ΣΥΝΑΙΣΘΗΜΑΤΙΚΗ ΝΟΗΜΟΣΥΝΗ-Ξ—-Συναισθηματική-ΞΞΏΞ·ΞΌΞΏΟƒΟΞ½Ξ·
EJTP · 2008. 5. 17. · some scalar field , a non-minimal coupling between the scalar curvature...
Transcript of EJTP · 2008. 5. 17. · some scalar field , a non-minimal coupling between the scalar curvature...
-
Volume 3 Number 11
Electronic Journal of Theoretical Physics
ISSN 1729-5254
EJTP
Editors
Ammar Sakaji Ignazio Licata
http://www.ejtp.com June, 2006 E-mail:[email protected]
-
Volume 3 Number 11
Electronic Journal of Theoretical Physics
ISSN 1729-5254
EJTP
Editors
Ammar Sakaji Ignazio Licata
http://www.ejtp.com June, 2006 E-mail:[email protected]
-
Editor in Chief
A. J. Sakaji
EJTP Publisher P. O. Box 48210 Abu Dhabi, UAE [email protected] [email protected]
Editorial Board
Co-Editor
Ignazio Licata,Foundations of Quantum Mechanics Complex System & Computation in Physics and Biology IxtuCyber for Complex Systems Sicily – Italy
[email protected]@ejtp.info [email protected]
Wai-ning Mei Condensed matter TheoryPhysics DepartmentUniversity of Nebraska at Omaha,
Omaha, Nebraska, USA e-mail: [email protected] [email protected]
Tepper L. Gill Mathematical Physics, Quantum Field Theory Department of Electrical and Computer Engineering Howard University, Washington, DC, USA e-mail: [email protected]
F.K. DiakonosStatistical Physics Physics Department, University of Athens Panepistimiopolis GR 5784 Zographos, Athens, Greece e-mail: [email protected]
Jorge A. Franco Rodríguez
General Theory of Relativity Av. Libertador Edificio Zulia P12 123 Caracas 1050 Venezuela e-mail: [email protected] [email protected]
J. A. MakiApplied Mathematics School of Mathematics University of East Anglia Norwich NR4 7TJ UK e-mail: [email protected]
Nicola Yordanov Physical Chemistry Bulgarian Academy of Sciences,BG-1113 Sofia, Bulgaria Telephone: (+359 2) 724917 , (+359 2) 9792546
e-mail: [email protected]
ndyepr[AT]bas.bg
S.I. ThemelisAtomic, Molecular & Optical Physics Foundation for Research and Technology - Hellas P.O. Box 1527, GR-711 10 Heraklion, Greece e-mail: [email protected]
T. A. HawaryMathematics Department of Mathematics Mu'tah University P.O.Box 6 Karak- Jordan e-mail: [email protected]
Arbab Ibrahim Theoretical Astrophysics and Cosmology Department of Physics, Faculty of Science, University of Khartoum, P.O. Box 321, Khartoum 11115, Sudan
e-mail: [email protected] [email protected]
-
Sergey Danilkin Instrument Scientist, The Bragg Institute Australian Nuclear Science and Technology Organization PMB 1, Menai NSW 2234 AustraliaTel: +61 2 9717 3338 Fax: +61 2 9717 3606
e-mail: [email protected]
Robert V. Gentry The Orion Foundation P. O. Box 12067 Knoxville, TN 37912-0067 USAe-mail: gentryrv[@orionfdn.org
Attilio Maccari Nonlinear phenomena, chaos and solitons in classic and quantum physics Technical Institute "G. Cardano" Via Alfredo Casella 3 00013 Mentana RM - ITALY
e-mail: [email protected]
Beny Neta Applied Mathematics Department of Mathematics Naval Postgraduate School 1141 Cunningham Road Monterey, CA 93943, USA
e-mail: [email protected]
Haret C. Rosu Advanced Materials Division Institute for Scientific and Technological Research (IPICyT) Camino a la Presa San José 2055 Col. Lomas 4a. sección, C.P. 78216 San Luis Potosí, San Luis Potosí, México
e-mail: [email protected]
A. AbdelkaderExperimental Physics Physics Department, AjmanUniversity Ajman-UAE e-mail: [email protected]
Leonardo Chiatti Medical Physics Laboratory ASL VT Via S. Lorenzo 101, 01100 Viterbo (Italy) Tel : (0039) 0761 236903 Fax (0039) 0761 237904
e-mail: [email protected]
Zdenek Stuchlik Relativistic Astrophysics Department of Physics, Faculty of Philosophy and Science, Silesian University, Bezru covo n´am. 13, 746 01 Opava, Czech Republic
e-mail: [email protected]
Copyright © 2003-2006 Electronic Journal of Theoretical Physics (EJTP) All rights reserved
-
Table of Contents
No Articles Page
1 Non-Minimal Coupling Effects of the Ultra-Light Particles on Photons Velocities in the Radiation Dominated Era of the Universe. El-Nabulsi Ahmad Rami
1
2 A Toy Model of Financial Markets J. P. Singh and S. Prabakaran
11
3 Rayleigh process and matrix elements for the one-dimensional harmonic oscillator J.H. Caltenco, J.L. López-Bonilla, and J. Morales
29
4 Identical synchronization in chaotic jerk dynamical systemsVinod Patidar and K. K. Sud
33
5 Second Order Perturbation of Heisenberg Hamiltonian for Non-Oriented Ultra-Thin Ferromagnetic Films P. Samarasekara
71
6 Frameable Processes with Stochastic Dynamics Enrico Capobianco
85
7 Ab-initio Calculations for Forbidden M1/E2 Decay Rates in Ti XIX ion A. Farrag
111
8 Some Properties of Generalized Hypergeometric Thermal Coherent States Dusan Popov
123
9 Space-Filling Curves for Quantum Control Parameters Fariel Shafee
133
10 The Spectrum of the Lagrange Velocity Autocorrelation Function in Confined Anisotropic LiquidsSakhnenko Elena I and Zatovsky Alexander V.
143
11 On the Quantum Correction of Black Hole ThermodynamicsKourosh Nozari and S. Hamid Mehdipour
151
12 A Graphic Representation of States for Quantum CopyingSara Felloni and Giuliano Strini
159
-
EJTP 10 (2006) 1–10 Electronic Journal of Theoretical Physics
Non-Minimal Coupling Effects of the Ultra-LightParticles on Photons Velocities in the Radiation
Dominated Era of the Universe
El-Nabulsi Ahmad Rami ∗
Plasma Application Laboratory, Department of Nuclear andEnergy Engineering and Faculty of Mechanical, Energy and Production Engineering,
Cheju National University, Ara-dong 1, Jeju 690-756,Korea
Received 6 September 2005 , Accepted 27 November 2005, Published 25 May 2006
Abstract: The effect of the ultra-light masses of the order of the Hubble constant, implementedin Einstein’s field equations from non-minimal coupling and supergravities arguments, onphotons velocities in the radiation dominated epoch of the Universe within the frameworkof non-minimal interaction of electromagnetic fields with gravity is developed and discussed indetails.c© Electronic Journal of Theoretical Physics. All rights reserved.
Keywords: Non-minimal coupling, ultra-light masses, effective cosmological constant, photonsvelocity.PACS (2006): 04.40 Nr, 98.80 -k, 95.30 SI
1. Introduction
A standard result of Einstein’s gravity is that massless particles, in particular photons,
move at light celerity ‘c’. A question worth examining is whether the velocity of massless
photons is shifted when these later propagate in exotic background filled of ultra-light
particles (ULP) of tiny masses in the order of the Hubble constant (m ≈ H). This couldhave important cosmological and astrophysical implications. In fact, the possibility of
shifting photon propagation (SPP) in gravitational fields (or non-trivial topologies) is
an interesting prediction of quantum field theory in curved space-time. It appears that
photon propagation may depend on their direction and polarisation, travel with speeds
exceeding the normal speed of light ‘c’ [1]. It is a quantum effect induced by vacuum
-
2 Electronic Journal of Theoretical Physics 10 (2006) 1–10
polarisation (allowing the photons to exist as a virtual e+e−pair so that at the quantumlevel it is characterized by the Compton wavelength of the electron) and implies that
the Principle of Equivalence does not hold for interacting quantum field theories such
as QED. The propagation of photon in Schwarzschild, Robertson-Walker, gravitational
wave, de Sitter backgrounds, charged black hole were done and remarkable results were
discovered [2]. In each case (except the totally isotropic de Sitter space-time) it was
possible to find directions and polarisations for which the photon velocity exceeds ‘c’.
Generalization to neutrino propagation in a Robertson-Walker metric using the Weinberg-
Salam model was done in [3]. In a gravitational field, the photon propagation is sensitive
to an anisotropic space-time curvature and may depend on this later [4,5]. Recently,
a series of papers has appeared in which the light velocity varies in the early Universe
and this solves the horizon, monopole and the flatness problems in standard cosmology
[6,7,8,9]. In this work, we will investigate further the consequences of non-minimal
coupling on light velocity in the presence of ultra-light particles.
2. Non-minimal Coupling, Supergravities Arguments and Ein-
stein Fields Equations
We start with the non-minimal interaction of electromagnetic fields with gravity in the
following form L̃ =√
gξRμνFμα F
νμ, ξ being the coupling constant, Rμν the Riemann
tensor, g the metric scalar and Fμν = ∂μAν −∂νAμ is the electromagnetic strength (Aμ isthe vector potential). Terms like RF 2 are neglected here. In this way, the field equations
read [10,11,12]:
Dν [Fμν − 2ξ (RμαFαν − RναFαμ)] = 0
where Dν is the covariant derivative. Let us now restrict our attention to the form of the
Riemann tensor we will choose for this work. In a recent paper [13], we introduced, for
some scalar field , a non-minimal coupling between the scalar curvature and the density of
the scalar field in the following form L = −ξ√gRφ∗φ, ξ = 1/6 . R is the scalar curvatureand is the complex conjugate of . From a view point of quantum field theory in curved
space-time, it is natural to consider such a non-minimal coupling. In fact, the conformal
case results in an extension of the property of conformal invariance for massless fields,
which is attractive from physical point of view. This parameter describes the strength
of the coupling between the curvature of spacetime and the inflation. Minimal coupling
corresponds to ξ = 0. It was shown that in this case and for a particular scalar negative
complex potential field V (φφ∗) = 3/4m2(ωφ2φ∗2 − 1),ω being a tiny parameter inspiredfrom supergravity inflation theories, ultra-light masses ‘m’ are implemented naturally in
Einstein field equations (EFE), leading to a cosmological constant ‘Λ’ in accord with
observations2. In matter-free background, the scalar curvature was found to be =4Λ̄
2 It has been argued that a non-minimal coupling term-generated by quantum corrections-is to be expectedwhenever the space-time curvature is large; in most theories that describe inflationary scenarios, it turnsout that a value of ξ different from zero is unavoidable. As a matter of fact, it seems sensible to consideran explicit non-minimal coupling in the supergravities inflationary paradigm.
