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Grassmann Variables, Supersymmetry and Supersymmetric ...

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Dirac field<br />

Fermionic Path Integral<br />

SUSY<br />

References<br />

The end<br />

<strong>Grassmann</strong> <strong>Variables</strong><br />

Path Integral<br />

In similar way we can prove:<br />

� dη � dη ηiηje ηAη = (detA)(A −1 )ji<br />

A <strong>Grassmann</strong> field is a function of spacetime whose values are<br />

anticommuting numbers. We can define a <strong>Grassmann</strong> field ψ(x) in<br />

terms of any set of orthonormal basis functions:<br />

ψ(x) = �<br />

ψiφi(x)<br />

The basis functions φi(x) are ordinary complex valued functions,<br />

while the coefficients ψi are <strong>Grassmann</strong> numbers.<br />

To describe the Dirac field we take the φi to be a basis of<br />

four-component spinors.<br />

i<br />

Anna Pachol GV,SUSY ans SHO

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