Pionic bremsstrahlung in heavy-ion collisions

Pionic bremsstrahlung in heavy-ion collisions

291~ Nuclear Physics A428 (1984) 291~304~ North-Holland, Amsterdam PIONIC BREMSSTRAHLUNG IN HEAVY-ION COLLISIONS+ David VASAK Gesellschaft fir Sc...

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291~

Nuclear Physics A428 (1984) 291~304~ North-Holland, Amsterdam

PIONIC BREMSSTRAHLUNG

IN HEAVY-ION

COLLISIONS+

David VASAK Gesellschaft fir Schwerionenforschung, 6100 Darmstadt 11, West Germany

PlanckstraRe

1, Postfach 11 05 41,

, Berndt MILLER, Thomas STAHL and Mark UHLIG,

Walter GREINER*

Institut fiir Theoretische Physik der Johann-Wolfgang-Goethe Robert-Mayer-StraRe 8-10, Postfach 11 19 32, 6000 Frankfurt am Main 11, West Germany

Universitat,

We apply the bremsstrahlung model for pion production to symmetric nuclear collisions at energies far below the single NN-threshold. All main features of recent neutral pion measurements can be explained by a single value of the deceleration parameter of the theory which is consistent with hydrodynamica1 calculations. Since the y-ray bremsstrahlunq also reflects the kinematics of its source, a simultaneous measurement-of pion and Y-ray bremsstrahlung should be used to further test the collision dynamics. Results of our calculations for both kinds of radiation are presented. An extension of this approach to asymmetric systems is proposed.

Subthreshold recent years,

pion production particularly

(or cooperative)

has become of considerable

effects. The idea to consider

anism for the production

of secondary

a bremsstrahlung-type

particles

not newl. If this model can be shown to describe collisions

In the following we apply the bremsstrahlung

2 do A=q dsldE

pion production

'

I =--(I 3 '

about the time develop.2 nuclei .

model to collisions

threshold

of equal

for pion production.

cross section for radiation of neutral pions is

to the Fourier-transformof

d2n 71 dodE

is

in nuclear

structure of the colliding

nuclei far below the single nucleon-nucleon

proportional

mech-

in hadronic collisions

it carld be a useful source of information

ment of the reaction and the spin-isospin

The inclusive differential

interest during

in connection with the search for cumulative

1 I; 3 II

P

the current density.

? ': sP,sT

' 13k(p)?

(1)

k

fsupported by the Bundesministerium fir Forschung und Technologie. "Invited Speaker at the Conference on Theoretical Approaches to Heavy Ion Reactions Mechanisms, Paris, 14-18 May 1984

0375-9474/84/$03.00 0 Elsevier Science Publishers B.V. (North-Holland Physics Publishing Division)

292c

D. Vasak et al. / Pionic bremsstrahlung

in heavy-ion collisions

with n L

_C_ clj (PII*=; k

‘TSP

$

k

I*WT(A) *W,(A)]*

IK(p)I*

(2)

where E is the pion energy, p = (E*-m*)l'*, m = 135 MeV the mass of the neutral pion, M = 930 MeV that of a bound nucleon and o the pion solid angle. The pion 2 nucleon coupling constantgohas the usual value go /4~ = 14. Averaging over the spin direction

fi of both nuclei

(i = P projectile,

i = T target) is indicated

by i. The index k runs over the three isospin values of the pion; the factor l/3 in (1) and (2) accounts

for the fact that (1) describes

only one sort of

pions, in this case the neutral ones. For equal nuclei the factor cl0 has been set equal the geometrical

cross section 4nR2 with R being the half-density

radius of the gaussian density P(r) = '7~~ exp T-(r/*a)*l of the colliding

nuclei

n = P/p, the compression, condition).

(3)

(p, = 0.17 fm l/a = &

-3

is the normal nuclear density and

(o/A)~'~

is obtained

from the normalization

In

K(P) = z i=P,T

+I- [C(pi) ("i'p)/(ui'p)l' - 0)

exp[i(Et-c.iti(t))ldt

(4)

(prime denotes total time-derivative) all the information

about collision

are the (linear) trajectories system, parametrized multiple

dynamics

is contained.