-
Electronic Journal of Theoretical Physics 10 (2006) 1–10 3
where Λ̄ = Λ−3/4m2 is the effective cosmological constant3 (in natural units, m ≈ �H/c2where ‘�’ is the Planck constant and ‘c’ being the celerity of light). As a result, one
candidate Einstein field equations is(� = c = 1):
Gμν ≡ Rμν − 12gμνR = −Λ̄gμν (1)
Λ̄ = Λ − 3m2/4 ≡ Λ1 + Λ2 is the effective cosmological constant (Λ2 = −3λ̄−2C whereλC = �/mc is the Compton wavelength in natural units). Remark that for Λ1 = 0, the
scalar curvature is negative and the space-time is not Minkowskian. Other field equations
exist also but correspond only for p = ρ/3 (radiation era):
Rμν − 12gμνR + Λgμν = −8πG
[(p + ρ +
3m2
8πG
)uμuν + pgμν
](2a)
Rμν − 12gμνR = −8πG
[(p + ρ +
3m2
8πG
)uμuν +
(p +
Λ
8πG
)gμν
](2b)
= −8πG[(p + ρ̄) uμuν +
(p +
Λ
8πG
)gμν
](2c)
≡ −8πG[Tμν (p, ρ) +
Λ
8πGgμν + tμν (m)
](2d)
≡ −8πG [Tμν (p, ρ) + Tμν (Λ,m)] (2e)≡ −8πG
∑Tμν (2f)
p and ρ are the pressure and density of matter,ρ̄ = ρ + 3m2/8πG, tμν = 3m2/8πGuμuν
and:
Tμν (p, ρ) = (p + ρ) uμuν + pgμν (3)
Tμν (Λ,m) = tμν +Λ
8πGgμν =
1
8πG
[3m2uμuν + Λgμν
](4)
Contracting equations (2) with gμν using gμνuμuν = −1 yields of course. In this way,the ultra-light masses and the cosmological constant are parts of the matter contents of
the Universe rather than geometrical entities. The radiative field equations (RFE) (2-
a,b,c,d,e,f) are identical to that of Einstein standard ones but with an additional energy
density ρm = 3m2/8πG(m ≤ H). One can also refer to equation (4) as the stress-energy
tensor of vacuum and light particles, which is a ”microscopic stress-energy tensor”. In
fact, the conservation law holds and we have:
∇ν∑
Tμν ≡ ∇νTμν (p, ρ) + ∇νTμν (Λ,m) = 0 (5)
When Tμν (p, ρ) = 0, the microscopic stress-energy tensor will behave as the macroscopic
one if we assume that:
P (Λ,m) ≡ PΛ = Λ/8πG (6)3 In [13], 8πG ≡ κ was set equal to unity.
-
4 Electronic Journal of Theoretical Physics 10 (2006) 1–10
ρ (Λ,m) =3m2 − Λ
8πG(7)
That is, in the microscopic version, if Λ = 0, P = 0 but the density is positive. While
for Λ > 3m2, the pressure is positive and the density is negative. If 0 < Λ < 3m2, then
both the pressure and the density are positive.
Before treating the non-minimal coupling scenario, we will discuss briefly the impli-
cations of equations (2) in standard cosmology. For this, we consider a homogenous and
isotropic Universe in the radiation dominated epoch described by Friedman-Robertson-
Walker line element with scale factor a (t)[14]. The radiative field equations read:
ȧ2
a2+
k
a2=
8πGρ
3+
Λ
3+ m2 (8)
ä
a= −8πGρ
3+
Λ
3− m
2
2(9)
k = −1, 0, +1 is the curvature constant for open, flat or closed space-time and dim (Λ) =dim (m2) = length−2. If the cosmological constant and the ultra-light masses are assumedto be constant with time, then from the energy conservation law: ρ ∝ a−4. For zerodensity, 2Λ > ( ( Λ, Λ̂ → 3/4m2. If for instance, we assume that m2 = β/a2and Λ = δȧ2/a2 +ηä/a, β, δ, η are constants [20,21], than from equation (10)4:
ä
a
(1 − 2η
3
)+
ȧ2
a2
(1 − 2δ
3
)+
(k − β
2
)1
a2= 0 (12)
which gives:
ȧ2 =3 (β − 2k)2 (3 − 2δ) + Da
− 2(3−2δ)3−2η , D = const. (13)
4 The fact that the two terms Λ and m2 play the role of two cosmological constant in the theory, wehave the freedom to choose Λ = δ1ȧ2
/a2 + η1ä/a + β1
/a2 and m2 = δ2ȧ2
/a2 + η2ä/a + β2
/a2where
δ1,2, η1,2, β1,2 are constants. In this work, we simplified our assumptions just to have at the beginning asimple idea about the effects of the ultra-light masses in the theory.
-
Electronic Journal of Theoretical Physics 10 (2006) 1–10 5
For D = 0 which corresponds to singular solutions, one finds for flat space-time(k = 0):
a =
√3β
2 (3 − 2δ)t (14)
where δ < 3/2, β > 0. In this way :
m2 =2 (3 − 2δ)
3t2(15)
Λ =δ
t2(16)
From equation (8), we find:
ρ =3 (δ − 1)8πGt2
(17)
with 1 < δ < 3/2. In this way, we don’t have an inflationary phase and no horizon
problem appears. From the above equations, we see that the ultra-light masses, the
cosmological constant and the density are independent of the value of β and η. The
Hubble parameter is H = ȧ/a = 1/t and the density matter of the Universe is given by
Ωr = ρ/ρc = δ − 1 < 1/2 where ρc = 3H2/8πG is the critical density. The decelerationparameter is q ≡ −äa/ȧ2 = 0. The density parameter due to vacuum contribution isΩΛ = Λ/3H2 = δ/3 and that due to ultra-light particles contributions is Ωm = m2/H2 =
2 (3 − 2δ)/3. In this way ΩTotal = Ωr + Ωm + ΩΛ = 1 as required by inflation [22]. Theultra-light particles than contribute to the total energy density and their masses decrease
as inverse to time. Note from equations (15) and (16) that Λ = 3δm2/2 (3 − 2δ) < 9m2/4.Finally, note that when the ‘Λ’ and ‘m2’ terms dominate the dynamics of equation (8)
with the assumption that the Universe undergoes a long period of evolution during which
the celerity of light changes as c = c0an, c0, n =constants [8]:
ȧ2
a2=
Λc2 (t)
3+ m2c2 (t) →
(Λ
3+ m2
)c2n0 a
2n (18)
So at large times, we have a ∝ t−1/n and it was found in [8] that for negative ”n”, thereis a solution to the quasi-lambda problem.
In order to have a very simple idea about the role of the ultra-light masses in the
theory, we suppose that the space-time is flat, that is k = 0 with the following behavior of
the ultra-light masses m2 = β/a2and the cosmological constant Λ = δ/a2, β, η=constants
(see footnote 4 ) [23,24,25]. In this case, when ‘Λ’ and ‘m2’ terms dominate at large
times the dynamics of equation (8):
ȧ2
a2=
Λc2 (t)
3+ m2c2 (t) =
(β +
δ
3
)c20a
2n−2 (19)
That is a ∝ t−1/n−1 and from [8,26], it is required that n < 0 and c = c0t−n/n−1. Insummary, m2 ∝ t2/n−1 and as a result mc ∝ 1/t. Another way to study shifting andtime-varying photons velocities is by using the non-minimal coupling of electromagnetic
fields and gravity.
-
6 Electronic Journal of Theoretical Physics 10 (2006) 1–10
3. Varying Photons Velocities From Non-Minimal Coupling
Following [10,11], we admit the existence of a surface S represented by φ (x) = 0. The
wavenumber of the photon trajectories is given by the gradient of its phase kλ = ∇λφwhere the Faraday tensor vanishes at its hypersurface, that is (Fμν)S = 0. Its derivative
defines a function φμν such that:
(∂λFμν)S = (DλFμν)S = kλφμν (20)
As a consequence, equation (1) takes the form:
[φμν − 2ξ (Rμαφαν − Rναφαμ)] kν = 0 (21)
In the radiation dominated era, it follows that:
φμνkν − 2ξ{[
φαν . (−χ){{
4ρ
3+ ρm
}uμuν +
{ρ
3+
ρm2
− Λχ
}}δμν
]
+
[−φαμ. (−χ)
{{4ρ
3+ ρm
}uνuα +
{ρ
3+
ρm2
− Λχ
}}δνα
]}kν = 0 (22)
where χ = 8πG (� = c = 1). For simplicity, we let k0 = kμuμ and we use the antisym-
metric fact of (φμν − φνμ = 2φμν) as well as Maxwell equations:
φμνkλ + ϕνλkμ + φλμkν = 0 (23)
By contracting by kλ the last equation, equation (23) reduces to:
φμνkν =−2ξχ (4ρ
3+ ρm
)1 + 4χ
(ρ3
+ ρm2− Λ
χ
)ξk0φ
μνuν ≡ (N) k0φμνuν (24)
Replacing (24) into (23), then:
φμνk2 + N (−φμνkλ − ϕλμkν − kνφμλ) k0uλ = 0 (25)
The antisymmetric of φμνeliminates all the terms in the parentheses of equation (25) and
we are left with:
φμν(k2 − Nk20
)= 0 ⇒ k2 − Nk20 = 0,∀φμν (26)
The effective photons velocity, in case allρ, ρm, Λ = 0, ∀ξ is then given by [6]:
v2 =|kiki|k20
= |1 + N | =∣∣∣∣∣∣ 1 − 4ξΛ − 4ξχ
ρ3
1 + 4ξχ(
ρ3
+ ρm3− Λ
χ
)∣∣∣∣∣∣ (27)
and the light velocities is not equal to ‘c’. Adopting equations (15), (16) and (17),
equation (27) takes the form in normal units:
v2 =
∣∣∣∣∣1 − 4 ξt2 (2δ − 1)1 + 4 ξt2
(5 − 4δ)
∣∣∣∣∣ (28)
-
Electronic Journal of Theoretical Physics 10 (2006) 1–10 7
with 1 < δ < 3/2. As a result, for ξ > () c (light celerity). Adopting
the fact c = c0an with n < 0, than the photons velocities decreases with time whatever
is the sign of the coupling constant.
