Scientific credibility and framework details

 Klevex (India) Pvt. Ltd. conducts research focused on the

structure and behavior of ultra-dense astrophysical

objects, with a special emphasis on neutron stars.

Our work uses observational inputs—mass—radius

measurements, density distributions, stability limits,

and phase-transition indicators—and integrates them

into our scientific framework, Dillip's Cosmological

Equations of State (DCEOS). This approach allows us

to model the internal composition of neutron stars,

identify high-density phases such as A=6, and

generate precise plots that appear across this page.

Through DCEOS and the underlying KUTE

mathematical architecture, we analyse how pressure,

energy density, and compressibility evolve across

extreme regimes. The figures displayed here—EOS

curves, structural transitions, central-density

mappings, and compact-star solution tracks—

represent ongoing research aimed at improving the

predictability of neutron-star physics and advancing

next- eneration cosmolo ical modellin