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Submitted on 1 Jan 1990

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Exploring photoproduction dynamics through

polarization experiments

F. Arash, G.R. Goldstein, M. J. Moravcsik

To cite this version:

(2)

Exploring photoproduction

dynamics

through

polarization

experiments (*)

F. Arash

(1,3),

G. R. Goldstein

(2)

and M. J. Moravcsik

(3, ~)

(1)

Department

of

Physics, Temple University, Philadelphia,

PA 19122, U.S.A.

(2)

Department

of

Physics,

Tufts

University,

Medford, Mass 02155 U.S.A.

(3)

Department

of

Physics

and Institute of Theoretical Science,

University

of

Oregon, Eugene,

Oregon

97403 U.S.A.

(Reçu

le Il décembre 1989,

accepté

le 21

février 1990)

Abstract. 2014 The structure of

spin-0

meson

photoproduction

from

spin-1 /2 particles

is

given

in several useful

optimal

frames Polarization

experiments

for this reaction are then discussed from the

point

of view of

a) determining

the reaction

amplitudes, b) studying one-particle-exchange

mechanisms,

c) detecting

patterns in the

amplitude

structure. The

existing

data are then

analyzed

in terms of the above

considerations,

and the need for future

experiments

is

specified.

Classification

Physics

Abstracts 13.60 -

13.75G - 13.88

1. Introduction.

Spin-0

meson

photoproduction

from

spin-1/2

hadrons has

always

played

an

important

role in

our

longstanding quest

to discover the laws

underlying strong

interactions.

Experimentally,

such reactions have been

relatively easily

accessible

through

the various electron accelerators.

Theoretically,

the reaction is

partly strong

and

partly electromagnetic,

and since the latter is

to a

large

extend under our calculational

control,

such reactions have formed an

important

alternative to the

entirely

strong

interaction processes.

Photoproduction

reactions are also

favorable in the richness of their

spin

structure,

being

neither

overly

simple

nor too

complicated. Unfortunately,

this

advantage

has not been well

exploited

in the

past,

as we will

see, and in fact one of the aims of the

present

paper is to describe the ways in which this defect

can be remedied.

In any case,

however,

photoproduction played

a crucial role in the

exploration

of the

pion-nucleon interaction at the lowest

energies

in the very

early days

of

particle physics [1],

and

interest in such reactions has continued into the

present.

A number of

present

day

laboratories

[2]

concern themselves with such reactions and

plan experimental

programs around them.

(3)

It

is,

therefore,

our aim to

give

a

comprehensive exposition

of the

polarization

structure of this reaction and of the uses of this structure for

exploring

the

dynamics underlying

such a

reaction. The outline will be as follows :

Section 2 : Formalisms

describing photoproduction.

Section 3 : The

observable-amplitude

structure for Lorentz-invariance

only.

Section 4: The

observable-amplitude

structure with Lorentz invariance and

parity

conservation for several useful formalisms.

Section 5 :

Determining

the

amplitudes

from the observables.

Section 6 : Polarization

signatures

of various

dynamical

mechanisms. Section 7 : The

analysis

of

existing

data.

Section 8 :

Looking

at the future.

2. Formalisms

describing photoproduction.

There have been two

major types

of

phenomenological

formalisms for the

description

of

photoproduction

reactions.

The first and

chronologically

older one is the

partial

wave cum

multipole

formalism

[3],

used from the very

beginnings

of the studies for

photoproduction.

This formalism results in

parameters,

each of which

gives

the reaction

strength

in a

given angular

momentum and

multipole

state of the

photon-hadron

and meson-hadron

systems.

This

description

is

not

as

economical for this reaction as the

corresponding angular

momentum

(phase shift) description

is for elastic

scattering,

since

unitarity

does not reduce the number of

parameters

needed,

except

when Watson’s theorem can be used to link

photoproduction

with the

corresponding

elastic

scattering.

The

description,

however,

still results in economy at the lowest

energies

where

only

a very few states need to be included. The

description

also has some theoretical

advantages

in energy

regions

where certain

angular

momentum and

multipole

states dominate the

dynamics,

such as at a few hundred MeV’s. Another theoretical

advantage

is that certain

mechanisms in the interaction

(such

as the meson-current

term)

can be

explicitely

included

[4],

thus

making

the

angular

momentum

expansion

converge better. An

important advantage

of the

description

is that it links data at different

angles (at

a

given energy).

The

disadvantages

of this

description

manifest themselves

increasingly

as one goes to

higher

energies.

There the number of

parameters

needed becomes very

large,

and since the method

requires

data in an

increasingly complete

range of

angles,

the determination of the

parameters

becomes

experimentally

more and more difficult. At the

higher energies

the distinctive role of

particular angular

momentum and

multipole

states also subsides.

Furthermore,

in this method

there are

always

uncertainties about where the

angular

momentum and

multipole expansion

can be cut off without

mutilating

the

analysis.

The other

type

of formalism used for

phenomenological analyses

of

photoproduction

reactions is in terms of reaction

amplitudes [5].

This method

performs

the

analysis

at every energy and

angle separately,

which

represents

a loss of economy, at least at lower

energies,

but offers

greater flexibility

since data at

single angles

can thus be treated. The number of

reaction

amplitudes

for a

given

reaction is

independent

of energy, and this

eventually

favors

this method over the first one in which the number of

parameters

increases with energy

indefinitely.

