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More about Tunnelling Times, the Dwell Time and the
“Hartman Effect”
Vladislav Olkhovsky, Erasmo Recami, Fabio Raciti, Aleksandr Zaichenko
To cite this version:
Vladislav Olkhovsky, Erasmo Recami, Fabio Raciti, Aleksandr Zaichenko. More about Tunnelling
Times, the Dwell Time and the “Hartman Effect”. Journal de Physique I, EDP Sciences, 1995, 5 (10),
pp.1351-1365. �10.1051/jp1:1995202�. �jpa-00247141�
J. Phys. I France 5
(1995)
1351-1365 OCTOBER 1995, PAGE 1351Classification Physics Abstracts
73.40Gk 03.80+r 03.65Bz
More about TunnelEng Times, trie Dwell Time and trie "Hartman
Elfiect" (*)
Vladislav S.
Olkhovsky (~),
Erasmo Recami(2),
Fabio Raciti(3)
and Aleksandr K.Zaichenko
(~)
(~) Institute for Nuclear Research, Ukrainian Academy of Sciences, Kiev, Ukraine and I.N.F.N., Sezione di Catania, 57 Corsitalia, Catania, Italy
(~) Facoltà di Ingegneria, Università Statale di Bergamo, Dalmine
(BG),
Italy; I.N.F.N., Sezione di Milano, Milan, Italy; Dept. of Apphed Mathematics, State University at Campinas, Camp- inas, S-P-, Brazil(~) Dipartim. di Fisica, Università di Catania, Catama, Italy
(~) Institute for Nuclear Research, Ukrainian Academy of Sciences, Kiev, Ukraine
(Received
18 April 1995, received in final form 29 May 1995, accepted 20 June1995)
Abstract. In a recent review paper
[Phys.
Reports 214(1992)
339] we proposed, withinconventional quantum mechanics, new definitions for the sub-borner tunnelling and reflection times. Aims of the present paper are: 1) presenting and analysing the results of various numerical
calculations
(based
on our
equations)
on the penetration and retum times < rp~n >, < rRet >, during tunnelling inside a rectangular potential barrer, for vanous penetration depths xi;ii)
putting fortin and discussmg suitable definitions, besides of the mean values, also of the uanances
(or dispersions)
DTr and DrR for the time durations of transmission and reflection processes;iii) mentioning, moreover, that our definition < rr > for the average transmission time results to constitute an improuement of trie ordinary dwell-time f~~ formula:
iv)
commenting, at last,on the basis of our new numencal results, upon some recent criticism by C.R. Leavens. We stress
that our numencal evaluations confim that our approach implied, and implies, the existence
of the lfartman ejfect: an effect that in these days
(due
to the theoretical connections between tunnefling and evanescent-wavepropagation)
is receivmg -at Cologne, Berkeley, Florence andVienna- indirect, but quite interesting, expenmental venfications. Eventully, we briefly analyze
some other definitions of tunnelling times.
1. Introduction
In our review article
[ii
we put forth ananalysis
of the main theoretical definitions of the sub-barrertunnelling
and reflection times, andproposed
new definitions for such durations(*)Work
partially supported by INFN, MURST and CNR(Italy),
by CNPq(Brazil),
and by the I.N.R.(Kiev, Ukraine)
and S-K-S-T- of Ukraine(project
no.2.3/68).
© Les Editions de Physique 1995
which seem to be self-consistent within con~entionai quantum nlechanics
(~).
In
particular,
the"prediction" by
ourtheory [ii
of thereality
of the Hartmanejfect
[2] intunnelling
processes hasrecently
received -due to theanalogy
[3] betweentunnelling
electronsand evanescent waves- quite
interesting,
even ifindirect, experimental
verifications atCologne
[4],
Berkeley
[5], Florence [6] and Vienna [6].Main a1nls of the present paper are:
presenting
andanalysing
the results of several numerical calculations of thepenetration
and return times inside arectangular potential
barrierduring tunnelling (Sect. 3);
andproposing
new suitable formulae for the distribution variances of the transmission and reflection times(Sect. 2).
The results of our numerical evaluations seem to confirm that ourapproach
isphysically acceptable,
and that it moreoverimplied,
andimplies,
the existence of the so-called "Hartman
ejfect
" even fornon-quasi-nlonochromatic packets.
