J
OURNAL DE
T
HÉORIE DES
N
OMBRES DE
B
ORDEAUX
M
ICHEL
P
LANAT
From Planck to Ramanujan : a quantum 1/ f
noise in equilibrium
Journal de Théorie des Nombres de Bordeaux, tome
14, n
o2 (2002),
p. 585-601
<http://www.numdam.org/item?id=JTNB_2002__14_2_585_0>
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Article numérisé dans le cadre du programme Numérisation de documents anciens mathématiques
From Planck
to
Ramanujan:
aquantum
1/f
noise in
equilibrium
par MICHEL PLANAT
RÉSUMÉ. J’introduis un nouveau modèle de bosons
thermiques
sans masse ; il
prédit,
pour lesfluctuations,
un spectrehyper-bolique
aux bassesfréquences.
On trouve que la fonction de par-tition par mode est la fonctiongénératrice
d’ Euler pour lenom-bre de
partitions
p(n).
Lesquantités
thermodynamiques
ont une structurearithmétique profonde :
elles sont données par desséries,
dont les coefficients de Fourier sont les fonctions sommatoires03C3k(n)
despuissances
des diviseurs de n, avec k = 20141 pourl’énergie
libre,
k = 0 pour le nombre departicules,
et k = 1 pourl’énergie
interne. Les contributions de bassefréquence
sont calculées parl’usage
de transformées de Mellin. Enparticulier, l’énergie
internepar mode
diverge
comme E/kT =
03C02/6x,
avec x =h03BD/kT, au
contraire del’énergie
de Planck E = kT. La théorie estappliquée
à la correc-tion de la loi de rayonnement du corps noir et au solide deDebye.
Les fluctuations fractionnaires de
l’énergie présentent
un spectreen
1/v
aux bassefréquences.
On en déduit un modèle satisfaisantpour les fluctuations d’un résonateur à quartz. On
rappelle
aussiles résultats essentiels de la théorie
mathématique
despartitions
deRamanujan-Rademacher.
ABSTRACT. We describe a new model of massless thermal bosons
which
predicts
anhyperbolic
fluctuation spectrum at lowfrequen-cies. It is found that the
partition
function per mode is the Eulergenerating
function for unrestrictedpartitions
p(n).
Thermody-namical
quantities
carry a strong arithmetical structure:they
aregiven by
series with Fourier coefficientsequal
to summatoryfunc-tions
03C3k(n)
of the power ofdivisors,
with k = -1 for the freeenergy, k = 0 for the number of
particles
and k = 1 for thein-ternal energy. Low
frequency
contributions are calculatedusing
Mellin transform methods. In
particular
the internal energy per modediverges
asE/kT=03C02/6x
with x=h03BD/kT
in contrast to the Planckenergy
E
= kT. Thetheory
isapplied
to calculate correctionsin black
body
radiation and in theDebye
solid. Fractionallow
frequency
range. Asatisfactory
model offrequency
fluctua-tions in a quartz
crystal
resonator follows. A sketch of the wholeRamanujan-Rademacher theory
ofpartitions
is reminded as well.1. Introduction
According
to theequipartition
law of statisticalmechanics,
the available noise powerP
in thefrequency
interval dv isequal
to[15]:
this result isessentially Nyquist’s
theorem for thevoltage
noisev2
at a resistorR,
,
P -
= kTdv where means the avera e value. Since
-
kT is
i.e.,
4R
=kTdv,
where()
means theaverage value. Since 2? = kT is
the mean energy per
mode, Nyquist proposed
to addquantum
correctionsas
E
=p(x),
with the Planck factorp(x) =
which x =hv/kT .
kT
_ exp (
-1
This result was
generalized
asFT-
= p(x)
+
to account for the zeropoint
energy. There are still controversies
concerning
thephysical
relevance ofthese relations: the Planck factor removed the ultraviolet
divergence
but this wasreincorporated
in the frame ofquantum
electrodynamics
~1~,~4~.
At the
present
stage,
quantum
statistical mechanics does not include infrared corrections of the1/v
type.
The infraredcatastrophe
was studiedpreviously
innon-stationary
processes such as thescattering
of electrons in an atomic field[3],[9].
Here we derive an alternative
approach
in which1/v
noise is aproperty
of
non-degenerate
bosons inequilibrium.
We first observe that thequantum
mechanicalpartition
function of a boson gas, withequally spaced energy
levels,
is the Eulergenerating
functionof p(n) :
the number of indiscernible collections of theinteger
n. It relates toelliptic
modular functions whichare very exactly known. As a result the main contribution in the mean
energy per mode is the infrared term
t - M2-
instead ofunity.
