| • • • We do not use the following data for averages, fits, limits, etc. • • • |
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1 |
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SENS |
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2 |
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C100 |
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3 |
|
ANAI |
| $<6.4 \times 10^{-10}$ |
90 |
4 |
|
XE1T |
|
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5 |
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|
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6 |
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|
7 |
|
THEO |
|
|
8 |
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C100 |
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|
9 |
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|
10 |
|
ICCB |
|
|
11 |
|
XMAS |
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|
12 |
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DS50 |
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13 |
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SCDM |
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|
14 |
|
LUX |
|
|
15 |
|
EDE3 |
|
|
16 |
|
SKAM |
| $<1 \times 10^{-12}$ |
90 |
17 |
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DMIC |
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|
18 |
|
X100 |
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|
19 |
|
X100 |
|
|
20 |
|
X100 |
|
|
21 |
|
X100 |
| $<4 \times 10^{-3}$ |
90 |
22 |
|
CRES |
|
|
23 |
|
X100 |
|
|
24 |
|
X100 |
|
1
ABRAMOFF 2019 search for MeV scale DM via DM$−{{\mathit e}}$ scattering and dark photon DM via absorption in ${}^{}\mathrm {Si}$; limits set in coupling vs. m(${{\mathit \chi}}$) plane and on dark photon in m(${{\mathit A}}$) vs. kinetic mixing parameter plane.
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2
ADHIKARI 2019 search for annual modulation signal from WIMP scatter on ${}^{}\mathrm {Na}{}^{}\mathrm {I}$ with 1.7 yr exposure; result consistent with both DAMA/LIBRA and null hypothesis.
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3
AMARE 2019 is ANAIS-112 search for WIMP scatter annual modulation on ${}^{}\mathrm {NaI}$; 157.55 kg yr exposure; result compatible with null hypothesis; confirm goal of reaching sensitivity at 3${{\mathit \sigma}}$ to DAMA/LIBRA result in 5 years.
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4
APRILE 2019 search for WIMP-pion scattering in ${}^{}\mathrm {Xe}$; no signal: require ${{\mathit \sigma}}$( ${{\mathit \chi}}{{\mathit \pi}}$ ) $<$ $6.4 \times 10^{-10}$ pb for m(${{\mathit \chi}}$) = 30 GeV.
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5
BRINGMANN 2019 derive theoretically limits on GeV and sub-GeV mass dark matter, in its high energy component generated by interaction with cosmic rays; place limits on ${{\mathit \sigma}^{SI}}$ and ${{\mathit \sigma}^{SD}}$ $<$ $10^{5}$ pb.
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6
BRUNE 2019 examine possibility of Majoron dark matter; limits placed on Majoron mass vs. coupling from SN1987a and ${{\mathit \nu}}$-less double beta decay.
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7
CHOI 2019 from multimessenger observation finds limit on ${{\mathit \sigma}}$( ${{\mathit \nu}}{{\mathit \chi}}$ )/m(DM) $<$ $5.1 \times 10^{-23}$ cm${}^{2}$/GeV based on 290 TeV IceCube neutrino event.
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8
HA 2019 search for inelastic boosted MeV scale dark photon using COSINE-100 data; limits placed in m vs. epsilon plane for various mediators.
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9
KLOPF 2019 search for DM via ${{\mathit n}}$ $\rightarrow$ ${{\mathit \chi}}{{\mathit e}^{+}}{{\mathit e}^{-}}$ ; no signal: limits placed in branching fraction vs. m( ${{\mathit e}^{+}}{{\mathit e}^{-}}$ ) plane.
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10
AARTSEN 2018D search for long-lived DM particles decaying ${{\mathit \chi}}$ $\rightarrow$ ${{\mathit \nu}}{{\mathit X}}$ ; no excess seen; for DM masses above 10 TeV, excluding lifetimes shorter than $10^{28}$ s.
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11
ABE 2018F search for keV mass ALPs and hidden photons (HP) scatter on electrons; limits set on mass vs. coupling.