The present research
field,
however, isdeveloping
sorapidly
and in such a controversial manner, that it may be convenient to add here -before ail- some brief comnlents about a few papersappeared during
the last three years:1)
First,
let us mention that we had overlooked a new expression for the dwell-limeY~~
derived
by Jaworsky
and Wardlaw[7,8]
Y~~ (xi,
~i;k)
=/~
dt tJ(xf, t) /~
dt tJ(xi,
t)) /~
dt J;n(xi,
t))
~
il
-m -m -m
which is indeed
equivalent
[7] to ourequation (16)
of reference[ii (all
notationsbeing
defined
therein):
ce xi ce -1
Y~~ (~;,
xf;k)
=~Îoe
dtÎ,
dzp(~, t) ~Îoe
dt Inlx;, t) (2)
This
equivalence
reduces thedifference,
between our definition < rT > of the average transmission lime -under oufassumptions-
andquantity Y~~,
ta the difference betweenthe average made
by using
thepositive-definite probability density
dtJ+(x,t)/ fc~dtJ+(x,t)
and the average madeby using
theordinary "probability density"
dtJ(x,t)/ fÎ~
dtJ(x,t). Generally speaking,
the lastexpression
is notalways
positive
definite,
as it wasexplained
at page 350 of reference[ii,
and hence does non possess any directphysical meaning.
ii)
In reference [9] an attempt was made toanalyze
the evolution of the wavepacket
mean position <x(t)
>("center
ofgravity" ), averaged
overpdx, during
ilstunnelling through
a
potential
barrier. Let us here observe that the conclusion to be foundtherein,
about the absence of a causal relation between the incident space centroid and its transmittedequivalent,
holdsoniy
when the contributioncoming
front the barrierregion
to the spaceintegral
isnegligible.
iii)
Let us also add that in reference[loi
it wasanalyzed
the distribution of the transmission time rT in a rathersophisticated
way, which is very similar to the dwell-timeapproach,
however with an
artificial, abrupt switching
on of the initial wavepacket.
We aregoing
to propose, on the contrary, and inanalogy
with ourequations (30)
to(31)
in reference [11, (~) Let us take advantage of the present opportumty for pointing out that a mispnnt entered our equation(10)
in reference [1], whose last term ka ought to be elimmated. Moreover, due to an editorial error, m the footnote at page 32 of Dur reference [16] the dependence of G on Ak disappeared,whilst in that paper we had assumed
G(k Î)
% Cexp[-(k
k)~/(Ak)~]
N°10 TUNNELLING TIMES AND THE "HARTMAN EFFECT" 1353
the
following
expressions, asphysically adequate
definitions for the ~ariances(or disper- sions)
DrT and DrR of the transmission and reflection time[see
Sect.2], respectively:
DTr
+Dt+ lxf)
+Dt+ (xi
13)and
DrR
+ Dt-ix;
+ Dt-(xi (4)
where
ii
dl t~J+jx, tj ii
dt tJ+jx, tj
~~~~ i~i
~jr~
dtJ+ j~, t) jz~
dtJ+ j~, t)
i~~Equations (3)
to(5)
are based on the formalismexpounded
in reference[iii,
as wellas on our definitions for
J+(~,t)
in referenceiii.
Of course, we aresupposing
that theintegrations
overJ+(~f)dt, J+(x;)dt
andJ-(x;)dt
areindependent
of one another. We shall devote Section2, below,
to theseproblems,
1-e-, to theproblem
ofsuitably defining
mean values and variances of
durations,
for various transmission and reflection processesduring tunnelling.
iv) Below,
in Section4,
we shallbriefly re-analyse
some other definitions oftunnelling
dura- tions.Before
going
on, let us recall that several reasons"justify"
the existence of different ap-proaches
to the definition oftunnelling
times:a)
theproblem
ofdefining tunnelling
durations isdosely
connected with that ofdefining
a time operator, 1-e-, ofintroducing
time as a(non-
selfadjoint)
quantum mechanicalobservable,
andsubsequently
ofadopting
ageneral
definition for collision durations in quantum mechanics. Suchpreliminary problems
did receive some clar-ification in recent times
(see,
forexample,
reference[ii
and citations [8] and [22]therein); b)
the motion of a
particle tunnelling
inside apotential
barrier is apurely
quantumphenomenon,
devoid of anyclassical,
intuitivelimit; c)
the various theoreticalapproaches
may dioEer in the choice of theboundary
conditions or in themodelling
of theexperimental
situations.2. Mean Values and Variances for Various Penetration and Return Times
during
Tunnelling
In our previous papers, we
proposed
for the transmission andreflection
times some formulae whichimply
-as functions of the penetrationdepth- integrations
over time ofJ+ ix, t)
andJ-
ix, t), respectively.
