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In physics, a free particle is a particle that, in some sense, is not bound by an external force, or equivalently not in a region where its potential energy varies. In classical physics, this means the particle is present in a "field-free" space. In quantum mechanics, it means a region of uniform potential, usually set to zero in the region of interest since potential can be arbitrarily set to zero at any point (or surface in three dimensions) in space.

Contents

Classical free particleEdit

The classical free particle is characterized simply by a fixed velocity v. The momentum is given by

 

and the kinetic energy (equal to total energy) by

 

where m is the mass of the particle and v is the vector velocity of the particle.

Quantum free particleEdit

 
Propagation of de Broglie waves in 1d - real part of the complex amplitude is blue, imaginary part is green. The probability (shown as the colour opacity) of finding the particle at a given point x is spread out like a waveform, there is no definite position of the particle. As the amplitude increases above zero the curvature decreases, so the decreases again, and vice versa - the result is an alternating amplitude: a wave. Top: Plane wave. Bottom: Wave packet.

Mathematical descriptionEdit

A free particle in non-relativistic quantum mechanics is described by the free Schrödinger equation:

 

where ψ is the wavefunction of the particle at position r and time t. The solution for a particle with momentum p or wave vector k, at angular frequency ω or energy E, is given by the complex plane wave:

 

with amplitude A. As for all quantum particles free or bound, the Heisenberg uncertainty principles

 

(similarly for the y and z directions), and the De Broglie relations:

 

apply. Since the potential energy is (set to) zero, the total energy E is equal to the kinetic energy, which has the same form as in classical physics:

 

Measurement and calculationsEdit

The integral of the probability density function

 

where * denotes complex conjugate, over all space is the probability of finding the particle in all space, which must be unity if the particle exists:

 

This is the normalization condition for the wave function. The wavefunction is not normalizable for a plane wave, but is for a wavepacket.

Increasing amounts of wavepacket localization, meaning the particle becomes more localized.
In the limit ħ → 0, the particle's position and momentum become known exactly.
Interpretation of wave function for one spin-0 particle in one dimension. The wavefunctions shown are continuous, finite, single-valued and normalized. The colour opacity (%) of the particles corresponds to the probability density (which can measure in %) of finding the particle at the points on the x-axis.

Fourier decompositionEdit

The free particle wave function may be represented by a superposition of momentum eigenfunctions, with coefficients given by the Fourier transform of the initial wavefunction:[1]

 

where the integral is over all k-space and   (to ensure that the wave packet is a solution of the free particle Schrödinger equation). Here   is the value of the wave function at time 0 and   is the Fourier transform of  . (The Fourier transform   is essentially the momentum wave function of the position wave function  , but written as a function of   rather than  .)

The expectation value of the momentum p for the complex plane wave is

 ,

and for the general wave packet it is

 .

The expectation value of the energy E is

 .

Group velocity and phase velocityEdit

 
Propagation of a wave packet, with the motion of a single peak shaded in purple. The peaks move at the phase velocity while the overall packet moves at the group velocity.

The phase velocity is defined to be the speed at which a plane wave solution propagates, namely

 .

Note that   is not the speed of a classical particle with momentum  ; rather, it is half of the classical velocity.

Meanwhile, suppose that the initial wave function   is a wave packet whose Fourier transform   is concentrated near a particular wave vector  . Then the group velocity of the plane wave is defined as

 ,

which agrees with the formula for the classical velocity of the particle. The group velocity is the (approximate) speed at which the whole wave packet propagates, while the phase velocity is the speed at which the individual peaks in the wave packet move.[2] The figure illustrates this phenomenon, with the individual peaks within the wave packet propagating at half the speed of the overall packet.

Spread of the wave packetEdit

The notion of group velocity is based on a linear approximation to the dispersion relation   near a particular value of  .[3] In this approximation, the amplitude of the wave packet moves at a velocity equal to the group velocity without changing shape. This result is an approximation that fails to capture certain interesting aspects of the evolution a free quantum particle. Notably, the width of the wave packet, as measured by the uncertainty in the position, grows linearly in time for large times. This phenomenon is called the spread of the wave packet for a free particle.

Specifically, it is not difficult to compute an exact formula for the uncertainty   as a function of time, where   is the position operator. Working in one spatial dimension for simplicity, we have:[4]

 ,

where   is the time-zero wave function. The expression in parentheses in the second term on the right-hand side is the quantum covariance of   and  .

Thus, for large positive times, the uncertainty in   grows linearly, with the coefficient of   equal to  . If the momentum of the initial wave function   is highly localized, the wave packet will spread slowly and the group-velocity approximation will remain good for a long time. Intuitively, this result says that if the initial wave function has a very sharply defined momentum, then the particle has a sharply defined velocity and will (to good approximation) propagate at this velocity for a long time.

Relativistic quantum free particleEdit

There are a number of equations describing relativistic particles: see relativistic wave equations.

See alsoEdit

ReferencesEdit

  • Quantum Mechanics, E. Abers, Pearson Ed., Addison Wesley, Prentice Hall Inc, 2004, ISBN 978-0-13-146100-0
  • Quantum Physics of Atoms, Molecules, Solids, Nuclei, and Particles (2nd Edition), R. Eisberg, R. Resnick, John Wiley & Sons, 1985, ISBN 978-0-471-87373-0
  • Stationary States, A. Holden, College Physics Monographs (USA), Oxford University Press, 1971, ISBN 0-19-851121-3
  • Hall, Brian C. (2013), Quantum Theory for Mathematicians, Graduate Texts in Mathematics, 267, Springer, ISBN 978-1461471158 
  • Quantum Mechanics Demystified, D. McMahon, Mc Graw Hill (USA), 2006, ISBN 0-07-145546 9
  • Elementary Quantum Mechanics, N.F. Mott, Wykeham Science, Wykeham Press (Taylor & Francis Group), 1972, ISBN 0-85109-270-5
  • Quantum mechanics, E. Zaarur, Y. Peleg, R. Pnini, Schaum’s Oulines, Mc Graw Hill (USA), 1998, ISBN 007-0540187
Specific
  1. ^ Hall 2013 Section 4.1
  2. ^ Hall 2013 Sections 4.3 and 4.4
  3. ^ Hall 2013 Equation 4.24
  4. ^ Hall 2013 Proposition 4.10

Further readingEdit

  • The New Quantum Universe, T.Hey, P.Walters, Cambridge University Press, 2009, ISBN 978-0-521-56457-1.
  • Quantum Field Theory, D. McMahon, Mc Graw Hill (USA), 2008, ISBN 978-0-07-154382-8
  • Quantum mechanics, E. Zaarur, Y. Peleg, R. Pnini, Schaum’s Easy Oulines Crash Course, Mc Graw Hill (USA), 2006, ISBN 978-007-145533-6