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	<title>Física clàssica - Historial de revisions</title>
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	<updated>2026-04-14T16:25:34Z</updated>
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	<entry>
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		<title>Jose2 en 18:39 20 dec 2025</title>
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		<updated>2025-12-20T18:39:05Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Revisió anterior&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revisió de 18:39 20 dec 2025&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l3&quot;&gt;Llínea 3:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Llínea 3:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Es denomina &amp;#039;&amp;#039;&amp;#039;física clàssica&amp;#039;&amp;#039;&amp;#039; a la [[física]] basada en els principis previs a l&amp;#039;aparició de la [[mecànica quàntica]]. Inclou l&amp;#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], l&amp;#039;[[electromagnetisme]], l&amp;#039;[[òptica]], l&amp;#039;[[acústica]], la [[dinàmica de fluits]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&amp;#039;estat d&amp;#039;un sistema tancat en el futur depén exclusivament de l&amp;#039;estat del sistema en el moment actual.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Es denomina &amp;#039;&amp;#039;&amp;#039;física clàssica&amp;#039;&amp;#039;&amp;#039; a la [[física]] basada en els principis previs a l&amp;#039;aparició de la [[mecànica quàntica]]. Inclou l&amp;#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], l&amp;#039;[[electromagnetisme]], l&amp;#039;[[òptica]], l&amp;#039;[[acústica]], la [[dinàmica de fluits]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&amp;#039;estat d&amp;#039;un sistema tancat en el futur depén exclusivament de l&amp;#039;estat del sistema en el moment actual.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Algunes voltes, es reserva  la frase nominal &quot;física clàssica&quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que subyacen en la teoria quàntica. Per eixa raó resulta convenient des d&#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Algunes voltes, es reserva  la frase nominal &quot;física clàssica&quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que subyacen en la teoria quàntica. Per eixa raó resulta convenient des d&#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques. &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt; &lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;== Referències ==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;== Referències ==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

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		<author><name>Jose2</name></author>
	</entry>
	<entry>
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		<title>Lluísm en 10:08 16 feb 2023</title>
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		<updated>2023-02-16T10:08:25Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Revisió anterior&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revisió de 10:08 16 feb 2023&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l5&quot;&gt;Llínea 5:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Llínea 5:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Algunes voltes, es reserva  la frase nominal &amp;quot;física clàssica&amp;quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que subyacen en la teoria quàntica. Per eixa raó resulta convenient des d&amp;#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Algunes voltes, es reserva  la frase nominal &amp;quot;física clàssica&amp;quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que subyacen en la teoria quàntica. Per eixa raó resulta convenient des d&amp;#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;== Referències ==&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;*  Barut, Asim O. (1980) [1964]. Introduction to Classical Mechanics. New York: Dover Publications. ISBN 9780486640389&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;* Jaeger, Gregg (September 2014). «What in the (quantum) world is macroscopic?». American Journal of Physics 82 (9): 896-905.Bibcode:2014AmJPh..82..896J. doi:10.1119/1.4878358&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;* Landau &amp;amp; Lifshitz, Teoría clásica de los campos, Ed. Reverté, ISBN 84-291-4082-4&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;* Weidner and Sells, Elementary Modern Physics Preface p.iii, 1968&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;== Bibliografia ==&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;* Feynman, Richard (1996). Six Easy Pieces. Perseus Publishing. ISBN 0-201-40825-2&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;* Feynman, Richard (1999). Lectures on Physics. Perseus Publishing. ISBN 0-7382-0092-1&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;* Landau, L. D.; Lifshitz, E. M. (1972). Mechanics and Electrodynamics 1. Franklin Book Company, Inc. ISBN 0-08-016739-X&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;* Kleppner, D.; Kolenkow, R. J. (1973). , McGraw-Hill, ed. An Introduction to Mechanics. ISBN 0-07-035048-5&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;* M. Alonso, J. Finn. Addison-Wesley, ed. &quot;Fundamental university physics&quot;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;* Robert Martin Eisberg (1961). John Wiley &amp;amp; Sons, ed. Fundamentals of Modern Physics&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Categoria:Física]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Categoria:Física]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-added&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;{{Traduït de|es|Física Clásica}}&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-added&quot;&gt;&lt;/td&gt;&lt;/tr&gt;

