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

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

INSPIRE   PDGID:
S030DP5
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. • •
$<1 \times 10^{4}$ 90 1
AALBERS
2023A
LZ SD scatter on ${}^{}\mathrm {Xe}$
$<2 \times 10^{5}$ 90 2
ADHIKARI
2022B
C100 sub-GeV WIMP via SD coupling/Migdal effect
$<9 \times 10^{4}$ 90 3
ANGLOHER
2022
CRES SD limit using ${}^{}\mathrm {Li}$
$<40$ 90 4
ANGLOHER
2022A
CRES SD limit using ${}^{}\mathrm {Li}$ and ${}^{}\mathrm {Al}$
$<8 \times 10^{4}$ 90 5
ABDELHAMEED
2020A
CRES ${}^{}\mathrm {LiAlO}_{2}$
$<1 \times 10^{6}$ 95 6
ABDELHAMEED
2019
CRES GeV-scale WIMPs on ${}^{}\mathrm {Li}$
$<3 \times 10^{-4}$ 90 7
AMOLE
2019
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<1.7 \times 10^{4}$ 90 8
APRILE
2019C
XE1T light DM on ${}^{}\mathrm {Xe}$ via Migdal/brem effect
$<8 \times 10^{6}$ 90 9
ARMENGAUD
2019
EDEL GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<70$ 90 10
XIA
2019A
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<100$ 90 11
AGNESE
2018
SCDM GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<1$ 90 12
AKERIB
2017A
LUX ${}^{}\mathrm {Xe}$
$<0.6$ 90 13
FU
2017
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<0.2$ 90 14
AMOLE
2015
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<0.16$ 90 15
ARCHAMBAULT
2012
PICA ${}^{19}\mathrm {F}$
1  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.
2  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.
3  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.
4  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.
5  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.
6  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.
7  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.
8  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.
9  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.
10  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.
11  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.
12  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.
13  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.
14  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.
15  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