Let us recall that the total fluxJ(x,t)
inside a barrier consists of two components,J+
and J-, associated with motionalong
thepositive
and thenegative
x-direction,respectively.
Work in similar directions didrecently
appear in reference [12].Let us refer ourselves -here- to
tunnelling
and reflection processes of apartide by
apotential barrier, confining
ourselves to one space dimension.Namely,
let usstudy
the evolution of a wavepacket l#(x,t), starting
from the initial statel#in(x,t);
and follow the notation introduced in reference[ii.
In the case of uni-directional motions it isalready
known [13]that the flux
density J(x,t)
eRe[(ià/m) l#(x,t) àl#*(x,t)/ôx]
can beactually interpreted
as the
probability
that thepartide (wave packet)
passesthrough position
xduring
a unitary time-interval centered at t, as iteasily follows from
thecontinuity eq~ation
andfrom
thefact
that
quantity p(x,t)
e(l#(x,t)(~
is theprobabiiity density
for our"partide"
to belocated,
at time t, inside a unitary space-interval centered at x.Thus,
in order to determine the meaninstant at which a
moving
wavepacket l#(x, t)
passesthrough
position x, we have to take theaverage of the time variable t with respect to the
weight w(x, t)
%J(x, t) / ff~~ J(x, t)
dt.However,
if the motion direction can ~ary, thenquantity w(x, t)
is nolonger positive definite,
and moreover is not
bounded,
because of thevariability
of theJ(x, t) sign.
In such a case, onecan introduce the two
weights:
w+
ix, t)
m
J+ ix, t) /°' J+ ix, tj tj
~~j6j
w~jx,tj
mJ~jx,tj /°' J~jx,tj tj
~~jij
where
J+(x, t)
and J-lx, t)
represent the positive andnegative
parts ofJ(x,t), respectively,
which are
bounded, positive-definite functions,
normalized to 1. Let us showthat,
from theordinary probabilistic interpretation
ofp(x, t)
and from the well-knowncontinuity equation
apjx, tj aJjx, tj
at + ax = ° 18)
it follows aiso in this
(more generai)
case that quantities w+ and w-,represented by
equa-tions
(6), iii,
can beregarded
as theprobabilities
that our"particle"
passesthrough position
x
during
a unit time-interval centered at t(in
the case of forward and backward motion,respectively).
Actually,
for those time mtervals for which J=
J+
or J= J-, one can rewrite equation
(8)
as follows:
~~ÎÎ~
~~
~~ÎÎÎ~
~~ ~~~~~~ÎÎ~
~~ ~~
ÎÎ~
~~~~~~
respectively.
Relations(9a)
and(9b)
can be considered as formal definitions ofôp> lût
andôp< lût.
Let us nowintegrate equations (9a)
and(9b)
over time from -cc to t; we obtain:p>
ix, t)
=
j~ ~~(~'~~~
dt'j10a)
p<
ix, t)
m/~ ôJ-j~'~')
dt'jiob)
with the initial conditions p>
(x, -ccl
=
p<(x, -cc)
= 0. Then, let us introduce the quantities
N> ix,
cc;t)
e p>ix', t)
dz'=
J+ ix, t')
dt' > 0il la)
Î~ oe
N< j-cc,
x;t)
e/~ p<jxi, t)
dz' m/~ J~jx, t')
dt' > ojiib)
which have the
meaning
ofprobabilities
for our"partide"
to be located at time t on thesemi-axis
ix, cc)
or(-cc, x) respectively,
as functions of the flux densitiesJ+ lx, t)
or J-lx, t),
provided
that the normalization conditionfÎ~ p(x, t)dx
= 1 is fulfilled. The r-h-s-'s of equa- tions
Il la)
and(1lb)
have been obtainedby integrating
the r.h.s.'s of equations(10a)
and(lob)
and
adopting
theboundary
conditionsJ+(-cc,t)
=
J-1-cc, t)
= 0. Now,
by dioEerenciating
equations(lia)
and(llb)
with respect to t, one obtains:~~~ijj "'~~
=J+jx, t)
> 0j12a)
N°10 TUNNELLING TIMES AND THE "HARTMAN EFFECT" 1355
~~~~( "'~~
= J-lx, t)
> 0.(12b) Finaiiy,
fromequations (lia), (llb), (12a)
and(12b),
one can infer that:~°~~~'~~ ~Î(Î~~ÎÎÎÎ~
~~~~~~°-l~,t)
"
~))~j£))/~ l13b)
, ,
which
justify
the abovementionedprobabilistic
interpretation of w+ix, t)
and w-ix, t).
