<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>0864-084X</journal-id>
<journal-title><![CDATA[Nucleus]]></journal-title>
<abbrev-journal-title><![CDATA[Nucleus]]></abbrev-journal-title>
<issn>0864-084X</issn>
<publisher>
<publisher-name><![CDATA[CUBAENERGIA]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0864-084X2007000100004</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[The qweak experiment: A search for new physics at the tev scale by measurement of the proton's weak charge]]></article-title>
<article-title xml:lang="es"><![CDATA[El experimento qweak: una búsqueda de nueva física en la escala de tev mediante la medición de la carga débil del protón]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Desmond Ramsay]]></surname>
<given-names><![CDATA[]W.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,University of Manitoba Department of Physics and Astronomy ]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>06</month>
<year>2007</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>06</month>
<year>2007</year>
</pub-date>
<numero>41</numero>
<fpage>20</fpage>
<lpage>25</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://scielo.sld.cu/scielo.php?script=sci_arttext&amp;pid=S0864-084X2007000100004&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://scielo.sld.cu/scielo.php?script=sci_abstract&amp;pid=S0864-084X2007000100004&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://scielo.sld.cu/scielo.php?script=sci_pdf&amp;pid=S0864-084X2007000100004&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[El acoplamiento observado del protón al bosón-Z, es decir, la «carga débil» del protón, varía con la escala de distancia. Experimentos de alta energía han medido con gran precisión el acoplamiento a cortas distancias. Qweakrealizará la medición a una transferencia de momentum de sólo 0,3 (GeV/c)2. El «corrimiento» del acoplamiento de altas a bajas energías se puede calcular corrigiendo por efectos de nubes de partículas virtuales en el vacío. Debido a que las correcciones dependen de todas las partículas que existen en la naturaleza, y no únicamente de las descubiertas hasta la fecha, cualquier diferencia entre la carga débil medida a bajas energías y la calculada, podría indicar la existencia de nueva física. Una medición de Qweak al 4% sería sensible a nueva física en la escala de unos cuantos TeV. El experimento Qweak aprovechará el hecho de que el poder analizador longitudinal (que viola la paridad), Az, es proporcional a la carga débil del protón. El experimento intentará medir Az (cuyo valor predicho es -0,3 ppm) con una incertidumbre combinada, estadística y sistemática, del 2,2% correspondiente a una incertidumbre total del 4% en Qweak. Esto requiere de una precisión estadística de 5 x <img src="http:/img/revistas/nuc/nuc41/images/e01044107.jpg" width="18" height="15">, que se puede alcanzar en 2, 200 horas con un haz de electrones de 180 µA, polarizado al 85%, incidente sobre un blanco de hidrógeno líquido de 0,35 m. Un sistema sincronizado de adquisición de datos integrará las señales de corriente del detector sobre cada estado de espín y extraerá la componente que viola paridad, correlacionada con la helicidad.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[The observed coupling of the proton to the Z-boson, i.e. the «weak charge» of the proton, varies with distance scale. The coupling has already been accurately measured at short distances by high energy experiments. Qweak will make the measurement at a momentum transfer of only 0.3 (GeV/c)2. The «running» of the coupling from high to low energy can be calculated by correcting for the effect of clouds of virtual particles in the vacuum. Because the corrections depend on all of nature&#8217;s particles, not only those which have been discovered, a difference between the calculated and measured low energy weak charge could signal new physics. A measurement of Qweak to 4% will be sensitive to new physics at the few TeVscale. The Qweak experiment will use the fact that the parity-violating longitudinal analyzing power, Az, is proportional to the proton&#8217;s weak charge. The experiment plans to measure the predicted Az of -0.3 ppm with a combined statistical and systematic uncertainty of 2.2%, corresponding to a total uncertainty of 4% in Qweak. This requires a statistical precision of 5 x <img src="http:/img/revistas/nuc/nuc41/images/e01044107.jpg" width="19" height="13">, which can be achieved in 2200 hours with an 85% polarized, 180 µA electron beam incident on a 0.35 m liquid hydrogen target. A synchronous data acquisition system will integrate the detector current signals over each spin state and extract the helicity correlated, parity violating component.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[scattering]]></kwd>
