As a professional physicist who doesn't do any research, what exactly is it that you get paid for?
Education. I am still in education.
See..? Direct questions equal direct anwers. Put that into an equation.
As a professional physicist who doesn't do any research, what exactly is it that you get paid for?
Direct questions equal direct anwers.
Come on - stick to your promises!Hold on, so you're not a professional physicist? You're a student?
"The Dirac equation is superficially similar to the Schrödinger equation for a free particle:
$$ -\frac{\hbar^2}{2m}\nabla^2\phi = i\hbar\frac{\partial}{\partial t}\phi $$
The left side represents the square of the momentum operator divided by twice the mass, which is the nonrelativistic kinetic energy. If one wants to get a relativistic generalization of this equation, then the space and time derivatives must enter symmetrically, as they do in the relativistic Maxwell equations—the derivatives must be of the same order in space and time. In relativity, the momentum and the energy are the space and time parts of a geometrical space-time vector, the 4-momentum, and they are related by the relativistically invariant relation
$$ \frac{E^2}{c^2} - p^2 = m^2c^2 $$
which says that the length of this vector is the rest mass m. Replacing E and p by derivative operators as Schrödinger theory requires, we get a relativistic equation:
$$ \left(\nabla^2 - \frac{1}{c^2}\frac{\partial^2}{\partial t^2}\right)\phi = \frac{m^2c^2}{\hbar^2}\phi $$
and the wave function$$ \phi\ $$, is a relativistic scalar, it is a complex number which has the same numerical value in all frames. Because the equation is second order in the time derivative, one must specify both the initial value of$$ \partial_t \phi\ $$, and not just $$ \phi\ $$,. This is normal for classical water waves, the initial conditions are the position and velocity, but in quantum mechanics the wavefunction is supposed to be the complete description, just knowing the wavefunction should determine the future.
In the Schrödinger theory, the probability density is given by the positive definite expression
$$ \rho=\phi^*\phi\, $$
and its current by
$$ J = -\frac{i\hbar}{2m}(\phi^*\nabla\phi - \phi\nabla\phi^*) $$
and the conservation of probability density has a local form:
$$ \nabla\cdot J + \frac{\partial\rho}{\partial t} = 0 $$
In a relativistic theory, the form of the probability density and the current must form a four vector, so the form of the probability density can be found from the current just by replacing$$ \nabla $$ by$$ \,\partial_t: $$
$$ \rho = \frac{i\hbar}{2m}(\phi^*\partial_t\phi - \phi\partial_t\phi^*) $$
Everything is relativistic now, but the probability density is not positive definite, because the initial values of both$$ \phi\ $$, and$$ \,\partial_t\phi $$can be freely chosen. This expression reduces to Schrödinger's density and current for superpositions of positive frequency waves whose wavelength is long compared to the compton wavelength, that is, for nonrelativistic motions.
It reduces to a negative definite quantity for superpositions of negative frequency waves only. It mixes up both signs when forces which have an appreciable amplitude to produce relativistic motions are involved, at which point scattering can produce particles and antiparticles.
Although it was not a successful description of a single particle, this equation is resurrected in quantum field theory, where it is known as the Klein–Gordon equation, and describes a relativistic spin-0 complex field. The non-positive probability density and current are the charge-density and current, while the particles are described by a mode-expansion.
In order to give the Klein–Gordon equation an interpretation as an equation for the probability amplitude for a single particle to have a given position, the negative frequency solutions need to be interpreted as describing the particle travelling backwards in time, so that they propagate into the past. The equation with this interpretation does not predict the future from the present except in the nonrelativistic limit, rather it places a global constraint on the amplitudes.
This can be used to construct a perturbation expansion with particles zipping backwards and forwards in time, the Feynman diagrams, but it does not allow a straightforward wavefunction description, since each particle has its own separate proper time."
-the wikipedists
It's just wikipedia's entry for the Dirac electron. Now to derive that action integral for a non-relativistic one.Saxion said:..what book are you working from?
Are you admitting to the following: you are not a professional physicist, but are in fact a student?
What indeed?BTM said:What does "phase of a probability" mean?
the example said:Let the function $$ \theta_I $$ be the probability amplitude that the particle actually takes the path $$l $$ between A and B. It is referred to as a phase factor. If the point is held fixed, then the propagator is only a function of the location , and can simply be written as the probability wave solution of the Dirac equation for a free electron.
