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Order-by-order expansions for intermediate Hamiltonians by the shift technique

A. Zaitsevskii

To cite this version:

A. Zaitsevskii. Order-by-order expansions for intermediate Hamiltonians by the shift technique. Jour-

nal de Physique II, EDP Sciences, 1993, 3 (4), pp.435-441. �10.1051/jp2:1993101�. �jpa-00247844�

(2)

Classification Physics Abstracts 31.15

Short Communication

Order-by-order expansions for intermediate Hamitonians by the shit technique

A-V- Zaitsevskii

Laboratory of Molecular Structure and Quantum Mechanics, Chemical Department, M. Lomonossov Moscow State University, 119899 Moscow GSP, Russia

(Received

lo December 1992; accepted 16 February

1993)

Abstract The level shift technique is applied to derive rigorous order-by-order intermediate

Hamiltouiau QDPT expansions. The novel approach offers an insight into the relations between

different intermediate Hamiltonian theories. The direct comparison with the shifted QDPT expansions for conventional effective Hamiltouiau is also presented.

1 Introduction.

Although

the effective Hamiltonian

quasidegenerate perturbation theory (QDPT)

is

usually

considered as a

quite general approximate

method in atomic

physics

and quantum

chemistry

[1, 2], its

applicability

to

highly degenerate

systems is

seriously

limited

by

the convergence

difficulties in the presence of intruder states [3]. These difficulties are

usually

associated with the appearance of small energy denominators in

QDPT expansions;

it seems, however [4], that

they

stem from the fundamental

properties

of effective Hamiltonians defined

according

to Bloch [5] and des Cloizeaux [6]. To solve the

problem,

Malrieu et al. [7] had

proposed

the intermediate effective Hamiltonian

approach

where the

requirements imposed

on several

"intermediate"

eigenstates

of the effective Hamiltonian had been relaxed. For a model space of dimension N, an intermediate Hamiltonian should

provide only

M < N

eigenvalues coinciding

with those of the total

Hamiltonian,

the

remaining (M-N)

roots

being only

more or less reliable

approximations

for exact ones. Over the last few years several different versions of the intermediate Hamiltonian

QDPT

have been

developed. They

fall into two distinct

categories:

I) those

deriving

the intermediate Hamiltonian from some reference Bloch wave operator assc-

ciated with a

pre-selected subspace

of the model space

(sc-called

main model

space) [7-9];

it)

those which do not need any a

priori

subdivision of the model space and use the intermediate level shift

technique

to eliminate numerical instabilities

[10-12].

(3)

436 JOURNAL DE PHYSIQUE II N°4

The methods of the first group offer the

possibility

to

expand

the intermediate Hamiltonian

as a strict power series in

perturbation

and to reduce

significantly

convergence difficulties in

comparison

with the conventional

QDPT.

Some of them are able to

reproduce semiquantita- tively

the effective interactions of the intermediate

eigenstates (I.e.

to dress these states [7,

9]).

Unfortunatelyi

in the case of

strong coupling

of main model states to intermediate ones the

QDPT

series converge

asymptotically

or even

diverge.

It should be also noted that the

rigor-

ous derivation of

working

formulae

(especially

for

non-degenerate

model spaces [9]) is not too

transparent.

Recent versions of the shift

technique completely

eliminate the intruder state

problem

and

guarantee

the true convergence of

QDPT

series in rather

complicated

situations.

Moreover,

the

approaches

of this group have the

advantage

of

conceptual simplicity

and enable to

produce

a

wide

variety

of intermediate Hamiltonians and to control the

dressing

of intermediate states in

a

physically

transparent manner. These

advantages

are offset somewhat

by

the fact that the

resulting expansions

are

only approximate

power series in

perturbation

and thus seem to be unsuitable for the

many-body

treatment.

In the present communication we undertake to

develop

the

rigorous order-by-order

inter- mediate Hamiltonian

expansions

in the frame of the shift

techniquei introducing

the

auxiliary

Bloch wave operator associated with a fixed main model space. The

analysis

of this expan-

sion should offer us

insight regarding

the relations between the two above mentioned groups of methods. The choice of the shift parameters and convergence

properties

are discussed. To

demonstrate the

generality

and

flexibility

of the level shift

approach,

we

study

its

ability

to gen- erate the

analogs

of

previously

described intermediate Hamiltonian theories. Furthermore, we

compare

directly

the shifted intermediate Hamiltonian

approach

with the level shift

technique

used to

improve

the convergence of the conventional effective Hamiltonian

QDPT.