$(t)

= +R(t)gz

of the nuclear centers in the center-of-mass

by the deceleration

of the "passing time" T

time T. We express T as a unique

= R/(2yin

vin), where

vin is the initial

c.m. velocity and yin = (l-v:,) -S1'2, i.e.,

T

=

with an

v*

(5)

S

adjustable

energy-independent

parameter

u.

0: the spin-vectors

boosted from the ' are the corresponding four-velocities, 'i particle's rest frame into the c.m. system, and z(p) the Fourier-transform of (3) with BT(t) = I$]* - (S.Gi(t)* taking time-dependent

Lorentz-contraction

(5) into account. The statistical

factors

D. Vasak et al. / Pionic bremsstrahlung in heavy-ion collisions

WS(A) and WT(A) result from single statistical spin-isospin-strength fluctuations

wS

estimation

293~

of the nuclei's

to which the pions couple and which is non-zero due to

during the collision

(see below).

In ref. 2 we have used

= WT ZJFi-. 7

(7)

The parametrization hydrodynamical

used here was strongly motivated

calculations

which show excellent

by the results of

agreement with the experimental

findings even at low energies.

In fig. 1 the calculated3proton

compared with the experimental

yield from a I2c + Ig7Au collision

spectrum

is

at 84 MeV/n.

A short remark to the role of the spin

z c

'2C+197A" 84MNn II'-

-

Experiment

----

Theory

2 E E 5

density is appropriate:

In the schema-

tic approach of ref. 2 it was assumed that the spin vectors of the projectile and target are not correlated This assumption

addition of the pion yields

II'-

at all.

leads to incoherent from both

nuclei. On the other hand, in the hydrodynamical collisions

picture of heavy ion

the nucleons

tion zone, consisting

l-

nuclear matter,

in the reac-

of hot compressed

do not "remember"

their origin. Thus there is only one spin direction,

lo-'-

I

0

and the pion yields

should be added coherently. I

I

100

50

[MeVI, 1 150

FIGURE 1 Comparison of the present theory and the ex erimental data for 12C(84 MeV/nucleon) + P g7A~+p + x. Full lines correspond to the experiment; dashed lines represent the calculations (from ref.3).

coherent addition pion production

at 90' in the c.m.

system, in case of coherence tive interference forward-backward

sideways

angular distribution

of pion radiation

appear preferably collisions

is a consequence

take place and lead to occupation addition

in the

and gives a In fact, a

of spin fluctuations4,

in the reaction zone, where the individual

light, the coherent

a nega-

leaves a

enhancement

smaller total pion yield. non-zerosource

While in-

leads to enhanced

which

nucleon-nucleon

of vacant states. Seen in this

is the natural one.

In order to avoid complications

caused by the Coulomb force when looking at

charged pion data5 we compare our calculations6

(cf. fig. 2) with recent ex-

periments on neutral pion production 7,8,9 . The measured pion angular distributions exhibit a forward-backward

behaviour

and thus favour the coherent addition

294~

D. Vasak et at. / Pionic ~rems~tra~l~ng in heavy-ion collisions

0

-1.0 -0.5

0 0.5 cos~~c‘m,l

50 100 150 200 pion cm. beg

0

1.0

FIGURE 2 (a) Theangulardistribution forpions produced at 84 MeVin in the energy region O-50 MeV (top), 50-100 MeV and loo-150 MeV, respectively. The data are from ref. 7. (b) The angle-integrated spectra at ion energies between 20 and 84 MeV/n. (c) The excitation function. The data are taken from refs.7 (solid dots),5 (open circles), 8 (open triangles), 9 (solid triangles), and 10 (solid squares). The dashed line exhibits the thermal pions. of the pion yields

from the projectile

and target nuclei: in fig, Z(a) the experimental

pion angular distribution

are compared with our results. The7 dashed curve in the upper energy cut is obtained by incoherent addition the deceleration adjusted

(here

has been

to v = 0.55). The solid lines show the results from coherent addition.

