148 results on '"Heinz Oberhummer"'
Search Results
2. Das Universum ist eine Scheissgegend
- Author
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Heinz Oberhummer, Martin Puntigam, and Werner Gruber
- Published
- 2015
3. Neutron-induced fission cross section ofNp237in the keV to MeV range at the CERN n_TOF facility
- Author
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L. Sarchiapone, S. Andriamonje, G. Cortes, J. Marganiec, R. C. Haight, P. E. Koehler, H. Álvarez, Masayuki Igashira, K. Ioannidis, M. Oshima, C. Lamboudis, J. L. Tain, C. Paradela, E. Chiaveri, P. F. Mastinu, A. Dorochenko, J. Andrzejewski, G. Aerts, J. Cox, A. J. M. Plompen, Isabel Lopes, B. Haas, Matthias Heil, J. Pancin, E. Skordis, L. Audouin, F. Voss, P. Cennini, S. David, Roberto Capote, P.A. Assimakopoulos, Thomas Rauscher, F. Neves, P. M. Milazzo, A. Tsinganis, Y. Kadi, G. Tagliente, I. Duran, H. Frais-Koelbl, Carlos Guerrero, U. Abbondanno, M. Mosconi, P. Pavlopoulos, D. Karadimos, Nicola Colonna, C. Rubbia, M. Kokkoris, Michael Wiescher, V. Konovalov, F. Bečvář, Heinz Oberhummer, S. O'Brien, E. González-Romero, Isabel S. Gonçalves, K. C. Stamoulis, S. Marrone, W. Dridi, I. Savvidis, J. Salgado, D. Cano-Ott, Marco Calviani, M. Diakaki, A. Poch, Vasilis Vlachoudis, A. Lindote, M. Sedysheva, R. Terlizzi, A. Goverdovski, M. Kerveno, Rene Reifarth, E. Griesmayer, V. Ketlerov, A. Plukis, F. Alvarez-Velarde, A. Carrillo de Albornoz, C. Papadopoulos, M. Embid-Segura, L. Ferrant, L. Tavora, K. Fuji, Gerald Badurek, F. Käppeler, Paraskevi Demetriou, L. Fitzpatrick, F. Gramegna, Ralf Plag, R. Dolfini, A. Pavlik, J. M. Quesada, C. Eleftheriadis, M. Rosetti, C. Pretel, Manuel Lozano, C. Domingo-Pardo, L. Tassan-Got, M. C. Vincente, D. Villamarin, P. Rullhusen, M. Krtička, F. Calviño, W.I. Furman, L. Perrot, Corrie S. Moreau, R. Ferreira-Marques, S. Lukic, V. Chepel, A. Herrera-Martinez, N. Patronis, G. Rudolf, L. Marques, P. Vaz, Arnaud Ferrari, Aaron Couture, P. Baumann, Alberto Mengoni, S. Isaev, A. Ventura, R. Vlastou, E. Berthoumieux, G. Vannini, R. Gallino, K. Wisshak, D. Karamanis, H. Wendler, D. Kolokolov, H. Leeb, C. Stephan, F. Gunsing, Cristian Massimi, and E. Jericha
- Subjects
Physics ,Large Hadron Collider ,010308 nuclear & particles physics ,Fission ,Model parameters ,7. Clean energy ,01 natural sciences ,Nuclear physics ,0103 physical sciences ,Homogeneity (physics) ,Ionization chamber ,Neutron cross section ,Neutron ,Atomic physics ,Nuclear Experiment ,010306 general physics ,Spectroscopy - Abstract
The neutron-induced fission cross section of Np237 was experimentally determined at the high-resolution and high-intensity facility n-TOF, at CERN, in the energy range 100 keV to 9 MeV, using the U235(n,f) and U238(n,f) cross section standards below and above 2 MeV, respectively. A fast ionization chamber was used in order to detect the fission fragments from the reactions and the targets were characterized as far as their mass and homogeneity are concerned by means of α spectroscopy and Rutherford backscattering spectroscopy respectively. Theoretical calculations within the Hauser-Feshbach formalism have been performed, employing the empire code, and the model parameters were tuned in order to successfully reproduce the experimental fission cross-sectional data and simultaneously all the competing reaction channels.
- Published
- 2016
4. 237Np(n,f) Cross Section: New Data and Present Status
- Author
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B. Haas, I. Savvidis, C. Lampoudis, A. Pavlik, C. Domingo-Pardo, G. Cortes, Martin Heil, P. Cennini, S. David, D. Tarrío, D. Cano-Ott, W. Dridi, Roberto Capote, P.A. Assimakopoulos, M. Mosconi, S. O'Brien, G. Tagliente, Marco Calviani, M. Oshima, R. Terlizzi, Corrie S. Moreau, S. Walter, J. Andrzejewski, L. Tavora, Ralf Plag, F. Calviño, H. Leeb, J. Salgado, Isabel Lopes, P. Rullhusen, J. Marganiec, S. Andriamonje, A. Poch, C. Santos, E. Kossionides, E. Chiaveri, K. Wisshak, P. F. Mastinu, A. J. M. Plompen, Christoph A. Stephan, J. Pancin, A. Herrera-Martinez, N. Patronis, A. Ventura, F. Gunsing, D. Trubert, L. Ferrant, Cristian Massimi, Javier Praena, I. Duran, Arnaud Ferrari, G. Aerts, M. Dahlfors, Y. Kadi, R. C. Haight, M. Embid-Segura, P. Vaz, Rene Reifarth, H. Álvarez, S. Lukic, D. Villamarin, Alberto Mengoni, James L. Cox, C. Paradela, M. C. Vicente, C. Eleftheriadis, Thomas Rauscher, Aaron Couture, M. Krtička, S. Isaev, J. M. Quesada, Manuel Lozano, L. Tassan-Got, Carlos Guerrero, U. Abbondanno, J. L. Tain, L. Audouin, B. Berthier, P. E. Koehler, L. Sarchiapone, D. Karadimos, R. Ferreira-Marques, T. Martinez, Heinz Oberhummer, E. Jericha, C. Le Naour, E. González-Romero, P. Pavlopoulos, Michael Wiescher, F. Voss, F. Becvar, W.I. Furman, F. Alvarez-Velarde, R. Vlastou, Marco T. Pigni, Nicola Colonna, Masayuki Igashira, E. Berthoumieux, Gerald Badurek, A. Plukis, Vasilis Vlachoudis, C. A. Papachristodoulou, F. Gramegna, K. Fujii, C. T. Papadopoulos, A. Lindote, C. Rubbia, C. Pretel, F. Käppeler, Isabel S. Gonçalves, S. Marrone, M. Kerveno, F. Neves, P. M. Milazzo, L. Perrot, V. Chepel, G. Rudolf, P. Baumann, G. Vannini, C. Carrapiço, D. Karamanis, I. Dillmann, Universitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear, Universitat Politècnica de Catalunya. GREENER - Grup de recerca d'estudis energètics i de les radiacions, Paradela C., Tassan-Got L., Audouin L., Berthier B., Ferrant L., Isaev S., Naour C. Le, Stephan C., Trubert D., David S., Duran I., Tarrio D., Alvarez H., Abbondanno U., Fujii K., Milazzo P. M., Moreau C., Aerts G., Alvarez-Velarde F., Cano-Ott D., Embid-Segura M., Gonzalez-Romero E., Guerrero C., Martinez T., Villamarin D., Vicente M. C., Andriamonje S., Berthoumieux E., Dridi W., Gunsing F., Pancin J., Perrot L., Plukis A., Andrzejewski J., Marganiec J., Assimakopoulos P., Karadimos D., Karamanis D., Papachristodoulou C., Patronis N., Badurek G., Jericha E., Leeb H., Oberhummer H., Pigni M. T., Baumann P., Kerveno M., Lukic S., Rudolf G., Becvar F., Krticka M., Calvino F., Cortes G., Poch A., Pretel C., Calviani M., Gramegna F., Mastinu P., Praena J., Capote R., Carrapico C., Cennini P., Chiaveri E., Dahlfors M., Ferrari A., Herrera-Martinez A., Kadi Y., Sarchiapone L., Vlachoudis V., Chepel V., Ferreira-Marques R., Lindote A., Lopes I., Neves F., Colonna N., Tagliente G., Terlizzi R., Couture A., Cox J., Marrone S., Obrien S., Wiescher M., Dillmann I., Heil M., Kappeler F., Mosconi M., Voss F., Walter S., Wisshak K., Domingo-Pardo C., Plag R., Plompen A., Tain J. L., Eleftheriadis C., Savvidis I., Furman W., Goncalves I., Salgado J., Santos C., Tavora L., Vaz P., Haas B., Haight R., Reifarth R., Igashira M., Koehler P., Kossionides E., Lampoudis C., Lozano M., Quesada J., Massimi C., Vannini G., Mengoni A., Oshima M., Papadopoulos C., Pavlik A., Pavlopoulos P., Vlastou R., Rauscher T., Rubbia C., Rullhusen P., Ventura A., Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Aval du cycle et Energie Nucléaire (ACEN), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Département Recherches Subatomiques (DRS-IPHC), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Pôle Universitaire Léonard de Vinci, Pôle Universitaire Léonard de Vinci (PULV), nTOF, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Energies::Energia nuclear [Àrees temàtiques de la UPC] ,Physics ,neutron fission cross section ,Np-237 ,Fission ,Nuclear data ,General Physics and Astronomy ,Nuclear energy ,020206 networking & telecommunications ,Energies::Energia nuclear::Reactors nuclears de fissió [Àrees temàtiques de la UPC] ,02 engineering and technology ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,Nuclear physics ,TIME-OF-FLIGHT ,Cross section (physics) ,Fusion reactors ,Reactors nuclears ,n TOF experiment ,0202 electrical engineering, electronic engineering, information engineering ,Energia nuclear ,020201 artificial intelligence & image processing ,Energy (signal processing) ,Neutron-induced ssion reactions - Abstract
In this document, we present the nal result obtained at the n TOF experiment for the neutron- induced ssion cross section of the 237Np, from the ssion threshold up to 1 GeV. The method applied to get this result is brie y discussed. n TOF data are compared to the last experimental measurements using other TOF facilities or the surrogate method, reported experiments performed with monoenergetic sources and the FISCAL systematic, including a discussion about the existing discrepancies.
