Meaning of coefficients in polynomial potential for scalar field

PhysicsRock
Messages
121
Reaction score
19
Homework Statement
For a potential ##V(\phi) = \sum_{k=0}^N c_k \phi^k##, we set ##c_k = 0## for all ##k \neq 2##. What is the physical meaning of ##c_2##?
Relevant Equations
Equation of motion ##\partial_\mu \partial^\mu \phi = 2c_2 \phi##.
For the solution of the equation of motion, we take a plane wave ##\phi(x) = e^{ik_\mu x^\mu}##. Plugged in, we obtain

$$
-(k_0)^2 + (\vec{k})^2 = 2c_2 \Rightarrow k_\mu k^\mu = 2c_2
$$

One can then find the group velocity (using ##(k_0)^2 = \omega^2##) to be

$$
\vec{v}_g = \frac{\vec{k}}{\sqrt{ \vec{k}^2 - 2c_2 }}
$$

which does not break causality only if ##c_2 \leq 0##. This leads to the assumption, at least from my perspective, that ##c_2## must be related to the mass / be the mass of the field, since if ##m = 0##, the field would propagate at the speed of light. However, using ##2c_2 = k_\mu k^\mu##, we can see that ##c_2## must have the same unit as ##k_\mu k^\mu##, i.e. m##^{-2}## in S.I. units.

Did I make a mistake along the way or am I misinterpreting the meaning of ##c_2 \leq 0##? Help is highly appreciated.
 
Physics news on Phys.org
I think I've figured it out. We can set ##c = \hbar = 1##. Then ##p^\mu = k^\mu##, which implies ##k_\mu k^\mu = p_\mu p^\mu = p^2 = -m^2##. Thus, we get ##2c_2 = -m^2 \Leftrightarrow c_2 = -\frac{m^2}{2}##.
 
##|\Psi|^2=\frac{1}{\sqrt{\pi b^2}}\exp(\frac{-(x-x_0)^2}{b^2}).## ##\braket{x}=\frac{1}{\sqrt{\pi b^2}}\int_{-\infty}^{\infty}dx\,x\exp(-\frac{(x-x_0)^2}{b^2}).## ##y=x-x_0 \quad x=y+x_0 \quad dy=dx.## The boundaries remain infinite, I believe. ##\frac{1}{\sqrt{\pi b^2}}\int_{-\infty}^{\infty}dy(y+x_0)\exp(\frac{-y^2}{b^2}).## ##\frac{2}{\sqrt{\pi b^2}}\int_0^{\infty}dy\,y\exp(\frac{-y^2}{b^2})+\frac{2x_0}{\sqrt{\pi b^2}}\int_0^{\infty}dy\,\exp(-\frac{y^2}{b^2}).## I then resolved the two...
It's given a gas of particles all identical which has T fixed and spin S. Let's ##g(\epsilon)## the density of orbital states and ##g(\epsilon) = g_0## for ##\forall \epsilon \in [\epsilon_0, \epsilon_1]##, zero otherwise. How to compute the number of accessible quantum states of one particle? This is my attempt, and I suspect that is not good. Let S=0 and then bosons in a system. Simply, if we have the density of orbitals we have to integrate ##g(\epsilon)## and we have...
Back
Top