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

For ${\boldsymbol m}_{{{\boldsymbol X}^{0}}}$ in GeV range INSPIRE search

We provide here limits fo ${\mathit m}_{{{\mathit X}^{0}}}$ $<$ 5 GeV
VALUE (pb) CL% DOCUMENT ID TECN  COMMENT
• • • We do not use the following data for averages, fits, limits, etc. • • •
$<0.01$ 90 1
ABDELHAMEED
2019A
CRES ${}^{}\mathrm {CaWO}_{4}$
$<5.4 \times 10^{-6}$ 90 2
AGNESE
2019A
SCDM GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<1$ 90 3
AKERIB
2019
LUX light DM on ${}^{}\mathrm {Xe}$ via Migdal/brem effect
$<1 \times 10^{-6}$ 90 4
AMOLE
2019
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<1.6 \times 10^{-3}$ 90 5
APRILE
2019C
XE1T DM on ${}^{}\mathrm {Xe}$
$<1 \times 10^{-7}$ 90 6
APRILE
2019D
XE1T DM on ${}^{}\mathrm {Xe}$
$<0.1$ 90 7
ARMENGAUD
2019
EDEL GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<1.6 \times 10^{3}$ 90 8
KOBAYASHI
2019
XMAS annual modulation ${}^{}\mathrm {Xe}$
$<700$ 90 9
LIU
2019B
CDEX ${}^{}\mathrm {Ge}$; sub-GeV DM via Migdal
$<7 \times 10^{-7}$ 90 10
AGNES
2018
DS50 GeV-scale WIMPs on ${}^{}\mathrm {Ar}$
$<1.5 \times 10^{-5}$ 95 11
AGNESE
2018
SCDM GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<2 \times 10^{-8}$ 90 12
APRILE
2018
XE1T ${}^{}\mathrm {Xe}$, SI
$<4.5 \times 10^{-3}$ 90 13
ARNAUD
2018
NEWS low mass WIMP, ${}^{}\mathrm {Ne}$
$<8 \times 10^{-6}$ 90 14
JIANG
2018
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<3 \times 10^{-5}$ 90 15
YANG
2018
CDEX WIMPs on ${}^{}\mathrm {Ge}$
$<1 \times 10^{-6}$ 90 16
AKERIB
2017
LUX ${}^{}\mathrm {Xe}$
$<100$ 90 17
ANGLOHER
2017A
CRES GeV-scale WIMPs
$<7 \times 10^{-5}$ 90 18
ANGLOHER
2016
CRES ${}^{}\mathrm {CaWO}_{4}$
$<3 \times 10^{-5}$ 90 19
APRILE
2016
X100 ${}^{}\mathrm {Xe}$
$<4.3 \times 10^{-4}$ 90 20
ARMENGAUD
2016
EDE3 GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<7 \times 10^{-5}$ 90 21
HEHN
2016
EDE3 SI WIMP on ${}^{}\mathrm {Ge}$
$<6 \times 10^{-5}$ 90 22
ZHAO
2016
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<1 \times 10^{-4}$ 90 23
AMOLE
2015
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<8 \times 10^{-5}$ 90 24
XIAO
2015
PNDX WIMPs on ${}^{}\mathrm {Xe}$
$<3 \times 10^{-5}$ 90 25
AGNESE
2014
SCDM GeV-scale WIMPs
$<1 \times 10^{-3}$ 90 26
AKERIB
2014
LUX WIMP on ${}^{}\mathrm {Xe}$
$<9 \times 10^{-4}$ 90 27
LI
2013B
TEXO WIMPs on ${}^{}\mathrm {Ge}$
$<3 \times 10^{-4}$ 90 28
ARCHAMBAULT
2012
PICA ${}^{}\mathrm {C}_{4}{}^{}\mathrm {F}_{10}$
$<2 \times 10^{-4}$ 90 29
AALSETH
2011
CGNT GeV WIMPs on ${}^{}\mathrm {Ge}$
$<5 \times 10^{-4}$ 90 30
AHMED
2011B
CDM2 GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<8 \times 10^{-5}$ 90 31
ANGLE
2011
XE10 ${}^{}\mathrm {Xe}$
$<5 \times 10^{-4}$ 90 32
AKERIB
2010
CDM2 WIMPs on ${}^{}\mathrm {Ge}/{}^{}\mathrm {Si}$
1  ABDELHAMEED 2019A search for GeV scale dark matter SI scatter on ${}^{}\mathrm {CaWO}_{4}$; no signal, limits placed in ${{\mathit \sigma}}$ vs. mass plane for m(DM) $\sim{}$ $0.1 - 10$ GeV. The listed limit is for m(DM) = 1 GeV.
2  AGNESE 2019A search for $1.5 - 10$ GeV WIMP scatter on ${}^{}\mathrm {Ge}$ in CDMSlite dataset. Limits set in a likelihood analysis. No signal was observed. Limit reported for m(${{\mathit \chi}}$) = 5 GeV.