The title is an incomplete phrase. Perhaps "phase of a probability amplitude"? (??)I.E. show that both the gravitational field and electromagnetic field act upon the propagator in the same manner.
Both induce a phase shift which causes the wave function to disperse in the direction which minimizes the action, thereby decreasing the relative energy of the wave. The difference is that the gravitational field contribution is the result of the mass/energy, and the electromagnetic field contribution is a result of the electromagnetic energy. Both fields are representative of the local environment of a test particle.
"The Dirac equation is superficially similar to the Schrödinger equation for a free particle:
$$ -\frac{\hbar^2}{2m}\nabla^2\phi = i\hbar\frac{\partial}{\partial t}\phi $$
The left side represents the square of the momentum operator divided by twice the mass, which is the nonrelativistic kinetic energy. If one wants to get a relativistic generalization of this equation, then the space and time derivatives must enter symmetrically, as they do in the relativistic Maxwell equations—the derivatives must be of the same order in space and time. In relativity, the momentum and the energy are the space and time parts of a geometrical space-time vector, the 4-momentum, and they are related by the relativistically invariant relation
$$ \frac{E^2}{c^2} - p^2 = m^2c^2 $$
which says that the length of this vector is the rest mass m. Replacing E and p by derivative operators as Schrödinger theory requires, we get a relativistic equation:
$$ \left(\nabla^2 - \frac{1}{c^2}\frac{\partial^2}{\partial t^2}\right)\phi = \frac{m^2c^2}{\hbar^2}\phi $$
and the wave function$$ \phi\ $$, is a relativistic scalar, it is a complex number which has the same numerical value in all frames. Because the equation is second order in the time derivative, one must specify both the initial value of$$ \partial_t \phi\ $$, and not just $$ \phi\ $$,. This is normal for classical water waves, the initial conditions are the position and velocity, but in quantum mechanics the wavefunction is supposed to be the complete description, just knowing the wavefunction should determine the future.
In the Schrödinger theory, the probability density is given by the positive definite expression
$$ \rho=\phi^*\phi\, $$
and its current by
$$ J = -\frac{i\hbar}{2m}(\phi^*\nabla\phi - \phi\nabla\phi^*) $$
and the conservation of probability density has a local form:
$$ \nabla\cdot J + \frac{\partial\rho}{\partial t} = 0 $$
In a relativistic theory, the form of the probability density and the current must form a four vector, so the form of the probability density can be found from the current just by replacing$$ \nabla $$ by$$ \,\partial_t: $$
$$ \rho = \frac{i\hbar}{2m}(\phi^*\partial_t\phi - \phi\partial_t\phi^*) $$
Everything is relativistic now, but the probability density is not positive definite, because the initial values of both$$ \phi\ $$, and$$ \,\partial_t\phi $$can be freely chosen. This expression reduces to Schrödinger's density and current for superpositions of positive frequency waves whose wavelength is long compared to the compton wavelength, that is, for nonrelativistic motions.
It reduces to a negative definite quantity for superpositions of negative frequency waves only. It mixes up both signs when forces which have an appreciable amplitude to produce relativistic motions are involved, at which point scattering can produce particles and antiparticles.
Although it was not a successful description of a single particle, this equation is resurrected in quantum field theory, where it is known as the Klein–Gordon equation, and describes a relativistic spin-0 complex field. The non-positive probability density and current are the charge-density and current, while the particles are described by a mode-expansion.
In order to give the Klein–Gordon equation an interpretation as an equation for the probability amplitude for a single particle to have a given position, the negative frequency solutions need to be interpreted as describing the particle travelling backwards in time, so that they propagate into the past. The equation with this interpretation does not predict the future from the present except in the nonrelativistic limit, rather it places a global constraint on the amplitudes.
This can be used to construct a perturbation expansion with particles zipping backwards and forwards in time, the Feynman diagrams, but it does not allow a straightforward wavefunction description, since each particle has its own separate proper time."
-the wikipedists
K.prometheus said:the Dirac equation. That is $$ \left( i \gamma^\mu \partial_\mu -m \right) \psi = 0$$. A solution to the Dirac equation is automatically a solution to the Klein Gordon equation, since the KG equation is simply an expression of the relativistic dispersion relation. However, solutions to the Klein Gordon equation are not necessarily solutions to the Dirac equation.