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		<summary type="html">&lt;p&gt;Repair Quantum Collection B backlink template&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Quantum book backlink|Advanced and frontier topics}}&lt;br /&gt;
The holographic principle was motivated by the discovery that black hole entropy is proportional to the area of the event horizon rather than the volume:&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
S \propto A.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
This suggests that the fundamental degrees of freedom of a region scale with its boundary, not its interior.&amp;lt;ref&amp;gt;{{cite journal |last=Susskind |first=Leonard |title=The World as a Hologram |journal=Journal of Mathematical Physics |year=1995}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
[[File:Holografisch principe_ Informatie en volume.jpg|thumb|400px|Holographic principle: information in a volume encoded on its boundary surface.]]&lt;br /&gt;
==Origin==&lt;br /&gt;
=== Basic idea ===&lt;br /&gt;
&lt;br /&gt;
The principle states that a physical theory in a volume can be equivalently described by a theory defined on its boundary.&lt;br /&gt;
&lt;br /&gt;
This is analogous to a hologram, where a two-dimensional surface encodes a three-dimensional image.&lt;br /&gt;
&lt;br /&gt;
In this sense, spacetime itself may be an emergent phenomenon.&lt;br /&gt;
&lt;br /&gt;
=== AdS/CFT correspondence ===&lt;br /&gt;
&lt;br /&gt;
The most concrete realization of the holographic principle is the AdS/CFT correspondence.&lt;br /&gt;
&lt;br /&gt;
It states that:&lt;br /&gt;
&lt;br /&gt;
* a gravitational theory in anti-de Sitter (AdS) space  &lt;br /&gt;
* is equivalent to a conformal field theory (CFT) on its boundary  &lt;br /&gt;
&lt;br /&gt;
This duality provides a powerful tool for studying quantum gravity and strongly interacting systems.&amp;lt;ref&amp;gt;{{cite journal |last=Maldacena |first=Juan |title=The Large N Limit of Superconformal Field Theories and Supergravity |journal=Advances in Theoretical and Mathematical Physics |year=1998}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Information and entropy ===&lt;br /&gt;
&lt;br /&gt;
The holographic principle implies that the maximum entropy in a region is bounded by its surface area:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
S \le \frac{k c^3 A}{4 G \hbar}.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This bound is known as the &amp;#039;&amp;#039;&amp;#039;Bekenstein bound&amp;#039;&amp;#039;&amp;#039;.&lt;br /&gt;
&lt;br /&gt;
It places a fundamental limit on the amount of information that can be stored in a given region of space.&lt;br /&gt;
&lt;br /&gt;
=== Physical significance ===&lt;br /&gt;
&lt;br /&gt;
The holographic principle:&lt;br /&gt;
&lt;br /&gt;
* suggests spacetime may be emergent,  &lt;br /&gt;
* connects gravity with quantum information,  &lt;br /&gt;
* provides insight into black hole physics,  &lt;br /&gt;
* plays a central role in modern quantum gravity.  &lt;br /&gt;
&lt;br /&gt;
=See also=&lt;br /&gt;
{{#invoke:PhysicsQC|tocHeadingAndList|Physics:Quantum basics/See also}}&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
{{reflist|3}}&lt;br /&gt;
&lt;br /&gt;
{{Author|Harold Foppele}}&lt;br /&gt;
&lt;br /&gt;
{{Sourceattribution|Quantum Holographic principle|1}}&lt;/div&gt;</summary>
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