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NSR database version of April 25, 2024.

Search: Author = L.Guerro

Found 3 matches.

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2014BL12      Phys.Rev. C 90, 044317 (2014)

N.Blasi, L.Atanasova, D.Balabanski, S.Das Gupta, K.Gladinski, L.Guerro, S.Nardelli, A.Saltarelli

E0 decay from the first 0+ state in 156Dy and 160Er

RADIOACTIVITY 160Tm(β+), (EC)[from 150Sm(14N, 4n), E=72 MeV]; 156Er, 156Ho(β+), (EC)[from 148Sm(12C, 4n), E=72 MeV]; measured Eγ, Iγ, ce and conversion coefficients using a mini-orange spectrometer at INFN-LN Catania's Tandem accelerator facility; 156Dy, 160Er; deduced levels, J, π, multipolarity, X(E0/E2) ratios of reduced transition probabilities, E0 admixtures in transitions from the lower members of β and γ bands. Comparison with IBA-1 model calculations and systematics of neighboring Dy and Er nuclei.

NUCLEAR STRUCTURE 154,156,158,160,162Dy, 156,158,160,162,164,166Er; calculated levels, J, π, X(E0/E2) ratios of reduced transition probabilities, isotope shifts with IBA-1 calculations. Comparison with experimental data.

doi: 10.1103/PhysRevC.90.044317
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Data from this article have been entered in the XUNDL database. For more information, click here.


2014GU26      Eur.Phys.J. A 50, 171 (2014)

L.Guerro, A.Di Leva, L.Gialanella, A.Saltarelli, D.Schurmann, U.Tabassam, M.Busso, N.De Cesare, A.D'Onofrio, M.Romoli, F.Terrasi

A pair spectrometer for nuclear astrophysics experiments

doi: 10.1140/epja/i2014-14171-1
Citations: PlumX Metrics


2013BL07      Phys.Rev. C 88, 014318 (2013)

N.Blasi, L.Guerro, A.Saltarelli, O.Wieland, L.Fortunato

E0 decay from the first excited 0+ state in 162Yb

RADIOACTIVITY 162Lu(β+), (EC)[from 147Sm(19F, 4n), E=95 MeV]; measured Eγ, Iγ, conversion electrons at the INFN, LNS facility in Catania. 162Yb; deduced levels, J, π, X(E0/E2), multipolarity, internal conversion coefficients. 159,161Ho, 161,163Tm, 162Er; measured Eγ, Iγ, ce. Comparison with calculations using IBA-1 model.

NUCLEAR STRUCTURE 160,162,164,166,168Yb; calculated isotope shifts and X(E0/E2) for 2+, 4+ yrast states and 0+, 2+ members of β band using the IBA-1 model. Comparison with experimental data.

doi: 10.1103/PhysRevC.88.014318
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Data from this article have been entered in the XUNDL database. For more information, click here.


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