Let us notice,incidentally,
that ourapproach
does not assume any ad hocpostulate, contrarily
to what believedby
the author of reference [14].At this
point,
we caneventually
define the mean ~aiue of the time at which our"parti-
de" passes
through
position x,travelling
in thepositive
ornegative
direction of the x axis,respectively,
as:ff~~
tJ+
(X,t)
dt~ ~~~~~ ~
ff~~ J+
(X,t)
dt ~~~~~ii tJ~jx, t)
dt<
~-i~i
> ~jz~ J-ix, tj
dti~~~i
and,
moreover, the ~ariances of the distributions of these times as:ii
t~J+ ix, t)dt
~~~
i~~ ~jz~ J+j~, tjdt l~
~~i~~~i
~ i~~~~~~-i~~
+Îi~ J~jÎ, )Ît
1<~-i~i >i~ i~~~i
in accordance with the
proposal presented
in referencesil,15].
Thus,
we have a formahsm fordefining
mean values, variances(and
other centralmoments)
related to the duration distributions of all
possible
processes for apartide, tunnelling through
a
potential
barrier located in the interval(0,a) along
the ~ axis; and notonly
fortunnelling,
but also for all
possible
kinds ofcollisions,
witharbitrary energies
andpotentials.
For instance,we have that
<
r~j~~,x~j
> a <t+jx~j
> <t+j~jj
>j16j
with -cc < ~j < 0 and a < ~f < cc; and therefore
(as
anticipated in equation(3))
that~TT (~i, ~f)
~
~~+(~f)
~~~+ (~i
for transmissions from region
i-cc, 0)
to region(a, cc)
which we called[ii regions
I and III,respectively. Analogously,
for the pure(complete) tunnelling
process one has:<
~Tuni°, ~)
> ~ <t+i~)
> <t+i°)
>i~~)
and
DrTuni0, aj
aDt+ jaj
+Dt+ j0j il 8j
while one has
<
rpen(0,~f)
> + <t+(~f)
> <t+(0)
>(19)
and
Drpen
(0, ~f)
+Dt+ (xf)
+Dt+ (0) (20)
[with
0 < xf <ai
for penetration mside the barrierregion (which
we calledregion II).
Moreover:
<
r~e~(~,x)
> e <t~(x)
> <t+(x)
>(21)
Dr~e~
(x, x)
e Dt~(xi
+Dt+ ix) j22)
[with
0 < x <ai
for "returnprocesses"
inside the barrier. Atlast,
forreflections
inregion I,
we have that:
<
r~jx;, xi)
> + < t~(xi)
> <t+jx~)
>j23) [with
-cc < xi <ai,
and(as
anticipated inequation (4))
that DrR(xj, xi)
+ D t-(xi)
+ D t+(xi).
Let us stress that our definitions hold within the framework of conventional quantum me-
chanics,
without the introduction of any newpostulates,
and with thesingle
measureexpressed by weights (13a), (13b)
for all time averages(both
in the initial and in the finalconditions).
According
to ourdefinition,
thetunnelling phase
time(or, rather,
the transmissionduration),
defined
by
the stationaryphase
approximation forquasi-monochromatic partides,
ismeaningful oniy
in the limit xi- cc when
J+ ix, t)
is the fluxdensity
of the initialpacket
Jjn of incomingwaves
(in
absenceof reflected
wa~es,therefore).
Analogously,
the dwelltime,
which can berepresented (cf. Eqs. (l)
and(2) by
theexpression
[7,8,16]
Y~~(xi> xf)
=/~
tJ(xf, t)
dt/~
tJ(xi> t)
dt/~ Jin(xi, t)
dt,
-m -m -m
with -cc < ~j < 0, and ~f > a, is not
acceptable, generally speaking.
Infact,
theweight
in the time averages ismeaningful, positive
definite and normalized to 1oniy
in the rare cases when ~j - -cc and Jjn = JIIIii-e-,
when the barrier istransparent).
3. Penetration and Return Process
Durations,
inside aRectangular Barrier,
forTunnelling
Gaussian Wave Packets: Numerical ResultsWe put forth here the results of our calculations of mean durations for various
penetration (and return)
processes, inside arectangular barrier,
fortunnelling gaussian
wavepackets;
oneof our aims
being
tomvestigate
thetunneiiing speeds.
