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Theory of Lattice and Electronic Fluctuations in Weakly Localized Spin-Peierls Systems

C. Bourbonnais, B. Dumoulin

To cite this version:

C. Bourbonnais, B. Dumoulin. Theory of Lattice and Electronic Fluctuations in Weakly Local- ized Spin-Peierls Systems. Journal de Physique I, EDP Sciences, 1996, 6 (12), pp.1727-1744.

�10.1051/jp1:1996185�. �jpa-00247278�

(2)

Theory of Lattice and Electronic Fluctuations in Weakly

Localized Spin.Peierls Systems

C.

Bourbonnais (*)

and B. Dumoulin

Centre de Recherche

en

Physique

du Solide et

Département

de

Physique,

Université de

Sherbrooke, Sherbrooke, Québec,

Canada JIK 2Rl

(Received

18

July

1996, received in final form 26

August

1996,

accepted

29

August 1996)

PACS.71.20.Rv

Polymers

and organic compounds

PACS.64.60.Ak

Renormalization-group, fractal,

and

percolation

studies of

phase

transitions PACS.75.40.-s

Critical-point

effects, specific heats,

short-range

order

Abstract. A theoretical

approach

to the influence of one-dimensional lattice fluctuations

on electronic

properties

in

weakly

locahzed

spin-Peierls

systems is

proposed

using the renormal- ization group and the functional

integral techniques.

The

interplay

between the renormalization group flow of correlated electrons and one-dimensional lattice fluctuations is taken into account

by

the

ope-dimensional

functional

integral

method in the adiabatic limit. Calculations of spin- Peierls precursor effects on response functions are carried eut

explicitly

and the

prediction

for the temperature

dependent magnetic susceptibility

and nuclear relaxation is compared with

available

experimental

data for

(TMTTF)2PF6.

1. Introduction

Among

the

possible

structural

phase

transitions in low-dimensional

systems,

trie

spin-Peierls (SP) instability

bas

recently

received

particular

attention

[1, 2j.

In contrast with trie Peierls

transition,

whose normal

phase

is

metallic, pronounced insulating properties

and

antiferromag-

netic

spin

correlations are found far ahead of trie SP

ordering temperature. However, owing

to trie

quasi-one-dimensional

character of these systems, precursor eifects should appear m both

types

of transitions. Since

spin

correlations are

essentially

one-dimensional m

character,

lattice fluctuations should emerge as diffuse

scattering

in

X-ray experiments,

and as a so-called

pseudo-gap

eifect in

magnetic properties.

The

pseudo-gap

eflect is well known to be the hall- mark of

strongly amsotropic

Peierls

systems [1,3j,

but

surprisingly,

its observation is a rather

uncommon feature of most SP

systems

and trie

underlying explanation

for this is not known

so far

[2j. Correspondingly,

the mcitement to achieve a theoretical

description

of fluctuation eifects

m the SP case did not receive any

experimental justification,

so that most theoretical

efforts were rather devoted to the

description

of the ordered state

[2,4, 5j. However,

recent observations of SP fluctuation eifects in the orgamc

systems (TMTTF)2X

and

(BCPTTF)2X

with X

=

PF6, AsF6,

has

prompted

a renewed interest for this

problem [6-10j.

In both cases, one-dimensional SP precursors are

clearly

seen m structural and

magnetic

measurements well above the true SP

ordering

temperature.

(*)Author

for

correspondence le-mail: cbourbonslphysique.usherb.ca)

©

Les

Éditions

de

Physique

1996

(3)

This paper will be

entirely

devoted to the theoretical

description

of one-dimensional lattice and electromc correlations in SP

systems

of trie

(TMTTF)2X

series. Unhke

(BCPTTF)2X,

which are

already good

insulators at room

temperature, (TMTTF)2X

are

weakly

localized and still show a metallic behaviour in this

temperature

range. It is

only

around

Tp

=t 220 K that carriers

undergo

a Mott-Hubbard

locahzation,

below which trie

resistivity

becomes

thermally

activated

Ill].

Albeit trie

magnetic susceptibility

remains unaifected at

Tp,

NMR

spin-lattice

relaxation rate measurements bave revealed trie existence of

strong

1D

antiferromagnetic spin

correlations below this temperature range

[î,12].

Below 60

K,

one-dimensional SP lattice soft-

ening

is borne out

by X-rays

and bas a marked influence on trie

temperature dependence

of both

susceptibility

and nuclear relaxation

[6, 7].

In order to tackle the

problem

of one-dimensional electromc and lattice fluctuations eifects in SP

systems

we shall combine the renormalization group

technique

for fermions and the

functional-integral

method

[9,10].

A similar

approach

has been

recently applied

with some success to

strongly

localized SP

systems

of the

(BCPTTF)2X

serres

[10].

Since the

itineracy

of carriers is much more

pronounced

in the

high

temperature

domam of

(TMTTF)2X series,

both spm and

charge degrees

of freedom must be considered in the renormalization

flow,

which in

practice

makes the extension of the

previous approach slightly

more

complicated.

2. The Model and the Partition Function

In

setting

up the essential

ingredients

of the

model,

it is first convenient to

study

the

parti-

tion function of the

electron-acoustic-phonon

interaction

model, namely

when direct electron-

electron interaction is absent. The

corresponding

Hamiltonian is well known to take the form

[13]:

H =

£ ep(k)c)

~ ~c~ k a +

£uJ(Q)(b[bQ

+

p,k,a ' ' Q

~

+lL)~~~~ ~j 9(k> Q)C),k+Q,aC-P.k,a(b~

Q + bQ)>

Il)

jp,k,Q,ai

where

e~(k)

=

vF(pk kF)

is the linearized spectrum around the 1D Fermi

points pkf

"

+kF

for free fermions and

uJ(Q)

" UJDÎ

sin(Qa/2)1

is the

dispersion

relation for the

phonons là

=

1).

Here VF is the Fermi

velocity

and UJD is the

Debye frequency,

which coincides with the

phonon

energy at

Q

"

+2kF("

+7r

la,

when the band is

half-filled).

