Energie: Difference between revisions

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<source lang="text">
<source lang="text">
$Assumptions = c > 0 && Subscript[m, 0] >= 0 && p >= 0 && v >= 0;
$Assumptions = c > 0 && Subscript[m, 0] >= 0 && p >= 0 && v >= 0;
\[CapitalEpsilon]nergy :=  
 
  Series[Sqrt[Subscript[m, 0]^2*c^4 + p^2*c^2], {p, 0, 5}] //  
Energy      := Sqrt[Subscript[m, 0]^2*c^4 + p^2*c^2];
  Simplify;
EnergyAppox := Series[Energy, {p, 0, 5}] // Simplify;
Print["E" == \[CapitalEpsilon]nergy]
 
Print["E" == EnergyAppox]
</source>
</source>
<math>E=c^2 m_0+\frac{p^2}{2 m_0}-\frac{p^4}{8 \left(c^2 m_0^3\right)}+O\left(p^6\right)</math>
<math>E=c^2 m_0+\frac{p^2}{2 m_0}-\frac{p^4}{8 \left(c^2 m_0^3\right)}+O\left(p^6\right)</math>


[[Kategorie:Definition]]
[[Kategorie:Definition]]

Revision as of 19:44, 11 July 2009

E2=m2c4+p_2c2 Taylor-Entwicklung für kleine Geschwindigkeiten:

$Assumptions = c > 0 && Subscript[m, 0] >= 0 && p >= 0 && v >= 0;

Energy      := Sqrt[Subscript[m, 0]^2*c^4 + p^2*c^2];
EnergyAppox := Series[Energy, {p, 0, 5}] // Simplify;

Print["E" == EnergyAppox]

E=c2m0+p22m0p48(c2m03)+O(p6)

Kategorie:Definition