In ourcalculations,
the initial wavepacket
isl#jn(x, t)
=/ ~ G(k -1) exp[ikx iEt/à]
dk(24)
with
G(k ii
eCexp[-(k -1)~ /(2 Ak)~] (25)
ezactly
as in reference [8]; and with E =à~k~/2m; quantity
Cbeing
the normalization constant, and m the electron mass. Ourprocedure
ofintegration
was descnbed in reference [16].N°10 TUNNELLING TIMES AND THE '~HARTMAN EFFECT" 1357
1o
io
0 2 3 5
X(À)
Fig. 1. Behaviour of the average penetration time <
rp~n(0,x)
>(expressed
inseconds)
as afunction of the penetration depth xi % x
(expressed
inAngstroms)
through a rectangular barrier with width a= 5 À, for Ak
= 0.02 À~~
(dashed fine)
and Ak= 0.01 À~~
(continuous fine),
respectively.The other parameters are listed in footnote
(1).
It is worthwhile to notice that < rpen > rapidlyincreases for the first, few initial àngstroms (+~ 2.5
À),
tending afterwards to a saturation value. Thisseems to confirm the existence of the so-called "Hartman eifect" [1,
2,15].
Let us express the
penetration depth
inAngstroms,
and the penetration time m seconds.In
Figure
1 we show theplots corresponding
to a = 5À,
for Ak= 0.02 and 0.01
À~~,
respectively.
The penetration time < rpen >always
tends to a saturation value.In
Figure
2 weshow,
for the case Ak= 0.01
À~~,
theplot corresponding
to a = 10À.
Itis
interesting
that < rpen > ispractically
the same(for
the sameAk)
for a= 5 and a
= 10
À,
a result that
confirm,
let us repeat, the existence[ii
of the so-called Hartmanejfect
[2]. Let usadd
that,
when varying the parameter Ak between 0.005 and 0.15À~l
andletting
a to assume values evenlarger
than 10À, analogous
results have beenalways
gotten. Similar calculations have beenperformed (with
quite reasonableresults)
also for variousenergies
É in the range 1to10 eV
(~).
In
Figures
3, 4 and 5 we show the behaviour of the meanpenetration
and return durations as function of the penetrationdepth (with
xi= 0 and 0 < xf e x <
a),
for barriers withheight
Vo " 10 eV and width a
= 5
Àor
10À.
InFigure
3 we present theplots
of <rpen(0, xi
>correspol~ding
to different values of the mean kinetic energy: É= 2.5 eV, 5 eV and 7.5 eV
(plots
1, 2 and 3,respectively)
with Ak = 0.02À;
and E = 5 eV with Ak = 0.04À~~ (plot 4), always
with a= 5
À.
InFigure
4 we show theplots
of <rpen(0, xi
>,corresponding
to (~) For the interested reader, let us recall that, when integrating over dl, we used the interval-10~~~
s to
+10~~~
s
(symmetrical
with respect to t =o),
very much larger than the tempo- ral wave packet extension.[Recall
that tl~e extension in time of a wave packets is of the order of1/(ô6k)
=
(Akfi$)~~
ci 10~~~ si. Our "centroid" has been always ÉD
" 0j ~o = 0. For clanty's
sake, let us underline again that in our approach the initial wave packet 4fjn(~,
t)
is net regarded as prepared at a certain instant of time, but it is expected to flow through any(initial)
point ~, dunng the infinite time intervalj-oc, +oc),
even if with a jimte time-centroid to. The value of such centrera to is essentially defined by the phase of the weight amplitudeG(k k),
and in our case is equal to 0when
G(k
k) is real.0 2 6 8 10
X(À)
Fig. 2. Trie same plot as m Figure 1, for Ak
= 0.01
À~~,
except that Dow trie barrer width isa = 10 À. Let
us observe that the numencal values of the
(total)
tunnelling time < rr > practicallydoes not change when passing from a
= 5 À to
a = 10
À,
again in agreement with the charactensticfeatures 1 of the Hartman eifect. Figures 1 and 2 do improve
(and correct)
the corresponding ores,preliminarily presented by us in reference [16].
q
Î
Îc~
Î)~~0 0 2.0 3.0 1-O 5.0
(À)
Fig. 3. Behaviour of <
rPen(0,~)
>(expressed
inseconds)
as a function of ~(expressed
inAngstroms),
for tunnelling through a rectangular barrer with width a= 5 À and for diiferent values of É and of Ak.
(curve
1): Ak= 0.02 À~~ and E
= 2.5 eV;
(curve
2): Ak= 0.02 À~~ and É
= S-o eV;
(curve
3): Ak= 0.02 À~~ and E
= 7.5 eV;
(curve
4): Ak= 0.04 À~~ and E
= s-ù eV.