The newkT -
6
law also leads to fractional energy fluctuations of the whole gas.
Using
the newapproach
and thedensity
of states of the conventionalap-proach
we calculate the corrections toblack-body
radiationlaws,
including
thedensity
ofphotons,
theemissivity
and infrared fluctuations. We alsoapply
the calculations to thephonon
gas in aquartz
resonator.The
partition
function Z of a nondegenerate
boson gas isgiven
fromwhere the summation is
performed
over all the states s of theassembly.
In the conventionalapproach
it is thus considered that thepartition
function Z per mode offrequency
es =hvs
is such that ln Z = -In
black-body
radiation one accounts for the wave character of thequan-tum states
by
counting
the number I ofwavelengths
in a cubic box of size Lwhere the summation
(1)
should beperformed
over allintegers II, 12,
13
obeying (2).
This can be achieved
by removing
the discreteness of energy levels andreplacing
the sum(1)
by
anintegral
with
D(v) =
2 x thedensity
of states[11]:
the factor 2 occurs due to the twodegrees
of freedom ofpolarization,
c is thelight velocity
andV =
L3
the volume of thecavity.
From now we consider that with each mode is associated a set of
equally
spaced
energy levelsnhv, n integer,
so that thepartition
per mode becomesAs shown in Section
(2.1)
this accounts for newmultiparticle
microstatesnot considered so far.
The summation above is well known in number
theory
and can be veryaccurately
describedusing elliptic
modular functions. At is will beshown,
there are drastic consequences in the lowfrequency
part
of thespectrum,
while the
high frequency
part
is leftunchanged.
In the
following
thethermodynamical
quantities
will be defined as usualthe
occupation
number,
the internal energy, theentropy,
-, the
spectral
energy density,, the free energy,
the fluctuations of the internal energy.
In all the paper the
subscript -
will indicate that we restrict the calculation2.
Thermodynamics
of the Euler gas2.1. Euler
generating
function. Thepartition
function per mode Z in(4)
can be written in the Euler form[14]
with y = and 2? = This is
equivalent
to the Boltzmannsummation
where
p(n)
is thedegeneracy
parameter
of the energy level nhv. It is known in numbertheory
as the number of unrestrictedpartitions
of theinteger
n,that is the number of different ways of
calculating n
as a sum ofintegers.
For
example
with n = 4 we havep(4)
= 5 and thecorresponding
indis-cernible collections are
This can be
pictured
in terms of the energy levels. The collection(a)
means one
particle
on the level of index 4 and the threeremaining particles
on theground
state of index0,
i.e. 4hv = 1 x 4hv + 3 x Ohv. Thiscollection is the
only
one considered in the conventionalapproach.
Theother microstates from
(b)
to(d)
correspond
to differentpossibilities
ofbunching
of theparticles.
Collection(b)
means the fourparticles
on thelevel of index
1,
i.e. 4hv = 4 xhv,
collection(c)
means twoparticles
on thelevel 2 and two
particles
on theground
state,
i.e. 4hv = 2 x 2hv + 2 xOhv,
and so on.
Properties
of Eulergenerating
function were studied in full detailsby
Ramanujan
[10]
in 1918 andcompleted by
Rademacher[14]
in 1973. Animportant
result is theasymptotic
formula2.2. Riemann zeta function and the free energy of the Euler gas. The
partition
function2(x)
defined in(4)
is related to the Riemann zetafunction
((s)
through
the Mellin transform as follows(Ref.
[12],
Eq.
(6.3)
Introducing
as the sum ofkth
powers of the divisors of n and theDirichlet series
and
computing
the inverse Mellin transform one obtains([12],
p.467)
thefree
energy F
as followswith =
Ql(n)/n.
There is thus a closerelationship
between thearithmetic of and that of divisors. This will be confirmed in the derivation of the other
thermodynamical quantities.
Since the main contributions to
Z(x)
aregiven by
thepoles
at s = 0 ofr(s)
and~(s+1)
and at s = 1 ofC (s),
the free energy may beapproximated
in the low
frequency
part
of thespectrum
([5],
p.58)
with the error term
ln(1 -
2.3. Dedekind eta function and the internal energy of the Euler gas. One
easily
shows that the Mellin transform of theoccupation
number isr(s)~(s)2.