3  AKERIB 2019 search for $0.4 - 5$ GeV DM using bremsstrahlung photons and "Migdal" electrons; $1.4 \times 10^{4}$ kg d exposure of liquid ${}^{}\mathrm {Xe}$; constraint ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ 1 pb for m(${{\mathit \chi}}$) = 5 GeV in light scalar mediator model.
4  AMOLE 2019 search for SI WIMP scatter on ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$ in PICO-60 bubble chamber; no signal: set limit for spin independent coupling ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ $1 \times 10^{-6}$ pb for m(${{\mathit \chi}}$) = 5 GeV.
5  APRILE 2019C search for light DM scatter on ${}^{}\mathrm {Xe}$ via atomic excitation, ionization (Migdal effect) or bremsstrahlung; no signal, limits placed in ${{\mathit \sigma}}$ vs. m(DM) plane for m(DM) $\sim{}$ $0.085 - 2$ GeV. The listed limit is for m(DM) = 1 GeV.
6  APRILE 2019D search for light DM scatter on ${}^{}\mathrm {Xe}$ via ionization to probe SI, SD, and ${{\mathit \chi}}{{\mathit e}}$ cross sections; with 22 t d exposure, limits placed in various ${{\mathit \sigma}}$ vs. m(DM) planes. Quoted limit is for m(DM) = 5 GeV.
7  ARMENGAUD 2019 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $0.045 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
8  KOBAYASHI 2019 search for sub-GeV WIMP annual modulation in ${}^{}\mathrm {Xe}$ via brems; no signal; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $0.3 - 1$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 0.5 GeV.
9  LIU 2019B seach for sub-GeV DM using Migdal effect on ${}^{}\mathrm {Ge}$ at CDEX-IB; no signal, require ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ $700$ pb for m(${{\mathit \chi}}$) = 0.1 GeV.
10  AGNES 2018 search for $1.8 - 20$ GeV WIMP SI scatter on ${}^{}\mathrm {Ar}$; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
11  AGNESE 2018 search for GeV scale WIMPs using CDMSlite; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $1.5 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
12  APRILE 2018 search for WIMP scatter on 1 t yr ${}^{}\mathrm {Xe}$; no signal, limits set in ${{\mathit \sigma}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $6 - 1000$ GeV; quoted limit is for m = 6 GeV.
13  ARNAUD 2018 search for low mass WIMP scatter on ${}^{}\mathrm {Ne}$ via SPC at NEWS-G; limits set in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $0.5 - 20$ GeV; quoted limit is for m = 5 GeV.
14  JIANG 2018 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $3 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
15  YANG 2018 search for WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $2 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
16  AKERIB 2017 search for WIMP scatter on ${}^{}\mathrm {Xe}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $5 - 1 \times 10^{5}$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
17  ANGLOHER 2017A search for GeV scale WIMP scatter on ${}^{}\mathrm {Al}_{2}{}^{}\mathrm {O}_{3}$ crystal; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $0.15 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
18  ANGLOHER 2016 search for GeV scale WIMP scatter on ${}^{}\mathrm {CaWO}_{4}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $0.5 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
19  APRILE 2016 search for low mass WIMPs via ionization at XENON100; limits placed in ${{\mathit \sigma}}{}^{SI}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs m(${{\mathit \chi}}$) plane for m $\sim{}$ $3.5 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
20  ARMENGAUD 2016 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
21  HEHN 2016 search for low mass WIMPs via SI scatter on ${}^{}\mathrm {Ge}$ target using profile likelihood analysis; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
22  ZHAO 2016 search for GeV-scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
23  AMOLE 2015 search for WIMP scatter on ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$ in PICO-2L; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 25$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
24  XIAO 2015 search for WIMP scatter on ${}^{}\mathrm {Xe}$ with PandaX-I; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $5 - 100$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
25  AGNESE 2014 search for GeV scale WIMPs SI scatter at SuperCDMS; no signal, limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $3.5 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
26  AKERIB 2014 search for WIMP scatter on ${}^{}\mathrm {Xe}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $5 - 5000$ GeV. Limit given for m(${{\mathit \chi}}$) = 5 GeV.
27  LI 2013B search for WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 100$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
28  ARCHAMBAULT 2012 search for low mass WIMP scatter on ${}^{}\mathrm {C}_{4}{}^{}\mathrm {F}_{10}$; limits set in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $4 - 12$ GeV; quoted limit is for m = 5 GeV.
29  AALSETH 2011 search for GeV-scale SI WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed on ${{\mathit \sigma}}{}^{SI}$( ${{\mathit \chi}}{{\mathit N}}$ ) for m(${{\mathit \chi}}$) $\sim{}$ $3.5 - 100$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
30  AHMED 2011B search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$ in CDMS II; limits placed in ${{\mathit \sigma}^{SD}}$( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $4 - 12$ GeV.
