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Bogaert, G.
Paris-11 Univ., 91 - Orsay (France). Centre de Spectrometrie Nucleaire et de Spectrometrie de Masse1984
Paris-11 Univ., 91 - Orsay (France). Centre de Spectrometrie Nucleaire et de Spectrometrie de Masse1984
AbstractAbstract
[en] Average lifetimes and multipolarities of unresolved transitions deexciting very high spin states of the light Rare Earth nuclei (N approximately 86) have been determined by a measure of Doppler shift attenuation and their anisotropy. The spin selection is provided by the total energy spectrometer technique; great care was taken of the existence of many long lived isomeric states in the studied nuclei. The N approximately 86 nuclei have been formed in the 84Kr(340 MeV) + 74Ge → 158Er* reactions using the 84Kr beam of the Orsay ALICE facilities and targets of 74Ge built at the PARIS Isotope separator of the CSNSM. NaI γ spectra have been thoroughly cleared of the discrete lines contribution through a carefull subtraction procedure synthetising NaI spectra from the Ge ones. At very high spin the continuum γ rays feed two well separated bumps with Esub(γ) approximately .65 MeV and Esub(γ) approximately 1.3 MeV. The 1.3 MeV transitions appear at I > 30 h and their energy does not vary with the increasing spin like expected in the rotational case of the well deformed nuclei; they are strongly collectively enhanced with B(E2) > 130 W.u. Below 1 MeV the anisotropy of transitions is R approximately 0.7, indicating their stretched dipole nature. Recent calculations of nuclear shape deformation (following Strutinsky shell correction method) reproduce the two bumps shape of the experimental spectra and the origin of the excitation is explained in terms of nuclear vibration (γ-vibration, wobbling motion)
[fr]
La duree de vie et la multipolarite des transitions du continuum γ des noyaux de terres rares transitionnels (voisins de 154Er: N approximately 86) formes a tres haut spin par reaction entre ions lourds ont ete etudiees par la mesure de l'attenuation de leur decalage Doppler et de leur anisotropie. La selection des niveaux, selon leur spin, utilisant la technique de spectrometrie d'energie totale a ete realisee en tenant compte de l'existence de nombreux isomeres de longue duree de vie dans les noyaux etudies. Ces noyaux N approximativement 86 ont ete formes par reaction de 84Kr (340 MeV) accelere par ALICE (Orsay) sur des cibles de 74Ge fabriquees au separateur d'isotopes PARIS (CSNSM-Orsay). Les spectres NaI de transitions γ ont ete meticuleusement debarrasses de la contribution des raies discretes par une procedure utilisant la synthese de spectres NaI fictifs a partir des spectres Ge. A tres haut spin, les transitions du continuum γ alimentent deux bosses d'energie .65 MeV et 1.3 MeV. Les transitions de 1.3 MeV apparaissent pour I > 30 h et leur energie ne varie pas comme dans le cas rotationnel des noyaux bien deformes; elles sont de nature collective tres accelerees avec B(E2) > 130 u.W. En dessous de 1 MeV l'anisotropie des transitions est R approximativement 0.7 indiquant leur caractere dipolaire etire. Les calculs recents de deformation nucleaire (correction de couche de Strutinsky) reproduisent remarquablement la forme en deux bosses des spectres experimentaux et l'origine de l'excitation est vraisemblablement la vibration du noyau (vibration γ - mouvement de wobbling)Original Title
Etude a tres haut spin des noyaux d'Erbium transitionnels (N=86). Mise en evidence de transitions dipolaires et mesures de vies moyennes dans le continuum
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1984; 116 p; These (3e Cycle).