The

amplitude description

also has the

advantage

of

offering

greater

variety

and

flexibility,

since the number of different

amplitude

formalisms that can be used for the

description

of a

given

reaction is very

large,

and so one can

adjust

the choice of formalism to the

specific

aim at hand.

In this paper

only

the

amplitude

formalisms will be

used,

partly

because the other

(4)

above a GeV

(or

even

starting

from below

that) only

the

amplitude description

is

practically

feasible.

Thus the next

step

is the choice of

amplitude

formalisms.

For a

given

reaction,

and for a

given

set of

symmetries holding

for that

reaction,

the number of

amplitudes

is the same for any formalism. This number

depends only

on the values of the

spins

of the

particles participating

in the reaction and on which

symmetries (conservation

laws) apply.

This has been discussed

extensively

before,

and hence we will

just apply

those

results to our

present

reaction. In

particular,

for the reaction of

the number of

complex

reaction

amplitudes

with the

imposition

of Lorentz invariance alone is

8,

while if

parity

conservation is also

imposed,

the number reduces to 4.

Since the observables

depend linearly

on bilinear

products

of the

complex amplitudes,

there are, for the case of Lorentz invariance

alone,

64 different bilinear

products

and hence 64

different

linearly independent

observables. If non-linear

dependences

are also

considered,

the number of

independent

observables is

only

2 x 8 - 1 = 15

(because

one overall

phase

factor is

always arbitrary).

The

corresponding

numbers for the case when both Lorentz invariance and

parity

conservation are

imposed

are 16 and 7.

The

relationship

between observables and the bilinear

products

of

amplitudes

is

given by

a

(large)

matrix. In order to achieve economy and

simplicity

of structure, this matrix should be

as close to a

diagonal

one as

possible.

It can be shown that at

complete diagonalization

of this

matrix is

prohibited

by

requirements

of

Hermiticity (which corresponds

to the

requirement

that observables be

real).

The class of formalisms in which the matrix is as close to

diagonal

as

possible [6]

is called «

optimal

». In it this matrix consists of a

string

of small matrices

along

the main

diagonal

and zeroes

everywhere

else. The sizes of the small

matrices,

for any

four-particle

reaction,

are

1-by-1, 2-by-2, 4-by-4,

or

8-by-8.

If one of the four

particles

has zero

spin

(as

it is the case in our

reaction),

there are no

8-by-8

matrices.

In this paper we will consider

only

formalisms that are «

optimal »

in the sense

explained

above. Other

amplitude

formalisms have no

advantages

over

optimal

ones and are less

economical and more

complicated

and obscure in their structure.

Although

some

amplitude

formalisms used in the

past

are

non-optimal,

many others are

optimal,

and will appear as

special

cases of our discussion.

The observables referred to above are of the

« primary »

type,

that

is,

in them the

polarization

states of each of the three

particles

with

spins

are

specified.

In actual

practice

one

deals often with

experiments

in which the

polarization

state of one or several

particles

is

averaged

over, that

is,

in which

unpolarized

particles

are used. Such observables

(which

can

be obtained from the

primary

observables

by averaging)

are called «

secondary

» observables

[7].

The numbers of

amplitudes

and observables in the various submatrices of the

optimal

formalism can be ascertained

easily.

The situation for the case when

only

Lorentz invariance

is

imposed

is

given

in table I. This

applies

to all

optimal

formalisms.

When

parity

conservation is also

imposed [8],

the size of the submatrices and the related numbers

depend

on which

type

of

optimal

formalism we consider. Because of

that,

and

because of the submatrix structure

being

very much

simpler

anyway in that case, tables

analogous

to table 1 for the

parity conserving

case will not be

given.

Optimal

formalisms differ from each other in the orientation of the

quantization

axis for the

participating particles.

When

only

Lorentz invariance

applies,

each of these axes can

point

in

(5)

Table I. - Submatrix structure in the

optimal formalism

with

only

Lorentz invariance

imposed.

Legend for

the columns : A : Size of the submatrix

B : Number of submatrices with Re’s C : Number of submatrices with Im’s

D : Number of observables in such submatrices E : Which indices are the same ?

F : Number of observables

including

secondary

ones

(6)

is also

imposed,

the orientation for a

given

of these four axes must be either in the reaction

plane (« planar

formalism

»)

or

perpendicular

to the reaction

plane (« transversity

forma-lism

»).

Unless time reversal invariance or identical

particle

constraints are

additionally

imposed,

however,

the four

(or,

in our case,

three)

orientation axes can be chosen

independently

of each other. This is the case for the reaction under consideration. Thus in this

case we have the

possibility

also of so-called

hybrid

formalisms in which some of the

particles

are in a

planar

frame and others in a

transversity

frame.

For the

photon

(or,

for any zero-mass

particle)

the

helicity

formalism

[9]

appears to be the

most « natural » one since the zero-mass

particle

can have

only

two

polarization

states, which

are the

positive

and

negative helicity

states. For this reason all formalisms we will consider

have the

photon

in the

helicity

frame.

For the two

nucleon, however,

we have a choice. There appears to be no reason to treat the two nucleons

differently

from each

other,

though

we are not

compelled by

conservation laws

to do so. Thus we will consider

only

formalisms in which the two nucleons are either both in

the

transversity

frame or in the

planar

frame.

Having

the two nucleons in the

transversity

frame offers some

advantages.