As for the

interacting

part, the

electron-phonon coupling

constant is

given by:

9~~'Q~

" ~~

àfi ~~~~Q~/~~ ~°~~~~

+

Q~/~~'

~~~

where II is the molecular mass and ga =

-dta /dz

> o is the

spatial

modulation of the

longitu-

dinal

hoppmg integral

ta. The

dynamics

of

phonons being purely harmonic,

their

integration

m the

partition

function Z

= Tr

e~P~

can be carried out

exactly, yielding

an effective re- tarded interaction among electrons

(fl

=

1/T, kB

"

1).

The result can be put in the

following

functional-integral

form

~ ~

P

Z =

[d~~][dfl e~e'~

'~l

exp(- dTidT2 ~(Ti T2)), (3)

over the

anticommuting

Grassman variables

#(*1

The free electromc action is

given by

S)[i~,*, ~]

=

/~

dT

~j ~j ~(k, T)[G((k, T)]~~~~,~(k, T), (4)

o ~

'

(4)

where

G((k,T)

=

[-à/ôT ep(k)]~~

is the free electron

propagator.

As for trie retarded interaction

~(Ti T2),

we will

proceed

to a

"g-ology" decomposition

which

only

retains

2kF phonon exchange

between electrons at

+kF,

with the result

~(Tl

T2)

"

(~~)

~

~ 91,ph(T~

T2)

~~,ai

(~~ +

P~~F

+ ~,

T~)~~p,a2 (~2 P~kF

~>T2) (P,k,q,a)

X

~p,~~(k2,T2)~-p,ai(k~,T~)

+

(~~)

~

~ 93,ph(T~

T2)

~Îp,ai

(~~ +

P~~F

~ P~i>

T~)~Îp,a2 (~2 P~kF

+ ~>T2)

ip,k,q,aj

~ ~P,0E2(k2>

T2)~p,ai(k~,T~), là)

where G

=

4kF

is a

reciprocal

lattice vector. The retarded

backscattering

and

umklapp

cou-

pling

constants are

given by

gi,ph(Ti

T2) "

g(-PkF, p2kF)g(pkf, -P2kF)D° (2kF,

Ti T2)

#

~~~ D~ (2kF,

T~ T2

), MàJD

93,ph(T~

T2) "

~~Î9~,ph(T~

T2)>

where

D°(2kF,T~

T2)

=

-[e~~D'~i~~2'

+

2(eP"D -1)~~cosh(U~D(T~ T2))j

is the

phonon propagator

at

2kF. Here,

~/ < 1 is a

positive

constant that reflects the half-filled character of trie band. For a

single

half-filled

band,

~/

= 1 while for

systems

hke

(TMTTF)2X

with a

quarter-filled

band and a small dimerization gap, one can take ~/ < 1

[14j.

From

above,

one

observes that for

exchange

of

2kF

acoustic

phonons,

g3,ph and g~,ph are

opposite

m sign. Trie retarded interaction can then be written

umquely

m terms of

composite

fields:

~(Tl

T2)

"

/

dz

~j g$(Tl T2)°~*(X, T~)°~(Z,

T2), (6)

~

where we have introduced the

composite

field

°~* (~, T)

#

(°*(Z, T)

+

àΰ(T, T)),

2 with

°(~'~)

"

~j ~5,a(~> T)~+,OE(~, Tl'

a

These

corresponds

to "site"

(M

=

+)

and "bond"

(M

=

-) charge-density-wave (CDW)

correlations at

half-filling.

The related combinations of

couphngs

are given

by g$(T~

T2) "

9~,ph(T~

T2) +

~Îg3,ph(T~ T2).

In order to

analyze

these

correlations,

we

apply

an Hubbard-Stratonovich transformation on the retarded

part

of the interaction

z "

/ld~~lldùlld4~l~~~i~~'~'

x

exp(- dzdT~dT2 ~ 4~(z,

T~)

gf(T~

T2) Î~~

4~(z,T2))

M=+

x

exp(-

d~dT

~j ÀMO~(z,T)çi~(z,T)), (7)

M=+

(5)

where

çi*

are real

auxiliary

fields for site and bond fluctuations

respectively,

and

À+

=

2,

À-

=

21. It is worth

noting that,

in the absence of

umklapp scattering, gj~

=

g)~

and there is no

diiference between bond and site

density

wave fluctuations so that bath

auxiliary

fields will combine to

produce amplitude

and

phase

fluctuations of the

complex

field çi

=

çi+

+

içi~

=

(çi(e~~, as found in incommensurate Peierls

systems.

Unretarded

repulsive

electron-electron interaction at

half-filling

will

promote

bond with re-

spect

to site electronic correlations. These essential

ingredients

of trie SP

instability

can be added to trie model

by following

trie

"g-ology" prescription [15j,

in which trie direct interaction among

right-

and

left-moving

carriers is

decomposed

in terms of backward

(g~),

forward

(g2)

and

(g3) umklapp scattering coupling

constants. Trie full

partition

function of trie model in trie Fourier-Matsubara space then becomes

Zlh~l

"

"

/ld~*1ldill ld4~l

exP

SI fil*, ill

+

S°14~l

+

Si W*, ~, 4'~I

+

Si fil*, 4

+

ShW*, ~, h'~I

+

/ldt~*lldt~lld4~l

exp

~ IGÎ(1)l~~ #],a(1)~/,p,a(1) ~14~(4)l~lg$(uJm)l~~

p,1,a 4

+

/~jÀMO'~(4)4'~14)

4

+

~ ~

g~t~],~~ li~

+

Q)t~lp,~~ll~ Q)t~-p,ai ll~)t~p,a~lÎ2)

lP,1,Q,al

+~ ~ ~j

92il],ai lÎ~

+

4)ilLp,a~ lÎ2 4)ilp,ai (Î~)il-p,a~(12)

jp,à,<,aj

+

) ~

g3t~],~~ lt~

+

Qp)t~],~~ ll~ Qp

+

p©)~-~,~~ (l~ )~-~,~~ (i~)

lP,1,Q,al

+

~j (°f(Q)hf*14)

+

H-C) ), 18)

4,v

where k

=

(k,uJn

=

(2n +1)7rT)), Qp

=

(pQ,

mm

=

27rmT),

G

=

(4kF,o), G((k)

= [iuJn

ep(k)]~~,

and

gf(uJm)

=

8g((MUJD)~~(1- M~/)D°(2kF, mm).

Trie

integration

measures are

[d~l*][d~l]

=

fl

j

~

d~l(,~(k)d~lp,~(k)

and

[dçi'~]

=

fl~ Q~~ gf(uJm) (~~dçi'~(Q)dçi'~(-Q)

for fermion and

alxiliary fields, respectively.