- Published
- 2011
5. Neutron reactions and nuclear cosmo-chronology
- Author
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I. Goncalves, D. Karamanis, L. Ferrant, Thomas Rauscher, L. Fitzpatrick, D. Karadimos, M. Dahlfors, F. Gramegna, P. Vaz, P. Cennini, M. Rosetti, J. Cox, Rene Reifarth, M. C. Vincente, Alberto Ventura, Aaron Couture, Laurent Tassan-Got, P. M. Milazzo, V. Ketlerov, A. Pavlik, P. Pavlopoulos, Ralf Plag, J. M. Quesada, D. Villamarin, C. Lamboudis, J. L. Tain, G. Vannini, M. Oshima, F. Voss, E. Jericha, L. Sarchiapone, M. Mosconi, J. Andrzejewski, W.I. Furman, R. Gallino, Carlo Rubbia, V. Vlachoudis, Nicola Colonna, M. Embid-Segura, C. T. Papadopoulos, A. Lindote, J. Pancin, E. Griesmayer, C. Stephan, S. O'Brien, V. Konovalov, E. Chiaveri, D. Cano-Ott, K. Fujii, H. Alvarez-Pol, R. Vlastou, C. A. Papachristodoulou, R. Terlizzi, B. Haas, Michael Heil, Manuel Lozano, C. Paradela, A. Carrillo de Albornoz, F. Calviño, H. Leeb, S. Marrone, A. J. M. Plompen, I. Dillman, G. Aerts, S. Lukic, L. Tavora, Carlos Guerrero, C. Eleftheriadis, Masayuki Igashira, S. Isaev, U. Abbondanno, E. Kossionides, M. Kerveno, Heinz Oberhummer, G. Rudolf, Yacine Kadi, I. Lopes, G. Cortes, P. Rullhusen, C. Domingo Pardo, R. C. Haight, H. Frais-Koelbl, A. Herrera-Martinez, Alfredo Ferrari, R. Ferreira-Marques, Alberto Mengoni, C. Pretel, N. Patronis, W. Dridi, S. Bisterzo, K. Wisshak, L. Audouin, Roberto Capote, P.A. Assimakopoulos, Michael Wiescher, E. Berthoumieux, F. Neves, S. Walter, H. Wendler, A. Goverdovski, F. Gunsing, F. Alvarez-Velarde, I. Savvidis, Gerald Badurek, R. Dolfini, P. E. Koehler, I. Duran, V. Chepel, P. Baumann, J. Marganiec, S. Andriamonje, P. F. Mastinu, L. Perrot, F. Käppeler, M. Krtička, C. Moreau, J. Salgado, L. Marques, A. Poch, E. Gonzalez-Romero, A. Plukis, F. Bečvář, S. David, G. Tagliente, Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Pole Universitaire Leonard de Vinci, Pôle Universitaire Léonard de Vinci (PULV), nTOF, Universitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear, Universitat Politècnica de Catalunya. GREENER - Grup de recerca d'estudis energètics i de les radiacions, and Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
stars ,Neutron capture ,Nuclear and High Energy Physics ,Estels -- Estructura ,Inelastic scattering ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,01 natural sciences ,Nuclear physics ,Stellar cross sections ,Cross section (physics) ,0103 physical sciences ,Stars--Structure ,Neutron cross section ,Neutron ,cross-sections ,capture ,010303 astronomy & astrophysics ,milky-way ,isotopes ,Physics ,Neutrons ,Física [Àrees temàtiques de la UPC] ,Re/Os cosmo-chronometer ,010308 nuclear & particles physics ,stellar cross sections ,nucleosynthesis ,inelastic scattering ,Neutron temperature ,re/os cosmo-chronometer ,age ,13. Climate action ,r-process ,Atomic physics ,s-process ,s process ,neutron capture - Abstract
The beta-decay of Re-187 (t(1/2) = 42.3 Gyr) represents a suited cosmo-chronometer for the age of the r-process abundances, since the radiogenic part of the daughter isotope (OS)-O-187 is defined by the difference between the solar Os-187 abundance and s-process contribution to Os-187. The latter component can be determined via the s-process systematics based on the stellar neutron capture cross sections of Os-186 and Os-187. The laboratory cross section of Os-187 requires a significant correction for the effect of the low-lying excited state at 9.75 keV, which is strongly populated under stellar conditions. This theoretical correction can be improved by an experimental cross section for inelastic scattering to the 9.75 keV state. High resolution time-of-flight measurements of (n, gamma) cross sections of (OS)-O-186,187,188 from I eV to I MeV at CERN n-TOF facility are reported. The inferred stellar cross sections differ from previously recommended values. In addition, the inelastic scattering cross section has been measured at 30 keV neutron energy via time-of-flight at the Karlsruhe 3.7 MV Van de Graaff. The implications of these results for the Re/Os clock are discussed. (c) 2007 Elsevier B.V. All rights reserved. ispartof: Progress in Particle and Nuclear Physics vol:59 issue:1 pages:165-173 ispartof: location:ITALY, Erice status: published
- Published
- 2007
6. Teil 2: Innen
- Author
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Werner Gruber, Martin Puntigam, and Heinz Oberhummer
- Published
- 2015
7. Teil 3: Aussen
- Author
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Werner Gruber, Heinz Oberhummer, and Martin Puntigam
- Published
- 2015
8. Anhang
- Author
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Heinz Oberhummer, Martin Puntigam, and Werner Gruber
- Published
- 2015
9. Das Universum ist eine Scheißgegend
- Author
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Martin Puntigam, Werner Gruber, and Heinz Oberhummer
- Published
- 2015
10. Teil 1: Vorspiel im Himmel
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Werner Gruber, Martin Puntigam, and Heinz Oberhummer
- Published
- 2015
11. Teil 4: Jenseits
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Martin Puntigam, Heinz Oberhummer, and Werner Gruber
- Published
- 2015
12. Public Awareness Activities: NUPEX: Nuclear Physics Experience or How to Squeeze a Camel through the Needle's Eye
- Author
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Heinz Oberhummer and Rafael Reyeros-Bienert
- Subjects
Nuclear and High Energy Physics ,Process (engineering) ,business.industry ,Political science ,European Research Area ,Public relations ,business ,Public awareness - Abstract
One of the basic requirements for the process of creating and maintaining an innovative research area is the existence of a sufficient number of scientists and technicians. Scientific research at universities and research institutions is primarily dependent on enough students and young researchers being recruited for scientific research and careers. However, in the European research area already in the year 2010 about 700,000 scientific researchers and 1.2 million science-related personnel will be missing [1]. At many universities and other technological educational institutions the number of science—and in particular, physics—students has been stagnating at a low level for years.
- Published
- 2005
13. New experimental validation of the pulse height weighting technique for capture cross-section measurements
- Author
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L. Perrot, J. Pancin, F. Voss, Marco Radici, K. Wisshak, Ch.O. Bacri, V. Chepel, E. Berthomieux, L. Zanini, S. Marrone, P. Baumann, A. Lindote, T. Papaevangelou, M. Vincente-Vincente, Nicola Colonna, C. Tapia, M. Dahlfors, P. Vaz, G. Vannini, Per Carlson, M. Embid-Segura, H. Frais-Koelbl, E. Savvidis, F. Rejmund, H. Wendler, J. Salgado, A. Poch, Y. Giomataris, H. Álvarez, J. L. Tain, Saed Dababneh, L. Tavora, K.G. Ioannides, F. Gramegna, I. Duran, Aaron Couture, D. Cortina, M. Terrani, A. Goverdovski, George Kitis, F. Neves, P. M. Milazzo, A. Herrera-Martinez, Manuel Lozano, B. Berthier, R. Vlastou, F. Gunsing, Gerald Badurek, Ralf Plag, J. Benlliure, Alberto Mengoni, G. Cortes, A. Molina-Coballes, G. Aerts, A. Pavlik, N. Tsangas, Enrico Chiaveri, M. Rosetti, W. Rapp, P. Rullhusen, E. Gonzalez-Romero, R. Dolfini, N. Janeva, C. Domingo-Pardo, C. Eleftheriadis, E. Boscolo-Marchi, C. Paradela, E. Jericha, S. Markov, Roberto Capote, S. Lukic, A. Perez-Parra, Rene Reifarth, P. E. Koehler, P.A. Assimakopoulos, A. Kelic, I. F. Gonçalves, D. Cano-Ott, A. Plukis, P. Pavlopoulos, M.I. Lopes, F. Bečvář, P. Cennini, José M. Martínez-Val, S. David, J. M. Quesada, L. Tassan-Got, Sigfrido Boffi, S. Andriamonje, G. Tagliente, U. Abbondanno, Yacine Kadi, J.C. Soares, José Manuel Perlado, L. Ferrant, D. Karamanis, C. Borcea, C. Coceva, L. Ferreira-Lourenco, R. C. Haight, Heinz Oberhummer, Alfredo Ferrari, R. Ferreira-Marques, C. Stephan, S. O'Brien, E. Griesmayer, P. F. Mastinu, Michael Heil, A. Ventura, H. Beer, R. Terlizzi, E. Kossionides, H. Leeb, V. Ketlerov, D. Villamarin-Fernandez, F. Käppeler, Michael Wiescher, W.I. Furman, Carlo Rubbia, E. Mínguez, Subramanian Raman, A. J. M. Plompen, V. Peskov, V. Vlachoudis, A. Angelopoulos, N. Bustreo, G. Rudolf, P. Calviño, C. Moreau, V. Konovalov, V. Lacoste, C. Pretel, James L. Cox, Thomas Rauscher, A.J.P.L. Policarpo, Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), TOF, U.Abbondanno, G.Aert, H.Alvarez, S.Adriamonje, A.Angelopoulo, P.Assimakopoulo, C.Bacri, C.Badurek, P.Bauman, F.Becvar, H.Beer, J.Benlliure, B.Berthier, E.Berthoumieux, S.Boffi, C.Borcea, N.Bustreo, F.Calvino, D.Cano-Ott, R.Capote, P.Carlson, P.Cennini, V.Chepel, E.Chiaveri, N.Colonna, G.Corte, D.Cortina, A.Couture, J.Cox, S.Dababneh, M.Dahlfor, S.David, R.Dolfini, C.Domingo, I.Dura-Escribano, C.Eleftheriadi, M.Embid-Segura, L.Ferrant, A.Ferrari, L.Ferreira-Lourenco, R.Ferreira-Marque, H.Frais-Koelbl, W.Furman, Y.Giomatari, I.Goncalve, E.Gonzales-Romero, A.Goverdovski, F.Gramegna, E.Griiesmayer, F.GGunsing, R.Haight, M.Heil, A.Errera-Martinez, K.Ioannide, N.Janeva, E.Jericha, Y.Kadi, F.Kappeler, D.Karamani, A.Kelic, V.Ketlerov, G.Kiti, P.Koehler, V.Konovalov, E.Kossionide, V.Lacoste, H.Leeb, A.Lindote, I.Lope, M.Lozano, S.Lukic, S.Markov, S.Marrone, J.Martinez-Val, P.Mastinu, A.Mengoni, P.Milazzo, E.Minguez, C.Moreau, F.Neve, H.Oberhummer, S.O’Brien, J.Pancin, C.Paradela, A.Pavlik, P.Pavlopoulo, A.Perez-Parra, J.Perlado, L.Perrot, V.Peskov, R.Plag, A.Plomplen, A.Pluki, A.Poch, A.policarpo, C.Pretel, J.Quesada, M.Radici, W.Rapp, R.Reifarth, F.Rejmund, M.Rosetti, C.Rubbia, G.Rudolf, P.Rullhusen, J.Salgado, E.Savvidi, C.Stephan, G.Tagliente, J.Tain, C.Tapia, L.Tassan-Got, L.Tavora, M.Terrani, N.Tsanga, G.Vannini, P.Vaz, A.Ventura, D.Villamarin-Fernandez, M.Vincente-Vincente, V.Vlachoudi, R.Vlastou, F.Vo, H.Wendler, M.Wiescher, K.Wisshak, and L.Zanini
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Nuclear and High Energy Physics ,TheoryofComputation_COMPUTATIONBYABSTRACTDEVICES ,Monte Carlo method ,NUCLEAR PHYSICS ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,ComputingMethodologies_ARTIFICIALINTELLIGENCE ,01 natural sciences ,monte carlo simulations ,Cross section (physics) ,Optics ,0103 physical sciences ,neutron capture cross-sections ,010306 general physics ,Instrumentation ,Pulse height ,Physics ,010308 nuclear & particles physics ,business.industry ,Liquid scintillation counting ,Detector ,TheoryofComputation_GENERAL ,Experimental validation ,NEUTRON CROSS SECTIONS ,pulse height weighting technique ,c6d6 scintillation detectors ,Weighting ,Neutron capture ,ComputingMethodologies_PATTERNRECOGNITION ,business - Abstract
The accuracy of the pulse height weighting technique for the determination of neutron capture cross-sections is investigated. The technique is applied to measurements performed with C6D6 liquid scintillation detectors of two different types using capture samples of various dimensions. The data for well-known (n, gamma) resonances are analyzed using weighting functions obtained from Monte Carlo simulations of the experimental set-up. Several causes of systematic deviation are identified and their effect is quantified. In all the cases measured the reaction yield agrees with the standard value within 2%. (C) 2003 Elsevier B.V. All rights reserved. Nuclear Instruments & Methods in Physics Research Section a-Accelerators Spectrometers Detectors and Associated Equipment
- Published
- 2004
14. Temporal variation of coupling constants and nucleosynthesis
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M. M. Sharma, Attila Csoto, H. Schlattl, Heinz Oberhummer, and Malcolm Fairbairn
- Subjects
Coupling constant ,Physics ,Nuclear and High Energy Physics ,Particle physics ,Nuclear Theory ,Meson ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Fine-structure constant ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Oklo ,Nuclear Theory (nucl-th) ,High Energy Physics - Phenomenology ,General Relativity and Quantum Cosmology ,High Energy Physics - Phenomenology (hep-ph) ,Nucleosynthesis ,Time variations ,Nuclear Experiment ,Nucleon ,Variation (astronomy) - Abstract
We investigate the triple-alpha process and the Oklo phenomenon to obtain constraints on possible cosmological time variations of fundamental constants. Specifically we study cosmological temporal constraints for the fine structure constant and nucleon and meson masses., Comment: 4 pages. Proceedings of the Nuclear Physics in Astrophysics Conference, Debrecen, Hungary, September 30 - October 3, 2002. To be published in Nuc. Phys. A
- Published
- 2003
15. Neutron capture measurements of the noble gas isotopes 22Ne, 40Ar and 78,80,84,86Kr in the keV energy region
- Author
-
Walter Rochow, Heinz Oberhummer, H. Beer, Peter Mohr, and P. V. Sedyshev
- Subjects
Physics ,Nuclear reaction ,Nuclear and High Energy Physics ,Range (particle radiation) ,education.field_of_study ,Isotope ,Population ,Neutron temperature ,law.invention ,Neutron capture ,law ,Van de Graaff generator ,Neutron ,Atomic physics ,education - Abstract
At the Karlsruhe and Tubingen 3.75 MV Van de Graaff accelerators the cross sections of 22Ne(n,γ)23Ne (37.2 s), 40Ar(n,γ)41Ar (1.83 h), and the Kr isotopes 78Kr(n,γ)79Krm (50 s), 78Kr(n,γ)79Kr (35.04 h), 80Kr(n,γ)81Krm (13.1 s), 84Kr(n,γ)85Krm (4.48 h), and 86Kr(n,γ)87Kr (76.3 m), were measured in the keV energy range by the regular and/or the fast cyclic activation techniques via the characteristic γ-ray lines in the decay of the respective residual nuclei. High pressure gas samples which consisted of 22Ne–Kr and 40Ar–Kr mixtures were irradiated using the 7Li(p,n) and T(p,n) reactions. The measurements were carried out at the neutron energies 25, 30, 52, 104, 149, 180, and 215 keV. Stellar reaction rates for thermal energies kT between 1 and 250 keV were determined. The population probability of the 85Krm isomeric state by neutron capture of 84Kr was studied as a function of neutron energy. No significant energy dependence was found.
