Difference between revisions of "2012 NSF Proposal"

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[[File:09142012_C_slide3.pdf]]
 
[[File:09142012_C_slide3.pdf]]
  
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==CLAS Polarized Structure Function==
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[[NSF_2012_CLAS_PSF]]
  
 
===== The CLAS12 Polarized Structure Function Program =====
 
===== The CLAS12 Polarized Structure Function Program =====
  
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\paragraph{The CLAS12 Polarized Structure Function Program}
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\paragraph{The CLAS12 Polarized  
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Spin structure functions of the nucleon have been measured in deep inelastic lepton scattering (DIS) for nearly 30 years since the first experiments at SLAC. Interest increased substantially in the 1980s when the EMC collaboration reported that quarks only made a small contribution to the overall spin of the proton. This ``spin crisis" led to a vigorous theoretical and experimental effort that continues to this day.  A substantially amount of data has been collected at CERN, SLAC, DESY, and JLab with covers a kinematic range that is sensitive to both valence quarks and the quark-antiquark pairs. 
 
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Interest in the quark contribution to a nucleon's structure continues unabated. At large Bjorken $x$, new data from JLab address for the first time the question of the helicity structure of the nucleon in a kinematic realm where sea quark and gluon contributions are minimal thereby making one mostly sensitive to valence quarks. An example of these results is shown in Fig.~\ref{deltadJLab}. To extend this region to higher $x$ and moderate $Q^2$, one needs higher beam energies than presently available at JLab. In particular, to test various models of the asymptotic value of the virtual photon asymmetry $A_1(x)$ as $x \rightarrow 1$, one needs the upgraded CEBAF with 12~GeV beam energy.
 
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\singlespace
 
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\begin{figure} [t]
 
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\begin{center}
 
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{
 
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\scalebox{0.4} [0.5]{\includegraphics[height=5in]{figs/DeltaDoverD_CLAS12.eps}}
 
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\caption{The expected statistical uncertainty of a $\Delta d/d$ measurement from CLAS12.  The dashed line represents a pQCD prediction while the solid line represents the prediction from a hyperfine perturbed constituent quark model. The solid triangles are measurements from X.~Zheng {\it et al.}~\cite{Zhang}, and the diamonds are from A.~Airapetian {\it et al.}~\cite{AirapetianHERMES}. The squares represent a prediction of the precision obtained by a SIDIS measurement performed using the energy upgraded CEBAF and the upgraded CLAS. The risers represent systematic uncertainty and the error bar lines are statistical uncertainties.}
 
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\label{deltadJLab}
 
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\end{center}
 
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\end{figure}
 
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\doublespace
 
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The comprehensive data set to be collected by experiment PR12-06-109 will contribute substantially to our knowledge of polarized parton distribution functions for all quark flavors and even the polarized gluon distribution $\Delta g$. Through Next-to-Leading Order (NLO) analysis of the world data on inclusive DIS (using the DGLAP evolution equations), one can constrain these distribution functions and their integrals. Existing CLAS data from 6 GeV have already made an impact on these fits. The expected data from the proposed experiment at 11~GeV will further reduce the uncertainties of these distributions. Semi-inclusive DIS (SIDIS) data will also be collected, where, in addition to the scattered electron,  hadrons produced after the struck quark hadronizes are also detected. These data will further constrain the NLO fits and improve the separation of the various quark flavors' contribution to nucleon observables.
 
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{| border="1"  |cellpadding="20" cellspacing="0
 
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| [[File:DeltaDoverD_CLAS12.png]]
 
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| The dashed line represents a pQCD prediction while the solid line represents the prediction from a hyperfine perturbed constituent quark model.  The solid triangles are measurements from X.~Zheng {\it et al.}, Phys.~Rev.~Lett.~92 (2004) 012004 and the diamonds are from Phys.Rev.D71:012003,2005.  The squares represent a prediction of the precision obtained by a SIDIS measurement performed using and energy upgrade CEBAF and the upgraded CLAS.  The risers represent systematic uncertainty and the error bar lines are statistical uncertainties.
 
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[[NSF]]
 
[[NSF]]

Revision as of 02:14, 22 October 2012

The competition

000416256

JeV

Institution 2 year Budget Physics
ASU 340 http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969201
Rutgers 800 http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969239
CS LA 264 http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969380
Catholic 328 http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969434
Catholic 311 http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=1019521
Ohio U 484 http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969297
Hampton 509 http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=1002644
RPI 520 http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0965606
Kent State 465 http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969129
Ohio Univ 327 http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969788

Physics topics

5 students

Section on training our JLab students in Hardware


Student do physics at JLab and gain experience with hardware using ISU facilities.

CLAS can also be categorized as a bunch of "One off" experiments. Perhaps review publication record of the experiments. PV experiments take 10 years from construction to publication some CLAS experiments took less.


Project Personnel Status pgs
[math] \frac{\Delta d}{d}[/math] Polarization Forest Approved 2
N* Cole Approved 3
[math]G_E^p(Q^2=0)[/math] Khandaker , McNulty Approved 2
PV (nucleus size, weak mixing angle, astro physics) McNulty Cond. Approved 3



File:09142012 A SDME.pdf

File:09142012 B Ks.pdf

File:09142012 C slide3.pdf

CLAS Polarized Structure Function

NSF_2012_CLAS_PSF

The CLAS12 Polarized Structure Function Program

\paragraph{The CLAS12 Polarized

NSF

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