DAMA/LIBRA–phase2 results and implications on several dark matter scenarios

The first DAMA/LIBRA–phase2 model-independent results (exposure: [Formula: see text], and software energy threshold at 1 keV). They further confirm — with high confidence level — the evidence already observed by DAMA/NaI and DAMA/LIBRA–phase1 on the basis of the exploited model-independent dark matter (DM) annual modulation signature. The total exposure of the three experiments above the 2 keV software energy threshold is [Formula: see text]. Here, several DM candidate particles and related scenarios are analyzed including the latest results. Thanks to the increased exposure and to the lower software energy threshold, corollary model-dependent analyses permit to significantly restrict the allowed regions for the parameters spaces of various dark matter candidates and astrophysical, particle and nuclear physics scenarios.

[1]  Vitaly Beylin,et al.  Hadronic and Hadron-Like Physics of Dark Matter , 2019, Symmetry.

[2]  G. Tomar,et al.  Probing DAMA/LIBRA data in the full parameter space of WIMP effective models of inelastic scattering , 2019, Physical Review D.

[3]  Jong-Hyun Yoon,et al.  Proton-philic spin-dependent inelastic dark matter as a viable explanation of DAMA/LIBRA-phase2 , 2018, Physical Review D.

[4]  K. Freese,et al.  Dark Matter implications of DAMA/LIBRA-phase2 results , 2018, Physics Letters B.

[5]  Cambridge,et al.  SHM$^{++}$: A Refinement of the Standard Halo Model for Dark Matter Searches , 2018, 1810.11468.

[6]  A. Mattei,et al.  First results from DAMA/LIBRA–phase2 , 2018, Nuclear and Particle Physics Proceedings.

[7]  A. Mattei,et al.  First Model Independent Results from DAMA/LIBRA–Phase2 , 2018, Universe.

[8]  A. Mattei,et al.  First model independent results from DAMA/LIBRA-phase2 , 2018, Nuclear Physics and Atomic Energy.

[9]  Jong-Hyun Yoon,et al.  DAMA/LIBRA-phase2 in WIMP effective models , 2018, Journal of Cosmology and Astroparticle Physics.

[10]  F. Kahlhoefer,et al.  Model-independent comparison of annual modulation and total rate with direct detection experiments , 2018, Journal of Cosmology and Astroparticle Physics.

[11]  A. Green Astrophysical uncertainties on the local dark matter distribution and direct detection experiments , 2017, 1703.10102.

[12]  Z. Berezhiani,et al.  DAMA annual modulation and mirror Dark Matter , 2017, 1701.08590.

[13]  Z. Berezhiani,et al.  DAMA annual modulation effect and asymmetric mirror matter , 2015, 1507.04317.

[14]  Univ. Jing Gangshan,et al.  No role for neutrons, muons and solar neutrinos in the DAMA annual modulation results , 2014, 1409.3516.

[15]  Univ. Jing Gangshan,et al.  Final model independent result of DAMA/LIBRA–phase1 , 2013, 1308.5109.

[16]  Univ. Jing Gangshan,et al.  DARK MATTER INVESTIGATION BY DAMA AT GRAN SASSO , 2013, 1306.1411.

[17]  P. Prosposito,et al.  Performances of the new high quantum efficiency PMTs in DAMA/LIBRA , 2012 .

[18]  R. Wang,et al.  No role for muons in the DAMA annual modulation results , 2012, 1202.4179.

[19]  R. Cerulli,et al.  Observations of annual modulation in direct detection of relic particles and light neutralinos , 2011, 1106.4667.

[20]  R. Lang,et al.  Effect of thallium impurities in the DAMA experiment on the allowed parameter space for inelastic dark matter. , 2011, Physical review letters.

[21]  R. Lang,et al.  Impure Thoughts on Inelastic Dark Matter , 2010, 1007.2688.

[22]  P. Belli,et al.  New results from DAMA/LIBRA , 2010, 1002.1028.

[23]  V. Tretyak,et al.  Semi-empirical calculation of quenching factors for ions in scintillators , 2009, 0911.3041.

[24]  D. Finkbeiner,et al.  Inelastic dark matter and DAMA/LIBRA: An experimentum crucis , 2009, 0906.0002.

[25]  G. Bregar,et al.  Does dark matter consist of baryons of new stable family quarks , 2008, 0907.0196.

[26]  Univ. Jing Gangshan,et al.  First results from DAMA/LIBRA and the combined results with DAMA/NaI , 2008, 0804.2741.

[27]  Univ. Jing Gangshan,et al.  The DAMA/LIBRA apparatus , 2008, 0804.2738.

[28]  Univ. Jing Gangshan,et al.  INVESTIGATION ON LIGHT DARK MATTER , 2008, 0802.4336.

[29]  Univ.,et al.  Investigating electron interacting dark matter , 2007, 0712.0562.

[30]  Yehui Zhang,et al.  Possible implications of the channeling effect in NaI(Tl) crystals , 2007, 0710.0288.

[31]  Investigating halo substructures with annual modulation signature , 2006, astro-ph/0604303.

[32]  H. Newberg,et al.  A dark matter stream through the solar neighborhood , 2005 .

[33]  N. Weiner,et al.  Status of inelastic dark matter , 2004, hep-ph/0402065.

[34]  H. Newberg,et al.  Detectability of weakly interacting massive particles in the Sagittarius dwarf tidal stream , 2003, astro-ph/0309279.

[35]  Univ.,et al.  DARK MATTER PARTICLES IN THE GALACTIC HALO: RESULTS AND IMPLICATIONS FROM DAMA/NaI , 2004, astro-ph/0501412.

[36]  F. Ling,et al.  Diurnal and annual modulation of cold dark matter signals , 2004, astro-ph/0405231.

[37]  H. Newberg,et al.  Effects of the Sagittarius dwarf tidal stream on dark matter detectors. , 2003, Physical review letters.

[38]  Univ.,et al.  Dark matter search , 2003, astro-ph/0307403.

[39]  R. Cerulli,et al.  Effect of the galactic halo modeling on the DAMA/NaI annual modulation result: an extended analysis of the data for WIMPs with a purely spin-independent coupling , 2002, hep-ph/0203242.

[40]  J. Ma,et al.  Investigating the DAMA annual modulation data in the framework of inelastic dark matter , 2002 .

[41]  J. Ma,et al.  Investigating the DAMA annual modulation data in a mixed coupling framework , 2001 .

[42]  N. Weiner,et al.  Inelastic dark matter , 2001, hep-ph/0101138.

[43]  P. Gondolo,et al.  WIMP Annual Modulation with Opposite Phase in Late-Infall Halo Models , 2000, hep-ph/0012315.

[44]  P. Belli,et al.  Extending the DAMA annual-modulation region by inclusion of the uncertainties in astrophysical velocities , 1999, hep-ph/9903501.

[45]  Mario Pillon,et al.  New limits on WIMP search with large-mass low-radioactivity NaI(Tl) set-up at Gran Sasso , 1996 .

[46]  J. D. Lewin,et al.  Review of mathematics, numerical factors, and corrections for dark matter experiments based on elastic nuclear recoil , 1996 .

[47]  Richard H. Helm,et al.  Inelastic and Elastic Scattering of 187-Mev Electrons from Selected Even-Even Nuclei , 1956 .