-
1
-
-
34247577572
-
QM05 Proceedings
-
Compare NUPABL 0375-9474
-
Compare QM05 Proceedings, Nucl. Phys. A774 (2006); NUPABL 0375-9474
-
(2006)
Nucl. Phys.
, vol.774
-
-
-
2
-
-
0037060611
-
-
for specialized reviews, see also NUPABL 0375-9474 10.1016/S0375-9474(01) 01350-1
-
for specialized reviews, see also K.J. Eskola, Nucl. Phys. A698, 78 (2002); NUPABL 0375-9474 10.1016/S0375-9474(01)01350-1
-
(2002)
Nucl. Phys.
, vol.698
, pp. 78
-
-
Eskola, K.J.1
-
3
-
-
0031644837
-
-
or PPNPDB 0146-6410 10.1016/S0146-6410(98)00058-1
-
or S.A. Bass, Prog. Part. Nucl. Phys. 41, 255 (1998). PPNPDB 0146-6410 10.1016/S0146-6410(98)00058-1
-
(1998)
Prog. Part. Nucl. Phys.
, vol.41
, pp. 255
-
-
Bass, S.A.1
-
4
-
-
0001663103
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.3.181
-
G. Goldhaber, Phys. Rev. Lett. 3, 181 (1959); PRLTAO 0031-9007 10.1103/PhysRevLett.3.181
-
(1959)
Phys. Rev. Lett.
, vol.3
, pp. 181
-
-
Goldhaber, G.1
-
5
-
-
23544448704
-
-
PHRVAO 0031-899X 10.1103/PhysRev.120.300
-
G. Goldhaber Phys. Rev. 120, 300 (1960). PHRVAO 0031-899X 10.1103/PhysRev.120.300
-
(1960)
Phys. Rev.
, vol.120
, pp. 300
-
-
Goldhaber, G.1
-
6
-
-
32644452928
-
-
In fact, at the beginning the observed effect was called GGLP effect in distinction to an apparently similar effect observed in astronomy and known as HBT effect which was used to obtain stellar dimensions, see IMPEER 0218-3013 10.1142/S0218301306003977
-
In fact, at the beginning the observed effect was called GGLP effect in distinction to an apparently similar effect observed in astronomy and known as HBT effect which was used to obtain stellar dimensions, see T.J. Humanic, Int. J. Mod. Phys. E 15, 197 (2006) for most recent review and references therein. IMPEER 0218-3013 10.1142/S0218301306003977
-
(2006)
Int. J. Mod. Phys. e
, vol.15
, pp. 197
-
-
Humanic, T.J.1
-
7
-
-
34247563401
-
-
Other important reviews are in whereas pedagogical descriptions of BEC are provided in. Finally, in one can find a valuable collection of seminal papers concerning different aspects of BEC.
-
Other important reviews are in whereas pedagogical descriptions of BEC are provided in. Finally, in one can find a valuable collection of seminal papers concerning different aspects of BEC.
-
-
-
-
8
-
-
0000319858
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.35.3396
-
W.A. Zajc, Phys. Rev. D 35, 3396 (1987). PRVDAQ 0556-2821 10.1103/PhysRevD.35.3396
-
(1987)
Phys. Rev. D
, vol.35
, pp. 3396
-
-
Zajc, W.A.1
-
9
-
-
34247597339
-
-
hep-ph/0610292 [BJPHE6 0103-9733
-
It means that the unobserved yield acts as a kind of heath bath influencing measured observables. Actually this is the main origin of the known spectacular success of the statistical description of such reactions with temperature T being the most important parameter describing the influence of such a heath bath, see G. Wilk, hep-ph/0610292 [Braz. J. Phys. (to be published)], and references therein. BJPHE6 0103-9733
-
Braz. J. Phys.
-
-
Wilk, G.1
-
10
-
-
0347172030
-
-
PRPLCM 0370-1573 10.1016/S0370-1573(99)00032-0
-
U.A. Wiedemann and U. Heinz, Phys. Rep. 319, 145 (1999); PRPLCM 0370-1573 10.1016/S0370-1573(99)00032-0
-
(1999)
Phys. Rep.
, vol.319
, pp. 145
-
-
Wiedemann, U.A.1
Heinz, U.2
-
11
-
-
0034164795
-
-
PRPLCM 0370-1573 10.1016/S0370-1573(99)00114-3
-
R.M. Weiner, Phys. Rep. 327, 249 (2000); PRPLCM 0370-1573 10.1016/S0370-1573(99)00114-3
-
(2000)
Phys. Rep.