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		<author><name>Lluísm</name></author>
	</entry>
	<entry>
		<id>https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=259593&amp;oldid=prev</id>
		<title>Lluísm en 10:03 16 feb 2023</title>
		<link rel="alternate" type="text/html" href="https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=259593&amp;oldid=prev"/>
		<updated>2023-02-16T10:03:28Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Revisió anterior&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revisió de 10:03 16 feb 2023&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l3&quot;&gt;Llínea 3:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Llínea 3:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Es denomina &amp;#039;&amp;#039;&amp;#039;física clàssica&amp;#039;&amp;#039;&amp;#039; a la [[física]] basada en els principis previs a l&amp;#039;aparició de la [[mecànica quàntica]]. Inclou l&amp;#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], l&amp;#039;[[electromagnetisme]], l&amp;#039;[[òptica]], l&amp;#039;[[acústica]], la [[dinàmica de fluits]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&amp;#039;estat d&amp;#039;un sistema tancat en el futur depén exclusivament de l&amp;#039;estat del sistema en el moment actual.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Es denomina &amp;#039;&amp;#039;&amp;#039;física clàssica&amp;#039;&amp;#039;&amp;#039; a la [[física]] basada en els principis previs a l&amp;#039;aparició de la [[mecànica quàntica]]. Inclou l&amp;#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], l&amp;#039;[[electromagnetisme]], l&amp;#039;[[òptica]], l&amp;#039;[[acústica]], la [[dinàmica de fluits]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&amp;#039;estat d&amp;#039;un sistema tancat en el futur depén exclusivament de l&amp;#039;estat del sistema en el moment actual.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Algunes voltes, es reserva  la frase nominal &quot;física clàssica&quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;subyacer &lt;/del&gt;en la teoria quàntica. Per eixa raó resulta convenient des d&#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Algunes voltes, es reserva  la frase nominal &quot;física clàssica&quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;subyacen &lt;/ins&gt;en la teoria quàntica. Per eixa raó resulta convenient des d&#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;

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		<author><name>Lluísm</name></author>
	</entry>
	<entry>
		<id>https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=156483&amp;oldid=prev</id>
		<title>Jose2 en 00:57 16 nov 2019</title>
		<link rel="alternate" type="text/html" href="https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=156483&amp;oldid=prev"/>
		<updated>2019-11-16T00:57:15Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Revisió anterior&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revisió de 00:57 16 nov 2019&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot;&gt;Llínea 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Llínea 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;{{En desenroll}}&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-added&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-added&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Archiu:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&amp;#039;estructura general del sistema solar i l&amp;#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Archiu:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&amp;#039;estructura general del sistema solar i l&amp;#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;

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		<author><name>Jose2</name></author>
	</entry>
	<entry>
		<id>https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=110959&amp;oldid=prev</id>
		<title>Jose2 en 19:05 9 dec 2016</title>
		<link rel="alternate" type="text/html" href="https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=110959&amp;oldid=prev"/>
		<updated>2016-12-09T19:05:54Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Revisió anterior&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revisió de 19:05 9 dec 2016&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l3&quot;&gt;Llínea 3:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Llínea 3:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Archiu:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&amp;#039;estructura general del sistema solar i l&amp;#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Archiu:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&amp;#039;estructura general del sistema solar i l&amp;#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Es denomina &#039;&#039;&#039;física clàssica&#039;&#039;&#039; a la [[física]] basada en els principis previs a l&#039;aparició de la [[mecànica quàntica]]. Inclou l&#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;el  &lt;/del&gt;[[electromagnetisme]], &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;la &lt;/del&gt;[[òptica]], &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;la &lt;/del&gt;[[acústica]], la [[dinàmica de fluits]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&#039;estat d&#039;un sistema tancat en el futur depén exclusivament de l&#039;estat del sistema en el moment actual.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Es denomina &#039;&#039;&#039;física clàssica&#039;&#039;&#039; a la [[física]] basada en els principis previs a l&#039;aparició de la [[mecànica quàntica]]. Inclou l&#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;l&#039;&lt;/ins&gt;[[electromagnetisme]], &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;l&#039;&lt;/ins&gt;[[òptica]], &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;l&#039;&lt;/ins&gt;[[acústica]], la [[dinàmica de fluits]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&#039;estat d&#039;un sistema tancat en el futur depén exclusivament de l&#039;estat del sistema en el moment actual.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Algunes voltes, es reserva  la frase nominal &amp;quot;física clàssica&amp;quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que subyacer en la teoria quàntica. Per eixa raó resulta convenient des d&amp;#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Algunes voltes, es reserva  la frase nominal &amp;quot;física clàssica&amp;quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que subyacer en la teoria quàntica. Per eixa raó resulta convenient des d&amp;#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