An interesting case is when the background is ‘free from matter ’ . From (27) we get:
v2 =
∣∣∣∣ 1 − 4ξΛ1 + 4ξ (m2 − Λ)∣∣∣∣ (29)
If m2 = 0, than v2 = 1 which is light celerity in units (� = c = 1). Assuming m2 = β/t2,
4Λ = 3m2 or Λ̄ = 0 and as a result R = 0. In this case, equation (28) gives:
v2 =
∣∣∣∣1 − 3m2ξ1 + m2ξ∣∣∣∣ =
∣∣∣∣∣1 − ξ 3βt21 + ξ βt2
∣∣∣∣∣ =∣∣∣∣t2 − 3ξβt2 + ξβ
∣∣∣∣ (30)Again, if ξ > () c (light celerity). As a result, the velocity of photons is
affected and shifted by the presence of the ultra-light tiny masses and depends on the sign
of the coupling constant. It doesn’t correspond in fact to null geodesics as in the standard
case. Positive coupling constant corresponds to friction and negative one corresponds to
superluminal case [27,28]. If we adopt the fact c = c0an, then the photons velocities not
only is shifted but also decrease with time if n < 0 and increase if n > 0.
The constancy of the speed of light is not preserved in this analysis. It depends on
how is filled the background space and how is used a coupling constant different of zero
that modifies presentation of the Einstein’s Field Equations (EFT ), with an additional
term. It is important to notice that the environment where speed of light reaches its
maximum value is the lightest one: the empty space, all because of the constancy of the
speed of light law, which in time, originates the fourth time-coordinate. In our case, the
red-shift coefficient ‘z’ varies with time according to cz = Hr combined to equations (29)
or (30) for a matter free background. ‘r’ is supposed to be the distance form the galaxy
to the earth [14]. If the coupling constant is assume to be positive, one can than have a
cosmological model based on interpretation of the red shift by decrease of the light speed
with time everywhere in the universe beginning with a certain moment of time in the
past. Of course, the agreement with the fundamental physics laws will be completed by
introducing in a future work the evolution of other fundamental constants synchronously
with the variation of the light speed [29].
Finally, we note that recently, growing amount of astrophysical data show important
evidence for statistical and apparent physical association between low-redshift galaxies
and high-redshift quasi-stellar objects suggesting noncosmological origin of their redshift
and as a result failure of classical quasar explanation [30]. The author found analytical
solution of Einstein equations describing bubbles made from axions with periodic inter-
action potential considered as one of the leading dark matter candidate. Remember that
in our model [13], the ultra-light masses implemented in Einstein field equations enabled
us to solve the ‘missing mass problem’ and as result considered as dark matter candidate.
In Minkowski space, objects at constant proper distance with respect to an observer have
zero redshift. However, in an expanding universe special relativistic concepts do not gen-
erally apply. In fact, a galaxy with zero total velocity does not have zero redshift even
-
8 Electronic Journal of Theoretical Physics 10 (2006) 1–10
in the empty universe case. This demonstrates that cosmological redshifts are not spe-
cial relativity Doppler shifts [31,32]. It was also proved that Minkowski coordinate and
the Robertson-Walker coordinates (FRW universe) are interchangeable descriptions for
an empty universe. However, velocities in the Minkowski universe are not equivalent to
velocities in the FRW universe because of the different definitions of time and distance in
these two models. A coordinate transform relates velocities in the Minkowski universe to
velocities in the FRW universe. Superluminal recession velocities in the FRW universe
do not violate special relativity because they are not in the observer’s inertial frame.
4. Conclusions:
In this work, we used the Einstein’s field equations with effective cosmological constant
inspired from non-minimal coupling and supergravities arguments to study the conse-
quences of non-minimal coupling between electromagnetic fields and gravity on light
velocity in the presence of ultra-light particles at the radiation dominated epoch of the
Universe. We showed that if the cosmological constant and the ultra-light square masses
varies as Λ = δȧ2/a2+ηä/a and m2 = β/a2, then at singular solutions and for a flat space-
time, Λ, m2 and ρ decreases with time as 1/t2, the Hubble parameter vary as H = 1/t,
the deceleration parameter is zero and ΩTotal = Ωr +Ωm+ΩΛ = 1 as required by inflation.
As a result, the ultra-light particles than contribute to the total energy density and their
masses decrease as inverse to time. When the ‘Λ’ and ‘m2’ terms dominate the dynamics
of our field equations with the assumption that the Universe undergoes a long period of
evolution during which the celerity of light changes as c = c0an, it was found that at large
times a ∝ t−1/n and that for negative ‘n’, there is a solution to the quasi-lambda problem.Finally, we studied varying light velocities from non-minimal coupling. We found that
photons velocities depends on the coupling constant and only on δ ∈ (1, 3/2)in a waythat ξ > () c with m
2 > 0.
The model described in this paper could have important implications in various sys-
tems, in particular cosmological scenarios, black hole physics and quantum interactions
[33,34,35,36,37]. It is important to discuss the impact of the assumptions established to
reach the model and the fact that a non-Minkowskian space is necessary to obtain speeds
greater than that of light, and that photon could be represented by a positron-electron
pair for characterizing it with the electron’s Compton wavelength.
To further investigate all these issues, further studies will be necessary and work is in
progress.
Acknowledgments:
The author is grateful for the referees for their useful comments and suggestions.
-
Electronic Journal of Theoretical Physics 10 (2006) 1–10 9
References
[1] I.T. Drummond and S.J. Hathrell, Phys. Rev. D 22, 343 (1980).
[2] R.D. Daniels and G.M. Shore, Nucl. Phys. B 425,634 (1994).
[3] Y. Ohkuwa, Prog. Theor. Phys. 65, 1058 (1981).
[4] R. G. Cai, Nucl. Phys. B 524,639 (1998).
[5] G. M. Shore, Nucl. Phys. B 460, 379 (1996).
[6] J. D. Barrow, astro-ph/9811022.
[7] A. Albrecht and J. Maguiejo, Phys. Rev D 59, 043516 (1999) 043516.
[8] J. D. Barrow and J. Maguiejo, Phys. Lett. B 443, 104-110 (1998).
[9] P. Teyssandier, Annales de la Fondation Louis de Broglie, Volume 29 no 1-2, (2004)(gr-qc/0303081 ).
[10] M. Novello, L. A. R Olivera and J. M. Salim J.M., Class. Quant. Grav. 7, 51 (1990).
[11] M. Novello and S. D. Jorda, Mod. Phys. Lett. A, vol 4, n19, 1809, (1989).
[12] 1-I. L. Buchbinder, S. D. Odintsov and I. L. Shapiro, Effective Action in QuantumGravity, IOP-Publishing Ltd, (1982).
[13] R. A. El-Nabulsi, Phys. Letts. B, Vol. 619, 26 (2005).
[14] S. Weinberg, Gravitation and Cosmology, NY, Wiley (1972).
[15] J. M. Overduin and F. I. Cooperstock, astro-ph/9805260.
[16] J. W. Moffat, Int. J. Mod. Phys. D2, 351 (1993).
[17] J. W. Moffat, Found. Of Phys., 23, 411 (1993).
[18] M. A. Clayton and J. W. Moffat, Phys. Lett.B 460, 263 (1999).
[19] M. A. Clayton and J. W. Moffat, Phys. Lett.B 477, 269 (2000).
[20] A. S. Al-Rawaf, Mod. Phys. Lett. A 13, 429 (1998).
[21] A. I. Arbab, Spacetime and Substance 1(6), 39 (2001).
[22] A. H. Guth, Phys. Rev. D 23, 347 (1981).
[23] M. S. Berman, Nuovo Cimento 74B, 182 (1983).
[24] M. S. Berman, Gen. Rel. Grav. 23, 465 (1991).
[25] M. S. Berman and F. M. Gomide, Gen. Rel. Grav. 20, 191 (1988).
[26] M. S. Berman and L. A. Trevisan, gr-qc/0112011.
[27] D. Syer, astro-ph/9404063.
[28] T. Chiba and K. Kohri, Prog. Theor. Phys. 107, 631 (2002).
[29] V. S. Troitskii, Astrophysics and Space Science 139, 389 (1987).
[30] A. A. Svidzinsky, astro-ph/0409064.
-
10 Electronic Journal of Theoretical Physics 10 (2006) 1–10
[31] Davis T. M., Lineweaver C. H., 2001, in Durrer R., Garcia-Bellido J., ShaposhnikovM., eds, Cosmology and Particle Physics 2000, American Institute of Physics conferenceproceedings, Volume 555. New York, p. 348.
[32] Davis T. M., Lineweaver C. H., Webb J. K., Am. J. Phys., 71, 358 (2003)
[33] C. F. E. Holzhey and F. Wilzeck, Nucl. Phys. B 380, 447 (1992).
[34] R. A. El-Nabulsi, Chinese Phys. Lett. 23 No 5, 1124-1127 (2006).
[35] R. A. El-Nabulsi, Elec. J. Theor. Phys. 7, 27-46 (2005).
[36] R. A. El-Nabulsi, Elec. J. Theor. Phys. 9, 1-5 (2006).
[37] R. A. El-Nabulsi, Supergravity, Non-mimimal Coupling and Eternal AcceleratedExpansion: Some important Cosmological Features of Ultra-Light Particles andInduced Cosmological Constant, Submitted to Elec. J. Theor. Phys.
-
EJTP 3, No. 11 (2006) 11–27 Electronic Journal of Theoretical Physics
A Toy Model of Financial Markets
J. P. Singh and S. Prabakaran ∗ †
Department of Management StudiesIndian Institute of Technology Roorkee
Roorkee 247667, India
Received 27 October 2005 , Accepted 9 January 2006, Published 25 June 2006
Abstract: Several techniques of fundamental physics like quantum mechanics, field theoryand related tools of non-commutative probability, gauge theory, path integral etc. are beingapplied for pricing of contemporary financial products and for explaining various phenomenaof financial markets like stock price patterns, critical crashes etc.. In this paper, we apply thewell entrenched methods of quantum mechanics and quantum field theory to the modeling ofthe financial markets and the behaviour of stock prices. After defining the various constituentsof the model including creation & annihilation operators and buying & selling operators forsecurities, we examine the time evolution of the financial markets and obtain the Hamiltonianfor the trading activities of the market. We finally obtain the probability distribution of stockprices in terms of the propagators of the evolution equations.c© Electronic Journal of Theoretical Physics. All rights reserved.
