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<art>
	<ui>1754-0410-1-6</ui>
	<ji>1754-0410</ji>
	<fm>
		<dochead>Research article</dochead>
		<bibl>
			<title>
				<p>Exclusive <it>&#961;</it><sup>0 </sup>production in deep inelastic scattering at HERA</p>
			</title>
			<aug>
				<au id="A1">
					<cnm>ZEUS Collaboration</cnm>
					<email>gallo@mail.desy.de</email>
				</au>
			</aug>
			<source>PMC Physics A</source>
			<issn>1754-0410</issn>
			<pubdate>2007</pubdate>
			<volume>1</volume>
			<issue>1</issue>
			<fpage>6</fpage>
			<url>http://www.physmathcentral.com/1754-0410/1/6</url>
			<xrefbib>
				<pubid idtype="doi">10.1186/1754-0410-1-6</pubid>
			</xrefbib>
		</bibl>
		<history>
			<rec>
				<date>
					<day>13</day>
					<month>8</month>
					<year>2007</year>
				</date>
			</rec>
			<acc>
				<date>
					<day>12</day>
					<month>11</month>
					<year>2007</year>
				</date>
			</acc>
			<pub>
				<date>
					<day>12</day>
					<month>11</month>
					<year>2007</year>
				</date>
			</pub>
		</history>
		<cpyrt>
			<year>2007</year>
			<collab>Zeus Collaboration; This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/2.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.  </collab>
		</cpyrt>
		<abs>
			<sec>
				<st>
					<p>Abstract</p>
				</st>
				<p>Exclusive <it>&#961;</it><sup>0 </sup>electroproduction at HERA has been studied with the ZEUS detector using 120 pb<sup>-1 </sup>of integrated luminosity collected during 1996&#8211;2000. The analysis was carried out in the kinematic range of photon virtuality 2 &lt;<it>Q</it><sup>2 </sup>&lt; 160 GeV<sup>2</sup>, and <it>&#947;</it>*<it>p </it>centre-of-mass energy 32 &lt;<it>W </it>&lt; 180 GeV. The results include the <it>Q</it><sup>2 </sup>and <it>W </it>dependence of the <it>&#947;</it>*<it>p </it>&#8594; <it>&#961;</it><sup>0</sup><it>p </it>cross section and the distribution of the squared-four-momentum transfer to the proton. The helicity analysis of the decay-matrix elements of the <it>&#961;</it><sup>0 </sup>was used to study the ratio of the <it>&#947;</it>*<it>p </it>cross section for longitudinal and transverse photon as a function of <it>Q</it><sup>2 </sup>and <it>W</it>. Finally, an effective Pomeron trajectory was extracted. The results are compared to various theoretical predictions.</p>
				<p/>
				<p><b>PACS Codes:</b> 13.60.Hb, 13.60.Le</p>
			</sec>
		</abs>
	</fm>
	<bdy>
		<sec>
			<st>
				<p>1 Introduction</p>
			</st>
			<p>Two of the most surprising aspects of high-energy deep inelastic scattering (DIS) observed at the HERA <it>ep </it>collider have been the sharp rise of the proton structure function, <it>F</it><sub>2</sub>, with decreasing value of Bjorken <it>x </it>and the abundance of events with a large rapidity gap in the hadronic final state <abbrgrp><abbr bid="B1">1</abbr></abbrgrp>. The latter are identified as due to diffraction in the deep inelastic regime. A contribution to the diffractive cross section arises from the exclusive production of vector mesons (VM).</p>
			<p>High-energy exclusive VM production in DIS has been postulated to proceed through two-gluon exchange <abbrgrp><abbr bid="B2">2</abbr><abbr bid="B3">3</abbr></abbrgrp>, once the scale, usually taken as the virtuality <it>Q</it><sup>2 </sup>of the exchanged photon, is large enough for perturbative Quantum Chromodynamics (pQCD) to be applicable. The gluons in the proton, which lie at the origin of the sharp increase of <it>F</it><sub>2</sub>, are also expected to cause the VM cross section to increase with increasing photon proton centre-of-mass energy, <it>W</it>, with the rate of increase growing with <it>Q</it><sup>2</sup>. Moreover, the effective size of the virtual photon decreases with increasing <it>Q</it><sup>2</sup>, leading to a flatter distribution in <it>t</it>, the four-momentum-transfer squared at the proton vertex. All these features, with varying levels of significance, have been observed at HERA <abbrgrp><abbr bid="B4">4</abbr><abbr bid="B5">5</abbr><abbr bid="B6">6</abbr><abbr bid="B7">7</abbr><abbr bid="B8">8</abbr><abbr bid="B9">9</abbr><abbr bid="B10">10</abbr></abbrgrp> in the exclusive production of <it>&#961;</it><sup>0</sup>, <it>&#969;</it>, <it>&#966;</it>, and <it>J</it>/<it>&#968; </it>mesons.</p>
			<p>This paper reports on an extensive study of the properties of exclusive <it>&#961;</it><sup>0</sup>-meson production,</p>
			<p>
				<display-formula><it>&#947;</it>*<it>p </it>&#8594; <it>&#961;</it><sup>0</sup><it>p</it>,</display-formula>
			</p>
			<p>based on a high statistics data sample collected with the ZEUS detector during the period 1996&#8211;2000, corresponding to an integrated luminosity of about 120 pb<sup>-1</sup>.</p>
		</sec>
		<sec>
			<st>
				<p>2 Theoretical background</p>
			</st>
			<p>Calculations of the VM production cross section in DIS require knowledge of the <inline-formula><m:math name="1754-0410-1-6-i1" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:mi>q</m:mi><m:mover accent="true"><m:mi>q</m:mi><m:mo>&#175;</m:mo></m:mover></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdghaXjqbdghaXzaaraaaaa@2DE3@</m:annotation></m:semantics></m:math></inline-formula> wave-function of the virtual photon, specified by QED and which depends on the polarisation of the virtual photon. For longitudinally polarised photons, <inline-formula><m:math name="1754-0410-1-6-i2" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>&#947;</m:mi><m:mi>L</m:mi><m:mo>&#8727;</m:mo></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciab=n7aNnaaDaaaleaacqWGmbataeaacqGHxiIkaaaaaa@2EE0@</m:annotation></m:semantics></m:math></inline-formula>, <inline-formula><m:math name="1754-0410-1-6-i1" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:mi>q</m:mi><m:mover accent="true"><m:mi>q</m:mi><m:mo>&#175;</m:mo></m:mover></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdghaXjqbdghaXzaaraaaaa@2DE3@</m:annotation></m:semantics></m:math></inline-formula> pairs of small transverse size dominate <abbrgrp><abbr bid="B3">3</abbr></abbrgrp>. The opposite holds for transversely polarised photons, <inline-formula><m:math name="1754-0410-1-6-i3" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>&#947;</m:mi><m:mi>T</m:mi><m:mo>&#8727;</m:mo></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciab=n7aNnaaDaaaleaacqWGubavaeaacqGHxiIkaaaaaa@2EF0@</m:annotation></m:semantics></m:math></inline-formula>, where <inline-formula><m:math name="1754-0410-1-6-i1" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:mi>q</m:mi><m:mover accent="true"><m:mi>q</m:mi><m:mo>&#175;</m:mo></m:mover></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdghaXjqbdghaXzaaraaaaa@2DE3@</m:annotation></m:semantics></m:math></inline-formula> configurations with large transverse size dominate. The favourable feature of exclusive VM production is that, at high <it>Q</it><sup>2</sup>, the longitudinal component of the virtual photon is dominant. The interaction cross section in this case can be fully calculated in pQCD <abbrgrp><abbr bid="B11">11</abbr></abbrgrp>, with two-gluon exchange as the leading process in the high-energy regime. For heavy vector mesons, such as the <it>J</it>/<it>&#968; </it>or the &#978;, perturbative calculations apply even at <it>Q</it><sup>2 </sup>= 0, as the smallness of the <inline-formula><m:math name="1754-0410-1-6-i1" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:mi>q</m:mi><m:mover accent="true"><m:mi>q</m:mi><m:mo>&#175;</m:mo></m:mover></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdghaXjqbdghaXzaaraaaaa@2DE3@</m:annotation></m:semantics></m:math></inline-formula> dipole originating from the photon is guaranteed by the mass of the quarks.</p>
