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

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

INSPIRE   JSON  (beta) PDGID:
S030DN5
We provide here limits fo ${\mathit m}_{{{\mathit X}^{0}}}$ $<$ 5 GeV
S030DN5
VALUE (pb) CL% DOCUMENT ID TECN  COMMENT
• • We do not use the following data for averages, fits, limits, etc. • •
$<4 \times 10^{-4}$ 90 1
APRILE
2025
 
XENT light DM search
$<0.016$ 90 2
ZHANG
2025B
 
PNDX wimp search
$<1 \times 10^{10}$ 90 3
ANGLOHER
2024B
 
CRES low mass DM search
$<100$ 90 4
AALBERS
2023A
 
LZ SD scatter on ${}^{}\mathrm {Xe}$
$<1 \times 10^{6}$ 90 5
ANGLOHER
2022
 
CRES SD limit using ${}^{}\mathrm {Li}$
$<570$ 90 6
ANGLOHER
2022A
 
CRES SD limit using ${}^{}\mathrm {Li}$ and ${}^{}\mathrm {Al}$
$<1 \times 10^{8}$ 90 7
ABDELHAMEED
2020A
 
CRES ${}^{}\mathrm {LiAlO}_{2}$
$<1 \times 10^{10}$ 95 8
ABDELHAMEED
2019
 
CRES SD low mass DM on ${}^{}\mathrm {Li}$
$<230$ 90 9
APRILE
2019C
 
XE1T light DM on ${}^{}\mathrm {Xe}$ via Migdal/brem effect
$<0.01$ 90 10
APRILE
2019D
 
XE1T light DM on ${}^{}\mathrm {Xe}$ via ionization
$<4 \times 10^{4}$ 90 11
ARMENGAUD
2019
 
EDEL GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<0.08$ 90 12
XIA
2019A
 
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<3$ 90 13
AGNESE
2018
 
SCDM GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<3$ 90 14
JIANG
2018
 
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<10$ 90 15
YANG
2018
 
CDEX WIMPs on ${}^{}\mathrm {Ge}$
$<0.1$ 90 16
AKERIB
2017A
 
LUX ${}^{}\mathrm {Xe}$
$<0.1$ 90 17
FU
2017
 
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<20$ 90 18
ZHAO
2016
 
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<150$ 90 19
AHMED
2011B
 
CDM2 GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
1  APRILE 2025 report GeV-scale DM search near edge of neutrino fog using XENONnT. No signal observed. Limits set in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit N}}$) vs. m(${{\mathit \chi}}$) plane. Quoted limit is for m(${{\mathit \chi}}$) = 6 GeV.
2  ZHANG 2025B search for light GeV-scale wimps using run 0 and run 1 PandaX-4T data. No signal observed. Quoted limit is for m(${{\mathit \chi}}$) = 3 GeV.
3  ANGLOHER 2024B search for low mass wimps. No signal observed. Limits placed in ${{\mathit \sigma}}$ vs. m plane. Quoted limit for m = 100 MeV.
4  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.
5  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.
6  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.
7  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.
8  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.
9  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.
10  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.
11  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.
12  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.
13  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.
14  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.
15  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.
16  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.
17  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.
18  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.
19  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