# For ${\boldsymbol m}_{{{\boldsymbol X}^{0}}}$ = 100 GeV INSPIRE search

For limits from ${{\mathit X}^{0}}$ annihilation in the Sun, the assumed annihilation final state is shown in parenthesis in the comment.
VALUE (pb) CL% DOCUMENT ID TECN  COMMENT
• • • We do not use the following data for averages, fits, limits, etc. • • •
$<4 \times 10^{-5}$ 90 1
 2019
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<4 \times 10^{-4}$ 90 2
 2019 A
XE1T ${}^{}\mathrm {Xe}$, SD
$<8 \times 10^{-4}$ 90 3
 2019 A
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<8 \times 10^{-4}$ 90 4
 2017 A
LUX ${}^{}\mathrm {Xe}$
$<5 \times 10^{-5}$ 90 5
 2017
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<0.033$ 90 6
 2017 A
X100 ${}^{}\mathrm {Xe}$ inelastic
$<0.28$ 90 7
 2017
DRFT ${}^{}\mathrm {C}{}^{}\mathrm {S}_{2}$
$<1.5 \times 10^{-3}$ 90 8
 2017
PNDX ${}^{}\mathrm {Xe}$
$\text{< 0.553 - 0.019}$ 95 9
 2016 D
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit j}}$ + $\not E_T$
$<1 \times 10^{-5}$ 90 10
 2016 F
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \gamma}}$ + $\not E_T$
$<1 \times 10^{-4}$ 90 11
 2016 C
ICCB solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<2 \times 10^{-4}$ 90 12
 2016
ANTR solar ${{\mathit \nu}}$ ( ${{\mathit W}}{{\mathit W}}$ , ${{\mathit b}}{{\overline{\mathit b}}}$ , ${{\mathit \tau}}{{\overline{\mathit \tau}}}$ )
$<3 \times 10^{-3}$ 90 13
 2016 A
LUX ${}^{}\mathrm {Xe}$
$<5 \times 10^{-4}$ 90 14
 2016
PICO CF$_{3}$I
$<1.5 \times 10^{-3}$ 90
 2015
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<3.19 \times 10^{-3}$ 90
 2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<2.80 \times 10^{-4}$ 90
 2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<1.24 \times 10^{-4}$ 90
 2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<800$ 90 15
 2015
NAGE ${}^{}\mathrm {C}{}^{}\mathrm {F}_{4}$
$<1.7 \times 10^{-3}$ 90 16
 2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.045$ 90 16
 2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<7.1 \times 10^{-4}$ 90 16
 2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<6 \times 10^{-3}$ 90
 2014
SMPL C$_{2}$ClF$_{5}$
$<2.68 \times 10^{-4}$ 90 17
 2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.0147$ 90 17
 2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<8.5 \times 10^{-4}$ 90 18
 2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.055$ 90 18
 2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<3.4 \times 10^{-4}$ 90 18
 2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<0.01$ 90 19
 2013
X100 ${}^{}\mathrm {Xe}$
$<7.1 \times 10^{-4}$ 90 20
 2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<8.4 \times 10^{-3}$ 90 20
 2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<3.1 \times 10^{-4}$ 90 20
 2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<7.07 \times 10^{-4}$ 90 21
 2012
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.0453$ 90 21
 2012
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<0.07$ 90 22
 2012
PICA ${}^{}\mathrm {F}$ (C$_{4}F_{10}$)
$<0.01$ 90
 2012
COUP CF$_{3}$I
$<1.8$ 90
 2012
DRFT F (CF$_{4}$)
$<9 \times 10^{-3}$
 2012
SMPL C$_{2}$ClF$_{5}$
$<0.02$ 90
 2012
KIMS CsI
$<2 \times 10^{3}$ 90 15
 2011
DMTP F (CF$_{4}$)
$<0.07$ 90
 2011
COUP CF$_{3}$I
$<2.7 \times 10^{-4}$ 90 23
 2011
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<4.5 \times 10^{-3}$ 90 23
 2011
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
24
 2010
SMPL C$_{2}$ClF$_{3}$
$<6 \times 10^{3}$ 90 15
 2010
NAGE CF$_{4}$
$<0.4$ 90
 2009
PICA ${}^{}\mathrm {F}$
$<0.8$ 90
 2009 A
ZEP3 ${}^{}\mathrm {Xe}$
$<1.0$ 90
 2008 A
XE10 ${}^{}\mathrm {Xe}$
$<15$ 90
 2007
ZEP2 ${}^{}\mathrm {Xe}$
$<0.2$ 90
 2007 A
KIMS CsI
$<1 \times 10^{4}$ 90 15
 2007
NAGE F (CF$_{4}$)
$<5$ 90 25
 2006
CDMS ${}^{73}\mathrm {Ge}$, ${}^{29}\mathrm {Si}$
$<2$ 90
 2006 A
CNTR F (CaF$_{2}$)
$<0.3$ 90
 2005
NAIA NaI
$<2$ 90
 2005
PICA F (C$_{4}F_{10}$)
$<100$ 90
 2005
EDEL ${}^{73}\mathrm {Ge}$
$<1.5$ 90
 2005
SMPL F (C$_{2}$ClF$_{5}$)
$<0.7$ 26
 2005 A
RVUE
27
 2004
RVUE
28
 2004 A
RVUE
$<35$ 90
 2003
BOLO LiF
$<40$ 90
 2003
BOLO NaF
1  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 ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit p}}$ ) $<$ $4 \times 10^{-5}$ pb for m(${{\mathit \chi}}$) = 100 GeV.
