[Brahms-l] Fw: Release of STAR PRC on Flow

From: flemming videbaek <videbaek@rcf.rhic.bnl.gov>
Date: Wed Sep 22 2004 - 18:19:43 EDT
FYI
----------------------------------------------------------------
Flemming Videbaek
Physics Department
Brookhaven National Laboratory

e-mail: videbaek@bnl.gov
phone: 631-344-4106
----- Original Message ----- 
From: "Timothy Hallman" <hallman@bnl.gov>
To: "Kirk, Tom" <tkirk@bnl.gov>; "William A. Zajc"
<zajc@nevis.columbia.edu>; "'Wit Busza'" <busza@MIT.EDU>; "Videbaek,
Flemming" <videbaek@bnl.gov>
Cc: <Hallman@bnl.gov>
Sent: Wednesday, September 22, 2004 4:36 PM
Subject: Release of STAR PRC on Flow


> Dear Tom, Bill, Flemming, and Wit,
>
> I am pleased to announce STAR's intention to submit a new
> paper on:
>
> "Azimuthal anisotropy in Au+Au collisions at roots_NN = 200 GeV"
>
> to Physical Review C one week from today. The title and
> abstract for the paper are enclosed.
>
>                         Sincerely,
>
>                              Tim
>
>
>
>
>
> Title:     "Azimuthal anisotropy in Au+Au collisions at roots_NN = 200
GeV"
>
> Abstract:   The results from the STAR Collaboration on directed flow (v1),
>             elliptic flow (v2), and the fourth harmonic (v4) in the
>             anisotropic azimuthal distribution of particles from Au+Au
>             collisions at roots_NN = 200 GeV are summarized and compared
>             with results from other experiments and theoretical models.
>             Results for identified particles are presented and fit with
>             a Blast Wave model. For v2, scaling with the number of
>             constituent quarks and parton coalescence is discussed. For
v4,
>             scaling with v2**2 and quark coalescence predictions for
higher
>             harmonic flow is discussed. The different anisotropic flow
>             methods are compared and nonflow effects are extracted from
>             the data.
>


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Received on Wed Sep 22 18:15:57 2004

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