scholarly journals Solar and Atmospheric Neutrinos: Limitations for Direct Dark Matter Searches

2012 ◽  
Vol 229-232 ◽  
pp. 536 ◽  
Author(s):  
A. Gütlein ◽  
W. Potzel
Keyword(s):  
Dark Matter ◽  
Solar And Atmospheric Neutrinos ◽  
Atmospheric Neutrinos ◽  
Direct Dark Matter

scholarly journals Solar and atmospheric neutrinos: Background sources for the direct dark matter searches

2010 ◽  
Vol 34 (2) ◽  
pp. 90-96 ◽  
Author(s):  
A. Gütlein ◽  
C. Ciemniak ◽  
F. von Feilitzsch ◽  
N. Haag ◽  
M. Hofmann ◽  
...  
Keyword(s):  
Dark Matter ◽  
Solar And Atmospheric Neutrinos ◽  
Atmospheric Neutrinos ◽  
Direct Dark Matter

scholarly journals Reconciling dark matter, solar and atmospheric neutrinos

1993 ◽  
Vol 406 (1-2) ◽  
pp. 409-422 ◽  
Author(s):  
J.T. Peltoniemi ◽  
J.W.F. Valle
Keyword(s):  
Dark Matter ◽  
Solar And Atmospheric Neutrinos ◽  
Atmospheric Neutrinos

scholarly journals Dark atom solution for the puzzles of direct dark matter search

2021 ◽  
Author(s):  
Timur Bikbaev ◽  
Maxim Khlopov ◽  
Andrey Mayorov
Keyword(s):  
Dark Matter ◽  
Dark Matter Search ◽  
Direct Dark Matter

scholarly journals Global interpretation of direct Dark Matter searches after CDMS-II results

2010 ◽  
Vol 2010 (02) ◽  
pp. 014-014 ◽  
Author(s):  
Joachim Kopp ◽  
Thomas Schwetz ◽  
Jure Zupan
Keyword(s):  
Dark Matter ◽  
Direct Dark Matter

Halo-independent analysis of direct dark matter detection through electron scattering

2021 ◽  
Vol 2021 (12) ◽  
pp. 048
Author(s):  
Muping Chen ◽  
Graciela B. Gelmini ◽  
Volodymyr Takhistov
Keyword(s):  
Dark Matter ◽  
Direct Detection ◽  
Dark Matter Halo ◽  
Dark Halo ◽  
Sufficient Energy ◽  
Independent Analysis ◽  
Dark Matter Detection ◽  
Dark Matter Scattering ◽  
Matter Detection ◽  
Direct Dark Matter

Abstract Sub-GeV mass dark matter particles whose collisions with nuclei would not deposit sufficient energy to be detected, could instead be revealed through their interaction with electrons. Analyses of data from direct detection experiments usually require assuming a local dark matter halo velocity distribution. In the halo-independent analysis method, properties of this distribution are instead inferred from direct dark matter detection data, which allows then to compare different data without making any assumption on the uncertain local dark halo characteristics. This method has so far been developed for and applied to dark matter scattering off nuclei. Here we demonstrate how this analysis can be applied to scattering off electrons.

scholarly journals Experiments on lepton and baryon stability and oscillation phenomena

1982 ◽  
Vol 304 (1482) ◽  
pp. 105-134 ◽  
Keyword(s):  
Neutrino Mass ◽  
Neutrino Oscillations ◽  
Nuclear Reactors ◽  
Solar And Atmospheric Neutrinos ◽  
High Energy ◽  
Lepton Number ◽  
Atmospheric Neutrinos ◽  
Nucleon Decay ◽  
Number Conservation ◽  
Experimental Approaches

The various experiments on lepton number conservation and on nucleon stability currently being done or prepared are reviewed, and their relative merits compared and discussed. The first part of the paper is devoted to the measurement of the neutrino mass and to the present limits on the conservation of the total lepton number and of the various lepton flavours. The existing results and future projects on the strictly connected problems of neutrino oscillations at nuclear reactors, pion factories and high energy accelerators will be also discussed, together with oscillations of solar and atmospheric neutrinos. The second part of the paper concerns the few results and the m any planned detectors on nucleon decay with particular emphasis on the problems of background radioactivity and of the variety of experimental approaches. Oscillation experiments on neutron—antineutron oscillations at nuclear reactors are also considered.

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