. and Stein, M. and Street, J. and Tanaka, H. A. and Toback, D. and Underwood, R. and Villano, A. N. and von Krosigk, B. and Welliver, B. and Wilson, J. S. and Wright, D. H. and Yellin, S. and Yen, J. J. and Young, B. A. and Zhang, X. and Zhao, X.},
abstractNote = {SuperCDMS SNOLAB will be a next-generation experiment aimed at directly detecting low-mass (< 10 GeV/c$^2$) particles that may constitute dark matter by using cryogenic detectors of two types (HV and iZIP) and two target materials (germanium and silicon). The experiment is being designed with an initial sensitivity to nuclear recoil cross sections ~ 1 x 10$^{-43}$ cm$^2$ for a dark matter particle mass of 1 GeV/c$^2$, and with capacity to continue exploration to both smaller masses and better sensitivities. The phonon sensitivity of the HV detectors will be sufficient to detect nuclear recoils from sub-GeV dark matter. A detailed calibration of the detector response to low energy recoils will be needed to optimize running conditions of the HV detectors and to interpret their data for dark matter searches. Low-activity shielding, and the depth of SNOLAB, will reduce most backgrounds, but cosmogenically produced $^{3}$H and naturally occurring $^{32}$Si will be present in the detectors at some level. Even if these backgrounds are x10 higher than expected, the science reach of the HV detectors would be over three orders of magnitude beyond current results for a dark matter mass of 1 GeV/c$^2$. The iZIP detectors are relatively insensitive to variations in detector response and backgrounds, and will provide better sensitivity for dark matter particle masses (> 5 GeV/c$^2$). The mix of detector types (HV and iZIP), and targets (germanium and silicon), planned for the experiment, as well as flexibility in how the detectors are operated, will allow us to maximize the low-mass reach, and understand the backgrounds that the experiment will encounter. Upgrades to the experiment, perhaps with a variety of ultra-low-background cryogenic detectors, will extend dark matter sensitivity down to the "neutrino floor", where coherent scatters of solar neutrinos become a limiting background.},
doi = {10.1103/PhysRevD.95.082002},
journal = {Physical Review D},
number = 8,
volume = 95,
place = {United States},
year = {Fri Apr 07 00:00:00 EDT 2017},
month = {Fri Apr 07 00:00:00 EDT 2017}
}
Web of Science
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Physics beyond colliders at CERN: beyond the Standard Model working group report
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- Deutsches Elektronen-Synchrotron, DESY, Hamburg
Cosmogenic activation of materials
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Physics Beyond Colliders at CERN: Beyond the Standard Model Working Group Report
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- Beacham, J.; Burrage, C.; Curtin, D.
- Deutsches Elektronen-Synchrotron, DESY, Hamburg
Exploring light mediators with low-threshold direct detection experiments
text, January 2017
- Kahlhoefer, Felix; Kulkarni, Suchita; Wild, Sebastian
- Deutsches Elektronen-Synchrotron, DESY, Hamburg
Cosmogenic activation of materials
conference, January 2013
- Cebrián, S.
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Examining the origin of dark matter mass at colliders
text, January 2016
- Kim, Minho; Lee, Hye-Sung; Park, Myeonghun
- arXiv
Magnetic Bubble Chambers and Sub-GeV Dark Matter Direct Detection
text, January 2017
- Bunting, Philip C.; Gratta, Giorgio; Melia, Tom
- arXiv
New constraints and discovery potential of sub-GeV dark matter with xenon detectors
text, January 2017
- McCabe, Christopher
- arXiv
Directly Detecting MeV-scale Dark Matter via Solar Reflection
text, January 2017
- An, Haipeng; Pospelov, Maxim; Pradler, Josef
- arXiv
Thermal Dark Matter Through the Dirac Neutrino Portal
text, January 2017
- Batell, Brian; Han, Tao; McKeen, David
- arXiv
Light Dark Matter: Models and Constraints
text, January 2017
- Knapen, Simon; Lin, Tongyan; Zurek, Kathryn M.
- arXiv
Casting a Wide Signal Net with Future Direct Dark Matter Detection Experiments
text, January 2018
- Gelmini, Graciela B.; Takhistov, Volodymyr; Witte, Samuel J.
- arXiv
First Dark Matter Constraints from a SuperCDMS Single-Charge Sensitive Detector
text, January 2018
- Collaboration, SuperCDMS; Agnese, R.; Aralis, T.
- arXiv
Energy Loss Due to Defect Formation from $^{206}$Pb Recoils in SuperCDMS Germanium Detectors
text, January 2018
- Agnese, Robert; Aralis, Taylor; Aramaki, Tsuguo
- arXiv
Directional Detection of Light Dark Matter with Polar Materials
text, January 2018
- Griffin, Sinead; Knapen, Simon; Lin, Tongyan
- arXiv
How high is the neutrino floor?
text, January 2018
- Boehm, C.; Cerdeno, D. G.; Machado, P. A. N.
- arXiv
Diamond Detectors for Direct Detection of Sub-GeV Dark Matter
text, January 2019
- Kurinsky, Noah; Yu, To Chin; Hochberg, Yonit
- arXiv
$Z'$ Mediated WIMPs: Dead, Dying, or Soon to be Detected?
text, January 2019
- Blanco, Carlos; Escudero, Miguel; Hooper, Dan
- arXiv