A similar derivation to the oneperformed
in Section(2.2)
leads toIn the low
frequency region
onegets
(see [6],
p.27)
where 0.577 is Euler constant.
The Mellin transform of the internal energy is
r(s)~(s)~(s -1)
and from the same method than aboveAn alternative derivation involves
elliptic
modularaspects.
According
toNinham
[12]:
All rrcathematics is atautology,
and allphysics
usesmathe-matics to look in
different
ways at afundamental
problem
of philosophy
The link between the modular group and the Euler
generating
functionis from the
equality
[14]
where the domain of
integration
ofZ(y)
is taken to be the upper halfcomplex plane
of the new variable THere we have
As shown in Section
(5)
Dedekind eta function acts on the full modulargroup
SL(2,
Z).
At thisstage
we do not enter into the full ramifications of thetheory
andonly emphasize
the connexion to the modular Eisenstein functionwhere the summation is
performed
over all non-zero relativeintegers
m and n and9(r)
> 0. It can be shown([16],
p.29)
thatG2(T)
connects to thelogarithmic
derivative ofq(T)
- - I I , , , ’"
with the Fourier
expansion
Using
(22), (23)
and(25)-(27)
the relation(21)
iseasily
recovered. The lowfrequency
expansion
of internal energy is as followsinstead of the Planck result E - kT.
One can also
compute
theentropy
S
fromAt very low
frequency
it results that the internal energy equals the3.
Application
toblack-body
radiation3.1. Stefan-Boltzmann constant revisited. The Stefan-Boltzmann
constant is an
integrated
measure of theemissivity
of a blackbody
[11].
In the conventional
approach
thepartition
function is calculated from theintegral
(3)
using
thedensity
of statesD(v)
= 8~
that iswith
((4) =
7r4 /90
and we used the Mellinintegral
formulaThe Stefan-Boltzmann constant CRSB is defined from the free energy
If instead of
(30)
one uses thegeneral
formulathe
interchange
of theintegral
and the sum leads toAs a result we find a free energy
(and
a modified Stefan-Boltzmanncon-stant)
in excess with a factor =((3) ~
1.20. If one uses thealternative derivation in terms of
the divisors
one recovers themathemati-cal formula
(16)
with s = 3 and k = -1.3.2. The
density
ofphotons.
The number ofphotons
in the bandwidth dv iswith the
occupation
numberN(v,
T) =
in the conventionalIn the
general approach
theoccupation
number is defined from thesum-mation
(19)
and we need to evaluateThis is in excess of a factor
((3) ~
1.20 as for the free energy. If onecompares the calculation in terms of divisors one recovers the mathematical
formula
(16)
with s = 3 and = 0.3.3. Planck radiation formula revisited. The energy within the
band-width dv is defined as
with
E(v,T)
= in the conventionalapproach
and withu(v,T)
the energyspectral density.
Weget
the Planck radiation formulaThe
black-body emissivity
is defined asAt very low
frequency
the conventional result leads to theRayleigh-Jeans
formulawhich is
independent
of Planck constant and isproportional
to the inverse of the square ofwavelength
A =c/v.
In the new
approach
theemissivity
isAt very low
frequency
one uses(28)
with the resultThus the
v2T dependence
isreplaced by
thevT 2
dependence,
the lowfrequency
emissivity
nowdepends
on the Planck constant and on the inversewavelength;
there is a ratio7’2between
the new result and the onepredicted
s3.4. Radiative atomic transitions. Let us now consider the
equilibrium
between atoms and a radiation
field, allowing
the emission orabsorption
ofphotons
offrequency
where 62 =
hv2
is the energy in the upper state and f¡ = in the lowerstate.
The conventional
theory,
as derived for the first timeby
Einstein[l 1],
states that the rate at which atoms make a transition 1 --3 2 in which one
photon
is absorbed isequal
to the rate at which atoms emitphotons,
sothat
where
Nl
andN2
are theoccupation
numbers of atoms in levels 1 and2,
A21
is thespontaneous
absorption
rate,
B12
is the induced emission rateand
u(v)
is the energydensity
in the radiation field asgiven
in(39).