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&lt;/table&gt;</summary>
		<author><name>Jose2</name></author>
	</entry>
	<entry>
		<id>https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=109501&amp;oldid=prev</id>
		<title>EirVal en 18:37 23 nov 2016</title>
		<link rel="alternate" type="text/html" href="https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=109501&amp;oldid=prev"/>
		<updated>2016-11-23T18:37:13Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;vlc&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Revisió anterior&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revisió de 18:37 23 nov 2016&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l3&quot;&gt;Llínea 3:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Llínea 3:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Archiu:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&amp;#039;estructura general del sistema solar i l&amp;#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Archiu:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&amp;#039;estructura general del sistema solar i l&amp;#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Es denomina &#039;&#039;&#039;física clàssica&#039;&#039;&#039; a la [[física]] basada en els principis previs a l&#039;aparició de la [[mecànica quàntica]]. Inclou l&#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], el  [[electromagnetisme]], la [[òptica]], la [[acústica]], la [[dinàmica &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;d&#039;@fluido&lt;/del&gt;]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&#039;estat d&#039;un sistema tancat en el futur depén exclusivament de l&#039;estat del sistema en el moment actual.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Es denomina &#039;&#039;&#039;física clàssica&#039;&#039;&#039; a la [[física]] basada en els principis previs a l&#039;aparició de la [[mecànica quàntica]]. Inclou l&#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], el  [[electromagnetisme]], la [[òptica]], la [[acústica]], la [[dinàmica &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;de fluits&lt;/ins&gt;]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&#039;estat d&#039;un sistema tancat en el futur depén exclusivament de l&#039;estat del sistema en el moment actual.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Algunes voltes, es reserva  la frase nominal &amp;quot;física clàssica&amp;quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que subyacer en la teoria quàntica. Per eixa raó resulta convenient des d&amp;#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Algunes voltes, es reserva  la frase nominal &amp;quot;física clàssica&amp;quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que subyacer en la teoria quàntica. Per eixa raó resulta convenient des d&amp;#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

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&lt;/table&gt;</summary>
		<author><name>EirVal</name></author>
	</entry>
	<entry>
		<id>https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=109500&amp;oldid=prev</id>
		<title>EirVal en 18:36 23 nov 2016</title>
		<link rel="alternate" type="text/html" href="https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=109500&amp;oldid=prev"/>
		<updated>2016-11-23T18:36:46Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;vlc&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Revisió anterior&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revisió de 18:36 23 nov 2016&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot;&gt;Llínea 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Llínea 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{En desenroll}}&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{En desenroll}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Archivo&lt;/del&gt;:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&#039;estructura general del sistema solar i l&#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Archiu&lt;/ins&gt;:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&#039;estructura general del sistema solar i l&#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Es denomina &amp;#039;&amp;#039;&amp;#039;física clàssica&amp;#039;&amp;#039;&amp;#039; a la [[física]] basada en els principis previs a l&amp;#039;aparició de la [[mecànica quàntica]]. Inclou l&amp;#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], el  [[electromagnetisme]], la [[òptica]], la [[acústica]], la [[dinàmica d&amp;#039;@fluido]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&amp;#039;estat d&amp;#039;un sistema tancat en el futur depén exclusivament de l&amp;#039;estat del sistema en el moment actual.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Es denomina &amp;#039;&amp;#039;&amp;#039;física clàssica&amp;#039;&amp;#039;&amp;#039; a la [[física]] basada en els principis previs a l&amp;#039;aparició de la [[mecànica quàntica]]. Inclou l&amp;#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], el  [[electromagnetisme]], la [[òptica]], la [[acústica]], la [[dinàmica d&amp;#039;@fluido]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&amp;#039;estat d&amp;#039;un sistema tancat en el futur depén exclusivament de l&amp;#039;estat del sistema en el moment actual.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

