Self-similar solutions for A- dependences in relativistic nuclear collisions in the transition energy region. A.A.Baldin
Jan 04, 2016
Self-similar solutions for A-dependences in relativistic nuclear collisions in the
transition energy region.
A.A.Baldin
One of the most important problems nowadays, formulated by a distinguished scientist S.Nagamia in 1994, is the determination of the conditions in which hadrons lose their identity, and sub-nucleonic degrees of freedom begin to play a leading role.
A.M.Baldin proposed a classification of applicability of the notion “elementary particle” on the basis of the variable bik introduced by him.
12122
ki
kikikikiik mm
ppEEUUUUb
1ch212 ikkiik UUb
• the region
relates to non-relativistic nuclear physics, where nucleons can be considered as point objects;
• the region
relates to excitation of internal degrees of freedom of hadrons;
• the region
should, in principle, be described by quantum chromodynamics.
2100 ikb
1~ikb
1ikb
PDG
0.1 1 10 100
101
102
tot
[mb]
b12
pp
-p
+p
K. Hagiwara et al., Phys. Rev. D 66, 010001 (2002) (http://www-pdg.lbl.gov/)
• PDG
0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0
101
102
QCD -> transition region<-nucleon physics
tot
[mb]
pp
p p K-p
K+p
K. Hagiwara et al., Phys. Rev. D 66, 010001 (2002) (http://www-pdg.lbl.gov/)
V.Burov at.al. Phys.Lett. B67:46,1977 , PEPAN,15:1249-1295,1984
Cumulative ProcessesCumulative Processes
Structure of the nuclei at short distances
33
3 3
2/ 2 3 3( 1)
1 2 3 4
3
0
3( ) ( )
(2 )
( ) ( ) ; ( / ) ;
10
1, 5%, 0.3%, 0.
0.75 ;
0
1
(180 )
2
,
.
2%
1
f
f
k kk
p
ff
i rk kk k
p
p
f
E GeV T GeV
pp
p
ddEd p
r e d r r r r fm
p A X
dE p pd p
m
X
f
3M
1
11 A
PX
2
22 A
PX
,...,,,,,, 3331221 ihhPSAA
( ) ( )' 'X m u X m u M u X m u X m u M ukk
k1 0 1 2 0 2 3 32
1 0 1 2 0 24
2
ij i j i j i ju u P P M M /
21
122122
21 2
2
1 XXXX
Ed
d pC A A fX X
3
3 1 1 21 2
Self-similarity is a special symmetry of solutions which consists in that the change in the scales of independent variables can be compensated by the self-similarity transformation of other dynamical variables.
This results in a reduction of the number of the variables which any physical law depend upon.
The relationship between X1 and X2 is described by the laws of conservation written in the form
Here Mn is the nucleon mass, and M3 the mass of an emitted particle. Essentially, we are using an experimentally proved correlation depletion principle in the relative four-velocity space which enables us to neglect the relative motion of not detected particles, namely the quantity
in the right-hand part of the above equation. Employing this approximation, the correlation between X1 and X2 can
conveniently be written in the form
In the case of production of antiparticle with mass M3, the mass M4 is equal to M3 as a consequence of conservation of quantum numbers. In studying the production of protons and nuclear fragments M4 = M3 as far as minimal value of corresponds to the fact that any other additional particles are not produced. The X1 and X2 obtained from the minimum are used to construct an universal description of the A-dependencies.
The analysis of the experimental data shows that the A-dependence of the inclusive production cross section can be parametrized by a universal function , were X is equal to X1 and X2 , respectively.
X M u X M u M u M X u M X u M un n k kk
1 1 1 2 2 2 3 3
2
1 1 2 24
2
2 11
kl k lk
M M
X X XM
M
M
MX
M
M
M
M
M M
Mp p p p p1 2 12 1
313
42
323
4 42
32
12
0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.01E-10
1E-9
1E-8
1E-7
1E-6
1E-5
1E-4
1E-3
0.01
0.1
1
10
45 Gev 159o
Al Ti Mo W
10.14 GeV 97o
Al Cu Ta
inv A
11 A
22
[mb G
ev -
2 c3
sr -
1 ]
Cumulative processes
S.V.Boyarinov, et al. Yad. Fis. , v.57, N8, (1994) ,1452-1461.
O.P.Gavrishchuk et al. Nucl. Phys., A523 (1991) 589.
