Spin-Dependent Cross Section Limits for Dark Matter Particle (${{\boldsymbol X}^{0}}$) on Neutron

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. • • •
$<1 \times 10^{10}$ 95 1
ABDELHAMEED
2019
CRES SD low mass DM on ${}^{}\mathrm {Li}$
$<230$ 90 2
APRILE
2019C
XE1T light DM on ${}^{}\mathrm {Xe}$ via Migdal/brem effect
$<0.01$ 90 3
APRILE
2019D
XE1T light DM on ${}^{}\mathrm {Xe}$ via ionization
$<4 \times 10^{4}$ 90 4
ARMENGAUD
2019
EDEL GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<0.08$ 90 5
XIA
2019A
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<3$ 90 6
AGNESE
2018
SCDM GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<3$ 90 7
JIANG
2018
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<10$ 90 8
YANG
2018
CDEX WIMPs on ${}^{}\mathrm {Ge}$
$<0.1$ 90 9
AKERIB
2017A
LUX ${}^{}\mathrm {Xe}$
$<0.1$ 90 10
FU
2017
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<20$ 90 11
ZHAO
2016
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<150$ 90 12
AHMED
2011B
CDM2 GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
1  ABDELHAMEED 2019 search for GeV-scale WIMP SD scatter on ${}^{7}\mathrm {Li}$ crystal; set limit ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) for m(${{\mathit \chi}}$) $\sim{}$ $0.8 - 20$ GeV; quoted limit for m(${{\mathit \chi}}$) = 1 GeV.
2  APRILE 2019C search for light DM on ${}^{}\mathrm {Xe}$ via Migdal/bremsstrahlung effect; no signal, require ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) $<$230 pb for m(${{\mathit \chi}}$) = 1 GeV.
3  APRILE 2019D search for light DM scatter on ${}^{}\mathrm {Xe}$ via ionization; no signal, limits placed in ${{\mathit \sigma}}$ vs. m(DM) $\sim{}$ $3 - 6$ GeV; quoted limit is for m(DM) = 5 GeV.
4  ARMENGAUD 2019 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $0.5 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
5  XIA 2019A search for WIMP scatter on ${}^{}\mathrm {Xe}$ in PandaX-II; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $5 - 1 \times 10^{5}$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
6  AGNESE 2018 search for GeV scale WIMPs scatter at CDMSlite; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $1.5 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
7  JIANG 2018 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $3 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
8  YANG 2018 search for WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $2 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
9  AKERIB 2017A search for SD WIMP scatter on ${}^{}\mathrm {Xe}$ with 129.5 kg yr exposure; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $5 - 1 \times 10^{5}$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
10  FU 2017 search for SD WIMP scatter on ${}^{}\mathrm {Xe}$; limits set in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 1 \times 10^{3}$ GeV.; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
11  ZHAO 2016 search for GeV-scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
12  AHMED 2011B search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$ in CDMS II; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $4 - 12$ GeV. Limit given for m(${{\mathit \chi}}$) = 5 GeV.
  References:
ABDELHAMEED 2019
EPJ C79 630 First results on sub-GeV spin-dependent dark matter interactions with$^{7}$Li
APRILE 2019C
PRL 123 241803 Search for Light Dark Matter Interactions Enhanced by the Migdal effect or Bremsstrahlung in XENON1T
APRILE 2019D
PRL 123 251801 Light Dark Matter Search with Ionization Signals in XENON1T
ARMENGAUD 2019
PR D99 082003 Searching for low-mass dark matter particles with a massive Ge bolometer operated above-ground
XIA 2019A
PL B792 193 PandaX-II Constraints on Spin-Dependent WIMP-Nucleon Effective Interactions
AGNESE 2018
PR D97 022002 Low-Mass Dark Matter Search with CDMSlite
JIANG 2018
PRL 120 241301 Limits on Light Weakly Interacting Massive Particles from the First 102.8 kg ${\times}$ day Data of the CDEX-10 Experiment
YANG 2018
CP C42 023002 Limits on light WIMPs with a 1 kg-scale germanium detector at 160 eVee physics threshold at the China Jinping Underground Laboratory
AKERIB 2017A
PRL 118 251302 Limits on Spin-Dependent WIMP-Nucleon Cross Section Obtained from the Complete LUX Exposure
FU 2017
PRL 118 071301 Spin-Dependent Weakly-Interacting-Massive-Particle-Nucleon Cross Section Limits from First Data of PandaX-II Experiment
ZHAO 2016
PR D93 092003 Search of Low-Mass WIMPs with a $\mathit p$-Type Point Contact Germanium Detector in the CDEX-1 Experiment
AHMED 2011B
PRL 106 131302 Results from a Low-Energy Analysis of the CDMS II Germanium Data