Divergence of integral over vacuum energies (Free field)

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SUMMARY

The discussion centers on the Hamiltonian for a free scalar field, expressed using creation and annihilation operators. The Hamiltonian is defined as H = ∫ d³p [ωₚ a†ₚ aₚ + ½ωₚ δ³(0)], where ωₚ is derived from the relation ω²ₚ = |p|² + m². A key point of confusion arises regarding the Dirac delta function δ³(0), which represents an infinite value, leading to a divergence in the first term for infinite momentum p. The participant acknowledges a conceptual error in their understanding of the implications of δ³(0).

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soviet1100
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Hi,

The Hamiltonian for the free scalar field, expressed in terms of the creation/annihilation operators, is

H = \int d^{3}p [\omega_p a^{\dagger}_p a_p + \frac{1}{2}\omega_p \delta^{3}(0)] \hspace{3mm}

I thought: \omega_p is a function of p as \omega^{2}_p = |p|^{2} + m^2 and so the dirac delta will sift out the value of \omega_p at p = 0. Could someone tell me why this statement is incorrect? I think I've made some significant conceptual error. Is the first term divergent for infinite p as well?

P.S. wherever p appears above, it is to be taken as the 3-momentum
 
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What you expect would happen if the Dirac delta was ## \delta^3(p) ##. But ## \delta^3(0) ## is simply equal to infinity, or more precisely, the volume of whole space, which is a constant.
 
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Shyan said:
What you expect would happen if the Dirac delta was ## \delta^3(p) ##. But ## \delta^3(0) ## is simply equal to infinity, or more precisely, the volume of whole space, which is a constant.

Ah, of course. Thanks, that was silly of me.
 

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