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Submitted on 1 Jan 1990
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An alternative way of computation of amplitudes and
intensities in time-dependent Mössbauer spectroscopy
(TDMS)
I.D. Christoskov, E.I. Vapirev
To cite this version:
An
alternative
way
of
computation
of
amplitudes
and
intensities
in
time-dependent
Mössbauer
spectroscopy
(TDMS)
I. D. Christoskov and E. I.
Vapirev
Department
ofPhysics, University
of Sofia,Sofia-1126, Bulgarie
(Reçu
le 24juillet
1989,accepté
sousforme
définitive
le 13 novembre1989)
Résumé. 2014
Nous exposons une autre
façon
deprésenter
ladépendance temporelle
desamplitudes
et intensités de radiation obtenues dans desexpériences
de diffusion etd’absorption
résonnante. Des suites infinies de fonctions de Bessel avec des coefficientscomplexes
sontremplacées
par desintégrales
définiessimplement
calculables avec une seule fonction de Bessel parpoint
de tabulation. Il s’ensuit une réduction du temps de calcul pourl’ analyse
des résultatsexpérimentaux.
Abstract. 2014 An
alternative way of
presenting
thetime-dependent amplitudes
and intensities ofradiation,
corresponding
to resonantabsorption
andscattering experiments,
isdeveloped.
Infinite series of Bessel functions withcomplex
coefficients arereplaced by
simple
for calculation definiteintegrals
and the number of Bessel function calls is reduced to one per a tabulationpoint.
Thus the calculational effort for
experimental
dataprocessing
becomes smaller. ClassificationPhysics
Abstracts 24.30Classical
electromagnetic theory
-damped
oscillators,
dispersive
media,
and thecorrespondence
between thefrequency
and the time domain - has been used to describe thephenomenon
of « time filtration » both for transmission[1]
and resonantscattering
[2, 3].
Since then many similar
experiments
have beenperformed,
the interestarising
from the fact that thoseexperiments
are theonly
ones in whichquantum
effects in the time domain within the natural linewidth(or
the excited statelifetime)
could be observed.In the
present
work an alternativetechnique
(again
in terms of theelectromagnetic
approach)
isproposed
forpresenting
thetime-dependent amplitude
andintensity
ofradiation, corresponding
to resonantabsorption
andscattering experiments.
1. Resonant
absorption.
Let the source
(S)
linewidth be denotedby
Fs,
and the resonant level lifetime be,r, = 1 IF,
(h = 2 ir ).
The centralfrequency
of S is lds. The filter(F)
linewidth isT f,
its centralfrequency - w f,
and the effective resonantthickness - B = no- 0 fa.
444
n is the number of resonant absorber nuclei per
cm2,
o-o - the resonant cross-section andf a
- the recoilless fraction ofabsorption.
Thefrequency amplitude
of S isand the
frequency
amplitude
of F isHence the
time-dependent amplitude
of transmittedgamma-quanta
will be the Fourierimage
of theproduct
S(,w).
F(w ) [1] :
The factor
F,lFf
is introduced in theexponent,
thuspreserving
theabsorption
line area. If we introduce thefollowing designations
- relative shift V=
CI) s - CI) f,
relativebroadening
rs
sR =
r f/rs
[u
=(R - 1 )/2],
and time in source lifetime units T =Fs t ;
thefollowing
expression
forA,, (T,
B, R,
V )
can be obtained :J,,
are Bessel functions of order n. In TDMS transmissionexperiments
the time distribution ofcounts of transmitted
gamma-quanta
(t
= 0corresponds
to the moment of formation of theMôssbauer state in the
source)
can be describedby
thesquared amplitude
Expressions (2)
and(3)
for theamplitude
and theintensity
areusually applied
for numerical simulation ofexperiments
or forexperimental
dataprocessing
(least
squarefitting
forparameter
search,
etc.).
Nevertheless, they
are not very convenient because the series(2)
converges with reasonable accuracyonly
after order 5-7 and therefore for the calculation of(2)
at asingle
timepoint
several calls of the Bessel function are necessary. Here it should bespecified
that for the sake of better convergency the series(2)
mustalways
beabsolutely
convergent.
So,
at a fixed set ofparameters
(B,
R,
V ),
if T becomeslarge enough
and the modulus of the coefficient in front of the Bessel function exceedsunity,
the series(2)
must be transformedby
means of thegenerating
function ofln (z).
Atthat,
theapplication
of the recursion formula for calculation ofJ,,(z), n:--.
1 leads to anabrupt
loss of accuracy in thevicinity
of the critical value of T.Therefore,
it is reasonable to make use of the reverse recursion formula[6] [starting
at asufficiently big
order of the Bessel function n(e.g.
7 = 9)].
Furthermore,
the task iscomplicated
because for the purpose ofexperimental
datafitting
the transmittedintensity
Itr(T, B, R, V ),
together
with its derivatives withrespect
toall
parameters
subject
todetermination,
must be calculated for alarge
sequence of measuredThat is
why
wesuggest
a more convenientpresentation
ofexpressions
(2)
and(3).
Let us introduce thequantities a
=(u
+iV )/B
and z =ÙÔ.
If we make use of the connection[4] :
the transmission
amplitude
takes the form :The
integral
in the RHS of(4)
can be transformed :Finally,
forAtr(T,
B, R, V )
one obtains :The
intensity
takes the form :where
In this form the effect of the resonant interaction appears as an addition to the pure
exponential
decay
of the excited state in the source. Thesub-integral
function is smoothenough
and wellsuppressed
withtime,
and for areasonably
smallstep
of theargument
(which
is the case in
experimental
datafitting)
even thesimple
trapezoidal
rule for numericalquadrature
is sufficient forcalculating
theintegral.
Due to theadditivity
of theintegral only
one call of the Bessel function per tabulationpoint
is necessary, instead of several ones in the conventional case.Moreover,
its derivatives withrespect
of theparameters
(R,
B,
... )
have asimple
form.Therefore,
this methodrequires
asubstantially
smaller calculational effort. It has been tested in numerousapplications
and hasproved
to befast,
accurate andsimple
for realization. Here thefollowing
must bespecified :
if the values of theamplitude
and theintensity
are needed for a small number of remote moments oftime,
the conventional method is more suitable since the number of calls of the Bessel function does notdepend
on time.2. Resonant
scattering.
Let
/3
be the resonant thickness of alayer
of thescattering
filter.According
to theapproach
446
where
The
following generally applicable
relation[5]
between theamplitudes
Atr (T,
6,
R,
V )
andAsc(T, (3,
R,
V )
exists :Therefore,
all results demonstrated in section 1 can beapplied
in this case. For the final calculation of1 sc (T, B, R, V)
again
asimple
numericalquadrature
can beapplied,
thuseliminating
thenecessity
to use Bessel function series and allproblems
connected with their convergence. Modifications of this scheme have also been tested in severalapplications
and haveproved
to workeffectively.
References