<kwd lng="en"><![CDATA[parity]]></kwd>
<kwd lng="en"><![CDATA[proton beams]]></kwd>
<kwd lng="en"><![CDATA[weak charged currents]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="left"><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>CIENCIAS    NUCLEARES</b></font></p>     <p align="left">&nbsp;</p>     <p><strong><font size="4" face="Verdana, Arial, Helvetica, sans-serif">The qweak    experiment: A search for new physics at the tev scale by measurement of the    proton's weak charge </font></strong></p>     <p></p>     <p><font size="3" face="Verdana, Arial, Helvetica, sans-serif">El experimento    qweak: una b&uacute;squeda de nueva f&iacute;sica en la escala de tev mediante    la medici&oacute;n de la carga d&eacute;bil del prot&oacute;n </font></p>     <p></p>     <p>&nbsp;</p>     <p><font size="2" face="Verdana, Arial, Helvetica, sans-serif">W. Desmond Ramsay    (for the Qweak Collaboration)</font></p>     <p></p>     <p><font size="2" face="Verdana, Arial, Helvetica, sans-serif">Department of Physics    and Astronomy, University of Manitoba    ]]></body>
<body><![CDATA[<br>   </font></p>     <p><font size="2" face="Verdana, Arial, Helvetica, sans-serif">rams@triumf.ca    </font></p> <hr>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>ABSTRACT</b></font></p>     <p><font size="2" face="Verdana, Arial, Helvetica, sans-serif">The observed coupling    of the proton to the Z-boson, i.e. the &laquo;weak charge&raquo; of the proton,    varies with distance scale. The coupling has already been accurately measured    at short distances by high energy experiments. Qweak will make the measurement    at a momentum transfer of only 0.3 (GeV/c)2. The &laquo;running&raquo; of the    coupling from high to low energy can be calculated by correcting for the effect    of clouds of virtual particles in the vacuum. Because the corrections depend    on all of nature&#146;s particles, not only those which have been discovered,    a difference between the calculated and measured low energy weak charge could    signal new physics. A measurement of Qweak to 4% will be sensitive to new physics    at the few TeV scale. The Qweak experiment will use the fact that the parity-violating    longitudinal analyzing power, Az, is proportional to the proton&#146;s weak    charge. The experiment plans to measure the predicted Az of -0.3 ppm with a    combined statistical and systematic uncertainty of 2.2%, corresponding to a    total uncertainty of 4% in Qweak. This requires a statistical precision of 5    x <img src="/img/revistas/nuc/n41/e01044107.jpg" width="19" height="11">,    which can be achieved in 2200 hours with an 85% polarized, 180 &micro;A electron    beam incident on a 0.35 m liquid hydrogen target. A synchronous data acquisition    system will integrate the detector current signals over each spin state and    extract the helicity correlated, parity violating component.</font></p> <hr>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>RESUMEN</b></font></p>     <p><font size="2" face="Verdana, Arial, Helvetica, sans-serif">El acoplamiento    observado del prot&oacute;n al bos&oacute;n-Z, es decir, la &laquo;carga d&eacute;bil&raquo;    del prot&oacute;n, var&iacute;a con la escala de distancia. Experimentos de    alta energ&iacute;a han medido con gran precisi&oacute;n el acoplamiento a cortas    distancias. Qweak realizar&aacute; la medici&oacute;n a una transferencia de    momentum de s&oacute;lo 0,3 (GeV/c)2. El &laquo;corrimiento&raquo; del acoplamiento    de altas a bajas energ&iacute;as se puede calcular corrigiendo por efectos de    nubes de part&iacute;culas virtuales en el vac&iacute;o. Debido a que las correcciones    dependen de todas las part&iacute;culas que existen en la naturaleza, y no &uacute;nicamente    de las descubiertas hasta la fecha, cualquier diferencia entre la carga d&eacute;bil    medida a bajas energ&iacute;as y la calculada, podr&iacute;a indicar la existencia    de nueva f&iacute;sica. Una medici&oacute;n de Qweak al 4% ser&iacute;a sensible    a nueva f&iacute;sica en la escala de unos cuantos TeV. El experimento Qweak    aprovechar&aacute; el hecho de que el poder analizador longitudinal (que viola    la paridad), Az, es proporcional a la carga d&eacute;bil del prot&oacute;n.    El experimento intentar&aacute; medir Az (cuyo valor predicho es -0,3 ppm) con    una incertidumbre combinada, estad&iacute;stica y sistem&aacute;tica, del 2,2%    correspondiente a una incertidumbre total del 4% en Qweak. Esto requiere de    una precisi&oacute;n estad&iacute;stica de 5 x <img src="/img/revistas/nuc/n41/e01044107.jpg" width="19" height="13">,    que se puede alcanzar en 2, 200 horas con un haz de electrones de 180 <span style='font-size:10.0pt; font-family:Verdana'><span class=SpellE><font size="2" face="Verdana, Arial, Helvetica, sans-serif">&micro;</font></span></span>A,    polarizado al 85%, incidente sobre un blanco de hidr&oacute;geno l&iacute;quido    de 0,35 m. Un sistema sincronizado de adquisici&oacute;n de datos integrar&aacute;    las se&ntilde;ales de corriente del detector sobre cada estado de esp&iacute;n    y extraer&aacute; la componente que viola paridad, correlacionada con la helicidad.</font></p>     