Here '

D°(2kF, mm)

=

~

)~~

,

(9)

uJ~ uJ~

corresponds

to trie bare

phonon propagator. Finally, Sh

is an additional term which

couples

an infinitesimal source field

hf

to site bond

(M

=

+,

~t =

o)

CDW and site

(AI

= +,

~t =

1, 2,3)

SDW correlations. These

correspond

to composite fields defined

by Of*(i~)

=

Î~~Î(Q)

+

ÀΰH(Q)),

Wl~ll

°~=0,~,2,3(Q)

"

(~/~)~~~ ~Î(,~,pl~~,a(~

~

Q)~~~l~-,fl(~),

~l,2,3

and ao

being

the Pauli and the

identity

matrices

respectively.

In the

following

the source-field term will be useful for the calculation of relevant response functions for the SP

instability.

(6)

3. Renormalization

Group

Results

The

problem

of

low-energy

electronic and lattice correlations reduces to the

study

of

interacting

electrons

coupled

to the

fluctuating

field

çi'~,

which can be done

by

first

applying

the renor- malization group

approach developed

in references

[10,16]

for the fermion

degrees

of freedom.

It consists of first

integrating high-energy

fermion states,

namely

we write

~l(*)

-

~l(*) +1(*~,

where

~l(*)

describes

degrees

of freedom to be

integrated

over in the outer energy shell of thick-

ness

Eo(f)df

on both sides of the Fermi level at

+kF

and for all mn. Here

Eo(f)

=

Eoe~~

is 2

the band energy cut-off at the

step

f and

Eo

+

2EF

is the initial band

width,

which is twice the Fermi energy.

Keeping

trie

çi'~'s fixed,

this is

formally

written as

Z[h'~]

c~

/ [d~l*][d~lj[dçi~j e~'~*'~"" ~"lt~P~'~"t / [dj~j Idi] e~Î'~*~l

(e~~+~I+~h

~ ~_~

"

/ ldi~~lldi~lld4~l ~~'~~'~'~~"~~'i'~~~'~~"'~~P (~j j(IÉÀ

+

ÉI

+

Éh)~)o.s)

<

~

Î jd~j*jjd~/,jjdjmj ~s[~*,~,#~,h~]e+dt-8~Î4"lt+di~ jio)

which leads to a recursion relation for electromc parameters of trie action

mcluding

those related

to source fields for the calculation of response functions

(see below>

and for

7[çi~]1,

which is

a

free-energy

functional which collects all the contributions in the

auxiliary

field

çi'~.

At finite temperature, the

partial integration

is conducted down to

éT

=

In(EF/T).

In the

present

renormahzation group

procedure,

electronic

degrees

of freedom are treated in the continuum limit so that the discreteness of the

underlymg

lattice will be

neglected

in the

following [10].

3.1. ELECTRONIC PART

3.1.1.

Couplings

and One-Particle

Self-Energy.

It is useful for the

following

discussion to recall the well-known

two-loop

RG results for the

purely

electronic

part (çi'~

=

o)

in zero field

(h"

=

o).

The eifect of the lattice fluctuations and the calculation of relevant response func- tions will be considered afterwards. In this

purely

electronic

limit,

the

smgle-particle

fermion

propagator

transforms

according

to trie recursion relation z~

(é+dé)[G(]

~~ = z~

(é)z~ (dé) [G(]

~~

At trie

two-loop

level trie outer-shell correction to z~

(dé)

comes from trie n

= 2

(S/)~_~

terms of

(10),

which

yields

trie flow

equation:

~

()~

=

-jl12i~(é) i~(é)l~ fil(f)

+

31iil

+

3iilll, iii)

where trie

j~ (é)

e

g~(é) (7ruF )~~

are trie normalized

couplmg

constants at f. Trie latter transform

as

J(é

+

dé)

=

j~(é)zp~(dé)z2,3,4(dé), which, together

with zi, are obtained from

one-loop

(É/)~

~

and

two-loop (É/)~_~

outer shell corrections to

two-partiale four-point

vertex functions

r~,2,3(é

+

df)

=

z2,3,4(dé)r~,2,3(é).

This is known to

yield

the flow

equations [15-17]

d9~

~2

1~3

$

~~

2~~'

~~~~(j

~~~ = ii~11

~121~ J~ )i,

()

=

i~(21~ i~)11 121~

ii

)i

(ii, i12)

(7)

For

(TMTTF)2X compounds, j~

=t

j2

> o are

repulsive

at é

=

o,

whereas a finite dimerization of the TMTTF stacks can be

parametrized by

a small and

positive j3

<

j~ [9,14].

One then

gets

the

inequality j~ 2j2

<

j3 indicating

that

umklapp scattering

is relevant. The flow of

charge couplings 2j2 -à~

and

j3

then scales towards

strong coupling

while the

spin coupling j~

is found to be

margmally

irrelevant with the fixed

point

values

fi (é

-

cc)

-

2, fi (é

-

cc)

-

1,

and

fi

- o. The

strong coupling

sector of the RG flow is reached when

g3(é

e

ép)

m

1,

where ép =

In(EF/Tp)

defines the

temperature

scale for the presence of a

charge (Mott-Hubbard)

gap

~lp

e

2Tp. Neglecting

transients between weak and

strong coupling regimes, one-partiale self-energy

corrections

resulting

from the solution of

equation (11)

can be

put

in the

followmg scaling

form

zi~(é)

m

zi~(ép) (Eo(é)/Ap)°Î, (13)

which

depicts

the reduction of the

quasi-partiale weight

at the Fermi level with

9*(g(, g], g()

=

3/4 being

evaluated at trie fixed

point.

3.1.2.

Response

Fbnctions. Trie

pertinent

electronic response functions involved in trie de-

scription

of the SP

instability

m one dimension are those related to site SDW (~t

# o,

II =

+)

and bond CDW (~t =

o,M

=

-)

correlations [9].

They

can be

readily

calculated via the renormalization of the source field term

Sh

116]

which,

at scale

é,

reads

shl#~ #. h~li

"

~j (~f(é)hf~(4)°f (4)

+ H'~'

xfl~kf> é)hf~(4)hf14)), l14)

lv,M,ôl

where

zf lé)

is the renormalization factor for the

pair

vertex part, while

xÎ(2kF,é)

=

-(7ruF)~~ Î~ Ù$(é')dé', (15)

is the

2kF

response function and

ii

"

(zf)~

is the

auxiliary susceptibility

m the

(~t,M)

channel considered. The one- and

two-loop

corrections to

zf

come from the outer shell averages

(ÉhÉI)o.s

and

(ÉhÉ/)~_s

for n = 2 and n = 3

respectively.

