Feynman's Parton Picture
Before Einstein, the energymomentum relation for massive particles and massless particles were E = p^{2}/2m and E = cp respectively. Einstein combined these two separate formulas into one. As we know well, Einstein's work was not trivial.
It is only natural to regard the parton picture as a Lorentzboosted quark model. However, since the partons are so different from the quarks, we have been wondering whether they are really Lorentzboosted quarks.
 Further Contents of E = mc^{2}
 Covariant Model
 Lorentz Boost
 Feynman's Decoherence
 Infinite Number of Partons
 Boiling Quarks and Phase Transition
Further Contents of Einstein's Energymomentum Relation
 Click here for further contents
of Einstein's E = mc^{2}.
 According to Feynman,
the adventure of our science of physics is a perpetual attempt to
recognize that the different aspects of nature are really different
aspects of the same thing.
In this photo, one Feynman admirer is standing in front of Feynman's preterit at the entrance of the Feynman Computing Center at Fermi National Accelerator Center, Batavia, Illinois (June 2003). He has been doing Feynman's physics since 1970.
 According to Ne'eman, Feynman diagrams and
the parton model are the two greatest contributions Feynman made. Feynman
diagrams are well known and well understood, but his parton model is yet
to be understood. Why is it so difficult to understand the parton model?
It contains too much physics, including some of the current issues such as
decoherence, as well as future issues.
Einstein's World
 
 
 

How can we construct a covariant model for quarks and partons?
Let us start with a hadron consisting of two quarks bound together by a harmonic oscillator potential. The simplest wave function for this twoparticle system is is the harmonic oscillator wave function. Can this wave function be Lorentzboosted?
 Its boundary condition can be stated in terms of the spatial
coordinates in a given Lorentz frame. Then how about other frames
where the spatial and timelike coordinates are mixed?
In order to deal with this problem, we need the timeseparation variable.
Does this variable exist? We are quite familiar with the Bohr radius.
It measures the spatial separation between the constituent particles.
Then, is there a timelike separation? According to Einstein, the
answer is YES. This is the starting point of our plan to construct
a harmonic oscillator wave function which can be Lorentz transformed.
 Let us tackle this problem with the following three figures. The first
figure is a spacetime diagram of the harmonic oscillator wave function.
The second figure describes Lorentz boosts in the lightcone coordinate
system. The third figure combines quantum mechanics with special
relativity by combining the first two figures.
 The present form of quantum mechanics.
Let us consider a hadron consisting of two quarks bound together
by a harmonic oscillator potential. Then, Heisenberg's uncertainty
principle applies to positionmomentum coordinates,
and there are excited states along the spacelike directions. As
for the timelike (timeseparation between the quarks),
there are no excitations, but there still exist a timeenergy uncertainty
without excitation. According to Dirac, it is a cnumber timeenergy
uncertainty relation.
 Special relativity. Lorentz boost in the lightcone coordinate system.
We are quite familiar with the condition

(z^{2}  t^{2}) = constant
in special relativity. This equation gives the hyperbola in the graph. The above equation can also be written

(z + t)(z  t) = constant.
The Lorentz boost along the z direction expands (z + t) and contracts (z  t) while keeping the above product constant. This is called Dirac's lightcone coordinate system. The Lorentz boost is now a "squeeze" transformation.
 It is then easy to combine quantum mechanics and special relativity.
We can now Lorentzboost quantum mechanics given in the first figure.
We can simply squeeze the circle given in the first figure according
to the transformation law of special relativity given in the
second figure.
 The present form of quantum mechanics.
Let us consider a hadron consisting of two quarks bound together
by a harmonic oscillator potential. Then, Heisenberg's uncertainty
principle applies to positionmomentum coordinates,
and there are excited states along the spacelike directions. As
for the timelike (timeseparation between the quarks),
there are no excitations, but there still exist a timeenergy uncertainty
without excitation. According to Dirac, it is a cnumber timeenergy
uncertainty relation.
 Einstein and Feynman.
Dirac talks about them.
Can you boost a quarkmodel wave function to get a parton distribution?
 As the hadron moves fast, the quark distribution becomes
concentrated along one of the lightcone axes. The amplitude of
the oscillation becomes larger, indicating that the spring constant
appears to become weaker. The particles become free!
 The momentum distribution becomes also widespread. This is what
we see in the world through Feynman's parton model.
 The number of partons is infinite because free particles have
continuous momentum distribution as in the case of blackbody radiation.
 The major axis of the ellipse measures the period of oscillation. As Feynman observed, the interaction time between the quarks is dilated.
Y. S. Kim, Phys. Rev. Lett. 63 , 348 (1989). 
P. Hussar, Phys. Rev. 23, 2781 (1981). 
We are of course interested to know whether the parton distribution calculated from the covariant oscillator formalism is in agreement with the distribution observed in the real world. This graph will indicate that the answer is YES.
Feynman's Decoherence

Feynman's Decoherence.
Does the Lorentz boost destroy coherence?
 Covariant Oscillators. See Section on Feynman's decoherence in this paper.
Click here for a more comprehensive figure. 
In this picture of the Lorentzsqueezed hadron, the major axis corresponds to the period of oscillation. It tells how often the quarks inside the hadron meet. The minor axis tells how long it takes the external signal to interact with the single quark. If the total energy of the hadron is 1,000 times the mass, the ratio of the major axis to minor axis is 1,000,000. Thus, other quarks in the same hadron do not have a chance to interfere with the quark interacting with the external signal.
Of course these can be explained in terms of mathematical formulas, and they are given in many published papers. The following two review papers may be helpful.
Infinite Number of Partons

If the partons
and the quarks are the same particles viewed from different from
different Lorentz frames, why is the number of partons infinite while
the number of quarks is two or three.
Let us look at this figure. If you are not familiar with this figure, Click here for explanation.
As the hadron is boosted, both the spacetime and momentumenergy wave functions exhibit the Lorentzsqueeze. As a consequence, quarks become like massless particles moving with the speed of light. Because of the widespread longitudinal distribution, the spring constant appears like very weak, and quarks appear like free particles.
At the same time, the momentum distribution becomes widespread. If free massless particles have a widespread momentum distribution, it is like the blackbody radiation: infinite number of massless particles.
Boiling Quarks
In his 1972 book on statistical mechanics, said

When we solve a quantummechanical problem, what we really do
is divide the universe into two parts  the system in which we are
interested and the rest of the universe. We then usually act as if
the system in which we are interested comprised the entire universe.
To motivate the use of density matrices, let us see what happens
when we include the part of the universe outside the system.
The Bohr radius is an important quantity in quantum mechanics. It is a spacelike separation between two particles. However, if the system is boosted, the timelike separation becomes prominent. This problem goes back to Bohr and Einstein. They met often, but they never discussed this issue. Click here for a story.
Since there are no theoretical tools to deal with this problem, this variable is in the Feynman's rest of the universe.
On the other hand, von Neumann's approach to entropy tells us how to deal with the variable we do not measure. If they are not measured, they appear as an entropy increase. Let us look at this figure.
Click here for detailed calculations. The entropy increase means an increase in temperature. This thus leads to the following figure the phase transition from the confined state to a plasma state.
Thus, we are led to the phase transition of the form