2. Basic formalism.

Consider a quantum system described

by

the

time-independent Schr6dinger equation

H

j~~)

= E~

j~~) (i)

Suppose

that the Hamiltonian H is

split

into the zerc-order part Ho and the

perturba-

tion V

H=Ho+V (2)

and the zerc-order

problem

Holk)

=

6klk) (3)

is solved. Let us divide the functional space into two

subspaces,

the

(extended)

model space

Lp

with the

projector

P and its

orthogonal complement LQ (outer space) projected by Q

" I P.

The model space is assumed to be

spanned by

an

appropriate

set of zerc-order

eigenvectors.

We

are

going

to search for an intermediate Hamiltonian

ji

[1, 7]

acting

within Lp and

describing properly

M < dim Lp

eigensolutions

of

equation (I).

We

adopt

the

following

Ansatz for

ji

:

fl

= PHR

(4)

where R is the wave-like

operator obeying

the intermediate normalization

(4)

R = P +

QRP (5)

and

satisfying

the relations

RP i~bm) = i~bm), m =

ii

i

M

(6)

This Ansatz appears as a

straightforward generalization

of the Bloch effective llamiltonian [51

7].

M

eigenvectors

of

ji

should coincide with the

projections

of the

corresponding

exact

eigenstates

onto Lp.

Introducing

the

orthogonal projector

P onto the

subspace spanned by

these

"good" eigenvectors [Pi§m),

m

= I,

,

Mi

one can write the basic

equation

of the intermediate Hamiltonian

theory [10-13]

HAP =

RjiP

= RHRP

(7)

Substituting

the

partitioning (2)

into

equation (7),

we get

Q (R, Ho]

P =

Q(VR RVR)P (8)

This

equation

is

obviously

insufficient to define the wave-like operator

unambiguously.

Fol-

lowing ill,

12] we eliminate the redundant

degrees

of freedom

by postulating

Q (R,

HOI

(P P)

=

Q(VR

RVR

RS)(P P) (9)

where S is the shift operator.

Equation (9)

is

compatible

with

equation (8)

for an

arbitrary S;

the choice S

= 0 reduces

equations (8)

and

(9)

to the usual

equation

for the Bloch wave operator Q [5] associated with the model

subspace Lp

Q

IQ,HOI P =

Q(VQ QVQ)P (10)

[14].

For that

follows,

it is convenient to define the M-dimensional main model space LM E

Lp by

its

projector

M

PM = Jim P

=

£ (m

><

ml (II)

V-o

The

subspace

Li

Projected by

dim Lp

Pi

= P PM =

~

Ii >< I(

(12)

I=M+I

is to be referred to as the intermediate space. Now we

specify

the shift operator as

S=PISPI=~(i>s;<I( (13)

(s;)

are fixed real numbers.

Taking

into account that for this choice

Q (R,

HOI P +

QRS

=

Q [R, (Ho

+

S)]

P

(14)

we can convert

equations (8, 9)

into the form

Q [R, (Ho

+

S)]

P =

Q(VR RVR)

+ RS

(P

PM

(15)

(5)

438 JOURNAL DE PHYSIQUE II N°4

As it was shown earlier

[10,

12], similar

equations

are

readily

solved

by combining

the

approximate perturbation expansion

of R with a

non-perturbative (iterative)

treatment of the

V-dependent projector

P. However, the aim ofthe present work is to

study

the

rigorous (Taylor- type) order-by-order expansion

of the wave-like operator. To construct P

perturbatively,

we

introduce the

auxiliary

Bloch wave operator w associated with the main model space

w = w PM =

PM

+

(Q

+

Pi)w PM

QJPM

film)

"

film) (16)

and

expand

this operator as a power series in V

w = PM +

w(~l

+ w(~) +..

(17)

where

w(")

are

given by

the well-known recursion formula [14]

n-I

(Pi

+

Q) (w("~, Hoj

PM =

(Pi

+

Q) Vw~"~~)

+

£ w~'~vw~"~"~~~

PM

(18)

i=1

Since P may be

expressed

in terms of w and P as

P = Pw

(wtPw)

~~

wtP (19)

(the

verification of this formula is

straightforward),

one can write down the

corresponding expansion

for P

p = p~ +

p(1)

~

p(2)

~

p(1)

~

p~(1)

~

~(i)t

p

p(2)

~

p~(2)