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Report
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Thesis/Dissertation
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ANISOTROPY, COMPOUND-NUCLEUS REACTIONS, DEFORMED NUCLEI, DSA METHOD, DYSPROSIUM, E1-TRANSITIONS, E2-TRANSITIONS, ERBIUM 153, ERBIUM 154, ERBIUM 155, ERBIUM 156, GAMMA SPECTROSCOPY, GERMANIUM 76 TARGET, HIGH SPIN STATES, HOLMIUM, ISOMERIC NUCLEI, KRYPTON 86 REACTIONS, LIFETIME, MEV RANGE 100-1000, MULTIPOLARITY, NUCLEAR DEFORMATION, STRUTINSKY THEORY
BETA DECAY RADIOISOTOPES, COUNTING TECHNIQUES, DEFORMATION, ELECTRON CAPTURE RADIOISOTOPES, ELEMENTS, ENERGY LEVELS, ENERGY RANGE, ENERGY-LEVEL TRANSITIONS, ERBIUM ISOTOPES, EVEN-EVEN NUCLEI, EVEN-ODD NUCLEI, HEAVY ION REACTIONS, INTERMEDIATE MASS NUCLEI, ISOTOPES, METALS, MEV RANGE, MULTIPOLE TRANSITIONS, NUCLEAR REACTIONS, NUCLEI, RADIOISOTOPES, RARE EARTH NUCLEI, RARE EARTHS, SPECTROSCOPY, TARGETS
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AbstractAbstract
[en] The paper discusses the reaction rates at low energies, needed for the description of nucleosynthesis processes. In contrast to the stellar environment, the laboratory measurements are complicated by the coulomb potential screening caused by bound electrons. The consequences of recent 7Be+p reaction measurements on solar modelling are presented. The new high-energy laser facilities will open new possibilities for measurements of stellar reaction rates. Abstract provided by the editors. (author)
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Nuclear physics at the turn of the century: 26. Mazurian Lakes School of Physics; Krzyze (Poland); 1-11 Sep 1999; 15 refs, 8 figs, 2 tabs
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Journal Article
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Conference
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Acta Physica Polonica. Series B; ISSN 0587-4254; ; v. 31(2); p. 299-309
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[en] The gamma ray telescopes launched in the recent years provide observations which in turn trigger a better thought of the nuclear physics involved in the gamma ray production in stars, novae and supernovae. Two examples are presented, with suggestions of experiments to run, either with stable or unstable beams. (author)
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Trends in Nuclear Physics: 31. Zakopane School of Physics; Zakopane (Poland); 3-11 Sep 1996; 17 refs, 3 figs
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Journal Article
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Conference
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Acta Physica Polonica. Series B; ISSN 0587-4254; ; v. 28(1-2); p. 227-232
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ASTRONOMY, BARYON REACTIONS, BINARY STARS, CARBON ISOTOPES, DECAY, DETECTION, ERUPTIVE VARIABLE STARS, EVEN-EVEN NUCLEI, HADRON REACTIONS, ISOTOPES, LIGHT NUCLEI, MAGNESIUM ISOTOPES, NUCLEAR DECAY, NUCLEAR REACTIONS, NUCLEI, NUCLEON REACTIONS, OXYGEN ISOTOPES, RADIATION DETECTION, STABLE ISOTOPES, STARS, VARIABLE STARS
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Aguer, P.; Angulo, C.; Bogaert, G.; Coc, A.; Kiener, J.; Lefebvre, A.; Oliveira, F.; Thibaud, J.P.
207th ACS national meeting1994
207th ACS national meeting1994
AbstractAbstract
[en] Studies of the dissociation of fast projectiles in the Coulomb field of a heavy target nucleus have been proposed as an alternative access to radiative capture cross sections of astrophysical relevance. Instead of measuring the cross section A+b → C+γ, one considers the photodissociation process C+γ → A+b. Compared with the direct process, the cross section of the inverse one is enhanced due to the high density of virtual photons. The Coulomb break-up technique has been applied to radioactive beams in order to determine rates of reactions involved in the hot CNO cycle and the hot pp chain. 12N and 14O radioactive beams were produced through fragmentation of a primary 95.5 MeV/u heavy ion beam, and used to study the rates of the reactions 13N+p → 14O+γ and 11C+p → 12N+γ. Nuclear astrophysics requires many cross sections, and one could hope that the Coulomb break-up method would be of a large use. A survey of the most important reaction rates actually required in astrophysics will be made regarding the applicability of the break-up method to extract valuable experimental information
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Anon; 2247 p; 1994; p. 1045, Paper NUCL 62; American Chemical Society; Washington, DC (United States); 207. spring national meeting of the American Chemical Society (ACS); San Diego, CA (United States); 13-18 Mar 1994; American Chemical Society, 1155 16th St., N.W., Washington, DC 20036-4899 (United States)
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Book
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Conference
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BEAMS, BETA DECAY RADIOISOTOPES, BETA-PLUS DECAY RADIOISOTOPES, CARBON ISOTOPES, CHARGED PARTICLES, EVEN-EVEN NUCLEI, EVEN-ODD NUCLEI, HEAVY ION REACTIONS, ION BEAMS, IONS, ISOTOPES, LIGHT NUCLEI, MINUTES LIVING RADIOISOTOPES, NITROGEN ISOTOPES, NUCLEAR REACTIONS, NUCLEI, ODD-ODD NUCLEI, OXYGEN ISOTOPES, RADIOISOTOPES
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AbstractAbstract
[en] We report a case of a postoperative retroperitoneal haemorrhage due to an iatrogenic perioperative injury of an ureteric artery. Transcatheter embolization using microparticles stopped the bleeding and the patient stabilized immediately. Ureteric artery injury is a very rare condition but can be managed successfully by percutaneous interventional techniques. (orig.)