			<p>Irrespective of particular calculations <abbrgrp><abbr bid="B12">12</abbr></abbrgrp>, in the region dominated by perturbative QCD the following features are predicted:</p>
			<p>&#8226; the total <it>&#947;</it>*<it>p </it>&#8594; <it>Vp </it>cross section, <it>&#963;</it><sub><it>&#947;</it>*<it>p</it></sub>, exhibits a steep rise with <it>W</it>, which can be parameterised as <it>&#963; </it>~ <it>W</it><sup><it>&#948;</it></sup>, with <it>&#948; </it>increasing with <it>Q</it><sup>2</sup>;</p>
			<p>&#8226; the <it>Q</it><sup>2 </sup>dependence of the cross-section, which for a longitudinally polarised photon is expected to behave as <it>Q</it><sup>-6</sup>, is moderated to become <it>Q</it><sup>-4 </sup>by the rapid increase of the gluon density with <it>Q</it><sup>2</sup>;</p>
			<p>&#8226; the distribution of <it>t </it>becomes universal, with little or no dependence on <it>W </it>or <it>Q</it><sup>2</sup>;</p>
			<p>&#8226; breaking of the <it>s</it>-channel helicity conservation (SCHC) is expected.</p>
			<p>In the region where perturbative calculations are applicable, exclusive vector-meson production could become a complementary source of information on the gluon content of the proton. At present, the following theoretical uncertainties have been identified:</p>
			<p>&#8226; the calculation of <it>&#963;</it>(<it>&#947;</it>*<it>p </it>&#8594; <it>Vp</it>) involves the generalised parton distributions <abbrgrp><abbr bid="B13">13</abbr><abbr bid="B14">14</abbr></abbrgrp>, which are not well tested; in addition <abbrgrp><abbr bid="B15">15</abbr></abbrgrp>, it involves gluon densities outside the range constrained by global QCD analyses of parton densities;</p>
			<p>&#8226; higher-order corrections have not been fully calculated <abbrgrp><abbr bid="B16">16</abbr></abbrgrp>; therefore the overall normalisation is uncertain and the scale at which the gluons are probed is not known;</p>
			<p>&#8226; the rapid rise of <it>&#963;</it><sub><it>&#947;</it>*<it>p </it></sub>with <it>W </it>implies a non-zero real part of the scattering amplitude, which is not known;</p>
			<p>&#8226; the wave-functions of the vector mesons are not fully known.</p>
			<p>In spite of all these problems, precise measurements of differential cross sections separated into longitudinal and transverse components <abbrgrp><abbr bid="B17">17</abbr></abbrgrp>, should help to resolve the above theoretical uncertainties.</p>
			<p>It is important in these studies to establish a region of phase space where hard interactions dominate over the non-perturbative soft component. If the relative transverse momentum of the <inline-formula><m:math name="1754-0410-1-6-i1" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:mi>q</m:mi><m:mover accent="true"><m:mi>q</m:mi><m:mo>&#175;</m:mo></m:mover></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdghaXjqbdghaXzaaraaaaa@2DE3@</m:annotation></m:semantics></m:math></inline-formula> pair is small, the colour dipole is large and perturbative calculations do not apply. In this case the interaction looks similar to hadron-hadron elastic scattering, described by soft Pomeron exchange as in Regge phenomenology <abbrgrp><abbr bid="B18">18</abbr></abbrgrp>.</p>
			<p>The parameters of the soft Pomeron are known from measurements of total cross sections for hadron-hadron interactions and elastic proton-proton measurements. It is usually assumed that the Pomeron trajectory is linear in <it>t</it>:</p>
			<p>
				<display-formula id="M1">
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 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=MipeYlH8Hipec8Eeeu0xXdbba9frFj0xb9Lqpepeea0xd9q8qiYRWxGi6xij=hbbc9s8aq0=yqpe0xbbG8A8frFve9Fve9Fj0dmeaabaqaciaacaGaaeqabaqabeGadaaakeaaiiGacqWFXoqydaWgaaWcbaWefv3ySLgznfgDOjdaryqr1ngBPrginfgDObcv39gaiqaacqGFzecuaeqaaOGaeiikaGIaemiDaqNaeiykaKIaeyypa0Jae8xSde2aaSbaaSqaaiab+LriqbqabaGccqGGOaakcqaIWaamcqGGPaqkcqGHRaWkcuWFXoqygaqbamaaBaaaleaacqGFzecuaeqaaOGaemiDaqNaeiOla4caaa@46A8@</m:annotation>
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			<p>The parameter <it>&#945;</it><sub>&#8473;</sub>(0) determines the energy behaviour of the total cross section,</p>
			<p>
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			<p>and <inline-formula><m:math name="1754-0410-1-6-i6" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msub><m:msup><m:mi>&#945;</m:mi><m:mo>&#8242;</m:mo></m:msup><m:mi>&#8473;</m:mi></m:msub></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciqb=f7aHzaafaWaaSbaaSqaamrr1ngBPrwtHrhAYaqeguuDJXwAKbstHrhAGq1DVbaceaGae4xgHafabeaaaaa@3783@</m:annotation></m:semantics></m:math></inline-formula> describes the increase of the slope <it>b </it>of the <it>t </it>distribution with increasing <it>W</it>. The value of <inline-formula><m:math name="1754-0410-1-6-i6" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msub><m:msup><m:mi>&#945;</m:mi><m:mo>&#8242;</m:mo></m:msup><m:mi>&#8473;</m:mi></m:msub></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciqb=f7aHzaafaWaaSbaaSqaamrr1ngBPrwtHrhAYaqeguuDJXwAKbstHrhAGq1DVbaceaGae4xgHafabeaaaaa@3783@</m:annotation></m:semantics></m:math></inline-formula> is inversely proportional to the square of the typical transverse momenta participating in the exchanged trajectory. A large value of <inline-formula><m:math name="1754-0410-1-6-i6" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msub><m:msup><m:mi>&#945;</m:mi><m:mo>&#8242;</m:mo></m:msup><m:mi>&#8473;</m:mi></m:msub></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciqb=f7aHzaafaWaaSbaaSqaamrr1ngBPrwtHrhAYaqeguuDJXwAKbstHrhAGq1DVbaceaGae4xgHafabeaaaaa@3783@</m:annotation></m:semantics></m:math></inline-formula> suggests the presence of low transverse momenta typical of soft interactions. The accepted values of <it>&#945;</it><sub>&#8473;</sub>(0) <abbrgrp><abbr bid="B19">19</abbr></abbrgrp> and <inline-formula><m:math name="1754-0410-1-6-i6" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msub><m:msup><m:mi>&#945;</m:mi><m:mo>&#8242;</m:mo></m:msup><m:mi>&#8473;</m:mi></m:msub></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciqb=f7aHzaafaWaaSbaaSqaamrr1ngBPrwtHrhAYaqeguuDJXwAKbstHrhAGq1DVbaceaGae4xgHafabeaaaaa@3783@</m:annotation></m:semantics></m:math></inline-formula><abbrgrp><abbr bid="B20">20</abbr></abbrgrp> are</p>
			<p>
				<display-formula>
					<m:math name="1754-0410-1-6-i7" xmlns:m="http://www.w3.org/1998/Math/MathML">
						<m:semantics>
							<m:mrow>
								<m:mtable>
									<m:mtr>
										<m:mtd>
											<m:mrow>
												<m:msub>
													<m:mi>&#945;</m:mi>
													<m:mi>&#8473;</m:mi>
												</m:msub>
												<m:mo stretchy="false">(</m:mo>
												<m:mn>0</m:mn>
												<m:mo stretchy="false">)</m:mo>
												<m:mo>=</m:mo>
												<m:mn>1.096</m:mn>
												<m:mo>&#177;</m:mo>
												<m:mn>0.003</m:mn>
											</m:mrow>
										</m:mtd>
									</m:mtr>
									<m:mtr>
										<m:mtd>
											<m:mrow>
												<m:msub>
													<m:msup>
														<m:mi>&#945;</m:mi>
														<m:mo>&#8242;</m:mo>
													</m:msup>
													<m:mi>&#8473;</m:mi>
												</m:msub>
												<m:mo>=</m:mo>
												<m:mn>0.25</m:mn>
												<m:msup>
													<m:mrow>
														<m:mtext>&#160;Gev</m:mtext>
													</m:mrow>
													<m:mrow>
														<m:mo>&#8722;</m:mo>
														<m:mn>2</m:mn>
													</m:mrow>
												</m:msup>
												<m:mo>.</m:mo>
											</m:mrow>
										</m:mtd>
									</m:mtr>
								</m:mtable>
							</m:mrow>