~

~(2)t

p +

p~(1)~(i)t

p

~(i)t~(1)

~~~ ~~~j

Inserting (20)

into

equation (15)

and

setting

R = P + R~~~ + R~~) +

, one

readily

obtains the recursion formula

n-I

Q (R("), (Ho

+

S)j

P =

Q VR("~~) ~j (R(~)VR("~~~~) R(~)SP("~~))

P

(21)

k=1

which

yields

the desired

QDPT

series for R. The

perturbation expansion

for

k

is

immediately

obtained

using equation (4).

(6)

3. Discussion.

Now consider the

problem

of

choosing

the shift parameters S; and discuss the convergence of

our

expansions. Taking

into account the subdivision of the model space it is convenient to rewrite our zerc-order Hamiltonian in the form

Ho = PM Ho PM + Pi Ho Pi +

QHOQ

=£(m>em<m(+£(I>e;<I(+£(a>ea<a( (22)

m ; «

Let us first notice that once the main model space is

specified,

one is

always

able to choose the intermediate space in such a way that the PM HOPM and

QHOQ

spectra are well

separated

in energy, I-e- the differences

(em eo)

are not small. On the other

hand,

in

highly degenerate

system it is often

impossible

to eliminate

quasidegeneracies

em ~- e; and e;

~- ea with any

physically

reasonable choice of Ho Since the resolvent associated with the Liouvillian super- operator [15] in the I-h-s- of

equation (10)

involves energy denominators

(e; co),

the latter group of

quasidegeneracies

should

yield

ill-defined terms in the

perturbation expansion

of Q and

destroy

its convergence [1, 3]. This is the usual manifestation of the well-known intruder

state

problem. Similarly,

small energy differences

(em e;) entering

the Liouvillian in the I-h-s- of

equation (18)

can

provoke

a poor convergence of the series

(17)

and

(20).

In contrasti one is

always

able to prevent the appearance of small energy differences in the shifted Liouvillian

Q Ill, (Ho

+

S)I

P =

L ~ la

>

(em 6a)

<

al Rlm

><

ml

+

~ L la

> 16; +

S>

6«)

<

al Rli

><

il (23)

by

a proper choice ofthe shift parameters s;. Since the

perturbation

V remains

unchanged,

we

might

expect to

improve

the convergence of the shifted

expansion. Nevertheless,

the intruder

state

problem

is not

completely

avoided. It may be

brought

back into

higher-order

terms via the

expansion

of the

projection

operator

Pi poorly converging

in the presence of "main

intermediate~'

quasidegeneracies.

One can

easily verify

that the ill-defined terms may

generally

appear in

RI"),

n >

2,

and

jil"),

n > 3. We are

going

to show that the destructive role ofthese terms may be reduced

by

a careful choice of the shift.

Assume that Ho is

strictly degenerate

within the main model space

PM

HOPM

= eoPM

(24)

and S is chosen to lift all the intermediate zerc-order levels to co

S;

= co e;

(25)

The first-order correction takes the form

R(~)

=

Go

VP

Go

+

~

~

(26)

60 o

(7)

440 JOURNAL DE PHYSIQUE II N°4

corresponding

to the conventional "shifted Bk" scheme

[16].

R~~) should contain the terrrts

stemming

from the first-order correction to P.

Although

the

dangerous

denominators do enter

P~~),

we note that

R~~)SP~~)

= R~~)SPW~~)

= GOV

£

~ ~ ~' ~ ~ VPM

# GOVPIVPM

(27)

; ~° ~i

and arrive at a

remarkably simple expression R(~)

=

GOVGOVP G(VPVP

+

G(

VPIVPM

(28)

I-e- ill-defined terms do not appear up to the second order

(third

order for

ji) inclusively.

This result admits a

simple interpretation. Being sufficiently large

to avoid the intruder state

prob- lem,

the shift values

(25)

are still small

enough

to cause instabilities in R due to inaccuracies in P. For

non-degenerate

model spaces the rule

(25)

should be

generalized

as s; = max

((em ))

-e;.

It is

interesting

to note that

an

analogous

choice of the shift

was also advocated in the frame of the

semiperturbative approach involving

the iterative treatment of the

projector

P

[10,

12].

The

expressions (27, 28)

are similar to those

appearing

in the

generalized degenerate

pertur- bation

theory (GDPT)

of Malrieu et al. [7,

9], although

their derivation is

completely

different.

It seems that the present

approach essentially

recovers the GDPT and related theories [9] while

the

flexibility

and

physical

transparency of the shift methods

[10-12]

are still retained.

Finally,

it seems to be instructive to compare the present

approach

with the level shift

technique widely

used in the frame of the conventional effective Hamiltonian

QDPT.

