<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Physics-informed AI | Chayan Chatterjee</title><link>https://chayanchatterjee.com/tag/physics-informed-ai/</link><atom:link href="https://chayanchatterjee.com/tag/physics-informed-ai/index.xml" rel="self" type="application/rss+xml"/><description>Physics-informed AI</description><generator>Wowchemy (https://wowchemy.com)</generator><language>en-us</language><lastBuildDate>Fri, 10 Jul 2026 00:00:00 +0000</lastBuildDate><image><url>https://chayanchatterjee.com/media/icon_hu893f8f5c2fd565b3b8f53fe35f6c2a2b_550131_512x512_fill_lanczos_center_3.png</url><title>Physics-informed AI</title><link>https://chayanchatterjee.com/tag/physics-informed-ai/</link></image><item><title>The multimessenger Universe as a training ground for frontier AI</title><link>https://chayanchatterjee.com/publication/multimessenger_ai/</link><pubDate>Fri, 10 Jul 2026 00:00:00 +0000</pubDate><guid>https://chayanchatterjee.com/publication/multimessenger_ai/</guid><description>&lt;p>This Perspective grew out of the 2025 Vanderbilt workshop &amp;ldquo;Multimessenger Astronomy in the Era of Foundational AI&amp;rdquo; and frames multimessenger astronomy as a two-way opportunity: AI can help coordinate observations, accelerate inference and identify anomalies, while physically governed multimessenger data can help test whether frontier AI systems reason reliably about the natural world.&lt;/p>
&lt;table>
&lt;thead>
&lt;tr>
&lt;th style="text-align:center">
&lt;figure >
&lt;div class="d-flex justify-content-center">
&lt;div class="w-100" >&lt;img alt="Fig. 2 from the Nature Astronomy Perspective showing the projected multimessenger astronomy data surge through 2041" srcset="
/publication/multimessenger_ai/featured_hu0c254996f1d8d9249c3682a489af77f5_1469897_3800186b496b6ab78f734acd8dc4b563.webp 400w,
/publication/multimessenger_ai/featured_hu0c254996f1d8d9249c3682a489af77f5_1469897_55198741fe8ce6b54ef36063337631c3.webp 760w,
/publication/multimessenger_ai/featured_hu0c254996f1d8d9249c3682a489af77f5_1469897_1200x1200_fit_q75_h2_lanczos_3.webp 1200w"
src="https://chayanchatterjee.com/publication/multimessenger_ai/featured_hu0c254996f1d8d9249c3682a489af77f5_1469897_3800186b496b6ab78f734acd8dc4b563.webp"
width="760"
height="645"
loading="lazy" data-zoomable />&lt;/div>
&lt;/div>&lt;/figure>
&lt;/th>
&lt;/tr>
&lt;/thead>
&lt;tbody>
&lt;tr>
&lt;td style="text-align:center">&lt;em>Fig. 2: MMA&amp;rsquo;s data surge through 2041. The figure shows projected cumulative spacetime volume across messenger channels and the corresponding growth in observed binary neutron star multimessenger events.&lt;/em>&lt;/td>
&lt;/tr>
&lt;/tbody>
&lt;/table></description></item></channel></rss>