This is so

because if we consider the task of

determining

phenomenologically

the

amplitudes

from

experimental

measurements, for all

parity conserving

reactions this task can be most

simply

accomplished

for the

transverity amplitudes.

This is so because in that case the direction

normal to the reaction

plane,

which is the

distinguished

direction for the

operation

of space

reflection,

coincides with the orientation of the

quantization

axes of the

particles.

As a

result,

a

simpler

set of

experiments

can be used to determine the

amplitude

parameters.

Furthermore,

the determination of the

magnitudes

of the

amplitudes

from a subset of

experiments

can also be done more

easily

in the

transversity

frame.

One of the

formalisms, therefore,

that we will use to describe

photoproduction

with the additional constraint of

parity

conservation is the

hybrid

frame in which the

photon

is in the

helicity

frame and the two

spin-1/2 particles

in the

transversity

frame. We will call this formalism the

hybrid

formalism.

The second formalism is the one in which all three

particles

with

spin

are described in the

helicity

frame. This is a traditional formalism and hence deserves to be included.

The third formalism is one in which the

photon

is described in the

helicity

frame but the two

spin-1/2 particles

have their

quantization

directions oriented in the

« planar-transverse »

direction,

that

is,

in a direction in the reaction

plane

which is

perpendicular

to both the

helicity

direction and the

transversity

direction. Such a

planar-transverse

formalism has

attracted attention since in several other

strong

interaction

reactions,

and at a broad range of

energies,

the relative

phases

of the reaction

amplitudes

in such a

system

appear to be

multiples

of 90

degrees [10],

thus

marking

a

general

feature of

strong

interactions hitherto not

predicted by

any model. In the other reactions this feature

appeared

in a pure

planar-transverse

frame,

that

is,

in a frame in which all

particles

had

quantization

axes in the

planar-transverse direction. This is

slightly

different from our

present

situation where the

photons

are described in the

helicity

frame,

and so it is of interest to

explore

whether the feature

observed in other reactions appears in such a

hybrid planar system

or not.

Finally,

the fourth formalism we will use is the so-called

« magic »

formalism

[11],

which is

particularly

suited to

explore

the

degree

of dominance of t-channel

one-particle-exchange

mechanisms. The «

magic »

formalism is also a

planar

one in which the

quantization

axes of

particles

are in directions which can be obtained from the

helicity

directions

by

a rotation

(in

the reaction

plane) by angles

which are

given by expressions depending

on the kinematic

parameters

of the reaction.

(7)

any other frame

by

linear

transformations,

which will be

given

in this paper.

Thus,

in

obtaining

the

amplitudes

from the

experimental

measurements, one has two

options.

One is to determine the

amplitudes

in

question directly

from the

experimental

observables.

In that case one needs to have measured the

particular

set of observables which leads

directly

to such a determination. For that purpose, tables are

given linking

the

amplitudes

to observables in each of the four formalisms. The

advantage

of this method is a

possible

reduction of the uncertainties in the

amplitude

parameters.

The drawback is that the

particular

set of

experiments

needed to determine the

amplitude

in a

given system

may be

experimentally

more cumbersome or difficult to carry out.

The second

option

is to determine the

amplitudes

in a formalism in which this

determination is

experimentally

the

simplest (which,

almost

invariably,

turns.out to be the

transversity system,

as mentioned

above),

and then to use the transformation relations among

amplitudes

in different frames to obtain the

amplitudes

in the desired formalism. The

advantage

of

greater

experimental

ease is

coupled,

in this case,

by

the

disadvantage

of

additional uncertainties in the

amplitudes

due to the transformation relations themselves.

More

precisely,

in this second method the error matrix on the

amplitude

parameters

will tend

to have

larger off-diagonal

elements,

thus

resulting

in a less clear determination of the values

of the

amplitude parameters.

Another

disadvantage

of the second method is in the case when the set of

experimental

data is not

complete enough

to allow a

complete

determination of all the

amplitude

parameters.

This situation occurs

quite frequently

in

practice.

In such a situation the first of the above

methods may

possibly yield

some

partial knowledge

of the

amplitude parameters,

while the

second method does not.

One can see,

therefore,

that there is a

good justification

to exhibit the

amplitude-observables relations in several formalisms and to

give

the relations

connecting

the

amplitudes

in various frames to the

amplitudes

in other frames. We will do this in section 4. As said

earlier,

all this is not needed in section

3,

since for Lorentz invariance

alone,

the

observable-amplitude

structure

is,

formally speaking,

identical for all

optimal

formalisms.

3. The

observable-amplitude

structure for Lorentz-invariance alone.

The

generation

of the

amplitude

relations in the

optimal

formalism is

by

now a standard

procedure

since not

only

has the

general

formulation of it been available for a

long

time but

also numerous

specific examples

of it are available in the literature. It

is, therefore,

sufficient here to review the notation and then

supply

the relations

themselves.

The

amplitudes

are denoted

by D ( a ;

d,

b )

where d denotes the final

spin-1 /2 particle,

a the

photon,

and b the initial

spin-1 /2 particle.

As an abbreviation in the

tables,

the

amplitude

will

also be denoted

by

the

triplet

of indices in the

following

fashion :

The a, b and d denote the

spin projections along

the

quantization

axis. Since the

photon

will

always

be taken in the

helicity

frame,

a can assume the values + 1 and - 1

(denoted simply by

+ and

-).

