<?xml version="1.0" encoding="UTF-8"?><rss version="2.0"><channel><title>Pardeep Kumar — Research notes</title><description>Notes on numerical methods, scientific computing, and research software.</description><link>https://kumarpardeep.com/</link><language>en</language><item><title>From Einstein’s equations to BSSN and FO-CCZ4</title><link>https://kumarpardeep.com/blog/einstein-equations-bssn-fo-ccz4/</link><guid isPermaLink="true">https://kumarpardeep.com/blog/einstein-equations-bssn-fo-ccz4/</guid><description>Why the covariant field equations are not yet a time-marching algorithm, and how ADM, BSSN, CCZ4, and FO-CCZ4 reorganize spacetime geometry into numerical evolution systems.</description><pubDate>Sat, 18 Jul 2026 10:00:00 GMT</pubDate><category>numerical relativity</category><category>Einstein equations</category><category>BSSN</category><category>CCZ4</category><category>hyperbolic systems</category></item><item><title>A unified model for two-phase transport of CO₂-rich mixtures</title><link>https://kumarpardeep.com/blog/multicomponent-co2-pipeline-transport/</link><guid isPermaLink="true">https://kumarpardeep.com/blog/multicomponent-co2-pipeline-transport/</guid><description>How HEM, a Helmholtz-energy EOS, stability analysis, a reformulated UVN flash, and equilibrium sound speed combine in multicomponent pipeline simulations.</description><pubDate>Sat, 18 Jul 2026 09:00:00 GMT</pubDate><category>multicomponent flow</category><category>CO₂ pipelines</category><category>UVN flash</category><category>Riemann solvers</category><category>speed of sound</category></item><item><title>Solving the multicomponent UVN flash in TVN space</title><link>https://kumarpardeep.com/blog/uvn-flash-in-tvn-space/</link><guid isPermaLink="true">https://kumarpardeep.com/blog/uvn-flash-in-tvn-space/</guid><description>A step-by-step account of stability analysis, entropy maximization, the λ = −1/T result, the Helmholtz Q-function, and why eliminating nested temperature solves matters.</description><pubDate>Sat, 18 Jul 2026 08:00:00 GMT</pubDate><category>UVN flash</category><category>phase stability</category><category>thermodynamic optimization</category><category>Helmholtz energy</category></item><item><title>From four equilibrium equations to one: faster pure-CO₂ depressurization</title><link>https://kumarpardeep.com/blog/reduced-vle-pure-co2/</link><guid isPermaLink="true">https://kumarpardeep.com/blog/reduced-vle-pure-co2/</guid><description>How the saturation curve reduces the pure-component UV flash, how differentiating the constraint yields a temperature ODE, and where the efficiency–conservation trade-off appears.</description><pubDate>Sat, 18 Jul 2026 07:00:00 GMT</pubDate><category>phase equilibrium</category><category>CO₂ depressurization</category><category>differential-algebraic equations</category><category>finite volume methods</category></item><item><title>Why CO₂ pipeline transport is a thermodynamics problem</title><link>https://kumarpardeep.com/blog/co2-pipeline-transport-foundations/</link><guid isPermaLink="true">https://kumarpardeep.com/blog/co2-pipeline-transport-foundations/</guid><description>From CCS infrastructure and phase envelopes to Riemann waves, water hammer, and a proposed CO₂-hammer benchmark: an accessible map of the modelling problem.</description><pubDate>Sat, 18 Jul 2026 06:00:00 GMT</pubDate><category>carbon capture and storage</category><category>CO₂ transport</category><category>multiphase flow</category><category>thermodynamics</category><category>numerical methods</category></item></channel></rss>