![]() |
|||||||
STAR Newsletter #77December 2000 |
|||||||
| Star Home Page |
Editor: Howard Matis
|
||||||
I would like to say that the STAR Analysis Workshop, held at LBNL on 15 - 19 November, was a pleasure to attend. The status of the various topics of physics analysis in STAR and that of papers in progress were discussed. The day with the theorists was very informative and will be useful as we develop our understanding of the data and what it is telling us. I look forward to having another meeting of this type in the future.
I have placed a draft white paper for STAR's long range plan and its accompanying report of the STAR Long Range Plan Committee on the web. The next Long Range Plan Workshop will be held at BNL on December 8. This workshop will focus on the physics and upgrades of RHIC and its detectors. Information on this workshop the its agenda can also be found on the web.
The STAR Elliptic Flow Paper has been accepted by Physical Review Letters and is scheduled tentatively for the issue which will appear on January 8, 2001.
Talks from the RHIC experiments for Quark Matter 2001 will be decided by the Program Committee next week (December 6 - 8).
I am looking forward to seeing everyone at the next STAR Collaboration Meeting in Austin, Texas (7 - 11 January 2001). The schedule is as follows (updated -December 7):
- Sunday, Jan. 7 - Plenary Presentation of New/Updated Data for Quark Matter
- Monday, Jan. 8 - Physics Working Group Meetings
- Tuesday, Jan. 9 - Plenary Session (Physics and QM Talks)
- Wednesday, Jan. 10 - Plenary Session (QM Talks, Other topics)
- Thursday, Jan. 11 - Council Meeting and Physics Working Group Meetings (adjourn by ~ 4 PM)
I will consult with the Physics Working Group Convenors to optimize the agenda and then send out a more detailed schedule.
The Brookhaven Program Advisory Meeting was held at BNL on November 30 and December 1. I presented the Beam Use Proposal for STAR. Yes, we will get beam. The PAC and BNL have decided that Plan B will be the operating scenario for RHIC next year. This will mean that we will close-up STAR in the Wide-Angle Hall on May 1, and commence running once the machine is up to full energy with Au (expected to be ~ 2 weeks). The run will last into FY 2002 (past October 2001). The present operating scenario can be found on the BNL web site.
Les Bland and I made presentations before the PAC of the STAR Proposal to complete the full EMC including pre-shower detectors. The recommendation from the PAC is that STAR should complete the full barrel. However, the PAC had questions regarding the pre-shower detector (PSD). The PSD was the new scope that we have proposed to add to the EMC, as compared to the EMC in previous PAC reviews. Since the pre-shower detector is essential for electron identification / hadron suppression (it gains us a factor of ~ 3 suppression of hadrons, or factor of 9 for electron pairs) we must make our case to be able to complete the PSD's. The PAC has provided us with a list of questions and asked us to submit to a separate PSD review, before they decide about incorporating the PSD's into the scope of the barrel EMC. I am consulting with the EMC Task Force to determine the best course of action and the time scale of our response and the review. I am confident that we will be successful at this, but this will require more work.
This section contains summaries of the status of the physics working groups. These articles are in a protected area for STAR collaboration members only. This link uses the standard STAR account and password for physics results. If you do not have this information, please contact your council representative.
|
||||||||||||||||||||||||||||||||||||||||||||||
STAR's volleyball team has been enjoying a fun season so far in the Brookhaven volleyball leagues. With many good teams in the league this year, and many new faces on the STAR team, success has not come easy this year. However, we ended November on the high note of our first win for the season and are looking forward to continued improvement! Especially when we face the PHENIX team in December! :-) STAR experimenters who have played with the team so far include: Lee Barnby, Bill Christie, Curtis Lansdell, Gaspare LoCurto, Akio Ogawa, Markus Oldenburg, Sylvester Radomski, Dennis Reichhold, and this year's captain, Gene Van Buren.
Applications are invited for a postdoctoral fellow position in the HEP Division at Argonne National Laboratory to start in winter or spring 2001. The major research focus will be the determination of the gluon spin distribution in the proton within the RHIC spin program at the STAR detector. Argonne physicists are collaborating on the construction of the STAR endcap electromagnetic calorimeter, which will play a vital role in measuring the gluon spin. Half of the calorimeter is planned to be installed in summer 2002, with the remainder in summer 2003. The primary responsibilities will involve the construction and testing of a scintillator strip shower maximum detector for the endcap calorimeter. Participation in ongoing experimental programs involving spin is also expected.
This is a two-year appointment with the possibility of renewal for a third year. Interested candidates should have obtained a Ph.D. in experimental nuclear or high energy physics within the last three years. Applicants are requested to send a list of publications, curriculum vitae, and the names of four references no later than January 15, 2001 to H. Spinka, High Energy Physics Division, Building 362, Argonne National Laboratory, Argonne, Illinois 60439.
Return to the Newsletter Index - Last Modified: