SUSY with vanishing vacuum energy. The experimental data indeed indicates a near-flatness of the present universe [@WMAP3] with a vanishingly small vacuum energy. Simple model like no-scale supergravity scenario can give plausible explanation for nearly vanishing vacuum energy. However these models have limitations to produce viable susy phenomenology at low energies($\sim$TeV) [@noscale1; @noscale2]. Therefore the search for a near-Minkowski/de-Sitter vacua has attracted considerable interest in recent years. In this regard various supergravity and string motivated models generating de-Sitter vacua at the TeV scale have been proposed [@KKLT; @Maldacena; @choi; @vempati; @susskind; @KKLT2; @Copeland; @Douglas; @Blumenhagen; @Burgess; @Douglas2; @Bertolini; @Mambrini; @Yoshioka; @Watson; @Misra]. Substantial progress have been made in this direction by a model developed in 2003[@KKLT] in the context of string theory known as the KKLT model. This was followed by a plethora of propositions [@choi; @KKLT2; @Copeland; @Blumenhagen; @ArkhaniHamed; @Burgess; @Douglas2; @Bertolini; @Mambrini]which revolve around building an effective description of low energy physics through a superpotential generated by background fluxes and a convenient choice of Kähler potential motivated by a suitable compactification scheme arising in String/M-Theory.\
In this backdrop we address the following question in the present article :

-   What are the general set of criteria that the 