Direction-Sensitive Direct Dark Matter Search
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211School of Astronomy and Space Science, University of Chinese Academy of Sciences, Chaoyang District, Beijing 100864, China 212University of Southampton, Southampton SO17 1BJ, United
This allows usto identify parameter regions satisfying the observed DMrelicdensity, whichare constrainedby indirect detection experiments.Applying thelatest Fermi-LATandH.E.S.S.. data
We analyse all the relevant production processes that contribute to the dark matter relic abundance, and broadly classify them in two different scenarios, a dark matter is primarily
The number of expected events per unit time, the event rate R ∝NTnvσ where, NT=Number of target nuclei per unit mass n = Mρx x=Number density of DM particles of mass Mx v=average
In the present work, we consider the possibility of boosted SIDM where heavier DM annihilates into the lighter one followed by the scattering of the latter off electrons at the XENON1T
However, due to the small mixing between the singlet and doublet fermions, the thermal relic of long-lived fermion doublet gets converted into singlet DM at late epochs, typically
For suitable choices of the model parameters, we show that such interconversion can explain the observed relic abundance when the doublet dark matter component has mass in
To expand the results, next step is to construct the HT-KZ HorizonT-Kazakhstan detector system in order to study the ground-breaking phenomena of the multi-modal signals that possibly