Keywords: Economic Physics , Financial Markets , Stock Prices, Quantum ModelsPACS (2006): 89.65.Gh , 03.65.-w, 02.50.-r, 05.30.-d, 02.30.Tb
1. Introductionn
The specialty of “physics” is the study of interactions between the various mani-
festations of matter and its constituents. The development of this subject over the last
several centuries has led to a gradual refining of our understanding of natural phenomena.
Accompanying this has been a spectacular evolution of sophisticated mathematical tools
for the modeling of complex systems. These analytical tools are versatile enough to find
application not only in point processes involving particles but also aggregates thereof
leading to field theoretic generalizations and condensed matter physics.
Furthermore, with the rapid advancements in the evolution and study of disordered
∗ [email protected]† Jatinder [email protected]
-
12 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27
systems and the associated phenomena of nonlinearity, chaos, self organized criticality
etc., the importance of generalizations of the extant mathematical apparatus to enhance
its domain of applicability to such disordered systems is cardinal to the further develop-
ment of science.
A considerable amount of work has already been done and success achieved in the
broad areas of q-deformed harmonic oscillators [1], representations of q-deformed rotation
and Lorentz groups [2-3]. q-deformed quantum stochastic processes have also been studied
with realization of q-white noise on bialgebras [4]. Deformations of the Fokker Planck’s
equation [5], Langevin equation [6] and Levy processes [7-8] have also been analysed and
results reported.
Though at a nascent stage, the winds of convergence of physics and finance are unmis-
takably perceptible with several concepts of fundamental physics like quantum mechanics,
field theory and related tools of non-commutative probability, gauge theory, path integral
etc. being applied for pricing of contemporary financial products and for explaining var-
ious phenomena of financial markets like stock price patterns, critical crashes etc. [8-19].
The origin of the association between physics and finance, though, can be traced way back
to the seminal works of Pareto [20] and Batchlier [21], the former being instrumental in
establishing empirically that the distribution of wealth in several nations follows a power
law with an exponent of 1.5, while the latter pioneered the modeling of speculative prices
by the random walk and Brownian motion. The cardinal contribution of physicists to the
world of finance came from Fischer Black & Myron Scholes through the option pricing
formula [22] which bears their epitaph and which won them the Nobel Prize for economics
in 1997 together with Robert Merton [23]. They obtained closed form expressions for the
pricing of financial derivatives by converting the problem to a heat equation and then
solving it for specific boundary conditions.
The theory of stochastic processes constitutes the “golden thread” that unites the
disciplines of physics and finance. Modeling of non relativistic quantum mechanics as
energy conserving diffusion processes is, by now, well known [24]. Unification of the
general theory of relativity and quantum mechanics to enable a consistent theory of
quantum gravity has also been attempted on “stochastic spaces” [25]. Time evolution of
stock prices has been, by suitable algebraic manipulations, shown to be equivalent to a
diffusion process [26].
Contemporary empirical research into the behavior of stock market price /return pat-
terns has found significant evidence that financial markets exhibit the phenomenon of
anomalous diffusion, primarily superdiffusion, wherein the variance evolves with time
according to a power law tαwith α > 1.0. The standard technique for the study of su-
perdiffusive processes is through a stochastic process that evolves according to a Langevin
equation and whose probability distribution function satisfies a nonlinear Fokker Planck
equation [27].
There is an intricate yet natural relationship between the power law tails observed in
stock market data and probability distributions that emanate as the solution of the Fokker
Planck equation. The Fokker Planck equation is known to describe anomalous diffusion
-
Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27 13
under time evolution. Empirical results [28-31] establish that temporal changes of several
financial market indices have variances that that are shown to undergo anomalous super
diffusion under time evolution.
One of the most exhaustive set of studies on stock market data in varying dimensions
has been reported in [32-36]. In [36], a phenomenological study was conducted of stock
price fluctuations of individual companies using data from two different databases cover-
ing three major US stock markets. The probability distributions of returns over varying
timescales ranging from 5 min. to 4 years were examined. It was observed that for
timescales from 5 minutes upto 16 days the tails of the distributions were well described
by a power law decay. For larger timescales results consistent with a gradual convergence
to Gaussian behaviour was observed. In another study [32] the probability distributions
of the returns on the S & P 500 were computed over varying timescales. It was, again,
seen that the distributions were consistent with an asymptotic power law behaviour with
a slow convergence to Gaussian behaviour. Similar findings were obtained on the analysis
of the NIKKEI and the Hang –Sang indices [32].
Stock market phenomena are assumed to result from complicated interactions among
many degrees of freedom, and thus they were analyzed as random processes and one could
go to the extent of saying that the Efficient Market Hypothesis [37-38] was formulated
with one primary objective – to create a scenario which would justify the use of stochastic
calculus [39] for the modeling of capital markets.
The Efficient Market Hypothesis contemplates a market where all assets are fairly
priced according to the information available and neither buyers nor sellers enjoy any
advantage. Market prices are believed to reflect all public information, both fundamental
and price history and prices move only as sequel to new information entering the market.
Further, the presence of large number of investors is believed to ensure that all prices
are fair. Memory effects, if any at all, are assumed to be extremely short ranging and
dissipate rapidly. Feedback effects on prices are, thus, assumed to be marginal. The
investor community is assumed rational as benchmarked by the traditional concepts of
risk and return.
An immediate corollary to the Efficient Market Hypothesis is the independence of
single period returns, so that they can be modeled as a random walk and the defining
probability distribution, in the limit of the number of observations being large, would be
Gaussian.
Anomalous diffusion is a hallmark of several intensively studied physical systems. It
is observed, for example, in the chaotic dynamics of fluid in rapidly rotating annulus [40],
conservative motion in a periodic potential [41], transport of fluid in a porous media [42],
percolation of gases in porous media [43], crystal growth spreading of thin films under
gravity [44], radiative heat transfer [45], systems exhibiting surface to surface growth [46]
and so on.
Several analogies between physical systems and financial processes have been explored
in the last decade, some of which have already been mentioned above. Perhaps, the most
striking one is that between financial crashes witnessed in stock markets and critical
-
14 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27
phenomena like phase transitions is discussed here to place the main theme of this paper
in its proper perspective.
Stock market crashes are believed to exhibit log periodic oscillations which are char-
acteristic of systems exhibiting discrete scale invariance i.e. invariance through rescaling
by integral powers of some length scale like the Serpinski triangle and other similar fractal
shapes. In the years preceding the infamous crash of October 19, 1987, the S & P market
index was seen to fit the following expression exceedingly precisely [47-48],
(S & P )t = Ω + Γ (tc − t)γ {1 + Ξ cos [θ ln (tc − t) + φ]}Physicists working in solid state and condensed matter physics would immediately
recognize the analogy of the above expression with the one obtained for critical phe-
nomenon in spin model of ferromagnetism [49]. We briefly elucidate the salient features
of this model. Crystalline solids comprise of atoms arranged in a lattice. Each such
atom generates a magnetic field parallel to the direction of the atom’s spin. In the case
of substances that do not exhibit ferromagnetic character, these spin directions are ran-
domly oriented so that the aggregate magnetic field vanishes. However, in ferromagnetic
substances these spins are polarized in a particular direction resulting in a nonzero ag-
gregate field. Ferromagnetic substances usually exhibit two distinct phases. one in which
the spins orient themselves in a particular direction resulting in an aggregate magnetic
moment at temperatures below a well defined critical temperature tc and the other where
the spins are disoriented with a zero aggregate moment above the critical temperature.
At temperatures below tc, the coupling force between neighboring atoms predominates
resulting in an alignment of spins whereas above tc the additional energy manifests itself
in disorienting (randomizing) the spins.
Renormalization group theory enables us to group these atoms in blocks of spins
whose composite spins are equal to the algebraic sum of the spins of the atoms con-
stituting the block. It then provides that a model involving interactions between these
composite spins of a block can be constructed that replicates the macroscopic proper-
ties of the block and yet cannot depend on the size of the block. That is, the sys-
tem would exhibit a scaling symmetry, which is discrete, if we allow for the finite size
of the atom and continuous otherwise. The magnetic susceptibility of such a mag-
netic substance defined by χ (T ) = ∂M∂B
∣∣B=0
, where the symbols have their usual mean-
ing, obeys a power law of the form χ (T ) = Re[(T − Tc)α+iβ
]or equivalently χ (T ) =
(T − Tc)α {1 + β cos [ln (T − Tc)] + O (β2)}which is reminiscent of op cited expression forlog periodic oscillations in financial crashes.
Furthermore, the access to enhanced computing power during the last decade has
enabled analysts to try refined methods like the phase space reconstruction methods
for determining the Lyapunov Exponents [50] of stock market price data, besides doing
Rescaled Range Analysis [51] etc. A set of several studies has indicated the existence
of strong evidence that the stock market shows chaotic behavior with fractal return
structures and positive Lyapunov exponents. Results of these studies have unambiguously
established the existence of significant nonlinearities and chaotic behavior in these time
-
Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27 15
series [52-55].
In this paper, we attempt one such model. The objective is to apply the well en-
trenched methods of quantum mechanics and quantum field theory to the study of the
financial markets and the behaviour of stock prices. Section 2, which forms the essence of
this paper, arrives at various results for financial markets by modeling them as quantum
Hamiltonian systems. The probability distribution for stock prices in efficient markets is
also obtained. Section 3 concludes.
1.1 Quantum Model of Financial Markets
We consider an “isolated” financial market comprising of n investors and m type of
securities. The market is “isolated” in the sense that new types of securities are nei-
ther created nor are existing ones destroyed. Further, the number of investors is also
constant. The investor i, i = 1, 2, 3.......n is assumed to possess a cash balance of
xi, i = 1, 2, 3.......n (which may be negative, representing borrowings) and yij (z) , i =
1, 2, 3.....n; j = 1, 2, 3....m units of security j at a unit price of z . Obviously, yij ≥ 0,∀i, j.Towards constructing a basis for our Hilbert space representing the financial market,
we define a pure state of the system as
|Ψi〉 = |{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉 (1)Thus, a pure state represents a state of the market where the entire holdings of cash
and securities of every investor are known with certainty. This represents a complete
measurement of the market and hence, is in conformity with the standard definition of
“pure state” of a system.