<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Key words:</b>    scattering; parity; proton beams; weak charged currents; electron beams    <br>   </font></p> <hr>     <p><font size="2" face="Verdana, Arial, Helvetica, sans-serif"><strong>INTRODUCTION</strong></font></p>     ]]></body>
<body><![CDATA[<p><font size="2" face="Verdana, Arial, Helvetica, sans-serif">The <img src="/img/revistas/nuc/n41/e02044107.jpg" width="33" height="18">experiment    [1] (figure 1) plans to make a precision measurement of parity violation in    the elastic scattering of longitudinally polarized electron from protons. A    longitudinally polarized electron beam is passed through a 35 cm thick liquid    hydrogen target and forward scattered electrons are detected using a magnetic    spectrometer and detector system. The experiment measures the fractional difference    in cross section for right-handed and left-handed electron elicities. It is    expected that <img src="/img/revistas/nuc/n41/e03044107.jpg" width="180" height="16">    ppm, the negative sign indicating that the cross section is slightly higher    for the left-handed helicity.</font></p>     
<p><img src="/img/revistas/nuc/n41/f01044107.jpg" width="757" height="249"></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">In conventional,    parity conserving, electron scattering experiments the effective probe is the    photon, which couples to the &laquo;normal&raquo; electromagnetic charge and    current. Many such experiments have been done and the distribution of electric    charge and magnetism in the proton is quite well known. In parity violating    electron scattering experiments, on the other hand, the effective probe is the    Z-boson, which couples to the weak charge. The weak charge of the proton has    not been measured yet. To do this is the goal of the experiment.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">It is well established    that observed charges vary with the distance at which the charge is measured.    For example the electric charge on the electron is given by the Particle Data    Group as 1.60217653(14) x <img src="/img/revistas/nuc/n41/e04044107.jpg" width="23" height="10">C,    where the (14) is the uncertainty in the last two digits - a value of impressive    accuracy. The electromagnetic coupling, which is the square of this charge expressed    in dimensionless units, is <img src="/img/revistas/nuc/n41/e05044107.jpg" width="108" height="18">=    1/137.0359911(46). This is indeed the value measured at a large distance, corresponding    to measurements made at very low momentum transfer (low Q). As the momentum    transfer is increased, corresponding to probing closer and closer to the bare    charge, the observed charge increases [2]. At, <img src="/img/revistas/nuc/n41/e06044107.jpg" width="54" height="17">corresponding    to the mass of the W-boson <img src="/img/revistas/nuc/n41/e17044107.jpg" width="32" height="16">    is ~1/128. This dependence on distance is referred to as &laquo;running&raquo;.    The physical reason for the running is that the bare charge is seen through    the distorting effect of clouds of virtual particles. In the case of QED, fermion    pairs &laquo;screen&raquo; the bare charge and cause it to appear smaller at    larger distances. In the case of the strong coupling of the non-abelian QCD,    the behavior is the opposite. The strong coupling is observed to be larger at    longer distances and very weak close up. The screening behavior in QED and the    anti-screening in QCD have been both calculated and confirmed by experiment    [2,3]. The situation for the weak charge is not as clear. </font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The weak charge    of the proton depends on the weak mixing angle, given by <img src="/img/revistas/nuc/n41/e08044107.jpg" width="67" height="17">,    where g' is the U(1) gauge group coupling and g the SU(2) gauge group coupling,    or by <img src="/img/revistas/nuc/n41/e09044107.jpg" width="69" height="15">,    with Mz and Mw the masses of the Z and W bosons. The actual numerical value    of <img src="/img/revistas/nuc/n41/e10044107.jpg" width="38" height="15">    