, vol.327
, pp. 249
-
-
Weiner, R.M.1
-
13
-
-
0000062376
-
-
edited by W. Kittel et al., NATO Science Series C Kluwer Academic, Dordrecht
-
Particle Production Spanning MeV and TeV Energies, edited by, W. Kittel,,, NATO Science Series C Vol. 554 (Kluwer Academic, Dordrecht, 2000), p. 203;
-
(2000)
Particle Production Spanning MeV and TeV Energies
, vol.554
, pp. 203
-
-
-
14
-
-
33744522103
-
-
APOBBB 0587-4254
-
W. Kittel, Acta Phys. Pol. B APOBBB 0587-4254 32, 3927 (2001);
-
(2001)
Acta Phys. Pol. B
, vol.32
, pp. 3927
-
-
Kittel, W.1
-
15
-
-
0038054579
-
-
RPPHAG 0034-4885 10.1088/0034-4885/66/4/202
-
G. Alexander, Rep. Prog. Phys. 66, 481 (2003). RPPHAG 0034-4885 10.1088/0034-4885/66/4/202
-
(2003)
Rep. Prog. Phys.
, vol.66
, pp. 481
-
-
Alexander, G.1
-
16
-
-
0001544143
-
-
edited by H.H.Gutbrod and J. Rafelski (Plenum Press, New York
-
W.A. Zajc, in Particle Production in Highly Excited Matter, edited by, H.H.Gutbrod, and, J. Rafelski, (Plenum Press, New York, 1993), p. 435.
-
(1993)
Particle Production in Highly Excited Matter
, pp. 435
-
-
Zajc, W.A.1
-
18
-
-
0141918667
-
-
PRVCAN 0556-2813 10.1103/PhysRevC.68.024901
-
G.A. Kozlov, O.V. Utyuzh, and G. Wilk, Phys. Rev. C 68, 024901 (2003); PRVCAN 0556-2813 10.1103/PhysRevC.68.024901
-
(2003)
Phys. Rev. C
, vol.68
, pp. 024901
-
-
Kozlov, G.A.1
Utyuzh, O.V.2
Wilk, G.3
-
20
-
-
28844432975
-
-
Closer inspection reveals that one rather gets in this way a Fourier transform of distributions of spatiotemporal two-particle separations (or correlation lengths). Recently the possibility of sort of imaging the hadronization region by using data on C2 has been pursued, see PRVCAN 0556-2813 10.1103/PhysRevC.72.054902
-
Closer inspection reveals that one rather gets in this way a Fourier transform of distributions of spatiotemporal two-particle separations (or correlation lengths). Recently the possibility of sort of imaging the hadronization region by using data on C2 has been pursued, see D.A. Brown, Phys. Rev. C 72, 054902 (2005), and references therein. PRVCAN 0556-2813 10.1103/PhysRevC.72.054902
-
(2005)
Phys. Rev. C
, vol.72
, pp. 054902
-
-
Brown, D.A.1
-
21
-
-
0042626113
-
-
PYLBAJ 0370-2693 10.1016/0370-2693(96)00894-5
-
M. Biyajima, N. Suzuki, G. Wilk, and Z. Włodarczyk, Phys. Lett. B 386, 297 (1996). PYLBAJ 0370-2693 10.1016/0370-2693(96)00894-5
-
(1996)
Phys. Lett. B
, vol.386
, pp. 297
-
-
Biyajima, M.1
Suzuki, N.2
Wilk, G.3
Włodarczyk, Z.4
-
22
-
-
0000542764
-
-
ZPAHEX 0939-7922 10.1007/s002180050232
-
H. Merlitz and D. Pelte, Z. Phys. A ZPAHEX 0939-7922 357, 175 (1997). 10.1007/s002180050232
-
(1997)
Z. Phys. a
, vol.357
, pp. 175
-
-
Merlitz, H.1
Pelte, D.2
-
23
-
-
0346581435
-
-
Compare also PRVCAN 0556-2813 10.1103/PhysRevC.56.R614
-
Compare also U.A. Wiedemann, Phys. Rev. C 56, R614 (1997); PRVCAN 0556-2813 10.1103/PhysRevC.56.R614
-
(1997)
Phys. Rev. C
, vol.56
, pp. 614
-
-
Wiedemann, U.A.1
-
24
-
-
0001017332
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.80.916
-
T. Csörgo and J. Zimányi, Phys. Rev. Lett. 80, 916 (1998); PRLTAO 0031-9007 10.1103/PhysRevLett.80.916
-
(1998)
Phys. Rev. Lett.
