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Dive into the research topics where W. Gelletly is active.

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Featured researches published by W. Gelletly.


Journal of Physics G | 1996

New results on

S. Rastikerdar; W. Gelletly; B. J. Varley; I.S. Grant

The very neutron-deficient isotope was produced in the reaction at 195 MeV and was identified using the Daresbury recoil separator. A pure -ray spectrum belonging to the de-excitation of the excited states of was obtained in-beam. Twenty -ray lines were identified, ten of them for the first time. The intensity balance concerning some of these -rays together with the results obtained from the coincident measurements show the existence of a new set of levels which may be interpreted as being a side band confirming the coupling of and configurations.


Physics Letters B | 1997

Delayed g9/2 Alignment in the N=Z Nucleus 72Kr

G. de Angelis; C. Fahlander; A. Gadea; E. Farnea; W. Gelletly; A. Aprahamian; D. Bazzacco; F. Becker; P.G. Bizzeti; A. Bizzeti-Sona; F. Brandolini; D. De Acuña; M. De Poli; J. Eberth; D. Foltescu; S. M. Lenzi; Santo Lunardi; T. Martinez; D. R. Napoli; P. Pavan; C.M. Petrache; C. Rossi Alvarez; D. Rudolph; B. Rubio; W. Satula; S. Skoda; P. Spolaore; H.G. Thomas; C. A. Ur; R. Wyss

The structure of Kr-72 has been investigated at GASP through the Ca-40(Ca-40,2 alpha) reaction at a beam energy of 160 MeV using the 4 pi ISIS Si-ball for reaction channel selection. The level scheme has been extended up to an excitation energy of approximate to 8.5 MeV. The spins and parities of the observed levels are assigned tentatively. The observed band shows the predicted change from oblate to prolate shape. The four quasi-particle g(9/2) alignment is found to be significantly delayed in rotational frequency with respect to the heavier Kr isotopes. Such a delay contradicts the predictions of standard mean-field calculations and may reflect either additional correlations in the T = 0 pairing channel or coupling to vibrational degrees of freedom or both


Physics Letters B | 1998

Competing T=0 and T=1 structures in the N=Z nucleus 6231Ga

S. M. Vincent; P. H. Regan; R.A. Bark; Daniel J. Blumenthal; M. P. Carpenter; C. N. Davids; W. Gelletly; R. V. F. Janssens; C.D. O'Leary; C. J. Lister; J. Simpson; D. Seweryniak; Takashi Saitoh; Jennifer L. Schwartz; S. Törmänen; O. Juillet; F. Nowacki; P. Van Isacker

Abstract The low-lying levels in the odd-odd N = Z nucleus 62 Ga have been identified for the first time. These data reveal a cascade of stretched-E2 transitions based on a T =0, 1 + bandhead which decays directly to the T =1, 0 + ground state. The observed levels are interpreted in the context of theshell model, using as a basis, the pf 5/2 g 9/2 orbits with a 56 Ni core.


Physical Review Letters | 2015

Total Absorption Spectroscopy Study of (92)Rb Decay: A Major Contributor to Reactor Antineutrino Spectrum Shape.

M. Fallot; A. Porta; A. Algora; E. Valencia; S. Rice; S. Cormon; M. Estienne; J. Agramunt; M. Bowry; R. Caballero-Folch; D. Cano-Ott; A. Cucoanes; T. Eronen; W. Gelletly; J. Hakala; A. Jokinen; P. Karvonen; T. Martinez; E. Mendoza; F. Molina; I. D. Moore; M. Reponen; J. Rissanen; B. Rubio; T. Shiba; Christian Weber

The antineutrino spectra measured in recent experiments at reactors are inconsistent with calculations based on the conversion of integral beta spectra recorded at the ILL reactor. (92)Rb makes the dominant contribution to the reactor antineutrino spectrum in the 5-8 MeV range but its decay properties are in question. We have studied (92)Rb decay with total absorption spectroscopy. Previously unobserved beta feeding was seen in the 4.5-5.5 region and the GS to GS feeding was found to be 87.5(25)%. The impact on the reactor antineutrino spectra calculated with the summation method is shown and discussed.