This leads to the flow

equation

~

~()"

=

if(é) (àÎ(é)

+

iiÎ(é) à~(é)12(é)

+

)iiÎ(é)1, (16)

where

j* lé)

=

j2(é)

~

j3 If) 2j~ lé)

for the CDW channel and

j+~~(é)

=

j2(é)

+

j3(é)

for the SDW channel.

Followmg

the

example

of

(13)

for the

one-particl$self-energy renormalization,

if

can be

expressed

in the

followmg scaling

form

xi jt)

~s

ii (t~) jEo(t) /à~) ~~i'~, (17)

where

if (ép)

is the weak

couphng

contribution below the

charge

gap. The exponents

~[(

~ =

~*~

=

3/2

obtained

by evaluating

the r-h-s of

(16)

at the fixed

point

indicate that

onli'site

SDW and bond CDW correlations are

singular

at

half-filling.

It should be

mentioned, however,

the

g]

obtained at

two-loop

level are well known to overestimate the values of the

exponents.

Higher

order contributions are

expected

to

bring

them doser to the exact value

~~Î,3

"

~*~

+

~* "1, (18)

which is known to result from more elaborate calculations at é » ép

[18j.

(8)

Before

closing

this section, it is useful for

applications (see

Sects. 3.2.5 and

4.2)

to compute the

imaginary part

of the retarded response function at low

(real) frequency.

From reference

[16],

it is

directly

connected to

if

as follows:

Im

,yf(2kF

+ q,uJ) =

if (T)

Im

y°(q

+

2kF, uJ),

uJ - o

(19)

for ufq < T, where

Im

x° (q

+

2kF,

uJ)

=

~~Im ~j Gf (k, uJn)G( (k

+

2kF

+

q, mn + uJ +

io+)

~ k,w~

=

uJ -

o, (20)

Tufcosh (flufq/4)

is the

imagmary part

of the

low-frequency non-interacting

response function near

2kF (see Appendix A.2).

3.2. INFLUENCE OF LATTICE FLUCTUATIONS

3.2.1.

Ginzburg-Landau

Functional. When the lattice

auxiliary

field

çi'~

is taken into ac- count, the

partial integration (8) generates

a series of terms m n > 2 powers of the

çi'~'s

ma the closed fermion

loops (É[) In!.

This will not

only

lead to corrections for

S° [çi'~]1

for n =

2,

but it

yields

a recursion relation for the

quantum Ginzburg-Landau free-energy

functional

7[çi'~]1,

when combined to the n > 2 terms

[10,16j.

Since

only 2kF

bond correlations are

smgular

in the CDW channel for

repulsive couplings, only

the

dependence

on the bond field

çi~

needs to be

retained,

with the result

flJ~i<~ii+di

=

flJ~i<~ii ~ ~ Bnidé) <-141) <-14n)ôz ~~a. 121)

n22

o

The

quadratic (n

=

2)

and

quartic (n

=

4)

outer shell contributions lead to

82(dé)

=

(7ruF)~~[z~(é)]~ dé,

~~

~~~~

Î~ÎÎÎEOÎÎÎ]~

~~'

~~~~

where

((3)

ci 1.2... For the

problem

at

hand,

one can assume that

adiabaticity

between electrons and the lattice is

sufliciently strong

that

quantum

lattice corrections can be

neglected, thereby allowing

the static limit.

Up

to the

quartic

term, one obtains the

followmg Ginzburg-

Landau free energy functional

lin

real

space)

71<~ii~

=

/

dz

aiT)(<~ ix))

~ + c

()

+

b14~ ix))

~

l, (23)

~

at

temperature T,

where

a(T),

c and b are trie

Ginzburg-Landau parameters.

Trie coefficients

a(T)

and c of the

quadratic

term are

respectively given by

~(~)

"

Î9ph(°)1 ~+X (~~F>l~)

m

a'(T/T)p-1)

c m

~a'(uF/7rT)p)~, (24)

2

(9)

where a'

=

(7ruF)~~i~(T)p).

Here the bond CDW response function

X~(2kF,T)

in equa- tion

(15), together

with

(17),

bave been used in trie linearization of

a(T)

around trie SP

mean-field

temperature

T)p

m

Tp((jj~((~(Tp))~~~~ (25)

for

Tp

»

T)p.

It is worth

noting

that smce

(jj~(

e

(7ruF)~~Î9jhÎ

c~

g(,

then

T)p

c~

g(

for

~*

=

1,

which turns out to be trie same power

dependence

on trie

electron-phonon coupling

constant that was found in previous mean-field calculations on more localized

systems

[4]. As

for trie

rigidity parameter

c, it is

readily

obtained in Fourier space from trie

Q

"

2kF

+ q

expansion of

x~(Q, T)p) using

trie

approximate expression

é(T(p, 2kF

+

q)

= In

~

[1 +

(ufq/7rT(p)~]~i

TSP

,

as

boundary

condition of trie

logarithmic integration

m

(15)

near

T)p.

This form

essentially

comcides with trie

Q dependence

of trie

elementary

Peierls bubble near

2kF. Finally,

trie flow of trie mode-mode

coupling

m

(22)

is

stopped

at

éTo

and reads

"

~~~~~

~

16(1

Î~ÎÎ7rT)p)2

~~

~~~~~~~'

~~~~

for

Tp

»

T)p.

Fluctuation eifects in

çi~

below

T)p

are then

governed by

trie classical functional

integral

Z =

J [dçi~j exp(-fl7[ô~j ),

which can be carried out

exactly using

trie transfer matrix method

[19].

An

important quantity

to compute is trie static 1D SP response function ~sP. From trie

results of reference

[19],

one finds

xsp(2kF

+ q,

T)

=

j /

d~

((4~ (z)4~10)))

e~~~~+~~~~~

2fl (( (4~)~ )) (SP

l +

q~fip

' ~~~~

where

(( (. ))

=

z-~ /id<-i (. exp(-flJ~i<-1),

denotes a statistical average over

ô~

Here

(sP

is trie correlation

length

of trie real order field

çi~,

which grows

exponentially

below

T)p according

to

(sP

"

~ ~

eP/~, (28)

p (a(

where

~~

~ =

(29)

~~~~~~~~~~~

~

~'~~~P'

for T <

T)p.