							<m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=MipeYlH8Hipec8Eeeu0xXdbba9frFj0xb9Lqpepeea0xd9q8qiYRWxGi6xij=hbbc9s8aq0=yqpe0xbbG8A8frFve9Fve9Fj0dmeaabaqaciaacaGaaeqabaqabeGadaaakeaafaqadeGabaaabaacciGae8xSde2aaSbaaSqaamrr1ngBPrwtHrhAYaqeguuDJXwAKbstHrhAGq1DVbaceaGae4xgHafabeaakiabcIcaOiabicdaWiabcMcaPiabg2da9iabigdaXiabc6caUiabicdaWiabiMda5iabiAda2iabgglaXkabicdaWiabc6caUiabicdaWiabicdaWiabiodaZaqaaiqb=f7aHzaafaWaaSbaaSqaaiab+LriqbqabaGccqGH9aqpcqaIWaamcqGGUaGlcqaIYaGmcqaI1aqncqqGGaaicqqGhbWrcqqGLbqzcqqG2bGDdaahaaWcbeqaaiabgkHiTiabikdaYaaakiabc6caUaaaaaa@5527@</m:annotation>
						</m:semantics>
					</m:math>
				</display-formula>
			</p>
			<p>The non-universality of <it>&#945;</it><sub>&#8473;</sub>(0) has been established in inclusive DIS, where the slope of the <it>&#947;</it>*<it>p </it>total cross section with <it>W </it>has a pronounced <it>Q</it><sup>2 </sup>dependence <abbrgrp><abbr bid="B21">21</abbr></abbrgrp>. The value of <inline-formula><m:math name="1754-0410-1-6-i6" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msub><m:msup><m:mi>&#945;</m:mi><m:mo>&#8242;</m:mo></m:msup><m:mi>&#8473;</m:mi></m:msub></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciqb=f7aHzaafaWaaSbaaSqaamrr1ngBPrwtHrhAYaqeguuDJXwAKbstHrhAGq1DVbaceaGae4xgHafabeaaaaa@3783@</m:annotation></m:semantics></m:math></inline-formula> can be determined from exclusive VM production at HERA via the <it>W </it>dependence of the exponential <it>b </it>slope of the <it>t </it>distribution for fixed values of <it>W</it>, where <it>b </it>is expected to behave as</p>
			<p>
				<display-formula>
					<m:math name="1754-0410-1-6-i8" xmlns:m="http://www.w3.org/1998/Math/MathML">
						<m:semantics>
							<m:mrow>
								<m:mi>b</m:mi>
								<m:mo stretchy="false">(</m:mo>
								<m:mi>W</m:mi>
								<m:mo stretchy="false">)</m:mo>
								<m:mo>=</m:mo>
								<m:msub>
									<m:mi>b</m:mi>
									<m:mn>0</m:mn>
								</m:msub>
								<m:mo>+</m:mo>
								<m:mn>4</m:mn>
								<m:msub>
									<m:msup>
										<m:mi>&#945;</m:mi>
										<m:mo>&#8242;</m:mo>
									</m:msup>
									<m:mi>&#8473;</m:mi>
								</m:msub>
								<m:mi>ln</m:mi>
								<m:mo>&#8289;</m:mo>
								<m:mfrac>
									<m:mi>W</m:mi>
									<m:mrow>
										<m:msub>
											<m:mi>W</m:mi>
											<m:mn>0</m:mn>
										</m:msub>
									</m:mrow>
								</m:mfrac>
								<m:mo>,</m:mo>
							</m:mrow>
							<m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=MipeYlH8Hipec8Eeeu0xXdbba9frFj0xb9Lqpepeea0xd9q8qiYRWxGi6xij=hbbc9s8aq0=yqpe0xbbG8A8frFve9Fve9Fj0dmeaabaqaciaacaGaaeqabaqabeGadaaakeaacqWGIbGycqGGOaakcqWGxbWvcqGGPaqkcqGH9aqpcqWGIbGydaWgaaWcbaGaeGimaadabeaakiabgUcaRiabisda0GGaciqb=f7aHzaafaWaaSbaaSqaamrr1ngBPrwtHrhAYaqeguuDJXwAKbstHrhAGq1DVbaceaGae4xgHafabeaakiGbcYgaSjabc6gaULqbaoaalaaabaGaem4vaCfabaGaem4vaC1aaSbaaeaacqaIWaamaeqaaaaacqGGSaalaaa@4832@</m:annotation>
						</m:semantics>
					</m:math>
				</display-formula>
			</p>
			<p>where <it>b</it><sub>0 </sub>and <it>W</it><sub>0 </sub>are free parameters. The value of <inline-formula><m:math name="1754-0410-1-6-i6" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msub><m:msup><m:mi>&#945;</m:mi><m:mo>&#8242;</m:mo></m:msup><m:mi>&#8473;</m:mi></m:msub></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciqb=f7aHzaafaWaaSbaaSqaamrr1ngBPrwtHrhAYaqeguuDJXwAKbstHrhAGq1DVbaceaGae4xgHafabeaaaaa@3783@</m:annotation></m:semantics></m:math></inline-formula> can also be derived from the <it>W </it>dependence of <it>d&#963;</it>/<it>dt </it>at fixed <it>t</it>,</p>
			<p>
				<display-formula id="M2">
					<m:math name="1754-0410-1-6-i9" xmlns:m="http://www.w3.org/1998/Math/MathML">
						<m:semantics>
							<m:mrow>
								<m:mfrac>
									<m:mrow>
										<m:mi>d</m:mi>
										<m:mi>&#963;</m:mi>
									</m:mrow>
									<m:mrow>
										<m:mi>d</m:mi>
										<m:mi>t</m:mi>
									</m:mrow>
								</m:mfrac>
								<m:mo stretchy="false">(</m:mo>
								<m:mi>W</m:mi>
								<m:mo stretchy="false">)</m:mo>
								<m:mo>=</m:mo>
								<m:mi>F</m:mi>
								<m:mo stretchy="false">(</m:mo>
								<m:mi>t</m:mi>
								<m:mo stretchy="false">)</m:mo>
								<m:msup>
									<m:mi>W</m:mi>
									<m:mrow>
										<m:mn>2</m:mn>
										<m:mo stretchy="false">[</m:mo>
										<m:mn>2</m:mn>
										<m:msub>
											<m:mi>&#945;</m:mi>
											<m:mi>&#8473;</m:mi>
										</m:msub>
										<m:mo stretchy="false">(</m:mo>
										<m:mi>t</m:mi>
										<m:mo stretchy="false">)</m:mo>
										<m:mo>&#8722;</m:mo>
										<m:mn>2</m:mn>
										<m:mo stretchy="false">]</m:mo>
									</m:mrow>
								</m:msup>
								<m:mo>,</m:mo>
							</m:mrow>
							<m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=MipeYlH8Hipec8Eeeu0xXdbba9frFj0xb9Lqpepeea0xd9q8qiYRWxGi6xij=hbbc9s8aq0=yqpe0xbbG8A8frFve9Fve9Fj0dmeaabaqaciaacaGaaeqabaqabeGadaaakeaajuaGdaWcaaqaaiabdsgaKHGaciab=n8aZbqaaiabdsgaKjabdsha0baakiabcIcaOiabdEfaxjabcMcaPiabg2da9iabdAeagjabcIcaOiabdsha0jabcMcaPiabdEfaxnaaCaaaleqabaGaeGOmaiJaei4waSLaeGOmaiJae8xSde2aaSbaaWqaamrr1ngBPrwtHrhAYaqeguuDJXwAKbstHrhAGq1DVbaceaGae4xgHafabeaaliabcIcaOiabdsha0jabcMcaPiabgkHiTiabikdaYiabc2faDbaakiabcYcaSaaa@5136@</m:annotation>
						</m:semantics>
					</m:math>
				</display-formula>
			</p>
			<p>where <it>F</it>(<it>t</it>) is an arbitrary function. This approach has the advantage that no assumption needs to be made about the <it>t </it>dependence. The first indications from measurements of <it>&#945;</it><sub>&#8473;</sub>(<it>t</it>) in exclusive <it>J</it>/<it>&#968; </it>photoproduction <abbrgrp><abbr bid="B8">8</abbr><abbr bid="B22">22</abbr></abbrgrp> are that <it>&#945;</it><sub>&#8473;</sub>(0) is larger and <inline-formula><m:math name="1754-0410-1-6-i6" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msub><m:msup><m:mi>&#945;</m:mi><m:mo>&#8242;</m:mo></m:msup><m:mi>&#8473;</m:mi></m:msub></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciqb=f7aHzaafaWaaSbaaSqaamrr1ngBPrwtHrhAYaqeguuDJXwAKbstHrhAGq1DVbaceaGae4xgHafabeaaaaa@3783@</m:annotation></m:semantics></m:math></inline-formula> is smaller than those of the above soft Pomeron trajectory.</p>
		</sec>
		<sec>
			<st>
				<p>3 Experimental set-up</p>
			</st>
			<p>The present measurement is based on data taken with the ZEUS detector during two running periods of the HERA <it>ep </it>collider. During 1996&#8211;1997, protons with energy 820 GeV collided with 27.5 GeV positrons, while during 1998&#8211;2000, 920 GeV protons collided with 27.5 GeV electrons or positrons. The sample used for this study corresponds to an integrated luminosity of 118.9 pb<sup>-1</sup>, consisting of 37.2 pb<sup>-1 </sup><it>e</it><sup>+ </sup><it>p </it>sample from 1996&#8211;1997 and 81.7 pb<sup>-1 </sup>from the 1998&#8211;2000 sample (16.7 pb<sup>-1 </sup><it>e</it><sup>- </sup>and 65.0 pb<sup>-1 </sup><it>e</it><sup>+</sup>)<sup>1</sup>.</p>
			<p>A detailed description of the ZEUS detector can be found elsewhere <abbrgrp><abbr bid="B23">23</abbr><abbr bid="B24">24</abbr></abbrgrp>. A brief outline of the components that are most relevant for this analysis is given below.</p>
			<p>Charged particles are tracked in the central tracking detector (CTD) <abbrgrp><abbr bid="B25">25</abbr><abbr bid="B26">26</abbr><abbr bid="B27">27</abbr></abbrgrp>. The CTD consists of 72 cylindrical drift chamber layers, organised in nine superlayers covering the polar-angle<sup>2 </sup>region 15&#176; &lt;<it>&#952; </it>&lt;164&#176;. The CTD operates in a magnetic field of 1.43 T provided by a thin solenoid. The transverse-momentum resolution for full-length tracks is <it>&#963;</it>(<it>p</it><sub><it>T</it></sub>)/<it>p</it><sub><it>T </it></sub>= 0.0058<it>p</it><sub><it>T </it></sub>&#8853; 0.0065 &#8853; 0.0014/<it>p</it><sub><it>T</it></sub>, with <it>p</it><sub><it>T </it></sub>in GeV.</p>
