Cross-Section Limits for Dark Matter Particles (${{\boldsymbol X}^{0}}$) on electron

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
AKERIB
2020
LUX mirror DM with ${}^{}\mathrm {Xe}$
$<2 \times 10^{6}$ 90 2
ABRAMOFF
2019
SENS WIMP-${{\mathit e}}$ scatter on ${}^{}\mathrm {Si}$
3
AGUILAR-AREVA..
2019A
DMIC MeV scale DM scatter on ${{\mathit e}}$ in ${}^{}\mathrm {Si}$
$<1 \times 10^{-4}$ 90 4
APRILE
2019D
XE1T light DM on ${}^{}\mathrm {Xe}$ via ionization
$<9 \times 10^{-3}$ 90 5
AGNES
2018B
DS50 ${}^{}\mathrm {Ar}$
$<1 \times 10^{4}$ 90 6
AGNESE
2018B
SCDM ${{\mathit e}}{{\mathit \chi}}$ scatter
$<5 \times 10^{3}$ 90 7
CRISLER
2018
SENS ${}^{}\mathrm {Si}$ CCD
8
APRILE
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