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ECR 2001: 13. European congress of Radiology, with exhibits; Vienna (Austria); 2-6 Mar 2001
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Landre, V.; Bogaert, G.; Aguer, P.; Lefebvre, A.; Thibaud, J.P.; Fortier, S.; Maison, J.M.; Vernotte, J.
Proceedings of 22. Zakopane school on physics, Zakopane, Poland, 1-15 May 1987. Part 11987
Proceedings of 22. Zakopane school on physics, Zakopane, Poland, 1-15 May 1987. Part 11987
AbstractAbstract
[en] The 17O(p,α)14N and 17O(p,γ)18F reactions involved in the secondary branch of the main CNOcycle of stellar evolution are examined. The spectroscopic factor related to the width is deduced for a 5.668 MeV level from a stripping reaction 17O(3He,d)18F at the Orsay Tandem. 13 refs., 1 fig. (M.F.W.)
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Broda, R.; Stachura, Z. (eds.); Institute of Nuclear Physics, Cracow (Poland); Uniwersytet Jagiellonski, Cracow (Poland); 454 p; 1987; p. 367-370; 22. Zakopane school on physics; Zakopane (Poland); 1-15 May 1987
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Report
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Conference
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BARYON REACTIONS, BETA DECAY RADIOISOTOPES, BETA-PLUS DECAY RADIOISOTOPES, CHARGED PARTICLES, DIRECT REACTIONS, ELECTROMAGNETIC RADIATION, ENERGY RANGE, FLUORINE ISOTOPES, HADRON REACTIONS, HELIUM IONS, HOURS LIVING RADIOISOTOPES, IONIZING RADIATIONS, IONS, ISOMERIC TRANSITION ISOTOPES, ISOTOPES, LIGHT NUCLEI, MEV RANGE, NITROGEN ISOTOPES, NUCLEAR REACTIONS, NUCLEI, NUCLEON REACTIONS, ODD-ODD NUCLEI, RADIATIONS, RADIOISOTOPES, STABLE ISOTOPES, STAR BURNING, SYNTHESIS, TARGETS, TRANSFER REACTIONS
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Related RecordRelated Record
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AbstractAbstract
[en] The energy of the first level above the proton threshold in /sup 18/F has been determined to be 5672.57 +- 0.32 keV by γ-ray measurements using the /sup 14/N(α,γ)/sup 18/F reaction. The change in the excitation energy of this level previously measured at 5668 +- 2 keV affects significantly the calculated reaction rate for /sup 17/O destruction during hydrogen burning in stars
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Journal Article
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ACCELERATORS, BETA DECAY RADIOISOTOPES, BETA-PLUS DECAY RADIOISOTOPES, ELECTROMAGNETIC RADIATION, ELECTROSTATIC ACCELERATORS, ENERGY RANGE, EVEN-ODD NUCLEI, FLUORINE ISOTOPES, HOURS LIVING RADIOISOTOPES, IONIZING RADIATIONS, ISOTOPES, LIGHT NUCLEI, MEV RANGE, NUCLEAR REACTIONS, NUCLEI, ODD-ODD NUCLEI, OXYGEN ISOTOPES, RADIATIONS, RADIOISOTOPES, STABLE ISOTOPES, STAR BURNING, SYNTHESIS, TARGETS
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Aguer, P.; Bogaert, G.; Coc, A.; Kiener, J.; Lefebvre, A.; Tatischeff, V.; Thibaud, J.P.
