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First Penning Trap Mass Measurements beyond the Proton Drip Line

Identifieur interne : 000024 ( Hal/Curation ); précédent : 000023; suivant : 000025

First Penning Trap Mass Measurements beyond the Proton Drip Line

Auteurs : C. Rauth ; D. Ackermann ; K. Blaum ; M. Block ; A. Chaudhuri ; Z. Di ; S. Eliseev ; R. Ferrer ; D. Habs ; F. Herfurth ; F. P. He Berger ; S. Hofmann ; H. J. Kluge ; G. Maero ; A. Martín ; G. Marx ; M. Mukherjee ; J. B. Neumayr ; W. R. Pla ; S. Rahaman ; D. Rodríguez [France] ; C. Scheidenberger ; L. Schweikhard ; P. G. Thirolf ; G. Vorobjev ; C. Weber

Source :

RBID : Hal:in2p3-00337194

Abstract

The masses of six neutron-deficient rare holmium and thulium isotopes close to the proton drip line were determined with the SHIPTRAP Penning trap mass spectrometer. For the first time the masses of the proton-unbound isotopes 144,145Ho and 147,148Tm were directly measured. The proton separation energies were derived from the measured mass values and compared to predictions from mass formulas. The new values of the proton separation energies are used to determine the location of the proton drip line for holmium and thulium more accurately.

Url:
DOI: 10.1103/PhysRevLett.100.012501

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Le document en format XML

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<div type="abstract" xml:lang="en">The masses of six neutron-deficient rare holmium and thulium isotopes close to the proton drip line were determined with the SHIPTRAP Penning trap mass spectrometer. For the first time the masses of the proton-unbound isotopes 144,145Ho and 147,148Tm were directly measured. The proton separation energies were derived from the measured mass values and compared to predictions from mass formulas. The new values of the proton separation energies are used to determine the location of the proton drip line for holmium and thulium more accurately.</div>
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<date type="whenReleased">2008-11-06 14:14:55</date>
<date type="whenProduced">2008</date>
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<forename>Sandrine</forename>
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<idno type="halRefHtml">Physical Review Letters, American Physical Society, 2008, 100, pp.012501. <10.1103/PhysRevLett.100.012501></idno>
<idno type="halRef">Physical Review Letters, American Physical Society, 2008, 100, pp.012501. <10.1103/PhysRevLett.100.012501></idno>
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<idno type="stamp" n="IN2P3">Institut National de Physique Nucléaire et de Physique des Particules</idno>
<idno type="stamp" n="LPC-CAEN">Laboratoire de Physique Corpusculaire de Caen</idno>
<idno type="stamp" n="CNRS">CNRS - Centre national de la recherche scientifique</idno>
<idno type="stamp" n="UNIV-CAEN">Université de Caen</idno>
<idno type="stamp" n="ENSI-CAEN">Ecole Nationale Supérieure d'Ingénieurs de Caen</idno>
<idno type="stamp" n="COMUE-NORMANDIE">Normandie Université</idno>
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<title xml:lang="en">First Penning Trap Mass Measurements beyond the Proton Drip Line</title>
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<forename type="first">C.</forename>
<surname>Rauth</surname>
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<forename type="first">K.</forename>
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<persName>
<forename type="first">M.</forename>
<surname>Block</surname>
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<author role="aut">
<persName>
<forename type="first">A.</forename>
<surname>Chaudhuri</surname>
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<persName>
<forename type="first">Z.</forename>
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<forename type="first">S.</forename>
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<forename type="first">R.</forename>
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<forename type="first">D.</forename>
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<forename type="first">F.</forename>
<surname>Herfurth</surname>
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<persName>
<forename type="first">F.P.</forename>
<surname>Heßberger</surname>
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<persName>
<forename type="first">S.</forename>
<surname>Hofmann</surname>
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<persName>
<forename type="first">H.J.</forename>
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<forename type="first">G.</forename>
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<persName>
<forename type="first">A.</forename>
<surname>Martín</surname>
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<idno type="halAuthorId">210975</idno>
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<forename type="first">G.</forename>
<surname>Marx</surname>
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</author>
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<persName>
<forename type="first">M.</forename>
<surname>Mukherjee</surname>
</persName>
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</author>
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<persName>
<forename type="first">J.B.</forename>
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</author>
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<persName>
<forename type="first">W.R.</forename>
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</author>
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<persName>
<forename type="first">S.</forename>
<surname>Rahaman</surname>
</persName>
<idno type="halAuthorId">59381</idno>
</author>
<author role="aut">
<persName>
<forename type="first">D.</forename>
<surname>Rodríguez</surname>
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</author>
<author role="aut">
<persName>
<forename type="first">C.</forename>
<surname>Scheidenberger</surname>
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<persName>
<forename type="first">L.</forename>
<surname>Schweikhard</surname>
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<author role="aut">
<persName>
<forename type="first">P.G.</forename>
<surname>Thirolf</surname>
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</author>
<author role="aut">
<persName>
<forename type="first">G.</forename>
<surname>Vorobjev</surname>
</persName>
<idno type="halAuthorId">210977</idno>
</author>
<author role="aut">
<persName>
<forename type="first">C.</forename>
<surname>Weber</surname>
</persName>
<idno type="halAuthorId">29213</idno>
</author>
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<idno type="halJournalId" status="VALID">17980</idno>
<idno type="issn">0031-9007</idno>
<idno type="eissn">1079-7114</idno>
<title level="j">Physical Review Letters</title>
<imprint>
<publisher>American Physical Society</publisher>
<biblScope unit="volume">100</biblScope>
<biblScope unit="pp">012501</biblScope>
<date type="datePub">2008</date>
</imprint>
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<idno type="doi">10.1103/PhysRevLett.100.012501</idno>
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<langUsage>
<language ident="en">English</language>
</langUsage>
<textClass>
<classCode scheme="classification">21.10.Dr, 07.75.+h, 23.50.+z, 27.60.+j</classCode>
<classCode scheme="halDomain" n="phys.nexp">Physics [physics]/Nuclear Experiment [nucl-ex]</classCode>
<classCode scheme="halTypology" n="ART">Journal articles</classCode>
</textClass>
<abstract xml:lang="en">The masses of six neutron-deficient rare holmium and thulium isotopes close to the proton drip line were determined with the SHIPTRAP Penning trap mass spectrometer. For the first time the masses of the proton-unbound isotopes 144,145Ho and 147,148Tm were directly measured. The proton separation energies were derived from the measured mass values and compared to predictions from mass formulas. The new values of the proton separation energies are used to determine the location of the proton drip line for holmium and thulium more accurately.</abstract>
</profileDesc>
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