The ratio sigmaO/lambda at RHIC (2005)
- Autores:
- Autores USP: TOLEDO, ALEJANDRO SZANTO DE - IF ; MUNHOZ, MARCELO GAMEIRO - IF ; SUAIDE, ALEXANDRE ALARCON DO PASSO - IF
- Unidade: IF
- Assuntos: FÍSICA NUCLEAR; ÍONS PESADOS; COLISÕES; INTERAÇÕES NUCLEARES
- Idioma: Inglês
- Imprenta:
-
ABNT
BUREN, G. Van et al. The ratio sigmaO/lambda at RHIC. . São Paulo: IFUSP. Disponível em: http://xxx.if.usp.br/PS_cache/nucl-ex/pdf/0512/0512018.pdf. Acesso em: 24 abr. 2024. , 2005 -
APA
Buren, G. V., Szanto de Toledo, A., Moura, M. M. de, Munhoz, M. G., & Suaide, A. A. do P. (2005). The ratio sigmaO/lambda at RHIC. São Paulo: IFUSP. Recuperado de http://xxx.if.usp.br/PS_cache/nucl-ex/pdf/0512/0512018.pdf -
NLM
Buren GV, Szanto de Toledo A, Moura MM de, Munhoz MG, Suaide AA do P. The ratio sigmaO/lambda at RHIC [Internet]. 2005 ;[citado 2024 abr. 24 ] Available from: http://xxx.if.usp.br/PS_cache/nucl-ex/pdf/0512/0512018.pdf -
Vancouver
Buren GV, Szanto de Toledo A, Moura MM de, Munhoz MG, Suaide AA do P. The ratio sigmaO/lambda at RHIC [Internet]. 2005 ;[citado 2024 abr. 24 ] Available from: http://xxx.if.usp.br/PS_cache/nucl-ex/pdf/0512/0512018.pdf - Neutral pion production in d-Au collisions at ''S IND.NN' POT. 1/2 '= 200 GeV'
- Dissipation and fragmentation of low-Q^2 scattered partons in Au-Au collisions at RHIC
- Soft physics from STAR
- Anisotropic flow in AuAu and CuCu at 62 GeV and 200 GeV
- Transverse-momentum $p_t$ correlations on $(\eta, \phi)$ from mean-$p_{t}$ fluctuations in Au-Au collisions at $\sqrt{s_{NN}} = $ 200 GeV
- AA versus pp and dA: A puzzling scaling in HBT@RHIC
- High transverse momentum Xi baryon correlations in p+p collisions at s^(1/2)=200 GeV
- Charged kaon results from dAu and pp collisions at 's ANTIPOT. NN''POT. 1/2' = 200 GeV
- The geometry of hadronization in Au+Au collisions at 'ANTIPOT. s NN''POT. 1/2' = 130 and 200 GeV studied with charge-dependent, two-particle number fluctuations and correlations
- Quantum interference in ''rô'GRAUS' production in ultra-peripheral heavy ion collisions
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