A basis for our Hilbert space may then be constituted by the set of all the pure states
of the type (1) i.e.
Ψ = {|{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉} (2)The elements of this basis set Ψ satisfy the orthogonality condition 〈Ψi | Ψj〉 = δij withrespect to the scalar product defined in the sequel. The orthogonality condition makes
sense in the financial world – it implies that if a market is in a pure state |Ψi〉 then itcannot be in any other pure state.
However, a complete measurement of the market is, obviously, not practicable in real
life. At any point in time, we are likely to have certain information only about a fraction
of the market constituents. Hence, the instantaneous state of the market |ψ (t)〉 may berepresented by a linear combination of the pure states |Ψl (t)〉 i.e.
|ψ (t)〉 =∑
l
Cl |Ψl (t)〉 (3)
We endow our Hilbert space H with the scalar product
〈ψ (t) | ξ (t)〉 =∑l,m
C∗l Dm 〈Ψl (t) | Ψm (t)〉 =∑l,m
C∗l Dmδlm =∑
l
C∗l Dl (4)
-
16 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27
where we have assumed the orthogonality of the pure states.
The components of the state space vector |ψ (t)〉are given byCl = 〈Ψl (t) | ψ (t)〉 andare related to the probability of finding the market in the pure state |Ψl (t)〉.
Since our basis comprises of all possible measurable pure states, the completeness of
the basis is ensured so that
I =∑
l
|Ψl (t)〉 〈Ψl (t)| (5)
In analogy with the no particle state or ground state in quantum mechanics, we can
define a ground state of our financial market as
|0〉 = |xi = 0, yij (z) = 0∀i, j, z〉 (6)
i.e. the ground state is the market state in which no investor has any cash balances nor
any securities. This state is, obviously, a pure state being fully measurable and would
also not evolve in time since no trade can take place in this market.
We define the cash and security coordinate operators x̂i& ŷij (z) by their action on
the basis state (1) to provide respectively the balances of cash and the jth security (at
price z) with the ith investor as the eigenvalues i.e.
x̂i |{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉 = xi |{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉(7)
ŷij (z) |{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉 = yij (z) |{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉(8)
A cash translation operator T̂i (z) is also defined by the following
T̂i (z′) |{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉 = |{xi + z′, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉 (9)
i.e. it transfers an amount of cash z to the ith investor.
The operator T̂i (z) obviously satisfies the following properties
T̂i (z1) T̂i (z2) = T̂i (z1 + z2) (10)
T̂i (0) = Î (11)[T̂i (z) , x̂j
]= T̂i (z) x̂j − x̂jT̂i (z) = −zδijT̂i (z) (12)
T̂ ↑i (z) = T̂i (−z) (13)Towards obtaining an explicit representation of the cash translation operator, we assume
p̂i =dT̂i(z)
dz
∣∣∣z=0
as the generator of infinitesimal cash translations dz to the investor i.
Expanding T̂i (z) as a Taylor’s series and using eqs. (10), (11) we have
dT̂i (z)
dz= lim
dz→0T̂i (z + dz) − T̂i (z)
dz= lim
dz→0
�T̂i (dz) − 1
�T̂i (z)
dz= lim
dz→0
�T̂i (0) +
dT̂i(z)dz
���z=0
dz... − 1�
T̂i (z)
dz= p̂iT̂i (z)
(14)
-
Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27 17
with the solution T̂i (z) = ezp̂i . Furthermore, we have (suppressing the yij indices for the
sake of brevity)
|{xi + dz, i = 1, 2, ...n}〉 = T̂i (dz) |{xi, i = 1, 2, ...n}〉 =[T̂i (0) +
dT̂i(z)dz
∣∣∣z=0
dz...]|{xi, i = 1, 2, ...n}〉
= [I + p̂idz...] |{xi, i = 1, 2, ...n}〉(15)
Hence,
∂〈{xi,i=1,2,...n}|ψ〉∂xi
= limdz→0
〈{xi+dz,i=1,2,...n}|ψ〉−〈{xi,i=1,2,...n}|ψ〉dz
= p̂↑i 〈{xi, i = 1, 2, ...n} | ψ〉 = −p̂i 〈{xi, i = 1, 2, ...n} | ψ〉 ⇒ p̂i = − ∂∂xi(16)
so that T̂i (z) = e−z ∂
∂xi . The following commutation rule holds between x̂iand p̂i
[x̂i, p̂j] = δij (17)
The condition of an isolated market ensures that the basis and hence the Hilbert space
does not depend on time. This implies that the temporal evolution of the system is
unitary.
Creation & Annihilation Operators for Securities
We define âij (z)as the annihilation operator of the security j from the portfolio of
investor i for a price z i.e. when operator âij (z) acts on a state, the number of units of
security j is reduced by one from the portfolio of investor i for a price z.Similarly, we
define creation operators â↑ij (z) as the adjoint of the annihilation operators that increasethe number of units of security j in the portfolio of investor i for a price z.The precise
action of these operators on a state vector is defined by the following
âij(z) |{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉 =√
yij(z).z |{xi, {yij (z) − 1, j = 1, 2, ...m} , i = 1, 2, ...n}〉(18)
and
â↑ij(z) |{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉 =√
(yij(z) + 1)z |{xi, {yij (z) + 1, j = 1, 2, ...m} , i = 1, 2, ...n}〉(19)
where the factor ‘z’ has been introduced in the eigenvalues to ensure “scale invariance”
of the theory.
These operators satisfy the following commutation relations:-[âij(z), â
↑ij(z
′)]
= zδzz′δikδjl (20)
and
[âij(z), âkl(z′)] =
[â↑ij(z), â
↑ij(z
′)]
= 0 (21)[T̂i (z) , âjk (z
′)]
=[T̂i (z) , â
↑jk (z
′)]
= 0 (22)[T̂ ↑i (z) , âjk (z
′)]
=[T̂ ↑i (z) , â
↑jk (z
′)]
= 0 (23)
-
18 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27
Further more
â↑ij (z) âij (z) |{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉 = zyij (z) |{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉(24)
which implies that the number operator would be
ŷij (z) =â↑ij (z) âij (z)
z(25)
Using the aforesaid operators we can construct an arbitrary basis state from the ground
state as follows
|{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉 =n∏
i=1
T̂i (xi)m∏
j=1
∏{z,yij(z)∈N}
(â↑ij (z)
)yij(z) |0〉(26)
Buying and selling operators
The buying (selling) operation of a security is, in each case, a composite operation
consisting of the following:-
i. the creation (annihilation) of a security at the relevant price z; and
ii. the decrease (increase) in the cash balance by z of the investor undertaking the
trade.
Hence we can define the buying (selling) operator as composite of the cash translation
operator and the creation (annihilation) operators for securities as follows:-
b̂↑ij (z) = â↑ij (z) T̂
↑i (z) = â
↑ij (z) T̂i (−z) (27)
for the “buying” operation and
b̂ij (z) = âij (z) T̂i (z) (28)
for the “selling” operation. These operators satisfy the following commutation rules[b̂ij (z) , b̂
↑kl (z
′)]
= zδzz′δikδjl (29)
[b̂ij (z) , b̂kl (z
′)]
=[b̂↑ij (z) , b
↑kl (z
′)]
= 0 (30)
[b̂ij (z) , T̂k (z
′)]
=[b̂↑ij (z) , T̂k (z
′)]
= 0 (31)
[b̂↑ij (z) , x̂k
]= zδikb̂
↑ij (z) (32)[
b̂ij (z) , x̂k
]= −zδikb̂ij (z) (33)
-
Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27 19
1.2 Temporal Evolution of Financial Markets
In analogy with quantum mechanics, we mandate that the state of the market at a given
instant of time ‘t’, is represented by a vector in the Hilbert space H whose components
determine the statistical nature of the market. Hence the temporal evolution of the
market in essentially determined by the evolution of this vector with the flow of time. In
the Schrödinger picture, the time evolution of a system can be characterized through a
unitary evolution operator∧U (t, t0) in H, that acts on the initial state |ψ (t0)〉 to transform
it to |ψ (t)〉 i.e|ψ (t)〉 = Û (t, t0) |ψ (t0)〉 (34)
The assumption of the market being isolated and hence
Ψ = {|{xi, {yij (z) , j = 1, 2, ...m} , i = 1, 2, ...n}〉} being a complete basis at all times, andthe conservation of probability i.e.
∑l
|Cl (t)|2 = 1,∀t together with the group property
of∧U (t, t0) implies that the temporal evolution is unitary i.e.
U (t, t0) U↑ (t, t0) = U↑ (t, t0) U (t, t0) = 1 (35)
Furthermore Û (t0, t0) = 1. Defining the Hamiltonian Ĥ (t) = i∂∂t
Û (t, t0)∣∣∣t=t0
as the in-
finitesimal generator of time translations (evolution) we obtain, through a Taylor’s ex-
pansion up to first order Û (t + δt, t0) = Û (t, t0) +∂Û∂t
(t + δt, t)∣∣∣δt=0
Û (t, t0) δt + ...or
∂Û (t, t0)
∂t= lim
δt→0Û (t + δt, t0) − Û (t, t0)
δt= −iĤ (t) Û (t, t0) (36)
with the immediate solution Û (t, t0) = e− � tt0 Ĥ(t)dt where time ordering of the operators
constituting the Hamiltonian is assumed.
Before progressing further with the development of the model, some observations are in
order about the theory developed thus far.
(1) In standard quantum mechanics, Ĥ (t) is usually a bounded operator and hence the
exponential series in Û (t, t0) = e− � tt0 Ĥ(t)dtconverges so that its approximation to first
order is acceptable giving i∂|ψ(t)〉∂t
= Ĥ (t) |ψ (t)〉 which is the Schrödinger equationof wave mechanics. This may not always be the case in financial markets.
(2) Since time evolution of financial market, essentially, occurs through trades in securi-
ties, it is appropriate to infer that the Hamiltonian represents the trading activities
of the market.
(3) In order that the evolution operator Û (t, t0) is well defined, we mandate that the
Hilbert space His so constructed that the kernel of Û (t, t0) is empty.