			<p>The high-resolution uranium-scintillator calorimeter (CAL) <abbrgrp><abbr bid="B28">28</abbr><abbr bid="B29">29</abbr><abbr bid="B30">30</abbr><abbr bid="B31">31</abbr></abbrgrp> covers 99.7% of the total solid angle and consists of three parts: the forward (FCAL), the barrel (BCAL) and the rear (RCAL) calorimeters. Each part is subdivided transversely into towers and longitudinally into one electromagnetic section (EMC) and either one (in RCAL) or two (in BCAL and FCAL) hadronic sections. The CAL energy resolutions, as measured under test-beam conditions, are <it>&#963;</it>(<it>E</it>)/<it>E </it>= 0.18/<inline-formula><m:math name="1754-0410-1-6-i10" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msqrt><m:mi>E</m:mi></m:msqrt></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaamaakaaabaGaemyrauealeqaaaaa@2C23@</m:annotation></m:semantics></m:math></inline-formula> for electrons and <it>&#963;</it>(<it>E</it>)/<it>E </it>= 0.35/<inline-formula><m:math name="1754-0410-1-6-i10" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msqrt><m:mi>E</m:mi></m:msqrt></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaamaakaaabaGaemyrauealeqaaaaa@2C23@</m:annotation></m:semantics></m:math></inline-formula> for hadrons, with <it>E </it>in GeV.</p>
			<p>The position of the scattered electron was determined by combining information from the CAL, the small-angle rear tracking detector <abbrgrp><abbr bid="B32">32</abbr></abbrgrp> and the hadron-electron separator <abbrgrp><abbr bid="B33">33</abbr></abbrgrp>.</p>
			<p>In 1998, the forward plug calorimeter (FPC) <abbrgrp><abbr bid="B34">34</abbr></abbrgrp> was installed in the 20 &#215; 20 cm<sup>2 </sup>beam hole of the FCAL with a small hole of radius 3.15 cm in the centre to accommodate the beam pipe. The FPC increased the forward calorimeter coverage by about one unit in pseudorapidity to <it>&#951; </it>&#8804; 5.</p>
			<p>The leading-proton spectrometer (LPS) <abbrgrp><abbr bid="B35">35</abbr></abbrgrp> detected positively charged particles scattered at small angles and carrying a substantial fraction, <it>x</it><sub><it>L</it></sub>, of the incoming proton momentum; these particles remained in the beam-pipe and their trajectories were measured by a system of silicon microstrip detectors, located between 23.8 m and 90.0 m from the interaction point. The particle deflections induced by the magnets of the proton beam-line allowed a momentum analysis of the scattered proton.</p>
			<p>During the 1996&#8211;1997 data taking, a proton-remnant tagger (PRT1) was used to tag events in which the proton dissociates. It consisted of two layers of scintillation counters perpendicular to the beam at <it>Z </it>= 5.15 m. The two layers were separated by a 2 mm-thick lead absorber. The pseudorapidity range covered by the PRT1 was 4.3 &lt;<it>&#951; </it>&lt; 5.8.</p>
			<p>The luminosity was measured from the rate of the bremsstrahlung process <it>ep </it>&#8594; <it>e&#947;p</it>. The photon was measured in a lead-scintillator calorimeter <abbrgrp><abbr bid="B36">36</abbr><abbr bid="B37">37</abbr><abbr bid="B38">38</abbr></abbrgrp> placed in the HERA tunnel at <it>Z </it>= -107 m.</p>
		</sec>
		<sec>
			<st>
				<p>4 Data selection and reconstruction</p>
			</st>
			<p>The following kinematic variables are used to describe exclusive <it>&#961;</it><sup>0 </sup>production and its subsequent decay into a <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>pair:</p>
			<p>&#8226; the four-momenta of the incident electron (<it>k</it>), scattered electron (<it>k'</it>), incident proton (<it>P</it>), scattered proton (<it>P'</it>) and virtual photon (<it>q</it>);</p>
			<p>&#8226; <it>Q</it><sup>2 </sup>= -<it>q</it><sup>2 </sup>= -(<it>k </it>- <it>k'</it>)<sup>2</sup>, the negative squared four-momentum of the virtual photon;</p>
			<p>&#8226; <it>W</it><sup>2 </sup>= (<it>q </it>+ <it>P</it>)<sup>2</sup>, the squared centre-of-mass energy of the photon-proton system;</p>
			<p>&#8226; <it>y </it>= (<it>P</it>&#183;<it>q</it>)/(<it>P</it>&#183;<it>k</it>), the fraction of the electron energy transferred to the proton in its rest frame;</p>
			<p>&#8226; <it>M</it><sub><it>&#960;&#960;</it></sub>, the invariant mass of the two decay pions;</p>
			<p>&#8226; <it>t </it>= (<it>P </it>- <it>P'</it>)<sup>2</sup>, the squared four-momentum transfer at the proton vertex;</p>
			<p>&#8226; three helicity angles, &#934;<sub><it>h</it></sub>, <it>&#952;</it><sub><it>h </it></sub>and <it>&#966;</it><sub><it>h </it></sub>(see Section 9).</p>
			<p>The kinematic variables were reconstructed using the so-called "constrained" method <abbrgrp><abbr bid="B10">10</abbr><abbr bid="B39">39</abbr></abbrgrp>, which uses the momenta of the decay particles measured in the CTD and the reconstructed polar and azimuthal angles of the scattered electron.</p>
			<p>The online event selection required an electron candidate in the CAL, along with the detection of at least one and not more than six tracks in the CTD.</p>
			<p>In the offline selection, the following further requirements were imposed:</p>
			<p>&#8226; the presence of a scattered electron, with energy in the CAL greater than 10 GeV and with an impact point on the face of the RCAL outside a rectangular area of 26.4 &#215; 16 cm<sup>2</sup>;</p>
			<p>&#8226; <it>E </it>- <it>P</it><sub><it>Z </it></sub>> 45 GeV, where <it>E </it>- <it>P</it><sub><it>Z </it></sub>= &#8721;<sub><it>i</it></sub>(<it>E</it><sub><it>i </it></sub>- <inline-formula><m:math name="1754-0410-1-6-i11" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msub><m:mi>p</m:mi><m:mrow><m:msub><m:mi>Z</m:mi><m:mi>i</m:mi></m:msub></m:mrow></m:msub></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdchaWnaaBaaaleaacqWGAbGwdaWgaaadbaGaemyAaKgabeaaaSqabaaaaa@2F5A@</m:annotation></m:semantics></m:math></inline-formula>) and the summation is over the energies and longitudinal momenta of the final-state electron and pions, was imposed. This cut excludes events with high energy photons radiated in the initial state;</p>
			<p>&#8226; the <it>Z </it>coordinate of the interaction vertex within &#177; 50 cm of the nominal interaction point;</p>
			<p>&#8226; in addition to the scattered electron, exactly two oppositely charged tracks, each associated with the reconstructed vertex, and each having pseudorapidity |<it>&#951;</it>| less than 1.75 and transverse momentum greater than 150 MeV; this excluded regions of low reconstruction efficiency and poor momentum resolution in the CTD. These tracks were treated in the following analysis as a <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>pair;</p>
			<p>&#8226; events with any energy deposit larger than 300 MeV in the CAL and not associated with the pion tracks (so-called 'unmatched islands') were rejected <abbrgrp><abbr bid="B40">40</abbr><abbr bid="B41">41</abbr><abbr bid="B42">42</abbr></abbrgrp>.</p>
			<p>In addition, the following requirements were applied to select kinematic regions of high acceptance:</p>
			<p>&#8226; the analysis was restricted to the kinematic regions 2 &lt;<it>Q</it><sup>2 </sup>&lt; 80 GeV<sup>2 </sup>and 32 &lt;<it>W </it>&lt; 160 GeV in the 1996&#8211;1997 data and 2 &lt;<it>Q</it><sup>2 </sup>&lt; 160 GeV<sup>2 </sup>and 32 &lt;<it>W </it>&lt; 180 GeV in the 1998&#8211;2000 sample;</p>
			<p>&#8226; only events in the <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>mass interval 0.65 &lt;<it>M</it><sub><it>&#960;&#960; </it></sub>&lt; 1.1 GeV and with |<it>t</it>| &lt; 1 GeV<sup>2 </sup>were taken. The mass interval is slightly narrower than that used previously <abbrgrp><abbr bid="B10">10</abbr></abbrgrp>, in order to reduce the effect of the background from non-resonant <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>production. In the selected <it>M</it><sub><it>&#960;&#960; </it></sub>range, the resonant contribution is &#8776; 100% (see Section 8).</p>
