scholarly journals Gaugino mass nonuniversality and dark matter in supergravity, strings, and D-brane models

2001 ◽  
Vol 64 (12) ◽  
Author(s):  
Achille Corsetti ◽  
Pran Nath
2006 ◽  
Vol 2006 (04) ◽  
pp. 041-041 ◽  
Author(s):  
Howard Baer ◽  
Azar Mustafayev ◽  
Eun-Kyung Park ◽  
Stefano Profumo ◽  
Xerxes Tata
Keyword(s):  

2014 ◽  
Vol 2014 (2) ◽  
Author(s):  
Joydeep Chakrabortty ◽  
Subhendra Mohanty ◽  
Soumya Rao
Keyword(s):  

2017 ◽  
Vol 32 (15) ◽  
pp. 1740002 ◽  
Author(s):  
Andrea Addazi ◽  
Maxim Yu. Khlopov

We review our recent results on dark matter from Starobinsky supergravity. In this context, a natural candidate for cold dark matter is the gravitino. On the other hand, assuming the supersymmetry broken at scales much higher than the electroweak scale, gravitinos are superheavy particles. In this case, they may be non-thermally produced during inflation, in turn originated by the scalaron field with Starobinsky’s potential. Assuming gravitinos as Lightest Supersymmetric Particles (LSSP), the non-thermal production naturally accounts for the right amount of cold dark matter. Metastability of the gravitino LSSP leads to observable effects of their decay, putting constraints on the corresponding Unstable or Decaying Dark Matters scenarios. In this model, the gravitino mass is controlled by the inflaton field and it runs with it. This implies that a continuous spectrum of superheavy gravitinos is produced during the slow-roll epoch. Implications in phenomenology, model building in Grand Unified Theory (GUT) scenarios, intersecting D-brane models and instantons in string theories are discussed.


2009 ◽  
Vol 79 (9) ◽  
Author(s):  
Utpal Chattopadhyay ◽  
Debottam Das ◽  
D. P. Roy
Keyword(s):  

2007 ◽  
Vol 2007 (10) ◽  
pp. 088-088 ◽  
Author(s):  
Howard Baer ◽  
Azar Mustafayev ◽  
Heaya Summy ◽  
Xerxes Tata
Keyword(s):  

2015 ◽  
Vol 91 (3) ◽  
Author(s):  
Manimala Chakraborti ◽  
Utpal Chattopadhyay ◽  
Soumya Rao ◽  
D. P. Roy
Keyword(s):  

2021 ◽  
Vol 81 (6) ◽  
Author(s):  
John Ellis ◽  
Jason L. Evans ◽  
Natsumi Nagata ◽  
Keith A. Olive

AbstractWe explore a missing-partner model based on the minimal SU(5) gauge group with $$\mathbf{75} $$ 75 , $$\mathbf{50} $$ 50 and $$\overline{\mathbf{50 }}$$ 50 ¯ Higgs representations, assuming a super-GUT CMSSM scenario in which soft supersymmetry-breaking parameters are universal at some high scale $$M_{\mathrm{in}}$$ M in above the GUT scale $$M_{\mathrm{GUT}}$$ M GUT . We identify regions of parameter space that are consistent with the cosmological dark matter density, the measured Higgs mass and the experimental lower limit on $$\tau (p \rightarrow K^+ \nu )$$ τ ( p → K + ν ) . These constraints can be satisfied simultaneously along stop coannihilation strips in the super-GUT CMSSM with $$\tan \beta \sim $$ tan β ∼ 3.5–5 where the input gaugino mass $$m_{1/2} \sim $$ m 1 / 2 ∼ 15–25 TeV, corresponding after strong renormalization by the large GUT Higgs representations between $$M_{\mathrm{in}}$$ M in and $$M_{\mathrm{GUT}}$$ M GUT to $$m_{\mathrm{LSP}}, m_{{\tilde{t}}_1} \sim $$ m LSP , m t ~ 1 ∼ 2.5–5 TeV and $$m_{{\tilde{g}}} \sim $$ m g ~ ∼ 13–20 TeV, with the light-flavor squarks significantly heavier. We find that $$\tau (p \rightarrow K^+ \nu ) \lesssim 3 \times 10^{34}$$ τ ( p → K + ν ) ≲ 3 × 10 34  years throughout the allowed range of parameter space, within the range of the next generation of searches with the JUNO, DUNE and Hyper-Kamiokande experiments.


2013 ◽  
Vol 23 ◽  
pp. 335-344
Author(s):  
S. SCOPEL

Light neutralinos implemented in an effective Minimal Supersymmetric extension of the Standard Model at the electroweak scale without requirement of a gaugino-mass unification at a grand unification scale may have a mass around 10 GeV, i.e. in the range of interest for present data of direct search for dark matter particles in the galactic halo. In this talk we discuss the challenges and prospects of searching for them at the Large Hadron Collider.


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