<?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>0035-001X</journal-id>
<journal-title><![CDATA[Revista mexicana de física]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. mex. fis.]]></abbrev-journal-title>
<issn>0035-001X</issn>
<publisher>
<publisher-name><![CDATA[Sociedad Mexicana de Física]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0035-001X2006000700007</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Can spectroscopic informations be extracted from transfer reactions?]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Mukhamedzhanov]]></surname>
<given-names><![CDATA[A.M]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Nunes]]></surname>
<given-names><![CDATA[F.M]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Texas A & M University College Station Cyclotron Institute]]></institution>
<addr-line><![CDATA[ TX]]></addr-line>
<country>USA</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Michigan State University Department of Physics and Astronomy ]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
<country>U.S.A</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>01</month>
<year>2006</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>01</month>
<year>2006</year>
</pub-date>
<volume>52</volume>
<fpage>30</fpage>
<lpage>34</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2006000700007&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2006000700007&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2006000700007&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[We revise the standard method of extracting spectroscopic factors from transfer reactions and show the strong dependence on the single particle parameters. We propose an alternative method applicable whenever there is a significant contribution from the interior to the reaction amplitude while still being well described within Distorted Wave Born Approximation (DWBA). The energies for such reactions should be well above the Coulomb barrier. The alternative method is based on fixing the contribution of the peripheral part of the reaction amplitude, depending on the Asymptotic Normalisation Coefficient (ANC), through another independent totally peripheral reaction. Then, by combining this information with the transfer data above the barrier, one can determine the spectroscopic factor and control the uncertainty coming from the single particle parameters.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Se revisa el método standard para extraer factores espectroscópicos de reacciones de transferencia y se muestra la fuerte dependencia que el método tiene en los parámetros de partícula independiente. Proponemos un método alternativo aplicable siempre que exista una contribución significante del interior de la amplitud de reacción, además de que el fenómeno pueda describirse adecuadamente con el método aproximado de la onda distorsionada de Born (DWBA). Las energías para esta reacción deben ser dependientes del coeficiente de normalización asintótico (ANC) a través de otra reacción periférica totalmente independiente. De esta forma, al combinar esta información con los datos de transferencia sobre la barrera, es posible determinar el factor espectroscópico y controlar la incertidumbre originada en los parámetros de partícula independiente.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Spectroscopic factors]]></kwd>
<kwd lng="en"><![CDATA[ANC]]></kwd>
<kwd lng="en"><![CDATA[DWBA analysis]]></kwd>
<kwd lng="en"><![CDATA[transfer reactions]]></kwd>
<kwd lng="es"><![CDATA[Factores espectroscópicos]]></kwd>
<kwd lng="es"><![CDATA[ANC]]></kwd>
<kwd lng="es"><![CDATA[análisis DWBA]]></kwd>
<kwd lng="es"><![CDATA[Reacciones de transferencia]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="center"><font face="verdana" size="4"><b>Can spectroscopic informations be extracted from transfer reactions?</b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>A.M. Mukhamedzhanov* and F.M. Nunes**</b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i>* Cyclotron Institute, Texas A &amp; M University, College Station, TX 77843, USA</i></font></p>     <p align="justify"><font face="verdana" size="2"><i>** N.S.C.L. and Department of Physics and Astronomy, Michigan State University, U.S.A.</i></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Recibido el 29 de enero de 2005    <br> Aceptado el 25 de mayo de 2005</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2"><b>Abstract</b></font></p>     <p align="justify"><font face="verdana" size="2">We revise the standard method of extracting spectroscopic factors from transfer reactions and show the strong dependence on the single particle parameters. We propose an alternative method applicable whenever there is a significant contribution from the interior to the reaction amplitude while still being well described within Distorted Wave Born Approximation (DWBA). The energies for such reactions should be well above the Coulomb barrier. The alternative method is based on fixing the contribution of the peripheral part of the reaction amplitude, depending on the Asymptotic Normalisation Coefficient (ANC), through another independent totally peripheral reaction. Then, by combining this information with the transfer data above the barrier, one can determine the spectroscopic factor and control the uncertainty coming from the single particle parameters.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords: </b>Spectroscopic factors; ANC; DWBA analysis; transfer reactions.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>Resumen</b></font></p>     <p align="justify"><font face="verdana" size="2">Se revisa el m&eacute;todo standard para extraer factores espectrosc&oacute;picos de reacciones de transferencia y se muestra la fuerte dependencia que el m&eacute;todo tiene en los par&aacute;metros de part&iacute;cula independiente. Proponemos un m&eacute;todo alternativo aplicable siempre que exista una contribuci&oacute;n significante del interior de la amplitud de reacci&oacute;n, adem&aacute;s de que el fen&oacute;meno pueda describirse adecuadamente con el m&eacute;todo aproximado de la onda distorsionada de Born (DWBA). Las energ&iacute;as para esta reacci&oacute;n deben ser dependientes del coeficiente de normalizaci&oacute;n asint&oacute;tico (ANC) a trav&eacute;s de otra reacci&oacute;n perif&eacute;rica totalmente independiente. De esta forma, al combinar esta informaci&oacute;n con los datos de transferencia sobre la barrera, es posible determinar el factor espectrosc&oacute;pico y controlar la incertidumbre originada en los par&aacute;metros de part&iacute;cula independiente.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Descriptores: </b>Factores espectrosc&oacute;picos; ANC; an&aacute;lisis DWBA; Reacciones de transferencia.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">PACS: 21.10.Jx; 24.10.&#150;i; 24.50.+g; 25.40.Hs</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2"><a href="/pdf/rmf/v52s1/v52s1a7.pdf">DESCARGAR ART&Iacute;CULO EN FORMATO PDF</a></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>Acknowledgments</b></font></p>     <p align="justify"><font face="verdana" size="2">This work has been partially supported by the NSCL at Michigan State University, U. S. DOE under Grant No. DE&#150;FG03&#150;93ER40773, by NSF Award No. PHY&#150;0140343.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>References</b></font></p>     <!-- ref --><p align="justify"><font face="verdana" size="2">1. L. Lapikas, I Wesseling, and R.B. Wiringa, <i>Phys. Rev. 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