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. • • •
$<30$ 95 1
 2018
CDMS ${}^{}\mathrm {Ge}$
$<0.0132$ 90 2
 2017
PICA ${}^{}\mathrm {C}_{4}{}^{}\mathrm {F}_{10}$
$<5 \times 10^{-4}$ 90 3
 2016 A
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<2 \times 10^{-6}$ 90 4
 2016 AJ
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
 2015
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<1.43 \times 10^{-3}$ 90
 2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<1.42 \times 10^{-4}$ 90
 2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<5 \times 10^{-3}$ 90
 2014
SMPL C$_{2}$ClF$_{5}$
$<0.0129$ 90 5
 2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<0.0317$ 90 6
 2013
X100 ${}^{}\mathrm {Xe}$
$<0.03$ 90
 2012
PICA ${}^{}\mathrm {F}$ (C$_{4}F_{10}$)
$<0.06$ 90
 2012
COUP CF$_{3}$I
$<20$ 90
 2012
DRFT F (CF$_{4}$)
$<7 \times 10^{-3}$
 2012
SMPL C$_{2}$ClF$_{5}$
$<0.15$ 90
 2012
KIMS CsI
$<1 \times 10^{5}$ 90 7
 2011
DMTP F (CF$_{4}$)
$<0.1$ 90 7
 2011
COUP CF$_{3}$I
$<0.015$ 90 8
 2011
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<0.2$ 90
 2009
PICA ${}^{}\mathrm {F}$
$<4$ 90
 2009 A
ZEP3 ${}^{}\mathrm {Xe}$
$<0.6$ 90
 2008 A
XE10 ${}^{}\mathrm {Xe}$
$<100$ 90
 2007
ZEP2 ${}^{}\mathrm {Xe}$
$<1$ 90
 2007 A
KIMS CsI
$<20$ 90 9
 2006
CDMS ${}^{73}\mathrm {Ge}$, ${}^{29}\mathrm {Si}$
$<2$ 90
 2006 A
CNTR F (CaF$_{2}$)
$<0.5$ 90
 2005
NAIA NaI
$<1.5$ 90
 2005
PICA F (C$_{4}F_{10}$)
$<1.5$ 90
 2005
SMPL F (C$_{2}$ClF$_{5}$)
$<35$ 90
 2003
BOLO LiF
$<30$ 90
 2003
BOLO NaF
1  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.
2  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.
3  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.
4  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.
5  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.
6  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.
7  Use a direction-sensitive detector.
8  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.
References:
 AGNESE 2018
PR D97 022002 Low-Mass Dark Matter Search with CDMSlite
 BEHNKE 2017
ASP 90 85 Final Results of the PICASSO Dark Matter Search 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
 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
 APRILE 2014A
ASP 54 11 Analysis of the XENON100 Dark Matter Search Data