- Published
- 2002
16. Maßarbeit im Universum: Spezial: Kosmologie
- Author
-
Heinz Oberhummer
- Abstract
Es existieren in der modernen Physik mehrere eindrucksvolle Beispiele der Feinabstimmung des Kosmos fur die Existenz von Leben. Diese sehr unwahrscheinliche Feinabstimmungen liese sich durch die Existenz von unendlich vielen Universen (Multiversum) erklaren. Daruber hinaus haben physikalische Untersuchungen der Feinabstimmung des Universums Konsequenzen fur eine endgultige „Theorie fur Alles” und sind zu einer wahren Fundgrube fur Wissenschaftsdisziplinen jenseits der Physik geworden.
- Published
- 2002
17. Measurement and analysis of theAm243neutron capture cross section at the n_TOF facility at CERN
- Author
-
N. Colonna, S. David, G. Tagliente, B. Haas, M. Dahlfors, Masayuki Igashira, C. T. Papadopoulos, P. Vaz, W. Dridi, A. Ventura, Rene Reifarth, M. Oshima, J. M. Quesada, L. Tassan-Got, Aaron Couture, K. Wisshak, I. Savvidis, A. Plukis, C. Rubbia, J. Andrzejewski, Marco T. Pigni, J. Salgado, A. Poch, F. Voss, G. Vannini, L. Tavora, Isabel S. Gonçalves, S. Marrone, Christoph A. Stephan, J. Marganiec, L. Ferrant, L. Sarchiapone, M. C. Vicente, C. Pretel, G. Aerts, P. Rullhusen, Vasilis Vlachoudis, M. Krtička, D. Karamanis, I. Dillmann, E. Kossionides, J. Balibrea, H. Wendler, L. Fitzpatrick, F. Neves, R. C. Haight, J. L. Tain, R. Ferreira-Marques, T. Martinez, F. Gramegna, Javier Praena, S. Lo Meo, P. M. Milazzo, P. Cennini, Matthias Heil, J. Pancin, D. Villamarin, F. Gunsing, A. Herrera-Martinez, N. Patronis, S. Andriamonje, A. Lindote, C. Lampoudis, C. Paradela, L. Audouin, Isabel Lopes, M. Mosconi, Y. Kadi, H. Frais-Koelbl, M. Kerveno, G. Cortes, A. Goverdovski, Michael Wiescher, S. Isaev, P. E. Koehler, E. Chiaveri, P. F. Mastinu, A. Pavlik, C. Domingo-Pardo, F. Alvarez-Velarde, Cristian Massimi, Gerald Badurek, S. O'Brien, C. Carrapiço, Arnaud Ferrari, L. Perrot, K. Fujii, Marco Calviani, R. Dolfini, Roberto Capote, R. Terlizzi, A. Carrillo de Albornoz, P.A. Assimakopoulos, S. Lukic, P. Pavlopoulos, Fabio Belloni, D. Cano-Ott, R. Vlastou, E. Berthoumieux, F. Calviño, H. Leeb, V. Chepel, C. Santos, G. Rudolf, F. Bečvář, E. Mendoza, E. Jericha, R. Lossito, E. Griesmayer, P. Baumann, I. Duran, Carlos Guerrero, U. Abbondanno, C. Eleftheriadis, Heinz Oberhummer, Thomas Rauscher, D. Karadimos, E. González-Romero, A. Mengoni, V. Ketlerov, W.I. Furman, C. A. Papachristodoulou, S. Walter, Ralf Plag, V. Konovalov, F. Käppeler, L. Marques, Manuel Lozano, Corrie S. Moreau, A. J. M. Plompen, and James L. Cox
- Subjects
Physics ,Nuclear reaction ,Nuclear physics ,Nuclear and High Energy Physics ,Cross section (physics) ,Nuclear transmutation ,Neutron cross section ,Neutron ,7. Clean energy ,Resonance (particle physics) ,Neutron temperature ,Calorimeter - Abstract
Background: The design of new nuclear reactors and transmutation devices requires to reduce the present neutron cross section uncertainties of minor actinides. Purpose: Improvement of the 243Am(n,? ) cross section uncertainty. Method: The 243Am(n,? ) cross section has been measured at the n_TOF facility at CERN with a BaF2 total absorption calorimeter, in the energy range between 0.7 eV and 2.5 keV. Results: The 243Am(n,? ) cross section has been successfully measured in the mentioned energy range. The resolved resonance region has been extended from 250 eV up to 400 eV. In the unresolved resonance region our results are compatible with one of the two incompatible capture data sets available below 2.5 keV. The data available in EXFOR and in the literature have been used to perform a simple analysis above 2.5 keV. Conclusions: The results of this measurement contribute to reduce the 243Am(n,? ) cross section uncertainty and suggest that this cross section is underestimated up to 25% in the neutron energy range between 50 eV and a few keV in the present evaluated data libraries.
- Published
- 2014
18. Neutron-induced fission cross section ofU234measured at the CERN n_TOF facility
- Author
-
C. Domingo-Pardo, J. Salgado, A. Poch, M. Kerveno, G. Cortes, M. Sedysheva, F. Gunsing, M. Oshima, R. C. Haight, J. Andrzejewski, Cristian Massimi, L. Sarchiapone, Carlo Rubbia, Ralf Plag, V. Vlachoudis, Roberto Capote, L. Audouin, K. C. Stamoulis, P. Assimakopoulos, F. Neves, E. Griesmayer, V. Ketlerov, M. Diakaki, I. Duran, Alberto Mengoni, C. Papadopoulos, A. J. M. Plompen, V. Chepel, Michael Wiescher, G. Rudolf, I. Lopes, A. Herrera-Martinez, N. Patronis, P. Baumann, H. Leeb, M. Igashira, G. Vannini, P. E. Koehler, P. M. Milazzo, W. Dridi, B. Haas, Alfredo Ferrari, R. Ferreira-Marques, S. G. Isaev, R. Gallino, E. Gonzalez-Romero, E. Berthoumieux, Michael Heil, W.I. Furman, L. Perrot, C. Eleftheriadis, F. Bečvář, K. Ioannidis, S. Marrone, Rene Reifarth, K. Wisshak, R. Vlastou, A. Plukis, A. Lindote, C. Moreau, M. Rosetti, H. Frais-Koelbl, J. Pancin, E. Chiaveri, D. Cano-Ott, V.Y. Konovalov, Yacine Kadi, H. Wendler, P. Vaz, H. Álvarez, C. Lamboudis, J. L. Tain, I. Goncalves, Thomas Rauscher, Alberto Ventura, Aaron Couture, D. Karadimos, Carlos Guerrero, Heinz Oberhummer, A. Dorochenko, M. Krtička, F. Calviño, G. Aerts, E. Jericha, J. Marganiec, S. Andriamonje, L. Fitzpatrick, P. F. Mastinu, S. O'Brien, M. Embid-Segura, C. Pretel, A. Carrillo de Albornoz, Manuel Lozano, L. Ferrant, D. Villamarin, J. Cox, Laurent Tassan-Got, L. Marques, M. C. Vincente, A. Goverdovski, L. Tavora, F. Alvarez-Velarde, K. Fuji, Gerald Badurek, C. Paradela, R. Dolfini, S. Lukic, P. Rullhusen, U. Abbondanno, I. Savvidis, F. Voss, A. Tsinganis, D. Kolokolov, Nicola Colonna, P. Pavlopoulos, S. David, G. Tagliente, P. Cennini, J. M. Quesada, D. Karamanis, M. Mosconi, C. Stephan, R. Terlizzi, F. Gramegna, F. Käppeler, Paraskevi Demetriou, and A. Pavlik
- Subjects
Physics ,Nuclear and High Energy Physics ,Large Hadron Collider ,010308 nuclear & particles physics ,Fission ,Detector ,Flux ,01 natural sciences ,7. Clean energy ,Nuclear physics ,Cross section (physics) ,0103 physical sciences ,Ionization chamber ,Neutron ,Nuclear Experiment ,010306 general physics ,High energy resolution - Abstract
The neutron-induced fission cross section of U234 has been measured at the CERN n-TOF facility relative to the standard fission cross section of U235 from 20 keV to 1.4 MeV and of U238 from 1.4 to 200 MeV. A fast ionization chamber (FIC) was used as a fission fragment detector with a detection efficiency of no less than 97%. The high instantaneous flux and the low background characterizing the n-TOF facility resulted in wide-energy-range data (0.02 to 200 MeV), with high energy resolution, high statistics, and systematic uncertainties bellow 3%. Previous investigations around the energy of the fission threshold revealed structures attributed to β-vibrational levels, which have been confirmed by the present measurements. Theoretical calculations have been performed, employing the talys code with model parameters tuned to fairly reproduce the experimental data. © 2014 American Physical Society.