In thermal
equilibrium
theoccupation
numbers in states 1 and 2obey
the Boltzmann law
Using
(46)
and(39)
onegets
the well known formulaswhere A =
c/v
is thewavelength
of the radiation field.If one uses the
general
formula onegets
lowfrequency
corrections inthe
spontaneous
to stimulated emission ratio.Using
the lowfrequency
expression
(28)
for the internal energy thisyields
The
A/B
lowfrequency
ratio nowdepends
on the inverse of the square ofwavelength
A and isindependent
of the Planck constant~,
in contrast tothe
hi À3 dependence
of the standard ratio. The spontaneous to stimulatedabsorption
rate is enhanced afactor ’ 2over
the conventional one.6x
3.5. Einstein’s fluctuation law revisited.
According
to theconven-tional Einstein’s
approach
[13]
the energy fluctuations of asystem
inOne can reformulate this relation for the fluctuations of the energy dE =
u(v,T)dv
in the bandwidth dvwith u the energy
spectral density
andSu (v)
the powerspectral density
of the fluctuations of u. Onegets([13],
p.429 )
The first term on the
right
hand side is the onecorresponding
to thehigh
frequency
part
of thespectrum
(Wien’s law):
it is of a purequantum
natureand is
corpuscular-like;
the second onecorresponds
to the lowfrequency
(Rayleigh-Jeans)
region:
it ispurely
classical and wavelike. In the lowfrequency
part
of thespectrum
they
are fractional energy fluctuations ofthe random walk
type
In the new
approach
one uses the lowfrequency
energydensity
u(v,
4~ v~
so that instead of(52)
onegets
This is the announced
quantum
1/v
fluctuationspectrum.
There is are-duced low
frequency
noise and the ratio between the new result and theEinstein-Rayleigh-Jeans
one is~.
4.
Application
to aphonon
gas and to the1/ f
frequency
noise of aquartz
resonator4.1. The
specific
heat of aphonon
gas revisited. Theproperties
ofthe
phonon
gas arequite
similar to those of thephoton
gasexcept
for thenew form of the density of modes as g(v) -
with3
=2 1
wherecph ph t 1
cph
represents
the average wavevelocity
and ct and cl are the transverse andlongitudinal
velocities for anisotropic
solid[11].
The maximal vibrationalfrequency
Vm(Debye
frequency)
is defined from the total number of allowedquantum states
In the conventional
theory
[11]
weget
The internal energy follows from the formula
and the constant volume
specific
heatCv
=equals
the
Debye function,
and xm -flp,
with
---; the
Debye
characteristictemperature.
The case
D(0D) -
1corresponds
to theDulong-Petit
valueCv
-3R. At very lowtemperatures
onegets
the cubictemperature
dependence
In the new
approach
Debye
results are foundunchanged
except
for an extramultiplicative
factor in thespecific
heat as was the case for theintegrated emissivity
in Section(3.1)
that isAt very low
temperatures
the electronic contribution to thespecific
heat which decreases asT,
dominates the latticecontribution,
which decreases asT3.
This is accounted for in the conventional way.4.2.
1 /f
noise in aquartz
resonator.Specific
heat is involved in theenergy fluctuations of a canonical ensemble from the relation
The relative energy fluctuations follows as
2013y ==
E7 which is of the3No
order
10-11.
TheAvogadro
numberequals
No
= 6.02 x1023 .
For energy fluctuations in the bandwidth
dv,
the main difference with the conventionaltheory
lies in the lowfrequency region,
as was the case ofThe method can be used to
predict
fractionalfrequency
fluctuations in aquartz
crystal
resonator from theformula ~[7]-[8]
where a; and
Q
are thefrequency
andquality
factor of the resonator.Using
cph - 3.5 x
103
m/s,
we findAph -
5 x10-4.
For a 5 MHz P5quartz
crystal
resonator withQ -
2 x106,
the activeregion
under the electrodes has thickness t =5A/2 -
3 mm, and section S N 3cwn2,
that is V - 1cm3.
The
resulting
1/v
factor ish-1
=A h 102
6 XlO-24.
This is the order ofmagnitude
found inexperiments
[7].
5.
R.amanujan-R,ademacher theory
ofpartitions:
a short reminder
Besides the low
frequency approximations
encountered in Section(2)
there is a an exact method to calculate the number ofpartitions
p(n)
first discoveredby Ramanujan
[10]
andimproved by
Rademacher[14]
thanks toan
integration
along
Ford circles in thecomplex
halfplane.
For complete-ness we remind here the mainpoints
of thetheory
from which the resultsin Section
(2)
may also be derived .From well-known mathematical
arguments
[10]
(p. 113)
one canget
theleading
term for the case 0 y 1 and y -3 1 from theexpression
The use
of y =
exp(-hv/kT)
corresponds
to the lowfrequency
approxima-tion at v -0,
that is1 - y
= 1 -hvlkt.