depends on the renormalization scheme. In terms of the weak mixing angle, the    proton's weak charge is <img src="/img/revistas/nuc/n41/e02044107.jpg" width="33" height="18">=1-4<img src="/img/revistas/nuc/n41/e10044107.jpg" width="38" height="15">+    corrections. The corrections depend on how much has been included in the definition    of <img src="/img/revistas/nuc/n41/e10044107.jpg" width="38" height="15">    (i.e. on the renormalization scheme). Figure 2 shows the running of <img src="/img/revistas/nuc/n41/e10044107.jpg" width="38" height="8">calculated    in the MS (&quot;MS bar&quot;) renormalization scheme [4]. Note that large values    of correspond to small values of correspond to small values of <img src="/img/revistas/nuc/n41/e02044107.jpg" width="33" height="18">.    Also shown on the figure are some existing measurements [5] and the uncertainty    of the proposed measurement.</font></p>     
<p><img src="/img/revistas/nuc/n41/f02044107.jpg" width="755" height="399"></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Because the radiative    corrections, or loop diagrams, which give rise to the running, depend not only    on known particles, but on particles which have not yet been discovered, a departure    from the theoretical predictions could indicate new physics. Our proposed measurement    of falta f&oacute;rmula<img src="/img/revistas/nuc/n41/e02044107.jpg" width="33" height="18">    to 4% corresponds to 0.3% in <img src="/img/revistas/nuc/n41/e10044107.jpg" width="38" height="15">    and would be sensitive to new physics on the few TeV scale. On the other hand,    agreement with the calculations would put strong constraints on Standard Model    extensions.</font></p>     
<p></p>     <p></p>     <p> </p>     ]]></body>
<body><![CDATA[<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>The experiment</b></font></p>     <p><b><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Principle</font></b></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">At forward angles    and low falta f&oacute;rmula<img src="/img/revistas/nuc/n41/e11044107.jpg" width="15" height="17">,    the parity violating analyzing power is [6]</font></p>     
<p><img src="/img/revistas/nuc/n41/e13044107.jpg" width="164" height="25"></p>     
<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">where <img src="/img/revistas/nuc/n41/e18044107.jpg" width="17" height="14">    is the Fermi coupling and a the fine structure constant. Putting in the numbers    and expressing the analyzing power in parts per million (ppm) and the momentum    transfer, Q, in GeV/c, gives.</font></p>     
<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The first term,    proportional to <img src="/img/revistas/nuc/n41/e11044107.jpg" width="15" height="17">,    is for a point-like proton. The second term, proportional to <img src="/img/revistas/nuc/n41/e14044107.jpg" width="16" height="14">,    is a correction involving hadronic form factors. Ideally we would like to run    at low enough <img src="/img/revistas/nuc/n41/e11044107.jpg" width="15" height="17">    that the proton would look like a point and hadronic corrections would be negligible.    Unfortu&shy;nately, lower <img src="/img/revistas/nuc/n41/e11044107.jpg" width="15" height="17">    also reduces our signal, so some compromise is needed. We will use <img src="/img/revistas/nuc/n41/e11044107.jpg" width="15" height="17">=    0.03 (GeV/c)2 and a scattering angle of 8 degrees. Based on standard model calculations    and global fits to existing hadronic data [7], we expect</font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><img src="/img/revistas/nuc/n41/e16044107.jpg" width="16" height="17">=    -0.194 ppm -0.074 ppm = -0.268 ppm.</font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The second term    will be constrained by results from JLab (Gzero, HAPPEX), Mainz (PV-A4), and    MIT-Bates (SAMPLE), so by measuring <img src="/img/revistas/nuc/n41/e16044107.jpg" width="16" height="17">,    we can extract the weak charge,<img src="/img/revistas/nuc/n41/e02044107.jpg" width="33" height="18">    .</font></p>     
]]></body>