- Published
- 2014
19. Study of 234U(n,f) resonances measured at the CERN n TOF facility
- Author
-
B. Berthier, E. Kossionides, Javier Praena, V. Chepel, B. Haas, J. Marganiec, P. Cennini, S. Andriamonje, G. Vannini, C. Lampoudis, S. David, G. Tagliente, S. Lukic, E. Chiaveri, Corrie S. Moreau, W. Dridi, S. Walter, P. Baumann, A. Pavlik, Ralf Plag, P. F. Mastinu, P. E. Koehler, M. Mosconi, M. Kerveno, A. Ventura, C. Domingo-Pardo, L. Sarchiapone, R. Vlastou, C. Pretel, A. J. M. Plompen, J. Salgado, C. Stephan, S. O'Brien, Rene Reifarth, M. Embid-Segura, G. Aerts, E. Berthoumieux, F. Voss, A. Poch, P. Pavlopoulos, J. M. Quesada, L. Tassan-Got, G. Cortes, G. Rudolf, I. Lopes, I. Dillmann, D. Tarrío, Manuel Lozano, Matthias Heil, M. Oshima, Nicola Colonna, R. Terlizzi, L.S. Leong, Carlos Guerrero, M. C. Vincente, James L. Cox, Marco T. Pigni, Vasilis Vlachoudis, I. Duran, J. Andrzejewski, A. Herrera-Martinez, L. Tavora, Heinz Oberhummer, F. Gramegna, Arnaud Ferrari, Roberto Capote, Masayuki Igashira, D. Cano-Ott, Y. Kadi, A. Plukis, L. Perrot, F. Käppeler, E. Leal-Cidoncha, C. Eleftheriadis, P. Rullhusen, L. Ferrant, W.I. Furman, C. Carrapiço, S. Isaev, Thomas Rauscher, K. Fujii, R. C. Haight, F. Alvarez-Velarde, Marco Calviani, U. Abbondanno, M. Krtička, F. Calviño, Alberto Mengoni, D. Karadimos, M. Dahlfors, C. Paradela, K. Wisshak, R. Ferreira-Marques, T. Martinez, P. Vaz, I. Savvidis, Gerald Badurek, E. González-Romero, L. Audouin, H. Álvarez, Aaron Couture, J. L. Tain, Michael Wiescher, J. Pancin, C. T. Papadopoulos, D. Villamarin, C. Rubbia, Isabel S. Gonçalves, S. Marrone, A. Lindote, H. Leeb, E. Jericha, F. Gunsing, D. Trubert, Cristian Massimi, F. Neves, P. M. Milazzo, C. Santos, F. Bečvář, C. Le Naour, Universitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear, and Universitat Politècnica de Catalunya. GREENER - Grup de recerca d'estudis energètics i de les radiacions
- Subjects
Physics ,Nuclear reaction ,Neutrons ,Energies::Energia nuclear [Àrees temàtiques de la UPC] ,Nuclear and High Energy Physics ,Fission ,Large Hadron Collider ,Cross section ,TOF ,Resonance ,Nuclear data ,Neutron ,Nuclear physics ,Cross section (physics) ,Neutron cross section ,Nuclear Reactions - Abstract
We present the analysis of the resolved resonance region for the 234U(n,f) cross section data measured at the CERN n TOF facility. The resonance parameters in the energy range from 1 eV to 1500 eV have been obtained with the SAMMY code by using as initial parameters for the fit the resonance parameters of the JENDL-3.3 evaluation. In addition, the statistical analysis has been accomplished, partly with the SAMDIST code, in order to study the level spacing and the Mehta-Dyson correlation.
- Published
- 2014
20. The Nambu–Jona–Lasinio model of light nuclei
- Author
-
N. I. Troitskaya, A. N. Ivanov, Heinz Oberhummer, and Manfried Faber
- Subjects
Quark ,Physics ,Quantum chromodynamics ,Nuclear and High Energy Physics ,Particle physics ,High Energy Physics::Lattice ,Critical phenomena ,High Energy Physics::Phenomenology ,Nuclear Theory ,Hadron ,Quantum electrodynamics ,Nambu–Jona-Lasinio model ,Nuclear fusion ,Nuclear Experiment ,Nucleon ,Excitation - Abstract
The Nambu–Jona–Lasinio model of the deuteron suggested by Nambu and Jona–Lasinio (Phys. Rev. 124 (1961) 246) is formulated from the first principles of QCD. The deuteron appears as a neutron–proton collective excitation, i.e. a Cooper np–pair, induced by a phenomenological local four–nucleon interaction in the nuclear phase of QCD. The model describes the deuteron coupled to itself, nucleons and other particles through one–nucleon loop exchanges providing a minimal transfer of nucleon flavours from initial to final nuclear states and accounting for contributions of nucleon–loop anomalies which are completely determined by one–nucleon loop diagrams. The dominance of contributions of nucleon–loop anomalies to effective Lagrangians of low–energy nuclear interactions is justified in the large NC expansion, where NC is the number of quark colours.
- Published
- 2000
21. [Untitled]
- Author
-
Peter Habison, Christian Gottfried, and Heinz Oberhummer
- Subjects
Physics ,Multimedia ,Space and Planetary Science ,ESPACE ,ComputingMilieux_COMPUTERSANDEDUCATION ,Astronomy and Astrophysics ,computer.software_genre ,computer - Abstract
The paper describes the European System for Particle and AstrophysicalCyber Education (ESPACE). After a general introduction to the projectand its ideas the contents of the multimedia teaching and learning systemare presented. It is followed by a discussion about the didactical aspectsof modern multimedia technology related to the project. Finally themultimedia and programming structures are explained and futureperspectives are given.
- Published
- 2000
22. Neutron capture of46Caat thermonuclear energies
- Author
-
Peter J. Mohr, Yu. P. Popov, W. Stadler, Heinz Oberhummer, Walter Rochow, P. V. Sedyshev, and H. Beer
- Subjects
Nuclear physics ,Physics ,Nuclear and High Energy Physics ,Neutron capture ,Thermonuclear fusion ,Radiative capture ,Neutron cross section ,r-process ,Neutron ,Neutron scattering - Published
- 1999
23. Thermal neutron induced (n,p) and (n,α) reactions on 37Ar
- Author
-
B. Denecke, M. Gaelens, C. Wagemans, R. Bieber, M. Loiselet, P. Geltenbort, Gert Goeminne, Heinz Oberhummer, and Jan Wagemans
- Subjects
Physics ,Nuclear and High Energy Physics ,High flux ,Analytical chemistry ,FOS: Physical sciences ,Alpha (ethology) ,Nuclear Experiment (nucl-ex) ,Nuclear Experiment ,Neutron temperature - Abstract
The 37Ar(n_th,alpha)34S and 37Ar(n_th,p)37Cl reactions were studied at the high flux reactor of the ILL in Grenoble. For the 37Ar(n_th,alpha_0) and 37Ar(n_th,p) reaction cross sections, values of (1070+/-80)b and (37+/-4)b, respectively, were obtained. Both values are about a factor 2 smaller than results of older measurements. The observed suppression of the 37(n_th,alpha_1) transition could be verified from theoretical considerations. Finally, evidence was found for the two-step 37Ar(n_th,gamma-alpha) process., 11 pages, 5 figures, accepted for publication in Nuclear Physics A
- Published
- 1999
24. Absolute measurement of the5/2+resonance of36Ar(p,γ)37KatEp=918 keV
- Author
-
Á.Z. Kiss, I. Borbely-Kiss, E. Somorjai, Heinz Oberhummer, Gyuri Gyürky, and Peter Mohr
- Subjects
Physics ,Nuclear and High Energy Physics ,Absolute measurement ,Radiative capture ,Resonance ,Atomic physics ,Omega - Abstract
The strength of the ${5/2}^{+}$ resonance of the reaction ${}^{36}\mathrm{Ar}(p,\ensuremath{\gamma}{)}^{37}\mathrm{K}$ at ${E}_{p}=918 \mathrm{keV}$ was measured absolutely: $\ensuremath{\omega}\ensuremath{\gamma}=(258\ifmmode\pm\else\textpm\fi{}24) \mathrm{meV}.$ The new result is consistent with previous results. This resonance was used in several experiments as a calibration standard. Therefore we discuss our experimental uncertainties in detail which is important for the reliability of previous experiments and our new result.
- Published
- 1999
25. Nuclei in the Cosmos
- Author
-
Heinz Oberhummer and Heinz Oberhummer
- Subjects
- Nuclear astrophysics
- Abstract
Nuclear astrophysics as it stands today is a fascinating science. Even though, compared to other scientific fields, it is a young discipline which has developed only in this century, it has answered many questions concerning the under standing of our cosmos. One of these great achievements was the concept of nucleosynthesis, the creation of the elements in the early universe in interstellar matter and in stars. Nuclear astrophysics has continued, to solve many riddles of the evolution of the myriads of stars in our cosmos. This review volume attempts to provide an overview of the current status of nuclear astrophysics. Special emphasis is given to the interdisciplinary nature of the field: astronomy, nuclear physics, astrophysics and particle physics are equally involved. One basic effort of nuclear astrophysics is the collection of ob servational facts with astronomical methods. Laboratory studies of the nuclear processes involved in various astrophysical scenarios have provided fundamen tal information serving both as input for and test of astrophysical models. The theoretical understanding of nuclear reaction mechanisms is necessary, for example, to extrapolate the experimentally determined reaction rates to the thermonuclear energy range, which is relevant for the nuclear processes in our cosmos. Astrophysical models and calculations allow us to simulate how nuclear processes contribute to driving the evolution of stars, interstellar matter and the whole universe. Finally, elementary particle physics also plays an important role in the field of nuclear astrophysics, for instance through weak interaction processes involving neutrinos.
