L. Batist
Petersburg Nuclear Physics Institute
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Featured researches published by L. Batist.
Physica Scripta | 2013
Dinko Atanasov; D. L. Balabanski; L. Batist; Klaus Blaum; F. Bosch; D. Boutin; C. Brandau; C. Dimopoulou; H G Essel; T. Faestermann; H. Geissel; S. Hagmann; R Hess; P.-M. Hillenbrand; P. Kienle; R. Knöbel; C. Kozhuharov; J. Kurcewicz; M. Lestinsky; S. Litvinov; Yu. A. Litvinov; X. W. Ma; R Märtin; M. Mazzocco; G. Münzenberg; F. Nolden; T. Ohtsubo; Z. Patyk; M. S. Sanjari; C. Scheidenberger
In recent years several measurements of the orbital electron capture half-lives of few-electron ions have been carried out employing the storage ring ESR at GSI. Hydrogen-like and helium-like 140Pr and 142Pm as well as hydrogen-like 122I were studied. Half-lives of the corresponding fully ionized nuclides provide the three-body β+ decay constants.
Physical Review C | 2017
E. Valencia; J. L. Tain; A. Algora; J. Agramunt; E. Estevez; M. D. Jordan; B. Rubio; S. Rice; P. H. Regan; W. Gelletly; Zs. Podolyák; M. Bowry; P. Mason; G. F. Farrelly; A.-A. Zakari-Issoufou; M. Fallot; A. Porta; V. M. Bui; J. Rissanen; T. Eronen; I. D. Moore; H. Penttilä; J. Äystö; V.-V. Elomaa; J. Hakala; A. Jokinen; V. S. Kolhinen; M. Reponen; Volker Sonnenschein; D. Cano-Ott
We investigate the decay of 87Br, 88Br and 94Rb using total absorption gamma-ray spectroscopy. These important fission products are beta-delayed neutron emitters. Our data show considerable gamma-intensity, so far unobserved in high-resolution gamma-ray spectroscopy, from states at high excitation energy. We also find significant differences with the beta intensity that can be deduced from existing measurements of the beta spectrum. We evaluate the impact of the present data on reactor decay heat using summation calculations. Although the effect is relatively small it helps to reduce the discrepancy between calculations and integral measurements of the photon component for 235U fission at cooling times in the range 1 to 100 s. We also use summation calculations to evaluate the impact of present data on reactor antineutrino spectra. We find a significant effect at antineutrino energies in the range of 5 to 9 MeV. In addition, we observe an unexpected strong probability for gamma emission from neutron unbound states populated in the daughter nucleus. The gamma branching is compared to Hauser-Feshbach calculations which allow one to explain the large value for bromine isotopes as due to nuclear structure. However the branching for 94Rb, although much smaller, hints of the need to increase the radiative width by one order-of-magnitude. This leads to a similar increase in the calculated (n,gamma) cross section for this very neutron-rich nucleus with a potential impact on r-process abundance calculations.
Physical Review C | 2017
E. Valencia; J. L. Tain; A. Algora; J. Agramunt; E. Estevez; M. D. Jordan; B. Rubio; S. Rice; P. H. Regan; W. Gelletly; Zs. Podolyák; M. Bowry; P. Mason; G. F. Farrelly; A.-A. Zakari-Issoufou; M. Fallot; A. Porta; V. M. Bui; J. Rissanen; T. Eronen; I. D. Moore; H. Penttilä; J. Äystö; V.-V. Elomaa; J. Hakala; A. Jokinen; V. S. Kolhinen; M. Reponen; Volker Sonnenschein; D. Cano-Ott
We investigate the decay of 87Br, 88Br and 94Rb using total absorption gamma-ray spectroscopy. These important fission products are beta-delayed neutron emitters. Our data show considerable gamma-intensity, so far unobserved in high-resolution gamma-ray spectroscopy, from states at high excitation energy. We also find significant differences with the beta intensity that can be deduced from existing measurements of the beta spectrum. We evaluate the impact of the present data on reactor decay heat using summation calculations. Although the effect is relatively small it helps to reduce the discrepancy between calculations and integral measurements of the photon component for 235U fission at cooling times in the range 1 to 100 s. We also use summation calculations to evaluate the impact of present data on reactor antineutrino spectra. We find a significant effect at antineutrino energies in the range of 5 to 9 MeV. In addition, we observe an unexpected strong probability for gamma emission from neutron unbound states populated in the daughter nucleus. The gamma branching is compared to Hauser-Feshbach calculations which allow one to explain the large value for bromine isotopes as due to nuclear structure. However the branching for 94Rb, although much smaller, hints of the need to increase the radiative width by one order-of-magnitude. This leads to a similar increase in the calculated (n,gamma) cross section for this very neutron-rich nucleus with a potential impact on r-process abundance calculations.
