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

For ${\mathit m}_{{{\mathit X}^{0}}}$ in GeV range

INSPIRE   PDGID:
S030DE5
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. • •
$<3 \times 10^{-3}$ 90 1
AGNES
2023A
 DS50 LDM scatter on ${{\mathit e}}$
$<0.3$ 90 2
ARNQUIST
2023A
 DAMC LDM search via CCDs
$<2 \times 10^{-5}$ 90 3
LI
2023F
 PNDX light DM limits
4
AGOSTINI
2022A
 GERD search for superWIMPs
$<1000$ 90 5
APRILE
2022
XE1T WIMP-${{\mathit e}}$ scatter
6
BATTAGLIERI
2022
BDX-MINI search for light DM from beam dump
$<2 \times 10^{-9}$ 95 7
BOSE
2022
DM-${{\mathit e}}$ limits from solar ${{\mathit \gamma}}$s
$<100$ 8
GHOSH
2022
boosted DM-${{\mathit e}}/DM-{{\mathit \nu}}$ scatter
9
HOCHBERG
2022
SNSP superconducting nanowire search for light DM
10
ZHANG
2022A
 CDEX light DM search on ${{\mathit e}}$ in ${}^{}\mathrm {Ge}$
$<10$ 90 11
CHENG
2021
PNDX MeV-scale DM on ${{\mathit e}}$
12
AKERIB
2020
LUX mirror DM with ${}^{}\mathrm {Xe}$
$<870$ 90 13
AMARAL
2020
SCDM light DM scatter on ${{\mathit e}}$ in ${}^{}\mathrm {Si}$
14
APRILE
2020
XE1T excess keV electron recoil in ${}^{}\mathrm {Xe}$
$<100$ 90 15
ARNAUD
2020
EDEL MeV DM scatter on ${{\mathit e}}$ in ${}^{}\mathrm {Ge}$
$<0.6$ 90 16
BARAK
2020
SENS MeV scale DM scatter from ${{\mathit e}}$ in ${}^{}\mathrm {Si}$
$<2 \times 10^{6}$ 90 17
ABRAMOFF
2019
SENS WIMP-${{\mathit e}}$ scatter on ${}^{}\mathrm {Si}$
18
AGUILAR-AREVA..
2019A
 DMIC MeV scale DM scatter on ${{\mathit e}}$ in ${}^{}\mathrm {Si}$
$<1 \times 10^{-4}$ 90 19
APRILE
2019D
 XE1T light DM on ${}^{}\mathrm {Xe}$ via ionization
$<9 \times 10^{-3}$ 90 20
AGNES
2018B
 DS50 ${}^{}\mathrm {Ar}$
$<1 \times 10^{4}$ 90 21
AGNESE
2018B
 SCDM ${{\mathit e}}{{\mathit \chi}}$ scatter
$<5 \times 10^{3}$ 90 22
CRISLER
2018
SENS ${}^{}\mathrm {Si}$ CCD
23
APRILE
2017
X100 ${}^{}\mathrm {Xe}$, annual modulation
1  AGNES 2023A search for MeV-scale DM scatter from ${{\mathit e}}$ using ${}^{}\mathrm {Ar}$. No signal observed. ${{\mathit \sigma}}({{\mathit \chi}}{{\mathit e}}$) $<$ $3 \times 10^{-3}$ pb for m(${{\mathit \chi}}$) = 30 MeV.
2  ARNQUIST 2023A search for LDM scatter on ${{\mathit e}}$ using CCDs. No signal observed. Require ${{\mathit \sigma}}({{\mathit \chi}}{{\mathit e}}$) $<$ $0.3$ pb for m(${{\mathit \chi}}$) = 10 MeV and F$_{DM}$ = 1 (Fig. 3b).
3  LI 2023F search for light DM in MeV range via scatter from ${{\mathit e}}$. No signal observed. Limits set. The quoted limit is for m(${{\mathit \chi}}$) = 0.2 GeV with F$_{DM}$ = 1.
4  AGOSTINI 2022 search for superWIMP particles using GERDA detector; no signal observed; limits placed in mass vs coupling plane for m(DM) $0.06 - 1$ MeV.
5  APRILE 2022 place new limits on WIMP-${{\mathit e}}$ scatter for dark photon and various multipole moments vs. WIMP mass for various DM models; quoted limit for m(WIMP) = 1 GeV in light mediator model.
6  BATTAGLIERI 2022 search for light MeV scale DM particles produced in JLAB beam dump; no signal observed; limits set in kinetic mixing vs. m(DM) plane for m(DM) $\sim{}$ $1 - 200$ MeV .
7  BOSE 2022 theoretically derive limits on WIMP-${{\mathit e}}$ scatter from solar gamma rays using data of Fermi-LAT; limit quoted for m(WIMP) = 5 GeV.
8  GHOSH 2022 derive limits on sub-GeV boosted DM scatter from ${{\mathit e}}$ or ${{\mathit \nu}}$ using SuperK/XENON1T data; quoted limit for m(${{\mathit \chi}}$) = 1 MeV.
9  HOCHBERG 2022 search for sub-eV or sub-MeV scale DM scatter/absorption on ${{\mathit e}}$ in superconducting nanowire; no signal observed; limits set in m(DM) vs. cross section plane for sub-MeV-scale DM and in m(DM) vs. kinetic mixing plane for sub-eV-scale DM.
10  ZHANG 2022A search for DM scatter on ${{\mathit e}}$ using CDEX-10; no signal observed; limits placed on ${\mathit \sigma (}{{\mathit \chi}}{{\mathit e}}{)}$ vs. m(DM) plane for m(DM) $\sim{}$ $0.07 - 10$ GeV for various simplified models.
11  CHENG 2021 search for MeV-scale DM scatter from ${{\mathit e}}$ in PANDAX-II. No signal detected. Limits set in ${{\mathit \sigma}}({{\mathit \chi}}{{\mathit e}}$) vs. m(DM) plane for two choices of form factors; ${{\mathit \sigma}}({{\mathit \chi}}{{\mathit e}}$) $<$ 10 pb for m(${{\mathit \chi}}$) = 10 MeV and F$_{DM}$ = 1.
12  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.
13  AMARAL 2020 search SuperCDMS data for low mass DM scatter from ${{\mathit e}}$ in ${}^{}\mathrm {Si}$; no signal; quoted limit ${{\mathit \sigma}_{{{e}}}}$ $<$ $8.7 \times 10^{2}$ pb for m(DM) = 10 MeV with form factor F$_{DM}$ = 1.
14  APRILE 2020 report excess at electron recoil around $2 - 3$ keV in ${}^{}\mathrm {Xe}$; data compared to unforeseen tritium background, and various signal models (bosonic DM, solar axion, and neutrino magnetic moment).
15  ARNAUD 2020 search for MeV DM scattering from ${{\mathit e}}$ in ${}^{}\mathrm {Ge}$; no signal; quoted limit is for m(DM) = 10 MeV with form factor F$_{DM}$ = 1.
16  BARAK 2020 report search for MeV scale DM scatter from ${{\mathit e}}$ in ${}^{}\mathrm {Si}$; limits placed in ${{\mathit \sigma}_{{{e}}}}$ vs. m(DM) plane; quoted limit is for m(DM) = 10 MeV and form factor F$_{DM}$ = 1.
17  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.
18  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.
19  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.
20  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.
21  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.
22  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.
23  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