, vol.80
, pp. 916
-
-
Csörgo, T.1
Zimányi, J.2
-
26
-
-
0006722066
-
-
ZPAHEX 0939-7922 10.1007/BF01289528
-
H. Merlitz and D. Pelte, Z. Phys. A ZPAHEX 0939-7922 351, 187 (1995). 10.1007/BF01289528
-
(1995)
Z. Phys. a
, vol.351
, pp. 187
-
-
Merlitz, H.1
Pelte, D.2
-
28
-
-
16644386483
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.59.014024
-
T. Osada, M. Maruyama, and F. Takagi, Phys. Rev. D 59, 014024 (1998). PRVDAQ 0556-2821 10.1103/PhysRevD.59.014024
-
(1998)
Phys. Rev. D
, vol.59
, pp. 014024
-
-
Osada, T.1
Maruyama, M.2
Takagi, F.3
-
29
-
-
1542679991
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.58.094013
-
K. Fiałkowski, R. Wit, and J. Wosiek, Phys. Rev. D 58, 094013 (1998); PRVDAQ 0556-2821 10.1103/PhysRevD.58.094013
-
(1998)
Phys. Rev. D
, vol.58
, pp. 094013
-
-
Fiałkowski, K.1
Wit, R.2
Wosiek, J.3
-
30
-
-
0000922504
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.53.3586
-
T. Wibig, Phys. Rev. D 53, 3586 (1996); PRVDAQ 0556-2821 10.1103/PhysRevD.53.3586
-
(1996)
Phys. Rev. D
, vol.53
, pp. 3586
-
-
Wibig, T.1
-
32
-
-
17044387664
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.61.054002
-
K. Geiger, J. Ellis, U. Heinz, and U.A. Wiedemann, Phys. Rev. D 61, 054002 (2000); PRVDAQ 0556-2821 10.1103/PhysRevD.61.054002
-
(2000)
Phys. Rev. D
, vol.61
, pp. 054002
-
-
Geiger, K.1
Ellis, J.2
Heinz, U.3
Wiedemann, U.A.4
-
33
-
-
0002378261
-
-
PYLBAJ 0370-2693 10.1016/S0370-2693(97)00710-7
-
Q.H. Zhang, U.A. Wiedemann, C. Slotta, and U. Heinz, Phys. Lett. B 407, 33 (1997). PYLBAJ 0370-2693 10.1016/S0370-2693(97)00710-7
-
(1997)
Phys. Lett. B
, vol.407
, pp. 33
-
-
Zhang, Q.H.1
Wiedemann, U.A.2
Slotta, C.3
Heinz, U.4
-
34
-
-
0032498697
-
-
NUPBBO 0550-3213 10.1016/S0550-3213(97)00722-0
-
B. Andersson and M. Ringner, Nucl. Phys. NUPBBO 0550-3213 B513, 627 (1998). 10.1016/S0550-3213(97)00722-0
-
(1998)
Nucl. Phys.
, vol.513
, pp. 627
-
-
Andersson, B.1
Ringner, M.2
-
35
-
-
0002116746
-
-
EPCFFB 1434-6044 10.1007/s100520050131
-
L. Lönnblad and T. Sjöstrand, Eur. Phys. J. C 2, 165 (1998). EPCFFB 1434-6044 10.1007/s100520050131
-
(1998)
Eur. Phys. J. C
, vol.2
, pp. 165
-
-
Lönnblad, L.1
Sjöstrand, T.2
-
36
-
-
0035856728
-
-
PYLBAJ 0370-2693 10.1016/S0370-2693(01)01306-5
-
O.V. Utyuzh, G. Wilk, and Z. Włodarczyk, Phys. Lett. B 522, 273 (2001). PYLBAJ 0370-2693 10.1016/S0370-2693(01)01306-5
-
(2001)
Phys. Lett. B
, vol.522
, pp. 273
-
-
Utyuzh, O.V.1
Wilk, G.2
Włodarczyk, Z.3
-
38
-
-
33645962247
-
Proceedings of the XXXII ISMD, Alushta, Crimea, Ukraine, 2002
-
edited by A. Sissakian, G. Kozlov, and E. Kolganova
-
O.V. Utyuzh, G. Wilk, and Z. Włodarczyk, in Proceedings of the XXXII ISMD, Alushta, Crimea, Ukraine, 2002, edited by, A. Sissakian,,, G. Kozlov,, and, E. Kolganova,, [Acta Phys. Polon. B 33, 2681 (2002)].
-
(2002)
Acta Phys. Polon. B
, vol.33
, pp. 2681
-
-
Utyuzh, O.V.1
Wilk, G.2
Włodarczyk, Z.3
-
39
-
-
34247639516
-
-
The only discussion of such changes we are aware of is in where it was shown that an enforcing effect of BEC into a simple cascade model results in the appearances of multicharged vertices, not present in the original scheme. For more details, see and references therein.
-
The only discussion of such changes we are aware of is in where it was shown that an enforcing effect of BEC into a simple cascade model results in the appearances of multicharged vertices, not present in the original scheme. For more details, see and references therein.
