A supersymmetric Model for Mixed Dark Matter

Author(s):  
Antonio Riotto
2006 ◽  
Vol 73 (11) ◽  
Author(s):  
Durmuş A. Demir ◽  
Mariana Frank ◽  
Ismail Turan

2017 ◽  
Vol 32 (38) ◽  
pp. 1750210 ◽  
Author(s):  
R. Sahu ◽  
V. K. B. Kota

The event detection rates for the Weakly Interacting Massive Particles (WIMP) (a dark matter candidate) are calculated with [Formula: see text]Ge as the detector. The calculations are performed within the deformed shell model (DSM) based on Hartree–Fock states. First, the energy levels and magnetic moment for the ground state and two low-lying positive parity states for this nucleus are calculated and compared with experiment. The agreement is quite satisfactory. Then the nuclear wave functions are used to investigate the elastic and inelastic scattering of WIMP from [Formula: see text]Ge; inelastic scattering, especially for the [Formula: see text] transition, is studied for the first time. The nuclear structure factors which are independent of supersymmetric model are also calculated as a function of WIMP mass. The event rates are calculated for a given set of nucleonic current parameters. The calculation shows that [Formula: see text]Ge is a good detector for detecting dark matter.


2013 ◽  
Vol 111 (5) ◽  
Author(s):  
Rouzbeh Allahverdi ◽  
Bhaskar Dutta ◽  
Rabindra N. Mohapatra ◽  
Kuver Sinha

2010 ◽  
Vol 2010 (12) ◽  
Author(s):  
Koji Ishiwata ◽  
Shigeki Matsumoto ◽  
Takeo Moroi

1991 ◽  
Vol 355 (1) ◽  
pp. 192-207 ◽  
Author(s):  
Keith A. Olive ◽  
David Thomas

2021 ◽  
Vol 2021 (10) ◽  
Author(s):  
Mariana Frank ◽  
Yaşar Hiçyılmaz ◽  
Subhadeep Mondal ◽  
Özer Özdal ◽  
Cem Salih Ün

Abstract We attribute deviations of the muon and electron magnetic moments from the theoretical predictions to the presence of an additional U(1)′ supersymmetric model. We interpret the discrepancies between the muon and electron anomalous magnetic moments to be due to the presence of non-universal U(1)′ charges. In a minimally extended model, we show that requiring both deviations to be satisfied imposes constraints on the spectrum of the model, in particular on dark matter candidates and slepton masses and ordering. Choosing three benchmarks with distinct dark matter features, we study implications of the model at colliders, concentrating on variables that can distinguish our non-universal scenario from other U(1)′ implementations.


2012 ◽  
Vol 2012 (1) ◽  
Author(s):  
J. N. Esteves ◽  
J. C. Romao ◽  
M. Hirsch ◽  
W. Porod ◽  
F. Staub ◽  
...  

2022 ◽  
Vol 2022 (1) ◽  
Author(s):  
Sebastian Baum ◽  
Marcela Carena ◽  
Nausheen R. Shah ◽  
Carlos E. M. Wagner

Abstract A new measurement of the muon anomalous magnetic moment, gμ− 2, has been reported by the Fermilab Muon g-2 collaboration and shows a 4.2 σ departure from the most precise and reliable calculation of this quantity in the Standard Model. Assuming that this discrepancy is due to new physics, we concentrate on a simple supersymmetric model that also provides a dark matter explanation in a previously unexplored region of supersymmetric parameter space. Such interesting region can realize a Bino-like dark matter candidate compatible with all current direct detection constraints for small to moderate values of the Higgsino mass parameter |μ|. This in turn would imply the existence of light additional Higgs bosons and Higgsino particles within reach of the high-luminosity LHC and future colliders. We provide benchmark scenarios that will be tested in the next generation of direct dark matter experiments and at the LHC.


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