
56 SPLIT-STEP MODEL
with an arbitrary width
QQ,
the soliton's energy being E = {LD/LN)
a,o^-
Inserting
this in the limiting forms of
Eqs.
(3.21) and (3.22) corresponding to LD, LN -^ 0, one
concludes that they are satisfied automatically, i.e., the VA correctly reproduces the
exact result for the fundamental soliton in the NLS limit. The same limit corresponds
to £^
—>
0 at finite LD and LN, as in this case the soliton becomes very broad, with the
dispersion length ZD '^ cfi ^ LD, LN, hence it must be asymptotically equivalent to
the ordinary NLS soliton.
It is also relevant to note that, as it follows from Eq. (3.21), the minimum width
amin may take any value from 0 to oo when E is varied from oo to 0. However, Eq.
(3.22) shows that the maximum width Omax diverges in both limits, E ^> 0 and E -+
oo,
which suggests that there is a finite smallest value that a^ax may assume. Indeed,
analysis of
Eq.
(3.22) demonstrates that this value is (aniax)„iin ~ \/(2/7r)L£i, and it
is attained at E =
\/'1-KLDL'^.
In this case, the minimum width is (l/V2) ('^max)min-
3.2.3 Comparison with numerical results
Direct simulations of the SSM were performed in works [50, 52]. The simulations
started with the initial wave form (3.10) that would generate a fundamental soliton in
the averaged NLS equation corresponding to the SSM. In the case when the soliton
period in the averaged equation (defined as per Eq. (1.16)) is comparable to the cell's
size L, a soliton readily self-traps in the SSM, with an extremely small radiation loss
and very little change of the shape against the initial form, see an example in Fig. 3.1.
If the opposite case, with L much larger than the soliton period (with the latter de-
fined as per the average NLS equation, see Eq. (1.16)), the adjustment of the soliton
and radiation loss accompanying its relaxation to the eventual shape are quite conspic-
uous,
as shown in Fig. 3.2. In this case, the established soliton features intrinsic chirp
(i.e.,
the wave field is complex), as shown in Fig. 3.2(d). Nevertheless, the amplitude
distribution in the soliton, |'U(T)|, is still well fitted by the usual sech ansatz, see Fig.
3.2(c). In fact, the proximity of the pulse to the classical shape of the NLS soliton may
be characterized by its area,
I- + 00
A= \u{T)\dT (3.24)
(unlike the energy (1.9), the area is not a dynamical invariant of the NLS equation).
For any soliton of the average NLS equation (3.9), A = n (note that the area does not
depend on the soliton's amplitude). For the established soliton displayed in Fig. 3.2,
the area is 3.25, i.e., quite close to
TT.
If L is very large in comparison with the soliton
period in the average NLS equation, the initial pulse completely decays into radiation,
as will be explained in more detail below.
To compare the analytical results outlined above with direct simulations in a sys-
tematic way, it is more convenient to cast the constitutive equation (3.21) in a
dif-
ferent form, which determines the maximum amplitude of the SSM soliton, A^ax =
A/E/ttmin (recall that E = J^a; obviously, the largest amplitude is achieved at a point