The indices b and

d,

which refer to

spin/ 1 /2 particles,

can assume values of

+ 1/2

and -

1/2,

which will be denoted

by

+ and -.

The observables are denoted

by

L

(uv, UV ; E fJ),

here u and v refer to the

photon,

U and V to the initial

spin/ 1 /2

particle,

and and n to the final

spin-1 /2

particle.

In the

primary

observables,

for each of the

arguments

in

L,

we can have the four

possibilities

of

(8)

The

relationship

between these states and the more traditional Cartesian

arguments

for the

spin-1 /2 particles

is

given by

where z is the

quantization

direction.

The

corresponding

relations for the

photon

are somewhat more

involved,

partly

on account

of the zero-mass of the

photon

and

partly

on account of a traditional

nomenclature,

originating

in classical

optics,

for the various states of

polarized light.

This is therefore discussed in detail in

appendix

A.

The

secondary

observables

contain,

for the

spin-1/2 particles,

R and 1 as

before, but,

instead of + +

and - - ,

the

unpolarized

states A =

( + + ) + ( - - )

and the vector

polarization along

the

quantization

axis, à

=

(+ + ) - ( - - ).

In the matrices

connecting

the bilinear

products

of

amplitudes

and the

experimental

observables,

for the case of Lorentz invariance alone all non-zero numbers are + 1 or

- 1,

which therefore are

denoted,

for the sake of

simplicity, by

+ and -,

respectively.

In the tabulated

relationships

the

headings

of the columns

give

two

amplitudes,

one below

the

other,

which denote

DD*,

with D

being

the upper and D * the lower one. The

designations

of the rows

give

the

observables,

with

L (

) omitted,

that

is,

showing only

the

arguments.

The

relationships

are

given

in table II.

Only

the

secondary

observables are indicated.

4.

Observables-amplitude

structure for Lorentz-invariance with

parity

conservation.

While the

observable-amplitude relationship

was the same for all

optimal

formalisms,

regardless

of the

quantization

directions of the

particles,

when

only

Lorentz invariance was

imposed

on the

reaction,

the situation is different when

parity

conservation is also

imposed.

We therefore have to consider the various formalisms of interest one

by

one. As

explained

in

section

2,

four

particular

formalisms will be discussed. In all of them the

photon

is in the

helicity

system,

and the differences among the four formalisms are therefore in the

quantization

axes of the two fermions.

In

particular,

in what we will call the

hybrid system,

the fermions are in the

transversity

frame. The second formalism is the

all-helicity system

in which the two fermions are also in

the

helicity

frame. The third formalism has the two fermions in the

planar

transverse

direction,

that

is,

their

quantization

axes are normal to both the transverse and the

helicity

directions.

Finally,

the

fourth,

the so-called «

magic »

frame has the

quantization

axes of the

two fermions in the reaction

plane

but rotated from the

helicity

directions

by

certain

angles

which can be calculated

(as

functions of the kinematic

parameters)

from a well defined and

known formula.

As far as the structure of the

relationship

between observables and

amplitude products

is

concerned,

the above four cases can be classed into two. In one the two fermions have

quantization

axes in the

transversity

direction,

in the other in the reaction

plane.

The latter class includes the

all-helicity,

the

planar

transverse, and the

magic

formalisms. These three will

only

differ from each other in the labels of the observables but not in the structure of the submatrices which connect observables with bilinear

products

of

amplitudes.

Thus it is useful

to discuss first these two

classes,

and then later turn to the differentiation of the various formalisms within the

planar

class.

As we discussed

earlier,

under

parity

conservation the

eight independent amplitudes

reduce

to four. Because all of the formalisms we are interested in have the

photon

in the

helicity

(9)

Table II. - The

(10)
(11)

These

equalities

are different for the

hybrid

and the

planar

cases, but are the same for all

formalisms in the

planar

class.

Indeed,

the

relationships

are as follows :

For the

hybrid

case :

For the

planar

case :

In these

relations,

the upper

signs

hold when the

product

of the four intrinsic

parities

of the

particles

in the reaction is

+ 1,

while the lower

signs

hold when this

product

is

- 1. For

photoproduction

of

pions

or kaons when both fermions are nucleons or

hyperons,

this

product

is + 1.

The notation of the

amplitudes

and of the observable

arguments,

for the latter

using

the conventional

symbols

often used

by experimentalists,

is

given

in table III. Not

given

are the

corresponding

observable

arguments

for the

magic

formalism,

since those

arguments,

expressed

in terms of this conventional

notation,

are

complicated

and

dependent

on

kinematic

parameters. Fortunately

this

complication

in no way

implies

that the

experiments

well suited for this

particular

formalism are also

complicated.

Since, however,

the

magic

frame is

simply

a

special

case of the

planar

formalism which is included in our tables and

results,

for any

particular application

of the

magic

frame

only

a small amount of

straightforward

calculation is needed to obtain

specific

result for that frame from the results

given

in the tables of this paper.

The actual

relationships

between observables and

amplitude products

are

given

in

tables IV-VII. We note from the remark at the bottom of table IV that results for the two

different values of the

product

of intrinsic

parities

are very

similar,

differing only

in the

signs

of some of the observables.

5. The

expérimental

détermination of the

amplitudes.

