Measurement of lifetimes in [superscript 23]Mg

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dc.creator Kirsebom, O. S.
dc.creator Bender, P.
dc.creator Cheeseman, A.
dc.creator Christian, G.
dc.creator Churchman, R.
dc.creator Cross, D. S.
dc.creator Davids, B.
dc.creator Evitts, L. J.
dc.creator Fallis, J.
dc.creator Galinski, N.
dc.creator Sanetullaev, Alisher
dc.date.accessioned 2018-01-29T14:31:27Z
dc.date.available 2018-01-29T14:31:27Z
dc.date.issued 2016-02-02
dc.identifier.issn 2469-9985
dc.identifier.uri http://library2.smu.ca/handle/01/27259
dc.description Publisher's Version/PDF
dc.description.abstract Several lifetimes in [superscript 23]Mg have been determined for the first time using the Doppler-shift attenuation method. A Monte Carlo simulation code has been written to model the [gamma]-ray line shape. An upper limit of [tau] < 12 fs at the 95% C.L. has been obtained for the astrophysically important 7787 keV state. en_CA
dc.description.provenance Submitted by Betty McEachern (betty.mceachern@smu.ca) on 2018-01-29T14:31:27Z No. of bitstreams: 1 Sanetullaev_A_article_2016.pdf: 1263972 bytes, checksum: b095f92142579730543819521a9a28fa (MD5) en
dc.description.provenance Made available in DSpace on 2018-01-29T14:31:27Z (GMT). No. of bitstreams: 1 Sanetullaev_A_article_2016.pdf: 1263972 bytes, checksum: b095f92142579730543819521a9a28fa (MD5) Previous issue date: 2016 en
dc.language.iso en en_CA
dc.publisher American Physical Society en_CA
dc.relation.uri https://doi.org/10.1103/PhysRevC.93.025802
dc.rights Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.
dc.subject.lcsh Magnesium -- Isotopes -- Decay
dc.subject.lcsh Doppler effect
dc.subject.lcsh Attenuation (Physics)
dc.subject.lcsh Gamma rays
dc.title Measurement of lifetimes in [superscript 23]Mg en_CA
dc.type Text en_CA
dcterms.bibliographicCitation Physical Review C 93(2), 25802. (2016) en_CA
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Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.
 
Published Version: https://doi.org/10.1103/PhysRevC.93.025802
 
 

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