The

temperature profile

of both

(sP

and the mean square fluctuations

(((çi~ )~))

are

plotted

in

Figure

1.

(10)

3.5 1.6

z

n __

n

«

~w °'~

?~Î

v -

"

0.4

O.o

0.4 O.fi

T/T~~

o

Fig.

l.

Temperature

variation of the mean square of the SP order parameter

(left scale)

and the

inverse of the correlation

length (right scale)

normalized

by

the lattice constant.

~+

~

~fi

Fig.

2.

Leading one-partiale self-energy

correction due to SP fluctuations for electrons at +kF. The

wiggly (dashed)

fine

corresponds

to the lattice field

(electronic -kF)

propagator xsP.

3.2.2.

Pseudo-Gap

Eisect. The influence of the static SP lattice fluctuations

governed by (23)

on

one-partiale

electronic

properties

at the

step éT

of the RG

procedure

will be

analyzed by considering

to

leading

order the one-electron

self-energy

contribution of

Figure

2 [3], which

can be obtained from

(8)

after an

integration

over the

çi~

field. The result is

Lj(k,(çi~))

=

-TL~~zp~zp ~j ~(k p2kF q,iuJn)xsP(2kF

+ q,

T). (30)

q

The bare

propagator

appearing in

S)

then becomes

iGpii,14~i)i~~

=

z~iGjii)i~~ Li(1,14~i)

~

~~

~ ~~~~

zi~(zi)~ ((14~i~))

" ~ ~~~~

iu~~ + ep

(k)

+

ivf(il (T)

A relevant

quantity

to

compute

is the reduction of the

density

of states per

spin resulting

from SP fluctuations

(pseudo-gap eifect).

After

analytic

continuation of

[Gp]~~

to real

frequencies,

this is found to be

~~~'~~

~~

iÎ~(~~~~~~'~'~~

~~

p,

~

i

a121d

+

4~/~

~~~~

7ruF

12(d

+

~) a2]d'

where trie presence of trie renormalization

factpr

z~ ensures that the

pseudo-gap

eifect is the result of lattice fluctuations.

Followmg

trie notation of reference

[3j,

we bave

~ ~

~-l((jfl~-j2)j-1/2

F SP

(11)

b)

, /

Fig.

3. Dressed electron-hole bubbles in the

a)

Landau and

b)

Peierls

(or Cooper)

channels. Thick and thin continuous

(dashed)

fines

correspond

to dressed and bore electron propagators,

respectively

at +kF

(-kF).

Fig.

4.

Two-trop a) one-partiale self-energy

and

b)

four points vertex

singular diagrams

involved

in the RG flow

including

the

leading

order corrections due to lattice fluctuations.

j

~((jfl~-j2))-~/2

~ = 1+

~o~-&i~

4

d =

(K~+i~a~)~/~, (33)

where we bave defined

(4l~

(~ =

zp~(z~)~

(çi~

(~

Therefore,

as trie

temperature

decreases below trie characteristic

T)p,

lattice fluctuations grow and will

progressively

freeze electromc

degrees

of freedom. In

tutu,

this reduction will affect trie RG flow of various

quantities

considered in Section 3. The inclusion of lattice fluctuation eifects m trie RG flow will be considered to

lowest order where vertex corrections due to

exchange

of lattice fluctuations are

neglected.

For

example,

at

one-loop

level of trie

RG,

this amounts to

substituting G(k, (çi~))

for one of trie

propagators

appearing in trie formal

expression

of trie

Landau, Peierls,

and

Cooper elementary susceptibilities (Fig.

3 and

Appendix A).

At trie

two-loop level,

all trie relevant

next-to-leading singular diagrams

shown m

Figure

4 involve

absorption

and emission of an electron-hole pair at small

fin

trie intermediate state, which can be dressed

by

lattice fluctuations

(Appendix B).

From the results of

Appendices

A and B, this amounts to

replacing

the outer shell

logarithmic

contribution of all

diagrams by

the

followmg expression

- 7ruF

D[Eo(é)/2, (çi~)jdé, (34)

where

D[Eo(f) /2, (çi~)j

is

density

of states

(32)

m the presence of a

pseudo-gap.

Substituting

this RG generator m the flow

equation

for the renormahzation factor

zp~

in

(11)

will slow down the electronic contribution to the

decay

of the

quasi-partiale weight

below

T)p.

(12)

Following

the

example

of the

purely

electronic case, the

approximate "scaling" (transient-free)

form

(13)

then becomes

~i~lT)

"

~i~ITÎP)(T/TÎP)~~~~i> 135)

where

zp~(T)p)

is

given by (11)

and

9j(T)

=

7ruFD[T,(çi~ )]9j

becomes a

temperature depen-

dent

exponent

below

T)p.

3.2.3.

Staggered Response

Fbnctions. The

pseudo-gap

will affect electronic correlations of the (~t,

AI)

channel as well.

Indeed, substituting (34)

in

(16) yields

the

following approximate

"scaling"

form

1$(T,i<-i)

m

t$(Tip)(T/Tipl~~*~°~~, (36)

where

if (T)p)

is

given by (1î)

and

~*(T)

=

7ruFD[T, (çi~)]~*.

As for the

imagmary part (19),

the above results and

Appendix

A.2 lead to Im

xi iq

+

2k~,

u~,

jçi-j)

=

-iijT, jçi-j)Im xiq

+

2kF, W,14~i)

~

~~fi~'i~~i~ ÎÎÎÎUÎÎ/Î/ÎÎ

~' ~ ~ ° ~~~~

which is further reduced

by

lattice fluctuations.

3.2.4.

Magnetic Susceptibility.

The calculation of the

spin

response function ys at small

(q,

uJ) is known in the

purely

electronic situation

[21j.

Its

generalization

when lattice fluctua- tions are

present

is

straightforward

and

yields

xs

(q,

W,

14~1)

=

(~~~~'~' i~ i~

,

138)

1

jgi(T)x(q, W,14~i)

where in the above scheme of

approximation ~(q,uJ, (çi~))

is the

elementary

electron-hole bubble dressed

by

lattice fluctuations

(Fig.

