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
| • • • We do not use the following data for averages, fits, limits, etc. • • • |
|
|
1 |
|
LUX |
| $<2 \times 10^{6}$ |
90 |
2 |
|
SENS |
|
|
3 |
|
DMIC |
| $<1 \times 10^{-4}$ |
90 |
4 |
|
XE1T |
| $<9 \times 10^{-3}$ |
90 |
5 |
|
DS50 |
| $<1 \times 10^{4}$ |
90 |
6 |
|
SCDM |
| $<5 \times 10^{3}$ |
90 |
7 |
|
SENS |
|
|
8 |
|
X100 |
|
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: |
|
| PR D101 012003 |
First direct detection constraint on mirror dark matter kinetic mixing using LUX 2013 data |
|
| PRL 122 161801 |
SENSEI: Direct-Detection Constraints on Sub-GeV Dark Matter from a Shallow Underground Run Using a Prototype Skipper-CCD |
|
| PRL 123 181802 |
Constraints on Light Dark Matter Particles Interacting with Electrons from DAMIC at SNOLAB |
|
| PRL 123 251801 |
Light Dark Matter Search with Ionization Signals in XENON1T |
|
| PRL 121 111303 |
Constraints on Sub-GeV Dark-Matter?Electron Scattering from the DarkSide-50 Experiment |
|
| PRL 121 051301 |
First Dark Matter Constraints from a SuperCDMS Single-Charge Sensitive Detector |
|
| PRL 121 061803 |
SENSEI: First Direct-Detection Constraints on sub-GeV Dark Matter from a Surface Run |
|
| PRL 118 101101 |
Search for Electronic Recoil Event Rate Modulation with 4 Years of XENON100 Data |
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