Third IN2P3-RIKEN symposium on heavy ion collisions1995
Third IN2P3-RIKEN symposium on heavy ion collisions1995
AbstractAbstract
[en] The technique of Coulomb break-up of a 12N radioactive beam has been used for the determination of the 11C + p stellar reaction rate. The consequences for the hot pp chain and the stellar production of 11B are examined. (authors). 14 refs., 2 figs
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Motobayashi, T.; Frascaria, N.; Ishihara, M. (eds.); [470 p.]; ISBN 981-02-2207-6; ; 1995; p. 56-65; World Scientific; Singapore (Singapore); 3. IN2P3-RIKEN symposium on heavy ion collisions; Shinrin-Koen, Saitama (Japan); 24-28 Oct 1994
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Book
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Conference
Country of publication
BARYON REACTIONS, BEAMS, BETA DECAY RADIOISOTOPES, BETA-PLUS DECAY RADIOISOTOPES, BORON ISOTOPES, CARBON ISOTOPES, DECAY, ENERGY, EVEN-ODD NUCLEI, HADRON REACTIONS, ION BEAMS, ISOTOPES, KINETICS, LIGHT NUCLEI, MINUTES LIVING RADIOISOTOPES, NITROGEN ISOTOPES, NUCLEAR REACTIONS, NUCLEI, NUCLEON REACTIONS, ODD-EVEN NUCLEI, ODD-ODD NUCLEI, RADIOISOTOPES, REACTION KINETICS, STABLE ISOTOPES, STAR BURNING
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Ferreira, O.; Bogaert, G.; Bonnemaison, A.; Drevillon, G.; Fleury, P.; Giebels, B.; Prat, P.; Bederede, D.; Bourgeois, P.; Cordier, B.; Gentit, F.X.; Horeau, B.; Piret, Y., E-mail: berrie@poly.in2p3.fr2004
AbstractAbstract
[en] This paper describes the results of vibration tests using the Validation Module of the GLAST Gamma Large Area Telescope calorimeter structure. The composite structure has been tested with different vibration spectra expected during the launch environment of GLAST. No degradation of the mechanical assembly was observed, and deformations and displacements stayed within stay-clear limits
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S0168900204010708; Copyright (c) 2004 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment; ISSN 0168-9002; ; CODEN NIMAER; v. 530(3); p. 323-329
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AbstractAbstract
[en] The capture reaction 14N(p,γ)15O has been investigated in the energy range Ep=0.2 to 3.6 MeV with the use of windowless gas targets as well as implanted 14N solid targets of high isotopic purity. The measurement of absolute cross sections, γ-ray angular distributions and excitation functions is reported. The data provide information on the capture amplitudes involved in the transitions to all bound states of 15O. The astrophysical S-factor at stellar energies has been determined by means of theoretical fits. The result of S(0)=3.20 keV . b is in good agreement with the value incorporated in the compilations. Also discussed are the nuclear physics aspects of the data. (orig.)
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CONTRACT DFG RO 429/13-3; DFG RO 429/15-1
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Journal Article
Literature Type
Numerical Data
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ANGULAR DISTRIBUTION, ANISOTROPY, CAPTURE, CNO CYCLE, DIFFERENTIAL CROSS SECTIONS, ENERGY DEPENDENCE, ENERGY LEVELS, ENERGY SPECTRA, EXCITATION FUNCTIONS, EXCITED STATES, EXPERIMENTAL DATA, GAMMA SPECTRA, GROUND STATES, HYDROGEN BURNING, KEV RANGE 100-1000, LEVEL WIDTHS, MEV RANGE 01-10, NITROGEN 14 TARGET, NUCLEAR REACTION KINETICS, OXYGEN 15, PARITY, PHOTONS, PROTON REACTIONS, RESONANCE, SPECTROSCOPIC FACTORS, SPIN, STAR BURNING
ANGULAR MOMENTUM, BARYON REACTIONS, BETA DECAY RADIOISOTOPES, BETA-PLUS DECAY RADIOISOTOPES, BOSONS, CROSS SECTIONS, DATA, DISTRIBUTION, ELEMENTARY PARTICLES, ENERGY RANGE, EVEN-ODD NUCLEI, HADRON REACTIONS, INFORMATION, ISOTOPES, KEV RANGE, KINETICS, LIGHT NUCLEI, MASSLESS PARTICLES, MEV RANGE, MINUTES LIVING RADIOISOTOPES, NUCLEAR REACTIONS, NUCLEI, NUCLEON REACTIONS, NUMERICAL DATA, OXYGEN ISOTOPES, PARTICLE PROPERTIES, RADIOISOTOPES, REACTION KINETICS, SPECTRA, TARGETS
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