A survey of the mSUGRA/CMSSM parameter space is presented .
The viable regions of the parameter space which satisfy standard experimental constraints are identified and discussed .
These constraints include a 124 - 127 GeV mass for the lightest CP-even Higgs and the correct relic density for cold dark matter ( CDM ) .
The superpartner spectra corresponding to these regions fall within the well-known hyperbolic branch ( HB ) and are found to possess sub-TeV neutralinos and charginos , with mixed Bino/Higgsino LSP ’ s with 200 - 800 GeV masses .
In addition , the models possess \sim 3 - 4 TeV gluino masses and heavy squarks and sleptons with masses m _ { \tilde { q } } , m _ { \tilde { l } } > m _ { \tilde { g } } .
Spectra with a Higgs mass m _ { h } \cong 125 GeV and a relic density 0.105 \leq \Omega _ { \chi ^ { 0 } } h ^ { 2 } \leq 0.123 are found to require EWFT at around the one-percent level , while those spectra with a much lower relic density require EWFT of only a few percent .
Moreover , the SI neutralino-proton direct detection cross-sections are found to be below or within the XENON100 2 \sigma limit and should be experimentally accessible now or in the near future .
Finally , it is pointed-out that the supersymmetry breaking soft terms corresponding to these regions of the mSUGRA/CMSSM parameter space ( m _ { 0 } \propto m _ { 1 / 2 } with m _ { 0 } ^ { 2 } > > m _ { 1 / 2 } ^ { 2 } and A _ { 0 } = - m _ { 1 / 2 } ) may be obtained from general flux-induced soft terms in Type IIB flux compactifications with D3 branes .