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( [ current - bifur1 ] ) except for the range of @xmath0 considered.,title="fig:",width=302 ] for @xmath78 and @xmath8 , plotted are current ( upper ) and bifurcation diagram ( lower ) versus @xmath0 with @xmath62 .
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note in particular in this figure that eyeball tests can be misleading .
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we see reversals without bifurcations in ( a ) whereas the zoomed version ( c ) shows that there are windows of periodic and chaotic regimes .
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this is further evidence that jumps in the current correspond in general to bifurcation.,title="fig:",width=302 ] for @xmath7 and @xmath79 , current ( upper ) and bifurcation diagram ( lower ) versus @xmath0.,title="fig:",width=302 ] however , a * different * rule of thumb , previously not proposed , emerges from our studies .
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this generalizes mateos conjecture to say that * ( iv ) bifurcations correspond to sudden current changes ( spikes or jumps)*. note that this means these changes in current are not necessarily reversals of direction .
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if this current jump or spike goes through zero , this coincides with a current reversal , making the mateos conjecture a special case .
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the physical basis of this argument is the fact that ensembles of particles in chaotic systems _ can _ have net directed transport but the details of this behavior depends relatively sensitively on the system parameters .
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this parameter dependence is greatly exaggerated at the bifurcation point , when the dynamics of the underlying single - particle system undergoes a transition a period - doubling transition , for example , or one from chaos to regular behavior .
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scanning the relevant figures , we see that this is a very useful rule of thumb . for example
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, it completely captures the behaviour of fig .
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( [ figure6 ] ) which can not be understood as either an example of the mateos conjecture , or even a failure thereof . as such
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, this rule significantly enhances our ability to characterize changes in the behavior of the current as a function of parameter .
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a further example of where this modified conjecture helps us is in looking at a seeming negation of the mateos conjecture , that is , an example where we seem to see current - reversal without bifurcation , visible in fig .
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( [ hidden - bifur ] ) .
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the current - reversals in that scan of parameter space seem to happen inside the chaotic regime and seemingly independent of bifurcation . however , this turns out to be a ` hidden ' bifurcation when we zoom in on the chaotic regime , we see hidden periodic windows .
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this is therefore consistent with our statement that sudden current changes are associated with bifurcations .
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each of the transitions from periodic behavior to chaos and back provides opportunities for the current to spike .
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however , in not all such cases can these hidden bifurcations be found .
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we can see an example of this in fig .
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( [ rev - nobifur ] ) .
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the current is seen to move smoothly across @xmath80 with seemingly no corresponding bifurcations , even when we do a careful zoom on the data , as in fig .
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( [ hidden - bifur ] ) .
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however , arguably , although subjective , this change is close to the bifurcation point .
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this result , that there are situations where the heuristics simply do not seem to apply , are part of the open questions associated with this problem , of course .
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we note , however , that we have seen that these broad arguments hold when we vary other parameters as well ( figures not shown here ) . in conclusion ,
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in this paper we have taken the approach that it is useful to find general rules of thumb ( even if not universally valid ) to understand the complicated behavior of non - equilibrium nonlinear statistical mechanical systems . in the case of chaotic deterministic ratchets
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, we have shown that it is important to factor out issues of size , location , spread , and transience in computing the ` current ' due to an ensemble before we search for such rules , and that the dependence on ensemble characteristics is most critical near certain bifurcation points .
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we have then argued that the following heuristic characteristics hold : bifurcations in single - trajectory behavior often corresponds to sudden spikes or jumps in the current for an ensemble in the same system .
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current reversals are a special case of this
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. however , not all spikes or jumps correspond to a bifurcation , nor vice versa .
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the open question is clearly to figure out if the reason for when these rules are violated or are valid can be made more concrete .
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a.k . gratefully acknowledges t. barsch and kamal p. singh for stimulating discussions , the reimar lst grant and financial support from the alexander von humboldt foundation in bonn . a.k.p .
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is grateful to carleton college for the ` sit , wallin , and class of 1949 ' sabbatical fellowships , and to the mpipks for hosting him for a sabbatical visit , which led to this collaboration .
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useful discussions with j .-
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m . rost on preliminary results are also acknowledged .
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p. hnggi and bartussek , in nonlinear physics of complex systems , lecture notes in physics vol .
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476 , edited by j. parisi , s.c .
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mueller , and w. zimmermann ( springer verlag , berlin , 1996 ) , pp.294 - 308 ; r.d .
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asturmian , science * 276 * , 917 ( 1997 ) ; f. jlicher , a. ajdari , and j. prost , rev . mod .
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phys . * 69 * , 1269 ( 1997 ) ; c. dring , nuovo cimento d*17 * , 685 ( 1995 ) s. flach , o. yevtushenko , and y. zolotaryuk , phys
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. rev .
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lett . * 84 * , 2358 ( 2000 ) ; o. yevtushenko , s. flach , y. zolotaryuk , and a. a. ovchinnikov , europhys .
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lett . * 54 * , 141 ( 2001 ) ; s. denisov et al .
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e * 66 * , 041104 ( 2002 )
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studies of laser beams propagating through turbulent atmospheres are important for many applications such as remote sensing , tracking , and long - distance optical communications .
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howerver , fully coherent laser beams are very sensitive to fluctuations of the atmospheric refractive index .
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the initially coherent laser beam acquires some properties of gaussian statistics in course of its propagation through the turbulence . as a result , the noise / signal ratio approaches unity for long - distance propagation .
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( see , for example , refs.@xcite-@xcite ) .