<body><![CDATA[<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Equipment</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">    <br>   Figure 3 shows the main parts of the Qweak experiment. The 1.165 GeV electron    beam, longitudinally polarized to more than 85%, enters from the left and passes    through a 35 cm long liquid hydrogen target. Electrons scattered at 8 degrees    pass through a series of collimators and an 8-sector toroidal magnetic spectrometer    to the main detectors. These are eight bars of synthetic quartz each fitted    at both ends with photomultipliers. Quartz was chosen because it is radiation    hard (we expect &gt;300 krad) and is insensitive to gamma, neutron and pion    backgrounds. The bars should operate essentially at counting statistics. The    main detector region will be enclosed in a shielding house. This has been removed    in the figure to show the detectors. The Luminosity monitors are located at    very small forward angles where the analyzing power is almost zero. They will    monitor variations in beam current and also look for effects of target boiling.    </font></p>     <p><img src="/img/revistas/nuc/n41/f03044107.jpg" width="756" height="498"></p>     
<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The spectrometer    is arranged such that inelastic electrons are deflected out away from the main    detectors and positive pions are defected inward. The collimator is designed    so that neutral particles hit the shield house inside the detector window.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The liquid hydrogen    target will be the highest power cryotarget ever. It will be 35 cm long with    a beam heat load of 2200 watts and a total heat load of 2500 watts. To achieve    the cooling, plans are to use a 500 W auxiliary heat exchanger using the end    station refrigerator and a 2000 W heat exchanger using the JLab central helium    liquefier extra capacity. </font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Also shown in figure    3 in the locations marked Region 1, Region 2 and Region 3, are position sensitive    detectors for dedicated low current (~10 nA) counting-mode calibration runs    which will be occasionally made to determine the absolute <img src="/img/revistas/nuc/n41/e11044107.jpg" width="15" height="17">    and study the backgrounds. Since the calibration is a secondary measurement,    only two chambers are used at each location. The pairs can be rotated to measure    all eight octants in 4 runs. When not in use, the chambers will be retracted.</font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The main technical    issues to be addressed can be seen from the expression for <img src="/img/revistas/nuc/n41/e16044107.jpg" width="16" height="17">:</font></p>     
<p><img src="/img/revistas/nuc/n41/e15044107.jpg" width="277" height="72"></p>     
]]></body>
<body><![CDATA[<p></p>     <p></p>     <p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Statistics:    N+ and N-</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Our goal is to    measure <img src="/img/revistas/nuc/n41/e16044107.jpg" width="16" height="17">    with a combined statistical and systematic uncertainty of 2%, corresponding    to &raquo; 4% on , or 0.3% on <img src="/img/revistas/nuc/n41/e07044107.jpg" width="38" height="14">.    We are planning for 5 x <img src="/img/revistas/nuc/n41/e01044107.jpg" width="19" height="13">    statistics. To achieve this in our expected 2200 hours of running demands a    count rate of 6.4 GHz, too high for conventional particle counting techniques.    For this reason the main data taking for the <img src="/img/revistas/nuc/n41/e02044107.jpg" width="33" height="18">experiment    will be done in current mode, using eight detectors running at 800 MHz each.    The detectors are 200 cm x 18 cm x 1.25 cm synthetic quartz bars, each with    two gain 1000 photomultipliers (PMTs), one at each end of the bar. Simulations    and preliminary tests indicate a signal of approximately 6&micro;A from each    PMT. Superimposed on this will be a very small parity violating signal synchronized    with the spin state. The small size of this signal is illustrated in figure.    4. This signal will be integrated over each spin state by precision digital    integrators being designed and built at TRIUMF. A synchronous data acquisition    system will then extract only the helicity-correlated part.</font></p>     
<p><img src="/img/revistas/nuc/n41/f04044107.jpg" width="754" height="403"></p>     
<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Beam polarization:    <img src="/img/revistas/nuc/n41/e19044107.jpg" width="14" height="14"></b></font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">We expect a longitudinal    beam polarization of &gt;85%. As seen from equation (1), any uncertainty in    the beam polarization,<img src="/img/revistas/nuc/n41/e19044107.jpg" width="14" height="14">    , will appear directly as the same fractional uncertainty in. In order to determine    the beam polarization with an absolute uncertainty <img src="/img/revistas/nuc/n41/e16044107.jpg" width="16" height="17">    in. In order to determine the beam polarization with observate uncertainty of    less that 1%, Jefferson Lab is installing a new Hall-C Compton polarimeter.    This polarimeter will be able to run continuously during data taking, unlike    the existing M&oslash;ller polarimeter, for which dedicated runs must be made.    The Compton polarimeter should have no difficulty achieving a statistical precision    of better than 1%, but it will have to be cross-calibrated against the M&oslash;ller    to get the absolute accuracy.</font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">    ]]></body>