			<p>The above selection yielded 22,400 events in the 1996&#8211;1997 sample and 49,300 events in the 1998&#8211;2000 sample, giving a total of 71,700 events for this analysis.</p>
		</sec>
		<sec>
			<st>
				<p>5 Monte Carlo simulation</p>
			</st>
			<p>The relevant Monte Carlo (MC) generators have been described in detail previously <abbrgrp><abbr bid="B10">10</abbr></abbrgrp>. Here their main features are summarised.</p>
			<p>The program ZEUSVM <abbrgrp><abbr bid="B43">43</abbr></abbrgrp> interfaced to HERACLES4.4 <abbrgrp><abbr bid="B44">44</abbr></abbrgrp> was used. The effective <it>Q</it><sup>2</sup>, <it>W </it>and <it>t </it>dependences of the cross section were parameterised to reproduce the data <abbrgrp><abbr bid="B42">42</abbr></abbrgrp>.</p>
			<p>The decay angular distributions were generated uniformly and the MC events were then iteratively reweighted using the results of the present analysis for the 15 combinations of matrix elements <inline-formula><m:math name="1754-0410-1-6-i12" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>r</m:mi><m:mrow><m:mi>i</m:mi><m:mi>k</m:mi></m:mrow><m:mrow><m:mn>04</m:mn></m:mrow></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdkhaYnaaDaaaleaacqWGPbqAcqWGRbWAaeaacqaIWaamcqaI0aanaaaaaa@312D@</m:annotation></m:semantics></m:math></inline-formula>, <inline-formula><m:math name="1754-0410-1-6-i13" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>r</m:mi><m:mrow><m:mi>i</m:mi><m:mi>k</m:mi></m:mrow><m:mi>&#945;</m:mi></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdkhaYnaaDaaaleaacqWGPbqAcqWGRbWAaeaaiiGacqWFXoqyaaaaaa@30EF@</m:annotation></m:semantics></m:math></inline-formula> (see Section 9).</p>
			<p>The contribution of the proton-dissociative process was studied with the EPSOFT <abbrgrp><abbr bid="B45">45</abbr></abbrgrp> generator for the 1996&#8211;1997 data and with PYTHIA <abbrgrp><abbr bid="B46">46</abbr></abbrgrp> for the 1998&#8211;2000 data. The <it>Q</it><sup>2</sup>, <it>W </it>and <it>t </it>dependences were parameterised to reproduce the control samples in the data. The decay angular distributions were generated as in the ZEUSVM sample.</p>
			<p>The generated events were processed through the same chain of selection and reconstruction procedures as the data, thus accounting for trigger as well as detector acceptance and smearing effects. For both MC sets, the number of simulated events after reconstruction was about a factor of seven greater than the number of reconstructed data events.</p>
			<p>All measured distributions are well described by the MC simulations. Some examples are shown in Fig. <figr fid="F1">1</figr>, for the <it>W</it>, <it>Q</it><sup>2</sup>, <it>t </it>variables, and the three helicity angles, <it>&#952;</it><sub><it>h</it></sub>, <it>&#966;</it><sub><it>h</it></sub>, and &#934;<sub><it>h</it></sub>, and in Fig. <figr fid="F2">2</figr> for the transverse momentum <it>p</it><sub><it>T </it></sub>of the pions, for different <it>Q</it><sup>2 </sup>bins.</p>
			<fig id="F1">
				<title>
					<p>Figure 1</p>
				</title>
				<caption>
					<p>Comparison between the data and the ZEUSVM MC distributions for (<it>a</it>) <it>W</it>, (<it>b</it>) <it>Q</it><sup>2</sup>, (<it>c</it>) |<it>t</it>|, (<it>d</it>) cos<it>&#952;</it><sub><it>h</it></sub>, (<it>e</it>) <it>&#966;</it><sub><it>h </it></sub>and (<it>f</it>) &#934;<sub><it>h </it></sub>for events with 0.65 &lt;<it>M</it><sub><it>&#960;&#960; </it></sub>&lt; 1.1 GeV and |<it>t</it>| &lt; 1.0 GeV<sup>2</sup></p>
				</caption>
				<text>
					<p>Comparison between the data and the ZEUSVM MC distributions for (<it>a</it>) <it>W</it>, (<it>b</it>) <it>Q</it><sup>2</sup>, (<it>c</it>) |<it>t</it>|, (<it>d</it>) cos<it>&#952;</it><sub><it>h</it></sub>, (<it>e</it>) <it>&#966;</it><sub><it>h </it></sub>and (<it>f</it>) &#934;<sub><it>h </it></sub>for events with 0.65 &lt;<it>M</it><sub><it>&#960;&#960; </it></sub>&lt; 1.1 GeV and |<it>t</it>| &lt; 1.0 GeV<sup>2</sup>. The MC distributions are normalised to the data.</p>
				</text>
				<graphic file="1754-0410-1-6-1"/>
			</fig>
			<fig id="F2">
				<title>
					<p>Figure 2</p>
				</title>
				<caption>
					<p>Comparison between the data and the ZEUSVM MC distributions for the transverse momentum, <it>p</it><sub><it>T</it></sub>, of <it>&#960;</it><sup>+ </sup>and <it>&#960;</it><sup>- </sup>particles, for different ranges of <it>Q</it><sup>2</sup>, as indicated in the figure</p>
				</caption>
				<text>
					<p>Comparison between the data and the ZEUSVM MC distributions for the transverse momentum, <it>p</it><sub><it>T</it></sub>, of <it>&#960;</it><sup>+ </sup>and <it>&#960;</it><sup>- </sup>particles, for different ranges of <it>Q</it><sup>2</sup>, as indicated in the figure. The events are selected to be within 0.65 &lt;<it>M</it><sub><it>&#960;&#960; </it></sub>&lt; 1.1 GeV and |<it>t</it>| &lt; 1.0 GeV<sup>2</sup>. The MC distributions are normalised to the data.</p>
				</text>
				<graphic file="1754-0410-1-6-2"/>
			</fig>
		</sec>
		<sec>
			<st>
				<p>6 Systematics</p>
			</st>
			<p>The systematic uncertainties of the cross section were evaluated by varying the selection cuts and the MC simulation parameters. The following selection cuts were varied:</p>
			<p>&#8226; the <it>E </it>- <it>P</it><sub><it>Z </it></sub>cut was changed within the appropriate resolution of &#177;3 GeV;</p>
			<p>&#8226; the <it>p</it><sub><it>T </it></sub>of the pion tracks (default 0.15 GeV) was increased to 0.2 GeV;</p>
			<p>&#8226; the distance of closest approach of the extrapolated track to the matched island in the CAL was changed from 30 cm to 20 cm;</p>
			<p>&#8226; the <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>-</sup>-mass window was changed to 0.65&#8211;1.2 GeV;</p>
			<p>&#8226; the <it>Z </it>vertex cut was varied by &#177;10 cm;</p>
			<p>&#8226; the rectangular area of the electron impact point on the CAL was increased by 0.5 cm in <it>X </it>and <it>Y </it>;</p>
			<p>&#8226; the energy of an unmatched island was lowered to 0.25 GeV and then raised to 0.35 GeV.</p>
			<p>The dependence of the results on the precision with which the MC reproduces the performance of the detector and the data was checked by varying the following inputs within their estimated uncertainty:</p>
			<p>&#8226; the reconstructed position of the electron was shifted with respect to the MC by &#177;1 mm;</p>
			<p>&#8226; the electron-position resolution was varied by &#177;10% in the MC;</p>
			<p>&#8226; the <it>W</it><sup><it>&#948;</it></sup>-dependence in the MC was changed by varying <it>&#948; </it>by &#177;0.03;</p>
			<p>&#8226; the exponential <it>t</it>-distribution in the MC was reweighted by changing the nominal slope parameter <it>b </it>by &#177;0.5 GeV<sup>-2</sup>;</p>
			<p>&#8226; the angular distributions in the MC were reweighted assuming SCHC;</p>
			<p>&#8226; the <it>Q</it><sup>2</sup>-distribution in the MC was reweighted by (<it>Q</it><sup>2 </sup>+ <inline-formula><m:math name="1754-0410-1-6-i14" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>M</m:mi><m:mi>&#961;</m:mi><m:mn>2</m:mn></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabd2eannaaDaaaleaaiiGacqWFbpGCaeaacqaIYaGmaaaaaa@2EFE@</m:annotation></m:semantics></m:math></inline-formula>)<sup><it>k</it></sup>, where <it>k </it>= &#177;0.05.</p>
			<p>The largest uncertainty of about &#177; 4% originated from the variation of the energy of the unmatched islands. All the other checks resulted on average in a 0.5% change in the measured cross sections. All the systematic uncertainties were added in quadrature. In addition, the cross-section measurements have an overall normalisation uncertainty of &#177;2% due to the luminosity measurement.</p>