- Published
- 2012
26. Thermonuclear reaction rate of23Mg(p,γ)24Al
- Author
-
P.M. Endt, Christian Iliadis, M. Fantini, Heinz Oberhummer, and H. Herndl
- Subjects
Physics ,Nuclear and High Energy Physics ,Photon ,Thermonuclear fusion ,Proton ,Astrophysics::High Energy Astrophysical Phenomena ,White dwarf ,Mass formula ,Nuclear physics ,Nucleosynthesis ,Astrophysics::Solar and Stellar Astrophysics ,Atomic physics ,Multiplet ,Excitation - Abstract
Updated stellar rates for the reaction {sup 23}Mg(p,{gamma}){sup 24}Al are calculated by using all available experimental information on {sup 24}Al excitation energies. Proton and {gamma}-ray partial widths for astrophysically important resonances are derived from shell-model calculations. Correspondences of experimentally observed {sup 24}Al levels with shell-model states are based on application of the isobaric multiplet mass equation. Our new rates suggest that the {sup 23}Mg(p,{gamma}){sup 24}Al reaction influences the nucleosynthesis in the mass A{gt}20 region during thermonuclear runaways on massive white dwarfs. {copyright} {ital 1998} {ital The American Physical Society}
- Published
- 1998
27. Neutron capture of26Mgat thermonuclear energies
- Author
-
Peter J. Mohr, H. Beer, Yu. P. Popov, Walter Rochow, W. Stadler, P. V. Sedyshev, and Heinz Oberhummer
- Subjects
Physics ,Nuclear physics ,Nuclear and High Energy Physics ,Cross section (physics) ,Neutron capture ,Thermonuclear fusion ,Astrophysics::High Energy Astrophysical Phenomena ,Activation technique ,Radiative capture ,Neutron cross section ,Resonance ,Atomic physics ,Nuclear theory - Abstract
The neutron capture cross section of 26Mg was measured relative to the known gold cross section at thermonuclear energies using the fast cyclic activation technique. The experiment was performed at the 3.75 MV Van-de-Graaff accelerator, Forschungszentrum Karlsruhe. The experimental capture cross section is the sum of resonant and direct contributions. For the resonance at E(n,lab) = 220 keV our new results are in disagreement with the data from Weigmann et al. An improved Maxwellian averaged capture cross section is derived from the new experimental data taking into account s- and p-wave capture and resonant contributions. The properties of so-called potential resonances which influence the p-wave neutron capture of 26}Mg are discussed in detail.
- Published
- 1998
28. Low–energy photodisintegration of 9Be and α+α+n→9Be +γ reactions at astrophysical conditions
- Author
-
Victor D. Efros, Heinz Oberhummer, Ian J. Thompson, and A. Pushkin
- Subjects
Physics ,Nuclear physics ,Reaction rate ,Nuclear and High Energy Physics ,Radionuclide ,medicine.anatomical_structure ,Low energy ,Photodisintegration ,Nuclear Theory ,medicine ,Alpha (ethology) ,Nuclear Experiment ,Nucleus - Abstract
A semi-microscopic model for the low-energy photodisintegration of the 9Be nucleus is constructed, and the experimental data are analyzed with its help. The older radioactive isotope data are supported by this analysis. The theoretical photodisintegration cross section is derived. The astrophysical rates for the reaction alpha + alpha + n -> 9Be + gamma and the reverse photodisintegration of 9Be are calculated. The new reaction rate for alpha + alpha + n -> 9Be + gamma is compared with previous estimations.
- Published
- 1998
29. Halo Properties of the First1/2+State inF17from theO16(p,γ)F17Reaction
- Author
-
G. Staudt, V. Kölle, Heinz Oberhummer, R. Morlock, Peter Mohr, A. Mayer, Axel H. E. Müller, J. W. Hammer, R. Kunz, and M. Jaeger
- Subjects
Physics ,Excited state ,General Physics and Astronomy ,State (functional analysis) ,Halo ,Atomic physics ,Energy (signal processing) ,Oxygen-16 - Abstract
The capture cross section of the reaction ${}^{16}\mathrm{O}(p,\ensuremath{\gamma}{)}^{17}\mathrm{F}$ was measured in the energy range from ${E}_{\mathrm{c}.\mathrm{m}.}\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}200--3750\mathrm{keV}$ using the windowless gas target facility Rhinoceros. The low-energy $S$ factor that is dominated by the transition to the $1/{2}^{+}$ first excited state in ${}^{17}\mathrm{F}$ increases strikingly with decreasing energy. This behavior is explained by the halo properties of this $1/{2}^{+}$ state within the framework of the direct capture model.
- Published
- 1997
30. Experimental cross section of 144Sm(α, γ)148Gd
- Author
-
H. P. Trautvetter, Zs. Fülöp, Uwe Greife, Á. Z. Kiss, Marc Rayet, E. Somorjai, Marcel Arnould, C. Rolfs, M. Junker, and Heinz Oberhummer
- Subjects
Nuclear physics ,Physics ,Nuclear and High Energy Physics ,Range (particle radiation) ,Cross section (physics) ,medicine.anatomical_structure ,Nuclear track ,Solid-state ,medicine ,Alpha decay ,Activation method ,Atomic physics ,Nucleus - Abstract
The cross section of the 144 Sm(α, γ) 148 Gd reaction have been measured in the bombarding energy range of 10.5–13.4 MeV, using activation method based on the off-line α-activity measurement of the 148 Gd residual nucleus. The long measuring time of the alpha decay demanded the utilization of solid state nuclear track detectors (SSNTD). The first results are compared to the latest statistical model calculations.
- Published
- 1997
31. Three-alpha structures in 12C
- Author
-
Heinz Oberhummer, Rudolf Pichler, Steven A. Moszkowski, and Attila Csoto
- Subjects
Physics ,Nuclear and High Energy Physics ,Alpha (programming language) ,Stellar nucleosynthesis ,Cluster (physics) ,Resonance ,State (functional analysis) ,Scaling ,Molecular physics - Abstract
We search for three-alpha resonances in C-12 by using the complex scaling method in a microscopic cluster model. All experimentally known low-lying natural-parity states are localized. For the first time we unambiguously show that the 0+_2 state in C-12, which plays an important role in stellar nucleosynthesis, is a genuine three-alpha resonance.
- Published
- 1997
32. 144Sm-αoptical potential at astrophysically relevant energies derived from144Sm(α,α)144Sm elastic scattering
- Author
-
Z. Máté, Peter Mohr, G. Staudt, M. Jaeger, Zs. Fülöp, Thomas Rauscher, E. Somorjai, and Heinz Oberhummer
- Subjects
Physics ,Elastic scattering ,Nuclear and High Energy Physics ,Angular distribution ,Nucleosynthesis ,Scattering ,Atomic physics ,Optical potential ,Nuclear theory ,Energy (signal processing) - Abstract
For the determination of the ${}^{144}$Sm-$\ensuremath{\alpha}$ optical potential we measured the angular distribution of ${}^{144}$Sm$(\ensuremath{\alpha}$,$\ensuremath{\alpha})$${}^{144}$Sm scattering at the energy ${E}_{\mathrm{lab}}=20\mathrm{ }\mathrm{MeV}$ with high accuracy. Using the known systematics of $\ensuremath{\alpha}$-nucleus optical potentials we are able to derive the ${}^{144}$Sm-$\ensuremath{\alpha}$ optical potential at the astrophysically relevant energy ${E}_{\mathrm{c}.\mathrm{m}.}=9.5$ MeV with very limited uncertainties.
- Published
- 1997
33. [Untitled]
- Author
-
A. N. Ivanov, Manfried Faber, Heinz Oberhummer, and N. I. Troitskaya
- Subjects
Physics ,Nuclear physics ,Reaction rate ,Nuclear reaction ,Deuterium ,Space and Planetary Science ,Solar neutrino ,Theoretical methods ,Astronomy and Astrophysics ,Solar neutrino problem ,Branching (polymer chemistry) ,Cosmology - Abstract
The present status of the nuclear reaction rates determining the solar neutrino flux is discussed. This includes the reaction rates for the two branching ratios of the three pp-chains involving the reactions 3He(3He,2p)4He and 3He(4He,γ)7Be for the first branching, and 7Be(e−, νe)7Li and 7Be(p, γ)8B for the second branching. Mainly we will concentrate on the basic nuclear reaction p + p → D + e+ + νe of the pp-chains. This reaction rate can only be determined using the theoretical methods. The present status of the application of the relativistic field theory model of the deuteron for this reaction will be discussed.
- Published
- 1997
34. Nuclei in the Cosmos: Present Status and the Future of Nuclear Astrophysics
- Author
-
Michael Wiescher and Heinz Oberhummer
- Subjects
Physics ,Nuclear astrophysics ,Astronomy ,Astrophysics - Published
- 1997
35. THE Am-243 NEUTRON CAPTURE MEASUREMENT AT THE n_TOF FACILITY
- Author
-
F. Gramegna, N. Colonna, Marco T. Pigni, A. Pavlik, G. Vannini, K. Fujii, L. Tavora, M. Rosetti, Fabio Belloni, A. Plukis, L. Perrot, I. Savvidis, F. Käppeler, P. Rullhusen, S. David, Manuel Lozano, D. Cano-Ott, C. Eleftheriadis, V. Chepel, F. Voss, G. Tagliente, A. Ventura, G. Rudolf, M. Dahlfors, F. Becvar, E. Mendoza, A. Lindote, F. Calviño, Thomas Rauscher, E. Jericha, P. Vaz, H. Leeb, I. Duran, G. Cortes, P. Baumann, C. Domingo Pardo, A. Herrera-Martinez, P. Cennini, Isabel Lopes, D. Karadimos, L. Marques, Aaron Couture, J. Salgado, R. Vlastou, A. Poch, E. Berthoumieux, J. Marganiec, E. González-Romero, L. Sarchiapone, Vasilis Vlachoudis, C. Pretel, A. Mengoni, A. Ferrari, K. Wisshak, M. Meaze, Roberto Capote, P.A. Assimakopoulos, R. C. Haight, A. Goverdovski, M. Mosconi, Costas G. Papadopoulos, B. Haas, V. Ketlerov, C. Paradela, L. Audouin, S. O'Brien, F. Alvarez-Velarde, L. Ferrant, D. Karamanis, N. Patronis, M. Oshima, Matthias Heil, J. Pancin, R. Terlizzi, J. Andrzejewski, Michael Wiescher, W.I. Furman, H. Wendler, S. Isaev, Masayuki Igashira, S. Lukic, Gerald Badurek, C. Stephan, F. Gunsing, W. Dridi, F. Neves, Y. Kadi, Rene Reifarth, H. Frais-Koelbl, Cristian Massimi, P. M. Milazzo, V. Konovalov, I. Dillman, J. M. Quesada, L. Tassan-Got, R. Dolfini, Marco Calviani, C. A. Papachristodoulou, D. Villamarin, A. Carrillo de Albornoz, E. Griesmayer, Carlos Guerrero, U. Abbondanno, Heinz Oberhummer, P. Pavlopoulos, S. Walter, P. E. Koehler, Ralf Plag, A. García-Rios, C. Rubbia, G. Aerts, Isabel S. Gonçalves, S. Marrone, M. Kerveno, Corrie S. Moreau, A. J. M. Plompen, James L. Cox, M. Krtička, R. Ferreira-Marques, T. Martinez, H. Álvarez, J. L. Tain, E. Kossionides, Javier Praena, S. Andriamonje, E. Chiaveri, P. F. Mastinu, and C. Lampoudis
- Subjects
Nuclear physics ,Neutron capture ,Materials science - Published
- 2013
36. The93Zr(n,γ) reaction up to 8 keV neutron energy
- Author
-
L. Perrot, M. Dahlfors, E. Jericha, P. Vaz, Aaron Couture, S. Walter, A. Herrera-Martinez, N. Patronis, Ralf Plag, H. Álvarez, S. David, C. Lamboudis, J. L. Tain, W.I. Furman, Arnaud Ferrari, L. Tavora, C. A. Papachristodoulou, M. Rosetti, G. Tagliente, D. Karamanis, I. Dillmann, Carlos Guerrero, U. Abbondanno, Heinz Oberhummer, K. Wisshak, E. Kossionides, A. Ventura, F. Käppeler, Corrie S. Moreau, C. Eleftheriadis, Javier Praena, M. Kerveno, J. Andrzejewski, G. Vannini, Marco Calviani, B. Haas, V. Chepel, G. Rudolf, P. Rullhusen, A. Plukis, J. Salgado, G. Aerts, A. Poch, C. Santos, D. Karadimos, F. Neves, P. M. Milazzo, P. Baumann, C. Carrapiço, D. Villamarin, F. Gunsing, E. González-Romero, A. Pavlik, A. Mengoni, C. Pretel, W. Dridi, M. Krtička, F. Calviño, Rene Reifarth, Cristian Massimi, F. Bečvář, C. Domingo-Pardo, L. Sarchiapone, R. Ferreira-Marques, T. Martinez, A. J. M. Plompen, J. M. Quesada, F. Voss, P. Cennini, Marco T. Pigni, Matthias Heil, I. Duran, J. Marganiec, S. Andriamonje, L. Tassan-Got, G. Cortes, P. Pavlopoulos, E. Chiaveri, M. Embid-Segura, F. Alvarez-Velarde, H. Leeb, I. Savvidis, M. Mosconi, P. F. Mastinu, Y. Kadi, S. O'Brien, Gerald Badurek, R. C. Haight, D. Cano-Ott, R. Terlizzi, Roberto Capote, C. Paradela, L. Audouin, Nicola Colonna, K. Fujii, Vasilis Vlachoudis, R. Vlastou, E. Berthoumieux, Fabio Belloni, M. C. Vincente, Christoph A. Stephan, S. Lukic, A. Lindote, F. Gramegna, Isabel Lopes, Michael Wiescher, C. T. Papadopoulos, C. Rubbia, Isabel S. Gonçalves, and S. Marrone
- Subjects
Physics ,Nuclear and High Energy Physics ,Radionuclide ,Range (particle radiation) ,Nuclear transmutation ,Physics::Instrumentation and Detectors ,010308 nuclear & particles physics ,Resonance ,7. Clean energy ,01 natural sciences ,Neutron temperature ,Nuclear physics ,Time of flight ,13. Climate action ,Nucleosynthesis ,0103 physical sciences ,Physics::Accelerator Physics ,Atomic physics ,Nuclear Experiment ,s-process ,010303 astronomy & astrophysics - Abstract
The (n,γ) reaction of the radioactive isotope 93Zr has been measured at the n-TOF high-resolution time-of-flight facility at CERN. Resonance parameters have been extracted in the neutron energy range up to 8 keV, yielding capture widths smaller (14%) than reported in an earlier experiment. These results are important for detailed nucleosynthesis calculations and for refined studies of waste transmutation concepts. © 2013 American Physical Society.