-
-
-
-
40
-
-
0000985993
-
-
ZPCFD2 0170-9739 10.1007/BF01557602
-
A. Giovannini and L. Van Hove, Z. Phys. C 30, 391 (1986); ZPCFD2 0170-9739 10.1007/BF01557602
-
(1986)
Z. Phys. C
, vol.30
, pp. 391
-
-
Giovannini, A.1
Van Hove, L.2
-
41
-
-
0000666743
-
-
see also IMPAEF 0217-751X 10.1142/S0217751X87000806
-
see also P. Carruthers and C.S. Shih, Int. J. Mod. Phys. A 2, 1447 (1987). IMPAEF 0217-751X 10.1142/S0217751X87000806
-
(1987)
Int. J. Mod. Phys. a
, vol.2
, pp. 1447
-
-
Carruthers, P.1
Shih, C.S.2
-
42
-
-
0346581435
-
-
PRVCAN 0556-2813 10.1103/PhysRevC.56.R614
-
U.A. Wiedemann, P. Foka, H. Kalechofsky, M. Martin, C. Slotta, and Q.H. Zhang, Phys. Rev. C 56, R614 (1997); PRVCAN 0556-2813 10.1103/PhysRevC.56.R614
-
(1997)
Phys. Rev. C
, vol.56
, pp. 614
-
-
Wiedemann, U.A.1
Foka, P.2
Kalechofsky, H.3
Martin, M.4
Slotta, C.5
Zhang, Q.H.6
-
43
-
-
0032409960
-
-
EPCFFB 1434-6044 10.1007/s100520050146
-
M. Martin, H. Kalechofsky, P. Foka, and U.A. Wiedemann, Eur. Phys. J. C 2, 359 (1998). EPCFFB 1434-6044 10.1007/s100520050146
-
(1998)
Eur. Phys. J. C
, vol.2
, pp. 359
-
-
Martin, M.1
Kalechofsky, H.2
Foka, P.3
Wiedemann, U.A.4
-
44
-
-
34247602577
-
-
The reason is obvious. When only mean multiplicity n̄ is fixed, the most probable distribution according to the IT approach is a geometrical (or Bose-Einstein) one. Such is therefore distribution of particles in each cell in rapidity, therefore their composition will result in P(n) of NB type.
-
The reason is obvious. When only mean multiplicity n̄ is fixed, the most probable distribution according to the IT approach is a geometrical (or Bose-Einstein) one. Such is therefore distribution of particles in each cell in rapidity, therefore their composition will result in P(n) of NB type.
-
-
-
-
45
-
-
0001412962
-
-
Actually one obtains in this way only some part of this intermittency signal. Nevertheless this fact suggests that fluctuations connected with intermittency are, at least to some extent, the same as those caused by BEC (or both have the same origin), cf. PYLBAJ 0370-2693 10.1016/0370-2693(89)90350-X
-
Actually one obtains in this way only some part of this intermittency signal. Nevertheless this fact suggests that fluctuations connected with intermittency are, at least to some extent, the same as those caused by BEC (or both have the same origin), cf. P. Carruthers, E.M. Friedlander, C.C. Shih, and R.M. Weiner, Phys. Lett. B 222, 487 (1989) and. PYLBAJ 0370-2693 10.1016/0370-2693(89)90350-X
-
(1989)
Phys. Lett. B
, vol.222
, pp. 487
-
-
Carruthers, P.1
Friedlander, E.M.2
Shih, C.C.3
Weiner, R.M.4
-
47
-
-
0033245331
-
-
NPBSE7 0920-5632 10.1016/S0920-5632(99)00135-8
-
K. Zalewski, Nucl. Phys. B, Proc. Suppl. NPBSE7 0920-5632 74, 65 (1999); 10.1016/S0920-5632(99)00135-8
-
(1999)
Nucl. Phys. B, Proc. Suppl.
, vol.74
, pp. 65
-
-
Zalewski, K.1
-
48
-
-
0141875137
-
-
LNPHA4 0075-8450
-
K. Zalewski Lect. Notes Phys. 539, 291 (2000). LNPHA4 0075-8450
-
(2000)
Lect. Notes Phys.
, vol.539
, pp. 291
-
-
Zalewski, K.1
-
49
-
-
36949085134
-
-
NATUAS 0028-0836 10.1038/1781449a0
-
E.E. Purcell, Nature (London) NATUAS 0028-0836 178, 1449 (1956). 10.1038/1781449a0
-
(1956)
Nature (London)
, vol.178
, pp. 1449
-
-
Purcell, E.E.1
-
50
-
-
0037545007
-
-
Compare also PPSOAU 0370-1328 10.1088/0370-1328/84/3/313
-
Compare also L. Mandel, E.C.G. Sudarshan, and E. Wolf, Proc. Phys. Soc. PPSOAU 0370-1328 84, 435 (1964). 10.1088/0370-1328/84/3/313
-
(1964)
Proc. Phys. Soc.
, vol.84
, pp. 435
-
-
Mandel, L.1
Sudarshan, E.C.G.2
Wolf, E.3
-
51
-
-
34247641702
-
-
NBI-HE-73-17 (unpublished).
-
A. Giovannini and H.B. Nielsen, The Niels Bohr Institute Report No. NBI-HE-73-17 (unpublished).
-
-
-
Giovannini, A.1
Nielsen, H.B.2
-
52
-
-
34247626873
-
-
See also edited by F. Duimio, A. Giovannini, and S. Ratii
-
See also Proceedings of the IV International Symposium on Multiparticle Hadrodynamics, Pavia, 1973, edited by, F. Duimio,,, A. Giovannini,, and, S. Ratii,, p. 538.
-
Proceedings of the IV International Symposium on Multiparticle Hadrodynamics, Pavia, 1973
, pp. 538
-
-
-
53
-
-
34247644395
-
-
Notice that, in general, the multiplicity distribution function satisfies the relation: P(n+1)/P(n)=g(n)/(n+1), where (n+1) is a reflection of the fact that with n particles given the (n+1)th one can be allocated in n+1 ways. Different g(n) result in different forms of P(n). In particular, for g(n)=a one gets (after normalization) P(n)=ane-a/n!, whereas g(n)=p(n+1) results (after normalization) in P(n)=(1-p)pn, i.e., in a geometrical distribution, which means that the emission of an extra particle is enhanced by a factor (n+1) and this is Bose-Einstein enhancement and the emission with this is usually called stimulated emission.