Physical Review C | 2010

Spectroscopy of neutron-rich Dy-168,Dy-170: Yrast band evolution close to the NpNn valence maximum

Pär-Anders Söderström; J. Nyberg; P. H. Regan; A. Algora; G. de Angelis; S. F. Ashley; S. Aydin; D. Bazzacco; R.J. Casperson; W. N. Catford; Joakim Cederkäll; R. Chapman; L. Corradi; Claes Fahlander; E. Farnea; E. Fioretto; S. J. Freeman; A. Gadea; W. Gelletly; A. Gottardo; E. Grodner; C. Y. He; G. A. Jones; K. L. Keyes; M. Labiche; X. Liang; Z. Liu; Santo Lunardi; N. Marginean; P. Mason

The yrast sequence of the neutron-rich dysprosium isotope Dy-168 has been studied using multinucleon transfer reactions following collisions between a 460-MeV Se-82 beam and an Er-170 target. The reaction products were identified using the PRISMA magnetic spectrometer and the gamma rays detected using the CLARA HPGe-detector array. The 2(+) and 4(+) members of the previously measured ground-state rotational band of Dy-168 have been confirmed and the yrast band extended up to 10(+). A tentative candidate for the 4(+) -> 2(+) transition in Dy-170 was also identified. The data on these nuclei and on the lighter even-even dysprosium isotopes are interpreted in terms of total Routhian surface calculations and the evolution of collectivity in the vicinity of the proton-neutron valence product maximum is discussed. (Less)


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2010

TIARA: A large solid angle silicon array for direct reaction studies with radioactive beams

M. Labiche; W. N. Catford; R. C. Lemmon; C. Timis; R. Chapman; N. A. Orr; B. Fernández-Domínguez; G. Moores; N. L. Achouri; N. Amzal; S. Appleton; N. I. Ashwood; Timothy Baldwin; M. Burns; L. Caballero; J. Cacitti; J.M. Casadjian; M. Chartier; N. Curtis; K. Faiz; Martin Freer; J.M. Gautier; W. Gelletly; G. Iltis; B. Lecornu; X. Liang; C. Marry; Y. Merrer; L. Olivier; S. D. Pain

A compact, quasi-4pi position sensitive silicon array, TIARA, designed to study direct reactions induced by radioactive beams in inverse kinematics is described here. The Transfer and Inelastic All-angle Reaction Array (TIARA) consists of 8 resistive-strip silicon detectors forming an octagonal barrel around the target and a set of double-sided silicon-strip annular detectors positioned at each end of the barrel. The detector was coupled to the gamma-ray array EXOGAM and the spectrometer VAMOS at the GANIL Laboratory to demonstrate the potential of such an apparatus with radioactive beams. The 14N(d,p)15N reaction, well known in normal kinematics, has been carried out in inverse kinematics for that purpose. The observation of the 15N ground state and excited states at 7.16 and 7.86 MeV is presented here as well as the comparison of the measured proton angular distributions with DWBA calculations. Transferred l-values are in very good agreement with both theoretical calculations and previous experimental results obtained in normal kinematics.


Physics Letters B | 2002

Isovector pairing in odd-odd N = Z 50Mn

C.D. O'Leary; M. A. Bentley; S. M. Lenzi; G. Martínez-Pinedo; A. M. Bruce; J. A. Cameron; M. P. Carpenter; Cary N. Davids; P. Fallon; L. Frankland; W. Gelletly; Rvf Janssens; D. T. Joss; C. J. Lister; P. H. Regan; P. Reiter; B. Rubio; D. Seweryniak; C. E. Svensson; S. M. Vincent; S. J. Williams

High-spin states in the odd–odd N=Z nucleus 5025Mn have been investigated. A sequence of states up to Jπ=6+ has been assigned as the T=1 analogue of the yrast band in 5024Cr for the first time. The differences in energy between levels in these bands are interpreted in terms of rotational alignments and the effect they have on the Coulomb energy of the nucleus. Comparisons with shell model calculations show that the Coulomb energy difference between the T=1 analogue structures is an important indicator of the competition between isovector pairing modes in N=Z nuclei and their isobars.


Physical Review Letters | 2015

Enhanced γ-Ray Emission from Neutron Unbound States Populated in β Decay.