		</sec>
		<sec>
			<st>
				<p>7 Proton dissociation</p>
			</st>
			<p>The production of <it>&#961;</it><sup>0 </sup>mesons may be accompanied by the proton-dissociation process, <it>&#947;</it>*<it>p </it>&#8594; <it>&#961;</it><sup>0</sup><it>N</it>. For low masses <it>M</it><sub><it>N </it></sub>of the dissociative system <it>N</it>, the hadronisation products may remain inside the beam-pipe, leaving no signals in the main detector. The contribution of these events to the exclusive <it>&#961;</it><sup>0 </sup>cross section was estimated from MC generators for proton-dissociative processes.</p>
			<p>A class of proton dissociative events for which the final-state particles leave observed signals in the surrounding detectors was used to tune the <it>M</it><sub><it>N </it></sub>and the <it>t </it>distribution in the MC. In the 1998&#8211;2000 running period, these events were selected by requiring a signal in the FPC detector with energy above 1 GeV. The comparison of the data with PYTHIA expectations for the energy distribution in the FPC is shown in Fig. <figr fid="F3">3(a)</figr>. The same procedure was repeated with a sample of <it>&#961;</it><sup>0 </sup>events for which the FPC energy was less than 1 GeV and a leading proton was measured in the LPS detector, with the fraction of the incoming proton momentum <it>x</it><sub><it>L </it></sub>&lt; 0.95. The comparison between the <it>x</it><sub><it>L </it></sub>distribution measured in the data and that expected from PYTHIA is shown in Fig. <figr fid="F3">3(b)</figr>, where the elastic peak in the data (<it>x</it><sub><it>L </it></sub>> 0.95) is also observed. Also shown in Fig. <figr fid="F3">3(c&#8211;e)</figr> is the fraction of proton-dissociative events expected in the selected <it>&#961;</it><sup>0 </sup>sample as a function of <it>Q</it><sup>2</sup>, <it>W </it>and <it>t</it>. The fraction is at the level of 19%, independent of <it>Q</it><sup>2 </sup>and <it>W</it>, but increasing with increasing |<it>t</it>|. The combined use of the FPC and LPS methods leads to an estimate of the proton dissociative contribution for |<it>t</it>| &lt; 1 GeV<sup>2 </sup>of 0.19 &#177; 0.02(stat.) &#177; 0.03(syst.). The systematic uncertainty was estimated by varying the parameters of the <it>M</it><sub><it>N </it></sub>distribution and by changing the FPC cut.</p>
			<fig id="F3">
				<title>
					<p>Figure 3</p>
				</title>
				<caption>
					<p>(<it>a</it>) The energy distribution in the FPC</p>
				</caption>
				<text>
					<p>(<it>a</it>) The energy distribution in the FPC. The data (full dots) are compared to the expectations from the PYTHIA MC, normalised to the data. (<it>b</it>) The <it>x</it><sub><it>L </it></sub>distribution in the LPS. The data (open circles) are compared to the expectations from the PYTHIA MC, normalised to the data for <it>x</it><sub><it>L </it></sub>&lt; 0.95. The extracted fraction of proton-dissociation events, from the FPC data (dots) and from the LPS data (open circles), as a function of (<it>c</it>) <it>Q</it><sup>2</sup>, (<it>d</it>) <it>W </it>and (<it>e</it>) |<it>t</it>|. All events were selected in the <it>&#961;</it><sup>0 </sup>mass window (0.65&#8211;1.1 GeV). The dotted line in (<it>c</it>) and (<it>d</it>) represents a fit of a constant to the proton-dissociation fraction.</p>
				</text>
				<graphic file="1754-0410-1-6-3"/>
			</fig>
			<p>In the 1996&#8211;1997 data-taking period, a similar procedure was applied, after tuning the EPSOFT MC to reproduce events with hits in the PRT1 or energy deposits in the FCAL. The proton-dissociative contribution for |<it>t</it>| &lt; 1 GeV<sup>2 </sup>was determined to be 0.07 &#177; 0.02 after rejecting events with hits in the PRT1 or energy deposits in the FCAL. This number is consistent with that determined from the LPS and FPC because of the different angular coverage of the PRT1.</p>
			<p>After subtraction of the proton-dissociative contribution, a good agreement between the cross sections derived from the two data-taking periods was found. For all the quoted cross sections integrated over <it>t</it>, the overall normalisation uncertainty due to the subtraction of the proton-dissociative contributions was estimated to be &#177; 4% and was not included in the systematic uncertainty. The proton-dissociative contribution was statistically subtracted in each analysed bin, unless stated otherwise.</p>
		</sec>
		<sec>
			<st>
				<p>8 Mass distributions</p>
			</st>
			<p>The <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>-</sup>-invariant-mass distribution is presented in Fig. <figr fid="F4">4</figr>. A clear enhancement in the <it>&#961;</it><sup>0 </sup>region is observed. Background coming from the decay <it>&#966; </it>&#8594; <it>K</it><sup>+ </sup><it>K</it><sup>-</sup>, where the kaons are misidentified as pions, is expected <abbrgrp><abbr bid="B42">42</abbr></abbrgrp> in the region <it>M</it><sub><it>&#960;&#960; </it></sub>&lt; 0.55 GeV. That coming from <it>&#969; </it>events in the decay channel <it>&#969; </it>&#8594; <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>-</sup><it>&#960;</it><sup>0</sup>, where the <it>&#960;</it><sup>0 </sup>remains undetected, contributes <abbrgrp><abbr bid="B42">42</abbr></abbrgrp> in the region <it>M</it><sub><it>&#960;&#960; </it></sub>&lt; 0.65 GeV. Therefore defining the selected <it>&#961;</it><sup>0 </sup>events to be in the window 0.65 &lt;<it>M</it><sub><it>&#960;&#960; </it></sub>&lt; 1.1 GeV ensures no background from these two channels.</p>
			<fig id="F4">
				<title>
					<p>Figure 4</p>
				</title>
				<caption>
					<p>The <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>acceptance-corrected invariant-mass distribution</p>
				</caption>
				<text>
					<p>The <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>acceptance-corrected invariant-mass distribution. The line represent the best fit of the S&#246;ding form to the data in the range 0.65 &lt;<it>M</it><sub><it>&#960;&#960; </it></sub>&lt; 1.1 GeV. The vertical lines indicate the range of masses used for the analysis. The dashed line is the shape of a relativistic Breit-Wigner with the fitted parameters given in the figure. The dotted line is the interference term between the non-resonant background (dash-dotted line) and the <it>&#961;</it><sup>0 </sup>signal.</p>
				</text>
				<graphic file="1754-0410-1-6-4"/>
			</fig>
			<p>In order to estimate the non-resonant <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>background under the <it>&#961;</it><sup>0</sup>, the S&#246;ding parameterisation <abbrgrp><abbr bid="B47">47</abbr></abbrgrp> was fitted to the data, with results shown in the figure. The resulting mass and width values are in agreement with those given in the Particle Data Group <abbrgrp><abbr bid="B48">48</abbr></abbrgrp> compilation. The integrated non-resonant background is of the order of 1% and is thus neglected.</p>
			<p>The <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>mass distributions in different regions of <it>Q</it><sup>2 </sup>and <it>t </it>are shown in Fig. <figr fid="F5">5</figr> and Fig. <figr fid="F6">6</figr>, respectively. The shape of the mass distribution changes neither with <it>Q</it><sup>2 </sup>nor with <it>t</it>. The results of the fit to the S&#246;ding parameterisation are also shown. Note that the interference term decreases with <it>Q</it><sup>2 </sup>as expected but is independent of <it>t</it>, indicating that the non-exclusive background is negligible.</p>
			<fig id="F5">
				<title>
					<p>Figure 5</p>
				</title>
				<caption>
					<p>The <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>acceptance-corrected invariant-mass distribution, for different <it>Q</it><sup>2 </sup>intervals, with mean values as indicated in the figure</p>
