Topology of “ white ” stars in relativistic fragmentation of
of 32
/32
Embed Size (px)
description
Topology of “ white ” stars in relativistic fragmentation of light nuclei in nuclear track emulsion P. I. Zarubin (JINR, Dubna). 0.5 μ m resolution , identification of charges and H&He isotopes. Au plate. 3.65A GeV 2 8 Si in emulsion. AVI MOV. 3.65A GeV 28 Si 2+2+2+2+2+2+1. - PowerPoint PPT Presentation
Transcript of Topology of “ white ” stars in relativistic fragmentation of
-
Topology of white stars in relativistic fragmentation of light nuclei in nuclear track emulsionP. I. Zarubin (JINR, Dubna)
-
Au plate 0.5 m resolution, identification of charges and H&He isotopes
-
3.65A GeV 28Si in emulsionAVIMOV
-
3.65A GeV 28Si 2+2+2+2+2+2+1
-
3.65A GeV 24Mg 2+2+2+2+2+2
-
bik=-(Pi/mi-Pk/mk)2
-
4.5A GeV/c 24Mg 5+2+2+1+1+1
-
4.5A GeV/c 24Mg 7+2+1+1+1
-
3.65A GeV 24Mg
-
3.3A GeV 22Ne 1400 inelastic stars
-
3.65A GeV 28Si
-
3.65A GeV 32S
-
3.65A GeV 28Si 1980 Inelastic Events
-
Q=(M*-M)/A
-
3.65A GeV 20Ne 2+2+2+2+2
-
T 0.05-2 0.005-0.03P 20-110 MeV 10-2 fm
-
4.5 A GeV/c 16O
-
4.5A GeV/c 16O
-
2.1 14N3He+Hjpg
-
3.65A GeV/c 14N
-
1A GeV 56Fe
-
158 A /c Pb
-
158 A /c Pb
-
1234158 A /c PbMOVAVI
-
123456158 A /c Pb
-
1234158 A /c Pb
-
1234Au 10.6 A
-
http://becquerel.jinr.ru/