1.3 Modeling Time Value of Money
Time value of money and interest rate instruments are classically modeled through the
first order differential equation dB(t)dt
= r (t) B (t)with the solution B (t) = B (0) e�
r(t)dt.
-
20 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27
A possible candidate for the Hamiltonian function H(in the classical picture) that would
generate this temporal development as the equations of motion is
H (x, p; t) =n∑
i=1
Hi (xi, pi; t) =n∑
i=1
ri (t) xi (t) pi (t) (37)
This Hamiltonian leads to the following equations of motion
dxi (t)
dt=
∂Hi (xi, pi; t)
∂pi= ri (t) xi (t) ,
dpi (t)
dt= −∂Hi (xi, pi; t)
∂xi= −ri (t) pi (t) (38)
While the interpretation of first of these equations is straightforward being the growth
of cash reserves of the ithinvestor with the instantaneous rate ri (t), the implications of
second equation are more subtle. To provide a financial logic to this equation, we note
that pi is the infinitesimal generator of cash translations in the classical picture and hencedpi(t)
dt= −∂Hi(xi,pi;t)
∂xi= −ri (t) pi (t) represents the rate of change of the cash translations
generator which, given a fixed rate of growth of cash, would decrease with the amount of
cash translations.
Using the Weyl formalism for transformation from the classical to the quantum pic-
ture, we require that the quantum mechanical analog of H (x, p; t) be Hermitian and
symmetric in its component operators. Hence, we postulate the ansatz
Ĥ (x̂ (t) , p̂ (t) ; t) =n∑
i=1
Ĥ (x̂i (t) , p̂i (t) ; t) =n∑
i=1
iri (t)
2(x̂ip̂i + p̂ix̂i) =
n∑i=1
iri (t) x̂i
(p̂i +
1
2Î
)(39)
for the quantum mechanical Hamiltonian representing the time value of money, so that
the time development operator is
Û (t, t0) = e
�−i
t�t0
Ĥ(t)dt
�= e
n�i=1
t�t0
ri(t)xi(p̂i+ 12 Î)dt(40)
which may be evaluated using standard methods like Green’s functions and Feynmann
propagator theory.
1.4 Representation of Trading Activity
Let us consider a deal in which an investor ‘i’ buys a security ‘j’ at a price of ‘z’ units
and immediately thereafter sells the same security to another investor ‘k’ at a price of
‘z′’ units and credits/debits the difference z′ − z to his cash account. The compositetransaction will, in our operator formalism, take the form b̂ij (z
′) b̂↑ij (z). In analogy withthis argument, we can represent the Hamiltonian for trading activity of the market as
HTr (t) =∑i,j,k,l
∞∫0
dz
z
∞∫0
dz′
z′hijkl (ξ, t) b̂
↑ij (z) b̂kl (z
′) (41)
where ξ = ln z′
zensures that the amplitudes are scale invariant.
-
Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27 21
1.5 Probability Distribution of Stock Prices
We now derive the probability distribution of stock prices in market equilibrium and show
that the prices follow a lognormal distribution, thereby vindicating the efficacy of this
model.
For this purpose, we assume that an investor i = α buys one unit of a security j = β
at time t = ti for a price z. We need to ascertain the probability PT (z′ |z )i.e. the
probability of the security j = β having a price z′ at time tf = ti + T .We assume thatduring the period tf − ti, investor α holds exactly one unit of β and that before ti andafter tf ,α holds no unit of β.
Let∣∣∣ψz
αβ(ti)
〉be the state that represents investor α holding exactly one unit of β at a
price z at time tiin the Hilbert space H. Hence, we have∣∣∣ψz
αβ(ti)
〉= b̂↑αβ (z)
∣∣∣ψαβ (ti)〉where∣∣∣ψαβ (ti)〉is the state that represents investor α not holding any unit of β. This also im-plies that b̂αβ (z)
∣∣∣ψαβ (ti)〉 = 0.Let us assume that the final state corresponding to theinitial state
∣∣∣ψzαβ
(ti)〉
is represented by∣∣∣ψz
αβ(tf )
〉so that
∣∣ψzαβ(tf )〉 = Û(ti, tf ) ∣∣ψzαβ(ti)〉 = e−itf�
ti
Ĥdt
b̂↑αβ(z)∣∣∣ψαβ(ti)〉 (42)
The amplitudes of∣∣ψz′αβ (tf )〉 are determined in the usual way by taking scalar product〈
ψz′
αβ(tf )
∣∣∣ ψzαβ
(tf )〉
and we have, for the matrix elements of the propagator
G (z′, tf ; z, ti) =〈ψαβ(tf )
∣∣∣ b̂αβ (z′) e−itf�
ti
Ĥdt
b̂↑αβ(z)∣∣∣ψαβ(ti)〉 (43)
In this case, the trading Hamiltonian will contain creation and annihilation operators
relating to the investor α and those relating to the securityβ i.e., it will be of the form
ĤTr (t) =∑k,l
∞∫0
dz
z
∞∫0
dz′
z′hαβkl (ξ, t) b̂
↑αβ (z) b̂kl (z
′) (44)
We further make the assumption that the amplitudes can be approximated by their first
two moments about ξ = 0, being sharply peaked about z′ = zsince, in the timescalesbeing considered, most trades would occur around z. Hence, we have
hαβkl ∼[Ωαβkl (t) − iξ−1Ξαβkl (t)
]δ (ξ) (45)
Noting that ξ = ln z′
z, we have ξ−1 =
(ln z
′z
)−1=(
z′z− 1)−1 = z
z′−z to first order and
δ (ξ) = δ(ln z
′z
)= δ (z′ − z)
[d�ln z
′z
�
dz′
]−1= z′δ (z′ − z). Using these results and eqs. (44)
& (45), we obtain
ĤTr (t) ∼∑k,l
∞∫0
dz
z
∞∫0
dz′
z′zδ (z′ − z)
[Ωαβkl (t) − i z
z′ − zΞαβkl (t)]b̂↑αβ (z) b̂kl (z
′)
-
22 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27
=∑k,l
∞∫0
dz
zb̂↑αβ (z)
[Ωαβkl (t) + izΞαβkl (t)
∂
∂z
]b̂kl (z
′) (46)
We note that this expression for the Hamiltonian is linear in ∂∂z
and hence it can be
diagonalized in the “momentum space” through a Fourier transformation and we have
ĤTr (t) =1
2π
∑k,l
∞∫0
dz
z
∞∫0
dz′
z′
∞∫−∞
dpb̂↑αβ (z) [Ωαβkl (t) + iΞαβkl (t) p] b̂kl (z′) eipξ (47)
The assumption of market equilibrium implies that the Hamiltonian should be inde-
pendent of time over the relevant timescales that would be much smaller than those
determining aggregate market behaviour so that we may write eq. (43) as
G (z′, tf ; z, ti) =〈ψ
αβ(ti)
∣∣∣ b̂αβ (z′) e−iĤ(ti)T b̂↑αβ (z) ∣∣∣ψαβ (ti)〉 (48)Because of the Hamiltonian being diagonal in momentum space, it is more convenient to
work in momentum space for evaluating the propagators and we have, for the equivalent
of eq. (48) in momentum space as
G̃ (p′, p;T, ti) =〈ψ
αβ(ti)
∣∣∣⎡⎣ ∞∫
0
dz′
z′eip
′ln(z′/κ)b̂αβ (z′)
⎤⎦ e−iĤ(ti)T⎡⎣ ∞∫
0
dz
ze−ipln(z/κ)b̂↑αβ (z)
⎤⎦ b̂↑αβ (z) ∣∣∣ψαβ (ti)〉(49)
To solve the problem further, we make use of second order perturbation theory. The first
step is to split the Hamiltonian into components as follows
Ĥ (t) =∑
l
∞∫0
dz
zb̂↑αβ (z) [Ωαβαl (t) + Ξαβαl (t) p] b̂αβ (z)+
∑k,l,k �=α
∞∫0
dz
zb̂↑αβ (z) [Ωαβkl (t) + iΞαβkl (t) p] b̂kl (z
′)
(50)
Let Eibe the energy eigenstate of the unperturbed Hamiltonian i.e. of the state of the
market before the purchase of security β by the investor α , then the energy eigenstate
of the Hamiltonian Ĥ (ti)i.e. after the purchase of security β by the investor α will be of
the form Ep = Ei +∑l
[Ωαβαl (ti) + iΞαβαl (ti) p]− ip2σ2where the second term representsthe impact on the energy eigenstates of the transactions involving investor α or security
β and the last term is the second order perturbation term due to the overall fluctuations
of the market. Substituting this value of Ep in eq. (49) and noting that the Hamiltonian
and hence the propagator G̃ (p′, p; T, ti)is also diagonal in “momentum space”, we have
G̃ (p′, p; T, ti) ∼ 2πδ (p′ − p) e−iTEp = 2πδ (p′ − p) e−iT [Ei+Ω(ti)+iΞ(ti)p−ip2σ2](51)
where∑l
Ωαβαl (ti) = Ω (ti) ,∑l
Ξαβαl (ti) = Ξ (ti) .
Inverting back to “coordinate space”, we obtain
G (z′, tf ; z, ti) =1
2π
∞∫−∞
dpe−iT [Ei+Ω(ti)+iΞ(ti)p−ip2σ2]−ip ln z′/z ∼ e
iT (Ei+Ω)
2σ√
πTe
�(ln(z′/z)+ΞT)2
4σ2T
�
(52)
-
Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27 23
The probability PT (z′ |z )i.e. the probability of the security j = β having a price z′ at
time tf = ti + T will then be proportional to the square of the above amplitude and
hence, we finally obtain
PT (z′ |z ) α |G (z′, tf ; z, ti)|2 =
(4πσ2T
)−1e
�(In(z′/z)+ΞT)2
2σ2T
�(53)
which agrees perfectly with the standard stochastic theory of finance wherein stock re-
turns are modeled extensively through lognormal distributions.
2. Conclusions
The following interesting observations emanate from the above analysis:-
(1) Eq. (53), on comparison with the standard expression for probability distribution
of stock price in the conventional stochastic calculus based approach to the Black Scholes
formula, identifies Ξ with the expected return on stock. This return is independent of
the eigenvalue Eiand hence, the state of the market. A financial interpretation of this
could be that the stock returns are dependent on the performance of the company and
independent of market dynamics.
(2) Independence of stock returns of the market dynamics would, however, mandate
that the stock volatility measured by the standard deviation σ is related to the stock
market dynamics which seems justified since higher trading volumes would imply greater
volatility and vice versa.