Since we want to determine four

complex

amplitudes,

and since one overall

phase

is

arbitrary

and

unmeasurable,

we need at least seven measurements to eliminate all continuous

ambiguities

from the

amplitude

determination. Since the

relationship

between observables and

amplitudes

is

bilinear,

not all sets of seven

linearly independent

observables will eliminate

the continuum of

ambiguities,

and even if a

given

set of seven

does,

there may still be discrete

ambiguities

left which will then be eliminated

by

additional measurements.

In this section we will comment on how the continuum of

ambiguities

can be eliminated

by

the various sets of seven measurements.

As for other

reactions,

the determination of the seven

amplitude parameters (apart

from

discrete

ambiguities)

can be

decomposed

into several

steps,

and it is useful to do so if definite

(12)

Table III. -

Notation

for amplitudes

and observable arguments

for

some

of

the

important

formalisms.

In the «

hybrid » formalism

the

photon

is in the

helicity frame

and the two

fermions

in the

transversity

frame.

In the «

all-planar » formalism

the

photon

is in the

helicity

frame

and the two

fermions

in a

general

planar frame.

The other two

formalisms

are

special

cases

of

the

« all

planar

»: the

« all-helicity »

formalism

hds the two

fermions

also in the

helicity

frame,

while the

« semi-planar-transverse »

has the two

fermions

in the

planar-transverse

optimal

frame.

The above observable arguments

pertain

to the fermions. For the situation in the case of the

photon,

see the

appendix.

done

quite accurately (much

more so than one can determine in later

steps

the relative

phases

of the

amplitudes),

and in the determination of the

magnitudes

there are never any discrete

ambiguities

which arise

exclusively

in the determination of the relative

phases.

What set of

experiments

are needed to determine the four

magnitudes

will

depend

on the

formalism used. It was shown on other reactions that the best

system

for the

phenomenologi-cal determination of

amplitudes

for a

parity-conserving

reaction is the

transversity

frame. We

do not have a pure

transversity

frame for our

present

reaction since the

photon

is

always

taken

in the

helicity

frame,

but even

taking just

the two fermions in the

transversity

frame

will,

as we will see,

represent

some

advantages

from this

point

of view.

It is also known

[12]

that the

magnitudes

can

always

be determined

through polarization

measurements in which the various

particles

are

polarized

along

their

quantization

directions. It is evident that once one carries out a

complete

set of

experiments,

one that is sufficient to determine the

amplitudes

in some

frame,

that set can also determine the

amplitudes

in any

(13)

Table IV. - The

relationship

between

secondary

observables and the bilinear

products of

reaction

amplitudes for

spin-zero

boson

photoproduction from spin-1/2 fermions,

with Lorentz invariance and

parity

conservation, in the

hybrid optimal formalism

in which the

photon

is in a

helicity

frame

and the

fermions

in a

transversity

frame.

For notation, see the text and the text

and the

caption

of

table II.

This table is for the

product

of the intrinsic

parities being

+ 1. If the

product

is - 1, the

signs

of the observables in which the

photon

argument is R or 1 should be reversed.

footing

from the

point

of view of the determination of the entire set of

amplitudes, they

differ in

merit,

as

explained

above,

when it comes to

obtaining

information from a

yet incomplete

set of

experiments.

Furthermore,

frames can also differ from each other in the

precision by

which

they yield

amplitude parameters,

since the error matrix connected with

amplitude

parameters

also

becomes transformed as we go from one frame to another.

These

general

remarks will now be demonstrated on the

particular

situation we have at

hand for our

photoproduction

reaction. For this purpose we look at tables IV-VII. In the

hybrid

formalism,

the four

magnitudes

can be determined

by

a set of

experiments

using only unpolarized photons,

and the fermion

polarizations

are

only

in the N direction.

(14)

Table V. - The

relationship

between

secondary

observables and the bilinear

products

of

reaction

amplitudes for spin-zero

boson

photoproduction from spin-1/2 fermions,

with Lorentz invariance and

parity

conservation, in the

all-planar optimal formalism.

For notation, see the

text and the

caption of

table II. For a note on intrinsic

parities,

see table IV.

Finally,

to determine also the

third

relative

phase (e.g.

between 1 and

3,

or between 1 and

4,

or between 2 and

3,

or between 2 and

4),

we need also

experiments

with

polarized photons.

We have a choice of whether we want to use

plane polarized

or

circularly polarized photons.

Thus,

in the

hybrid

formalism,

the

amplitude

determination is

neatly

divided into three

steps,

each

distinguished

from the others

by

the

type

of

experiment

needed,

and each

step

yielding

definite information on a subset of the seven

amplitude parameters.

In any

all-planar

formalism

(that

is,

also in the

all-helicity

and

semi-planar-transverse

formalisms)

the situation is less favorable. The subset of

experiments determining only

the

magnitudes

is of course also

present,

and it can involve

only

one

type

of fermion

polarization

(namely à).

The

subset, however,

requires

some measurements with

polarized photons,

in this case

circularly polarized.

One can also choose a set with

linearly polarized photons,

but then the fermion

polarizations

are not in the 4 direction.

Once the

magnitudes

are determined in the

all-planar frame, however,

we can determine the relative

phases

without

polarized photons.

This process can

again

be done

stepwise,

each

step consisting

of two measurements, and

yielding

two relative

phases.

(15)

Table VI. - The

relationship

between

secondary

observables and the bilinear

products of

reaction

amplitudes

for

spin-zero

boson

photoproduction

from spin-1/2 fermions,

with Lorentz invariance and

parity

conservation, with

all particles

in the

helicity frame.

