Ground State in Peskin and Schroeder

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Diracobama2181
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I am having a little confusion regarding the limit taken in Peskin and Schroeders quantum field theory book in ch. 4.
In P&S, it is shown that $$e^{-iHT}\ket{0}=e^{-iH_{0}T}\ket{\Omega}\bra{\Omega}\ket{0}+\sum_{n\neq 0}e^{-iE_nT}\ket{n}\bra{n}\ket{0}$$.
It is then claimed that by letting $$T\to (\infty(1-i\epsilon)) $$ that the other terms die off much quicker than $$e^{-iE_0T}$$, but my question is why is this the case? For example, why wouldn't the other terms also die off quicker if we simply sent $$T\to \infty$$ instead? Perhaps there is something about the limit of complex numbers I'm not understanding. Any insight would be appreciated. Thanks.
 
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Nevermind, I think I figured it our. I mistakenly assumed the $$e^{-iE_n T}\to 0$$ as $$T\to \infty$$, but that is not the case, which is why the substitution is needed.
 
It becomes much clearer by "renormalizing" the Hamiltonian such that ##E_0=0##, i.e., the ground state energy eigenvalue is set to 0 by shifting the total energy of the system (represented by the Hamilton operator) by adding a constant such that ##E_0=0##. Then all ##E_n>0##.

Now it is utmost important to add an infinitesimal imaginary part to ##T##, i.e., substituting ##T \rightarrow T-\mathrm{i} \epsilon##. This is crucial for all further developments of the theory to get the correct propagator (in vacuum QFT perturbation theory the time-ordered free-field propagator) and the correct "adiabatic switching" for the LSZ reduction. This is a pretty subtle point and should be very well studied!
 
vanhees71 said:
It becomes much clearer by "renormalizing" the Hamiltonian such that ##E_0=0##, i.e., the ground state energy eigenvalue is set to 0 by shifting the total energy of the system (represented by the Hamilton operator) by adding a constant such that ##E_0=0##. Then all ##E_n>0##.

Now it is utmost important to add an infinitesimal imaginary part to ##T##, i.e., substituting ##T \rightarrow T-\mathrm{i} \epsilon##. This is crucial for all further developments of the theory to get the correct propagator (in vacuum QFT perturbation theory the time-ordered free-field propagator) and the correct "adiabatic switching" for the LSZ reduction. This is a pretty subtle point and should be very well studied!

Can you perhaps say a bit more about vacuum QFT and adiabatic switching. Recently I saw these terms more frequently and would like to know more about them. Do you know a good reference to read about this subject?
 
Do you also happen to know which chapter? I think its either: chapter 16 Vacuum Expectation Values and S-Matrix or, chapter 17 Perturbation Theory