In this case the parameter negative

parameter

interference

v = 0.38 is somewhat smaller to c~pensate

mentioned

above.

clude that the spin distributions correlated

of the participating

or, in other words, that deceleration,

matter and pion production ent, the compression

are simultaneous

nuclei must be closely

creation of compressed nuclear

processes. Therefore,

to be consist-

has also to be taken into account by estimating

ence of the compression

on bombarding

for the

In the framework of our model we con-

energy from hydrodynamical

the depend-

calculations3,

295~

D. Vsak et al. / Pionic bremsstrahlung in heavy-ion collisions

although the validity of these results is questionable carbon and for energies

for nuclei as small as

as low as 20 MeV/n, where the mean free path of the

nucleus is large due to the action of the Pauli principle. Because the deceleration contribution

by the Coulomb force is very long range, its

to pion radiation

part of the available

is much less, but it takes away a considerable energy for heavy nuclei 2? We thus subtract the

scattering

energy Ecoul = ZpZT~Y/2R from the bombarding

In fig. 2(b) the experimental shown to coincide

energy Elab.

and theoretical

angle-integrated

in shape as well as in magnitude.

spectra are

The exponential

decay of

the cross sections with growing pion energy reflects the influence of the deceleration

as well as that of the gaussian form-factor,

the reaction zoneII. parameter

v is kept fixed at the value 0.38. At higher bombarding

experimental

is much

yield

other production isobarsI

mechanism

to contribute

too high. This is not surprising,

like the thermal production

Still, we find excellent

agreement with the pion production after these calculations

Ridge-GSI

collaboration"

GANIL8 (the yields are renormalized

and from Ar + Ca measured at 839 to be comparable

(dashed line) has been calculated

the upper bound for the thermal pion 12 with a hard in the shock-wave model

equation of state (Fermi gas) in which the temperatures higher than in the hydrodynamical 4T = ucl3

Rz

pound nucleus. Thermally

and the densities

d3p (2n)3

radius and T the temperature

created pions are obviously

of the compressed

negligible

low energy regime. The sum of the thermal and bremsstrahlung an overall quantitative An interesting

description

possibility

A classical

formula,

of the available

com-

in the very

pion yields gives

experimental

to test the time development

process would be a simultaneous

are

model:

7 [exp (E/T)-I]-' 0

where R, is the half-density

from a N + Ni

were already available

for the A-dependences

with the carbon data). For completeness,

otherm II

the deceleration

from the value v = 0.38 used at low energies.

collision at 35 MeV/n measured by the Stony Brook-Oak

energies the

since we expect

from highly excited

to the total pion yield. Moreover,

parameter may be different

yield

i.e., the shape of

In fig. 2(c) the pion excitation function is shown. The

data.

of the collision

measurement

of pion and y-ray bremsstrahlung8. 13 similar to (l), holds also for photons : z x f#) 1 exp [iw(t-z.Ei(t))ldt12 l-i;.;i(t)

(9)

296~

D. Vasak et al. / Pionic bremsstrahlung in heavy-ion collisions

where w is the photon frequency

and ?i the direction

of emission. Until now this 14 where also experimental

formula has been applied to low ion energy collisions

data15 exist. Our results, using the same nuclear trajectory duction, are presented

in fig. 3. If

move on a straight line the yield in the forward direction at 90' (c.m.) for symmetric differential

as for pion pro-

the sources of electromagnetic

radiation

is zero as it is

systems. These minima are clearly seen in the

cross section in the laboratory

intensity of high energy photons

system (fig. 3(a)). A significant

(25 MeV_'05 150 MeV) is predicted

(cf. fig.

3(b)).

*NJ3 s

15

c 5 E

10

3 B b

5 n 7.0

-0.5

0 0.5 cos kriaJ

10

u.

50 100 photon lab ekgy(MeV)

FIGURE 3 (a) The photon double-differential (b) The angle-integrated cross section at 84 MeV/n in the lab. in the lab.system. system. Recently, systems8.

photon bremsstrahlung

only. The reason is twofold:

the nuclear trajectories collisions

- the dependence

of the velocity

Firstly, our parametrization

of the deceleration

extrapolated parameter

T on the mass numbers

of refs.2and

Since, as shown above, 'the significant

the shape

of the total linear momentum

if AR = AT. To overcome these difficulties

trajectories

of

to asymmetric

nuclei has to be worked out. Secondly,

function must ensure conservation

during the collision the parametrized

model has been applied to syne-

cannot be unambiguously

AR and AT of the participating

y-ray spectra

spectra have been measured with asymmetric

But, up to now, the bremsstrahlung

tric collisions

150

6 by a classical

contribution

of the

we replace

dynamical model

16

.