3a and

Appendix A.1),

and g~

(T)

is given

by (12)

at

éT. According

to the results of

Appendix A,

one finds

~~

~~~'~' ~~

~~

Î~ ~~~" ~~

~~

ÎÎ'~ ~~' pÎÎ~

uJ'

p

IIU

Xl~,

~>

14~1)

"

/ ~ ~l~" 14~ Il (~ )) d~' ~j P~~F~ô(PUF~ ~) (39)

p

for the real and

imaginary

parts of the dressed electron-hole bubble. It follows that in the static

lu

-

o)

and uniform

(q

-

o) hmit,

the

temperature

variation of the

spin susceptibil- ity ~s(T, (çi~))

will be

depressed

in the presence of lattice fluctuations that grow up below

T)p (Fig. 5a).

In the very

low-temperature domam,

the SP correlation

length

becomes ex-

ponentially large

and the

magnetic susceptibility

becomes

thermally

activated. When these

temperature

conditions

prevail,

the

system

is almost

long-range

ordered.

3.2.5. Nuclear Relaxation Rate. From the above

results,

the

temperature dependence

of the nuclear

spin-lattice

relaxation rate

Tp~

can be

readily

calculated. The basic expression for

Tp~

in one dimension is well known to be

Tp~

=

(-Î(~T /dQ~~ ~~~'~~, (40)

uJ

(13)

4.0 a)

3.0 j

) ~°

Z-o

~

l-o

o-o

Î

b) 40

j

î zo

~~

0

O.o 0.5 1-o 1.5 Z-o 2.5 3.0

T/T~~

o

Fig.

5. Calculated low temperature variation of

a)

the uniform

magnetic susceptibility

and

b)

nu-

clear relaxation rate in the presence

(continuous fine)

and absence

(dashed fine)

of lattice fluctuations.

which can be taken in the limit uJ - o. Here Im x is the imagmary part of the retarded spm response function and

À

is

a constant

proportional

to the

hyperfine couphng [20j.

It is well

established that uniform

(Q

+~

o)

and AF

(Q

'~

2kF)

spm fluctuations grue the essential con- tributions to the relaxation in one dimension

[21], allowing

in tutu to make the

decomposition

t~

"

t~lo

'~ ol +

Ti~lo

'~

~kfj. (41)

For the

staggered

part

Tp~ [Q

'~

2kFÎ,

we have seen from

(37)

that Im

x(2kF

+q, uJ) whose defi- nition coincides with -Im

x$~o(2kF

+q,

uJ))

is

peaked

when q lies in the interval

[-T/uF, T/UFÎ,

which leads to

Tp~[Q

'~

2kFÎ

Cf

CITD[T, (çi~)]$((T, (çi~)), (42)

where C~ =

7rvj~(À(~tanh(1/4).

As for the uniform

contribution,

the use of

(38-39) immediately

leads to

~ ~

DjT, ii-11

,

TP lQ

'~

°'

"

~° (43)

ji jg~ (T)DjT, ii- iii

~

where

Go

"

47r(uF)~~ ÎÀ(~.

As

expected,

the reduction of spm fluctuations

by

short range lattice correlations below

T(p

will decrease the

amplitude

of the relaxation via the reduction of the

density

of states. At

sufliciently

low

temperature, namely

when the correlation

length (SP

becomes

exponentially large,

one finds

Ti~

'~ xs '~

e~P/~.

In the

high-temperature

regime, lattice fluctuations are small and the uniform component

Tp~

r-

COTXÎ eventually

dommates the relaxation.

Using

the

scaling

form

(36)

m

(42)

and

(43),

the

temperature dependence

of

Tp~

is summarized in

Figure

5b where it is

compared

to the case without fluctuations.

(14)

(TMTTFJ~PF~ iP i Bar)

_ o

~ ~sP

~

Q «

CD

j/

Tsp +

~t+#

+++

'

~

/

~~

+

O.O

0 20 40 60 80

TeniperaLure (K)

Fig.

6.

Comparison

between calculated

(continuous fine)

and observed

(crosses)

temperature pro- files of

magnetic susceptibility

for

(TMTTF)2PF6.

The data are taken from reference [7].

4.

Application

to the SP

System (TMTTF)2PF6

By

way of

application

of the

present theory

to the

sulphur

based

organic compound (TMTTF)2 PF6.

Previous

analysis

of this

system

in the normal

phase using

the one-dimensional electron gas mortel can be used for the determmation of the

input

bare

parameters

of the

purely

elec-

tronic

part

of the model. NMR

analysis

of Wzietek et ai.

[12]

have shown that

j~

ct

j2

Cf

0.9,

with

EF

Cf 1600

K, give

a rather

good description

of the

temperature dependent magnetic susceptibility

in the

high temperature

domain of this material. As for the observed character- istic

temperature

scale

Tp

re 220 K

(below

which the

system presents insulating properties),

it can be used to

identify, together

with

(12),

trie

low-temperature

domam of

strong umklapp scattering,

which then allows one to take

f3

~S o.2 [9]. As for trie

input parameters

for trie lattice

component,

one will fix trie value of

T)p

at 60 Il which is trie characteristic

temperature

scale for trie onset of

strong

lattice fluctuations in

X-ray experiments [6j.

From trie above set of

figures

ail

quantities

of interest can be calculated.

4.1. MAGNETIC SUSCEPTIBILITY. Trie

temperature-dependent

EPR

spin susceptibility

(TMTTF)2PF6

measured

by

Creuzet et ai.

I?i

is

reported

in trie

low-temperature

domam in

Figure

6.

xs(T)

decreases

monotonously

from trie

high temperature

domain and becomes

weakly temperature dependent

near 80

K, y7hich

is

typical

of all members of trie

sulphur

serres

m the normal state.

However,

m the low

temperature

domain below 60

K,

trie spm

suscepti- bility

decreases

by roughly

40$io down to the true SP transition at

TSF

~S 19

K,

below which it

becomes

thermally

activated.

Using

the above set of

parameters

for the

model,

the theoretical

prediction

for

ys(T. (çi~ ))

is illustrated in

Figure

6 and

gives

a

fairly good description

of the

temperature

variation of xs m the SP

pseudo-gap regime.

At very low

temperature,

the

present theory predicts

a

thermally

activated behaviour when

(sP

grows

exponentially,

which is found to mimic the actual

temperature dependence

below the true transition

temperature

at 19 K.

However,

a more realistic

description

of the SP system m this low temperature

region,

would require the inclusion of the interchain

coupling.

(15)

60

/

l'i&iTTF) PF

Ù 40

~

~

~

aj

~u sp

0 40

Temperature (K)

Fig.

7.

Comparison

between calculated

(continuous fine)

and observed

(crosses)

temperature pro- files of nuclear relaxation rate for

(TMTTF)2PF6.

The data

are taken from reference [7].

4.$.

NUCLEAR RELAXATION. The

temperature profile

of

Tp~

for

(TMTTF)2PF6,

measured

by

Creuzet et ai.

I?i,

is

given

in

Figure

7. From the

analysis

of nuclear relaxation in the

high temperature

domam

T)p

< T <

Tp,

where SP fluctuations are

weak,

the contribution to

Tp~

is well known to be

purely

electronic in character. A

quantitative description

of the relaxation rate in this

regime

can be obtained from

(42)

and

(43) neglecting

the

dependence

on

çi~ [12].

Below

T)p,

the relaxation rate shows a 30$io decrease between

T)p

and

TSF

due to one-dimensional lattice fluctuations.

According

to

(42)

and

(43)

both trie

staggered

and uniform parts of trie relaxation are aflected below

T)p.

Thus, usmg these

expressions

for trie above set of parameters, one obtains trie

Tp~ temperature profile

shown in

Figure

7. Trie theoretical curve is obtained from trie

expressions (43), (42)

and

(36)

in which trie values of trie

constants

Co(7ruF)~~

Cf 12.1 and

C~(7ruF)~~Tp(((Tp)

ci 9.6 results from trie

analysis

of

Tp~

data made

by

Wzietek et ai.

[12],

in trie

high temperature

domam T »

T)p.

Therefore trie above low temperature results for the nuclear relaxation rate

complete

the

previous analysis

made in reference

[12].

Acknowledgments

The authors thank J.-P.

Pouget

and L. G. Caron for numerous discussions. We would also like to thank D. Sénéchal for useful comments about the manuscript. Financial support from the Natural Sciences and

Engineering

Research Council of Canada

(NSERC),

le Fonds pour la

Formation de Chercheurs et l'Aide à la Recherche du Gouvernement du

Québec (FCAR)

and Canadian Institute for Advanced Research

(DAR)

is

gratefully acknowledged.

Appendix

A

Elementary Susceptibilities

in Presence of Phonons

In this

appendix,

we

proceed

to the calculation of the

elementary

electron-hole bubbles dressed

by

lattice fluctuations m the

Landau,

Peierls and

Cooper channels, respectively.

(16)

SUSCEPTIBILITY AT SMALL q AND u~. The

expression corresponding

ta the electron-hale bubble of

Figure

3a is

xii,14~i)

=

-) ~ Gpii,14~i)Giii

+

@, (A.l) p,1

for one

spm~rientation. Using

the

spectral representation

of

Gp(k, (çi~))

and

performmg

the fermion

frequency

sum, one finds