N°10 TUNNELLING TIMES AND THE "HARTMAN EFFECT" 1359
2
0 2 6 B 10
X(À)
Fig. 4. Behaviour of <
rp~n(0,
~) >(in seconds)
as a function of ~(in
Angstroms) for É= 5 eV
and diiferent values of a and Ak.
(curve
1): a= 5 À and Ak
= 0.02 À~~;
(curve
2): a= 5 À and
Ak = 0.04 À~~;
(curve
3): a =10 À and Ak= o.02 À~~;
(curve
4): a = 10 À and Ak= 0.04 À~~.
a = 5
À,
with Ak= 0.02
À~~
and 0.04À~~ (plots
1 and2, respectively);
and to a = 10À,
with Ak
= 0.02
À~~
and 0.04À~~ (plots
3 and 4,respectively),
the mean kinetic energy Ebeing
5eV,
1-e-, one half of Vo.In
Figure
5 theplots
are shown of <rRet(x, xi
>. The curves 1, 2 and 3correspond
toÉ
= 2.5
eV,
5 eV and 7.5eV, respectively,
for Ak= 0.02
À~~
anda = 5
À;
the curves 4,5 and 6
correspond
to E = 2.5eV,
5 eV and 7.5 eV,respectively,
for Ak= 0.04
À~~
anda = 5
À;
while the curves7,
8 and 9correspond
to Ak= 0.02
À~~
and 0.04À~~, respectively,
forÉ
= 5 eV and a
= 10
À.
Also from trie new
Figures
3-5 one can see tl~at:1)
at variance with reference [8], noplot
consideredby
us for tl~e meanpenetration
duration < rpen(0, xi
> of our wavepackets
presents any interval withnegative values,
nor with adecreasing
<rpen(0, x)
> forincreasing
x;and,
moreover, that
2)
the meantunnelling
duration <rTun(0, a)
> does notdepend
on the barrier width a("Hartman effect");
andfinally
that3) quantity
<rTun(0, a)
> decreases when theenergy increases.
Furthermore,
it is noticeable that also fromFigures
3-5 we observe:4)
arapid
increase for the value of the electronpenetration
time m the initial part of the barrierregion (near
x=
0);
and5)
atendency
of <rpen(0, x)
> to a saturation value m the final part of thebarrier,
near x = a.Feature 2,
firstly
observed forquasi-monocl~romatic partides,
[2] doesevidently
agree with thepredictions
made m reference[ii
forarbitrary
wavepackets.
Feature 3 is also m agreement with previous evaluationsperformed
forquasi-monochromatic
partiales andpresented,
for in- stance, in references[1,2,15].
Features 4 and 5 can beapparently explained by
interference8
0 2 6 8 10
x
(À)
Fig. 5. Behaviour of <
rRet(~,~)
>(in
seconds) as a function of ~(in
Angstroms) for diiferent values of a, É and Ak.(curve
1): a = 5 À, E = 2.5 eV and Ak = o.02 À~~;(curve
2): a = 5À,
É= à-o eV and Ak
= 0.02 À~~;
(curve
3): a = 5À,
E= 7.5 eV and Ak
= 0.02 À~~;
(curve 4):
a = 5
À,
E= 2.5 eV and Ak
= o.02 À~~;
(curve
5): a= 5
À,
É= S-o eV and Ak
= 0.02
À~~; (curve
6): a = 5À,
E= 7.5 eV and Ak
= 0.02 À~~;
(curve
7): a= 5
À,
E = S-o eV and Ak= 0.02 À~~;
(curve
8): a= 5
À,
E= S-o eV and Ak
= 0.02 À~~.
between those initial
penetrating
andreturning
waves inside thebarrier,
whosesuperposition yields
tl~eresulting
fluxesJ+
and J-. Inparticular,
if in tl~e initial part of tl~e barrier tl~eretuming-wave packet
iscomparatively large,
it doesessentially extinguisl~
theleading edge
of theincoming-wave packet. By
contrast, if forgrowing
x the returning-wavepacket quickly vanishes,
then the contribution of theleading edge
of theincoming-wave
packet to the meanpenetration duration <
rpen(0,x)
> doesinitially (quickly)
grow, while in the final barrierregion
its increase doesrapidly
slow down.Furthermore,
thelarger
is the barrier width a, thelarger
is the part of the backedge
of themcoming-wave
packet
which isextinguished by
interference with thereturning-wave packet.
