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	<title>black hole thermodynamics in modified gravity &#8211; Science</title>
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	<title>black hole thermodynamics in modified gravity &#8211; Science</title>
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		<title>Iyer–Wald Approach Links Generalized Entropy to Modified Gravity</title>
		<link>https://scienmag.com/iyer-wald-approach-links-generalized-entropy-to-modified-gravity/</link>
		
		<dc:creator><![CDATA[Grant Pearson]]></dc:creator>
		<pubDate>Wed, 21 Oct 2026 20:02:15 +0000</pubDate>
				<category><![CDATA[Space]]></category>
		<category><![CDATA[black hole entropy]]></category>
		<category><![CDATA[black hole thermodynamics in modified gravity]]></category>
		<category><![CDATA[cosmology]]></category>
		<category><![CDATA[curvature-dependent Lagrangian]]></category>
		<category><![CDATA[entropic exponent index]]></category>
		<category><![CDATA[entropy in alternative gravity theories]]></category>
		<category><![CDATA[f(R) gravity]]></category>
		<category><![CDATA[general relativity]]></category>
		<category><![CDATA[generalized]]></category>
		<category><![CDATA[generalized black hole entropy]]></category>
		<category><![CDATA[GRAVITY]]></category>
		<category><![CDATA[gravity-entropy connection]]></category>
		<category><![CDATA[horizon thermodynamics]]></category>
		<category><![CDATA[Iyer–Wald approach]]></category>
		<category><![CDATA[Iyer–Wald method]]></category>
		<category><![CDATA[modified gravity]]></category>
		<category><![CDATA[Schwarzschild black holes]]></category>
		<category><![CDATA[spherically symmetric vacuum]]></category>
		<category><![CDATA[spherically symmetric vacuum solutions]]></category>
		<category><![CDATA[theoretical black hole entropy models]]></category>
		<category><![CDATA[theory]]></category>
		<category><![CDATA[thermodynamic instability]]></category>
		<guid isPermaLink="false">https://scienmag.com/?p=330451</guid>

					<description><![CDATA[A theoretical analysis reconstructs generalized black-hole horizon entropy from a modified curvature Lagrangian within spherically symmetric vacuum solutions.]]></description>
										<content:encoded><![CDATA[<p>A theoretical study finds that generalized mass-to-horizon entropy for black holes can be reconstructed within modified <span class="math-inline">f(R)</span> gravity using the Iyer–Wald approach. The analysis considers spherically symmetric vacuum solutions with constant curvature in the massive branch of the theory and identifies a generalized Lagrangian proportional to <span class="math-inline">R^{1+\epsilon}</span>, where <span class="math-inline">\epsilon=(n-1)/2</span> measures departures from the standard formulation of general relativity.</p>
<p>The paper studies the gravitational basis of a generalized entropy description characterized by an entropic exponent index <span class="math-inline">n</span> and a multiplicative parameter <span class="math-inline">\gamma</span>. Applying the Iyer–Wald method in modified <span class="math-inline">f(R)</span> gravity, the authors show that the generalized mass-to-horizon entropy can be recovered from the specified curvature-dependent Lagrangian. The relation between the Lagrangian structure and the entropic exponent provides the central mathematical result of the work.</p>
<p>The finding is a formal connection between a class of modified-gravity solutions and the thermodynamic description of black-hole horizons. It is not an observational result and does not establish that a particular black hole in nature has a measured entropy beyond the standard general-relativistic treatment. The analysis is limited to the stated spherically symmetric vacuum configurations with constant curvature in the massive branch, so its conclusions should not be treated as a general demonstration for all black holes, gravitational fields or modified-gravity models.</p>
<p>The authors also discuss possible implications for cosmology and for the thermodynamic instability of Schwarzschild black holes. Those implications are presented as prospects within the theoretical framework; the supplied research summary does not report a new observation or demonstrate that the instability has been experimentally resolved. Overall, the work shows how an Iyer–Wald entropy calculation in modified <span class="math-inline">f(R)</span> gravity can reproduce generalized mass-to-horizon entropy under its stated assumptions, while leaving the broader physical consequences unresolved.</p>
<p><strong>Subject of Research:</strong> Generalized black-hole horizon entropy in modified f(R) gravity using the Iyer–Wald approach</p>
<p><strong>Article Title:</strong> Gravity theory of the generalized mass-to-horizon entropy: the Iyer–Wald approach</p>
<p><strong>Article References:</strong> Mondal, S., &amp; Choudhuri, A. (2026). Gravity theory of the generalized mass-to-horizon entropy: the Iyer–Wald approach. <em>General Relativity and Gravitation, 58</em>(10), Article 122. <a href="https://doi.org/10.1007/s10714-026-03625-z" rel="noopener noreferrer">https://doi.org/10.1007/s10714-026-03625-z</a></p>
<p><strong>Image Credits:</strong> AI Generated</p>
<p><strong>DOI:</strong> <a href="https://doi.org/10.1007/s10714-026-03625-z" rel="noopener noreferrer">10.1007/s10714-026-03625-z</a></p>
<p><strong>Keywords:</strong> black hole entropy, modified gravity, f(R) gravity, Iyer–Wald method, general relativity, Schwarzschild black holes, thermodynamic instability, spherically symmetric vacuum, cosmology, Gravity, theory, generalized</p>
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