For notation, see the

text and the

caption

of

table II. For a note on intrinsic

parities,

see table IV.

measurements with

polarized photons

were

available,

but various measurements with

unpolarized photons

but

polarized

nucleons were.

Using

the

hybrid

frame one could then

extract from the six available

experiments

six of the seven

amplitude parameters.

A similar

analysis

in,

say, the

all-helicity

frame would have

yielded

no

amplitude

parameter

at

all,

only

six

complicated

constraints among the seven

amplitudé

parameters.

We should remember that these considerations

apply

to

photoproduction

processes

regardless

of whether the

product

of intrinsic

parities

is + 1 or -

1,

since that switch

only

changes

the

signs

of some of the observables but not the way the observables and the

amplitude products decompose

into submatrices.

Some of these

possibilities

for the determination of the reaction

amplitudes

are shown in table VIII.

-6. The

polarization signatures

for various

dynamical

mechanisms.

The

dynamical

mechanism that has been most successful in

describing

an enormous range of data in

particle

reactions of all varieties and

energies

is the one

particle exchange (OPE)

(16)

Table VII. - The

relationship

between

secondary

observables and the bilinear

products of

reaction

amplitudes for

spin-zero

boson

photoproduction from spin-1/2 fermions,

with Lorentz invariance and

parity

conservation. The

photon

is in the

helicity frame,

the

fermions

in the

planar-transverse

optimal

frame.

For notation, see the text and the

caption of

table II. For a

note on intrinsic

parities,

see table IV.

amplitudes,

the existence of

specific

OPE leads to constraints among the

amplitudes

that reflect the

spin

and

parity

of the

exchange [14].

In the

following

we will consider those

constraints for

general amplitudes.

We will also construct the «

magic

frame »

amplitudes

for which the constraints take

especially simple

forms. In the course of this discussion the

special

properties

of the massless

photon

will be encountered.

The reaction in

question,

y + N --* 7r

+ N,

viewed in the t-channel becomes

y + p -

N

+ N with the

spin

structure

1 + 0 --> 1/2 + 1/2.

Because

helicity

0 is not allowed for the massless

photon,

there are 8

spin amplitudes,

which reduce to 4 due to

parity

conservation

(as

we assume for the remainder of this

section).

For definiteness let the t-channel reaction

amplitudes

be written as

D (a;

d,

b

),

where a,

d,

b are the

photon,

nucleon,

anti-nucleon

spin components (along

some

specific directions)

respectively,

and those

components

take the

values ± 1,

± 1 /2, ± 1 /2, respectively.

The four

independent amplitudes

will be chosen as

D( +

1 ;

+

1/2,

+

1/2 ),

D(+ 1 ;

+

1/2, - 1/2 ),

D (+

1 ;

-

1/2, + 1/2 ), D( +

1 ;

-

1/2, -

1/2 ) .

Note that

parity

allows us to choose the

complete

set of four

amplitudes

so that the

photon argument

is

always

positive.

Consider the

coupling

of a

spin

zero

exchanged particle.

At the

N

+ N vertex there can

only

be 1

unique

coupling

of the scalar or

pseudoscalar

to the

1/2

+

1/2

system.

This is also true at

(17)

Table VIII. - Some

of

the many

experimental procedures for

the determination

of

the reaction

amplitudes for

spin-0

boson

photoproduction

with

spin-1/2 fermions,

in the three

formalisms

considered in detail in this paper.

Step

# 1 :

Magnitudes only :

0 or ~ or A.

Step

#2 : Two

phases : 2022

or M or A.

Step

*3 : The third

phase :

x or + or

T.

hybrid

amplitude

for

spin

0

exchange.

For

higher spin exchange,

vector, axial vector and

beyond,

the number of

independent amplitudes

becomes

unrestricted,

i.e.

four,

although parity

conser-vation still

imposes

some additional constraints.

To

study

these various restrictions and express OPE in the most

transparent

formulation we

(18)

the

(planar)

frame for the s-channel process in which the

spins

of the external

particles

are

quantized along

the directions

given by

their

corresponding

s- to t-channel

crossing angles

[15].

More

precisely,

the

quantization

axis for

particle

A in A + B - C + D is

given by

a

counter-clockwise rotation in the

scattering plane

from the momentum direction of A

through

an

angle

X A which is the

crossing angle

for

particle

A,

and

similarly

for

particles B,

C,

D. The

magic

frame has the salubrious

interpretation

that it

corresponds

to the t-channel

helicity

frame. In that frame the

exchanged particle helicity

is conserved in its

coupling

to the external

particles

helicities

(without

any orbital

angular

momentum

component).

The

crossing angles

for the

photoproduction

reaction can be obtained from the

general

formulae of reference

[15] ;

the results are

where m is the nucleon mass, » is the

pion

mass, and s and t are the usual Mandelstam

kinematic variables. Note that because of the zero mass of the

photon,

the

crossing angle

is 0 for the

photon

for all

energies

and

angles

in the

scattering.

This leads to the

important

conclusion that the matic frame for

photoproduction always

leaves the

photon spin qùantized

along

its momentum, i.e.

helicity

is the

appropriate quantization

for the

photon.

The

magic

frame

amplitudes

with a

single spin J exchange satisfy

the

simple

factorization

equation [14]

from which it follows that

or

where the

signs depend

on the

parity

of the

exchanged particle

as well as the overall intrinsic

parity.