29%

D Vasak et al. / Pionic bremsstrahlung in heavy-ion collisions

bremsstrahlung relativistic

pions occurs

concepts

in the low energy region only, we may apply non-

like friction etc.. We describe

nuclei by means of four collective

the collision

of two

degrees of freedom r, 8, eI and e2 (see

fig. 4), freezing all other collective

modes (e.g. surface vibrations). The corresponding

Lagrangian

L=${~;*+~r

2 ,$2

+ II 6: t I2 6;

is

1

(10)

- Vi') - V,(r) with the reduced mass p of the nucleus, moments of inertia II, I2 and the Coulomb and nuclear potentials

V,(r)

and V,,,(r)given by the folding integrals

Vi(?) = j d3rI' j d3r2' oI(?I')

x Q;-;,t;,) FIGURE 4 Definitions employed.

interaction

and a short range nuclear

iN

(r)

z-vo

(II)

i = 0,M

of the degrees of freedom

of a long range Coulomb

p,(Q

17

interaction

approximated

by a gaussian

18

,-(rlr0)*

(13)

V, = '2.36 MeV, r. = 2.3 fm with the overlap of the nuclear densities. The coupling to microscopic dependent

+ FI(r) = - K J rqP') &ere

v~,

degrees of freedom is accomplished

by a velocity

friction force

v2

- ;*(;')I p2(?-F)

are the velocity distributions

of the nuclei 1 and 2. The universal

pI(

d3r' = -;,(r)

(14)

and pI,p2 the density distributions

constant

K is the coefficient

of friction.

298~

LX Vasak et al. / Pionic bre~~~ahI~ng

in heavy-ion collisions

0.3 0.2 0.1 I

Oo

FIGURE 5 The c.m. velocity function$(t)]of a carbon nucleus in a symmetric collision at 50 MeVln as calculated in the dynamical model (solid lines) for zero impact parameter. With the value ~10~ ~eV.f~of the coefficient of friction the previously used form parametrized by T (dashed line) is well reproduced (up to a time-shift). Small friction (~=2000 MeV.fm2) gives rise to smaller decelerations. For b=1.6 fm the velocity component vz along the beam axis and vx perpendicular to it are also plotted (dotted lines).

In fig. 5 some results of the dynamical model are shown. For the impact parameter b=O the dynamical model indeed can reproduce ries. Furthermore,

the classical

also for impact parameters

collision

b (dotted lines).

we are now in the position to generalize

kinematics

I, The parameter

trajecto-

b # 0. The slope of the velocity function can be

seen to decrease with increasing Therefore,

the parametrized

dynamical model allows to find trajectories

the description

of the

in three respects:

T, which in principle

by a single parameters

depends on A p, AT and b, is replaced

, the coefficient

of friction.

2. The total cross section

is obtained

unambiguously

from

~1~ = 1 n* (b) b db rather than from u

*

= 0d.n

f (c.f. eq. (1);~~ is effectively

as used previously it has physically 3. The motion

reasonable

a parameter,

although

values).

of nuclei in collisions

at these energies

(down to, e.g. 20 MeV/n)

does not occur along straight lines, when b # 0. The contribution collisions

to the total cross section and their influence

distribution

could not be accounted

linear trajectories

for in the old modelzy6,

were allowed. Now even cases

nuclei stick together

nuclei we are forced to reconsider ations

(to firstorderboth,

statistical

can be included!

from collisions

the statistical

of unequal

model for isospin fluctu-

spin and isospin, can be described

model since it is based on the group structure

We propose the following

where only

where the participating

forming a rotating nuclear molecule

To apply these dynamics to pion bremsstrahlung

of such

on the angular

by the same

only).

picture:

the system of m participating nucleons in the collision gives rise to a non-zero mean isospin value T (m) which is completely determined by vector addition

rules. The computation

is quite easy if one benefits

[n/2, n/2 > x 11/2,1/2 > = (tl) I(ntl)/2, (n+1)/2 > of the Clebsch-Gordan

from the property

n = 0,1,2,...

(15)

coefficients.

A system of Z protons and N neutrons with total isospin T' according

(Z+N=m) can then be coupled to states

to

/Z/2, Z/2 ' x /N/2$4/2 > = 1 am(T')!T;(Z-N)/2 >

(16)

T' where

4T')

=

1(1/2,

can be interpreted

N/2,+T'I Z/2.-N/Z, as the probability

(z-~)/2)1' for the state

(17) IT',$%.