~~~'~~

~~

~~~~

~~j Î_~ ~~'~~~~~~'~"~~ ~~iÎÎ~ÎÎ(Î~ÎqÎ~~ÎÎ' ~~'~~

,

~~ '

Since most of the

spectral weight

appears in the

region

uJ' re

ep(k),

one can

replace ep(k) by

uJ'

m the ratio of the above

integral,

which can be cut off at

+Eo/2.

From the definition of the

density

of states

(32),

one

finds,

after

analytic

continuation to real

frequencies,

~~

~~~'~'~~

~~

Î~~Î~ ~~~" ~~

~~

ÎÎ'~ ~~'~° pÎÎ~

uJ p

Im

x(q,

uJ.

(çi~ ))

=

~~~~~

D[uJ', (ô~)] (- Î~ du'~jp7ruFqô(pufq uJ). (A.3)

2 ~~/~ ôàJ

P

Here

D(uJ, (çi~ ))

is the

density

of states per spm in the presence of the

spin-Peierls pseudo-gap.

The calculation of

y(f, (çi~))

at the

step

é of the renormahzation group

procedure gives

the

same expression, except for

Eo

which is

replaced by Eo(é).

PEIERLS AND COOPER SUSCEPTIBILITIES. The calculation of the Peierls electron-hale bub- ble of

Figure

3b starts with the

following expression

x(2kF

+ q, mm,

(çi~))

=

~~

~j G-(k,

mn,

(çi~))G((k

+

2kF

+ q, uJn +

mm), (AA)

~ k,w~

for both

spin

orientations. At zero external variables and after a summation over the fermion

frequencies

and the use of the

spectral representation

for

G-(k, (çi~)),

one

gets

x(2kF, (4~))

"

-~ ~j /~~

du~' Im

G-(k,

u~,

(ô~)) ~~~), /) j~~~~, (A.5)

k -"

which

actually

coincides with the real

part

of the Peierls bubble.

Assummg

that Im

G-(k, uJ',

(çi-))

is

peaked

in the region uJ' re

e-(k),

from which one

replaces e-(k) by

uJ' m the ratio appearing m the

integral,

we find

"

x(2kF,14~i)

=

~°~~

DIW', ~ildW'~~~~~jÉ'~~~

IA-fi)

As for the electron-electron

(Cooper) elementary

bubble at zero external variables

correspond-

mg to trie expression

x(lP~i)

=

( ~ G-(1,14~i)Gi(-1), (A.7)

1

(17)

trie

property G( (-k,

-mn

=

-G( (k+2kF,

mn leads to trie relation

x(2kF, (4~ ))

"

xl (4~ ))

Within trie renormalization group scheme at

é,

trie same expressions become

dx(2k~,jçi-j)

=

-DjEo(é)/2,jçi-jjdé

=

-dx(14~i), (A.8)

when ekaluated in trie outer energy shell.

Finally,

after

analytic

continuation to

rell frequencies

of

(A4),

we can carry over trie same

type

of calculation for the

imaginary part

of the Peierls bubble at T in the hmit of small

frequency

and we find

Im

~~2kF

+ ~

i lil/Î[[~,lj~,,

j< ii ini~ii niuJl

+

vf~ii

à

i~'

+

~~ ~~~~/~~

~ 2 -Eo/2

(~'~~

=

~

)~~~~~~~ ~~

~

Appendix

B

One-Particle

Self-Energy

and Four-Point Vertex Part in Presence of Phonons

ONE-PARTICLE SELF-ENERGY. The

expression

for the one

particle self-energy diagram

of

Figure

4a reads

L+ (k, 14~1)

=

-2g~ )~

~

~

G-

(1',14~1)Gf (1'

+

@GÎ Ii

i>,1

ci

2g~ ~~ ~j ~j /~~ duJ'lm G(k', uJ', (çi~ ))

XL

~, _~

~

[iuJn

e+(k) -ÎÎÎÎ

+

ÎÎÎÎ ÎÎÎ'Î ÎÎÎ~~ e-(k')

+

uFqÎ' ~~'~~

where the second fine results from a fermion

frequency

summation and the use of the

spectral weight representation.

The

approximation

scheme of

Appendix

A then allows to put

e-(k')

m

uJ' m the ratio appearmg m r-h-s of this last

expression

and to cut off the

mtegral

over uJ' at

+Eo/2.

In trie RG

procedure,

trie outer energy shell evaluation of

L+

at

é,

which is obtained after trie

frequency

sum over mm leads to

dL+

=

dL(

+

dLj,

where

dLl(1,14~i)

=

-(DiEo(é)/2,i4~iidEo(é)

~

j ~~ ml+Eo(é)/2 vfql n1+Eo(é)/21) lnB1-vfql

+

nlvfq