0.5 1.0 1.5 2.0 2.5 3.010-7
10-6
10-5
10-4
10-3
10-2
10-1
100
101
102
103
inv/A
1 1 A2 2
[mb GeV
-2 c3
sr-1 ]
p+C->
150
350
450
600
800
1200
p+Al->
970
p+W-> 970
1.5 2.0 2.5 3.0 3.5 4.0 4.510-10
10-9
10-8
10-7
10-6
10-5
10-4
10-3
10-2
10-1
in
v A
1
1 A
2
2 [
mb
Gev
-2 c
3 sr-1
]
_ _ A+A--->P,K+... _ GeV/n Angle P
dC 3.65 24o
CC 3.65 24o
CCu 3.65 24o
SiSi 2.0 0o
SiSi 1.65 0o
_ K
dC 2.5 24o
CC 2.5 24o
SiSi 1.0 0o
SiSi 1.4 0o
SiSi 2.0 0o
CaCa 2.0 0o
Twice cumulative
Jim Carroll Nucl. Phys. A488 (1989) 2192.A.Shor et al. Phys. Rev. Lett. 62 (1989) 2192.A.A.Baldin et al. Nucl. Phys., A519 (1990) 407.A.A.Baldin et al. Rapid Communications JINR, 3-92 (1992) 20.
1.5 2.0 2.5 3.0 3.5 4.0 4.510-10
10-9
10-8
10-7
10-6
10-5
10-4
10-3
10-2
10-1
in
v A
1
1 A
2
2 [
mb
Gev
-2 c
3 sr-1
] _ _ A+A--->P,K +...
_ GeV/n 0o
P NeCu1.9 NeSn1.89 NeSn1.69 NeBi1.87 NiNi1.85 NiNI1.66
_ K
NeCu1.9 NeSn1.89 NeSn1.69 NeSn1.49 NeBi1.87 NiNi1.85 NiNi1.66
Twice cumulative
A.Schroter et al. Z.Phys. A350, (1994), 101-113.
0.5 1.0 1.5 2.0 2.5 3.0 3.510-10
10-9
10-8
10-7
10-6
10-5
10-4
10-3
10-2
10-1
100
101
102p(240 GeV)+Be--->h +... (0o)
p anti p d anti d
t ( 3He)
anti t ( 3He)
iv
n A
1 A
2
[m
b G
eV -2 c
3 s
r -1 ]
Antimatter production
0.5 1.0 1.5 2.0 2.510-3
10-2
10-1
1
10
102
103
104
in
v/A1 A
2
12C+181Ta 3.65 GeV/n
100,350,450,600,1000,1200
20Ne+64Cu,119Sn,209Bi 1.5-1.9 GeV/n
58Ni+58Ni 1.7-1.9GeV/n 00
0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 1.6
10-4
10-3
10-2
10-1
100
10-4in
24Mg+24Mg----> <N>=8.24
50
150
250
350
450
600
800
1000
1200
1500
inv/A
1 A
2
A.A.Baldin, E.N.Kladnitskaya, O.V. Rogachevsky, JINR Rapid Comm., (1999), N.2 [94]-99, p.20.M.Kh.Anikina, et al., Phys. Lett. B., (1997), v.397, p.30.
1.0 1.5 2.0 2.5 3.0
1
10
y
A+A ----> P +X 0o
Si+Au Si+Cu Si+Al
ivn
[mb/
GeV
2 /
c 3 ]
Rapidity (Lab Frame)
P.Stankus et al. Nucl. Phys. A544 (1992) p .603c-608c.
0.5 1.0 1.5 2.0 2.5 3.0
10-5
10-4
10-3
10-2
10-1
Au(25GeV/u)+Au->J/
inv
y
100
150
10
conclusion
• The proposed self-similar solution quantitatively describes the angular, energy and A- dependences of inclusive production cross sections of all hadrons with transverse momentum up to 2GeV. For higher transverse momenta the A-dependence becomes a function not only of X1, X2, but also of Рt (or mt).
• The analysis of inclusive spectra for the data selected in different ways shows that multiplicity in relativistic nuclear collisions has its origin basically in independent nucleon-nucleon interactions. Thus, high multiplicity at interaction of heavy nuclei is not a satisfactory criterion for search and study of collective interactions, or detection of exotic states of nuclear matter (such as quark-gluon plasma).
• It is natural to consider two types of collectivity in nuclear-nuclear collisions: the first is related to production of particles in the region kinematically forbidden for single nucleon-nucleon interactions (X1 or X2 or both greater than unity); the second is a result of collectivity of the initial state in nucleus-nucleus collisions) – high probability of a large number of independent nucleon-nucleon interactions in the collision. The analysis of multiple experimental data on the basis of the proposed self-similarity approach allows to conclude that the effect of the collectivity of the first type drops drastically with increasing energy of colliding particles and increases with increasing mass of the produced particle.
2
331
233
1
113
3
exp21
CAACpd
dE
XX
• Collective effects of the first type (cumulative) “die out” with increasing collision energy. Therefore, in order to investigate subthreshold processes, it is necessary to optimize the combination of the nucleus mass and energy to provide sufficient number of nucleons, on the one hand, and avoid
extra multiplicity, on the other hand.
21
122122
21 2
2
1 XXXX
We must remember that what we observe is not Nature itself, but Nature which uncovers in the form in which it is revealed by our way of putting questions. Scientific work in physics consists in putting questions about Nature in the language we use, and trying to get an answer in experiment performed by the means (tools) we have.
At that the words of Bohr about quantum theory come to mind: if harmony in life is sought for, one should never forget that in the game of life we are spectators and players at the same time.