Energy-Momentum Tensor in Phi^3 Theory

In summary, the equations provided are from quantum field theory, specifically from the quantization of a free scalar field. The first equation is the momentum state of a particle in terms of creation and annihilation operators, and the second equation is the matrix element of the energy-momentum tensor in terms of these operators. The LSZ reduction formula can be used to interpret the second equation as a limit of a time-ordered product of operators. To calculate terms like the one given in the second question using Feynman diagrams, one would need to follow the Feynman rules for the theory being studied and sum over all possible diagrams.
  • #1
Diracobama2181
75
2
TL;DR Summary
If I have an energy-momentum tensor
$$\hat{T}^{\mu \nu} (x)=\partial^{\mu}\Phi\partial^{\nu}\Phi-\\g^{\mu \nu}\mathcal{L}$$
,with
$$
\mathcal{L}=(\frac{1}{2}(\partial_{\mu}\Phi)^2-\frac{1}{2}m^2\Phi^2-\frac{\lambda \Phi^3}{3!})
$$
, how would I go about calculating
$$
\bra{ \vec{ p'}} T^{\mu,\nu} \ket{ \vec {p}}
$$ ?
Relevant Equations:: ##\ket{\vec{p}}=\hat{a}^{\dagger}(\vec{p})\ket{0}## for a free field with ##[\hat{a}({\vec{k})},\hat{a}^{\dagger}({\vec{k'})}]=2(2\pi)^3\omega_k\delta^3({\vec{k}-\vec{k'}})##

$$ \bra{ \vec{ p'}} T_{\mu,\nu} \ket{ \vec {p}}=\bra{\Omega}\hat{a}(\vec{p'})(\partial^{\mu}\Phi\partial^{\nu} \Phi-g^{\mu \nu}\mathcal{L})\hat{a}^{\dagger}(\vec{p})\ket{\Omega}=\bra{\Omega}(\hat{a}(\vec{p'})\partial^{\mu}\Phi\partial^{\nu} \Phi\hat{a}^{\dagger}(\vec{p})\\ -\hat{a}(\vec{p'})g^{\mu \nu}(\frac{1}{2}(\partial_{\mu}\Phi)^2-\frac{1}{2}m^2\Phi^2-\frac{\lambda \Phi^3}{3!}))\hat{a}^{\dagger}(\vec{p})\ket{\Omega}$$
In this instance, would this imply that, for example, $$\bra{\Omega}(\hat{a}(\vec{p'})(\frac{1}{2}(\partial_{\mu}\Phi)^2-\frac{1}{2}m^2\Phi^2-\frac{\lambda \Phi^3}{3!})\hat{a}^{\dagger}(\vec{p}))\ket{\Omega}=lim_{t \to \infty(1-i\epsilon)}\frac{\bra{0}[T(\hat{a}(\vec{p'})(\frac{1}{2}(\partial_{\mu}\Phi)^2-\frac{1}{2}m^2\Phi^2-\frac{\lambda \Phi^3}{3!})\hat{a}^{\dagger}(\vec{p}))e^{-i\int \lambda \frac{\Phi^3}{3!}dt}]\ket{0}}{\bra{0}T e^{-i\int \lambda \frac{\Phi^3}{3!}dt}\ket{0}}$$?
Also, how would I go about calculating terms like $$\bra{\Omega}\hat{a}(\vec{p'})(\partial^{\mu}\Phi\partial^v \Phi )\hat{a}^{\dagger}(\vec{p})\ket{\Omega}$$ using Feynman diagrams? Thanks in advance.
 
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  • #2


I would first clarify that the equations provided are from quantum field theory, specifically from the quantization of a free scalar field. The first equation is the momentum state of a particle in terms of creation and annihilation operators, and the second equation is the matrix element of the energy-momentum tensor in terms of these operators.

To answer the first question, yes, the expression given for the matrix element can be interpreted as a limit of a time-ordered product of operators. This is known as the LSZ reduction formula, and it is used to extract physical scattering amplitudes from quantum field theory calculations.

To calculate terms like the one given in the second question using Feynman diagrams, one would need to first understand the Feynman rules for the theory being studied. These rules dictate how to assign mathematical expressions to each vertex and propagator in the Feynman diagram. Then, one would need to follow the rules for calculating the amplitude, which involves summing over all possible diagrams and integrating over the loop momenta. The final result would be a mathematical expression that can be compared with the desired matrix element.
 

1. What is the Energy-Momentum Tensor in Phi^3 Theory?

The Energy-Momentum Tensor in Phi^3 Theory is a mathematical quantity that describes the energy and momentum of a system in the context of the Phi^3 field theory. It is a tensor, which means it is a mathematical object that has both magnitude and direction, and it is used to calculate the energy and momentum of particles within the theory.

2. How is the Energy-Momentum Tensor calculated in Phi^3 Theory?

The Energy-Momentum Tensor is calculated using mathematical equations that incorporate the values of the Phi^3 field and its derivatives. These equations take into account the energy and momentum of the particles within the theory and can be used to make predictions about their behavior.

3. What is the significance of the Energy-Momentum Tensor in Phi^3 Theory?

The Energy-Momentum Tensor is significant because it allows us to understand and predict the behavior of particles within the Phi^3 field theory. It is a fundamental concept in the theory and is used in many calculations and equations to describe the dynamics of the system.

4. How does the Energy-Momentum Tensor relate to conservation laws?

The Energy-Momentum Tensor is closely related to the conservation laws of energy and momentum. In fact, it is often used to derive these laws in the context of the Phi^3 field theory. The tensor is conserved, meaning that its value remains constant, and this conservation is directly related to the conservation of energy and momentum in the system.

5. Are there any limitations to the Energy-Momentum Tensor in Phi^3 Theory?

Like any mathematical concept, the Energy-Momentum Tensor in Phi^3 Theory has its limitations. It is a simplified model that does not take into account all possible factors and interactions within the system. It is also limited by the accuracy of the measurements and calculations used to determine its values. However, it is still a valuable tool for understanding and predicting the behavior of particles in the Phi^3 field theory.

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