
- •Chapter 1
- •Introduction to linear singular optics
- •I.I. Mokhun
- •Chapter 1
- •Introduction to linear singular optics
- •I.I. Mokhun
- •1.1. IntRoduction
- •1.2. Basic notions of scalar singular optics
- •1.2.1. Phase vortices
- •1.2.2. Topological charge and topological index of singular points. Elementary topological reactions
- •1.2.2.1. Topological charge
- •1.2.2.2. Topological index
- •1.2.2.3. Conservation law for topological charge
- •1.2.2.4. Elementary topological reactions
- •1.2.3. Experimental observation and identification of vortices into scalar fields
- •1.2.4. Generation of vortices using computer-generated holograms
- •1.3. Vortices and phase structure of a scalar field
- •1.3.1. Sign principle
- •1.3.2. Phase speckles. “breathing” of phase speckles
- •1.3.3. Birth of vortices
- •1.3.4. Appearance of wave front dislocations as a result of interference of waves with simple phase surfaces
- •1.3.5. Topological indices of the field of intensity. Extrema of phase and intensity. “correlation” of phase and intensity
- •1.3.6. Vortex nets. Phase skeleton of a scalar field
- •1.3.6.1. Reconstruction of the field’s phase on the basis of shifted vortex nets
- •1.3.6.2. Image reconstruction using a regular sampling found from analysis of the parameters of vortices in random field
- •1.3.6.3. Some remarks on the field reconstruction by the use of nets of the intensity sTationary points
- •1.4. Singularities of a vector field
- •1.4.1. Disclinations. Polarization singularities
- •1.4.2. Vortices of phase difference. Sign principle for a vector field
- •1.4.2.1. Field decomposition into orthogonally linearly polarized components
- •1.4.2.2. Principle of the vortex analysis of vector fields
- •1.4.2.3. Vortices of orthogonally polarized field components. Technique for study of polarizatioN singularities
- •1.4.3. “Correlation” of intensity and polariszation of the vector field
- •1.4.4. Interconnection of the component vortices and -points
- •1.4.5. Elementary polarization structures and elementary polarization singularities of vector fields
- •1.4.5.1. Polarization structures resulting from interference of orthogonally linearly polarized beams
- •1.4.5.2. Elementary polarization singularities resulting from interference of circularly polarized beams
- •1.4.5.3. Experimental mOdeling of elementary polarization singularities
- •1.4.6. Fine structure and averaged polarization characteristics of inhomogeneous vector fields
- •1.4.6.1. Avaraged stokes parameters
- •1.4.6.2. Analysis of the averaged parameters for decomposition of the field into linearly polarized components
- •1.4.6.3. Computer simulation of the vector field’s parameters
- •1.4.6.4. Analysis of the averaged parameters for the field decomposition into circular basis
- •1.4.6.5. Comparison of the experimental results and the data of computer simulation
- •1.4.7. “Stokes-formalism” for polarization singularites. “stokes-vortices”
- •1.5. Singularities of the Poynting vector and the structure of optical fields
- •1.5.1. General assumptions. Components of the poynting vector
- •1.5.2. Singularities of the poynting vector in scalar fields
- •1.5.2.1. Instantaneous singularities of a scalar field
- •1.5.2.2. Averaged singularities of the poynting vector of scalar field
- •1.5.3. Singularities of the Poynting vector at vector fields
- •1.5.3.1. Instantaneous singularities of vector field
- •1.5.3.2. Behavior of the Poynting vector in areas of elementary polarization singularities
- •1.5.3.2.1. Symmetric distributions of amplitude and phase of the interfering beams
- •1.5.3.2.2. Non-symmetrical distributions of amplitudes and phases of the interfering beams
- •1.5.3.2.3. Experimental proving of the existence of the orbital momentum in the vicinity of -point
- •1.5.3.3. The averaged Poynting vector of the vector field
- •Instantaneous singularities of the Poynting vector
- •Appendix 1.1. Wave fronts approximation
- •104. I.Mokhun, r.Brandel and Ju.Viktorovskaya, “Angular momentum of electromagnetic field in areas of polarization singularities”, ujpo, Vol. 7, pp. 63-73, (2006).
