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Relativistic Fragmentation of Light Nuclei in Nuclear Emulsion Tracks

Explore the topology of white stars in light nuclei fragmentation, identifying charges and isotopes in nuclear track emulsion at varying energy levels.

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Relativistic Fragmentation of Light Nuclei in Nuclear Emulsion Tracks

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  1. Topology of “ white ” stars in relativistic fragmentation of light nuclei in nuclear track emulsion P. I. Zarubin (JINR, Dubna)

  2. 0.5 μm resolution, identification of charges and H&He isotopes Au plate

  3. 3.65A GeV 28Si in emulsion AVIMOV

  4. 3.65A GeV 28Si 2+2+2+2+2+2+1

  5. 3.65A GeV 24Mg 2+2+2+2+2+2

  6. bik=-(Pi/mi-Pk/mk)2

  7. 4.5A GeV/c 24Mg 5+2+2+1+1+1

  8. 4.5A GeV/c 24Mg 7+2+1+1+1

  9. 3.65A GeV 24Mg

  10. 3.3A GeV 22Ne 1400 inelastic stars

  11. 3.65A GeV 28Si

  12. 3.65A GeV 32S

  13. 3.65A GeV 28Si 1980 Inelastic Events

  14. Q’=(M*-M)/A

  15. 3.65A GeV 20Ne 2+2+2+2+2

  16. Tα0.05-2 МэВ βα 0.005-0.03 Pα 20-110 MeV λ 10-2 fm

  17. 4.5 A GeV/c 16O

  18. 4.5A GeV/c 16O

  19. 2.1 А ГэВ 14N→3He+H jpg

  20. 3.65A GeV/c 14N

  21. 1A GeV 56Fe

  22. 158 A ГэВ/c Pb

  23. 158 A ГэВ/c Pb

  24. 158 A ГэВ/c Pb 1 2 AVI MOV 3 4

  25. 158 A ГэВ/c Pb 2 3 1 4 5 6

  26. 158 A ГэВ/c Pb 1 2 3 4

  27. Au 10.6 A ГэВ 2 1 4 3

  28. http://becquerel.jinr.ru/

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