Forward Physics Initiative at RHIC - PowerPoint PPT Presentation

1 / 18
About This Presentation
Title:

Forward Physics Initiative at RHIC

Description:

... coverage of strongly- interacting matter under extreme conditions. Good reason to believe the QCD phase diagram has ... Good reason to think that high(est? ... – PowerPoint PPT presentation

Number of Views:46
Avg rating:3.0/5.0
Slides: 19
Provided by: bnl
Category:

less

Transcript and Presenter's Notes

Title: Forward Physics Initiative at RHIC


1
Forward Physics Initiative at RHIC
F.Videbaek BNL
2
Overview
  • Background
  • Physics and experimental issues.
  • Further explore low-x physics (Gluon Saturation)
  • Polarized spin asymmetries at large xF
  • Fixed Target opportunities
  • Implications for RHIC planning

3
Background
  • Forward physics is at present being explored at
    RHIC by BRAHMS (charged identified hadrons) STAR
    (?0 ), PHENIX (muons), PHOBOS (charged particles)
    and via ZDC, PCAL measurements.
  • Physics opportunities exist for additional
    measurements at RHIC that are not covered in the
    present program, and should lead to new
    measurements with existing or modified detectors.
  • As of now a subset people from Brahms and Phobos
    have been discussing ideas a broader group would
    be helpful to carry this to a proposal and de
    facto experiment stage.

4
  • Such ideas were discussed at a one-day workshop
    in October, and in the BNL Physics Departments
    Planning Groups White-Paper.
  • The ideas brought forward cover a broad range of
    physics interests. It is not clear the execution
    of these can be covered within a single
    experi-mental setup.
  • Some of these ideas have connections to the
    future program with eRHIC In part via
    exploration at large y, small x and through
    possible common detector elements.

5
  • Heavy Ions
  • Low-x physics
  • Gluon saturation is best explored at forward
    rapidities or high energies corresponding to
    small x. The CGC approach is an intriguing
    description of initial state strong interactions
    and offers a connection between RHIC, HERA and
    eRHIC.
  • Extended measurements at forward rapidities will
    offer an additional experimental test of this.
    Particularly important will be p(d)-A, and A-d(p)
    measurements

6
d-Au Nuclear Modification factor at ? 3.2
RdAu compares the yield of negative particles
produced in dAu to the scaled number of
particles with same sign in p-p For d-Au min.bias
data Ncoll7.2 Error shown is systematic for
?3.2.
PRL 91 072305 (2003)
BRAHMS preliminary (DNP, Tucson)
7
What is needed to extend these measurements
significantly
  • Extend pt reach to 6 GeV/c for inclusive
    spectra.
  • Kinematic limit restrict such measurements to h
    2-3.5
  • Momenta and PID determination in range of 20-60
    GeV/c

8
Yields and rates needed.
  • A much larger solid angle than presently in
    Brahms is required.
  • Typical cross section at 5-6 GeV/c is d2N/dptdh
    10-6
  • With a factor 10 in d? and having IP2 with b2
    and with luminosities achieved in d-Au run one
    can extend reach to 6 GeV/c with a small but
    significant statistics (100) events/GeV/c) in a
    nominal RHIC run (10-14 wks) of running.

Ref spectrum Hijing 1.383
9
Straw man Detector
Magnet
Calorimeter
Rich
8
4
1.5
Tracking
Such a design can probably give a factor 10 in
solid angle. For larger rates, and forward jets a
radically different design is needed.
10
Benefits
  • Such a new/modified detector will bring the d-A
    measurements into a pt region where one might
    expect partonic hard scattering, and can quantify
    observed differences.
  • Observing these high-pt particles with the
    opposite side particle production might
    illuminate the question of di-jet vs. gluon
    fusion processes.
  • Making such quantitative measurements of the d-A
    and pp with detailed comparisons to theoretical
    descriptions is relevant to the future e-A
    program at eRHIC.

11
  • Forward Spin Physics
  • Needed measurements in Transverse polarization
    (AN)
  • analyzing power for ? and ?- .
  • pT dependence for fixed xF
  • Analyzing power for jet production
  • ?0 AN have been measured by STAR
  • Additional measurements are possible with Brahms
    but the range in xF is limited due to solid
    angles.

12
Polarized pp AN measurements
STAR, hep-ex/0310058 (PRL)
Low energy data (AGS) show clear differences
between pi-0. At higher energies the models
used to describe the data differ.Large spin
effects reported by STAR for ?s 200 GeV pp
collisions This makes it an appealing
measurement within the RHIC spin program, and has
been discussed within the RHIC spin group.
13
Fixed Target _at_ RHIC
  • Using internal targets, a whole new energy regime
    can be opened up. Potential exists to expand
    RHICs coverage of strongly- interacting matter
    under extreme conditions.
  • Good reason to believe the QCD phase diagram has
    interesting features in the region probed by
    10-100 GeV beams on fixed targets
  • Good reason to think that high(est??) baryon
    densities are created in collisions of beams
    around 20-30 GeV on fixed targets
  • RHIC will carry out some energy scans in coming
    years likely restricted to a few energies
    between 20 and 200 GeV.

14
Motivation
  • Recent intriguing SPS data from NA49 in Kaon
    yields and inverse slopes.

RHIC BEAM Colliding
RHIC BEAM Fixed
15
Some Details
  • Target options gas jet (only few available
    targets) or possibly atomic beam
  • The Physics of first interest have high cross
    sections.
  • Europeans are building a low energy machine
    (30GeV) partly justified by interest in this
    physics But it wont be completed for a decade
    or so.
  • Potential exists to expand the RHIC program into
    a whole new regime via dedicated runs.
  • Work is needed to develop target machine
    operations

16
Other connections
  • Other opportunities are present in diffractive
    physics and Ultra peripheral collisions. These
    are options that could be implemented within an
    area with an open geometry like IP2.
  • Relation to Cosmic ray physics
  • Large uncertainties in knowledge on atmospheric
    interactions, in particular inelasticity
    parameter. Regions of particular interest are
    large xF (0.4-0.9) and lighter ion beams (Fe, N,
    p)
  • Part of this community may be attracted to a
    forward physics program.

17
Incorporating this into RHIC decadal planning
  • The proposed d-A program will require other such
    run(s) within the frame of the decadal plan (and
    a new/modified detector, size to be determined).
  • The spin program would fall into a time-scale
    where polarization and intensities have been
    developed so a (relative) short program can make
    the AN measurements for p- to larger XF
  • A fixed target program is envisioned using an
    existing detector system on a shorter time-scale.

18
Conclusions
  • This initiative is clearly a work in progress,
    and has several options with details still have
    to be worked out. There are though several
    important physics issues that ought to be
    addressed by the RHIC physics program.
  • The region of forward physics do have a clear
    connection, experimental, instrumental as well as
    physics interest to the envisioned program at
    eRHIC.
Write a Comment
User Comments (0)
About PowerShow.com