31  ANGLE 2011 search for GeV scale WIMPs in Xenon-10; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$) = 5 GeV.
32  AKERIB 2010 search for WIMP scatter on ${}^{}\mathrm {Ge}/{}^{}\mathrm {Si}$ in CDMS2; limits place in ${{\mathit \sigma}}{}^{SI}({{\mathit \chi}}$N) vs. m(${{\mathit \chi}}$) plane for m~3-100 GeV . Limit given for m(DM)=5 GeV
  References:
ABDELHAMEED 2019A
PR D100 102002 First results from the CRESST-III low-mass dark matter program
AGNESE 2019A
PR D99 062001 Search for Low-Mass Dark Matter with CDMSlite Using a Profile Likelihood Fit
AKERIB 2019
PRL 122 131301 Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data
AMOLE 2019
PR D100 022001 Dark Matter Search Results from the Complete Exposure of the PICO-60 C$_3$F$_8$ Bubble Chamber
APRILE 2019C
PRL 123 241803 Search for Light Dark Matter Interactions Enhanced by the Migdal effect or Bremsstrahlung in XENON1T
APRILE 2019D
PRL 123 251801 Light Dark Matter Search with Ionization Signals in XENON1T
ARMENGAUD 2019
PR D99 082003 Searching for low-mass dark matter particles with a massive Ge bolometer operated above-ground
KOBAYASHI 2019
PL B795 308 Search for sub-GeV dark matter by annual modulation using XMASS-I detector
LIU 2019B
PRL 123 161301 Constraints on Spin-Independent Nucleus Scattering with sub-GeV Weakly Interacting Massive Particle Dark Matter from the CDEX-1B Experiment at the China Jinping Underground Laboratory
AGNES 2018
PRL 121 081307 Low-Mass Dark Matter Search with the DarkSide-50 Experiment
AGNESE 2018
PR D97 022002 Low-Mass Dark Matter Search with CDMSlite
APRILE 2018
PRL 121 111302 Dark Matter Search Results from a One Ton-Year Exposure of XENON1T
ARNAUD 2018
ASP 97 54
JIANG 2018
PRL 120 241301 Limits on Light Weakly Interacting Massive Particles from the First 102.8 kg ${\times}$ day Data of the CDEX-10 Experiment
YANG 2018
CP C42 023002 Limits on light WIMPs with a 1 kg-scale germanium detector at 160 eVee physics threshold at the China Jinping Underground Laboratory
AKERIB 2017
PRL 118 021303 Results from a Search for Dark Matter in the Complete LUX Exposure
ANGLOHER 2017A
EPJ C77 637 Results on MeV-scale Dark Matter from a Gram-Scale Cryogenic Calorimeter Operated above Ground
ANGLOHER 2016
EPJ C76 25 Results on Light Dark Matter Particles with a Low-Threshold CRESST-II Detector
APRILE 2016
PR D94 092001 Low-Mass Dark Matter Search using Ionization Signals in XENON100
ARMENGAUD 2016
JCAP 1605 019 Constraints on Low-Mass WIMPs from the EDELWEISS-III Dark Matter Search
HEHN 2016
EPJ C76 548 Improved EDELWEISS-III Sensitivity for Low-Mass WIMPs using a Profile Likelihood Approach
ZHAO 2016
PR D93 092003 Search of Low-Mass WIMPs with a $\mathit p$-Type Point Contact Germanium Detector in the CDEX-1 Experiment
AMOLE 2015
PRL 114 231302 Dark Matter Search Results from the PICO-2L C$_{3}F_{8}$ Bubble Chamber
XIAO 2015
PR D92 052004 Low-Mass Dark Matter Search Results from full Exposure of the PandaX-I Experiment
AGNESE 2014
PRL 112 241302 Search for Low-Mass Weakly Interacting Massive Particles with SuperCDMS
AKERIB 2014
PRL 112 091303 First Results from the LUX Dark Matter Experiment at the Sanford Underground Research Facility
LI 2013B
PRL 110 261301 Limits on Spin-Independent Couplings of WIMP Dark Matter with a p-Type Point-Contact Germanium Detector
ARCHAMBAULT 2012
PL B711 153 Constraints on Low-Mass WIMP Interactions on ${}^{19}\mathrm {F}$ from PICASSO
AALSETH 2011
PRL 106 131301 Results from a Search for Light-Mass Dark Matter with a $\mathit p$-Type Point Contact Germanium Detector
AHMED 2011B
PRL 106 131302 Results from a Low-Energy Analysis of the CDMS II Germanium Data
ANGLE 2011
PRL 107 051301 Search for Light Dark Matter in XENON10 Data
AKERIB 2010
PR D82 122004 Low-Threshold Analysis of CDMS Shallow-Site Data