A study of the di-hadron angular correlation function in event by event ideal hydrodynamics (2013)
- Authors:
- Autor USP: NORONHA JUNIOR, JORGE JOSE LEITE - IF
- Unidade: IF
- Subjects: COLISÕES; ÍONS PESADOS; HIDRODINÂMICA
- Language: Inglês
- Abstract: The di-hadron angular correlation function is computed within boost invariant, ideal hydrodynamics for Au+Au collisions at √ sNN = 200 GeV using Monte Carlo Glauber fluctuating initial conditions. When 0 < pT < 3 GeV, the intensity of the flow components and their phases, {vn, Ψn} (n = 2,3), are found to be correlated on an event by event basis to the initial condition geometrical parameters {ε2,n, Φ2,n}, respectively. Moreover, the fluctuation of the relative phase between trigger and associated particles, ∆n = Ψt n−Ψ a n, is found to affect the di-hadron angular correlation function when different intervals of transverse momentum are used to define the trigger and the associated hadron
- Imprenta:
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ABNT
ANDRADE, Rone Peterson Galvão de e NORONHA JUNIOR, Jorge José Leite. A study of the di-hadron angular correlation function in event by event ideal hydrodynamics. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: http://lanl.arxiv.org/pdf/1305.3098v2.pdf. Acesso em: 21 maio 2024. , 2013 -
APA
Andrade, R. P. G. de, & Noronha Junior, J. J. L. (2013). A study of the di-hadron angular correlation function in event by event ideal hydrodynamics. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de http://lanl.arxiv.org/pdf/1305.3098v2.pdf -
NLM
Andrade RPG de, Noronha Junior JJL. A study of the di-hadron angular correlation function in event by event ideal hydrodynamics [Internet]. 2013 ;[citado 2024 maio 21 ] Available from: http://lanl.arxiv.org/pdf/1305.3098v2.pdf -
Vancouver
Andrade RPG de, Noronha Junior JJL. A study of the di-hadron angular correlation function in event by event ideal hydrodynamics [Internet]. 2013 ;[citado 2024 maio 21 ] Available from: http://lanl.arxiv.org/pdf/1305.3098v2.pdf - Causality and existence of solutions of relativistic viscous uid dynamics with gravity
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