When these definite J t-channel

partial

wave

amplitudes

are combined with the

relevent rotation functions it is

only

relation

(4.2)

that survives since both

amplitudes

are

multiplied by

the same

dj, 0 (0,).

The final relation then becomes

This relation between the

magic

frame

amplitudes provides

a test of the

single

OPE

analogous

to the relation that has been used and tested for nucleon-nucleon

scattering [14].

The

special

case of

spin

0

exchange requires

some further

development.

To

begin

with,

(19)

constructed. For

pseudoscalar exchange

the boson vertex must have the form

E (k ) .

k’,

where k and k’ are the

photon

and

pion

momenta,

respectively.

Then the

coupling

vanishes for

photon

linear

polarization perpendicular

to the

scattering

plane, e(1- ) (k )

oc

y

oc

e +

+

e (- ).

That translates into the statement that

D (+ 1 ; d, b ) = - D (- 1 ; d, b ).

The latter is related

to

D( +

1 ;

-

d, -

b ) by parity,

so for

pseudoscalar exchange

Furthermore the

coupling

to the fermion vertex in the

magic

frame

imposes

the restriction of d =

b,

so that

D( + 1 ;

+ ,

+ ) = D (+ 1 ; - , - )

are non-zero, whereas the other 2

amplitudes

vanish. These results are correct whether the

pseudoscalar

is a

pion

or a heavier meson. Of course, when it is a

pion,

gauge invariance

requires

additional contributions

(nucleon poles

in the s- and

u-channels),

but this does not alter the

preceding

conclusions.

Lastly,

for

completeness,

we write the relations between the

magic

frame

amplitudes

{D(... )}

and the

helicity

amplitudes {Dh(... )},

,

where the

angles

are

given

from

equations (4.1).

7.

Analysis

of the

existing

data and conclusions.

One could summarize the situation of the

photoproduction

data in one sentence : there is no

energy and

angle

at which a sufficient number of different

polarization experiments

have been

carried out to allow a direct determination of the

photoproduction amplitudes,

without

dynamical assumptions.

The

existing

data can

be,

somewhat

arbitrarily,

divided into two

parts.

The old data before

1970,

starting

at the

beginning

of the

1950’s,

consisted almost

exclusively

of

unpolarized

differential cross section measurements. These data were then

analyzed

with the

help

of the

phase

shift

analogue

in

photoproduction, namely

the

multipole amplitude

series.

In this method of

analysis

it is assumed that

only

a finite number of

multipole

states will contribute to the process at the lower

energies

at which the data are

available,

and to

simplify

the

analysis

further,

the Watson theorem which links

photoproduction amplitudes

with

scattering amplitudes using unitarity

is used. This work is

by

now

old,

is limited in energy, is

constrained

by

the above

assùmptions,

and hence will not be further referred to here. The second

part

of the data are those taken after 1970. The various

experiments (other

than

unpolarized

differential cross

sections)

with

specifications

and references are listed in

table IX. In these

experiments

measurements other than

unpolarized

differential cross section

appear much more

frequently,

but

still,

the

types

of observables measured are limited.

Combining

the information of table IX with our

analysis

of the

experimental requirements

for the determination of the

amplitudes,

and,

particularly,

with the content of table

VIII,

it is easy for

experimenters

to deduce what

experiments,

and at what

energies

and what

angles,

would be the most useful to

complete

the

forming

of

complète

sets of

experiments.

In view of the marked

patterns

found in the

photoproduction amplitudes (even

if not

completely determined) by

reference

[13],

as well as the

striking

pattern

of reaction

amplitudes

found in other reactions

[16],

it would be most desirable to be able to determine

(20)

Table IX.

- Photoproduction

data since 1970. The notation

for

the observables in terms

of

the

(21)

Appendix

A. Photon

polarization

states.

The

complications

in the discussion of

photon polarization

states

originate

with the historical

fact that this

subject

was first covered in the context of classical

electromagnetic

waves, and much later in the context of the

quantized photon

as a

particle.

The two

terminologies

are

quite

different,

though

the same term

(« polarization »)

is used in both.

The

primary,

« natural » state in classical

optics

is the linear

polarization,

which denotes the E vector

pointing

in a

given

direction in the

plane perpendicular

to the direction in which the

light

wave goes. In this context the circular

polarization

state is a

secondary,

derived

quantity.

Thus here the E vector is

pictured

as

« polarized

».

In contrast, the « natural » states in the

description

of the

photon

as a massless

particle

of

spin

1 are the two

helicity

states, that

is,

the states in which the

spin

of this massless

particle

points

in the direction of

propagation

or

opposite

to it. As it turns out, these

primary

states

correspond,

in the classical

picture,

to the

secondary

states of circular

polarization,

whereas

the

primary

states of the classical

picture (the

linear

polarization states) correspond

to

composite,

quasi

fictitous states in the

particle

framework. We see that in this

particle picture

it is the

spin

of the

particle

that is

pictured

as

being

«

polarized

».

One can,

nevertheless,

construct the translation from one

language

to the

other, since,

after

all,

there can be no essential difference between the two. We will now review this

correspondence

between the two

terminologies

and also connect them with the states used in the

language

of the

optimal

formalism.

Let us denote the direction of

propagation

of the

photon

as z, and the two directions

perpendicular

to it as x and y, so x, y and z form the three axes of a usual Cartesian coordinate

system.