-
Notice that, in general, the multiplicity distribution function satisfies the relation: P(n+1)/P(n)=g(n)/(n+1), where (n+1) is a reflection of the fact that with n particles given the (n+1)th one can be allocated in n+1 ways. Different g(n) result in different forms of P(n). In particular, for g(n)=a one gets (after normalization) P(n)=ane-a/n!, whereas g(n)=p(n+1) results (after normalization) in P(n)=(1-p)pn, i.e., in a geometrical distribution, which means that the emission of an extra particle is enhanced by a factor (n+1) and this is Bose-Einstein enhancement and the emission with this is usually called stimulated emission.
-
-
-
-
54
-
-
0003444152
-
-
See, for example, Clarendon Press, Oxford, 2nd ed.;
-
See, for example, R. Loudon, The Quantum Theory of Light (Clarendon Press, Oxford, 1983), 2nd ed.;
-
(1983)
The Quantum Theory of Light
-
-
Loudon, R.1
-
56
-
-
0001278540
-
-
PTPKAV 0033-068X 10.1143/PTP.69.966
-
M. Biyajima, Prog. Theor. Phys. 69, 966 (1983); PTPKAV 0033-068X 10.1143/PTP.69.966
-
(1983)
Prog. Theor. Phys.
, vol.69
, pp. 966
-
-
Biyajima, M.1
-
57
-
-
0042042600
-
-
PYLBAJ 0370-2693 10.1016/0370-2693(84)90234-X
-
M. Biyajima Phys. Lett. 137B, 225 (1984). PYLBAJ 0370-2693 10.1016/0370-2693(84)90234-X
-
(1984)
Phys. Lett.
, vol.137
, pp. 225
-
-
Biyajima, M.1
-
58
-
-
0003168111
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.10.65
-
W.J. Knox, Phys. Rev. D 10, 65 (1974); PRVDAQ 0556-2821 10.1103/PhysRevD.10.65
-
(1974)
Phys. Rev. D
, vol.10
, pp. 65
-
-
Knox, W.J.1
-
59
-
-
0042042599
-
-
NUPBBO 0550-3213 10.1016/0550-3213(77)90106-7
-
E.H. De Groot and H. Satz, Nucl. Phys. NUPBBO 0550-3213 B130, 257 (1977); 10.1016/0550-3213(77)90106-7
-
(1977)
Nucl. Phys.
, vol.130
, pp. 257
-
-
De Groot, E.H.1
Satz, H.2
-
61
-
-
0039065847
-
-
PYLBAJ 0370-2693 10.1016/0370-2693(79)90562-8
-
A.M. Cooper, O. Miyamura, A. Suzuki, and K. Takahashi, Phys. Lett. 87B, 393 (1979); PYLBAJ 0370-2693 10.1016/0370-2693(79)90562-8
-
(1979)
Phys. Lett.
, vol.87
, pp. 393
-
-
Cooper, A.M.1
Miyamura, O.2
Suzuki, A.3
Takahashi, K.4
-
63
-
-
34247636710
-
-
edited by T. Csörgo World Scientific, Singapore, et al.
-
K. Fiałkowski, in Proceedings of the XXX ISMD, Tihany, Hungary, 2000, edited by, T. Csörgo,, (World Scientific, Singapore, 2001), p. 357;
-
(2001)
Proceedings of the XXX ISMD, Tihany, Hungary, 2000
, pp. 357
-
-
Fiałkowski, K.1
-
64
-
-
0036577075
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.65.096008
-
M. Stephanov, Phys. Rev. D 65, 096008 (2002). PRVDAQ 0556-2821 10.1103/PhysRevD.65.096008
-
(2002)
Phys. Rev. D
, vol.65
, pp. 096008
-
-
Stephanov, M.1
-
66
-
-
17544369993
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.37.2446
-
J. Finkelstein, Phys. Rev. D 37, 2446 (1988); PRVDAQ 0556-2821 10.1103/PhysRevD.37.2446
-
(1988)
Phys. Rev. D
, vol.37
, pp. 2446
-
-
Finkelstein, J.1
-
67
-
-
85038982333
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.58.017501
-
Ding-wei Huang, Phys. Rev. D 58, 017501 (1998). PRVDAQ 0556-2821 10.1103/PhysRevD.58.017501
-
(1998)
Phys. Rev. D
, vol.58
, pp. 017501
-
-
Huang, D.1
-
68
-
-
12144258567
-
-