Quantitatively,
thesephenomena
will be studied elsewhere.Finally,
m connection with theplots
of <rRet(x,x)
> as a function of x,presented
inFigure
5, let us observe that:i)
themean reflection duration <
rR(0, 0)
> % <rRet(0, 0)
> does notdepend
on the barrier width a;ii)
incorrespondence
with the barrier region betwen 0 andapproximately
0.6 a, the value of <rRet(0,x)
> is almost constant; whileiii)
its value increases with xonly
m the barrierregion
near x = a(even
if it should bepointed
out that our calculations near x = a are not sogood,
due to the very small values assumedby fÎ~
J-ix, t)dt therein).
Let us notice that point 1), also observedfirstly
forquasi-monochromatic partides,
[2] is as well in accordance with the results obtained in reference [1] forarbitrary
wavepackets. Moreover,
also pointsii)
and
iii)
can beexplained by
interferencephenomena
mside the barrier:if,
near x= a, the
initial
returning-wave packet
is almosttotally quenched by
the initial mcommg-wavepacket,
N°10 TUNNELLING TIMES AND THE "HARTMAN EFFECT" 1361
then
only
anegligibly
smallpiece
of its backedge (consisting
of the components with the smallestvelocities)
does remain. Withdecreasing
xix
-0),
theunquenched
part of thereturning-wave packet
seems to become more and morelarge (containing
more and morerapid components),
thusmaking
the difference <rRet(0,x)
> <rpen(0,x)
> almost constant.And the interference between
inconling
and reflected waves atpoints
x < 0 doeseffectively
constitute a
retarding phenomenon
[so that < t-ix
=
0)
> islarger
than <rR(x
=
0)],
whichcan
explain
tl~elarger
values of <rR(x
= 0,~
=
0)
> in comparison with <rTun(x
= 0,
~ =
a)
>.Therefore our
evaluations,
in ail the cases consideredabove,
appear to confirm ourprevious analysis
at page 352 of reference [1], and our conclusions thereinconcerning
inparticular
thevalidity
of the Hartman effect also fornon-quasi-monochromatic
wavepackets.
Even more, since the interference betweenincoming
and reflected waves before the barrier(or
betweenpenetrating
andretuming
waves, inside thebarrier,
near the entrancewall)
doesjust
increase thetunnelling
time as well as the transmissiontimes,
we can expect that our non-relativisticformulae for <
rTun(0, a)
> and <rT(xj
< 0, xf >a)
> willalways
forwardpositive
values(~).
At this
point,
it is necessary -however- to observe thefollowing.
Even if our non-relativistic equations are notexpected (as
we havejust seen)
toyield negative
times, nevertheless oneought
to bear in mind that(whenever
it is met anobject, tJ, travelling
atSuperluminal speed) negative
contributions should beexpected
to thetunnelling
times: and thisought
not to beregarded
asunphysical.
Infact,
whenever an"object"
tJ o~ercomes the infinitespeed
[18] with respect to a certainobserver,
it will afterwards appear to the same observer as its"anti-object"
à travelling
in theopposite
space direction[18].
For instance, whenpassing
from the lab toa frame F moving in tl~e same direction as the
partides
or waves entenng tl~e barrierregion,
theobjects
tJpenetrating through
the final part of the barrer(with
almost infinitespeeds,
like in
Figs. 1-5)
will appear in the frame F asanti-objects à crossing
thatportion
of the barrier in theopposite space-direction
[18]. In tl~e new frameF, therefore,
suchanti-objects à
would
yield
anegati~e
contribution to thetunnelling
time: which could evenresult,
intotal,
to be
negative
[2]. For anyclarifications,
see references[18]. So,
we have noobjections
apriori against
the fact that Leavens canfind,
in certain cases,negative
values [8,iii:
e-g, whenapplying
our formulae to wavepackets
with suitable initial conditions. What we want to stress here is that the appearance ofnegative
times(it being predicted by Relativity itself,
[18] when in presence ofanything travelling
faster thanc)
is not a valid reason to rule out a theoreticalapproach.
