Particle abundances and spectra in the hydrodynamical description of relativistic nuclear collisions with light projectiles (2003)
- Authors:
- USP affiliated authors: GRASSI, FREDERIQUE MARIE BRIGITTE SYLVIE - IF ; HAMA, YOGIRO - IF
- Unidade: IF
- Subjects: FÍSICA DE ALTA ENERGIA; HIDRODINÂMICA
- Language: Inglês
- Imprenta:
-
ABNT
GRASSI, Frederique Marie Brigitte Sylvie et al. Particle abundances and spectra in the hydrodynamical description of relativistic nuclear collisions with light projectiles. . São Paulo: IFUSP. Disponível em: http://snsbf2.if.usp.br/PS_cache/hep-ph/pdf/0307/0307306.pdf. Acesso em: 20 abr. 2024. , 2003 -
APA
Grassi, F. M. B. S., Hama, Y., Kodama, T., & Socolowski Júnior, O. (2003). Particle abundances and spectra in the hydrodynamical description of relativistic nuclear collisions with light projectiles. São Paulo: IFUSP. Recuperado de http://snsbf2.if.usp.br/PS_cache/hep-ph/pdf/0307/0307306.pdf -
NLM
Grassi FMBS, Hama Y, Kodama T, Socolowski Júnior O. Particle abundances and spectra in the hydrodynamical description of relativistic nuclear collisions with light projectiles [Internet]. 2003 ;[citado 2024 abr. 20 ] Available from: http://snsbf2.if.usp.br/PS_cache/hep-ph/pdf/0307/0307306.pdf -
Vancouver
Grassi FMBS, Hama Y, Kodama T, Socolowski Júnior O. Particle abundances and spectra in the hydrodynamical description of relativistic nuclear collisions with light projectiles [Internet]. 2003 ;[citado 2024 abr. 20 ] Available from: http://snsbf2.if.usp.br/PS_cache/hep-ph/pdf/0307/0307306.pdf - Large pt enhancement from freeze out
- Importance of granular structure in the initial conditions for the elliptic flow
- Hydrodynamics and the "Ridge"
- Fluctuation of the initial conditions and its consequences on some observables
- A closer look at the influence of tubular initial conditions on two-particle correlations
- Event-by-event hydrodynamical evolution
- Continuous emission versus freeze-out via Hanbury Brown-Twiss
- Kinetic freeze out models
- Large 'P IND.t' enhancement from freeze out
- HBT effect with SPheRIO code
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