- Published
- 2013
37. We are made up of stardust, literally
- Author
-
Heinz Oberhummer
- Abstract
Astrophysik beschaftigt sich mit den physikalischen Grundlagen der Erforschung des Universums und versucht, seinen Aufbau und seine Entstehungsgeschichte zu erklaren. Heinz Oberhummer gilt als Experte im Bereich der Feinabstimmung der Naturkonstante — eines physikalischen Messwerts, der sich weder raumlich noch zeitlich verandert: Der Forscher untersuchte die kosmologische Feinabstimmung der grundlegenden Krafte im Universum bei der Entstehung der „lebenswichtigen“ Elemente Kohlenstoff und Sauerstoff in Roten-Riesen- Sternen. Die Erkenntnisse wurden in der renommierten Fachzeitschrift „Science“ publiziert.
- Published
- 2013
38. Measurement of neutron capture onCa48at thermal and thermonuclear energies
- Author
-
C. Coceva, H. Beer, R. Hofinger, Yu. P. Popov, Peter Mohr, P. V. Sedyshev, Heinz Oberhummer, and H. Herndl
- Subjects
Physics ,Nuclear and High Energy Physics ,Astrophysics::High Energy Astrophysical Phenomena ,Binding energy ,Gamma ray ,Scattering length ,Neutron scattering ,law.invention ,Neutron capture ,law ,Van de Graaff generator ,Neutron ,Atomic physics ,Line (formation) - Abstract
At the Karlsruhe pulsed 3.75 MV Van de Graaff accelerator the thermonuclear $^{48}\mathrm{Ca}$(n,\ensuremath{\gamma}${)}^{49}$Ca(8.72 min) cross section was measured by the fast cyclic activation technique via the 3084.4 keV \ensuremath{\gamma}-ray line of the $^{49}\mathrm{Ca}$ decay. Samples of ${\mathrm{CaCO}}_{3}$ enriched in $^{48}\mathrm{Ca}$ by 77.87% were irradiated between two gold foils which served as capture standards. The capture cross section was measured at the neutron energies 25, 151, 176, and 218 keV, respectively. Additionally, the thermal capture cross section was measured at the reactor BR1 in Mol, Belgium, via the prompt and decay \ensuremath{\gamma}-ray lines using the same target material. The $^{48}\mathrm{Ca}$(n,\ensuremath{\gamma}${)}^{49}$Ca cross section in the thermonuclear and thermal energy range has been calculated using the direct-capture model combined with folding potentials. The potential strengths are adjusted to the scattering length and the binding energies of the final states in $^{49}\mathrm{Ca}$. The small coherent elastic cross section of $^{48}\mathrm{Ca}$+n is explained through the nuclear Ramsauer effect. Spectroscopic factors of $^{49}\mathrm{Ca}$ have been extracted from the thermal capture cross section with better accuracy than from a recent (d,p) experiment. Within the uncertainties both results are in agreement. The nonresonant thermal and thermonuclear experimental data for this reaction can be reproduced using the direct-capture model. A possible interference with a resonant contribution is discussed. The neutron spectroscopic factors of $^{49}\mathrm{Ca}$ determined from shell-model calculations are compared with the values extracted from the experimental cross sections for $^{48}\mathrm{Ca}$(d,p${)}^{49}$Ca and $^{48}\mathrm{Ca}$(n,\ensuremath{\gamma}${)}^{49}$Ca. \textcopyright{} 1996 The American Physical Society.
- Published
- 1996
39. Searching for three-nucleon resonances
- Author
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Heinz Oberhummer, Attila Csótó, and R. Pichler
- Subjects
Physics ,Nuclear and High Energy Physics ,Nuclear Theory ,Computer Science::Information Retrieval ,FOS: Physical sciences ,Resonance ,Few-body systems ,Three-body problem ,Nuclear Theory (nucl-th) ,Nuclear physics ,Pion ,Excited state ,Physics::Accelerator Physics ,Neutron ,Atomic physics ,Nuclear Experiment ,Nucleon ,Energy (signal processing) - Abstract
We search for three-neutron resonances which were predicted from pion double charge exchange experiments on He-3. All partial waves up to J=5/2 are nonresonant except the J=3/2^+ one, where we find a state at E=14 MeV energy with 13 MeV width. The parameters of the mirror state in the three-proton system are E=15 MeV and Gamma=14 MeV. The possible existence of an excited state in the triton, which was predicted from a H(He-6,alpha) experiment, is also discussed., Comment: LaTex with RevTex
- Published
- 1996
40. 70Ge(α, γ)74Se cross section measurements at energies of astrophysical interest
- Author
-
Zs. Fülöp, Thomas Rauscher, E. Somorjai, Heinz Oberhummer, C. Rolfs, Á. Z. Kiss, and H. P. Trautvetter
- Subjects
Reaction rate ,Physics ,Nuclear and High Energy Physics ,Cross section (physics) ,Range (particle radiation) ,Inverse ,Nuclear fusion ,Gamma spectroscopy ,Atomic physics ,Nuclear Experiment ,Coincidence - Abstract
The cross section of the reaction 70Ge(α, γ)74Se has been measured over the bombarding energy range of 5.05 MeV
- Published
- 1996
41. News from NuPECC: Public Awareness of Nuclear Science: Why and How
- Author
-
Heinz Oberhummer
- Subjects
Nuclear and High Energy Physics ,Public awareness of science ,business.industry ,media_common.quotation_subject ,Special needs ,Public relations ,Democracy ,Harm ,Political science ,Taxpayer ,business ,Schism ,Skepticism ,media_common ,Public awareness - Abstract
In the last few decades, public awareness of science has become of utmost importance for the prevalence and sometimes even the survival of scientific disciplines. This is especially the case in our democratic societies where there is a special need for justification on how the taxpayer's money is spent. The general public has become more and more critical about the necessity of research, either because of the scepticism that research brings no benefit for society, or even worse that scientific discoveries can bring harm to it. There exists a schism in this respect between the ivory towers of the academic world and the general public.
- Published
- 2004
42. Cross section ofS36(n,γ)37S
- Author
-
H. Beer, H. Herndl, Yu. P. Popov, W. Balogh, Heinz Oberhummer, and P. V. Sedyshev
- Subjects
Physics ,Nuclear and High Energy Physics ,Photon ,Thermonuclear fusion ,law ,Q value ,Van de Graaff generator ,Neutron ,Irradiation ,Atomic physics ,Nuclear density ,Excitation ,law.invention - Abstract
At the Karlsruhe pulsed 3.75 MV Van de Graaff accelerator the {sup 36}S({ital n},{gamma}){sup 37}S(5.05 min) cross section was measured by the fast cyclic activation technique via the 3.103 MeV {gamma}-ray line of the {sup 37}S decay. Samples of elemental sulfur enriched in {sup 36}S by 5.933% were irradiated between two gold foils which served as capture standards. The capture cross section was measured at neutron energies 25, 151, 176, and 218 keV, respectively. The {sup 36}S({ital n},{gamma}){sup 37}S cross section in the thermonuclear and thermal energy range has been calculated using the direct-capture (DC) model combined with the folding procedure used for the determination of the potentials. The nonresonant experimental data for this reaction can be reproduced excellently using this method. The input parameters of the DC calculation (masses, {ital Q} values, nuclear density distributions, spectroscopic factors, spin-parity assignments, and excitation energies of the low-lying states of the residual nucleus) have been taken from the available experimental data.
- Published
- 1995
43. On the relativistic field theory model of the deuteron
- Author
-
A. N. Ivanov, Manfried Faber, Heinz Oberhummer, and N. I. Troitskaya
- Subjects
Physics ,Nuclear and High Energy Physics ,Field (physics) ,Nuclear Theory ,Binding energy ,Zero (complex analysis) ,Order (ring theory) ,Nuclear physics ,Loop (topology) ,Deuterium ,Quantum electrodynamics ,Nambu–Jona-Lasinio model ,Field theory (psychology) ,Nuclear Experiment - Abstract
We suggest a relativistic field theory model of the deuteron. We start from a local unphysical deuteron field, taken as a bound proton-neutron state at zero binding energy. Following the Nambu-Jona-Lasinio prescription we construct the physical deuteron field. We describe all parameters of the physical deuteron in the one-nucleon loop approximation and in leading order of the long-wavelength expansion. The one-pion exchange contribution to the binding energy calculated in the two-nucleon loop approximation is found small compared with that obtained in the one-nucleon loop one. The present model can be applied to the description of the decouplet of dibaryons 10 f where the deuteron is the component with Y = 2 and I = 0.
