<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Model Checking | A Quest After Perspectives</title><link>https://iphysresearch.github.io/blog/tag/model-checking/</link><atom:link href="https://iphysresearch.github.io/blog/tag/model-checking/index.xml" rel="self" type="application/rss+xml"/><description>Model Checking</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Thu, 22 Oct 2026 00:00:00 +0000</lastBuildDate><image><url>https://iphysresearch.github.io/blog/media/sharing.png</url><title>Model Checking</title><link>https://iphysresearch.github.io/blog/tag/model-checking/</link></image><item><title>Assessing the consistency of the CPL dark-energy model with cosmological data: Simulation-calibrated neural posterior disagreement</title><link>https://iphysresearch.github.io/blog/mypublication/2026_cpl_dark_energy/</link><pubDate>Thu, 22 Oct 2026 00:00:00 +0000</pubDate><guid>https://iphysresearch.github.io/blog/mypublication/2026_cpl_dark_energy/</guid><description>&lt;p>Calibration uses independent simulated data sets to place posterior disagreement
on a global statistical scale. The observed-data test combines compressed CMB,
DESI and DESY5 measurements.&lt;/p></description></item></channel></rss>