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12
AGNES 2018B search for MeV-scale DM scatter on electrons in ${}^{}\mathrm {Ar}$; no signal; require ${{\mathit \sigma}}$( ${{\mathit \chi}}{{\mathit e}}$ ) $<$ $9 \times 10^{-3}$ pb for DM form factor F(DM) = 1 and $<$ 300 pb for F(DM) proportional to 1/q${}^{2}$ for m(${{\mathit \chi}}$) = 100 MeV.
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13
AGNESE 2018B search for MeV scale DM via DM-${{\mathit e}}$ scattering and dark photon DM via absorption in ${}^{}\mathrm {Si}$; limits set on MeV DM in coupling vs. m(${{\mathit \chi}}$) plane and on dark photon in m(${{\mathit A}^{\,'}}$) vs. kinetic mixing plane.
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14
AKERIB 2018A search for annual and diurnal modulation of DM scattering rate on electrons for recoil energy between 2 and 6 keVee; no signal found.
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15
ARMENGAUD 2018 search for ALP from the Sun and galactic bosonic DM, interacting in ${}^{}\mathrm {Ge}$; no signal; limits set for $0.8 - 500$ keV DM particles.
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16
KACHULIS 2018 search for an excess of elastically scattered electrons above the atmospheric neutrino background in Super-K; limits placed for simple annihilation or decay in the Sun or galactic center producing "boosted" dark matter.
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17
AGUILAR-AREVALO 2017 search for hidden photon DM scatter on ${}^{}\mathrm {Si}$ target CCD; limit kinetic mixing ${{\mathit \kappa}}$ $<$ $1 \times 10^{-12}$ for m = 10 eV.
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18
APRILE 2017 search for WIMP-${{\mathit e}}$ annual modulation signal for recoil energy in the $2.0 - 5.8$ keV interval using 4 years data with ${}^{}\mathrm {Xe}$. No significant effect seen.
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19
APRILE 2017D set limits on 14 WIMP-nucleon different interaction operators. No deviations found using 225 live days in the $6.6 - 240$ keV recoil energy range.
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20
APRILE 2017H search for keV bosonic DM via ${{\mathit e}}$ ${{\mathit \chi}}$ $\rightarrow$ ${{\mathit e}}$ , looking for electronic recoils with 224.6 live days of data and 34 kg of LXe. Limits set on ${{\mathit \chi}}{{\mathit e}}{{\mathit e}}$ coupling for m(${{\mathit \chi}}$) = $8 - 125$ keV.
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21
APRILE 2017K search for magnetic inelastic DM via ${{\mathit \chi}}$ ${{\mathit N}}$ $\rightarrow$ ${{\mathit \chi}^{*}}$ $\rightarrow$ ${{\mathit \chi}}{{\mathit \gamma}}$ . Limits set in DM magnetic moment vs. mass splitting plane for two DM masses corresponding to the DAMA/LIBRA best fit values.
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22
ANGLOHER 2016A require q${}^{2}$ dependent scattering $<$ $8 \times 10^{-3}$ pb for asymmetric DM $\mathit m$(WIMP) = 3 GeV on ${}^{}\mathrm {Ca}{}^{}\mathrm {W}{}^{}\mathrm {O}_{4}$ target. It uses a local dark matter density of 0.38 GeV/cm${}^{3}$.
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23
APRILE 2015 search for periodic variation of electronic recoil event rate in the data between Feb. 2011 and Mar. 2012. No significant modulation is found for periods up to 500 days.
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24
APRILE 2015A search for ${{\mathit X}^{0}}$ scattering off electrons. See their Fig. 4 for limits on cross section through axial-vector coupling for ${\mathit m}_{{{\mathit X}^{0}}}$ between 0.6 GeV and 1 TeV. For ${\mathit m}_{{{\mathit X}^{0}}}$ = 2 GeV, $\sigma <$ 60 pb (90$\%$CL) is obtained.
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