The mean isospin is defined simply by 7 (m) = 1 T'

a,(T') T'

(18)

3ooc

D. Vasak et al. 1 Pionic bremsstrahlung in heavy-ion collisions

In fig. 6 this expression is plotted against m (long-dashed line) for symmetric systems

(N = Z = m/Z), We see that the mean isospin may be approximated

quite

well by Y(m) = vm/3. Now we have to connect m, the number of participating numbers, Ap and AT , of the collision central symmetric

heavy-ion

partners.

collisions

nucleons with the mass

Under the assumption

all nucleons

participate

that in

we have

m = Al, + AT = 2A. The resulting

(20)

value WT = r(A) = V2A/3.

is somewhat modification

(21)

greater than the value in eq. (7) (this will lead to a slight of the parameter

v). For asymmetric

systems or/and non-zero

parameters we simply have to replace m by an effective

impact

number of participbnts,

i.e. m = AFff (b) + AFff (b)

(22)

with suitably chosen function Aieff (b). Because the final T3 component

is fixed by half the neutron excess

eq. 6) and T' cannot be smaller than 7. The dash-dotted

fine in fig. 6 displays r(m) for various realistic

when all involved nucleons excess this enhancement

participate.

for those

of

systems

It can be seen that for a large neutron

can be quite dramatic,

ment for pion bremsstrahlung

(c.f.

ITSI, N>Z gives rise to an enhancement

resulting

combinations

in a similar enhance-

of colliding

nuclei.

We conclude that 1. In particular

at low bombarding

can help to understand

energies

the bremsstrahlung

the (synnnetric) pion production

Within our bremsstrahlung

mechanism

cross section.

model the II'-data of refs. 7,8 and 9 can be

explained with the unique deceleration eration is similar to that obtained

parameter

v = 0.38. The decel-

from nuclear hydrodynamics3.

Other

pion production mechanisms 12,1g are suppressed in this enerqv reaime. 2. The forward-baclanardpeaking of the experimental angular distributions iS quantitatively

explained,

target are coherently threshold

if the pion radiation

added, supporting

pion production.

from the projectile

the cooperative

and

nature of sub-

301c

D. Vasak et al. / Pionic bretnsstrahlung in heavy-ion collisions

Number of h-ticipants

m

FIGURE 6 The mean isospin value T(m) is plotted as a function of the number of participants m for systems with N=Z. The dashed line gives the exact result according to eq. (18), which can be approximated by m (full line). To indicate the maximal possible isospin T = m/2 is drawn. With realistic target and projectile combinations all available nucleons coupled together (m = AP+AT) the dash-dotted curve is obtained. Significant deviations from the symmetrical case occur for m r 150. 3. Information contained

about the time-development

in electromagnetic

v-radiation

also processes

check the underlying

of the collision process is also

processes.

We therefore suggest that besides

such as electron

collision

emissions can be used to

dynamics.

4. To investigate

asynnietric collisions

and the A-dependence

bremsstrahlung

a slight modification

of the so far used parametrization

of the nuclear trajectories tical estimate

of the pion

is proposed together with an improved statis-

for the spin-isospin

strength.

Numerical work along these

lines is in progress. We thank G. Buchwald; G. Graebner and J. Maruhn for providing us with their results. We also acknowledge discussions with P. Braun-Munzinger, E. Grosse, J. Julien, Ch. Michel, H. Nell, F. Obenshain and P. Paul and are grateful that they made their data available to us prior to publication.We are grateful for a stimulating discussion with C.S. Warke.

D. Vasak et al. f Pionic ~remss~rahI~~~in heavy-ion cotIisions

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713.

G. Soff, J. Reinhardt, B. MUller and W. Greiner, Z. Phys. A 294 (1980) 137, and private communication.

21) Nevertheless we expect pion bremsstrahlung also from Rutherford trajectories as long as the total energy is above the pion threshold. It% should be observable in, e.g., U+U collisions at (or slightly below) the Coulomb barrier. There is also the process of fusion of nuclei by pion emission, allowing for the production of rather cold compound nuclei. This process was first predicted many years ago by M.G. Huber and his collaborators.(K. Klingenbeck, M. Dillig and M.G. Huber, Phys. Rev. Lett. 47 (1981) 1654).