(3) If we define the uncertainty of measurement of a random variate by its standard
deviation, then, from eqs. (52) & (53), we have the uncertainty for the stock price process
zand its Fourier conjugate p, after a time T , as σz = σ√
Tand σp =1
2σ√
Tso that σzσp =
12
as it should be, since the distribution of z is assumed Gaussian in the aforesaid analysis.
(4) Furthermore, σzσp
= 2σ2T which enables the identification of σ2 as the reciprocal
of the mass and hence, the inertia of the stock price process. It is intriguing to note that
the same analogy follows through another completely independent analysis i.e. the Black
Scholes equation for the option price in its standard form is given by ∂C∂t
= −rSt ∂C∂S −12σ2S2t
∂2C∂S2
+ rC, where C (St, t) denotes the instantaneous price of a call option with
exercise price E at any time t before maturity when the price per unit of the underlying
is St. Making the substitution St = exwe obtain ∂C
∂t= −r ∂C
∂x− 1
2σ2 ∂
2C∂x2
+ 12σ2 ∂C
∂x+ rC
which, when compared with the standard quantum mechanical Hamiltonian in one degree
of freedom identifies σ2 as the reciprocal of the mass of the underlying system.
Contemporary quantitative finance is dominated by stochastic modeling of market
behaviour. These models are essentially in the nature of tools of data analysis that aim
to predict future events by applying probabilistic methods to historical data. Empirical
evidence testifies that probability distributions of stock returns are negatively skewed,
have fat tails and show leptokurtosis [56]. Some of the features of empirical distributions
of stock prices are modeled through Levy distributions [57-60], stochastic volatility [61]
or cumulant expansions around the lognormal case. Each of these models, however,
-
24 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27
attempts to empirically attune the model parameters to fit observed data and hence, is
equivalent to interpolating or extrapolating observed data in one form or the other.
Hence, stochastic models fail to take cognizance of causal factors that get submerged
in the superficial patterns exhibited by the avalanche of data being analysed. In actual
fact, every new price determination of a security and hence, the fluctuation of prices is
attributable to a new trade in the relevant security at that price. The “trading process”
therefore manifests itself as a price history of a security. The fundamental limitation of
stochastic tools in simulating extended memory effects is circumvented by this approach.
An attempt has also been made through this “toy model” to establish that a quantum
mechanical version of financial markets results in a temporal evolution of the probabil-
ity distribution analogous to that of simple stochastic systems. Stochastic models also
lack ability to accommodate collective effects like phase coherency in lasers that could,
possibly, be built into this quantized description.
It need be emphasized here that the above is purely a phenomenological model for
modeling stock behavior. It is fair to say that the current stage of research in financial
processes is dominated by the postulation of phenomenological models that attempt to
explain a limited set of market behavior. There is a strong reason for this. A financial
market consists of a huge number of market players. Each of them is endowed with
his own set of beliefs about rational behavior and it is this set of beliefs that govern
his actions. The market, therefore, invariably generates a heterogeneous response to
any stimulus. Furthermore, “rationality” mandates that every market player should have
knowledge and understanding about the “rationality” of all other players and should take
full cognizance in modeling his response to the market. This logic would extend to each
and every market player so that we have a situation where every market player should have
knowledge about the beliefs of every other player who should have knowledge of beliefs
of every other player and so on. We, thus, end up with an infinitely complicated problem
that would defy a solution even with the most sophisticated mathematical procedures.
Additionally, unlike as there is in physics, financial economics does not possess a basic
set of postulates like General Relativity and Quantum Mechanics that find homogeneous
applicability to all systems in their domain of validity.
-
Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27 25
References
[1] A. J. Macfarlane, J.Phys., A 22, (1989), 4581;
[2] L.C. Biedenharn, J.Phys., A 22, (1989), L873;
[3] S. Zakrzewski, J.Phys., A 31, (1998), 2929 and references therein; Shahn Majid, J.Math. Phy., 34, (1993), 2045;
[4] Michael Schurmann, Comm. Math. Phy., 140, (1991), 589;
[5] C. Blecken and K.A. Muttalib, J.Phys., A 31, (1998), 2123;
[6] J. P. Singh, Ind. J. Phys., 76, (2002), 285;
[7] U. Franz and R. Schott, J. Phys., A 31, (1998), 1395;
[8] V.I. Man’ko et al, Phy. Lett., A 176, (1993), 173; V.I. Man’ko and R.Vileta Mendes,J.Phys., A 31, (1998), 6037;
[9] W. Paul & J. Nagel, Stochastic Processes, Springer, (1999);
[10] J. Voit, The Statistical Mechanics of Financial Markets, Springer, (2001);
[11] Jean-Philippe Bouchard & Marc Potters, Theory of Financial Risks, Publication bythe Press Syndicate of the University of Cambridge, (2000);
[12] J. Maskawa, Hamiltonian in Financial Markets, arXiv:cond-mat/0011149 v1, 9 Nov2000;
[13] Z. Burda et al, Is Econophysics a Solid Science?, arXiv:cond-mat/0301069 v1, 8 Jan2003;
[14] A. Dragulescu, Application of Physics to Economics and Finance: Money, Income,Wealth and the Stock Market, arXiv:cond-mat/0307341 v2, 16 July 2003;
[15] A. Dragulescu & M. Yakovenko, Statistical Mechanics of Money, arXiv:cond-mat/0001432 v4, 4 Mar 2000;
[16] B. Baaquie et al, Quantum Mechanics, Path Integration and Option Pricing:Reducing the Complexity of Finance, arXiv:cond-mat/0208191v2, 11 Aug 2002;
[17] G. Bonanno et al, Levels of Complexity in Financial markets, arXiv:cond-mat/0104369 v1, 19 Apr 2001;
[18] A. Dragulescu, & M. Yakovenko, Statistical Mechanics of money, income and wealth:A Short Survey, arXiv:cond-mat/0211175 v1, 9 Nov 2002;
[19] J. Doyne Farmer, Physics Attempt to Scale the Ivory Tower of Finance, adap-org/9912002 10 Dec 1999;
[20] V. Pareto, Cours d’Economie Politique (Lausannes and Paris),(1897);
[21] L. Batchlier, Annelas Scientifiques de l’Normal Superieure III-17 21-86,(1900); P.Cootner, The Random Character of Stock Market Prices (Cambridge, MA: MIT Press) Reprint ,(1964);
[22] F. Black & M. Scholes, Journal of Political Economy, 81, (1973), 637;
[23] R. C. Merton, Journal of Financial Economics, (1976), 125;
[24] M. Nagasawa, Stochastic Processes in Quantum Physics, Birkhauser, (2000);
-
26 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27
[25] E. Purgovecki, Stochastic Quantum Mechanics and Quantum Spacetime: Aconsistent unification of relativity and quantum theory based on stochastic spacesReidel, Dordrecht, 1st printing 1984, revised printing, 1986
[26] M. Baxter & E. Rennie, Financial Calculus, Cambridge University Press, (1992).
[27] H. Risken, The Fokker Planck Equation, Springer, (1996);
[28] R.N. Mantegna & H.E. Stanley, An Introduction to Econophysics, Cambridge, (2000);
[29] M.M. Dacrrogna et al, J. Int’l Money & Finance, 12, (1993), 413;
[30] R.N. Mantegna & H.E. Stanley, Nature, 383, (1996), 587;
[31] R.N. Mantegna, Physica A, 179, (1991), 232;
[32] P. Gopikrishnan et al, Phys. Rev. E 60, (1999), 5305;
[33] P. Gopikrishnan et al, Phys. Rev. E 62, (2000) R4493;
[34] P. Gopikrishnan et al, Physica A, 299, (2001), 137;
[35] P. Gopikrishnan et al, Phys. Rev. E 60, (1999) 5305;
[36] V. Plerou et al, Phys. Rev. E 60, (1999) 6519;
[37] W.F. Sharpe, Portfolio Theory & Capital Markets, McGraw Hill, (1970);
[38] E.J. Elton & M.J. Gruber, Modern Portfolio Theory, & Investment Analysis, Wiley,(1981);
[39] S.M. Ross, Stochastic Processes, John Wiley, (1999);
[40] A. Ott el al., Phys. Rev.Lett. 65, (1990) 2201; J.P.Bouchaud et al., J.Phys.(France)II 1, (1991), 1465 ; C.-K. Peng et al., Phys. Rev. Lett. 70, (1993), 1343; R.N Mantegnaand H.E Stanley, Nature (London) 376, (1995) 46; T.H.Solomon et al., Phys. Rev.Lett.71, 3975 (1993); F.Bardou et al., ibid. 72, (1994), 203 ;
[41] J. Klafter and G. Zumofen, Phys. Rev E 49, (1994), 4873,4;
[42] H. Spohn, J. Phys. (France) I 3, (1993), 69;
[43] M. Muskat, The Flow of Homogeneous Fluids Through Porous Media (McGraw-Hill,New York, (1937);
[44] J. Buckmaster, J. Fluid Mech. 81 (1995), 735;
[45] E.W. Larsen and G.C. Pomraning, SIAM J. Appl. Math. 39, (1980), 201;
[46] W.L Kath, Physica D 12, (1984), 375;
[47] J. Feigenbaum & P. G. O. Freund, Int. J Mod. Phys. B 10, (1996), 3737;
[48] D Sornette, A. Johansen & J.P. Bouchaud, J. Phys. I (France ) 6, (1996), 167;
[49] D. Sornette, Phys. Rep. 297, (1998), 239;
[50] A. Wolf, J.B. Swift, S.L. Swinney & J.A. Vastano, Determining Lyapunov ExponentsFrom a Time Series, Physica 16D, (1985), 285;
[51] B.B. Mandlebrot, The Fractal Geometry of Nature, Freeman Press, (1977);
[52] G. DeBoek, Ed., Trading on the Edge, Wiley, (1994);
-
Electronic Journal of Theoretical Physics 3, No. 11 (2006) 11–27 27
[53] J.G. DeGooijer, Testing Nonlinearities in World Stock Market Prices, EconomicsLetters, 31, (1989);
[54] E. Peters, A Chaotic Attractor for the S&P 500, Financial Analysts Journal,March/April, (1991);
[55] E. Peters, Fractal Structure in the Capital Markets, Financial Analysts Journal,July/August, 31, (1989); P. Cootner, Ed., The Random Character of Stock MarketPrices, Cambridge MIT Press, (1964);
[56] E. Peters, Chaos & Order in the Capital Markets, Wiley, (1996) and referencestherein;
[57] L. Andersen L & J. Andreasen, Review of Derivatives Research, 4, (2000), 231;
[58] J.P. Bouchaud et al, Risk 93, (1996), 61;
[59] J.P. Bouchaud & M.Potters, Theory of Financial Risks, Cambridge, (2000);
[60] E. Eberlein et al, Journal of Business 71(3), (1998), 371;
[61] B. Dupire, RISK Magazine, 8, January 1994;
-
EJTP 3, No. 11 (2006) 29–32 Electronic Journal of Theoretical Physics
Rayleigh process and matrix elements for theone-dimensional harmonic oscillator
J.H. Caltenco1∗, J.L. López-Bonilla1†, J. Morales2‡
1Escuela Superior de Ingenieŕıa Mecánica y EléctricaInstituto Politécnico Nacional
Edif. Z, Acc. 3-3er Piso Col. Lindavista C.P. 07738 México D.F.2Area de F́ısica AMA, CBI
Universidad Autónoma Metropolitana-Azc.Apdo. Postal 16-306, CP 02200 México DF
Received 21 December 2005 , Accepted 2 February 2005, Published 25 June 2006
Abstract: We show that, the matrix elements 〈m |e−γ x |n 〉 for the one-dimensional harmonicoscillator have application in Markov process theory, permitting thus to resolve the Fokker-Planck equation for the two-dimensional probability density corresponding to Rayleigh case.c© Electronic Journal of Theoretical Physics. All rights reserved.