2  APRILE 2019A search for SD WIMP scatter on 1 t yr ${}^{}\mathrm {Xe}$; no signal, limits placed in ${{\mathit \sigma}^{SD}}$ ( ${{\mathit \chi}}{{\mathit p}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $6 - 1000$ GeV.
3  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.
4  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.
5  AMOLE 2017 require ${\mathit \sigma (}WIMP-{{\mathit p}}{)}{}^{SD}$ $<$ $5 \times 10^{-5}$ pb for m(WIMP) = 100 GeV using PICO-60 1167 kg-days exposure at SNOLab.
6  APRILE 2017A require require ${\mathit \sigma (}WIMP-{{\mathit p}}{)}$(inelastic)${}^{SD}$ $<$ $0.033$ pb for m(WIMP) = 100 GeV, based on 7640 kg day exposure at LNGS.
7  BATTAT 2017 use directional detection of ${}^{}\mathrm {C}{}^{}\mathrm {S}_{2}$ ions to require ${\mathit \sigma (}SD{)}$ $<$ $0.28$ pb for 100 GeV WIMP with a 55 days exposure at the Boulby Underground Science Facility.
8  FU 2017 from a 33000 kg d exposure at CJPL, PANDAX II derive for m(DM) = 100 GeV, ${{\mathit \sigma}^{SD}}(WIMP-{{\mathit p}}$) $<2 \times 10^{-3}$ pb.
9  AABOUD 2016D use ATLAS 13 TeV 3.2 ${\mathrm {fb}}{}^{-1}$ of data to search for monojet plus missing $\mathit E_{T}$; agree with SM rates; present limits on large extra dimensions, compressed SUSY spectra and wimp pair production.
10  AABOUD 2016F search for monophoton plus missing $\mathit E_{T}$ events at ATLAS with 13 Tev and 3.2 fb${}^{-1}$; signal agrees with SM background; place limits on SD WIMP-proton scattering vs. mediator mass and large extra dimension models.
11  AARTSEN 2016C search for high energy ${{\mathit \nu}}$s from WIMP annihilation in solar core; limits set on SD WIMP-${{\mathit p}}$ scattering (Fig. 8).
12  ADRIAN-MARTINEZ 2016 search for WIMP annihilation into ${{\mathit \nu}}$s from solar core; exclude SD cross section $<$ few $10^{-4}$ depending on $\mathit m$(WIMP).
13  AKERIB 2016A using 2013 data exclude SD WIMP-proton scattering $>$ $3 \times 10^{-3}$ pb for $\mathit m$(WIMP) = 100 GeV.
14  AMOLE 2016 use bubble technique on CF$_{3}$I target to exclude SD WIMP-${{\mathit p}}$ scattering $>$ $5 \times 10^{-4}$ pb for $\mathit m$(WIMP) = 100 GeV.
15  Use a direction-sensitive detector.
16  AVRORIN 2014 search for neutrinos from the Sun arising from the pair annihilation of ${{\mathit X}^{0}}$ trapped by the Sun in data taken between 1998 and 2003. See their Table 1 for limits assuming annihilation into neutrino pairs.
17  AARTSEN 2013 search for neutrinos from the Sun arising from the pair annihilation of ${{\mathit X}^{0}}$ trapped by the sun in data taken between June 2010 and May 2011.
18  ADRIAN-MARTINEZ 2013 search for neutrinos from the Sun arising from the pair annihilation of ${{\mathit X}^{0}}$ trapped by the sun in data taken between Jan. 2007 and Dec. 2008.
