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	<title>Energia de Planck - Histórico de revisões</title>
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		<id>https://wiki.nivel-teorico.com/index.php?title=Energia_de_Planck&amp;diff=5728&amp;oldid=prev</id>
		<title>Calimero0000: uma edição</title>
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		<updated>2013-05-03T11:16:16Z</updated>

		<summary type="html">&lt;p&gt;uma edição&lt;/p&gt;
&lt;p&gt;&lt;b&gt;Página nova&lt;/b&gt;&lt;/p&gt;&lt;div&gt;Em [[física]], a unidade de [[energia]] no sistema de [[unidades naturais]] conhecida como [[unidades de Planck]] é chamada a &amp;#039;&amp;#039;&amp;#039;energia de Planck&amp;#039;&amp;#039;&amp;#039;, notada por &amp;#039;&amp;#039;E&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;P&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;E_p = \sqrt{\frac{\hbar c^5}{G}} \approx&amp;lt;/math&amp;gt; [[1 E9 J|1.956 &amp;amp;times; 10&amp;lt;sup&amp;gt;9&amp;lt;/sup&amp;gt;]] [[Joule|J]] &amp;lt;math&amp;gt;\approx&amp;lt;/math&amp;gt; [[1 E9 J|1.22 &amp;amp;times; 10&amp;lt;sup&amp;gt;19&amp;lt;/sup&amp;gt;]] [[GeV]] &amp;lt;math&amp;gt;\approx&amp;lt;/math&amp;gt; 0.5433 [[Quilowatt-hora|MWh]]&lt;br /&gt;
&lt;br /&gt;
onde &amp;#039;&amp;#039;c&amp;#039;&amp;#039; é a [[velocidade da luz]] no vácuo, &amp;lt;math&amp;gt;\hbar&amp;lt;/math&amp;gt; é a [[constante de Planck]] reduzida, e &amp;#039;&amp;#039;G&amp;#039;&amp;#039; é a [[constante gravitacional]]. &amp;#039;&amp;#039;E&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;P&amp;lt;/sub&amp;gt; é a &amp;#039;&amp;#039;derivada&amp;#039;&amp;#039;, como oposta a &amp;#039;&amp;#039;básica&amp;#039;&amp;#039;, unidade de Planck.&lt;br /&gt;
&lt;br /&gt;
Um definição equivalente é:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;E_p = {\frac{\hbar} {t_P}},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
onde &amp;lt;math&amp;gt;\ t_P&amp;lt;/math&amp;gt; é o [[tempo de Planck]].&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!--&lt;br /&gt;
&lt;br /&gt;
The [[ultra-high-energy cosmic ray]]s observed in [[1991]] had a measured energy of about 50 [[joule]]s, equivalent to about 2.5&amp;amp;times;10&amp;lt;sup&amp;gt;-8&amp;lt;/sup&amp;gt; &amp;#039;&amp;#039;E&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;. Most Planck units are fantastically small and thus are unrelated to &amp;quot;macroscopic&amp;quot; phenomena. One &amp;#039;&amp;#039;E&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;, on the other hand, is definitely macroscopic, approximately equaling the energy of a bolt of lightning, or two weeks&amp;#039; per capita consumption of electricity in the [[United States]] in 2001.{{Citations missing|date=maio 2008}}&lt;br /&gt;
&lt;br /&gt;
Even so, &amp;#039;&amp;#039;E&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; is a meaningful quantity in particle physics when [[gravitation]] is taken into account. The Planck energy is not only the energy needed (in principle) to probe the [[Planck length]], but is probably also the maximum possible energy that can fit into a region of that scale. A sphere 1 [[Planck length]] in diameter, containing 1 unit of Planck energy, will result in a tiny (and very hot) [[black hole]].&lt;br /&gt;
&lt;br /&gt;
Planck units are designed to normalize the [[physical constant]]s &amp;lt;math&amp;gt;\hbar&amp;lt;/math&amp;gt;, &amp;#039;&amp;#039;G&amp;#039;&amp;#039;, and &amp;#039;&amp;#039;c&amp;#039;&amp;#039; to 1. Hence given Planck units, the [[mass-energy equivalence]] &amp;#039;&amp;#039;E&amp;#039;&amp;#039;&amp;amp;nbsp;=&amp;amp;nbsp;&amp;#039;&amp;#039;mc&amp;#039;&amp;#039;² simplifies to &amp;#039;&amp;#039;E&amp;#039;&amp;#039;&amp;amp;nbsp;=&amp;amp;nbsp;&amp;#039;&amp;#039;m&amp;#039;&amp;#039;, so that the Planck energy and mass are numerically identical. In the equations of [[general relativity]], &amp;#039;&amp;#039;G&amp;#039;&amp;#039; is often multiplied by 8π. Hence writings in [[particle physics]] and [[physical cosmology]] often normalize 8π&amp;#039;&amp;#039;G&amp;#039;&amp;#039; to 1. This [[normalization]] results in the &amp;#039;&amp;#039;&amp;#039;reduced Planck energy&amp;#039;&amp;#039;&amp;#039;, defined as:&lt;br /&gt;
:&amp;lt;math&amp;gt;\sqrt{\frac{\hbar{}c^5}{8\pi G}}&amp;lt;/math&amp;gt; &amp;lt;math&amp;gt;\approx&amp;lt;/math&amp;gt; 0.390 &amp;amp;times; 10&amp;lt;sup&amp;gt;9&amp;lt;/sup&amp;gt; J &amp;lt;math&amp;gt;\approx&amp;lt;/math&amp;gt; 2.43 &amp;amp;times; 10&amp;lt;sup&amp;gt;18&amp;lt;/sup&amp;gt; GeV.&lt;br /&gt;
&lt;br /&gt;
 --&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== {{Ver também}} ==&lt;br /&gt;
* [[Unidades de Planck]]&lt;br /&gt;
* [[Constante de Planck]]&lt;br /&gt;
* [[Princípio holográfico]]&lt;br /&gt;
&lt;br /&gt;
{{esboço-física}}&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Energia Planck}}&lt;br /&gt;
[[Categoria:Unidades de medida]]&lt;br /&gt;
[[Categoria:Metrologia]]&lt;/div&gt;</summary>
		<author><name>Calimero0000</name></author>
	</entry>
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