Energie

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E2=m2c4+p_2c2 Taylor-Entwicklung für kleine Geschwindigkeiten: $Assumptions = c > 0 && Subscript[m, 0] >= 0 && p >= 0 && v >= 0; \[CapitalEpsilon] :=

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

Print["E" == \[CapitalEpsilon]] E=c2m0+p22m0p48(c2m03)+O(p6)