# For ${\boldsymbol m}_{{{\boldsymbol X}^{0}}}$ = 1 TeV 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. • • •
$<3 \times 10^{-4}$ 90 1
 2019
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<4 \times 10^{-3}$ 90 2
 2019 A
XE1T ${}^{}\mathrm {Xe}$, SD
$<5 \times 10^{-3}$ 90 3
 2019 A
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
4
 2018 C
HAWC DM annihilation in Sun to long-lived mediator
$<2.05 \times 10^{-5}$ 90 5
 2017 A
ICCB ${{\mathit \nu}}$, sun
$<7 \times 10^{-3}$ 90 6
 2017 A
LUX ${}^{}\mathrm {Xe}$
$<0.02$ 90 7
 2017
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
8
 2016 B
ANTR solar ${{\mathit \mu}}$ from WIMP annih.
$<0.01$ 90
 2015
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<1.5 \times 10^{3}$ 90
 2015
NAGE ${}^{}\mathrm {C}{}^{}\mathrm {F}_{4}$
$<2.7 \times 10^{-3}$ 90 9
 2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.069$ 90 9
 2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<8.4 \times 10^{-4}$ 90 9
 2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<4.48 \times 10^{-4}$ 90 10
 2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.01$ 90 10
 2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<8.9 \times 10^{-4}$ 90 11
 2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.02$ 90 11
 2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<2.3 \times 10^{-4}$ 90 11
 2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<0.0757$ 90 12
 2013
X100 ${}^{}\mathrm {Xe}$
$<5.4 \times 10^{-3}$ 90 13
 2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.042$ 90 13
 2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<1.5 \times 10^{-3}$ 90 13
 2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<2.50 \times 10^{-4}$ 90 14
 2012
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<7.86 \times 10^{-3}$ 90 14
 2012
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<0.08$ 90
 2012
COUP CF$_{3}$I
$<8$ 90
 2012
DRFT F (CF$_{4}$)
$<0.06$
 2012
SMPL C$_{2}$ClF$_{5}$
$<0.08$ 90
 2012
KIMS CsI
$<8 \times 10^{3}$ 90 15
 2011
DMTP F (CF$_{4}$)
$<0.4$ 90
 2011
COUP CF$_{3}$I
$<2 \times 10^{-3}$ 90 16
 2011
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<0.02$ 90 16
 2011
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<1 \times 10^{-3}$ 90 17
 2010
ICCB KK dark matter
$<2 \times 10^{4}$ 90 15
 2010
NAGE CF$_{4}$
$<8.7 \times 10^{-4}$ 90
 2009 B
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.022$ 90
 2009 B
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<3$ 90
 2009
PICA ${}^{}\mathrm {F}$
$<6$ 90
 2009 A
ZEP3 ${}^{}\mathrm {Xe}$
$<9$ 90
 2008 A
XE10 ${}^{}\mathrm {Xe}$
$<100$ 90
 2007
ZEP2 ${}^{}\mathrm {Xe}$
$<0.8$ 90
 2007 A
KIMS CsI
$<4 \times 10^{4}$ 90 15
 2007
NAGE F (CF$_{4}$)
$<30$ 90 18
 2006
CDMS ${}^{73}\mathrm {Ge}$, ${}^{29}\mathrm {Si}$
$<1.5$ 90
 2005
NAIA NaI
$<15$ 90
 2005
PICA F (C$_{4}F_{10}$)
$<600$ 90
 2005
EDEL ${}^{73}\mathrm {Ge}$
$<10$ 90
 2005
SMPL F (C$_{2}$ClF$_{5}$)
$<260$ 90
 2003
BOLO LiF
$<150$ 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 ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit p}}$ ) $<$ $3 \times 10^{-4}$ pb for m(${{\mathit \chi}}$) = 1000 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  ALBERT 2018C search for DM annihilation in Sun to long-lived mediator (LLM) which decays outside Sun, for DM masses above 1 TeV; assuming LLM, limits set on ${{\mathit \sigma}}{}^{SD}$( ${{\mathit \chi}}{{\mathit p}}$ ).
5  AARTSEN 2017A search for neutrinos from solar WIMP annihilation into ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ in 532 days of live time.
6  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.
7  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.
8  ADRIAN-MARTINEZ 2016B search for secluded DM via WIMP annihilation in solar core into light mediator which later decays to ${{\mathit \mu}}$ or ${{\mathit \nu}}$s; limits presented in Figures 3 and 4.
9  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.
10  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.
11  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.
12  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.
13  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.
14  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.
15  Use a direction-sensitive detector.
16  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.
17  ABBASI 2010 search for ${{\mathit \nu}_{{\mu}}}$ from annihilations of Kaluza-Klein photon dark matter in the Sun.
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
 ALBERT 2018C
PR D98 123012 Constraints on Spin-Dependent Dark Matter Scattering with Long-Lived Mediators from TeV Observations of the Sun with HAWC
 AARTSEN 2017A
EPJ C77 146 Search for Annihilating Dark Matter in the Sun with 3 Years of IceCube Data
 AKERIB 2017A
PRL 118 251302 Limits on Spin-Dependent WIMP-Nucleon Cross Section Obtained from the Complete LUX Exposure
 FU 2017
PRL 118 071301 Spin-Dependent Weakly-Interacting-Massive-Particle-Nucleon Cross Section Limits from First Data of PandaX-II Experiment
JCAP 1605 016 A Search for Secluded Dark Matter in the Sun with the ANTARES Neutrino Telescope
 AMOLE 2015
PRL 114 231302 Dark Matter Search Results from the PICO-2L C$_{3}F_{8}$ Bubble Chamber
 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
 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
 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
 ABBASI 2010
PR D81 057101 Limits on a Muon Flux from Kaluza-Klein Dark Matter Annihilations in the Sun from the IceCube 22-string Detector
 MIUCHI 2010
PL B686 11 First Underground Results with NEWAGE-0.3a Direction-Sensitive Dark Matter Detector
 ABBASI 2009B
PRL 102 201302 Limits on a Muon Flux from Neutralino Annihilations in the Sun with the IceCube 22-String 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
 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
 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