This leads tothe
leading
lowfrequency
term in the free energy(18)
and internal energy(28).
They
are similar formulas associated with rationalpoints
which arelo-cated at
on the unit circle
Iyl
= 1. Theleading
term in theexpansion
ofZ(y)
corresponds
to the fundamentalmode 2 - 1*
The
general
method tocompute
rational contributions is a masterpiece
of the mathematics of the 20th
century([10]),
([14) .
It uses the connectionof
Z(y)
to theelliptic
modular functions.I To establish the formula one writes the equation for a lossy harmonic oscillator and one
5.1. The fundamental contribution. To
compute
the contribution of the fundamentalpoint
1/1
of the unit circleIyl
= 1 one uses theproperty
((2), p. 96, [5],p.58)
In the low
frequency region y
=exp( -z) -
1 sothat
= 0and
2(y) ,
1. Lowfrequency approximations
of the free energy(18)
and of the internal energy(28)
follow. There are similar formulas associatedwith the other rational
points
of the circle as shown below.To
get
theleading
term inp(n)
one uses theCauchy
formulawhere i
means anarbitrary
closedloop
encircling
theorigin.
Substituting
(65)
in(66)
with2(y’)
= 1 one can obtainThis includes
(14)
in the limit n - oo but is much more accurate.5.2.
Farey
contributions and Ford circles. From now on we extendthe domain of definition of
Z(y)
to thecomplex plane
and we introduce the new variable T and the Dedekind eta function as defined in(22)-(24).
It can be shown that is a modular form of
degree
-1/2
on thefull modular group. It acts on the
generators
of such a groupthrough
therelations
[2] 2
To express the
partition
function one uses theCauchy
formulaIn the third term above this
corresponds
to apath
of unitlength starting
at an
arbitrary
point
in 7~.2For more general modular transformations, we have
The choice of the
integration path
comesalong
in a natural wayby using
the connection of
2(y)
to the modular group. Let us observe that the setof
images
of the line T = X +i,
Xreal,
under all modular transformationscan be written as
Equation
(71)
defines circlesC(p,
q)
centered atpoints T
= Q
+ 2~
with radius1/2q2.
They
are named after L. R. Ford who first studied theirprop-erties in 1938
(14~.
Ford circles areeasily generated by using
the orderedFarey
sequenceTo
each P
belongs
a Ford circle in the upper halfplane,
which istangent
to the real axis at
T - Q .
It can be observed that Ford circles neverintersect.
They
aretangent
to each other if andonly
ifthey
belong
tofractions which are
adjacent
in someFarey sequence.
If
q
q
are threeadjacent
fractions in aFarey sequence
then 1 q q2C(p, q)
touchesC(pl,
ql)
andC(P2, q2)
respectively
at thepoints
where
In Rademacher’s
approach
(which
improves
Ramanujan’s
one)
the unitlength
path
on 1-£ is chosen so as to goalong
Ford circleswhere is the upper arc on a Ford circle which connects
points
oftangency
at
T 9
and7~.
Each Ford circle
C(p, q)
is labelledby
theexpression
r= 9
+(,
where thevariable (
runs on an arc of the circle~~-2~~ - 2~.
If one uses z suchthat (
=FIGURE 1. Rademacher’s
path
ofintegration.
transforms as
where and
R
follow from(73).
5.3.
Farey
contributions and Dedekind sums. Tocompute
(76)
one uses the transformation formula(22).
After somemanipulations
andus-ing
z/q
instead of z(see
Ref.[14],
p.269),
onegets
the formula whichgeneralizes (65)
The so-called Dedekind sums
s(p,
q)
are introducedby
where
[ ] in (79)
denotes theinteger
part.
For the calculation
of p(n)
one uses anapproximation
similar to the oneused in
(65).
If z is a smallpositive
realnumber,
then y
is nearthe modulus at that
point
= 0 and2(y’) -
1.As a result
(76)
can bereadily integrated
and the final result isThe
physical
meaning
of thesehigher
modes has still to be understood.Acknowledgements
A first version of this
manuscript
waspresented
at the 8th Van der ZielQuantum
1/ f
NoiseSymposium
in St-Louis(Missouri),
June 5-6(2000).
I thanks P. Handel and C. Van Vliet for their useful comments.References
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Michel PLANAT
Laboratoire de Physique
et M6trologie des Oscillateurs du CNRS 32, Avenue de 1’Observa,toire
25044 Besanqon Cedex France