- Published
- 1995
44. Gedankenlesen durch Schneckenstreicheln
- Author
-
Heinz Oberhummer, Martin Puntigam, and Werner Gruber
- Published
- 2012
45. Publisher's Note: Measurement of resolved resonances of232Th(n,γ) at the n_TOF facility at CERN [Phys. Rev. C85, 064601 (2012)]
- Author
-
S. Andriamonje, A. Goverdovski, F. Alvarez-Velarde, M. C. Vincente, E. Chiaveri, K. Fujii, Gerald Badurek, P. F. Mastinu, A. Herrera-Martinez, N. Patronis, R. Dolfini, M. Mosconi, Arnaud Ferrari, Isabel Lopes, M. Embid-Segura, S. O'Brien, K. Wisshak, F. Voss, J. Salgado, A. Poch, B. Haas, S. Isaev, R. Terlizzi, G. Vannini, C. Lampoudis, G. Aerts, Manuel Lozano, C. T. Papadopoulos, A. Pavlik, C. Domingo-Pardo, N. Colonna, Vasilis Vlachoudis, F. Gramegna, E. Jericha, L. Tavora, I. Duran, M. Oshima, L. Ferrant, J. Marganiec, A. Lindote, L. Perrot, Masayuki Igashira, W. Dridi, J. Andrzejewski, H. Wendler, F. Bečvář, L. Marques, Corrie S. Moreau, C. Rubbia, P. Rullhusen, A. Plukis, L. Fitzpatrick, G. Cortes, R. Vlastou, C. Stephan, F. Gunsing, E. Berthoumieux, R. C. Haight, V. Chepel, G. Rudolf, Isabel S. Gonçalves, A. Ventura, C. Paradela, D. Villamarin, S. Marrone, M. Krtička, F. Calviño, L. Audouin, S. Lukic, V. Konovalov, Roberto Capote, P.A. Assimakopoulos, C. Pretel, P. Baumann, R. Ferreira-Marques, A. J. M. Plompen, F. Neves, D. Cano-Ott, H. Álvarez, I. Savvidis, P. M. Milazzo, J. L. Tain, Michael Wiescher, F. Käppeler, M. Dahlfors, P. Pavlopoulos, Marco T. Pigni, James L. Cox, H. Leeb, M. Kerveno, Rene Reifarth, P. Vaz, Aaron Couture, J. M. Quesada, L. Tassan-Got, A. Carrillo de Albornoz, E. Kossionides, D. Karamanis, S. Walter, Ralf Plag, Carlos Guerrero, U. Abbondanno, S. David, G. Tagliente, Heinz Oberhummer, W.I. Furman, C. A. Papachristodoulou, I. Dillman, L. Sarchiapone, Matthias Heil, J. Pancin, C. Eleftheriadis, Y. Kadi, Thomas Rauscher, H. Frais-Koelbl, D. Karadimos, P. E. Koehler, E. González-Romero, M. Rosetti, E. Griesmayer, A. Mengoni, V. Ketlerov, and P. Cennini
- Subjects
Physics ,Nuclear and High Energy Physics ,Neutron capture ,Large Hadron Collider ,Radiative capture ,Atomic physics - Published
- 2012
46. Measurement of resolved resonances of232Th(n,γ) at the n_TOF facility at CERN
- Author
-
G. Cortes, J. Marganiec, S. Andriamonje, G. Aerts, E. Chiaveri, P. F. Mastinu, D. Cano-Ott, Roberto Capote, L. Sarchiapone, M. C. Vincente, A. Ventura, P.A. Assimakopoulos, S. Lukic, Christoph A. Stephan, F. Gunsing, Marco T. Pigni, H. Álvarez, V. Ketlerov, A. J. M. Plompen, V. Chepel, E. Griesmayer, J. L. Tain, N. Colonna, G. Vannini, P. Cennini, G. Rudolf, I. Dillman, S. Isaev, Carlos Guerrero, C. Pretel, B. Haas, P. Baumann, U. Abbondanno, F. Voss, A. Plukis, James L. Cox, Heinz Oberhummer, Thomas Rauscher, M. Mosconi, L. Ferrant, C. T. Papadopoulos, Matthias Heil, J. Pancin, Vasilis Vlachoudis, D. Karadimos, S. Walter, S. O'Brien, M. Krtička, F. Calviño, I. Savvidis, Masayuki Igashira, Corrie S. Moreau, R. C. Haight, J. Salgado, W. Dridi, Ralf Plag, L. Fitzpatrick, R. Ferreira-Marques, R. Terlizzi, A. Poch, M. Embid-Segura, C. Paradela, E. González-Romero, F. Gramegna, Rene Reifarth, L. Audouin, F. Käppeler, L. Tavora, L. Perrot, D. Villamarin, A. Lindote, I. Duran, C. Rubbia, Y. Kadi, H. Frais-Koelbl, C. Lampoudis, M. Rosetti, A. Pavlik, A. Goverdovski, C. Domingo-Pardo, F. Alvarez-Velarde, J. M. Quesada, L. Tassan-Got, Michael Wiescher, W.I. Furman, P. Rullhusen, R. Vlastou, E. Kossionides, E. Berthoumieux, Manuel Lozano, Gerald Badurek, R. Dolfini, K. Fujii, Isabel S. Gonçalves, C. Eleftheriadis, P. Pavlopoulos, S. Marrone, S. David, M. Oshima, J. Andrzejewski, G. Tagliente, P. E. Koehler, M. Dahlfors, C. A. Papachristodoulou, P. Vaz, M. Kerveno, L. Marques, Aaron Couture, V. Konovalov, Isabel Lopes, A. Herrera-Martinez, N. Patronis, Arnaud Ferrari, Alberto Mengoni, K. Wisshak, H. Wendler, H. Leeb, D. Karamanis, F. Neves, P. M. Milazzo, F. Bečvář, A. Carrillo de Albornoz, and E. Jericha
- Subjects
Physics ,Nuclear and High Energy Physics ,Range (particle radiation) ,Large Hadron Collider ,010308 nuclear & particles physics ,Resonance ,01 natural sciences ,7. Clean energy ,Spectral line ,Nuclear physics ,Neutron capture ,Yield (chemistry) ,0103 physical sciences ,Neutron ,Atomic physics ,Nuclear Experiment ,010306 general physics ,Spectroscopy - Abstract
The yield of the neutron capture reaction 232Th(n,γ) has been measured at the neutron time-of-flight facility n-TOF at CERN in the energy range from 1 eV to 1 MeV. The reduction of the acquired data to the capture yield for resolved resonances from 1 eV to 4 keV is described and compared to a recent evaluated data set. The resonance parameters were used to assign an orbital momentum to each resonance. A missing level estimator was used to extract the s-wave level spacing of D0=17.2±0.9 eV. © 2012 American Physical Society.
- Published
- 2012
47. Neutron-induced fission cross section of 245Cm: New results from data taken at the time-of-flight facility n_TOF
- Author
-
G. Cortes, Gerald Badurek, P. Cennini, J. Pancin, E. Chiaveri, D. Cano-Ott, C. Eleftheriadis, B. Berthier, Michael Heil, E. Kossionides, J. Salgado, Javier Praena, C. Santos, I. Duran, M. Embid-Segura, S. Walter, Roberto Capote, Yacine Kadi, A. Poch, F. Bečvář, E. Mendoza, M. C. Vincente, J. Marganiec, S. Andriamonje, M. Dahlfors, Manuel Lozano, F. Neves, Ralf Plag, M. Mosconi, V. Ketlerov, P. Vaz, L. Ferrant, Peter Schillebeeckx, Iris Dillmann, D. Villamarin, W. Dridi, P. F. Mastinu, J. Cox, Alberto Ventura, S. Galanopoulos, Aaron Couture, Marco T. Pigni, G. Vannini, C. Lederer, C. Papadopoulos, Laurent Tassan-Got, C. Stephan, C. Lampoudis, Alfredo Ferrari, R. Ferreira-Marques, S. Marrone, A. Pavlik, C. Domingo-Pardo, L. Perrot, M. Kerveno, S. David, L. Sarchiapone, M. Meaze, G. Tagliente, M. Rosetti, R. Terlizzi, E. Gonzalez-Romero, G. Aerts, Carlos Guerrero, U. Abbondanno, F. Calviño, R. C. Haight, H. Leeb, P. E. Koehler, V. Chepel, Heinz Oberhummer, I. Goncalves, S. O'Brien, A. Plukis, P. Assimakopoulos, Mario Barbagallo, I. Savvidis, L. Tavora, Thomas Rauscher, Marco Calviani, L. Audouin, D. Karadimos, Michael Wiescher, H. Álvarez, W.I. Furman, P. Baumann, K. Wisshak, V. Variale, M. Krtička, R. Sarmento, J. L. Tain, A. J. M. Plompen, A. Herrera-Martinez, N. Patronis, P. Rullhusen, G. Rudolf, A. Lindote, T. Martinez, I. Lopes, C. A. Papachristodoulou, R. Vlastou, Alberto Mengoni, B. Haas, C. Carrapiço, Rene Reifarth, M. Igashira, P. Pavlopoulos, F. Gunsing, J. M. Quesada, Cristian Massimi, C. Paradela, S. Lukic, E. Jericha, D. Karamanis, E. Berthoumieux, F. Voss, F. Gramegna, Nicola Colonna, C. Moreau, P. M. Milazzo, J. Andrzejewski, Carlo Rubbia, V. Vlachoudis, V. Konovalov, G. Giubrone, C. Pretel, K. Fujii, Fabio Belloni, F. Käppeler, A. Goverdovski, F. Alvarez-Velarde, Universitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear, Universitat Politècnica de Catalunya. GREENER - Grup de recerca d'estudis energètics i de les radiacions, Universidad de Sevilla. Departamento de Física Atómica, Molecular y Nuclear, European Commission (EC), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Département Recherches Subatomiques (DRS-IPHC), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Aval du cycle et Energie Nucléaire (ACEN), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Pôle Universitaire Léonard de Vinci, Pôle Universitaire Léonard de Vinci (PULV), nTOF, Calviani M., Meaze M. H., Colonna N., Praena J., Abbondanno U., Aerts G., Alvarez H., Alvarez-Velarde F., Andriamonje S., Andrzejewski J., Assimakopoulos P., Audouin L., Badurek G., Barbagallo M., Baumann P., Bečvář F., Belloni F., Berthier B., Berthoumieux E., Calviño F., Cano-Ott D., Capote R., Carrapiço C., Cennini P., Chepel V., Chiaveri E., Cortes G., Couture A., Cox J., Dahlfors M., David S., Dillmann I., Domingo-Pardo C., Dridi W., Duran I., Eleftheriadis C., Embid-Segura M., Ferrant L., Ferrari A., Ferreira-Marques R., Fujii K., Furman W., Galanopoulos S., Giubrone G., Gonçalves I., Gonzalez-Romero E., Goverdovski A., Gramegna F., Guerrero C., Gunsing F., Haas B., Haight R., Heil M., Herrera-Martinez A., Igashira M., Jericha E., Käppeler F., Kadi Y., Karadimos D., Karamanis D., Ketlerov V., Kerveno M., Koehler P., Konovalov V., Kossionides E., Krtička M., Lampoudis C., Lederer C., Leeb H., Lindote A., Lopes I., Lozano M., Lukic S., Marganiec J., Marrone S., Martínez T., Massimi C., Mastinu P., Mendoza E., Mengoni A., Milazzo P. M., Moreau C., Mosconi M., Neves F., Oberhummer H., O’Brien S., Pancin J., Papachristodoulou C., Papadopoulos C., Paradela C., Patronis N., Pavlik A., Pavlopoulos P., Perrot L., Pigni M. T., Plag R., Plompen A., Plukis A., Poch A., Pretel C., Quesada J., Rauscher T., Reifarth R., Rosetti M., Rubbia C., Rudolf G., Rullhusen P., Salgado J., Santos C., Sarchiapone L., Sarmento R., Savvidis I., Schillebeeckx P., Stephan C., Tagliente G., Tain J. L., Tassan-Got L., Tavora L., Terlizzi R., Vannini G., Variale V., Vaz P., Ventura A., Villamarin D., Vincente M. C., Vlachoudis V., Vlastou R., Voss F., Walter S., Wiescher M., Wisshak K., Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Energies::Energia nuclear [Àrees temàtiques de la UPC] ,Nuclear and High Energy Physics ,Range (particle radiation) ,Isotope ,010308 nuclear & particles physics ,Fission ,Nuclear Theory ,Absolute value ,Energies::Energia nuclear::Reactors nuclears de fissió [Àrees temàtiques de la UPC] ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,7. Clean energy ,01 natural sciences ,Neutron temperature ,NEUTRON INDUCED FISSION ,Fissió nuclear ,Nuclear physics ,Time of flight ,Cross section (physics) ,0103 physical sciences ,Fission cross sections ,Neutron ,010306 general physics ,Nuclear Experiment ,TIME OF FLIGHT - Abstract