J. L. Tain; E. Valencia; A. Algora; J. Agramunt; B. Rubio; S. Rice; W. Gelletly; P. H. Regan; A.-A. Zakari-Issoufou; M. Fallot; A. Porta; J. Rissanen; T. Eronen; J. Äystö; L. Batist; M. Bowry; V. M. Bui; R. Caballero-Folch; D. Cano-Ott; V.-V. Elomaa; E. Estevez; G. F. Farrelly; A.R. García; B. Gomez-Hornillos; V. Gorlychev; J. Hakala; M. D. Jordan; A. Jokinen; V. S. Kolhinen; F. G. Kondev

Total absorption spectroscopy is used to investigate the β-decay intensity to states above the neutron separation energy followed by γ-ray emission in (87,88)Br and (94)Rb. Accurate results are obtained thanks to a careful control of systematic errors. An unexpectedly large γ intensity is observed in all three cases extending well beyond the excitation energy region where neutron penetration is hindered by low neutron energy. The γ branching as a function of excitation energy is compared to Hauser-Feshbach model calculations. For (87)Br and (88)Br the γ branching reaches 57% and 20%, respectively, and could be explained as a nuclear structure effect. Some of the states populated in the daughter can only decay through the emission of a large orbital angular momentum neutron with a strongly reduced barrier penetrability. In the case of neutron-rich (94)Rb the observed 4.5% branching is much larger than the calculations performed with standard nuclear statistical model parameters, even after proper correction for fluctuation effects on individual transition widths. The difference can be reconciled by introducing an enhancement of 1 order of magnitude in the photon strength to neutron strength ratio. An increase in the photon strength function of such magnitude for very neutron-rich nuclei, if it proves to be correct, leads to a similar increase in the (n,γ) cross section that would have an impact on r process abundance calculations.


International Journal of Modern Physics E-nuclear Physics | 2004

STRUCTURE OF NEUTRON–RICH NUCLEI FROM DEEP–INELASTIC REACTIONS

Zs. Podolyák; S. Mohammadi; G. de Angelis; Y. H. Zhang; M. Axiotis; D. Bazzacco; P. G. Bizzeti; F. Brandolini; R. Broda; D. Bucurescu; E. Farnea; W. Gelletly; A. Gadea; M. Ionescu-Bujor; A. Iordachescu; Th. Kröll; S. D. Langdown; S. Lunardi; N. Marginean; T. Martinez; N. H. Medina; B. Quintana; P. H. Regan; B. Rubio; C. A. Ur; J. J. Valiente-Dobón; P. M. Walker

Neutron rich nuclei have been populated using the 82Se+192Os deep-inelastic reaction. New experimental results on 188W, 188,190Os target-like nuclei, as well as 74,76,78Ge beam-like nuclei are presented.


Nuclear Physics | 1989

The deformation systematics of the light even-even neodymium isotopes

R. Moscrop; M. Campbell; W. Gelletly; L. Goettig; C.J. Lister; B. J. Varley

Abstract The gamma ray decays of excited states in the nuclei 128,130,132Nd have been identified as the result of measurements of multiple particle-gamma coincidences. The reactions 40Ca + 92Mo and 40Ca + 96Ru were studied at bombarding energies ranging from 147 to 200 MeV. Gamma-ray excitation functions were measured over this energy range. In the case of the 92Mo(40Ca, 2p)130Nd reaction, the angular distributions of the emitted gamma rays were also measured at 180 MeV bombarding energy. The lifetimes of the lowest states in the ground-state bands of these nuclei were measured using the recoil distance method. The results are consistent with these nuclei possessing large, permanent, ground state deformations with typical values of e2 ≈ 0.3. The ground state rotational bands of all the nuclei studied exhibit band crossings at h ω c ≈0.32 MeV . This appears to be due to the alignment of h 11 2 protons. The results are discussed in the light of recent potential energy surface and cranked-shell-model calculations.

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B. Rubio

Spanish National Research Council

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J. Agramunt

University of Valencia

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A. Algora

Spanish National Research Council

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J. Gerl

GSI Helmholtz Centre for Heavy Ion Research

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A. M. Bruce

University of Brighton

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J. L. Tain

Spanish National Research Council

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A. Algora

Spanish National Research Council

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