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

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

INSPIRE   PDGID:
S030DN5
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. • •
$<100$ 90 1
AALBERS
2023A
 LZ SD scatter on ${}^{}\mathrm {Xe}$
$<1 \times 10^{6}$ 90 2
ANGLOHER
2022
CRES SD limit using ${}^{}\mathrm {Li}$
$<570$ 90 3
ANGLOHER
2022A
 CRES SD limit using ${}^{}\mathrm {Li}$ and ${}^{}\mathrm {Al}$
$<1 \times 10^{8}$ 90 4
ABDELHAMEED
2020A
 CRES ${}^{}\mathrm {LiAlO}_{2}$
$<1 \times 10^{10}$ 95 5
ABDELHAMEED
2019
CRES SD low mass DM on ${}^{}\mathrm {Li}$
$<230$ 90 6
APRILE
2019C
 XE1T light DM on ${}^{}\mathrm {Xe}$ via Migdal/brem effect
$<0.01$ 90 7
APRILE
2019D
 XE1T light DM on ${}^{}\mathrm {Xe}$ via ionization
$<4 \times 10^{4}$ 90 8
ARMENGAUD
2019
EDEL GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<0.08$ 90 9
XIA
2019A
 PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<3$ 90 10
AGNESE
2018
SCDM GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<3$ 90 11
JIANG
2018
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<10$ 90 12
YANG
2018
CDEX WIMPs on ${}^{}\mathrm {Ge}$
$<0.1$ 90 13
AKERIB
2017A
 LUX ${}^{}\mathrm {Xe}$
$<0.1$ 90 14
FU
2017
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<20$ 90 15
ZHAO
2016
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<150$ 90 16
AHMED
2011B
 CDM2 GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
1  AALBERS 2023A search for GeV-scale WIMP scatter on ${}^{}\mathrm {Xe}$. No signal observed. Limits placed in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit n}}$) vs. m(${{\mathit \chi}}$) plane. Quoted limit is for m(${{\mathit \chi}}$) = 1 GeV via Migdal scattering.
2  ANGLOHER 2022 search for SD WIMP scatter on ${}^{}\mathrm {Li}$ target; no signal detected; limits placed on WIMP-neutron SD scatter versus m(WIMP); limit quoted for m(WIMP) = 1 GeV.
3  ANGLOHER 2022A search for spin-dependent DM scatter on ${}^{}\mathrm {Li}$ and ${}^{}\mathrm {Al}$ for m(DM) $\sim{}$ $0.2 - 6$ GeV; no signal observed; limits set in ${\mathit \sigma (}{{\mathit \chi}}{{\mathit n}}{)}$ vs. m(DM) plane; quoted limit is for m(DM) = 1 GeV.
4  ABDELHAMEED 2020A use ${}^{}\mathrm {LiAlO}_{2}$ target in CRESST to search for SD WIMP scatter; no signal; quoted limit is for m(DM) = 1 GeV.
5  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.
6  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.
7  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.
8  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.
9  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.
10  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.
11  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.
12  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.
13  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.
14  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.
15  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.
16  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