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		<title>Classical Gravitation from Quantum Scattering Amplitudes</title>
		<link>https://sagex.org/?p=1293</link>
		
		<dc:creator><![CDATA[Jenna Lane]]></dc:creator>
		<pubDate>Thu, 03 Oct 2019 08:38:36 +0000</pubDate>
				<category><![CDATA[Publications]]></category>
		<category><![CDATA[Gravity]]></category>
		<category><![CDATA[Heavy Black Hole Effective Theory]]></category>
		<category><![CDATA[LIGO]]></category>
		<category><![CDATA[scattering amplitudes]]></category>
		<category><![CDATA[VIRGO]]></category>
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					<description><![CDATA[Written by Kays Haddad. Based on the article &#8216;Heavy Black Hole Effective Theory&#8216;, P. H. Damgaard, K. Haddad, A. Helset, [arXiv.org]. Over a century after its formulation, predictions of Einstein&#8217;s theory of General Relativity, describing gravitational interactions, continue to be verified experimentally. One of the predicted phenomena is gravitational waves (GWs), gravitational radiation emitted when &#8230; <p class="link-more"><a href="https://sagex.org/?p=1293" class="more-link">Continue reading<span class="screen-reader-text"> "Classical Gravitation from Quantum Scattering Amplitudes"</span></a></p>]]></description>
		
		
		
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