+

e+(k)1) 2v~q

+ iu~n e+

jk)

Cf

( iG°ii)i~~ DiEoié)/2, 14~ ii dé, iB.2)

to

leading

order m

[G°(k)]~~

=

iuJn e+(k),

for

flEo(é)

»

1,

and where nB

(xi

=

(eP~ 1)~~

Here the

integration

over trie momentum transfer q is found to contribute

only

m the interval

2uFqo

>

2uF

(q( >

Eo(é),

where qo is a momentum transfer cut-off.

(18)

VERTEX PART. The evaluation of the

two-Îoop

vertex

part

in the presence of Îattice fluctu- ations

proceeds along

similar lines. The

diagrams

of

Figure

4b

corresponds

to

ni

+

r)~~

and

to the

generic expression

r[~)((çi~ ))

j~2

=

-g~

~

~j G~(k', çi~)G((k' -1)G( (k~,2 +1)G$(k~,2 +1 @. (B.3)

~ [,

)

In trie RG sense one can

drop

the

dependence

on the external variables

(ki, k2, iÎl Performing

frequency

sums on mn> and mm> and usmg trie above

approximation scheme,

one

gets

dr[11

t g~

~)~j DlEo (é)/2, 14 Il dEo (é)

x

/ j iniEo(é)/2

+

v~q'i

n

iEoié)/211 inB i-v~q'i

+ n

iv~q'ii

+

Eoié)

-

-Eo if))

t g~

jDlEoié)/2, Ii- Il dé, (B.4)

for

2uFqo

>

2uFÎq'Î

>

Eo lé), flufq'

»

1,

and

flEo(é)

> 1.

References

[1]

Schegolev I.F., Phys.

Status Soiidi A12

(19î2) 9;

Toombs

G-A-, Phys. Rep.

40

(1978)

181.

[2]

Bray J-W-,

Interrante

L.V.,

Jacobs I.S- and Bonner

J-C-,

m Eztended Linear Chain Com-

pounds,

J-S- Miller Ed.

(Plenum,

New

York, 1983)

Vol.

3,

p. 353.

[3] Lee

P-A-,

Rice T.M- and Anderson

P-W-, Phys.

Rev- Lett. 31

(1973)

462.

[4j Cross M.C. and Fisher

D.S., Phys-

Rev. B 19

(1979)

402- [5]

Fukuyama H., Synth.

Met. 19

(1987)

63 and references therein.

[fil

Pouget J-P-,

Moret

R.,

Comes

R., Bechgaard K-,

Fabre J-M- and Giral L., Moi.

Cryst- Liq- Cryst.

79

(1982)

129.

[7] Creuzet

F.,

Bourbonnais

C-,

Caron

L.G.,

Jérome D. and

Bechgaard K-, Synth-

Met- 19

(1987)

299.

[8] Liu

Q., Ravy S., Pouget J-P-,

Coulon C- and Bourbonnais

C., Synth.

Met. 55-57

(1993)

1840.

[9] Caron

L.G.,

Bourbonnais

C-,

Creuzet F- and Jérome

D., Synth.

Met. 19

(1987)

69.

[10] Dumoulin

B.,

Bourbonnais

C., Ravy S-, Pouget

J.-P. and Coulon

C-, Phys.

Rev. Lett. 76

(1996)

1360.

[Il]

Laversanne

R.,

Coulon

C.,

Gallois

B., Pouget

J.-P. and Moret

R.,

J.

Phys-

Lett. France 45

(1984)

L393.

[12]

Wzietek P. et

ai.,

J.

Phys.

I France 3

(1993)173.

[13]

Su

W-D-,

Schrieifer J-R- and

Heeger A.J., Phys-

Rev. B 22

(1980) 2099;

Barisic

S-, Phys.

Rev. B 5

(1972)

932.

[14j

Barisic S- and Brazovskii

S.,

m "Recent

Developments

m Condensed Matter

Physics",

Vol.

I,

J-T- Devreese Ed.

(Plenum,

New

York, 1981)

p. 237.

[15j

See for

example,

J.

Solyom,

Adv-

Phys.

28

(19î9)

201and references therem.

(19)

[16j

Bourbonnais C- and Caron L.G., Int. Journ. Mort.

Phys.

5

(1991) 1033;

Bourbonnais C.

and Caron

L.G.,

J.

Phys.

France 50

(1989)

2751.

[lîj

Kimura

M-, Prog.

Theor.

Phys.

53

(19î5) 955; Dzyaloshinskii

I.E. and Larkin

A.I.,

Sov.

Phys.

JETP 34

(1972)

422.

[18j

Voit

J-, Rep- Prog. Phys.

58

(1995)

977 and references therem-

[19j

Dieterich

W.,

Adv.

Phys.

25

(19î6) 615; Scalapino D.J.,

Sears M. and Ferrell

R-A-, Phys.

Rev. B 6

(1972)

3409.

[20]

Moryia T.,

J.

Phys-

Soc.

Jpn18 (1974)

2911.

[21] Bourbonnais

C.,

J.

Phys.

I France 3

(1993)

143.

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