<body><![CDATA[<br>   <b>Absolute <img src="/img/revistas/nuc/n41/e11044107.jpg" width="15" height="17"></b></font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Since our desired    <img src="/img/revistas/nuc/n41/e02044107.jpg" width="33" height="18">appears    multiplied by the square of the momentum transfer, any error in <img src="/img/revistas/nuc/n41/e11044107.jpg" width="15" height="17">    is a corresponding error in our extracted <img src="/img/revistas/nuc/n41/e02044107.jpg" width="33" height="18">.    For this reason the experiment is being built with the capability to run in    particle-counting, full-tracking mode. By reducing the beam current to 10 nA    and performing dedicated runs in counting mode with full tracking, we will be    able to make an absolute determination of <img src="/img/revistas/nuc/nuc41/images/e11044107.jpg" width="15" height="17">    to 0.5%. We will also require a detailed field map of the spectrometer magnet.    Dedicated runs including time-of-flight will be used to estimate our background    fraction. </font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Hadronic correction:    <img src="/img/revistas/nuc/n41/e14044107.jpg" width="16" height="14">B</b></font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The <b><img src="/img/revistas/nuc/n41/e14044107.jpg" width="16" height="14"></b>    term will be estimated from a combination of theory and existing experiments.    A considerable body of data already exists on the hadronic form factors, and    by the time <img src="/img/revistas/nuc/n41/e02044107.jpg" width="33" height="18">is    running, more results will be available from the JLab G zero experiment. Our    current estimates are that hadronic structure uncertainties will contribute    1.9% uncertainty to our <img src="/img/revistas/nuc/n41/e02044107.jpg" width="33" height="18">value.</font></p>     
<p> </p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Helicity correlated    beam properties</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Our signal is a    change in the detector current on helicity flip. If the only thing that changed    on helicity flip were the helicity, then the change in detector current would    be the true parity violating signal. Unfortunately, the detector signal also    depends on beam parameters other than helicity. For example, it obviously depends    directly on beam current; it will also depend to a lesser degree on parameters    such as beam position, beam size, and beam energy. Changes in such beam properties,    when coherent with spin flip, can imitate parity violation and introduce a systematic    error in our measurement. The approach to minimizing such systematic errors    is threefold. First, the experiment is designed in such a way as to minimize    the sensitivity to helicity correlated beam properties. Second, machine conditions    are carefully optimized to minimize unwanted changes on helicity flip. In some    cases active feedback may be useful. Third, the actual helicity correlated beam    properties are measured during running, the sesitivities to these properties    are measured, and corrections are made for the resultant systematic error. Of    course, each systematic error correction carries with it an uncertainty which    must be taken into account when quoting the final result. We have carried out    Monte Carlo simulations to estimate our sensitivities to coherent modulations    and have set acceptable limits on the beam parameters. Table 1 shows the results    of GEANT simulations. </font></p>     <p></p>     <p><img src="/img/revistas/nuc/n41/t01044107.jpg" width="755" height="316"></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The conditions    shown are those required to keep each false <img src="/img/revistas/nuc/n41/e16044107.jpg" width="16" height="17">    contribution to &lt; 6 x <img src="/img/revistas/nuc/n41/e01044107.jpg" width="20" height="12">.    Notice that conditions can be traded off. For example if the beam can be held    closer to the neutral axis, then more beam motion can be tolerated. The sensitivity    to position modulation also depends on the symmetry of the apparatus. As noted    in column three, this simulation assumed that the detector bars are positioned    radially to better than 19 mm and that the magnetic field is known to 1.6%.    We do not anticipate any serious problem meeting the beam quality specifications    as the G zero experiment has already achieved a similar quality of beam in Hall-C    [8].</font></p>     
