On the Apparent Superluminal Motion of a Damped Gaussian Pulse
📝 Original Info
- Title: On the Apparent Superluminal Motion of a Damped Gaussian Pulse
- ArXiv ID: 1112.1324
- Date: 2011-12-07
- Authors: N. Redington
📝 Abstract
Alicki has demonstrated that a travelling Gaussian pulse subject to damping is indistinguishable from an undamped pulse moving with greater speed; such an effect could create the illusion of a pulse moving faster than light. In this note, an alternative derivation of the same result is presented. However, it is unlikely that this particular illusion could explain the superluminal neutrino-velocities reported by OPERA.💡 Deep Analysis
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arXiv:1112.1324v1 [physics.gen-ph] 4 Dec 2011
On the Apparent Superluminal Motion of a
Damped Gaussian Pulse
N. Redington
Net Advance of Physics
redingtn@mit.edu
Alicki has demonstrated that a travelling Gaussian pulse subject
to damping is indistinguishable from an undamped pulse moving
with greater speed; such an effect could create the illusion of a pulse
moving faster than light. In this note, an alternative derivation of the
same result is presented. However, it is unlikely that this particular
illusion could explain the superluminal neutrino-velocities reported
by OPERA.
The recent claim that the measured velocity of mu neutrinos exceeds that of
light [1] has rekindled interest in the old subject of illusory superluminal motion.
Of the various proposals advanced to explain the OPERA results without jeop-
ardy to established physics [2], that of Alicki [3] is among the most intriguing.
Alicki argues that a stationary observer cannot tell a moving normal distribution
subject to global exponential damping from an undamped normal distribution
with different characteristic parameters, including higher (even apparently su-
perluminal) velocity. This result, which may be of some importance in optics
and other fields unrelated to neutrino physics, is re-derived in the present note
by very elementary means. Unfortunately (or otherwise, if one wishes to break
the light barrier in fact rather than appearance), such an effect seems unlikely
to be the solution to the OPERA puzzle: the CNGS-beam pulse lacks the “fat
tail” needed for the argument to apply.
To derive Alicki’s result, it is first helpful to consider the case of a Gaussian
pulse with no damping at all. Let ρ(x, t) denote the intensity, assumed non-
negative, of a signal moving at constant speed v > 0 in one dimension without
dispersion or distortion toward an observer at some fixed location x = L. By
hypothesis, observer and source are in a state of mutual rest. Let the profile
of the signal as initially transmitted be Gaussian with maximum height ρ0 and
full width σ at half maximum. Since transmission is perfect, the observer at L
will see:
ρ(t) = ρ0 exp −(L −vt)2
2σ2
1
The time derivative of ρ is:
˙ρ = ρ v
σ2 (L −vt)
so the observer will notice a peak at time
t = L/v
Prior to that time, ρ is increasing; afterwards, decreasing.
Knowing L and
measuring t, the observer easily determines the velocity of the pulse to be v, as
expected.
Now introduce a simple damping:
ρ(t) = (ρ0 exp −(L −vt)2
2σ2
) exp −γt
(1)
where γ is a positive constant. The time derivative of ρ becomes:
˙ρ = ρ v
σ2 (L −vt −δL)
where
δL ≡γσ2
v
≥0
(2)
The observer will now notice a peak at time
t = T ≡(L −δL)/v
Prior to that time, ρ is increasing; afterwards, decreasing. It is therefore rea-
sonable to define
v′ ≡L/T =
Lv
L −δL
(3)
Note that v′ ≥v provided 0 ≤δL ≤L.
To shew that v′ could in fact be interpreted as the velocity of a moving,
undamped Gaussian pulse, note that according to Eq. (2):
σ2γt = vtδL
(4)
Therefore, we may rewrite Eq. (1) in terms of δL as:
ρ(t) = ρ0 exp −F
2σ2
(5)
where
F ≡L2 + (vt)2 −2(L −δL)vt
(6)
Furthermore, define two new constants
σ′ ≡
σ
1 −(δL/L)
(7)
2
and
ρ′
0 ≡ρ0 exp −δL
2σ2 (2L −δL)
(8)
With the help of Eqs. (2), (3), (6), (7), and (8), Eq. (5) becomes:
ρ(t) = ρ′
0 exp −(L −v′t)2
2σ′2
(9)
quod erat demonstrandum.
Less formally, the Alicki effect can be understood in terms of the damping
acting on the signal over time. At t = 0, the value of ρ in the neighbourhood
of L is ρ0 exp −(L/σ)2/2. A few moments later, the part of the distribution
originally just a bit to the left of L will pass the observer; the damping force
will have acted upon it briefly, so its magnitude will be somewhat diminished.
By contrast, the regions of the distribution which at t = 0 were far to the left,
though they may have had initially large values of ρ, will arrive at the observer
much later, and the exponential decay induced by the damping force will have
acted on them for a long time. Thus, the magnitude of parts of a sufficiently
wide Gaussian may be greatly diminished by even a small damping, and the
peak of the received signal will be shifted to the right relative to the peak in
the signal as originally sent.
The constraint δL ≤L for positive v′ can also be given a qualitative in-
terpretation. Consider the three factors which define δL according to Eq. (2).
Should the damping constant γ be too large, or the initial velocity v too small,
the magnitude of the signal reaching the observer will diminish from the very
first observation at t = 0. The observer might conclude from this that the pulse
is moving to the left (in agreement with Eq. (3) for this case), and that only its
receding tail is being observed. The same is true, if perhaps less self-evidently,
for a very broad pulse: it rises too slowly to keep up with the decay, and may
also be construed as moving leftwards.
Since both source and observer are stationary in a common frame of refer-
ence, the initial velocity v may be given a
Reference
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