				</caption>
				<text>
					<p>The <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>acceptance-corrected invariant-mass distribution, for different <it>Q</it><sup>2 </sup>intervals, with mean values as indicated in the figure. The lines are defined in the caption of Fig. 4.</p>
				</text>
				<graphic file="1754-0410-1-6-5"/>
			</fig>
			<fig id="F6">
				<title>
					<p>Figure 6</p>
				</title>
				<caption>
					<p>The <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>acceptance-corrected invariant-mass distribution, for different <it>t </it>intervals, with mean values as indicated in the figure</p>
				</caption>
				<text>
					<p>The <it>&#960;</it><sup>+</sup><it>&#960;</it><sup>- </sup>acceptance-corrected invariant-mass distribution, for different <it>t </it>intervals, with mean values as indicated in the figure. The lines are defined in the caption of Fig. 4.</p>
				</text>
				<graphic file="1754-0410-1-6-6"/>
			</fig>
		</sec>
		<sec>
			<st>
				<p>9 Angular distributions and decay-matrix density</p>
			</st>
			<p>The exclusive electroproduction and decay of <it>&#961;</it><sup>0 </sup>mesons is described, at fixed <it>W</it>, <it>Q</it><sup>2</sup>, <it>M</it><sub><it>&#960;&#960; </it></sub>and <it>t</it>, by three helicity angles: &#934;<sub><it>h </it></sub>is the angle between the <it>&#961;</it><sup>0 </sup>production plane and the electron scattering plane in the <it>&#947;</it>*<it>p </it>centre-of-mass frame; <it>&#952;</it><sub><it>h </it></sub>and <it>&#966;</it><sub><it>h </it></sub>are the polar and azimuthal angles of the positively charged decay pion in the <it>s</it>-channel helicity frame. In this frame, the spin-quantisation axis is defined as the direction opposite to the momentum of the final-state proton in the <it>&#961;</it><sup>0 </sup>rest frame. In the <it>&#947;</it>*<it>p </it>centre-of-mass system, <it>&#966;</it><sub><it>h </it></sub>is the angle between the decay plane and the <it>&#961;</it><sup>0 </sup>production plane. The angular distribution as a function of these three angles, <it>W</it>(cos <it>&#952;</it><sub><it>h</it></sub>, <it>&#966;</it><sub><it>h</it></sub>, &#934;<sub><it>h</it></sub>), is parameterised by the <it>&#961;</it><sup>0 </sup>spin-density matrix elements, <inline-formula><m:math name="1754-0410-1-6-i15" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>&#961;</m:mi><m:mrow><m:mi>i</m:mi><m:mi>k</m:mi></m:mrow><m:mi>&#945;</m:mi></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciab=f8aYnaaDaaaleaacqWGPbqAcqWGRbWAaeaacqWFXoqyaaaaaa@313D@</m:annotation></m:semantics></m:math></inline-formula>, where <it>i</it>, <it>k </it>= -1, 0, 1 and by convention <it>&#945; </it>= 0, 1, 2, 4, 5, 6 for an unpolarised charged-lepton beam <abbrgrp><abbr bid="B49">49</abbr></abbrgrp>. The superscript denotes the decomposition of the spin-density matrix into contributions from the following photon-polarisation states: unpolarised transverse photons (0); linearly polarised transverse photons (1,2); longitudinally polarised photons (4); and from the interference of the longitudinal and transverse amplitudes (5,6).</p>
			<p>The decay angular distribution can be expressed in terms of combinations, <inline-formula><m:math name="1754-0410-1-6-i12" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>r</m:mi><m:mrow><m:mi>i</m:mi><m:mi>k</m:mi></m:mrow><m:mrow><m:mn>04</m:mn></m:mrow></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdkhaYnaaDaaaleaacqWGPbqAcqWGRbWAaeaacqaIWaamcqaI0aanaaaaaa@312D@</m:annotation></m:semantics></m:math></inline-formula> and <inline-formula><m:math name="1754-0410-1-6-i13" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>r</m:mi><m:mrow><m:mi>i</m:mi><m:mi>k</m:mi></m:mrow><m:mi>&#945;</m:mi></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdkhaYnaaDaaaleaacqWGPbqAcqWGRbWAaeaaiiGacqWFXoqyaaaaaa@30EF@</m:annotation></m:semantics></m:math></inline-formula>, of the density matrix elements</p>
			<p>
				<display-formula>
					<m:math name="1754-0410-1-6-i16" xmlns:m="http://www.w3.org/1998/Math/MathML">
						<m:semantics>
							<m:mrow>
								<m:mtable>
									<m:mtr>
										<m:mtd>
											<m:mrow>
												<m:msubsup>
													<m:mi>r</m:mi>
													<m:mrow>
														<m:mi>i</m:mi>
														<m:mi>k</m:mi>
													</m:mrow>
													<m:mrow>
														<m:mn>04</m:mn>
													</m:mrow>
												</m:msubsup>
											</m:mrow>
										</m:mtd>
										<m:mtd>
											<m:mo>=</m:mo>
										</m:mtd>
										<m:mtd>
											<m:mrow>
												<m:mfrac>
													<m:mrow>
														<m:msubsup>
															<m:mi>&#961;</m:mi>
															<m:mrow>
																<m:mi>i</m:mi>
																<m:mi>k</m:mi>
															</m:mrow>
															<m:mn>0</m:mn>
														</m:msubsup>
														<m:mo>+</m:mo>
														<m:mi>&#949;</m:mi>
														<m:mi>R</m:mi>
														<m:msubsup>
															<m:mi>&#961;</m:mi>
															<m:mrow>
																<m:mi>i</m:mi>
																<m:mi>k</m:mi>
															</m:mrow>
															<m:mn>4</m:mn>
														</m:msubsup>
													</m:mrow>
													<m:mrow>
														<m:mn>1</m:mn>
														<m:mo>+</m:mo>
														<m:mi>&#949;</m:mi>
														<m:mi>R</m:mi>
													</m:mrow>
												</m:mfrac>
												<m:mo>,</m:mo>
											</m:mrow>
										</m:mtd>
									</m:mtr>
									<m:mtr>
										<m:mtd>
											<m:mrow>
												<m:msubsup>
													<m:mi>r</m:mi>
													<m:mrow>
														<m:mi>i</m:mi>
														<m:mi>k</m:mi>
													</m:mrow>
													<m:mi>&#945;</m:mi>
												</m:msubsup>
											</m:mrow>
										</m:mtd>
										<m:mtd>
											<m:mo>=</m:mo>
										</m:mtd>
										<m:mtd>
											<m:mrow>
												<m:mrow>
													<m:mo>{</m:mo>
													<m:mrow>
														<m:mtable columnalign="left">
															<m:mtr columnalign="left">
																<m:mtd columnalign="left">
																	<m:mrow>
																		<m:mfrac>
																			<m:mrow>
																				<m:msubsup>
																					<m:mi>&#961;</m:mi>
																					<m:mrow>
																						<m:mi>i</m:mi>
																						<m:mi>k</m:mi>
																					</m:mrow>
																					<m:mi>&#945;</m:mi>
																				</m:msubsup>
																			</m:mrow>
																			<m:mrow>
																				<m:mn>1</m:mn>
																				<m:mo>+</m:mo>
																				<m:mi>&#949;</m:mi>
																				<m:mi>R</m:mi>
																			</m:mrow>
																		</m:mfrac>
																		<m:mo>,</m:mo>
																	</m:mrow>
																</m:mtd>
																<m:mtd columnalign="left">
																	<m:mrow>
																		<m:mi>&#945;</m:mi>
																		<m:mo>=</m:mo>
																		<m:mn>1</m:mn>
																		<m:mo>,</m:mo>
																		<m:mn>2</m:mn>
																	</m:mrow>
																</m:mtd>
															</m:mtr>
															<m:mtr columnalign="left">
																<m:mtd columnalign="left">
																	<m:mrow>
																		<m:mfrac>
																			<m:mrow>
																				<m:msqrt>
																					<m:mi>R</m:mi>
																				</m:msqrt>
																				<m:msubsup>
																					<m:mi>&#961;</m:mi>
																					<m:mrow>
																						<m:mi>i</m:mi>
																						<m:mi>k</m:mi>
																					</m:mrow>
																					<m:mi>&#945;</m:mi>
																				</m:msubsup>
																			</m:mrow>
																			<m:mrow>