Physical Review C | 2017
S. Rice; A. Algora; J. L. Tain; E. Valencia; J. Agramunt; B. Rubio; 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
The beta decays of 86Br and 91Rb have been studied using the total absorption spectroscopy technique. The nradioactive nuclei were produced at the Ion Guide Isotope Separator On-Line facility in Jyvaskyla and further npurified using the JYFLTRAP. 86Br and 91Rb are considered to be major contributors to the decay heat in reactors. nIn addition, 91Rb was used as a normalization point in direct measurements of mean gamma energies released in nthe beta decay of fission products by Rudstam et al. assuming that this decay was well known from high-resolution nmeasurements. Our results show that both decays were suffering from the Pandemonium effect and that the results nof Rudstam et al. should be renormalized. The relative impact of the studied decays in the prediction of the decay nheat and antineutrino spectrum from reactors has been evaluated
Physical Review C | 2016
E. Valencia; J. L. Tain; J. Hakala; D. Cano-Ott; H. Penttilä; F. G. Kondev; E. Estevez; V. M. Bui; M. Reponen; T. Martinez; A. Algora; V.-V. Elomaa; V. S. Kolhinen; B. Rubio; M. Bowry; V. Gorlychev; Zs. Podolyák; G. F. Farrelly; J. Äystö; B. Gomez-Hornillos; E. Mendoza; A.R. García; P. H. Regan; T. Eronen; W. Gelletly; A. Porta; L. Batist; Jordan; Volker Sonnenschein; J. Agramunt
We investigate the decay of 87Br, 88Br and 94Rb using total absorption gamma-ray spectroscopy. These important fission products are beta-delayed neutron emitters. Our data show considerable gamma-intensity, so far unobserved in high-resolution gamma-ray spectroscopy, from states at high excitation energy. We also find significant differences with the beta intensity that can be deduced from existing measurements of the beta spectrum. We evaluate the impact of the present data on reactor decay heat using summation calculations. Although the effect is relatively small it helps to reduce the discrepancy between calculations and integral measurements of the photon component for 235U fission at cooling times in the range 1 to 100 s. We also use summation calculations to evaluate the impact of present data on reactor antineutrino spectra. We find a significant effect at antineutrino energies in the range of 5 to 9 MeV. In addition, we observe an unexpected strong probability for gamma emission from neutron unbound states populated in the daughter nucleus. The gamma branching is compared to Hauser-Feshbach calculations which allow one to explain the large value for bromine isotopes as due to nuclear structure. However the branching for 94Rb, although much smaller, hints of the need to increase the radiative width by one order-of-magnitude. This leads to a similar increase in the calculated (n,gamma) cross section for this very neutron-rich nucleus with a potential impact on r-process abundance calculations.
Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016) | 2017
J. L. Tain; V. Guadilla; E. Valencia; A. Algora; A.-A. Zakari-Issoufou; S. Rice; J. Agramunt; J. Äystö; L. Batist; M. Bowry; J. A. Briz; V. M. Bui; R. Caballero-Folch; D. Cano-Ott; A. Cucoanes; V.-V. Elomaa; T. Eronen; E. Estevez; M. Estienne; M. Fallot; G. F. Farrelly; L. M. Fraile; E. Ganioglu; A.R. García; W. Gelletly; B. Gomez-Hornillos; D. Gorelov; V. Gorlychev; J. Hakala; A. Jokinen
EPJ Web of Conferences | 2017
M. Fallot; A. Porta; L. Le Meur; J.A. Briz; A.-A. Zakari-Issoufou; V. Guadilla; A. Algora; J. L. Tain; E. Valencia; S. Rice; V.M. Bui; S. Cormon; M. Estienne; J. Agramunt; J. Äystö; L. Batist; M. Bowry; R. Caballero-Folch; D. Cano-Ott; A. Cucoanes; V.-V. Elomaa; T. Eronen; E. Estevez; G. F. Farrelly; L. M. Fraile; M. Fleming; E. Ganogliu; A.R. García; W. Gelletly; M.B. Gómez-Hornillos
EPJ Web of Conferences | 2017
A. Algora; S. Rice; V. Guadilla; J. L. Tain; E. Valencia; A.-A. Zakari-Issoufou; J. Agramunt; J. Äystö; L. Batist; J.A. Briz; M. Bowry; V.M. Bui; R. Caballero-Folch; D. Cano-Ott; A. Cucoanes; T. Eronen; V.-V. Elomaa; E. Estevez; M. Estienne; M. Fallot; G. F. Farrelly; L. M. Fraile; M. Fleming; E. Ganioglu; A.R. García; W. Gelletly; B. Gomez-Hornillos; D. Gorelov; V. Gorlychev; J. Hakala
EPJ Web of Conferences | 2017
J. L. Tain; V. Guadilla; E. Valencia; A. Algora; A.-A. Zakari-Issoufou; S. Rice; L. Le Meur; J. Agramunt; J. Äystö; L. Batist; M. Bowry; J.A. Briz; V.M. Bui; R. Caballero-Folch; D. Cano-Ott; A. Cucoanes; V.-V. Elomaa; T. Eronen; E. Estevez; M. Estienne; M. Fallot; G. F. Farrelly; L. M. Fraile; E. Ganioglu; A.R. García; W. Gelletly; B. Gomez-Hornillos; D. Gorelov; V. Gorlychev; J. Hakala