[Brahms-l] Fw: New PHENIX PRL submission "Evidence for a long-range component in the pion emission source in Au+Au collisions at \sqrtsNN=200~GeV "

FYI
--------------------------------------------
Flemming Videbaek
Physics Department
Bldg 510-D
Brookhaven National Laboratory
Upton, NY11973

phone: 631-344-4106
cell:       631-681-1596
fax:        631-344-1334
e-mail: videbaek @ bnl.gov
----- Original Message ----- 
From: "W.A. Zajc" <zajc@nevis.columbia.edu>
To: "'Wit Busza'" <busza@MIT.EDU>; "'Timothy Hallman'" <hallman@bnl.gov>; "'Flemming Videbaek'" <videbaek@rcf.rhic.bnl.gov>; "'Bond, 
Peter D'" <bond@bnl.gov>
Sent: Friday, May 19, 2006 8:57 PM
Subject: New PHENIX PRL submission "Evidence for a long-range component in the pion emission source in Au+Au collisions at 
\sqrtsNN=200~GeV "


> Dear Wit, Tim, Flemming and Peter:
>
> The PHENIX Collaboration will submit in one week's time to Physical Review
> Letters a manuscript on an HBT-based analysis of the pion emission source in
> 200 GeV Au+Au collisions. The title and abstract are included below.
>
> Best regards,
>
> Bill
>
> ----------------------------------------------------------------------------
> ---------------------------------------------------------------
>
> TITLE: Evidence for a long-range component in the pion emission source in
> Au+Au collisions at \sqrtsNN=200~GeV
>
>
> ABSTRACT:
>
> Emission source functions are extracted from correlation functions
> constructed from charged pions produced at mid-rapidity in Au+Au collisions
> at \sqrtsNN=200~GeV. The source parameters extracted from these functions at
> low $k_T$, give first indications of a long tail for the pion emission
> source. The source extension cannot be explained solely by simple kinematic
> considerations. The possible role of a halo of secondary pions from
> resonance emissions is explored.
> 

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