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

For ${\boldsymbol m}_{{{\boldsymbol X}^{0}}}$ = 20 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. • • •
$<3 \times 10^{5}$ 95 1
ABDELHAMEED
2019
CRES ${}^{7}\mathrm {Li}$
$<2.5 \times 10^{-5}$ 90 2
AMOLE
2019
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<2.5 \times 10^{-4}$ 90 3
APRILE
2019A
XE1T ${}^{}\mathrm {Xe}$, SD
$<1 \times 10^{-3}$ 90 4
XIA
2019A
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<30$ 95 5
AGNESE
2018
SCDM ${}^{}\mathrm {Ge}$
$<1 \times 10^{-3}$ 90 6
AKERIB
2017A
LUX ${}^{}\mathrm {Xe}$
$<0.0132$ 90 7
BEHNKE
2017
PICA ${}^{}\mathrm {C}_{4}{}^{}\mathrm {F}_{10}$
$<2 \times 10^{-3}$ 90 8
FU
2017
PNDX SD WIMP on ${}^{}\mathrm {Xe}$
$<5 \times 10^{-4}$ 90 9
AMOLE
2016A
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<2 \times 10^{-6}$ 90 10
KHACHATRYAN
2016AJ
CMS 8 TeV ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit Z}}$ +$\not E_T$; ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}}{{\overline{\mathit \ell}}}$
$<1.2 \times 10^{-3}$ 90
AMOLE
2015
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<1.43 \times 10^{-3}$ 90
CHOI
2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<1.42 \times 10^{-4}$ 90
CHOI
2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<5 \times 10^{-3}$ 90
FELIZARDO
2014
SMPL C$_{2}$ClF$_{5}$
$<0.0129$ 90 11
AARTSEN
2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<0.0317$ 90 12
APRILE
2013
X100 ${}^{}\mathrm {Xe}$
$<0.03$ 90 13
ARCHAMBAULT
2012
PICA ${}^{}\mathrm {F}$ (C$_{4}F_{10}$)
$<0.06$ 90
BEHNKE
2012
COUP CF$_{3}$I
$<20$ 90
DAW
2012
DRFT F (CF$_{4}$)
$<7 \times 10^{-3}$
FELIZARDO
2012
SMPL C$_{2}$ClF$_{5}$
$<0.15$ 90
KIM
2012
KIMS CsI
$<1 \times 10^{5}$ 90 14
AHLEN
2011
DMTP F (CF$_{4}$)
$<0.1$ 90 14
BEHNKE
2011
COUP CF$_{3}$I
$<0.015$ 90 15
TANAKA
2011
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<0.2$ 90
ARCHAMBAULT
2009
PICA ${}^{}\mathrm {F}$
$<4$ 90
LEBEDENKO
2009A
ZEP3 ${}^{}\mathrm {Xe}$
$<0.6$ 90
ANGLE
2008A
XE10 ${}^{}\mathrm {Xe}$
$<100$ 90
ALNER
2007
ZEP2 ${}^{}\mathrm {Xe}$
$<1$ 90
LEE
2007A
KIMS CsI
$<20$ 90 16
AKERIB
2006
CDMS ${}^{73}\mathrm {Ge}$, ${}^{29}\mathrm {Si}$
$<2$ 90
SHIMIZU
2006A
CNTR F (CaF$_{2}$)
$<0.5$ 90
ALNER
2005
NAIA NaI
$<1.5$ 90
BARNABE-HEIDE..
2005
PICA F (C$_{4}F_{10}$)
$<1.5$ 90
GIRARD
2005
SMPL F (C$_{2}$ClF$_{5}$)
$<35$ 90
MIUCHI
2003
BOLO LiF
$<30$ 90
TAKEDA
2003
BOLO NaF
1  ABDELHAMEED 2019 uses ${}^{}\mathrm {Li}_{2}{}^{}\mathrm {MoO}_{4}$ target to set limit for spin dependent coupling ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit p}}$ ) $<$ $3. \times 10^{5}$ pb for m(${{\mathit \chi}}$) = 20 GeV.
2  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 ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit p}}$ ) $<$ $2.5 \times 10^{-5}$ pb for m(${{\mathit \chi}}$) = 20 GeV.
3  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.
4  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.
5  AGNESE 2018 give limits for ${{\mathit \sigma}^{SD}}$( ${{\mathit p}}{{\mathit \chi}}$ ) for m(WIMP) between 1.5 and 20 GeV using CDMSlite mode data.
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  BEHNKE 2017 show final Picasso results based on 231.4 kg d exposure at SNOLab for WIMP scatter on ${}^{}\mathrm {C}_{4}{}^{}\mathrm {F}_{10}$ search via superheated droplet; require ${{\mathit \sigma}}$(SD) $<$ $0.0132$ pb for m(WIMP) = 20 GeV.
8  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.
9  AMOLE 2016A require SD WIMP-${{\mathit p}}$ scattering $<$ $5 \times 10^{-4}$ pb for $\mathit m$(WIMP) = 20 GeV; bubbles from ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$ target.
10  KHACHATRYAN 2016AJ require SD WIMP-${{\mathit p}}$ $<$ $2 \times 10^{-6}$ pb for $\mathit m$(WIMP) = 20 GeV from ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit Z}}$ + $\not E_T$; ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}}{{\overline{\mathit \ell}}}$ signal.
11  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.
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  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.
14  Use a direction-sensitive detector.
15  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.
16  See also AKERIB 2005 .
  References:
ABDELHAMEED 2019
EPJ C79 630 First results on sub-GeV spin-dependent dark matter interactions with$^{7}$Li
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
AGNESE 2018
PR D97 022002 Low-Mass Dark Matter Search with CDMSlite
AKERIB 2017A
PRL 118 251302 Limits on Spin-Dependent WIMP-Nucleon Cross Section Obtained from the Complete LUX Exposure
BEHNKE 2017
ASP 90 85 Final Results of the PICASSO Dark Matter Search Experiment
FU 2017
PRL 118 071301 Spin-Dependent Weakly-Interacting-Massive-Particle-Nucleon Cross Section Limits from First Data of PandaX-II Experiment
AMOLE 2016A
PR D93 061101 Improved Dark Matter Search Results from PICO-2L Run 2
KHACHATRYAN 2016AJ
PR D93 052011 Search for Dark Matter and Unparticles Produced in Association with a ${{\mathit Z}}$ Boson in Proton-Proton Collisions at $\sqrt {s }$ = 8 TeV
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
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
APRILE 2013
PRL 111 021301 Limits on Spin-Dependent WIMP-Nucleon Cross Sections from 225 Live Days of XEENON100 Data
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
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
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
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