At
last,
let us-incidentally-
recall and mention thefollowing
fact. Someprel1nlinary
calculations of
penetration
times(inside
arectangular barrier)
fortunnelling gaussian
wavepackets had been
presented by
us in 1994 in reference [16]. Later on-looking
for anypossible explanations
for thedisagreement
between the results in reference [8] and in our reference[16]-
wediscovered, however,
that anexponential
factor wasmissing
in a term of one of trie fundamental formulae on which the numericalcomputations (performed by
our group inKiev)
were based: a mistake that could not be
detected,
of course,by
our careful checks about the(~)A diiferent daim by Delgado, Brouard and Muga [17] does not seem to be relevant to our calcu-
lations, smce it is based once more, hke reference [8], not on our but on diiferent wave packets
(and
over-barrer components are also retained in reference [17], at vanance with us). Moreover, m their
classical example, they overlook the fact that the
mean entrance time < t+(0) > gets contribution
mainly by the rapid components of the wave packet; they forget, m fact, that the slow components
are
(almost)
totally reflected by the initial wall, causing a quantum-mechanical reshaping that con- tributes to the initial "time decrease" discussed by us already in the last few paragraphs of page 352in reference [1]. All such phenomena reduce the value of <
t+(0)
>, and we expect it to be(m
ournon-relativistic
treatment)
less than <t+(a)
>.computing
process.Therefore,
trie new results of oursappearing
inFigures
1-2 shouldreplace Figures
1-3 of reference [16]. One may observetl~at, by using
the same parameters as(or
parameters very near
to)
the onesadopted by
Leavens for hisFigures
3 and 4 in reference [8],our new, corrected
Figures
1 and 2 result to be more similar to Leavens' than the uncorrectedones
(and
this is of course a welcome step towards the solution of theproblem).
One canverify
once more,however,
that ourtheory
appears toyield for
those parametersnon-negative
results for <
rpen(xf)
>,contrarily
to a daim in reference [8].Actually,
ourprevious general
conclusions have not been
apparently
affectedby
the mentioned mistake. Inparticular,
tl~e value of <rpen(xf)
> increases withincreasing
xf, and tends to saturation for xf - a. Weacknowledge, however,
that the difference in theadopted integration
ranges[-cc
to +cc for us, and 0 to +cc forLeavens]
does Dotplay
animportant role, contranly
to ourprevious belief,
[16]in
explaining
theremaining discrepancy
between our results and Leavens'. Such adiscrepancy might perl~aps depend
on the fact tl~at the functions to beintegrated
do fluctuateheavily
(~)(anyway,
we didcarefully
check that our ownelementary integration
step in theintegration
over dk was small
enough
in order to guarantee thestability
of the numericalresult,
and, mparticular,
of their sign, forstrongly oscillating
functions in theintegrand).
Moreprobably,
thepersisting disagreement
can bemerely
due to the fact -asrecently
daimed alsoby Delgado
et ai.
Ii?i
thatdijferent
initial conditions for the wavepackets
wereactually
chosen in reference [8] and in referenceiii. Anyway,
ourapproach
seems to get support, at least insome
particular
cases, alsoby
a recent articleby
Brouard etai.,
which"generalizes"
-even ifstarting
from atotally
differentpoint
of view- some of our results[12,15].
Let us take
advantage
of the present opportunity foranswering
other criticismsappeared
in reference [8], where it has been furthermore commented about our way ofperforming
actual averages over thephysical
t1nle. We cannot agree with those comments: let usre-emphasize
in factthat,
within conventional quantummechanics,
the timet(x)
at which ourpartide (wave packet)
passesthrough
theposition
x is"statistically
distributed" with tl~eprobability
densitiesdtJ+ ix, t) / fÎ~ dtJ+ ix, t),
as weexplained
at page 350 of referenceiii.
Tl~is distribution meets tl~erequirements
of tl~etime-energy uncertainty
relation.We also answered in Section Leavens' comments about our
analysis iii
of tl~e dwell-time approacl~es [19].The last
object
of the criticisnl in reference [8] refers to theimpossibility,
m ourapproach,
ofdistinguishing
between "to be transmitted" and "to be reflected" wavepackets
at theleading edge
of tl~e barrier.Actually,
we dodistinguish
betweentl~em; only,
we cannot -~f course-separate
tl~em,
due to tl~e obvious superposition(and interference)
of both wave functions inp(x,t),
inJ(x,t)
and even inJ+ ix, t).
This is known to be an unavoidable consequence of the superpositionprinciple,
valid for wa~efunctions
m conventional quantum mechanics.That last
objection, tl~erefore,
sl~ould be addressed to quantummecl~anics,
ratl~er then to us.Nevertheless,
Leavens' aim ofcomparing
the definitionsproposed by
us for thetunnelling
times notonly
witl~ conventional, but also witl~ non-standard quantum mecl~anicsmight
beregarded
a priori as
stimulating
andpossibly
wortl~ of furtl~erinvestigation.
4. Further Remarks
In connection witl~ tl~e
question
of"causality"
for relativistictunnelling partides,
let us stress tl~at tl~e Hartman-Fletcl~erpl~enomenon (very
smalltunnelling durations),
witl~ tl~e conse-(~)We
can only say that we succeeded in reproducing results of the type put forth in reference [8]
by using larger steps; whilst the "non-causal" results disappeared -m the considered case- when
adopting small enough integration steps.