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

For ${\mathit m}_{{{\mathit X}^{0}}}$ = 20 GeV

INSPIRE   PDGID:
S030DN1
VALUE (pb) CL% DOCUMENT ID TECN  COMMENT
• • We do not use the following data for averages, fits, limits, etc. • •
$<2 \times 10^{-6}$ 90 1
AALBERS
2023
LZ SD scatter on ${}^{}\mathrm {Xe}$
$<5 \times 10^{6}$ 90 2
ANGLOHER
2022
CRES SD limit using ${}^{}\mathrm {Li}$
$<7 \times 10^{-6}$ 90 3
HUANG
2022
PNDX SD DM limits
$<5 \times 10^{7}$ 90 4
ABDELHAMEED
2020A
CRES ${}^{}\mathrm {LiAlO}_{2}$
$<0.1$ 5
FELIZARDO
2020
SMPL WIMPs via SIMPLE
$<8 \times 10^{-6}$ 90 6
APRILE
2019A
XE1T ${}^{}\mathrm {Xe}$, SD
$<3 \times 10^{-5}$ 90 7
XIA
2019A
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<1.5$ 95 8
AGNESE
2018
SCDM ${}^{}\mathrm {Ge}$
$<2.5 \times 10^{-5}$ 90 9
AKERIB
2017A
LUX ${}^{}\mathrm {Xe}$
$<7 \times 10^{-5}$ 90 10
FU
2017
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<2$ 90 11
ZHAO
2016
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<0.09$ 90
FELIZARDO
2014
SMPL C$_{2}$ClF$_{5}$
$<8$ 90 12
UCHIDA
2014
XMAS ${}^{129}\mathrm {Xe}$, inelastic
$<1.13 \times 10^{-3}$ 90 13
APRILE
2013
X100 ${}^{}\mathrm {Xe}$
$<0.02$ 90
AKIMOV
2012
ZEP3 ${}^{}\mathrm {Xe}$
$<0.06$ 90
AHMED
2009
CDM2 ${}^{}\mathrm {Ge}$
$<0.04$ 90
LEBEDENKO
2009A
ZEP3 ${}^{}\mathrm {Xe}$
$<50$ 14
LIN
2009
TEXO ${}^{}\mathrm {Ge}$
$<6 \times 10^{-3}$ 90
ANGLE
2008A
XE10 ${}^{}\mathrm {Xe}$
$<0.5$ 90
ALNER
2007
ZEP2 ${}^{}\mathrm {Xe}$
$<25$ 90
LEE
2007A
KIMS CsI
$<0.3$ 90 15
AKERIB
2006
CDMS ${}^{73}\mathrm {Ge}$, ${}^{29}\mathrm {Si}$
$<30$ 90
SHIMIZU
2006A
CNTR F (CaF$_{2}$)
$<60$ 90
ALNER
2005
NAIA NaI
$<20$ 90
BARNABE-HEIDE..
2005
PICA F (C$_{4}F_{10}$)
$<10$ 90
BENOIT
2005
EDEL ${}^{73}\mathrm {Ge}$
$<4$ 90
KLAPDOR-KLEIN..
2005
HDMS ${}^{73}\mathrm {Ge}$ (enriched)
$<600$ 90
TAKEDA
2003
BOLO NaF
1  AALBERS 2023 yield first LZ limits on SD WIMP-${{\mathit n}}$ scatter using ${}^{}\mathrm {Xe}$. ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit n}})<$ $2 \times 10^{-6}$ pb for m(${{\mathit \chi}}$) = 20 GeV.
2  ANGLOHER 2022 search for SD WIMP-neutron scatter from ${}^{}\mathrm {Li}$ target; no signal detected; limits placed in ${{\mathit \sigma}}$ vs. m(WIMP) plane.
3  HUANG 2022 search for SD DM scatter on ${}^{}\mathrm {Xe}$; no signal observed; limits placed in ${\mathit \sigma (}{{\mathit \chi}}{{\mathit n}}{)}$ vs. m(DM) plane; quoted limit is for m(DM) = 20 GeV.
4  ABDELHAMEED 2020A use ${}^{}\mathrm {LiAlO}_{2}$ target in CRESST to search for SD WIMP scatter on ${{\mathit n}}$; limits placed for m(WIMP): $0.3 - 30$ GeV in Fig. 8. Quoted limit is for M(WIMP) = 30 GeV.
5  FELIZARDO 2020 presents 2014 SIMPLE bounds on WIMP DM using ${}^{}\mathrm {C}_{2}{}^{}\mathrm {Cl}{}^{}\mathrm {F}_{5}$ target .
6  APRILE 2019A search for SD WIMP scatter on 1 t yr ${}^{}\mathrm {Xe}$; no signal: limits placed in ${{\mathit \sigma}^{SD}}({{\mathit \chi}}{{\mathit n}}$) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $6 - 1000$ GeV.
7  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.
8  AGNESE 2018 give limits for ${{\mathit \sigma}^{SD}}({{\mathit n}}{{\mathit \chi}}$) for m(WIMP) between 1.5 and 20 GeV using CDMSlite mode data.
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.
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.
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.
12  Derived limit from search for inelastic scattering ${{\mathit X}^{0}}$ ${+}$ ${}^{129}\mathrm {Xe}$ $\rightarrow$ ${{\mathit X}^{0}}{+}$ ${}^{129}\mathrm {Xe}^{*}$(39.58 keV).
13  The value has been provided by the authors. See also APRILE 2014A.
14  See their Fig. 6(b) for cross section limits for ${\mathit m}_{{{\mathit X}^{0}}}$ extending down to 2 GeV.
15  See also AKERIB 2005.
References