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

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. • • •
$<5 \times 10^{-5}$ 90 1
AMOLE
2017
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<0.033$ 90 2
APRILE
2017A
X100 ${}^{}\mathrm {Xe}$ inelastic
$<0.28$ 90 3
BATTAT
2017
DRFT ${}^{}\mathrm {C}{}^{}\mathrm {S}_{2}$
$<2 \times 10^{-3}$ 90 4
FU
2017
PNDX ${}^{}\mathrm {Xe}$
$\text{< 0.553 - 0.019}$ 95 5
AABOUD
2016D
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit j}}$ + $\not E_T$
$<1 \times 10^{-5}$ 90 6
AABOUD
2016F
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \gamma}}$ + $\not E_T$
$<1 \times 10^{-4}$ 90 7
AARTSEN
2016C
ICCB solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<2 \times 10^{-4}$ 90 8
ADRIAN-MARTIN..
2016
ANTR solar ${{\mathit \nu}}$ ( ${{\mathit W}}{{\mathit W}}$ , ${{\mathit b}}{{\overline{\mathit b}}}$ , ${{\mathit \tau}}{{\overline{\mathit \tau}}}$ )
$<3 \times 10^{-3}$ 90 9
AKERIB
2016A
LUX ${}^{}\mathrm {Xe}$
$<5 \times 10^{-4}$ 90 10
AMOLE
2016
PICO CF$_{3}$I
$<1.5 \times 10^{-3}$ 90
AMOLE
2015
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<3.19 \times 10^{-3}$ 90
CHOI
2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<2.80 \times 10^{-4}$ 90
CHOI
2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<1.24 \times 10^{-4}$ 90
CHOI
2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<800$ 90 11
NAKAMURA
2015
NAGE ${}^{}\mathrm {C}{}^{}\mathrm {F}_{4}$
$<1.7 \times 10^{-3}$ 90 12
AVRORIN
2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.045$ 90 12
AVRORIN
2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<7.1 \times 10^{-4}$ 90 12
AVRORIN
2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<6 \times 10^{-3}$ 90
FELIZARDO
2014
SMPL C$_{2}$ClF$_{5}$
$<2.68 \times 10^{-4}$ 90 13
AARTSEN
2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.0147$ 90 13
AARTSEN
2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<8.5 \times 10^{-4}$ 90 14
ADRIAN-MARTIN..
2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.055$ 90 14
ADRIAN-MARTIN..
2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<3.4 \times 10^{-4}$ 90 14
ADRIAN-MARTIN..
2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<0.01$ 90 15
APRILE
2013
X100 ${}^{}\mathrm {Xe}$
$<7.1 \times 10^{-4}$ 90 16
BOLIEV
2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<8.4 \times 10^{-3}$ 90 16
BOLIEV
2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<3.1 \times 10^{-4}$ 90 16
BOLIEV
2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<7.07 \times 10^{-4}$ 90 17
ABBASI
2012
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.0453$ 90 17
ABBASI
2012
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<0.07$ 90
ARCHAMBAULT
2012
PICA ${}^{}\mathrm {F}$ (C$_{4}F_{10}$)
$<0.01$ 90
BEHNKE
2012
COUP CF$_{3}$I
$<1.8$ 90
DAW
2012
DRFT F (CF$_{4}$)
$<9 \times 10^{-3}$
FELIZARDO
2012
SMPL C$_{2}$ClF$_{5}$
$<0.02$ 90
KIM
2012
KIMS CsI
$<2 \times 10^{3}$ 90 11
AHLEN
2011
DMTP F (CF$_{4}$)
$<0.07$ 90
BEHNKE
2011
COUP CF$_{3}$I
$<2.7 \times 10^{-4}$ 90 18
TANAKA
2011
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<4.5 \times 10^{-3}$ 90 18
TANAKA
2011
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
19
FELIZARDO
2010
SMPL C$_{2}$ClF$_{3}$
$<6 \times 10^{3}$ 90 11
MIUCHI
2010
NAGE CF$_{4}$
$<0.4$ 90
ARCHAMBAULT
2009
PICA ${}^{}\mathrm {F}$
$<0.8$ 90
LEBEDENKO
2009A
ZEP3 ${}^{}\mathrm {Xe}$
$<1.0$ 90
ANGLE
2008A
XE10 ${}^{}\mathrm {Xe}$
$<15$ 90
ALNER
2007
ZEP2 ${}^{}\mathrm {Xe}$
$<0.2$ 90
LEE
2007A
KIMS CsI
$<1 \times 10^{4}$ 90 11
MIUCHI
2007
NAGE F (CF$_{4}$)
$<5$ 90 20
AKERIB
2006
CDMS ${}^{73}\mathrm {Ge}$, ${}^{29}\mathrm {Si}$
$<2$ 90
SHIMIZU
2006A
CNTR F (CaF$_{2}$)
$<0.3$ 90
ALNER
2005
NAIA NaI
$<2$ 90
BARNABE-HEIDE..