																				<m:mn>1</m:mn>
																				<m:mo>+</m:mo>
																				<m:mi>&#949;</m:mi>
																				<m:mi>R</m:mi>
																			</m:mrow>
																		</m:mfrac>
																		<m:mo>,</m:mo>
																	</m:mrow>
																</m:mtd>
																<m:mtd columnalign="left">
																	<m:mrow>
																		<m:mi>&#945;</m:mi>
																		<m:mo>=</m:mo>
																		<m:mn>5</m:mn>
																		<m:mo>,</m:mo>
																		<m:mn>6</m:mn>
																		<m:mo>,</m:mo>
																	</m:mrow>
																</m:mtd>
															</m:mtr>
														</m:mtable>
													</m:mrow>
												</m:mrow>
											</m:mrow>
										</m:mtd>
									</m:mtr>
								</m:mtable>
							</m:mrow>
							<m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=MipeYlH8Hipec8Eeeu0xXdbba9frFj0xb9Lqpepeea0xd9q8qiYRWxGi6xij=hbbc9s8aq0=yqpe0xbbG8A8frFve9Fve9Fj0dmeaabaqaciaacaGaaeqabaqabeGadaaakeaafaqadeGadaaabaGaemOCai3aa0baaSqaaiabdMgaPjabdUgaRbqaaiabicdaWiabisda0aaaaOqaaiabg2da9aqcfayaamaalaaabaacciGae8xWdi3aa0baaeaacqWGPbqAcqWGRbWAaeaacqaIWaamaaGaey4kaSIae8xTduMaemOuaiLae8xWdi3aa0baaeaacqWGPbqAcqWGRbWAaeaacqaI0aanaaaabaGaeGymaeJaey4kaSIae8xTduMaemOuaifaaiabcYcaSaGcbaGaemOCai3aa0baaSqaaiabdMgaPjabdUgaRbqaaiab=f7aHbaaaOqaaiabg2da9aqaamaaceqabaqbaeaabiGaaaqaaKqbaoaalaaabaGae8xWdi3aa0baaeaacqWGPbqAcqWGRbWAaeaacqWFXoqyaaaabaGaeGymaeJaey4kaSIae8xTduMaemOuaifaaOGaeiilaWcabaGae8xSdeMaeyypa0JaeGymaeJaeiilaWIaeGOmaidabaqcfa4aaSaaaeaadaGcaaqaaiabdkfasbqabaGae8xWdi3aa0baaeaacqWGPbqAcqWGRbWAaeaacqWFXoqyaaaabaGaeGymaeJaey4kaSIae8xTduMaemOuaifaaOGaeiilaWcabaGae8xSdeMaeyypa0JaeGynauJaeiilaWIaeGOnayJaeiilaWcaaaGaay5Eaaaaaaaa@7476@</m:annotation>
						</m:semantics>
					</m:math>
				</display-formula>
			</p>
			<p>where <it>&#949; </it>is the ratio of the longitudinal- to transverse-photon fluxes and <it>R </it>= <it>&#963;</it><sub><it>L</it></sub>/<it>&#963;</it><sub><it>T</it></sub>, with <it>&#963;</it><sub><it>L </it></sub>and <it>&#963;</it><sub><it>T </it></sub>the cross sections for exclusive <it>&#961;</it><sup>0 </sup>production from longitudinal and transverse virtual photons, respectively. In the kinematic range of this analysis, the value of <it>&#949; </it>varies between 0.96 and 1 with an average value of 0.996; hence <inline-formula><m:math name="1754-0410-1-6-i17" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>&#961;</m:mi><m:mrow><m:mi>i</m:mi><m:mi>k</m:mi></m:mrow><m:mn>0</m:mn></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciab=f8aYnaaDaaaleaacqWGPbqAcqWGRbWAaeaacqaIWaamaaaaaa@3091@</m:annotation></m:semantics></m:math></inline-formula> and <inline-formula><m:math name="1754-0410-1-6-i18" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>&#961;</m:mi><m:mrow><m:mi>i</m:mi><m:mi>k</m:mi></m:mrow><m:mn>4</m:mn></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaGGaciab=f8aYnaaDaaaleaacqWGPbqAcqWGRbWAaeaacqaI0aanaaaaaa@3099@</m:annotation></m:semantics></m:math></inline-formula> cannot be distinguished.</p>
			<p>The Hermitian nature of the spin-density matrix and the requirement of parity conservation reduces the number of independent parameters to 15 <abbrgrp><abbr bid="B49">49</abbr></abbrgrp>. A 15-parameter fit was performed to the data and the obtained results are listed in Table <tblr tid="T1">1</tblr> and shown in Fig. <figr fid="F7">7</figr> as a function of <it>Q</it><sup>2</sup>. The published ZEUS results <abbrgrp><abbr bid="B50">50</abbr></abbrgrp> at lower <it>Q</it><sup>2 </sup>values and the expectations of SCHC, when relevant, are also included. The observed <it>Q</it><sup>2 </sup>dependence, expected in some calculations <abbrgrp><abbr bid="B51">51</abbr></abbrgrp> and previously reported by H1 <abbrgrp><abbr bid="B52">52</abbr></abbrgrp>, is driven by the <it>R </it>dependence on <it>Q</it><sup>2 </sup>under the assumption of helicity conservation and natural parity exchange. The significant deviation of <inline-formula><m:math name="1754-0410-1-6-i19" xmlns:m="http://www.w3.org/1998/Math/MathML"><m:semantics><m:mrow><m:msubsup><m:mi>r</m:mi><m:mrow><m:mn>00</m:mn></m:mrow><m:mn>5</m:mn></m:msubsup></m:mrow><m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdkhaYnaaDaaaleaacqaIWaamcqaIWaamaeaacqaI1aqnaaaaaa@2F63@</m:annotation></m:semantics></m:math></inline-formula> from zero shows that SCHC does not hold <abbrgrp><abbr bid="B51">51</abbr></abbrgrp> as was observed previously <abbrgrp><abbr bid="B50">50</abbr><abbr bid="B52">52</abbr></abbrgrp>.</p>
			<tbl id="T1">
				<title>
					<p>Table 1</p>
				</title>
				<caption>
					<p>Spin density matrix elements for electroproduction of <it>&#961;</it><sup>0</sup>, for different intervals of <it>Q</it><sup>2</sup>. The first uncertainty is statistical, the second systematic.</p>
				</caption>
				<tblbdy cols="6">
					<r>
						<c ca="center">
							<p>Element</p>
						</c>
						<c ca="center">
							<p>2 &lt;<it>Q</it><sup>2 </sup>&lt; 3 GeV<sup>2</sup></p>
						</c>
						<c ca="center">
							<p>3 &lt;<it>Q</it><sup>2 </sup>&lt; 4 GeV<sup>2</sup></p>
						</c>
						<c ca="center">
							<p>4 &lt;<it>Q</it><sup>2 </sup>&lt; 6 GeV<sup>2</sup></p>
						</c>
						<c ca="center">
							<p>6 &lt;<it>Q</it><sup>2 </sup>&lt; 10 GeV<sup>2</sup></p>
						</c>
						<c ca="center">
							<p>10 &lt;<it>Q</it><sup>2 </sup>&lt; 100 GeV<sup>2</sup></p>
						</c>
					</r>
					<r>
						<c cspan="6">
							<hr/>
						</c>
					</r>
					<r>
						<c ca="center">
							<p>
								<inline-formula>
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										<m:semantics>
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												<m:msubsup>
													<m:mi>r</m:mi>
													<m:mrow>
														<m:mn>00</m:mn>
													</m:mrow>
													<m:mrow>
														<m:mn>04</m:mn>
													</m:mrow>
												</m:msubsup>
											</m:mrow>
											<m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabdkhaYnaaDaaaleaacqaIWaamcqaIWaamaeaacqaIWaamcqaI0aanaaaaaa@304F@</m:annotation>
										</m:semantics>
									</m:math>
								</inline-formula>
							</p>
						</c>
						<c ca="right">
							<p>
								<inline-formula>
									<m:math name="1754-0410-1-6-i21" xmlns:m="http://www.w3.org/1998/Math/MathML">
										<m:semantics>
											<m:mrow>
												<m:mn>0.590</m:mn>
												<m:mo>&#177;</m:mo>
												<m:msubsup>
													<m:mrow>
														<m:mn>0.006</m:mn>
													</m:mrow>
													<m:mrow>
														<m:mo>&#8722;</m:mo>
														<m:mn>0.010</m:mn>
													</m:mrow>
													<m:mrow>
														<m:mo>+</m:mo>
														<m:mn>0.012</m:mn>
													</m:mrow>
												</m:msubsup>
											</m:mrow>
											<m:annotation encoding="MathType-MTEF">
 MathType@MTEF@5@5@+=feaafiart1ev1aaatCvAUfKttLearuWrP9MDH5MBPbIqV92AaeXatLxBI9gBaebbnrfifHhDYfgasaacH8bkY=wiFfYlOipiY=Hhbbf9v8qqaqFr0xc9vqpe0di9q8qqpG0dHiVcFbIOFHK8Feei0lXdar=Jb9qqFfeaYRXxe9vr0=vr0=LqpWqaaeaabiGaaiaacaqabeaabeqacmaaaOqaaiabicdaWiabc6caUiabiwda1iabiMda5iabicdaWiabgglaXkabicdaWiabc6caUiabicdaWiabicdaWiabiAda2maaDaaaleaacqGHsislcqaIWaamcqGGUaGlcqaIWaamcqaIXaqmcqaIWaamaeaacqGHRaWkcqaIWaamcqGGUaGlcqaIWaamcqaIXaqmcqaIYaGmaaaaaa@417F@</m:annotation>
										</m:semantics>
									</m:math>
								</inline-formula>
							</p>
						</c>
						<c ca="right">
							<p>
								<inline-formula>
									<m:math name="1754-0410-1-6-i22" xmlns:m="http://www.w3.org/1998/Math/MathML">
										<m:semantics>
											<m:mrow>
												<m:mn>0.659</m:mn>
												<m:mo>&#177;</m:mo>
												<m:msubsup>
													<m:mrow>
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