1.3.5. Topological indices of the field of intensity. Extrema of phase and intensity. “correlation” of phase and intensity
Let us emphasize that while the topological charges are intrinsic to the vortex-bearing fields alone, the Poincare index, N, can be introduced for the gradient fields as well [25]. Let us introduce the topological indices for the field of intensity and keep up with the changing of directions of the current lines for the intensity gradient in the vicinity of the stationary points. The extrema, including amplitude zeroes as the absolute minima of the field intensity, possess the index N=+1, and the saddles of intensity possess the negative index N=1. Accordingly, birth (annihilation) of the extremum must be accompanied by appearance (disappearance) of the saddle of intensity providing topological connection among the extremum and other field structures, as well as other extrema. Though the vortices and the maxima of intensity do not differ in the magnitude of the index N, nevertheless one can derive some conclusions concerning the numbers of them. It follows from simple physical considerations that if the extremum of any physical quantity exists in any area of definition of this quantity, then at least one opposite extremum must exist within the same area. Applying the approach close to the one described in [11], one concludes that the minimal number of the maxima and the saddles of intensity obeys the relation:
,
(1.24)
where
is the minimal number of maxima,
is the number of vortices, and
is the minimal number of the saddles of intensity.
Now we consider the question: how many extrema of phase and intensity might be generally?
In assumption that a complex amplitude of the field in a far zone is described by the relation
`
(1.25)
(i.e., the
dependence of a complex amplitude on
is determined by the constant phase factor alone), the following
system of equations has been derived [11,24]:
,
(1.26)
where
is the amplitude,
...etc.
are the partial derivatives of the first and the second orders from
the amplitude and phase, and in the rite sides of these equations
.
It is easily to see that the conclusion on impossibility for existence of the phase extrema in a far zone follows from the second equation (1.26). Indeed, this equation is transformed for the points of the phase extrema to the form:
,
(1.27)
which is wittingly not true, as the second derivatives at the points of extrema are always of the same sign.
However,
the analysis of the first equation (1.26) leads to much more
surprising conclusion, viz., that the maxima of intensity are
impossible in a far field. Indeed, consider the possibility of
appearance of the maxima of intensity. At these points
,
and
.
In this case, the sum of two terms of the first equation (1.26) is
always negative, while the quantity in the parentheses is always
positive. Thus, the left side of the first equation (1.26) does not
equal zero at the points of intensity maxima. This is obvious
contradiction, as the presence of amplitude zeroes presumes, at
least, the presence of the same number of intensity maxima.
Following, the assumption (1.25) is not acceptable in the case of
interest for analysis of the field in a far field.
The results of computer simulation of random fields [17,18] reliably confirm this conclusion. The authors of the cited papers state that phase extrema occur even in a far field (though in not great number). So, one additional phase extremum is on 14 to 20 vortices.
Let us attempt to cancel the contradiction following from the Eqs. (1.26). In general, the strength of the electrical field and the associated wave function are the vector quantities. As such a case, the scalar treatment of the problem is appropriate under the paraxial approximation alone. The Fourier approximation is too rough for analyzing a fine structure of the field, and we prefer use a more general Fresnel approximation (see for example ref. 53):
Let us
write a complex amplitude of the field,
,
at any distance
from the input plane within the domain corresponding to the Fresnel
diffraction:
,
(1.28)
where
is the boundary field.
To find the
explicit form of
,
we assume the area within which
change being much less than the area within which
change. In other words, we assume the area of analysis being much
larger than the transverse size of the scattering object. These
assumptions are true for the most practical situations. In this case,
one can neglect the factor
,
and Eq. (1.28) is reduced to the form:
,
(1.29)
where
,
and
designates Fourier transformation.
Then, neglecting the terms of the second order of magnitude one obtains, instead Eqs. (1.26) the following system:
.
(1.30)
For the
case of a phase extremum (
),
the Eqs. (1.30) is reduced to the form:
.
(1.31)
One can see from comparison of Eqs. (1.30) and (1.26) that the Eqs. (1.31), in contrast to the Eqs. (1.26) allows the existence of the phase extrema and asymmetric saddles.
For the
case of stationary points of intensity (
)
Eqs. (1.30) takes the form:
.
(1.32)
It follows from Eqs. (1.32) that the stationary points of intensity of all kinds (without any exclusion) exist.
One can estimate the number of the additional stationary points in comparison with the minimal number using the following considerations:
1.
The correlation length of the field,
,
is the universal characteristics of the field at far zone determining
the spatial scale of fluctuations for all other parameters of such
field [40].