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this unfavourable effect limits the performance of communication channels . to mitigate this negative effect
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the use of partially ( spatially ) coherent beams was proposed .
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the coherent laser beam can be transformed into a partially coherent beam by means of a phase diffuser placed near the exit aperture .
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this diffuser introduces an additional phase ( randomly varying in space and time ) to the wave front of the outgoing radiation .
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statistical characteristics of the random phase determine the initial transverse coherence length of the beam .
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it is shown in refs .
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@xcite,@xcite that a considerable decrease in the noise / signal ratio can occur under following conditions : ( i ) the ratio of the initial transverse coherence length , @xmath0 , to the beam radius , @xmath1 , should be essentially smaller than unity ; and ( ii ) the characteristic time of phase variations , @xmath2 , should be much smaller than the integration time , @xmath3 , of the detector .
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however , only limiting cases @xmath4 and @xmath5 have been considered in the literature .
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( see , for example , refs .
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@xcite,@xcite and ref .
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@xcite , respectively ) .
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it is evident that the inequality @xmath6 can be easily satisfied by choosing a detector with very long integration time . at the same time
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, this kind of the detector can not distinguish different signals within the interval @xmath3 .
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this means that the resolution of the receiving system might become too low for the case of large @xmath3 . on the other hand
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, there is a technical restriction on phase diffusers : up to now their characteristic times , @xmath2 , are not smaller than @xmath7 . besides that , in some specific cases ( see , for example , ref .
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@xcite ) , the spectral broadening of laser radiation due to the phase diffuser ( @xmath8 ) may become unacceptably high .
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the factors mentioned above impose serious restrictions on the physical characteristics of phase diffusers which could be potentially useful for suppressing the intensity fluctuations .
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an adequate choice of diffusers may be facilitated if we know in detail the effect of finite - time phase variation , introduced by them , on the photon statistics . in this case
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, it is possible to control the performance of communication systems . in what follows , we will obtain theoretically the dependence of scintillation index on @xmath9 without any restrictions on the value of this ratio
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this is the main purpose of our paper .
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further analysis is based on the formalism developed in ref .
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@xcite and modified here to understand the case of finite - time dynamics of the phase diffuser .
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the detectors of the absorbed type do not sense the instantaneous intensity of electromagnetic waves @xmath10 .
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they sense the intensity averaged over some finite interval @xmath3 i.e. @xmath11 usually , the averaging time @xmath3 ( the integration time of the detector ) is much smaller than the characteristic time of the turbulence variation , @xmath12 , ( @xmath13 ) .
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therefore , the average value of the intensity can be obtained by further averaging of eq .
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[ one ] over many measurements corresponding various realizations of the refractive - index configurations .
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the scintillation index determining the mean - square fluctuations of the intensity is defined by @xmath14\bigg /\big
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< \bar{i}\big > ^2=
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\frac{\big < : \bar i(t ) ^2:\big>}{\big<\bar i \big>^2}-1,\ ] ] where the symbol @xmath15 indicates the normal ordering of the creation and annihilation operators which determine the intensity , @xmath10 .
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( see more details in refs .
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@xcite,@xcite ) . the brackets @xmath16 indicate quantum - mechanical and atmospheric averagings .
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the intensity @xmath17 depends not only on @xmath18 , but also on the spatial variable @xmath19 . therefore , the detected intensity is the intensity @xmath20 averaged not only over @xmath18 as in eq .
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[ one ] , but also over the detector aperture . for simplicity , we will restrict ourselves to calculations of the intensity correlations for coinciding spatial points that correspond to `` small '' detector aperture .
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this simplification is quite reasonable for a long - distance propagation path of the beam . in the case of quasimonochromatic light
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, we can choose @xmath20 in the form @xmath21 where @xmath22 and @xmath23 are the creation and annihilation operators of photons with momentum @xmath24 .
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they are given in the heisenberg representation .
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@xmath25 is the volume of the system .
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it follows from eqs .
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[ two],[three ] that @xmath26 can be obtained if one knows the average @xmath27 it is a complex problem to obtain this value for arbitrary turbulence strengths and propagation distances .
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nevertheless , the following qualitative reasoning can help to do this in the case of strong turbulence .
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we have mentioned that the laser light acquires the properties of gaussian statistics in the course of its propagation through the turbulent atmosphere . as a result , in the limit of infinitely long propagation path , @xmath28 , only
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diagonal " terms , i.e. terms with ( i ) @xmath29 or ( ii ) @xmath30 , @xmath31 contribute to the right part of eq . [ four ] . for large but still finite @xmath28
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, there exist small ranges of @xmath32 in case ( i ) and @xmath33 , @xmath34 in case ( ii ) contributing into the sum in eq .
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the presence of the mentioned regions is due to the two possible ways of correlating of four different waves ( see ref .
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@xcite ) which enter the right hand side of eq .
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[ four ] . as explained in ref .
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@xcite , the characteristic sizes of regions ( i ) and ( ii ) depend on the atmospheric broadening of beam radii as @xmath35 , thus decreasing with increasing @xmath28 . in the case of long - distance propagation , @xmath36 is much smaller than the component of photon wave - vectors perpendicular to the @xmath28 axis .
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the last quantity grows with @xmath28 as @xmath37 .
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( see ref .
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@xcite ) . for this reason ,
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the overlapping of regions ( i ) and ( ii ) can be neglected . in this case
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eq . [ four ] can be rewritten in the convenient form : @xmath38 @xmath39 where the value @xmath40 , confining summation over @xmath41 , is chosen to be greater than @xmath42 but much smaller than the characteristic transverse wave vector of the photons ; this is consistent with the above explanations .
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