Supersymmetric Lagrangian Transformation (Grassmann Numbers)

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Lonsdale
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I've been tasked with showing that a Lagrangian under a set of transformations changes by a time derivative. All has gone well, except I'm left with two remaining terms, that I am completely confident, aren't there by mistake (as the 16 terms that should be expected have all popped out with the correct signs etc).

The two terms, I believe, probably cancel but I don't just want to speculate. Anyway, the two terms that remain are,

[tex]W'' W' (ψ^*ε^* + εψ)[/tex]

where W is the Superpotential (primes representing derivatives, w.r.t x) as a function of the spatial co-ordinate x. ψ represents the Superspace co-ordinate and epsilon represents the small change Grassmann parameter relevant to our transformation. Stars represent complex conjugates.

Now, I will also add that ψ is a Grassmann number so we can rewrite the terms such that,

[tex]W'' W' (ψ^*ε^* - ψε)[/tex]

So, briefly put, do these two terms cancel one another out? If so, why?

(also, please do not delete my post for not following the template, I didn't find it necessary given that this is quite a small scale question)

Thanks for your time, Physics forum!
 
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Ok... after some thought I don't think they can cancel in this way (or the rest of what I have done wouldn't make sense).

Anyway, instead of writing everything out in full, I'm basically working the Lagrangian on page 5 of this source http://www.phys.columbia.edu/~kabat/susy/susyQM.pdf and using the transforms also on the bottom of page 6.

The terms above come from the final term of the Lagrangian, i.e.

[itex]ψ^*ψW''[/itex]

The the 3rd and 7th terms when multiplying out the brackets. As I mentioned before, everything else canceled out in the calculation or was used to show that the change in the Lagrangian is a total time derivative, I was simply left with the aforementioned two terms.