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

For ${\mathit m}_{{{\mathit X}^{0}}}$ = 1 TeV

INSPIRE   PDGID:
S030DP3
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. • •
$<1.2 \times 10^{-3}$ 90 1
HUANG
2022
PNDX SD DM limits
$<200$ 90 2
IKEDA
2021
NAGE directional gas TPC
$<4.81 \times 10^{-3}$ 90 3
AARTSEN
2020C
 ICCB SD WIMP on ${{\mathit p}}$
$<3 \times 10^{-4}$ 90 4
AMOLE
2019
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<4 \times 10^{-3}$ 90 5
APRILE
2019A
 XE1T ${}^{}\mathrm {Xe}$, SD
$<5 \times 10^{-3}$ 90 6
XIA
2019A
 PNDX SD WIMP on ${}^{}\mathrm {Xe}$
7
ALBERT
2018C
 HAWC DM annihilation in Sun to long-lived mediator
$<2.05 \times 10^{-5}$ 90 8
AARTSEN
2017A
 ICCB ${{\mathit \nu}}$, sun
$<7 \times 10^{-3}$ 90 9
AKERIB
2017A
 LUX ${}^{}\mathrm {Xe}$
$<0.02$ 90 10
FU
2017
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
11
ADRIAN-MARTIN..
2016B
 ANTR solar ${{\mathit \mu}}$ from WIMP annih.
$<0.01$ 90
AMOLE
2015
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<1.5 \times 10^{3}$ 90
NAKAMURA
2015
NAGE ${}^{}\mathrm {C}{}^{}\mathrm {F}_{4}$
$<2.7 \times 10^{-3}$ 90 12
AVRORIN
2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.069$ 90 12
AVRORIN
2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<8.4 \times 10^{-4}$ 90 12
AVRORIN
2014
BAIK ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<4.48 \times 10^{-4}$ 90 13
AARTSEN
2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.01$ 90 13
AARTSEN
2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<8.9 \times 10^{-4}$ 90 14
ADRIAN-MARTIN..
2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.02$ 90 14
ADRIAN-MARTIN..
2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<2.3 \times 10^{-4}$ 90 14
ADRIAN-MARTIN..
2013
ANTR ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<0.0757$ 90 15
APRILE
2013
X100 ${}^{}\mathrm {Xe}$
$<5.4 \times 10^{-3}$ 90 16
BOLIEV
2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.042$ 90 16
BOLIEV
2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<1.5 \times 10^{-3}$ 90 16
BOLIEV
2013
BAKS ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<2.50 \times 10^{-4}$ 90 17
ABBASI
2012
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<7.86 \times 10^{-3}$ 90 17
ABBASI
2012
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<0.08$ 90
BEHNKE
2012
COUP CF$_{3}$I
$<8$ 90
DAW
2012
DRFT F (CF$_{4}$)
$<0.06$
FELIZARDO
2012
SMPL C$_{2}$ClF$_{5}$
$<0.08$ 90
KIM
2012
KIMS CsI
$<8 \times 10^{3}$ 90 18
AHLEN
2011
DMTP F (CF$_{4}$)
$<0.4$ 90
BEHNKE
2011
COUP CF$_{3}$I
$<2 \times 10^{-3}$ 90 19
TANAKA
2011
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<0.02$ 90 19
TANAKA
2011
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<1 \times 10^{-3}$ 90 20
ABBASI
2010
ICCB KK dark matter
$<2 \times 10^{4}$ 90 18
MIUCHI
2010
NAGE CF$_{4}$
$<8.7 \times 10^{-4}$ 90
ABBASI
2009B
 ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit W}^{+}}{{\mathit W}^{-}}$ )
$<0.022$ 90
ABBASI
2009B
 ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<3$ 90
ARCHAMBAULT
2009
PICA ${}^{}\mathrm {F}$
$<6$ 90
LEBEDENKO
2009A
 ZEP3 ${}^{}\mathrm {Xe}$
$<9$ 90
ANGLE
2008A
 XE10 ${}^{}\mathrm {Xe}$
$<100$ 90
ALNER
2007
ZEP2 ${}^{}\mathrm {Xe}$
$<0.8$ 90
LEE
2007A
 KIMS CsI
$<4 \times 10^{4}$ 90 18
MIUCHI
2007
NAGE F (CF$_{4}$)
$<30$ 90 21
AKERIB
2006
CDMS ${}^{73}\mathrm {Ge}$, ${}^{29}\mathrm {Si}$
$<1.5$ 90
ALNER
2005
NAIA NaI
$<15$ 90
BARNABE-HEIDE..
2005
PICA F (C$_{4}F_{10}$)
$<600$ 90
BENOIT
2005
EDEL ${}^{73}\mathrm {Ge}$
$<10$ 90
GIRARD
2005
SMPL F (C$_{2}$ClF$_{5}$)
$<260$ 90
MIUCHI
2003
BOLO LiF
$<150$ 90
TAKEDA
2003
BOLO NaF
1  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) = 1 TeV.
2  IKEDA 2021 use direction sensitive TPC NEWAGE to search for SD WIMPs. No signal observed. Limits set in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit p}}$ ) vs. m plane; ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit p}}$ ) $<$ 200 pb for m(DM) = 1000 GeV.
3  AARTSEN 2020C place combined IceCube and Pico-60 velocity-independent limits on spin-dependent WIMP-${{\mathit p}}$ scatter ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit p}}$ ) $<$ $3 \times 10^{-3}$ pb for m(WIMP) = 1 TeV assuming dominant annihilation to ${{\mathit W}}{{\mathit W}}$ .
4  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.
5  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.
6  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.
7  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 ${{\mathit \sigma}}{}^{SD}$( ${{\mathit \chi}}{{\mathit p}}$ ).
8  AARTSEN 2017A search for neutrinos from solar WIMP annihilation into ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ in 532 days of live time.
9  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.
10  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.
11  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.
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  Use a direction-sensitive detector.
19  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.
20  ABBASI 2010 search for ${{\mathit \nu}_{{\mu}}}$ from annihilations of Kaluza-Klein photon dark matter in the Sun.
21  See also AKERIB 2005 .
References:
HUANG 2022
PL B834 137487 Constraints on the axial-vector and pseudo-scalar mediated WIMP-nucleus interactions from PandaX-4T experiment
IKEDA 2021
PTEP 2021 063F01 Direction-sensitive dark matter search with the low-background gaseous detector NEWAGE-0.3b?
AARTSEN 2020C
EPJ C80 819 Velocity Independent Constraints on Spin-Dependent DM-Nucleon Interactions from IceCube and PICO
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
Also
EPJ C79 214 (errat.) 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
Also
PRL 120 049902 (errat.) Spin-Dependent Weakly-Interacting-Massive-Particle?Nucleon Cross Section Limits from First Data of PandaX-II Experiment
ADRIAN-MARTINEZ 2016B
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
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
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
Also
PR D90 079902 (errat.) Erratum to BEHNKE 2012 : First Dark Matter Search Results from a 4-kg CF3I 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