scholarly journals Model independent analysis of MeV scale dark matter. II. Implications from e−e+ colliders and direct detection

2019 ◽  
Vol 100 (7) ◽  
Author(s):  
Debajyoti Choudhury ◽  
Divya Sachdeva
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.


2015 ◽  
Vol 2015 (11) ◽  
pp. 038-038 ◽  
Author(s):  
Graciela B. Gelmini ◽  
Andreea Georgescu ◽  
Paolo Gondolo ◽  
Ji-Haeng Huh

2010 ◽  
Vol 25 (11n12) ◽  
pp. 951-961 ◽  
Author(s):  
CHUNG-LIN SHAN

In this article I review model-independent procedures for extracting properties of Weakly Interacting Massive Particles (WIMPs) from direct Dark Matter detection experiments. Neither prior knowledge about the velocity distribution function of halo Dark Matter particles nor about their mass or cross sections on target nucleus is needed. The unique required information is measured recoil energies from experiments with different detector materials.


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.


2013 ◽  
Vol 2013 (4) ◽  
Author(s):  
Biplob Bhattacherjee ◽  
Debajyoti Choudhury ◽  
Keisuke Harigaya ◽  
Shigeki Matsumoto ◽  
Mihoko M. Nojiri

2020 ◽  
Vol 2020 (10) ◽  
Author(s):  
Tommi Alanne ◽  
Giorgio Arcadi ◽  
Florian Goertz ◽  
Valentin Tenorth ◽  
Stefan Vogl

Abstract We systematically explore the phenomenology of the recently proposed extended dark matter effective field theory (eDMeft), which allows for a consistent effective description of DM scenarios across different energy scales. The framework remains applicable at collider energies and is capable of reproducing the correct relic abundance by including a dynamical mediator particle to the dark sector, while maintaining correlations dictated by gauge invariance in a ‘model-independent’ way. Taking into account present and future constraints from direct- and indirect-detection experiments, from collider searches for missing energy and for scalar resonances in vector-boson, di-jet, and Higgs-pair final states, as well as from the relic abundance as measured by Planck, we determine viable regions in the parameter space, both for scalar and pseudoscalar mediator. In particular, we point out regions where cancellations in the direct-detection cross section appear leading to allowed islands for scalar mediators that could be missed in a naive simplified-model approach, but are present in the full D = 5 effective theory, as well as a general opening of the parameter space due to consistently considering all operators at a given mass dimension. Thus, canonical WIMP-like scenarios can survive even the next generation of direct-detection experiments in different mass regimes, while potentially becoming testable at the high-luminosity LHC.


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