| • • We do not use the following data for averages, fits, limits, etc. • • |
| $<8 \times 10^{-4}$ |
90 |
1 |
|
DMIC |
| $<8 \times 10^{-4}$ |
90 |
2 |
|
LUX |
| $<0.01$ |
90 |
3 |
|
CRES |
| $<5.4 \times 10^{-6}$ |
90 |
4 |
|
SCDM |
| $<1$ |
90 |
5 |
|
LUX |
| $<1 \times 10^{-6}$ |
90 |
6 |
|
PICO |
| $<1.6 \times 10^{-3}$ |
90 |
7 |
|
XE1T |
| $<1 \times 10^{-7}$ |
90 |
8 |
|
XE1T |
| $<0.1$ |
90 |
9 |
|
EDEL |
| $<1.6 \times 10^{3}$ |
90 |
10 |
|
XMAS |
| $<700$ |
90 |
11 |
|
CDEX |
| $<7 \times 10^{-7}$ |
90 |
12 |
|
DS50 |
| $<1.5 \times 10^{-5}$ |
95 |
13 |
|
SCDM |
| $<2 \times 10^{-8}$ |
90 |
14 |
|
XE1T |
| $<4.5 \times 10^{-3}$ |
90 |
15 |
|
NEWS |
| $<8 \times 10^{-6}$ |
90 |
16 |
|
CDEX |
| $<3 \times 10^{-5}$ |
90 |
17 |
|
CDEX |
| $<1 \times 10^{-6}$ |
90 |
18 |
|
LUX |
| $<100$ |
90 |
19 |
|
CRES |
| $<7 \times 10^{-5}$ |
90 |
20 |
|
CRES |
| $<3 \times 10^{-5}$ |
90 |
21 |
|
X100 |
| $<4.3 \times 10^{-4}$ |
90 |
22 |
|
EDE3 |
| $<7 \times 10^{-5}$ |
90 |
23 |
|
EDE3 |
| $<6 \times 10^{-5}$ |
90 |
24 |
|
CDEX |
| $<1 \times 10^{-4}$ |
90 |
25 |
|
PICO |
| $<8 \times 10^{-5}$ |
90 |
26 |
|
PNDX |
| $<3 \times 10^{-5}$ |
90 |
27 |
|
SCDM |
| $<1 \times 10^{-3}$ |
90 |
28 |
|
LUX |
| $<9 \times 10^{-4}$ |
90 |
29 |
|
TEXO |
| $<3 \times 10^{-4}$ |
90 |
30 |
|
PICA |
| $<2 \times 10^{-4}$ |
90 |
31 |
|
CGNT |
| $<5 \times 10^{-4}$ |
90 |
32 |
|
CDM2 |
| $<8 \times 10^{-5}$ |
90 |
33 |
|
XE10 |
| $<5 \times 10^{-4}$ |
90 |
34 |
|
CDM2 |
|
1 |
AGUILAR-AREVALO 2020C search for WIMP SI scatter on ${}^{}\mathrm {Si}$ using DAMIC at SNOLab; some excess; limits placed in ${{\mathit \sigma}}$ vs m(DM) for m(DM) in $1.2 - 10$ GeV; quoted limit for m(WIMP) = 2 GeV.
|
|
|
2 |
AKERIB 2020A search for GeV-scale WIMPs via WIMP-nucleon scatter with single photon emission; no signal; limits placed in m(WIMP) vs ${{\mathit \sigma}^{SI}}$ plane: for example ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit n}}$ ) $<$ $8 \times 10^{-4}$ pb for m(WIMP) = 2.5 GeV.
|
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|
3 |
ABDELHAMEED 2019A search for GeV scale dark matter SI scatter on ${}^{}\mathrm {CaWO}_{4}$; no signal, limits placed in ${{\mathit \sigma}}$ vs. mass plane for m(DM) $\sim{}$ $0.1 - 10$ GeV. The listed limit is for m(DM) = 1 GeV.
|
|
|
4 |
AGNESE 2019A search for $1.5 - 10$ GeV WIMP scatter on ${}^{}\mathrm {Ge}$ in CDMSlite dataset. Limits set in a likelihood analysis. No signal was observed. Limit reported for m(${{\mathit \chi}}$) = 5 GeV.
|
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|
5 |
AKERIB 2019 search for $0.4 - 5$ GeV DM using bremsstrahlung photons and "Migdal" electrons; $1.4 \times 10^{4}$ kg d exposure of liquid ${}^{}\mathrm {Xe}$; constraint ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ 1 pb for m(${{\mathit \chi}}$) = 5 GeV in light scalar mediator model.
|
|
|
6 |
AMOLE 2019 search for SI WIMP scatter on ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$ in PICO-60 bubble chamber; no signal: set limit for spin independent coupling ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ $1 \times 10^{-6}$ pb for m(${{\mathit \chi}}$) = 5 GeV.
|
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|
7 |
APRILE 2019C search for light DM scatter on ${}^{}\mathrm {Xe}$ via atomic excitation, ionization (Migdal effect) or bremsstrahlung; no signal, limits placed in ${{\mathit \sigma}}$ vs. m(DM) plane for m(DM) $\sim{}$ $0.085 - 2$ GeV. The listed limit is for m(DM) = 1 GeV.