19  The value has been provided by the authors. APRILE 2013 note that the proton limits on ${}^{}\mathrm {Xe}$ are highly sensitive to the theoretical model used. See also APRILE 2014A.
20  BOLIEV 2013 search for neutrinos from the Sun arising from the pair annihilation of ${{\mathit X}^{0}}$ trapped by the sun in data taken from 1978 to 2009. See also SUVOROVA 2013 for an older analysis of the same data.
21  ABBASI 2012 search for neutrinos from the Sun arising from the pair annihilation of ${{\mathit X}^{0}}$ trapped by the Sun. The amount of ${{\mathit X}^{0}}$ depends on the ${{\mathit X}^{0}}$-proton cross section.
22  ARCHAMBAULT 2012 search for WIMP scatter on ${}^{}\mathrm {C}_{4}{}^{}\mathrm {F}_{10}$; limits set in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit p}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $4 - 500$ GeV.
23  TANAKA 2011 search for neutrinos from the Sun arising from the pair annihilation of ${{\mathit X}^{0}}$ trapped by the Sun. The amount of ${{\mathit X}^{0}}$ depends on the ${{\mathit X}^{0}}$-proton cross section.
24  See their Fig. 3 for limits on spin-dependent proton couplings for ${{\mathit X}^{0}}$ mass of 50 GeV.
26  GIULIANI 2005A analyze available data and give combined limits.
27  GIULIANI 2004 reanalyze COLLAR 2000 data and give limits for spin-dependent ${{\mathit X}^{0}}$-proton coupling.
28  GIULIANI 2004A give limits for spin-dependent ${{\mathit X}^{0}}$-proton couplings from existing data.
References:
 AMOLE 2019
PR D100 022001 Dark Matter Search Results from the Complete Exposure of the PICO-60 C$_3$F$_8$ Bubble Chamber
 APRILE 2019A
PRL 122 141301 Constraining the spin-dependent WIMP-nucleon cross sections with XENON1T
 XIA 2019A
PL B792 193 PandaX-II Constraints on Spin-Dependent WIMP-Nucleon Effective Interactions
 AKERIB 2017A
PRL 118 251302 Limits on Spin-Dependent WIMP-Nucleon Cross Section Obtained from the Complete LUX Exposure
 AMOLE 2017
PRL 118 251301 Dark Matter Search Results from the PICO-60 C$_{3}F_{8}$ Bubble Chamber
 APRILE 2017A
PR D96 022008 Search for WIMP Inelastic Scattering off Xenon Nuclei with XENON100
 BATTAT 2017
ASP 91 65 Low Threshold Results and Limits from the DRIFT Directional Dark Matter Detector
 FU 2017
PRL 118 071301 Spin-Dependent Weakly-Interacting-Massive-Particle-Nucleon Cross Section Limits from First Data of PandaX-II Experiment
 AABOUD 2016F
JHEP 1606 059 Search for New Phenomena in Events with a Photon and Missing Transverse Momentum in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 13 TeV with the ATLAS Detector
 AABOUD 2016D
PR D94 032005 Search for New Phenomena in Final States with an Energetic Jet and Large Missing Transverse Momentum in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 13 TeV using the ATLAS Detector
 AARTSEN 2016C
JCAP 1604 022 Improved Limits on Dark Matter Annihilation in the Sun with the 79-string IceCube Detector and Implications for Supersymmetry
PL B759 69 Limits on Dark Matter Annihilation in the Sun using the ANTARES Neutrino Telescope
 AKERIB 2016A
PRL 116 161302 Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment
 AMOLE 2016
PR D93 052014 Dark Matter Search Results from the PICO-60 CF$_{3}$I Bubble Chamber
 AMOLE 2015
PRL 114 231302 Dark Matter Search Results from the PICO-2L C$_{3}F_{8}$ Bubble Chamber
 CHOI 2015
PRL 114 141301 Search for Neutrinos from Annihilation of Captured Low-Mass Dark Matter Particles in the Sun by Super-Kamiokande
 NAKAMURA 2015
PTEP 2015 4 043F01 Direction-Sensitive Dark Matter Search with Gaseous Tracking Detector NEWAGE-0.3b'
 AVRORIN 2014
ASP 62 12 Search for Neutrino Emission from Relic Dark Matter in the Sun with the Baikal NT200 Detector
 FELIZARDO 2014
PR D89 072013 The SIMPLE Phase II Dark Matter Search
