A Free Particle

A free particle is not subjected to any forces, its potential energy is constant.  Set V(r,t)=0, since the origin of the potential energy may be chosen arbitrarily.  The Schroedinger equation then becomes 

.

Plane waves are possible solutions,

y(r,t)=Aexp(k×r-wt),

as long as  hw=h2k2/(2m).  

We have

,

 

using the de Broglie relations.

A plane wave represents a particle whose probability of presence is constant throughout space;

|y(r,t)|2=|A|2=constant.

But a plane wave is not square-integrable, it is not a proper solution.

The Schroedinger equation is a linear equation, the principle of superposition applies.  A linear combination of plane wave solutions is also a solution.  

will be a solution as long as for each k we have  hwk=h2k2/(2m).  
Since k is a continuous variable, the most general solution is not a sum, but an integral;

.

Such a wave function is called a three-dimensional wave packet and can represent any non-pathological square-integrable function.
(g(k) can be complex: g(k)=|g(k)|exp(ia(k))a(k) changes the phase of the plane wave.)
Proper wave functions of free particles are wave packets.

One-dimensional wave packets representing free particles

Let us first concentrate on one-dimensional systems.

 

is a superposition of plane waves traveling in the ±x direction.  At some instance of time, say t=0,

,

 ;

g(k) is the Fourier transform of y(x,0).

(Fourier series:  see appendix I, Cohen-Tannoudji)

Any piece-wise regular periodic function (finite # of discontinuities, finite # of extreme values) can be written as a series of imaginary exponentials.  Assume f(x) is a periodic function of x with fundamental period L;

.

The coefficients Cm are given by

.

In the limit  L ® ¥ this can be generalized to

,

where

;

f(x) and are Fourier transforms of each other.

Note: A Fourier transform is a linear transform;

.

 

Consider a wave packet  

,

and assume |g(k)|is centered at k0 where it reaches a maximum and has a width Dk.  Assume Dk<<k0.  Assume g(k)=|g(k)|exp(ia(k)).  Such a wave packet represents a particle with fairly well defined momentum p (Dp<<p).

In the neighborhood of k=k0 we may expand a(k) in a Taylor series expansion;

.

We are only interested in a(k) in a small range of k about k0.  Keeping only zeroth and first order terms we may write

,

and setting  

this becomes

.

Here |g(k)| is nonzero only in a small interval about k0.  Therefore we need to integrate only over this small interval of width ~Dk.  

In the integral |k-k0| ~£ Dk

If we write exp(i(k-k0)(x-x0))=exp(i2p(k-k0)/t) with  t=2p/(x-x0) we find that for |t|<<Dk or |x-x0|>>Dk-1 the function exp(i(k-k0)(x-x0)) oscillates very rapidly in the integration interval and the integral yields approximately zero.  

For x-x0 @ 0  |t| ® ¥  and the function  exp(i2p(k-k0)/t) @ 1 in the integration interval.  Then the integral yields its maximum value.  We therefore have

.

 

is the position of the center of the wave packet.

As |x-x0| increases |y(x,0)| decreases.  We expect the width of the wave packet Dx in coordinate space to be ~Dx=Dk-1.  Then  DxDk ~³ 1.  This is the classical relation for two functions which are Fourier transforms of each other.  The product DxDk has a lower bound.  The exact value of this bound depends on the precise definition of Dx and Dk.

Assume we want to build a wave packet representing a particle which has a high probability of being observed at position r=0 in a small time interval Dt about t0;

Here and y(0,t) are Fourier transforms of each other.  If y(0,t) is centered at t0 with small width Dt, then  has width Dw  such that  DtDw ~³ 1.

The Heisenberg uncertainty relations:

Quantum Mechanics implies that it is impossible to know, at any given time, the position and the momentum of a particle to an arbitrary degree of accuracy.

Similarly:

Link:

Heisenberg's Uncertainty Principle

Example:

An excited state of an atom decays emitting an electron.  If you are reasonably sure that the electron will be emitted in a time interval Dt<10-8s after you fired a picosecond Laser, the energy of the electron must have an uncertainty

.

If the energy of the ground state is known exactly, then the energy of the excited state must be uncertain by DE.

We may write the Fourier transform of y(x,0) in the following way:

.

Then

is the probability of finding the particle at a position between x and x+dx, and

is the probability of finding the particle with momentum between p and p+dp.  The constant C is the same in both expressions.  This follows from the Bessel-Parseval relation

(See appendix I, Cohen-Tannoudji).

For a plane wave y(x,0)=Aexp(ik0x) we have Dk=Dp=0, g(k)=d(k-k0), Dx=¥ .

Examples:

Consider a dust particle (m~10-15 kg, diameter ~10-6 m, v~10-3 m/s).  If you can practically measure its position to an accuracy of 10-8 m, how accurately can you determine its momentum?

The momentum of the particle is on the order of p=mv=10-18Js/m.  There are no practical restrictions on how accurately the particle’s momentum can be measured.

Consider the Bohr model of the atom.  It is assumed that the electron’s angular momentum is quantized (pr=nh), the electron must move in an orbit which is consistent with one of the allowed values for the angular momentum.  Does it make sense to speak of a classical trajectory or orbit?
To have a well defined trajectory we need:

.

But the uncertainty principle requires DpDx ³ h.  We therefore need h<<nh, which only holds if n>>1.  The uncertainty principle rejects the semi-classical Bohr model with Bohr orbits except for high Rydberg states.

Consider the Hydrogen atom, i.e. an electron in the Coulomb field of a proton.  The potential energy of an electron in the field of a stationary proton is 

(SI units).

Let us assume a spherically symmetrical wave function with mean radius r0.  
Then x @ r0 and V @ e2/r0.  For the ground state we have E=T+V=Emin.  The uncertainty principle requires

 .

To estimate r0 we let

.

The quantitative agreement is accidental, only qualitative agreement should be expected.

Classically:

 

  Emin = -¥  at r0=0.

Problem:

Assume that virtual p mesons are emitted and absorbed by a nucleus.  From this assumption, and the p meson mass, and the uncertainty principle, estimate the range of the nuclear potential r0.
Solution:

Assume that the p meson is the mediator of the nuclear force, the nucleus emits and absorbs p mesons.  For the p meson mc2»140 MeV.  Assume the p meson exists for a time interval Dt.  It has energy

  .

For an order of magnitude estimate we use:

.

To find the minimum of the product DEDt we minimize this expression with respect to v;

Then

.

(Rule of thumb: To estimate the range of a force, divide h by the mass of the particle that carries it times c, R=h/mc).

Link:

Wave packet Explorer