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|
8 |
APRILE 2019D search for light DM scatter on ${}^{}\mathrm {Xe}$ via ionization to probe SI, SD, and ${{\mathit \chi}}{{\mathit e}}$ cross sections; with 22 t d exposure, limits placed in various ${{\mathit \sigma}}$ vs. m(DM) planes. Quoted limit is for m(DM) = 5 GeV.
|
|
|
9 |
ARMENGAUD 2019 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $0.045 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
|
10 |
KOBAYASHI 2019 search for sub-GeV WIMP annual modulation in ${}^{}\mathrm {Xe}$ via brems; no signal; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $0.3 - 1$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 0.5 GeV.
|
|
|
11 |
LIU 2019B seach for sub-GeV DM using Migdal effect on ${}^{}\mathrm {Ge}$ at CDEX-IB; no signal, require ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ $700$ pb for m(${{\mathit \chi}}$) = 0.1 GeV.
|
|
|
12 |
AGNES 2018 search for $1.8 - 20$ GeV WIMP SI scatter on ${}^{}\mathrm {Ar}$; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
|
13 |
AGNESE 2018 search for GeV scale WIMPs using CDMSlite; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $1.5 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
|
14 |
APRILE 2018 search for WIMP scatter on 1 t yr ${}^{}\mathrm {Xe}$; no signal, limits set in ${{\mathit \sigma}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $6 - 1000$ GeV; quoted limit is for m = 6 GeV.
|
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|
15 |
ARNAUD 2018 search for low mass WIMP scatter on ${}^{}\mathrm {Ne}$ via SPC at NEWS-G; limits set in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $0.5 - 20$ GeV; quoted limit is for m = 5 GeV.
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16 |
JIANG 2018 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $3 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
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|
17 |
YANG 2018 search for WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $2 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
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|
18 |
AKERIB 2017 search for WIMP scatter on ${}^{}\mathrm {Xe}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $5 - 1 \times 10^{5}$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
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|
19 |
ANGLOHER 2017A search for GeV scale WIMP scatter on ${}^{}\mathrm {Al}_{2}{}^{}\mathrm {O}_{3}$ crystal; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $0.15 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
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|
20 |
ANGLOHER 2016 search for GeV scale WIMP scatter on ${}^{}\mathrm {CaWO}_{4}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $0.5 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
|
21 |
APRILE 2016 search for low mass WIMPs via ionization at XENON100; limits placed in ${{\mathit \sigma}}{}^{SI}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs m(${{\mathit \chi}}$) plane for m $\sim{}$ $3.5 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
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|
|
22 |
ARMENGAUD 2016 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
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|
|
23 |
HEHN 2016 search for low mass WIMPs via SI scatter on ${}^{}\mathrm {Ge}$ target using profile likelihood analysis; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
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|
24 |
ZHAO 2016 search for GeV-scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
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|
25 |
AMOLE 2015 search for WIMP scatter on ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$ in PICO-2L; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 25$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
|
26 |
XIAO 2015 search for WIMP scatter on ${}^{}\mathrm {Xe}$ with PandaX-I; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $5 - 100$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
|
27 |
AGNESE 2014 search for GeV scale WIMPs SI scatter at SuperCDMS; no signal, limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $3.5 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
|
28 |
AKERIB 2014 search for WIMP scatter on ${}^{}\mathrm {Xe}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $5 - 5000$ GeV. Limit given for m(${{\mathit \chi}}$) = 5 GeV.
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|
|
29 |
LI 2013B search for WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 100$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
|
30 |
ARCHAMBAULT 2012 search for low mass WIMP scatter on ${}^{}\mathrm {C}_{4}{}^{}\mathrm {F}_{10}$; limits set in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $4 - 12$ GeV; quoted limit is for m = 5 GeV.
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|
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31 |
AALSETH 2011 search for GeV-scale SI WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed on ${{\mathit \sigma}}{}^{SI}$( ${{\mathit \chi}}{{\mathit N}}$ ) for m(${{\mathit \chi}}$) $\sim{}$ $3.5 - 100$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
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|
32 |
AHMED 2011B search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$ in CDMS II; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $4 - 12$ GeV.
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33 |
ANGLE 2011 search for GeV scale WIMPs in Xenon-10; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
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34 |
AKERIB 2010 search for WIMP scatter on ${}^{}\mathrm {Ge}/{}^{}\mathrm {Si}$ in CDMS II; limits place in ${{\mathit \sigma}_{{SI}}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $3 - 100$ GeV. Limit given for m(DM) = 5 GeV.
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