It is interesting to notice at this point that the best fits to C2(δE) and C2(δpx) for σ0=0.1 presented here can be obtained by using, respectively [x=δi and y=C2(δi)], shifted Gaussian y=y0+2/πAexp[-2(x-xc)2/w2]/w (with y0=0.724, xc=-0.125, w=0.922, and A=1.186), and shifted Lorentzian y=y0+(2Aw/π)/[4(x-xc)2+w2] (with y0=0.744, xc=0.0003, w=1.221, and A=1.154). Notice that the later shape belongs to the category of Lévy distributions discussed in the context of BEC in EPCFFB 1434-6044 10.1140/epjc/s2004-01870-9
-
It is interesting to notice at this point that the best fits to C2(δE) and C2(δpx) for σ0=0.1 presented here can be obtained by using, respectively [x=δi and y=C2(δi)], shifted Gaussian y=y0+2/πAexp[-2(x-xc)2/w2]/w (with y0=0.724, xc=-0.125, w=0.922, and A=1.186), and shifted Lorentzian y=y0+(2Aw/π)/[4(x-xc)2+w2] (with y0=0.744, xc=0.0003, w=1.221, and A=1.154). Notice that the later shape belongs to the category of Lévy distributions discussed in the context of BEC in T. Csörgo, S. Hegyi, and W. Zajc, Eur. Phys. J. C 36, 36 (2004) because of their connection with the possible fractality of the hadronizing source. In fact one could as well use other forms of the G(E) function in Eq. 18 to get still another form of C2, EPCFFB 1434-6044 10.1140/epjc/s2004-01870-9
-
(2004)
Eur. Phys. J. C
, vol.36
, pp. 36
-
-
Csörgo, T.1
Hegyi, S.2
Zajc, W.3
-
69
-
-
0141909893
-
-
see, for example, PTPKAV 0033-068X 10.1143/PTP.91.905
-
see, for example, T. Mizoguchi, M. Biyajima, and T. Kageya, Prog. Theor. Phys. 91, 905 (1994); PTPKAV 0033-068X 10.1143/PTP.91.905
-
(1994)
Prog. Theor. Phys.
, vol.91
, pp. 905
-
-
Mizoguchi, T.1
Biyajima, M.2
Kageya, T.3
-
71
-
-
24544452517
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.49.1217
-
I.V. Andreev, M. Plümer, B.R. Schlei, and R.M. Weiner, Phys. Rev. D 49, 1217 (1994). PRVDAQ 0556-2821 10.1103/PhysRevD.49.1217
-
(1994)
Phys. Rev. D
, vol.49
, pp. 1217
-
-
Andreev, I.V.1
Plümer, M.2
Schlei, B.R.3
Weiner, R.M.4
-
73
-
-
34247625095
-
-
hep-ph/0612364 [BJPHE6 0103-9733
-
for references to high multiplicity measurement projects, see E. Kokoulina, A. Kutov, and V. Nikitin, hep-ph/0612364 [Braz. J. Phys. (to be published)]. BJPHE6 0103-9733
-
Braz. J. Phys.
-
-
Kokoulina, E.1
Kutov, A.2
Nikitin, V.3
-
74
-
-
84889235687
-
-
See, for example
-
See, for example, A.M. Gavrilik, Symm., Integ. Geom., Meth. Appl. 2, 074 (2006);
-
(2006)
Symm., Integ. Geom., Meth. Appl.
, vol.2
, pp. 074
-
-
Gavrilik, A.M.1
-
76
-
-
22044439525
-
-
This should be contrasted, for example, with the concept of resonant "halo" discussed in PRVCAN 0556-2813 10.1103/PhysRevC.57.3251
-
This should be contrasted, for example, with the concept of resonant "halo" discussed in S. Nickerson, T. Csörgo, and D. Kiang, Phys. Rev. C 57, 3251 (1998), which is not able to do so. PRVCAN 0556-2813 10.1103/PhysRevC.57.3251
-
(1998)
Phys. Rev. C
, vol.57
, pp. 3251
-
-
Nickerson, S.1
Csörgo, T.2
Kiang, D.3
-
77
-
-
33645948774
-
-
See, for example, NPBSE7 0920-5632 10.1016/j.nuclphysbps.2005.08.006
-
See, for example, O. Pooth (OPAL Collaboration), Nucl. Phys. B, Proc. Suppl. NPBSE7 0920-5632 152, 35 (2006), and references therein. 10.1016/j.nuclphysbps.2005.08.006
-
(2006)
Nucl. Phys. B, Proc. Suppl.
