Miscellaneous Results from Underground Dark Matter Searches INSPIRE search

VALUE CL% DOCUMENT ID TECN  COMMENT
• • • We do not use the following data for averages, fits, limits, etc. • • •
$<1 \times 10^{-12}$ 90 1
AGUILAR-AREVA..
2017
DMIC ${{\mathit \gamma}^{\,'}}$ on ${}^{}\mathrm {Si}$
2
APRILE
2017
X100 ${}^{}\mathrm {Xe}$
3
APRILE
2017D
X100 ${}^{}\mathrm {Xe}$
4
APRILE
2017H
X100 keV bosonic DM search
5
APRILE
2017K
X100 ${{\mathit \chi}}$ ${{\mathit N}}$ $\rightarrow$ ${{\mathit \chi}^{*}}$ $\rightarrow$ ${{\mathit \chi}}{{\mathit \gamma}}$
$<4 \times 10^{-3}$ 90 6
ANGLOHER
2016A
CRES ${}^{}\mathrm {Ca}{}^{}\mathrm {W}{}^{}\mathrm {O}_{4}$
7
APRILE
2015
X100 Event rate modulation
8
APRILE
2015A
X100 Electron scattering
1  AGUILAR-AREVALO 2017 search for hidden photon DM scatter on ${}^{}\mathrm {Si}$ target CCD; limit kinetic mixing ${{\mathit \kappa}}$ $<$ $1 \times 10^{-12}$ for m = 10 eV.
2  APRILE 2017 search for WIMP-${{\mathit e}}$ annual modulation signal for recoil energy in the $2.0 - 5.8$ keV interval using 4 years data with ${}^{}\mathrm {Xe}$. No significant effect seen.
3  APRILE 2017D set limits on 14 WIMP-nucleon different interaction operators. No deviations found using 225 live days in the $6.6 - 240$ keV recoil energy range.
4  APRILE 2017H search for keV bosonic DM via ${{\mathit e}}$ ${{\mathit \chi}}$ $\rightarrow$ ${{\mathit e}}$ , looking for electronic recoils with 224.6 live days of data and 34 kg of LXe. Limits set on ${{\mathit \chi}}{{\mathit e}}{{\mathit e}}$ coupling for m(${{\mathit \chi}}$) = $8 - 125$ keV.
5  APRILE 2017K search for magnetic inelastic DM via ${{\mathit \chi}}$ ${{\mathit N}}$ $\rightarrow$ ${{\mathit \chi}^{*}}$ $\rightarrow$ ${{\mathit \chi}}{{\mathit \gamma}}$ . Limits set in DM magnetic moment vs. mass splitting plane for two DM masses corresponding to the DAMA/LIBRA best fit values.
6  ANGLOHER 2016A require q${}^{2}$ dependent scattering $<$ $8 \times 10^{-3}$ pb for asymmetric DM $\mathit m$(WIMP) = 3 GeV on ${}^{}\mathrm {Ca}{}^{}\mathrm {W}{}^{}\mathrm {O}_{4}$ target. It uses a local dark matter density of 0.38 GeV/cm${}^{3}$.
7  APRILE 2015 search for periodic variation of electronic recoil event rate in the data between Feb. 2011 and Mar. 2012. No significant modulation is found for periods up to 500 days.
8  APRILE 2015A search for ${{\mathit X}^{0}}$ scattering off electrons. See their Fig. 4 for limits on cross section through axial-vector coupling for ${\mathit m}_{{{\mathit X}^{0}}}$ between 0.6 GeV and 1 TeV. For ${\mathit m}_{{{\mathit X}^{0}}}$ = 2 GeV, $\sigma <$ 60 pb (90$\%$CL) is obtained.
  References:
AGUILAR-AREVALO 2017
PRL 118 141803 First Direct-Detection Constraints on eV-Scale Hidden-Photon Dark Matter with DAMIC at SNOLAB
APRILE 2017D
PR D96 042004 Effective Field Theory Search for High-Energy Nuclear Recoils using the XENON100 Dark Matter Detector
APRILE 2017K
JCAP 1710 039 Search for Magnetic Inelastic Dark Matter with XENON100
APRILE 2017
PRL 118 101101 Search for Electronic Recoil Event Rate Modulation with 4 Years of XENON100 Data
APRILE 2017H
PR D96 122002 Search for Bosonic Super-WIMP Interactions with the XENON100 Experiment
ANGLOHER 2016A
PRL 117 021303 Limits on Momentum-Dependent Asymmetric dark Matter with CRESST-II
APRILE 2015A
SCI 349 851 Exclusion of Leptophilic Dark Matter Models using XENON100 Electronic Recoil Data
APRILE 2015
PRL 115 091302 Search for Event Rate Modulation in XENON100 Electronic Recoil Data