scholarly journals python package for dark matter scattering in dielectric targets

2022 ◽  
Vol 105 (1) ◽  
Author(s):  
Simon Knapen ◽  
Jonathan Kozaczuk ◽  
Tongyan Lin
2021 ◽  
Vol 2021 (12) ◽  
pp. 048
Author(s):  
Muping Chen ◽  
Graciela B. Gelmini ◽  
Volodymyr Takhistov

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.


2010 ◽  
Vol 2010 (01) ◽  
pp. 006-006 ◽  
Author(s):  
Spencer Chang ◽  
Aaron Pierce ◽  
Neal Weiner

2018 ◽  
Vol 98 (12) ◽  
Author(s):  
A. Albert ◽  
R. Alfaro ◽  
C. Alvarez ◽  
R. Arceo ◽  
J. C. Arteaga-Velázquez ◽  
...  

2020 ◽  
Vol 101 (3) ◽  
Author(s):  
Brian Campbell-Deem ◽  
Peter Cox ◽  
Simon Knapen ◽  
Tongyan Lin ◽  
Tom Melia

2014 ◽  
Vol 90 (9) ◽  
Author(s):  
G. Barello ◽  
Spencer Chang ◽  
Christopher A. Newby

2013 ◽  
Vol 2013 (10) ◽  
pp. 032-032 ◽  
Author(s):  
Paolo Gondolo ◽  
Stefano Scopel

2019 ◽  
Author(s):  
Davide Serini ◽  
Francesco Loparco ◽  
Mario Nicola Mazziotta ◽  

2020 ◽  
Vol 80 (12) ◽  
Author(s):  
Chun-Hao Lee ◽  
Chrisna Setyo Nugroho ◽  
Martin Spinrath

AbstractWe present prospects for discovering dark matter scattering in gravitational wave detectors. The focus of this work is on light, particle dark matter with masses below 1 $$\hbox {GeV}/\text {c}^{2}$$ GeV / c 2 . We investigate how a potential signal compares to typical backgrounds like thermal and quantum noise, first in a simple toy model and then using KAGRA as a realistic example. That shows that for a discovery much lighter and cooler mirrors would be needed. We also give some brief comments on space-based experiments and future atomic interferometers.


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