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

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

INSPIRE   JSON  (beta) PDGID:
S030DP5
We provide here limits fo ${\mathit m}_{{{\mathit X}^{0}}}$ $<$ 5 GeV
S030DP5
VALUE (pb) CL% DOCUMENT ID TECN  COMMENT
• • We do not use the following data for averages, fits, limits, etc. • •
1
ADAMS
2025
 
PICO fermionic DM absorption
$<30.9$ 90 2
ARORA
2025
 
NEWS light DM search
$<5$ 90 3
YU
2025
 
C100 wimp search
$<0.56$ 90 4
ZHANG
2025B
 
PNDX wimp search
$<1 \times 10^{9}$ 90 5
ANGLOHER
2024B
 
CRES low mass wimp search
$<1 \times 10^{4}$ 90 6
AALBERS
2023A
 
LZ SD scatter on ${}^{}\mathrm {Xe}$
$<2 \times 10^{5}$ 90 7
ADHIKARI
2022B
 
C100 sub-GeV WIMP via SD coupling/Migdal effect
$<9 \times 10^{4}$ 90 8
ANGLOHER
2022
 
CRES SD limit using ${}^{}\mathrm {Li}$
$<40$ 90 9
ANGLOHER
2022A
 
CRES SD limit using ${}^{}\mathrm {Li}$ and ${}^{}\mathrm {Al}$
$<8 \times 10^{4}$ 90 10
ABDELHAMEED
2020A
 
CRES ${}^{}\mathrm {LiAlO}_{2}$
$<1 \times 10^{6}$ 95 11
ABDELHAMEED
2019
 
CRES GeV-scale WIMPs on ${}^{}\mathrm {Li}$
$<3 \times 10^{-4}$ 90 12
AMOLE
2019
 
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<1.7 \times 10^{4}$ 90 13
APRILE
2019C
 
XE1T light DM on ${}^{}\mathrm {Xe}$ via Migdal/brem effect
$<8 \times 10^{6}$ 90 14
ARMENGAUD
2019
 
EDEL GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<70$ 90 15
XIA
2019A
 
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<100$ 90 16
AGNESE
2018
 
SCDM GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<1$ 90 17
AKERIB
2017A
 
LUX ${}^{}\mathrm {Xe}$
$<0.6$ 90 18
FU
2017
 
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<0.2$ 90 19
AMOLE
2015
 
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<0.16$ 90 20
ARCHAMBAULT
2012
 
PICA ${}^{19}\mathrm {F}$
1  ADAMS 2025 report on fermionic DM in MeV range search via nuclear absorption at PICO-60. No signal observed. Limits placed on m(DM) vs. absorption cross section for EFT operator O$_{4}$.
2  ARORA 2025 report search for light DM at NEWS-G. No signal observed. Limits placed in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) vs m(${{\mathit \chi}}$) plane. Quoted limit is for m(${{\mathit \chi}}$) = 0.76 GeV.
3  YU 2025 report on COSINE-100 wimp search in 3-year data. No signal observed. Limits placed in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) vs m(${{\mathit \chi}}$) plane. Quoted limit for m(${{\mathit \chi}}$) = 3 GeV.
4  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.
5  ANGLOHER 2024B search for low mass wimps. No signal observed. Limits placed in ${{\mathit \sigma}}$ vs. m plane. Quoted limit for m = 100 MeV.
6  AALBERS 2023A search for GeV-scale WIMP scatter on ${}^{}\mathrm {Xe}$. No signal observed. Limits placed in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) vs. m(${{\mathit \chi}}$) plane. Quoted limit is for m(${{\mathit \chi}}$) = 1 GeV via Migdal scattering.
7  ADHIKARI 2022B search for sub-GeV WIMPs via SI and SD detection; no signal detected; limits placed in m(${{\mathit \chi}}$) vs. ${{\mathit \sigma}}$ plane for m(${{\mathit \chi}}$): $0.2 - 3$ GeV; quoted limit is for SD m(${{\mathit \chi}}$) = 1 GeV.
8  ANGLOHER 2022 search for SD WIMP-proton scatter from ${}^{}\mathrm {Li}$ target; no signal detected; limits placed in ${{\mathit \sigma}}$ vs. m(WIMP) plane; limit quoted for m(WIMP) = 1 GeV.
9  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 ${\mathit \sigma (}{{\mathit \chi}}{{\mathit p}}{)}$ vs. m(DM) plane; quoted limit is for m(DM) = 1 GeV.
10  ABDELHAMEED 2020A use ${}^{}\mathrm {LiAlO}_{2}$ target in CRESST to search for SD WIMP scatter on ${{\mathit p}}$; no signal; quoted limit is for m(DM) = 1 GeV.
11  ABDELHAMEED 2019 search for SD WIMP scatter on ${}^{7}\mathrm {Li}$; limits placed on ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) for m(${{\mathit \chi}}$) $\sim{}$ $0.8 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 1 GeV.
12  AMOLE 2019 search for SD WIMP scatter on ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$ in PICO-60 bubble chamber; no signal: set limit for spin dependent coupling ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) $<$ $2 \times 10^{-4}$ pb for m(${{\mathit \chi}}$) = 5 GeV.
13  APRILE 2019C search for light DM on ${}^{}\mathrm {Xe}$ via Migdal/brem effect; no signal, require ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) $<$ $1.7 \times 10^{4}$ pb for m(${{\mathit \chi}}$) = 1 GeV.
14  ARMENGAUD 2019 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $0.5 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
15  XIA 2019A search for WIMP scatter on ${}^{}\mathrm {Xe}$ in PandaX-II; limits placed in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) 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.
16  AGNESE 2018 search for GeV scale WIMPs with CDMSlite; limits placed in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $1.5 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
17  AKERIB 2017A search for SD WIMP scatter on ${}^{}\mathrm {Xe}$ using 129.5 kg yr exposure; limits placed in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $6 - 1 \times 10^{5}$ GeV.
18  FU 2017 search for SD WIMP scatter on ${}^{}\mathrm {Xe}$; limits set in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) 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.
19  AMOLE 2015 search for WIMP scatter on ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$ in PICO-2L; limits placed in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 1 \times 10^{4}$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
20  ARCHAMBAULT 2012 search for SD WIMP scatter in ${}^{19}\mathrm {F}$ with PICASSO; limits set in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit p}}$) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $4 - 500$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
References