Keywords: Matrix elements, One-dimensional harmonic oscillator, Markov process theory,Fokker-Planck equationPACS (2006): 03.65.Ta , 03.65.Ge ,02.50.Ga, 46.25.Cc, 02.70.Ns
1. Introduction
In [1-4] were calculated the matrix elements:
f(γ) = 〈m| e−γx |n〉 =∫ ∝−∝
ψ∗m(x) e−γ xψn(x)dx (1)
for the harmonic oscillator in one dimension, where γ ≥ 0 is an arbitrary parameter.Then, it was deduced the following result for m ≥ n:
f(γ) =
√n !
m !
(− γ√
2
)m−neγ2/4Lm−nn
(−γ
2
2
)(2)
∗ [email protected]† jlopezb@ipn,mx, [email protected]‡ [email protected]
-
30 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 29–32
in terms of the associated Laguerre polynomials Lqn.
It is interesting to observe that the 2nd order differential equation [5-8] defining to
Lpq permits to show, via (2), that f(γ)satisfies the equation:
d2f
dγ2+
1
γ
df
dγ− 1
4γ2(γ4 + 4Aγ2 + 4Q
)f = 0 (3)
where A = m + n + 1 and Q = (m − n)2. That is, (2) is solution of (3), with which it ispossible to obtain [9] the Morse’s radial wave function [10].
In Sec. 2, f(γ)is employed to resolve the nonstationary stochastic Fokker-Planck
equation (FPE) [11] for the Rayleigh distribution.
2. Two-Dimensional Probability Density Associated to Rayleigh
Process.
The equation (3) has the structure:
D1(γ)f =
(γ2
4+ A +
Q
γ2
)f (4)
where it appears the important Bessel’s operator [12]:
DC(γ) =d2
dγ2+
C
γ
d
dγ(5)
for the case C = 1. The operator (5) has interesting applications in hydrodynamics,
the theory of subharmonic functions, electrostatics, the Euler-Poisson-Darboux equation,
elasticity, the generalized radiation problem, quantum mechanics and generalized axially
symmetric potential. Here we shall show that, the Bessel’s operator D1 is useful for to
determine the probability density ω associated to Rayleigh process in two dimensions,
because the FPE can adopt a form similar to (4).
In fact, the nonstationary stochastic FPE for the Rayleigh distribution is given by
[11] p. 73:
ω̇ =∂
∂ x
[(β x − k
2x
)ω
]+
k
2
∂2ω
∂ x2(6)
being k and β positive parameters, then the corresponding eigenfunctions X (x) are
solutions of:
σ2d2X
d x2+
(x − σ
2
x
)d X
d x+
(1 +
σ2
x2+
λ
β
)X = 0 (7)
with σ2 = k2β
. The operator D1 participates when in (7) we make the following change
of functions:
F (x) = x−1ex2
4σ2 X (8)
obtaining thus the relation:
D1(x)F =
(x2
4σ4− 1
σ2− λ
σ2β
)F (9)
-
Electronic Journal of Theoretical Physics 3, No. 11 (2006) 29–32 31
On the other hand, in (4) it is possible to realize the formal change of variable:
γ =i
σx , i =
√−1 (10)
then it results the equation:
D1(x)f =
(x2
4σ4+
Q
x2− A
σ2
)f , (11)
with the same structure as (9); therefore Q = 0, that is m = n, and A = 2n+ 1 = 1 + λβ
,
then λ = 2nβ , n= 0,1,2,. . . Besides, F is proportional to f given by (2) with the change
(10):
F ∝ e− x2
4σ2 Ln
(x2
2σ2
)(12)
then (8), (12) and factors of normalization lead us to the eigenfunctions:
Xn(x) =x
n!σ2e−
x2
2σ2 Ln
(x2
2σ2
)(13)
which are solutions of (7) for λ = 2nβ. The result (13) is our principal aim because
it permits to write immediately the two-dimensional probability density associated to
Rayleigh case, to see [11].
-
32 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 29–32
References
[1] A. E. Glassgold and D. Holliday, Phys. Rev. A139 (1965) 1717.
[2] J. Morales, J. López-Bonilla and A. Palma, J. Math. Phys. 28 (1987) 1032.
[3] J. Morales and A. Flores-Riveros, J. Math. Phys. 30 (1989) 393.
[4] J. López-Bonilla and G. Ovando, Bull. Irish Math. Soc. N.44 (2000) 61.
[5] C. Lanczos, Linear differential operators, D. Van Nostrand Co., London (1961).
[6] J. D. Talman, Special functions, W. A. Benjamin Inc. New York (1968).
[7] H. Hochstadt, The functions of Mathematical Physics, Dover, New York (1971).
[8] M. Abramowitz and I. A. Stegun, Handbook of mathematical functions, John Wileyand Sons, New York (1972).
[9] J. H. Caltenco, J. López-Bonilla and R. Peña-Rivero, J. Sci. Res. 50 (2002) 125.
[10] Ch. S. Johnson Jr. and L. G. Pedersen, Problems and solutions in QuantumChemistry and Physics, Dover, New York (1986).
[11] R. L. Stratonovich, Topics in the theory of random noise. Vol. I, Gordon and Breach,New York (1963).
[12] A. Weinstein, Ann. Mat. Pura Appl. 49 (1960) 359.
-
EJTP 3, No. 11 (2006) 33–70 Electronic Journal of Theoretical Physics
Identical synchronization in chaoticjerk dynamical systems
Vinod Patidar1∗ and K. K. Sud2
1Department of PhysicsBanasthali Vidyapith Deemed UniversityBanasthali - 304022, Rajasthan, INDIA
2Department of PhysicsCollege of Science Campus
M. L. S. University, Udaipur – 313002, INDIA
Received 23 December 2005 , Accepted 24 February 2006, Published 25 June 2006
Abstract: It has been recently investigated that the jerk dynamical systems are the simplest ever systems, which possessvariety of dynamical behaviours including chaotic motion. Interestingly, the jerk dynamical systems also describe various
phenomena in physics and engineering such as electrical circuits, mechanical oscillators, laser physics, solar wind driven
magnetosphere ionosphere (WINDMI) model, damped harmonic oscillator driven by nonlinear memory term, biological
systems etc. In many practical situations chaos is undesirable phenomenon, which may lead to irregular operations in
physical systems. Thus from a practical point of view, one would like to convert chaotic solutions into periodic limit cycle
or fixed point solutions. On the other hand, there has been growing interest to use chaos profitably by synchronizing chaotic
systems due to its potential applications in secure communication. In this paper, we have made a thorough investigation
of synchronization of identical chaotic jerk dynamical systems by implementing three well-known techniques: (i) Pecora-
Carroll (PC) technique, (ii) Feedback (FB) technique and (iii) Active Passive decomposition (APD). We have given a
detailed review of these techniques followed by the results of our investigations of identical synchronization of chaos in
jerk dynamical systems. The stability of identical synchronization in all the aforesaid methods has also been discussed
through the transversal stability analysis. Our extensive numerical calculation results reveal that in PC and FB techniques
the x-drive configuration is able to produce the stable identical synchronization in all the chaotic jerk dynamical systems
considered by us (except for a few cases), however y-drive and z-drive configurations do not lead to the stable identical
synchronization. For the APD approach, we have suggested a generalized active passive decomposition, which leads to the
stable identical synchronization without being bothered about the specific form of the jerk dynamical system. Several other
active passive decompositions have also been listed with their corresponding conditional Lyapunov exponents to achieve
the stable identical synchronization in various chaotic jerk dynamical systems.
c© Electronic Journal of Theoretical Physics. All rights reserved.
Keywords: Chaos, Jerk dynamical systems, Identical synchronization of chaos, synchronizedchaosPACS (2006): 05.45.+b; 47.52.+j; 05.45.-a
∗ vinod r [email protected]
-
34 Electronic Journal of Theoretical Physics 3, No. 11 (2006) 33–70
1. Introduction
Various studies of nonlinear dynamical systems in the last four decades have signif-
icantly extended the notion of oscillations in these systems. It has been shown that the
post-transient oscillations in dynamical systems can be associated not only with the regu-
lar behavior such as periodic or quasiperiodic oscillations, but also with chaotic behavior
[1-5].
Chaos has long-term unpredictable behavior, which is usually couched mathematically
as sensitivity to initial conditions i.e., where the system’s dynamics takes it, is hard to
predict from the starting point. One way to demonstrate this is to run two identical
chaotic systems side by side, starting both at very close, but not exactly equal initial
conditions. The systems soon diverge from each other, but both retain the same attractor
pattern. An interesting question to ask is: Can we force the two chaotic systems to follow
the same path on the attractor? i.e., Can chaotic systems be made synchronized? The
affirmative answer is possible to this question. It has been shown that some of the ideas of
synchronization can also be extended for the description of particular type of behaviour
in c