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		<titleInfo>
			<title>Amplitude analysis of the anomalous decay eta ' -&gt; pi(+) pi(-) gamma</title>
		</titleInfo>
		<name type="personal">
			<namePart type="family">Dai</namePart>
			<namePart type="given">L</namePart>
			<namePart type="given">Y</namePart>
			<role>
				<roleTerm authority="marcrelator" type="text">author</roleTerm>
			</role>
		</name>
		<name type="personal">
			<namePart type="family">Kang</namePart>
			<namePart type="given">X</namePart>
			<namePart type="given">W</namePart>
			<role>
				<roleTerm authority="marcrelator" type="text">author</roleTerm>
			</role>
		</name>
		<name type="personal">
			<namePart type="family">Meissner</namePart>
			<namePart type="given">U</namePart>
			<namePart type="given">G</namePart>
			<role>
				<roleTerm authority="marcrelator" type="text">author</roleTerm>
			</role>
		</name>
		<name type="personal">
			<namePart type="family">Song</namePart>
			<namePart type="given">X</namePart>
			<namePart type="given">Y</namePart>
			<role>
				<roleTerm authority="marcrelator" type="text">author</roleTerm>
			</role>
		</name>
		<name type="personal">
			<namePart type="family">Yao</namePart>
			<namePart type="given">D</namePart>
			<namePart type="given">L</namePart>
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		<originInfo>
			<dateIssued>2018</dateIssued>
		</originInfo>
		<language>English</language>
		<abstract>In this paper we perform an amplitude analysis of eta ' -&gt; pi(+)pi(-)gamma and confront it with the latest BESIII data. Based on the final-state interaction theorem, we represent the amplitude in terms of an Omnes function multiplied by a form factor that corresponds to the contributions from left-hand cuts and right-hand cuts in the inelastic channels. We also take into account the isospin violation effect induced by rho-omega mixing. Our results show that the anomaly contribution is mandatory in order to explain the data. Its contribution to the decay width of Gamma(eta ' -&gt; pi pi gamma) is larger than that induced by isospin violation. Finally we extract the pole positions of the rho and omega as well as their corresponding residues.</abstract>
		<note>WOS:000424904000003</note>
		<note>exported from refbase (https://references.ific.uv.es/refbase/show.php?record=3489), last updated on Mon, 26 Feb 2018 15:49:10 +0000</note>
		<typeOfResource>text</typeOfResource>
		<location>
			<url>http://arxiv.org/abs/1712.02119</url>
		</location>
		<identifier type="uri">http://arxiv.org/abs/1712.02119</identifier>
		<identifier type="doi">10.1103/PhysRevD.97.036012</identifier>
		<identifier type="citekey">Dai_etal2018</identifier>
		<relatedItem type="host">
			<titleInfo>
				<title>Physical Review D</title>
			</titleInfo>
			<titleInfo type="abbreviated">
				<title>Phys. Rev. D</title>
			</titleInfo>
			<originInfo>
				<dateIssued>2018</dateIssued>
				<publisher>Amer Physical Soc</publisher>
				<issuance>continuing</issuance>
			</originInfo>
			<genre authority="marcgt">periodical</genre>
			<genre>academic journal</genre>
			<part>
				<detail type="volume">
					<number>97</number>
				</detail>
				<detail type="issue">
					<number>3</number>
				</detail>
				<extent unit="page">
					<start>036012</start>
					<end>12pp</end>
				</extent>
			</part>
			<identifier type="issn">2470-0010</identifier>
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