]]></body>
<body><![CDATA[<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The expected contributions    of various sources of uncertainty are summarized in table 2. The errors shown    will lead to a 0.3% determination of <img src="/img/revistas/nuc/n41/e07044107.jpg" width="38" height="14">    . Actually, the raw uncertainty infalta f&oacute;rmula is closer to 0.2%, but    an additional uncertainty associated with QCD corrections applied to the extraction    of <img src="/img/revistas/nuc/n41/e07044107.jpg" width="38" height="14">    raises the </font><font face="Verdana, Arial, Helvetica, sans-serif" size="2">uncertainty    to 0.3%. </font></p>     
<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><img src="/img/revistas/nuc/n41/t02044107.jpg" width="756" height="346">    
<br>   <b>Status of the experiment</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The Qweak collaboration    was formed in May 2000. The JLab proposal was approved with an &laquo;A&raquo;    rating in January 2002 and the Technical Design Review was completed in January    2003. In 2003 and 2004 funding was approved by DOE, NSF and NSERC. In January    2005 a further JLab &laquo;Jeopardy&raquo; proposal was approved, again with    &laquo;A&raquo; rating. Here is a summary of the state of the major sub-systems:</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">&middot; All the    magnet parts are at MIT and have been assembled and surveyed. We expect to power    up the magnet in the summer of 2007 and perform a magnetic field map. Once this    is complete the magnet can be delivered to Jefferson Lab. The magnet should    ship to JLab in the summer of 2008.    <br>   &middot; The first prototype digital integrator for the main current-mode running    has been tested at TRIUMF and shipped to JLab for further testing. Following    tests in 2007, more digital integrators and low noise preamplifiers will be    built at TRIUMF and delivered to JLab.    <br>   &middot; All the quartz bars needed for the 8 main detectors are now at JLab    and are undergoing quality control testing. Work is also proceeding at JLab    on design and testing of the low-gain photomultiplier and base package.    <br>   &middot; Design is proceeding well on the liquid hydrogen target. Work now is    concentrating of heat exchanger design.     <br>   &middot; Prototypes of most of the tracking chambers have been built and are    being tested.    ]]></body>
<body><![CDATA[<br>   &middot; A luminosity monitor (lumi) will be tested at JLab in 2007.    <br>   &middot; JLab engineers have produced a full 3D CAD model of the experiment.    This will be vital to verify the interfaces between different parts of the experiment    and the fitting of the experiment in Hall-C.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Installation of    the experiment in Hall-C is scheduled to begin in March, 2009.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Acknowledgments</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">This work is supported    in part by the US DOE, NSF, NSERC (Canada), Jefferson Laboratory and TRIUMF.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>References</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">[1] CARLINI R,    et al. The Qweak Collaboration. Jefferson Lab. Proposal E05-008. 2005.    <!-- ref --><br>   [2] LEVINE I, et al. For example. Phys Rev Lett. 1997; ( 78): 424.    <!-- ref --><br>   [3] See Particle Data Group review. J Phys G. 2006; ( 33): 116.    <!-- ref --><br>   [4] ERLER J, RAMSEY-MUSOLF MJ. Phys Rev D. 2005; ( 72): 073003.    <!-- ref --><br>   [5] BENNETT SC, WIEMAN CE. Atomic Cesium. Phys Rev Lett. 1999; ( 82): 2484-5.    <!-- ref --><br>   [6] Wood CS, et al. SLAC E158. Science. 1997; ( 275): 1759.    <!-- ref --><br>   [7] Anthony PL. et al. Phys Rev Lett. 2005; ( 95): 081601.    <!-- ref --><br>   [8] Zeller GP, et al. NuTeV. Phys Rev Lett. 2002; ( 88): 091802.    <!-- ref --><br>   [9]MUSOLF MJ, et al. Physics Reports 1994; (239): 1.    <!-- ref --><br>   [10] YOUNG RD. Jefferson Lab. Private communication. 2006.    <!-- ref --><br>   [11] NAKAHARA K. Eur Phys J A. 2005;( 24): 119.    <br>   </font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Department of Physics    and Astronomy, University of Manitoba    <br>   <a href="mailto:rams@triumf.ca">rams@triumf.ca</a> </font></p>     ]]></body>
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