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The first part of the thesis is devoted to investigation of important phenomenological
and particle-cosmology-related issues in the context of Type IIB string compactifications.
After undertaking a brief review of (split) supersymmetry in the context
of Beyond Standard Model Physics, we discuss the possibility of realizing “μ-split
SUSY” scenario from a phenomenological model, which we show could be realizable
locally as the large volume limit of a type IIB Swiss-Cheese Calabi-Yau orientifold involving
a mobile space-time filling D3-brane localized at a nearly special Lagrangian
three-cycle embedded in the ”big” divisor (hence the local nature of the model’s realization)
and multiple fluxed stacks of space-time filling D7-branes wrapping the same
“big” divisor. Naturally realizing split-SUSY scenario of N. Arkani-Hamed and S. Dimopoulos
in our model, we show that the mass of one of the Higgs formed by a linear
combination of two Higgs doublets (related to the D3-brane position moduli), can be
produced to be of the order of 125 GeV whereas other Higgs as well as higgsino mass
parameter to be very heavy- the “μ-split SUSY” scenario. The squarks’/sleptons’
(the Wilson line moduli on D7-branes’ world volume) masses also turn out to be very
heavy. Motivated by the fact that the gravitino appears as the Lightest Supersymmetric
Particle (LSP) in our model, we explore the possibility of the gravitino as a
viable cold dark matter candidate by showing its life time to be of the order of or
greater than the age of the universe whereas lifetimes of decays of the co-NLSPs (the
first generation squark/slepton and the lightest neutralino) to the LSP (the gravitino)
turns out to be too short to disturb predictions of Big Bang Nucleosynthesis (BBN).
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Assuming non-thermal gravitino production mechanism, we estimate the gravitino
relic abundance to be around 0.1 by evaluating the neutralino/slepton annihilation
cross sections and hence show that the former satisfies the requirement for a dark
matter candidate. As another testing ground for split-SUSY scenarios, we estimate
Electric Dipole Moment (EDM) of electron/neutron up to two-loops in our model. By
explaining distinct O(1) CP violating phases associated with Wilson line moduli and
position moduli, we show that it is possible to obtain dominant contribution of EDM
of electron/neutron to be around 10−29 esu-cm at two-loop level by including heavy
sfermions and a light Higgs, around 10−27 esu-cm for a two-loop Barr-Zee diagram
involving W boson and SM interaction vertices, eEDM to be around 10−33 esu-cm
at one-loop by including heavy chargino and a light Higgs, and nEDM to be around
10−32 esu-cm at one-loop by including SM fermions and a light Higgs.
In second part of the thesis, we obtain local M-theory uplift of Type IIB background
involving non-compact (resolved) warped deformed conifold and (N) space
time filling D3-branes placed on the singularity of the conifold, (M) D5-branes wrapped
around compact S2, and (Nf ) D7-branes wrapped around non-compact four-cycle via
Strominger-Yau-Zaslow’s mirror symmetry prescription [1]. This work is mainly concerned
with the investigation of hydro/thermodynamical aspects relevant to explain
the behavior of thermal QCD with fundamental quarks, as well as to demonstrate the
thermodynamical stability of the M-theory uplift. The uplift gives a black M3-brane
solution whose near-horizon geometry near !1,2 = 0,"-branches, preserves 1/8 SUSY.
We propose a new MQGP limit corresponding to finite-string-coupling (gs ! 1)-
large-t’Hooft-coupling regime of M-theory in addition to the one discussed in [2]. Interestingly,
we obtain #/s = 1/4" for the uplift and the diffusion constant D ! 1/T
for types IIB/IIA backgrounds in the both limits. The thermodynamical stability
of M-theory uplift is checked by evaluating the D = 11 Euclideanized supergravity
action upto O(R4, |G4|2) term in the two limits, and thereafter showing the positive
sign of specific heat from the finite part of the action. |
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