How does one derive the Lagrangian densities used in QFT?

In summary: The most common example is the non-relativistic limit of a scalar field theory with a kinetic term containing second-order time derivatives. In the non-relativistic limit, the speed of light c goes to infinity and the time derivatives become important. This leads to a non-canonical kinetic term in the Hamiltonian, which is not the same as the Lagrangian used to derive the theory. This can cause some confusion and requires careful treatment when doing calculations.
  • #1
Maurice7510
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I've been working through a qft book by Sadovskii (while I wait for my Peskin book to come in) and I've used some later chapters of Griffith's Into to Elementary Particles as an introduction to some qft. My issue with both of these is that, where in classical mechanics we have the Lagrangian defined as the difference in potential and kinetic energy, we have no explicit definition of the Lagrangian density in qft. Everything I've seen has been, "so here's the basic Lagrangian density we want for this situation" with no derivation or even justification beyond, "we use this form because it gives us what we want later". This hardly seems like a legitimate method to me, and they have the tendency to imply that the additional terms in the density used ensure invariance are just happened upon, as though someone just kind of noticed it worked out if they added it on. I was wondering if there's a way to derive the Lagrangian density for, say, the free Klein-Gordon equation and how the additional terms are methodically sought out?
 
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  • #2
Maurice7510 said:
"we use this form because it gives us what we want later"

I would see it more in the light of "we use this form because it gives a good description of what experiments tell us". This is not particular for QFT, it goes for all of science, including Newton's equations. Of course there may be some leads as to what kind of terms are allowed and provide consistent QFTs, but all in all, science is mainly about trying to guess how the Universe works and checking if it does.
 
  • #3
In classical physics we first learn Newtonian mechanics. Then we learn that the same physics can be represented in a different way, with Lagrangian mechanics. We prove that if you set L = T - V, Lagrangian mechanics gives the same results as Newtonian mechanics. But note that we could have gone the other way. We could take Lagrangian mechanics as fundamental, and then derive Newton's laws from the Lagrangian. This would be perfectly valid; after all the two formulations are totally equivalent so you can take either one as fundamental and then derive the other.

In field theory it's convenient to take the Lagrangian formulation as the fundamental one. So our approach is basically, "let's write down all the possible Lagrangians and see what physics they produce." The reason it's convenient to start from a Lagrangian is that the symmetries of a theory are manifest in its Lagrangian. So for example if we want a Lorentz-invariant theory, we restrict ourselves to Lorentz-invariant Lagrangians. And the way we come up with the Klein-Gordon Lagrangian is that it's the simplest possible Lorentz-invariant Lagrangian for a spin-0 field.
 
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  • #4
As any fundamental physical law we take the Lagrangians of elementary particle physics from experience. Anything fundamental in physics is a (often extremely condensed) description of a lot of observations in nature.

There are of course some guide lines from mathematics. In this case it's the symmetries of space-time you start with (which are of course also just a description of empirical facts). In HEP you use Minkowski space-time with the Poincare symmetry. This already gives a lot of hints, which possible action functionals can be written down in terms of fields. Then there are more symmetries, all empirical facts deduced from observed conservation laws, which constrain the actions further.
 
  • #5
The Lagrangian you write down, still remains the Legendre transformation of the Hamiltonian of your system...
So even if you want to write down the Lagrangian of a photon field, you could as well take the Hamiltonian (the "photons' energy") and do the transformation to get the Lagrangian. It's not so unreasonable afterall...but more convenient...
 
  • #6
The approach via the Lagrangian is usually more convenient, because it's manifestly Lorentz invariant. Of course, the right way to quantize is via the Hamiltonian formalism. You come back to the Lagrangian formulation in almost all practically important cases by integrating out the canonical field momenta in the path-integral formula for the generating functional for Green's functions, but one must be careful, if there are time derivatives in couplings. Then you may not end up with the classical Lagrangian you expect!
 
  • #7
vanhees71 said:
but one must be careful, if there are time derivatives in couplings. Then you may not end up with the classical Lagrangian you expect!

Is there an example about that? I don't remember coming across any (it sounds like something new, or maybe it's the phrasing of something known that is changed)
 

Related to How does one derive the Lagrangian densities used in QFT?

1. How is the Lagrangian density derived in QFT?

The Lagrangian density in quantum field theory (QFT) is derived using the principle of least action, which states that the path taken by a system between two points in time is the one that minimizes the action integral. This action integral is a function of the Lagrangian, which is a mathematical expression that describes the dynamics of the system. By applying the principle of least action to the Lagrangian, we can derive the equations of motion for the system, including the quantum field equations in QFT.

2. What is the role of symmetries in deriving the Lagrangian density in QFT?

Symmetries play a crucial role in the derivation of the Lagrangian density in QFT. In particular, the principle of gauge invariance, which states that the laws of physics should be unchanged under a transformation of the fields, leads to the inclusion of gauge fields in the Lagrangian density. Additionally, other symmetries such as Lorentz invariance and global symmetries also play a role in determining the form of the Lagrangian density.

3. Are there different methods for deriving the Lagrangian density in QFT?

Yes, there are different methods for deriving the Lagrangian density in QFT. One common approach is to start with a classical Lagrangian, which describes the dynamics of a classical field, and then quantize it to obtain the corresponding quantum field equations. Another approach is to use the path integral formulation, which involves summing over all possible paths of the fields to determine the Lagrangian density. Both methods have their advantages and are used in different contexts in QFT.

4. How does the Lagrangian density in QFT differ from that in classical mechanics?

The Lagrangian density in QFT differs from that in classical mechanics in several ways. In classical mechanics, the Lagrangian is a function of the generalized coordinates and their derivatives, while in QFT, it is a function of the fields and their derivatives. Additionally, in QFT, the Lagrangian density is typically complex and includes terms involving the fields and their conjugate momenta. Furthermore, in QFT, the Lagrangian density can also depend on time, whereas in classical mechanics, it is usually a function of position and velocity only.

5. Can the Lagrangian density be derived for any quantum field theory?

The Lagrangian density can be derived for most quantum field theories, but there are some exceptions. In particular, theories that involve strong interactions, such as quantum chromodynamics (QCD), do not have a known classical Lagrangian and are instead described by a non-perturbative quantum field theory. In these cases, the Lagrangian density cannot be derived using the traditional methods and must be determined using alternative approaches, such as lattice QCD.

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