, vol.152
, pp. 35
-
-
Pooth, O.1
-
78
-
-
0034704693
-
-
This is a potentially very interesting result deserving further specialized consideration, which, however, would lead us outside the scope of the present paper. In this respect, we refer to the work by PYLBAJ 0370-2693 10.1016/S0370-2693(00)00223-9
-
This is a potentially very interesting result deserving further specialized consideration, which, however, would lead us outside the scope of the present paper. In this respect, we refer to the work by E.K.G. Sarkisyan, Phys. Lett. B 477, 1 (2000), where different multiplicity distributions were studied from the point of view of intermittency and higher-order correlations. PYLBAJ 0370-2693 10.1016/S0370-2693(00)00223-9
-
(2000)
Phys. Lett. B
, vol.477
, pp. 1
-
-
Sarkisyan, E.K.G.1
-
79
-
-
0035924227
-
-
Similarly, in PYLBAJ 0370-2693 10.1016/S0370-2693(01)01332-6
-
Similarly, in G. Abbiendi (OPAL Collaboration), Phys. Lett. B 523, 35 (2001), one can find studies of intermittency and especially of the higher-order genuine correlations made with an all-charge vs like-sign group of hadrons compared to the Bose-Einstein effect. PYLBAJ 0370-2693 10.1016/S0370-2693(01) 01332-6
-
(2001)
Phys. Lett. B
, vol.523
, pp. 35
-
-
Abbiendi, G.1
-
84
-
-
33645929101
-
-
EPJBFY 1434-6028 10.1140/epjb/e2006-00105-2
-
T. Osada, O.V. Utyuzh, G. Wilk, and Z. Włodarczyk, Eur. Phys. J. B 50, 7 (2006), and references therein. EPJBFY 1434-6028 10.1140/epjb/e2006- 00105-2
-
(2006)
Eur. Phys. J. B
, vol.50
, pp. 7
-
-
Osada, T.1
Utyuzh, O.V.2
Wilk, G.3
Włodarczyk, Z.4
-
85
-
-
0000181069
-
-
PYLBAJ 0370-2693 10.1016/0370-2693(95)00547-X
-
M. Biyajima, T. Mizoguchi, T. Osada, and G.Wilk, Phys. Lett. B 353, 340 (1995); PYLBAJ 0370-2693 10.1016/0370-2693(95)00547-X
-
(1995)
Phys. Lett. B
, vol.353
, pp. 340
-
-
Biyajima, M.1
Mizoguchi, T.2
Osada, T.3
G.wilk4
-
87
-
-
33845416801
-
-
see also the review by APCPCS 0094-243X 10.1063/1.2197475
-
see also the review by O.V. Utyuzh, AIP Conf. Proc. 828, 595 (2006). APCPCS 0094-243X 10.1063/1.2197475
-
(2006)
AIP Conf. Proc.
, vol.828
, pp. 595
-
-
Utyuzh, O.V.1
-
88
-
-
37649032947
-
-
Compare, for example, PLEEE8 1063-651X 10.1103/PhysRevE.71.016138
-
Compare, for example, A.E. Ezhov and A.Yu. Khrennikov, Phys. Rev. E 71, 016138 (2005); PLEEE8 1063-651X 10.1103/PhysRevE.71.016138
-
(2005)
Phys. Rev. e
, vol.71
, pp. 016138
-
-
Ezhov, A.E.1
Khrennikov, A.Yu.2
-
89
-
-
34247635612
-
-
cond-mat/0001436;
-
K. Stalinas, cond-mat/0001436;
-
-
-
Stalinas, K.1
-
90
-
-
34247567893
-
-
cond-mat/0001347.
-
K. Stalinas cond-mat/0001347.
-
-
-
Stalinas, K.1
-
91
-
-
0033184811
-
-
CPHCBZ 0010-4655 10.1016/S0010-4655(99)00412-9
-
R. Kutner and M. Regulski, Comput. Phys. Commun. 121-122, 586 (1999); CPHCBZ 0010-4655 10.1016/S0010-4655(99)00412-9
-
(1999)
Comput. Phys. Commun.
, vol.121-122
, pp. 586
-
-
Kutner, R.1
Regulski, M.2
-
92
-
-
21844510459
-
-
cf. also JPHAC5 0305-4470 10.1088/0305-4470/28/4/017
-
cf. also R. Kutner, K.W. Kehr, W. Renz, and R. Przeniosło, J. Phys. A JPHAC5 0305-4470 28, 923 (1995). 10.1088/0305-4470/28/4/017
-
(1995)
J. Phys. a
, vol.28
, pp. 923
-
-
Kutner, R.1
Kehr, K.W.2
Renz, W.3
Przeniosło, R.4
-
93
-
-
9744225341
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.86.5632
-
G. Bianconi and A.-L. Barabási, Phys. Rev. Lett. 86, 5632 (2001). PRLTAO 0031-9007 10.1103/PhysRevLett.86.5632
-
(2001)
Phys. Rev. Lett.
, vol.86
, pp. 5632
-
-
Bianconi, G.1
Barabási, A.-L.2
-
94
-
-
33751230197
-
-
RMPHAT 0034-6861 10.1103/RevModPhys.78.1267
-
R.J. Glauber, Rev. Mod. Phys. 78, 1267 (2006), and references therein. RMPHAT 0034-6861 10.1103/RevModPhys.78.1267
-
(2006)
Rev. Mod. Phys.