In the latter case the shift appears as a modification of the zerc-order

problem:

Ho-H[=Ho+S

V - V'= V S

(29)

While small denominators are

readily

avoided

by

a proper choice of

(s;),

the

divergence

often survives because of the

corresponding

increase of the numerators of the

higher-order QDPT

corrections

[17].

With the

assumptions (24, 25), agreeing perfectly

with the common

practice

of

lifting

all the zero-order model levels to the lowest one [2,

18],

we

immediately

obtain the

following expressions

for the Bloch wave operator Q:

Q(~)

= GOVP

(30)

Q(~)

=

GOVGOVP G(VPVP

+

G(V £ ii

>

(co e;)

< I(

(31)

(see

also

[18]).

Once the shift is chosen in a consistent way, Q(~) coincides with the first-order correction to the wave-like operator

(26).

The second-order formula

(31)

differs from its coun- terpart in the intermediate Hamiltonian

theory (28) only by

the last term. In both cases there should be no

problem

with the denominators. The numerators in

equation (28)

are of the same order

ofmagnitude

as those in the

corresponding

non-shifted formula. In contrast, if the energy range

spanned by

the model space

Lp

is

broad,

the last term in

equation (31) containing

the

differences

(co e;)

may be enormous. This situation

frequently

occurs in

many-body theory

when

complete

model spaces

(e.g.

valence spaces in quantum

chemistry)

are used. As a conse- quence, the second-order effective Hamiltonian associated with the wave operator

(30)

should deviate

significantly

from the third- and

higher-order approximations. 9n

the other

hand,

the

(8)

same operator may be also considered as a second-order shifted intermediate Hamiltonian. The latter

point

of

view, being formally equivalent

to the former one, is

physically

more reasonable because

higher-order

corrections for intermediate Hamiltonian are not

expected

to be as

large

as for the conventional effective Hamiltonian.

4. Conclusions.

The level shift

technique

is used to

expand

intermediate Hamiltonians as strict power series in

perturbation.

The

resulting

version of the intermediate Hamiltonian

QDPT

fills the gap be-

tween the

previously

formulated level shift

approaches

and the theories

deducing

intermediate Hamiltonians from the reference Bloch wave operators. The

analysis

of

explicit

second-order wave-like operator

expressions

advocates the

lifting

of zerc-order intermediate levels to main

ones. With this

particular

choice of the

shift,

the present method bears strong resemblance to

the

generalized quasidegenerate perturbation theory

of Malrieu et al. Our results suggest that the shift

technique

offers the

possibility

to

inspect

various intermediate Hamiltonian theories from a

general

and unified

point

of view.

Being important

for better

understanding

of thec- retical

backgrounds,

the novel

approach provides

also a

potentially

useful

computational tool;

applications

to several

problems

in quantum

chemistry

are now in progress.

References

ill

DURAND Ph. and MALRIEU J-P-, Ab iuitio methods of quantum chemistry. P-I-, K-P- Lawley Ed.

(Wiley, 1987)

p.321.

[2] HosE G. Many-Body Methods in Quantum Chemistry, U. Kaldor Ed.

(Springer-Verlag, 1989)

p.43.

[3] ELLIS P-J- and OSNES E., Rev. Mod. Phys. 49

(1977)

777.

[4] EVANGELISTI S., DAUDEY J-P- and MALRIEU J-P-, Phys. Rev. A: Math. Geu. Phys. 35

(1987)

4930.

[5] BLOCH C., Nucl. Pllys. 6

(1958)

329.

[6] DBS CLOIzBAUX J., Nucl. Pllys. 20

(1960)

321.

[7] MALRIBU J-P-, DURAND Ph. and DAUDBY J-P-, J. Phys. A: Math. Gen. Phys. 18

(1985)

809.

[8] HBULLY J.-L. and DAUDBY J-P-, J. Chem. Phys. 88

(1988)

1046.

[9] HBULLY J.-L., EVANGBLISTI S. and DURAND Ph., Inn. J. Quantum Chem., to be published.

[10] ZAITSBVSKII A-V- and DBMBNT'BV A-I-, J. Phys. B: At. Mol. Opt. Phys. 23

(1990)

L517.

[11] KOCH S., Theor. Chim. Acta 81

(1991)

169.

[12] ZAITSBVSKII A-V- and HBULLY J.-L., J.

Phys.

ES At. Mol. Opt. Phys. 25

(1992)

603.

[13] MUKHBRJBB D., private communication.

[14] LINDGRBN I., J. Phys. B: At. Mol. Phys. 7

(1974)

2441.

[15] EVANGBLISTI S., DURAND Ph. and HBULLY J.-L., Phys. Rev. A: Math Gen. Pltys. 43

(1991)

1258.

[16] GERSHGORN Z. and SHAVITT I., Iut. J. Quantum Chem. 2

(1968)

751.

[17] KALDOR U., Iut. J. Quantum Chem. 28

(1985)

103.

[18] HOSE G., Theor. Chim. Acta 72

(1987)

303.

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