scholarly journals Model-independent determination of the WIMP mass from direct dark matter detection data

2008 ◽  
Vol 2008 (06) ◽  
pp. 012 ◽  
Author(s):  
Manuel Drees ◽  
Chung-Lin Shan
2014 ◽  
Vol 29 (05) ◽  
pp. 1450014 ◽  
Author(s):  
Sen Miao ◽  
Chung-Lin Shan ◽  
Yu-Feng Zhou

In this paper, we introduce model-independent data analysis procedures for identifying inelastic WIMP-nucleus scattering as well as for reconstructing the mass and the mass splitting of inelastic WIMPs simultaneously and separately. Our simulations show that, with 𝒪(50) observed WIMP signals from one experiment, one could already distinguish the inelastic WIMP scattering scenarios from the elastic one. By combining two or more data sets with positive signals, the WIMP mass and the mass splitting could even be reconstructed with statistical uncertainties of less than a factor of two.


2011 ◽  
Vol 20 (08) ◽  
pp. 1453-1461 ◽  
Author(s):  
CHUNG-LIN SHAN

We reexamine the model-independent data analysis methods for extracting properties of Weakly Interacting Massive Particles (WIMPs) by using data (measured recoil energies) from direct Dark Matter detection experiments directly and, as a more realistic study, consider a small fraction of residue background events, which pass all discrimination criteria and then mix with other real WIMP-induced signals in the analyzed data sets. In this talk, the effects of residue backgrounds on the determination of the WIMP mass as well as the spin-independent WIMP coupling on nucleons will be discussed.


2008 ◽  
Author(s):  
Manuel Drees ◽  
Chung-Lin Shan ◽  
Pyungwon Ko ◽  
Deog Ki Hong

2018 ◽  
Vol 33 (20) ◽  
pp. 1850120
Author(s):  
Yu Bai ◽  
Weichao Sun ◽  
Chung-Lin Shan

In this paper, we revisit our model-independent methods developed for reconstructing properties of Weakly Interacting Massive Particles (WIMPs) by using measured recoil energies from direct Dark Matter detection experiments directly and take into account more realistically non-negligible threshold energy. All expressions for reconstructing the mass and the (ratios between the) spin-independent and the spin-dependent WIMP–nucleon couplings have been modified. We focus on low-mass ([Formula: see text] GeV) WIMPs and present the numerical results obtained by Monte Carlo simulations. Constraints caused by non-negligible threshold energy and technical treatments for improving reconstruction results will also be discussed.


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.


2017 ◽  
Vol 888 ◽  
pp. 012207
Author(s):  
G. Angloher ◽  
P. Carniti ◽  
L. Cassina ◽  
L. Gironi ◽  
C. Gotti ◽  
...  

2014 ◽  
Vol 2014 (11) ◽  
pp. 002-002 ◽  
Author(s):  
D. Cogollo ◽  
Alma X. Gonzalez-Morales ◽  
Farinaldo S. Queiroz ◽  
P. Rebello Teles

2012 ◽  
Vol 36 (6) ◽  
pp. 505-512 ◽  
Author(s):  
Ya-Zheng Chen ◽  
Jun-Mou Chen ◽  
Yan-An Luo ◽  
Hong Shen ◽  
Xue-Qian Li

Sign in / Sign up

Export Citation Format

Share Document