Bound states in relativistic quantum mechanics

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SUMMARY

The discussion centers on the existence of bound states in relativistic quantum mechanics for a particle subjected to a spherically symmetric potential V(r) defined as V(r) = -V_0 for 0 ≤ r ≤ a and V(r) = 0 elsewhere. Unlike non-relativistic particles, which have bound states for -V_0 < E < 0, relativistic particles exhibit bound states for |E| < mc², where mc² represents the rest energy. This distinction arises from the relativistic energy-momentum dispersion relation E² = p²c² + m²c⁴, indicating that even at zero momentum, the energy remains at mc², establishing a lower energy limit for bound states.

PREREQUISITES
  • Understanding of relativistic energy-momentum dispersion relation
  • Knowledge of quantum mechanics principles, specifically bound states
  • Familiarity with spherically symmetric potentials in quantum systems
  • Basic concepts of particle physics, including rest mass and energy
NEXT STEPS
  • Study the implications of the relativistic energy-momentum relation E² = p²c² + m²c⁴
  • Explore the concept of bound states in quantum mechanics for various potentials
  • Investigate the differences between non-relativistic and relativistic quantum mechanics
  • Learn about the applications of relativistic quantum mechanics in particle physics
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Physicists, quantum mechanics students, and researchers interested in the behavior of particles in relativistic frameworks and the implications for bound states in quantum systems.

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Suppose a particle is subject to a spherically symmetric potential V(r) such that V(r) = -V_0, V_0 &gt; 0, for 0\leq r \leq a and V(r) = 0 elsewhere. If we were considering a non-relativistic particle, we would have bound states for -V_0 &lt; E &lt; 0 (which I understand); however, since the particle is relativistic, apparently (or, at least, according to my professor), we have bound states for |E| &lt; mc^2. Could someone please explain why this is? I'm pretty sure it has something to do with the fact that the relativistic energy-momentum dispersion relation is E(p) = \sqrt{p^2c^2 + m^2c^4}, but I can't wrap my head around it.Thanks.
 
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A:The reason for this is that the energy dispersion relation can be written as $$E^2 = p^2c^2 + m^2c^4,$$where $m$ is the particle's rest mass and $p$ is its momentum. This means that even if the momentum is zero, the energy is still equal to $mc^2$, which sets a lower bound on the energy for a relativistic particle. For a non-relativistic particle, the energy dispersion relation is just $E=\frac{p^2}{2m}$, so the particle can have arbitrarily small energy if the momentum is zero.
 

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