, vol.78
, pp. 1267
-
-
Glauber, R.J.1
-
95
-
-
2442573793
-
-
That this point can be important is demonstrated, for example, in EPCFFB 1434-6044 10.1140/epjc/s2003-01265-6
-
That this point can be important is demonstrated, for example, in N. Borghini, Eur. Phys. J. C 30, 381 (2003) EPCFFB 1434-6044 10.1140/epjc/s2003- 01265-6
-
(2003)
Eur. Phys. J. C
, vol.30
, pp. 381
-
-
Borghini, N.1
-
96
-
-
33847404901
-
-
and PRVCAN 0556-2813 10.1103/PhysRevC.75.021904
-
and N. Borghini Phys. Rev. C 75, 021904 (2007); PRVCAN 0556-2813 10.1103/PhysRevC.75.021904
-
(2007)
Phys. Rev. C
, vol.75
, pp. 021904
-
-
Borghini, N.1
-
97
-
-
33244465173
-
-
PRVCAN 0556-2813 10.1103/PhysRevC.72.064906
-
B.B. Back, Phys. Rev. C 72, 064906 (2005) PRVCAN 0556-2813 10.1103/PhysRevC.72.064906
-
(2005)
Phys. Rev. C
, vol.72
, pp. 064906
-
-
Back, B.B.1
-
99
-
-
0000777155
-
-
For example, the sequential choice of energies from the distribution f′(E)=E•f(E) would result in an event reproducing the initial distribution f(E) and conserving energy [because sampling from uniform distribution xk[0,1-x1-x2 - xk-1] results in P(x)=1/x, cf., PRVDAQ 0556-2821 10.1103/PhysRevD.24.1847
-
For example, the sequential choice of energies from the distribution f′(E)=E•f(E) would result in an event reproducing the initial distribution f(E) and conserving energy [because sampling from uniform distribution xk[0,1-x1-x2 - xk-1] results in P(x)=1/x, cf., M. Shibata, Phys. Rev. D 24, 1847 (1981)]. This could be thought as a natural method to follow. However, it turns out that one cannot correct imbalances in momenta px,y,z just by rotating all angles by some fixed (ΔΘ,ΔΦ), the rescaling of at least one component is necessary. This ruins the original energy balance and needs further corrections. PRVDAQ 0556-2821 10.1103/PhysRevD.24. 1847
-
(1981)
Phys. Rev. D
, vol.24
, pp. 1847
-
-
Shibata, M.1
-
100
-
-
34247607749
-
-
It is interesting to note that distributions of QTOT in Fig. 16 follow Gaussian form for small P0, for P0=0.9 which becomes the so-called q-Gaussian distribution (known from Tsallis statistics, see reference in).
-
It is interesting to note that distributions of QTOT in Fig. 16 follow Gaussian form for small P0, for P0=0.9 which becomes the so-called q-Gaussian distribution (known from Tsallis statistics, see reference in).
-
-
-
-
101
-
-
10444268993
-
-
PYLBAJ 0370-2693 10.1016/0370-2693(92)90181-3
-
P. Abreu (DELPHI Collaboration), Phys. Lett. B 286, 201 (1992); PYLBAJ 0370-2693 10.1016/0370-2693(92)90181-3
-
(1992)
Phys. Lett. B
, vol.286
, pp. 201
-
-
Abreu, P.1
-
102
-
-
4243841516
-
-
PYLBAJ 0370-2693 10.1016/0370-2693(90)91062-G
-
P. Abreu Phys. Lett. B 247, 137 (1990). PYLBAJ 0370-2693 10.1016/0370-2693(90)91062-G
-
(1990)
Phys. Lett. B
, vol.247
, pp. 137
-
-
Abreu, P.1
-
103
-
-
0030137248
-
-
PRPLCM 0370-1573 10.1016/0370-1573(95)00069-0
-
E.A. De Wolf, I.M. Dremin, and W. Kittel, Phys. Rep. 270, 1 (1996); PRPLCM 0370-1573 10.1016/0370-1573(95)00069-0
-
(1996)
Phys. Rep.
, vol.270
, pp. 1
-
-
De Wolf, E.A.1
Dremin, I.M.2
Kittel, W.3
-
104
-
-
0000319693
-
-
PRPLCM 0370-1573 10.1016/0370-1573(94)00075-E
-
P. Boek, M. Płoszajczak, and R. Botet, Phys. Rep. 252, 101 (1995); PRPLCM 0370-1573 10.1016/0370-1573(94)00075-E
-
(1995)
Phys. Rep.
, vol.252
, pp. 101
-
-
Boek, P.1
Płoszajczak, M.2
Botet, R.3
-
105
-
-
0000195648
-
-
IMPAEF 0217-751X 10.1142/S0217751X95001856
-
I.V. Andreev, I.M. Dremin, M. Biyajima, and N. Suzuki, Int. J. Mod. Phys. A 10, 3951 (1995). IMPAEF 0217-751X 10.1142/S0217751X95001856
-
(1995)
Int. J. Mod. Phys. a
, vol.10
, pp. 3951
-
-
Andreev, I.V.1
Dremin, I.M.2
Biyajima, M.3
Suzuki, N.4
-
106
-
-
33645100814
-
-
CPHCBZ 0010-4655 10.1016/j.cpc.2005.11.010
-
A. Kisiel, T. Tałuć, W. Broniowski, and W. Florkowski, Comput. Phys. Commun. 174, 669 (2006). CPHCBZ 0010-4655 10.1016/j.cpc.2005.11. 010
-
(2006)
Comput. Phys. Commun.
, vol.174
, pp. 669
-
-
Kisiel, A.1
Tałuć, T.2
Broniowski, W.3
Florkowski, W.4
|