2005
PICA F (C$_{4}F_{10}$)
$<100$ 90
BENOIT
2005
EDEL ${}^{73}\mathrm {Ge}$
$<1.5$ 90
GIRARD
2005
SMPL F (C$_{2}$ClF$_{5}$)
$<0.7$ 21
GIULIANI
2005A
RVUE
22
GIULIANI
2004
RVUE
23
GIULIANI
2004A
RVUE
$<35$ 90
MIUCHI
2003
BOLO LiF
$<40$ 90
TAKEDA
2003
BOLO NaF
1  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.
2  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.
3  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.
4  FU 2017 from a 33000 kg d exposure at CJPL, PANDAX II derive for m(DM) = 100 GeV, ${{\mathit \sigma}}$(WIMP-p)${}^{SD}$ $<2 \times 10^{-3}$ pb and ${{\mathit \sigma}}$(WIMP-n)${}^{SD}<$ $6 \times 10^{-5}$ pb.
5  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.
6  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.
7  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).
8  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).
9  AKERIB 2016A using 2013 data exclude SD WIMP-proton scattering $>$ $3 \times 10^{-3}$ pb for $\mathit m$(WIMP) = 100 GeV.
10  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.
11  Use a direction-sensitive detector.
12  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.
13  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.
14  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.
15  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.
16  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.
17  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.
18  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.
19  See their Fig. 3 for limits on spin-dependent proton couplings for ${{\mathit X}^{0}}$ mass of 50 GeV.
20  See also AKERIB 2005 .
21  GIULIANI 2005A analyze available data and give combined limits.
22  GIULIANI 2004 reanalyze COLLAR 2000 data and give limits for spin-dependent ${{\mathit X}^{0}}$-proton coupling.
23  GIULIANI 2004A give limits for spin-dependent ${{\mathit X}^{0}}$-proton couplings from existing data.
  References:
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 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
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
AARTSEN 2016C
JCAP 1604 022 Improved Limits on Dark Matter Annihilation in the Sun with the 79-string IceCube Detector and Implications for Supersymmetry
ADRIAN-MARTINEZ 2016
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
ADRIAN-MARTINEZ 2013
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
SUVOROVA 2013
PAN 76 1367 Upper Limit on the Cross Section for Elastic Neutralino-Nucleon Scattering in a Neutrino Experiment at the Baksan Underground Scintillator Telescope
APRILE 2014A
ASP 54 11 Analysis of the XENON100 Dark Matter Search Data
COLLAR 2000
PRL 85 3083 First Dark Matter Limits from a Large-mass, Low-background, Superheated Droplet Detector
AKERIB 2005
PR D72 052009 Exclusion Limits on the WIMP-Nucleon Cross Section from the First Run of the Cryogenic Dark Matter Search in the Soudan Underground Laboratory