Optical resonators and Gaussian beams

Resonator stability

General study

Let's study a cavity with a periodic structure of optical elements as described before. Its transfer matrix is

For n periods, that is n round trips inside the cavity, the transfer matrix is Tn. If we write the vector representing an optical ray at the entrance of a period, and the exit vector, then ,

T can be diagonalized , and if P is the transition matrix and xi the eigenvectors of T, we can show that (see a course on linear algebra).

We can then deduce that

    The resonator is stable if the rays stay in the vicinity of the optical axis during the propagation when n goes to infinity. In other words, pn must have an upper bound, that is and .

In addition, the eigenvalues x1 and x2 verify the following relations :

  As x1 is a priori a complex number, we write and consequently

Then, as , we must have . Finally, the relation with the matrix trace leads to .

We deduce from this the stability condition, applicable to any resonator :

or

A resonator is stable when its ABCD coefficients verify the above condition.

Application

Let's d be the length of a simple two-mirrors linear resonator (radii of curvature R1 and R2). This resonator is equivalent to a periodic sequence made of two thin lenses with focal lengthes equal to f1 (=R1/2) and f2 (=R2/2), spaced by a distance d.

The T transfer matrix is (see figure 4):

it is then easy to show that

We classically use the notation and then obtain the stability condition for any two-mirrors linear resonator :

This relation is often drawn on a diagram representing the g2(g1) space, that is with g2 as y-axis and g1 as x-axis (figure 7).


   
    Figure 7 : stability condition for a two-mirrors linear resonator and some classical resonators.
Figure 7 : stability condition for a two-mirrors linear resonator and some classical resonators. [zoom...]Info

The stability condition is then figured by two hyperboles, and the stability zones are hatched in pale blue on figure 7.

Some special cases have to be noticed :

  • Right on the hyperbole g1g2=1 : we have then d=R1+R2, and the resonator is “concentric”

  • The straight lines g1=1 et g2=1 correspond to resonators with one plane mirror (infinite radius of curvature). The Fabry-Pérot (plano-plano cavity, that is two plane mirrors) is obtained for g1=g2=1.

  • For R1 = R2 =d (g1 = g2 = 0), the resonator is “confocal”.

There is a simple graphical method to know if a 2-mirrors resonator is stable or not : the point is to check if two circles (with diameter R1 and R2 respectively) centred on the focal points F1 and F2 have an intersection (see figure 8). If they do, the cavity is stable. Moreover, the circles intersection gives the position of the waist and the Rayleigh length (those two parameters will be defined in an upcoming paragraph)


   
    Figure 8 : Graphical method to check the stability
Figure 8 : Graphical method to check the stability [zoom...]Info

Unstable resonators

A stable resonator is not a necessary condition to make a laser. In some case, if the laser medium exhibits a gain coefficient high enough to allow a high level of losses, unstable resonators can even be very useful. This is for example the case with very high power lasers.


   
    Figure 9 : An example of hemispheric unstable resonator
Figure 9 : An example of hemispheric unstable resonator [zoom...]Info

The main advantage of such resonators is that the mode volume in the cavity can be large, which leads to low power densities on the mirrors (for high power lasers, the damage threshold of the mirrors could be easily reached). Moreover, the transverse modes undergo a high level of losses in an unstable resonator, leading to a natural transverse single-mode operation of the laser.

Those type of resonators are only possible with very high gain systems, because a given ray passes only a few times inside the amplifying medium before escaping from the cavity.

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