| • • • We do not use the following data for averages, fits, limits, etc. • • • |
| $<1 \times 10^{10}$ |
95 |
1 |
|
CRES |
| $<230$ |
90 |
2 |
|
XE1T |
| $<0.01$ |
90 |
3 |
|
XE1T |
| $<4 \times 10^{4}$ |
90 |
4 |
|
EDEL |
| $<0.08$ |
90 |
5 |
|
PNDX |
| $<3$ |
90 |
6 |
|
SCDM |
| $<3$ |
90 |
7 |
|
CDEX |
| $<10$ |
90 |
8 |
|
CDEX |
| $<0.1$ |
90 |
9 |
|
LUX |
| $<0.1$ |
90 |
10 |
|
PNDX |
| $<20$ |
90 |
11 |
|
CDEX |
| $<150$ |
90 |
12 |
|
CDM2 |
|
1
ABDELHAMEED 2019 search for GeV-scale WIMP SD scatter on ${}^{7}\mathrm {Li}$ crystal; set limit ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) for m(${{\mathit \chi}}$) $\sim{}$ $0.8 - 20$ GeV; quoted limit for m(${{\mathit \chi}}$) = 1 GeV.
|
|
2
APRILE 2019C search for light DM on ${}^{}\mathrm {Xe}$ via Migdal/bremsstrahlung effect; no signal, require ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) $<$230 pb for m(${{\mathit \chi}}$) = 1 GeV.
|
|
3
APRILE 2019D search for light DM scatter on ${}^{}\mathrm {Xe}$ via ionization; no signal, limits placed in ${{\mathit \sigma}}$ vs. m(DM) $\sim{}$ $3 - 6$ GeV; quoted limit is for m(DM) = 5 GeV.
|
|
4
ARMENGAUD 2019 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $0.5 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
5
XIA 2019A search for WIMP scatter on ${}^{}\mathrm {Xe}$ in PandaX-II; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) 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.
|
|
6
AGNESE 2018 search for GeV scale WIMPs scatter at CDMSlite; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $1.5 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
7
JIANG 2018 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $3 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
8
YANG 2018 search for WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $2 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
9
AKERIB 2017A search for SD WIMP scatter on ${}^{}\mathrm {Xe}$ with 129.5 kg yr exposure; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) 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.
|
|
10
FU 2017 search for SD WIMP scatter on ${}^{}\mathrm {Xe}$; limits set in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 1 \times 10^{3}$ GeV.; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
11
ZHAO 2016 search for GeV-scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
|
|
12
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. Limit given for m(${{\mathit \chi}}$) = 5 GeV.
|