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&lt;/table&gt;</summary>
		<author><name>EirVal</name></author>
	</entry>
	<entry>
		<id>https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=109499&amp;oldid=prev</id>
		<title>EirVal en 18:36 23 nov 2016</title>
		<link rel="alternate" type="text/html" href="https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=109499&amp;oldid=prev"/>
		<updated>2016-11-23T18:36:34Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Revisió anterior&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revisió de 18:36 23 nov 2016&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot;&gt;Llínea 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Llínea 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{En &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;desenrroll&lt;/del&gt;}}&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{En &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;desenroll&lt;/ins&gt;}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Archivo:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&amp;#039;estructura general del sistema solar i l&amp;#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Archivo:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&amp;#039;estructura general del sistema solar i l&amp;#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

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&lt;/table&gt;</summary>
		<author><name>EirVal</name></author>
	</entry>
	<entry>
		<id>https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=109498&amp;oldid=prev</id>
		<title>EirVal: Pàgina nova, en el contingut: «{{En desenrroll}}  Archivo:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics h...»</title>
		<link rel="alternate" type="text/html" href="https://www.lenciclopedia.org/w/index.php?title=F%C3%ADsica_cl%C3%A0ssica&amp;diff=109498&amp;oldid=prev"/>
		<updated>2016-11-23T18:33:07Z</updated>

		<summary type="html">&lt;p&gt;Pàgina nova, en el contingut: «{{En desenrroll}}  Archivo:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics h...»&lt;/p&gt;
&lt;p&gt;&lt;b&gt;Pàgina nova&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{En desenrroll}}&lt;br /&gt;
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[[Archivo:Cassini-science-br.jpg|thumb|La física clàssica és suficientment adequada per a solucionar la major part de problemes tècnics humans, aixina com per a explicar l&amp;#039;estructura general del sistema solar i l&amp;#039;univers. No obstant, oferix respostes parcials i insatisfactòries a certs [[cosmologia|problemes cosmològics]].]]&lt;br /&gt;
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Es denomina &amp;#039;&amp;#039;&amp;#039;física clàssica&amp;#039;&amp;#039;&amp;#039; a la [[física]] basada en els principis previs a l&amp;#039;aparició de la [[mecànica quàntica]]. Inclou l&amp;#039;estudi de la [[mecànica clàssica|mecànica]], la [[termodinàmica]], el  [[electromagnetisme]], la [[òptica]], la [[acústica]], la [[dinàmica d&amp;#039;@fluido]], entre unes atres. La física clàssica es considera [[Sistema deterministe|deterministe]] (encara que no necessàriament computable o computacionalment predible), en el sentit de que l&amp;#039;estat d&amp;#039;un sistema tancat en el futur depén exclusivament de l&amp;#039;estat del sistema en el moment actual.&lt;br /&gt;
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Algunes voltes, es reserva  la frase nominal &amp;quot;física clàssica&amp;quot; per a la [[mecànica newtoniana|física prerrelativista]]. No obstant, des del punt de vista teòric la [[teoria de la relativitat]] introduïx suposts menys radicals que els que subyacer en la teoria quàntica. Per eixa raó resulta convenient des d&amp;#039;un punt de vista metodològic considerar en conjunt les teories físiques no-quàntiques.&lt;br /&gt;
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[[Categoria:Física]]&lt;br /&gt;
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{{Traduït de|es|Física Clásica}}&lt;/div&gt;</summary>
		<author><name>EirVal</name></author>
	</entry>
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