[Brahms-l] heavy ion choice for run-5

From: flemming videbaek <videbaek@rcf.rhic.bnl.gov>
Date: Wed Aug 04 2004 - 18:48:58 EDT
about a week ago the exp were asked by t.Kirk, triggered by a CA-D request about the preferred specie for hI running; i responded that the BUP would request Fe i.e. an ion in the mass 60 range.
subsequently he received responses from other exp. the result is decided , and given below.
This has no implications, ie. it is still up to the PAC to decide on relative amount of hI vs pp, and if there should be a lower energy HI run in order of 1 week. This is by the way requested by the other experiments with Phobos asking for a week at 19.6 GeV too. Though the two big exp have yet to submit their proposals (see http://www.bnl.gov/henp/pac0904.asp for the submitted proposals and loi's) they both ask for 10 wks LI and 10 wks pp, with the twist of Phenix, thanks to tannenbaum asking for 1 week of 62.4 gev proton running.

flemming


. August 4, 2004

Colleagues:

In response to the July 26, 2004 email from Thomas
Roser requesting an early decision on the ion species
to be used in the FY05 heavy ion running, I have
investigated the requests of the four RHIC experiments
that will take data in the FY05 run.

After discussing the issue with the spokespersons,
individually, I discovered that three of the four 
collaborations had selected their desired ion from the 
Fe/Cu/Ni group and one, PHOBOS, desired Si.  I also 
asked Thomas Roser if he had a preference among the 
three closely-grouped heavier ions and he reported that 
Cu would yield the best luminosity for this group.

Accordingly, and in the interest of minimizing efforts in
the C-AD for non-productive work in preparing for multiple
heavy ion possibilities that are then not needed, I am 
here directing that the ions for the FY05 heavy ion running 
will be Cu x Cu.

I am aware that this decision comes without discussion
by the PAC but it does reflect the desires of 3/4 of
the BUPs. I further observe that the needs of PHOBOS can 
be met in a future Si run if this emerges as scientifically 
compelling in the RHIC physics program after a first look 
at Cu x Cu data.

Sincerely, Tom Kirk

----------------------------------------------------------------
Flemming Videbaek
Physics Department
Brookhaven National Laboratory

e-mail: videbaek@bnl.gov
phone: 631-344-4106



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Received on Wed Aug 4 18:47:15 2004

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