2. Mean size of a speckle in determined by the same quantity, , whose magnitude coincides with an average distance between the vortices [9,12,24,55-58]. Within the field of a phase, four topological elements are associated with an “average” speckle, viz. two vortices of opposite signs and two phase saddles. That is why, probability for a speckle to possess additional topological elements, such as the extremum and the associated with it saddle, is small.
3. Mean
size of a speckle of intensity is also determined by the magnitude of
.
4. The minimal number of topological elements within the field of intensity is determined by Eq. (1.24), i.e. it is the same as for the field of a phase.
5. Birth of two topological elements accompanies appearance of the additional extremum within the field of intensity, similarly to the field of a phase.
Thus, one can conclude that probability of appearance of the additional maxima or minima of intensity must be no exceeding probability of appearance of the phase extrema.
Accordingly, one can neglect such topological elements as rather rare ones and consider that the field of intensity at far zone possesses the “main” maxima, absolute minima of intensity (phase vortices) and saddles alone.
I
Figure
1.15.
Nets
of the singular points of intensity and phase produced by the
current lines of the intensity gradient and by the lines
.
Poincare indices for the intensity maxima, phase vortices – the
absolute minima, and saddle points of intensity (
)
designated by circles.
t
is obvious, the extrema of the some kind (maximum, maximum and
minimum, minimum) are connected to each other by the saddles of
intensity. In other words, the stationary points of intensity,
similarly to the singular points of a phase, form the corresponding
net. Figure 1.15 illustrates an example of such a net. While the
elements of the net of a phase and the net of intensity are
connected, intensity and a phase, to all appearance, can not change
independently [17-26].
Let us analyze the interconnection of the vortex net characterizing the phase behavior and the net of stationary points of intensity. To do this, we find out average magnitudes of the phase gradient and the intensity gradient in the stationary points of intensity and phase, respectively [25,26].
Modula of the gradients of intensity and phase are determined by the following equations:
,
(1.33)
,
(1.34)
where J
and
R
are the imaginary and the real parts of the complex amplitude U,
and
,…
are the partial derivatives of them,
.
Modula of these gradients at the stationary points are of the form:
at the stationary point of intensity:
;
(1.35)
at the stationary point of a phase:
.
(1.36)
It is
obvious, the average magnitudes of
and
and of their derivatives equal zero. We can assume that the
statistics of these quantities is the same. Then, analyzing Eqs.
(1.33, 1.34) and (1.35, 1.36), one can show that modulus
of a mean phase gradient at the stationary point of intensity is
times larger than in any other point of the field (excluding the
vortex zones).
The same is true for the stationary points of intensity. Namely,
modulus
of a mean intensity gradient at the stationary point of a phase is
times larger than in any other point of the field.
Thus we have established that in
statistical sense, slow changes of a phase correspond to fast changes
of intensity, and
vise versa, intensity
changes slowly within the areas where a phase changes rapidly
[20,21,25.26].
Figure
1.16.
Interconnection between the behavior of a phase and intensity of
scalar random field. (a) – intensity distribution; (b) – modulus
of the intensity gradient; squares designate the vortices of the
field; (c) – a phase map; phase magnitude corresponds to the level
of grey; (d) – loci of the zones with large modulus of the phase
gradient (
)
and with small modulus of the intensity gradient (
);
(e) – the stationary points of intensity and their loci in respect
to the field zones with large modulus of the phase gradient.
Note, the intensity maxima occur in the centers of speckles, near the saddle points of a phase [17,18]. Thus, the saddle points of intensity occur at zones with large magnitude of the phase gradient.
The results of computer simulation of scalar random field are shown in Figure 1.16. Fragments Figure 1.16(a),(b),(c) illustrate the behavior of intensity, and the modula of intensity gradient and phase gradient, respectively. Loci of zones with large magnitude of the modulus of the phase gradient and small magnitude of the intensity gradient are shown in Figure 1.16(d). One can see from Figure 1.16(d) that localizations of such zones are equal, in quite agreement with the above consideration. The regions of the field with small magnitude of the intensity gradient, where the intensity maxima are located, are the exclusions. This circumstance is additionally illustrated in Figure 1.16(e), where zones with considerable magnitude of the phase gradient and loci of the intensity maxima and saddle points of intensity are shown. One can see that almost all saddle points of intensity are in the areas of the field where a phase of the field changes rapidly.