 AARTSEN 2013
PRL 110 131302 Search for Dark Matter Annihilations in the Sun with the 79-String IceCube Detector
JCAP 1311 032 First Results on Dark Matter Annihilation in the Sun using the ANTARES Neutrino Telescope
 APRILE 2013
PRL 111 021301 Limits on Spin-Dependent WIMP-Nucleon Cross Sections from 225 Live Days of XEENON100 Data
 BOLIEV 2013
JCAP 1309 019 Search for Muon Signal from Dark Matter Annihilations in the Sun with the Baksan Underground Scintillator Telescope for 24.12 Years
 ABBASI 2012
PR D85 042002 Multiyear Search for Dark Matter Annihilations in the Sun with the AMANDA-II and IceCube Detectors
 ARCHAMBAULT 2012
PL B711 153 Constraints on Low-Mass WIMP Interactions on ${}^{19}\mathrm {F}$ from PICASSO
 BEHNKE 2012
PR D86 052001 First Dark Matter Search Results from a 4-kg CF$_{3}$I Bubble Chamber Operated in a Deep Underground Site
 DAW 2012
ASP 35 397 Spin-Dependent Limits from the DRIFT-IId Directional Dark Matter Detector
 FELIZARDO 2012
PRL 108 201302 Final Analysis and Results of the Phase II SIMPLE Dark Matter Search
 KIM 2012
PRL 108 181301 New Limits on Interactions between Weakly Interacting Massive Particles and Nucleons Obtained with CsI(Tl) Crystal Detectors
 AHLEN 2011
PL B695 124 First Dark Matter Search Results from a Surface Run of the 10-L DMTPC (Dark Matter Time Projection Chamber) Directional Dark Matter Detector
 BEHNKE 2011
PRL 106 021303 Improved Limits on Spin-Dependent WIMP-Proton Interactions from a Two Liter CF$_{3}$I Bubble Chamber
 TANAKA 2011
APJ 742 78 An Indirect Search for WIMPs in the Sun using 3109.6 Days of Upward-Going Muons in Super-Kamiokande
 FELIZARDO 2010
PRL 105 211301 First Results of the Phase II SIMPLE Dark Matter Search
 MIUCHI 2010
PL B686 11 First Underground Results with NEWAGE-0.3a Direction-Sensitive Dark Matter Detector
 ARCHAMBAULT 2009
PL B682 185 Dark Matter Spin-Dependent Limits for WIMP Interactions on ${}^{19}\mathrm {F}$ by PICASSO
 LEBEDENKO 2009A
PRL 103 151302 Limits on the Spin-Dependent WIMP-Nucleon Cross Sections from the First Science Run of the ZEPLIN-III Experiment
 ANGLE 2008A
PRL 101 091301 Limits on Spin-Dependent WIMP-Nucleon Cross Sections from the XENON10 Experiment
 ALNER 2007
PL B653 161 Limits on Spin-Dependent WIMP-Nucleon Cross-Sections from the First ZEPLIN-II Data
 LEE 2007A
PRL 99 091301 Limits on Interactions between Weakly Interacting Massive Particles and Nucleons Obtained with CsI(Tl) Crystal Detectors
 MIUCHI 2007
PL B654 58 Direction-Sensitive Dark Matter Search Results in a Surface Laboratory
 AKERIB 2006
PR D73 011102 Limits on Spin-dependent WIMP $−$ Nucleon Interactions from the Cryogenic Dark Matter Search
 SHIMIZU 2006A
PL B633 195 Dark Matter Search Experiment with CaF$_{2}$(Eu) scintillator at Kamioka Observatory
 ALNER 2005
PL B616 17 Limits on WIMP Cross-Sections from the NAIAD Experiment at the Boulby Underground Laboratory
 BARNABE-HEIDER 2005
PL B624 186 Improved Spin-Dependent Limits from the PICASSO Dark Matter Search Experiment
 BENOIT 2005
PL B616 25 Sensitivity of the EDELWEISS WIMP Search to Spin-Dependent Interactions
 GIRARD 2005
PL B621 233 Simple Dark Matter Search Results
 GIULIANI 2005A
PR D71 123503 Model-Independent Limits from Spin-Dependent WIMP Dark Matter Experiments
 GIULIANI 2004
PL B588 151 Exclusion Limits on Spin Dependent WIMP-Nucleon Couplings from the SIMPLE Experiment
 GIULIANI 2004A
PRL 93 161301 Model-Independent Assessment of Current Direct Searches for Spin-Dependent Dark Matter
 MIUCHI 2003
ASP 19 135 First Results from Dark Matter Search Experiment with LiF Bolometer at Kamioka Underground Laboratory
 TAKEDA 2003
PL B572 145 Limits on the WIMP$−$Nucleon Coupling Coefficients from Dark Matter Search Experiment with NaF Bolometer