In classical

optics,

then,

we denote

by

x

and ÿ

the linear

polarization

states of the

photon

in the x

and y

directions.

We will also introduce the

angle .0

to describe the direction of a

plane polarized photon (in

the x-y

plane)

in such a way that in the x

direction 0 =

0,

and in

the y

direction

.0 =

90

degrees.

A

plane polarized photon

in

the 0

direction can then be described as

Still in this classical

optical terminology,

the circular

polarization

states are

complex

linear

combinations of the

plane polarized

states.

Denoting

the

right circularly polarized photon

as

e(+ ),

and the left

circularly polarized photon

as

e (-

),

we have

These relations can of course be inverted to

give

Now we turn to the

particle description

of the

photon,

in which

by density

matrix

of a spin-1

particle

is,

in

general, given by

a

3-by-3

matrix. For a massless

spin-1 particle (and,

for that matter, for any massless

particle

of

arbitrary spin),

the

density

matrix reduces to a

2-by-2

matrix,

which is best

given

in the

helicity

frame. In

it,

the

density

matrix of a

photon polarized

(22)

Table A.1.

- Summary

of photon

polarization

states in the two

terminologies

of

classical

optics

and

quantized

particles.

P p

and

Pc

denote the

degree

of planar

and circular

polarization,

respectively.

The notation

of

In contrast, the

density

matrix for a

circularly polarized photon

is

where

P, is

+ 1 for

right

and - 1 for left circular

polarization

of maximum

degree,

that

is,

for

(23)

We can see from these two

density

matrices that the + + state of the

optimal

formalism

correspond

to a

right circularly polarized photon,

while the - - state to a left

circularly

polarized photon.

We can also

identify

the Re

(+ - )

and Im

(+ - )

states now with

linearly

polarized

states. In

particular,

for a

photon plane polarized

in the directions

of c/J = 0,

180,

360,

etc.

degrees

we

get -

Re

(+ - ),

for

plane polarization

in the directions of

c/J = 90,

270,

etc.

degrees

we

get

+ Re

(+ -

),

for

plane polarization

in the directions of

c/J =

45,

225,

etc.

degrees

we

get

+ Im

(+ -

), and

for

plane polarization

in the directions of

c/J = 135, 315,

etc.

degrees

we have - Im

(+ - ).

Possibly

at the risk of further

confusing

the

issue,

we

might

mention that for a massive

spin-1

particle,

the state in which the

particle

is

polarized

in the x direction is described

(in

terms of the three states with the

quantization

axis in the direction of

propagation)

as

This reduces to our

previous expression

for a

photon

because the

photon

does not have a

e ( 0 )

state

(and

hence the normalization factor

2 1/2

also

changes

to

2).

The results of this discussion can be summarized in table

A.l,

in which the three

customarily

used direction

designators

(L

for

longitudinal,

i.e. z in our

notation,

S for

sideways,

i.e. x in our

notation,

and N for

normal,

i.e. y

in our

notation)

also appear.

In this last context it is

important

to note,

however,

that the L-S-N notation is

meaningful

only

when the

photon

is considered in a reaction in which the reaction

plane

is

defined,

whereas the rest of the above discussion

applies

also to a

single photon

which is not

part

of the reaction. The results of the

table, therefore,

as far as

they pertain

to the connections between L-S-N and x-y-z rest on the convention of

identifying

S

with 0 =

0.

An observation of considerable

practical

interest can be derived from the above results. In

terms of the

optimal

formalism,

+ + and - - are

primary

observable

arguments

for the

photon,

but it turns out that these are at the same time also

secondary

observable

arguments

in that

they

denote

circularly polarized photons

which can be created in actual

experiments.

The consequence of this is the

general

statement that in reactions

involving

photons,

experiments involving

circular

polarized photons

are related to the

amplitude products

in a

way which is

simpler

than it is the case for

linearly

polarized photons,

and thus

efforts

should

always

be made to have

circularly polarized photons

available,

since

they yield simpler

information.

References

[1]

For this,

by

now classical, area of

particle physics,

see for

example

BETHE H. A. and DE

HOFFMANN F., Mesons and Fields, Vol. II, Row Peterson

(1955)

or G. Kallen,

Elementary

Particle

Physics (Addison Wesley, 1964).

[2]

For

example

SLAC, Cornell, Bonn,

Orsay,

Frascati, Kharkov and Bates.

[3]

See for

example

CHAU Y. C., DOMBEY N. and MOORHOUSE R. G.,

Phys.

Rev. 163

(1967)

1632.

[4]

MORAVCSIK M. J.,

Phys.

Rev. 104

(1956)

1451 ;

KNAPP E. A., KENNEY R. W. and PEREZ-MENDEZ V.,

Phys.

Rev. 114

(1959)

605.

[5]

See for

example

WALKER R. L.,

Phys.

Rev. 182

(1969)

1729.

[6]

GOLDSTEIN G. R. and MORAVCSIK M. J., Ann.

Phys.

N. Y. 98

(1976)

128.

[7]

MORAVCSIK M. J. and GOLDSTEIN G. R.,

Phys.

Rev. D 31

(1985)

2986,

appendix.

[8]

GOLDSTEIN G. R. and MORAVCSIK M. J., Ann.

Phys.

N. Y. 142

(1982)

219.

[9]

JACOB M. and WICK G. C., Ann.

Phys.

7

(1959)

404.

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