# For ${\boldsymbol m}_{{{\boldsymbol X}^{0}}}$ in GeV range INSPIRE search

We provide here limits fo ${\mathit m}_{{{\mathit X}^{0}}}$ $<$ 5 GeV
VALUE (pb) CL% DOCUMENT ID TECN  COMMENT
• • • We do not use the following data for averages, fits, limits, etc. • • •
1
 2020
LUX mirror DM with ${}^{}\mathrm {Xe}$
$<2 \times 10^{6}$ 90 2
 2019
SENS WIMP-${{\mathit e}}$ scatter on ${}^{}\mathrm {Si}$
3
 2019 A
DMIC MeV scale DM scatter on ${{\mathit e}}$ in ${}^{}\mathrm {Si}$
$<1 \times 10^{-4}$ 90 4
 2019 D
XE1T light DM on ${}^{}\mathrm {Xe}$ via ionization
$<9 \times 10^{-3}$ 90 5
 2018 B
DS50 ${}^{}\mathrm {Ar}$
$<1 \times 10^{4}$ 90 6
 2018 B
SCDM ${{\mathit e}}{{\mathit \chi}}$ scatter
$<5 \times 10^{3}$ 90 7
 2018
SENS ${}^{}\mathrm {Si}$ CCD
8
 2017
X100 ${}^{}\mathrm {Xe}$, annual modulation
1  AKERIB 2020 search for mirror DM with LUX 95 d ${\times }$ 118 kg data for mirror ${{\mathit e}}$ scatter from ${}^{}\mathrm {Xe}$; no signal, limits placed in kinetic mixing parameter vs. mirror ${{\mathit e}}$ temperature T $\sim{}$ $0.1 - 0.9$ keV plane.
2  ABRAMOFF 2019 search for MeV-scale WIMP scatter from ${}^{}\mathrm {Si}$ skipper-CCD; limits placed on ${{\mathit \sigma}}$( ${{\mathit \chi}}{{\mathit e}}$ ) for m(${{\mathit \chi}}$) $\sim{}$ $0.5 - 100$ MeV depending on DM form factors. Limit given for m(DM) = 1 MeV.
3  AGUILAR-AREVALO 2019A search for MeV scale DM scatter from ${{\mathit e}}$ in ${}^{}\mathrm {Si}$ CCDs at SNOLAB; no signal, limits placed in ${\mathit \sigma (}$e${)}$ vs. m(DM) plane for m(DM) $\sim{}$ $0.6 - 100$ MeV.
4  APRILE 2019D search for light DM scatter on ${}^{}\mathrm {Xe}$ via ionization; no signal, limits placed in ${{\mathit \sigma}}$ on nucleus vs. m(DM) plane for m(DM) $\sim{}$ $0.02 - 10$ GeV; quoted limit is for m(DM) = 0.2 GeV.
5  AGNES 2018B search for MeV scale WIMP scatter from ${{\mathit e}}$ in ${}^{}\mathrm {Ar}$; no signal, limits set in ${{\mathit \sigma}_{{e}}}$ vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $20 - 1000$ MeV and two choices of form factor F(DM); quoted limit for m(${{\mathit \chi}}$) = 100 MeV and F = 1.
6  AGNESE 2018B search for ${{\mathit e}}{{\mathit \chi}}$ scatter in SuperCDMS; limits placed in ${{\mathit \sigma}}$( ${{\mathit e}}{{\mathit \chi}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $0.3 - 1 \times 10^{4}$ MeV for two assumed form factors and also in m(dark photon) vs. kinetic mixing plane. Limit given for m(${{\mathit \chi}}$) = 1 GeV and F=1.
7  CRISLER 2018 search for ${{\mathit \chi}}$ ${{\mathit e}}$ $\rightarrow$ ${{\mathit \chi}}{{\mathit e}}$ scatter in ${}^{}\mathrm {Si}$ CCD; place limits on MeV DM in ${{\mathit \sigma}_{{e}}}$ vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $0.5 - 1000$ MeV for different form factors; quoted limit is for F(DM) = 1 and m(${{\mathit \chi}}$) = 10 MeV.
8  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.
References:
 AKERIB 2020
PR D101 012003 First direct detection constraint on mirror dark matter kinetic mixing using LUX 2013 data
 ABRAMOFF 2019
PRL 122 161801 SENSEI: Direct-Detection Constraints on Sub-GeV Dark Matter from a Shallow Underground Run Using a Prototype Skipper-CCD
 AGUILAR-AREVALO 2019A
PRL 123 181802 Constraints on Light Dark Matter Particles Interacting with Electrons from DAMIC at SNOLAB
 APRILE 2019D
PRL 123 251801 Light Dark Matter Search with Ionization Signals in XENON1T
 AGNES 2018B
PRL 121 111303 Constraints on Sub-GeV Dark-Matter?Electron Scattering from the DarkSide-50 Experiment
 AGNESE 2018B
PRL 121 051301 First Dark Matter Constraints from a SuperCDMS Single-Charge Sensitive Detector
 CRISLER 2018
PRL 121 061803 SENSEI: First Direct-Detection Constraints on sub-GeV Dark Matter from a Surface Run
 APRILE 2017
PRL 118 101101 Search for Electronic Recoil Event Rate Modulation with 4 Years of XENON100 Data