The neutron-induced fission cross section of 245Cm was measured at n-TOF in a wide energy range and with high resolution. The energy dependence, measured in a single measurement from 30 meV to 1 MeV neutron energy, has been determined with 5% accuracy relative to the 235U(n,f) cross section. In order to reduce the uncertainty on the absolute value, the data have been normalized at thermal energy to recent measurements performed at ILL and BR1. In the energy range of overlap, the results are in fair agreement with some previous measurements and confirm, on average, the evaluated cross section in the ENDF/B-VII.0 database, although sizable differences are observed for some important resonances below 20 eV. A similar behavior is observed relative to JENDL/AC-2008, a reactor-oriented database for actinides. The new results contribute to the overall improvement of the databases needed for the design of advanced reactor systems and may lead to refinements of fission models for the actinides. Comisión Europea FIKW-CT-2000-00107 249671
- Published
- 2012
48. Measurement and resonance analysis of the 237Np neutron capture cross section
- Author
-
M. Embid-Segura, Manuel Lozano, L. Perrot, R. Lossito, V. Chepel, Ralf Plag, Rene Reifarth, P. Baumann, I. Duran, P. Cennini, E. Kossionides, W.I. Furman, M. Mosconi, G. Aerts, A. Lindote, C. Stephan, C. A. Papachristodoulou, Javier Praena, P. Pavlopoulos, S. O'Brien, J. M. Quesada, A. Herrera-Martinez, N. Patronis, R. Terlizzi, F. Voss, F. Becvar, C. Eleftheriadis, M. C. Vicente, Alberto Mengoni, A. J. M. Plompen, P. M. Milazzo, A. Carrillo de Albornoz, G. Rudolf, L. Ferrant, M. Igashira, I. Lopes, Yacine Kadi, Nicola Colonna, D. Villamarin, P. E. Koehler, L. Fitzpatrick, J. Salgado, Marco T. Pigni, A. Poch, M. Oshima, J. L. Tain, J. Andrzejewski, Carlos Guerrero, Carlo Rubbia, Alfredo Ferrari, R. Ferreira-Marques, S. Isaev, Heinz Oberhummer, V. Vlachoudis, U. Abbondanno, L. Tavora, V. Konovalov, E. Griesmayer, J. Cox, Laurent Tassan-Got, S. David, G. Cortes, P. Rullhusen, G. Tagliente, C. Massimi, E. Jericha, R. C. Haight, Roberto Capote, V. Ketlerov, C. Carrapiço, P.A. Assimakopoulos, M. Kerveno, F. Neves, L. Audouin, F. Käppeler, G. Vannini, E. Gonzalez-Romero, Michael Wiescher, I. Goncalves, Thomas Rauscher, D. Karamanis, I. Dillmann, C. Moreau, D. Karadimos, Michael Heil, S. Walter, C. T. Papadopoulos, F. Gramegna, A. Plukis, A. Goverdovski, C. Santos, F. Alvarez-Velarde, Gerald Badurek, W. Dridi, R. Dolfini, M. Rosetti, S. Marrone, E. Mendoza, B. Haas, J. Marganiec, S. Andriamonje, R. Vlastou, P. F. Mastinu, E. Berthoumieux, I. Savvidis, M. Calviani, H. Frais-Koelbl, C. Paradela, S. Lukic, L. Marques, M. Krtička, C. Pretel, T. Martinez, K. Fujii, Fabio Belloni, F. Calviño, H. Leeb, L. Sarchiapone, M. Dahlfors, P. Vaz, Alberto Ventura, Aaron Couture, C. Lampoudis, A. Pavlik, C. Domingo-Pardo, F. Gunsing, J. Pancin, E. Chiaveri, D. Cano-Ott, K. Wisshak, H. Wendler, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Département Recherches Subatomiques (DRS-IPHC), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Aval du cycle et Energie Nucléaire (ACEN), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Pôle Universitaire Léonard de Vinci, Pôle Universitaire Léonard de Vinci (PULV), TOF, Universidad de Sevilla. Departamento de Física Atómica, Molecular y Nuclear, European Union (UE), Ministerio de Educación y Ciencia (MEC). España, Guerrero C., Cano-Ott D., Mendoza E., Abbondanno U., Aerts G., Alvarez-Velarde F., Andriamonje S., Andrzejewski J., Assimakopoulos P., Audouin L., Badurek G., Baumann P., Becvar F., Belloni F., Berthoumieux E., Calvino F., Calviani M., Capote R., Carrapico C., Carrillo de Albornoz A., Cennini P., Chepel V., Chiaveri E., Colonna N., Cortes G., Couture A., Cox J., Dahlfors M., David S., Dillmann I., Dolfini R., Domingo-Pardo C., Dridi W., Duran I., Eleftheriadis C., Embid-Segura M., Ferrant L., Ferrari A., Ferreira-Marques R., Fitzpatrick L., Frais-Koelbl H., Fujii K., Furman W., Goncalves I., Gonzalez-Romero E., Goverdovski A., Gramegna F., Griesmayer E., Gunsing F., Haas B., Haight R., Heil M., Herrera-Martinez A., Igashira M., Isaev S., Jericha E., Kaeppeler F., Kadi Y., Karadimos D., Karamanis D., Ketlerov V., Kerveno M., Koehler P., Konovalov V., Kossionides E., Krticka M., Lampoudis C., Leeb H., Lindote A., Lopes I., Lossito R., Lozano M., Lukic S., Marganiec J., Marques L., Marrone S., Martinez T., Massimi C., Mastinu P., Mengoni A., Milazzo P. M., Moreau C., Mosconi M., Neves F., Oberhummer H., O'Brien S., Oshima M., Pancin J., Papachristodoulou C., Papadopoulos C., Paradela C., Patronis N., Pavlik A., Pavlopoulos P., Perrot L., Pigni M. T., Plag R., Plompen A., Plukis A., Poch A., Praena J., Pretel C., Quesada J., Rauscher T., Reifarth R., Rosetti M., Rubbia C., Rudolf G., Rullhusen P., Salgado J., Santos C., Sarchiapone L., Savvidis I., Stephan C., Tagliente G., Tain J. L., Tassan-Got L., Tavora L., Terlizzi R., Vannini G., Vaz P., Ventura A., Villamarin D., Vicente M. C., Vlachoudis V., Vlastou R., Voss F., Walter S., Wendler H., Wiescher M., Wisshak K., Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,Nuclear and High Energy Physics ,Large Hadron Collider ,010308 nuclear & particles physics ,CAPTURE CROSS-SECTION ,Detector ,Nuclear data ,BARIUM-FLORIDE CALORIMETER ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,7. Clean energy ,01 natural sciences ,Resonance (particle physics) ,Calorimeter ,Nuclear physics ,Cross section (physics) ,0103 physical sciences ,Range (statistics) ,Neutron cross section ,Nuclear Physics - Experiment ,GAMMA SPECTROSCOPY ,010306 general physics ,EMERGING NUCLEAR TECHNOLOGIES - Abstract
The neutron capture cross section of 237Np was measured between 0.7 and 500 eV at the CERN n-TOF facility using the 4π BaF2 Total Absorption Calorimeter. The experimental capture yield was extracted minimizing all the systematic uncertainties and was analyzed together with the most reliable transmission data available using the sammy code. The result is a complete set of individual as well as average resonance parameters [D0=0.56(2) eV, Γγ=40.9(18) meV, 104S0=0.98(6), R ′=9.8(6) fm]. The capture cross section obtained in this work is in overall agreement with the evaluations and the data of Weston and Todd, thus showing sizable differences with respect to previous data from Scherbakov and large discrepancies with data Kobayashi. The results indicate that a new evaluation combining the present capture data with reliable transmission data would allow reaching an accuracy better than 4%, in line with the uncertainty requirements of the nuclear data community for the design and operation of current and future nuclear devices. Unión Europea NTOF-NDXADS IP-EUROTRANS CIEMAT-ENRESA Plan Nacional de Física de Partículas (España) FPA2005-06918-C03-01 Programa Consolider-Ingenio 2010 (España)
- Published
- 2012
49. Neutron-induced fission cross section measurement of233U,241Am and243Am in the energy range 0.5 MeV ⩽En⩽ 20 MeV at n_TOF at CERN
- Author
-
G. Cortes, J. Pancin, C. Lederer, R. Vlastou, H. Leeb, S. David, L. Perrot, P. Cennini, F. Calvino, Anton Wallner, Corrie S. Moreau, V. Chepel, Roberto Capote, P. Baumann, Y. Kadi, G. Tagliente, P.A. Assimakopoulos, M. Kerveno, C. Eleftheriadis, A. Goverdovski, F. Alvarez-Velarde, H. Frais-Koelbl, Thomas Rauscher, M. Dahlfors, F. Gunsing, Gerald Badurek, R. Dolfini, G. Aerts, M. Mosconi, P. Vaz, G. Vannini, J. Marganiec, S. Andriamonje, Marco Calviani, Cristian Massimi, P. Pavlopoulos, Aaron Couture, J. Salgado, A. J. M. Plompen, F. Belloni, C. Stephan, S. O'Brien, Mario Barbagallo, Carlos Guerrero, A. Poch, Marco T. Pigni, D. Karadimos, I. Dillmann, G. Rudolf, F. Cerutti, D. Cano-Ott, C. Pretel, E. Chiaveri, E. Jericha, L. Marques, I. Lopes, Michael Heil, A. Pavlik, Heinz Oberhummer, C. Santos, P. F. Mastinu, R. Terlizzi, S. Walter, C. Domingo-Pardo, L. Ferrant, K. Wisshak, A. Lindote, James L. Cox, E. González-Romero, L. Fitzpatrick, L. Tavora, K. Fujii, R. C. Haight, Masayuki Igashira, C. Paradela, H. Wendler, L. Audouin, M. Embid-Segura, D. Villamarin, P. E. Koehler, P. Rullhusen, V. Ketlerov, Michael Wiescher, L. Sarchiapone, ntof, F. Bečvář, M. Meaze, Manuel Lozano, Ralf Plag, H. Álvarez, M. Oshima, M. Krtička, J. L. Tain, C Lampoudis, J. Andrzejewski, M. Rosetti, F. Voss, W.I. Furman, C. T. Papadopoulos, E. Kossionides, R. Ferreira-Marques, T. Martinez, I. Duran, C. A. Papachristodoulou, F. Neves, P. M. Milazzo, C. Rubbia, V. Konovalov, Javier Praena, Isabel S. Gonçalves, A. Plukis, S. Marrone, A. Carrillo de Albornoz, F. Käppeler, E. Griesmayer, S. Lukic, Nicola Colonna, A. Herrera-Martinez, N. Patronis, Arnaud Ferrari, Vasilis Vlachoudis, Alberto Mengoni, A. Ventura, F. Gramegna, I. Savvidis, B. Haas, M. C. Vincente, W. Dridi, Rene Reifarth, J. M. Quesada, L. Tassan-Got, S. Isaev, U. Abbondanno, E. Berthoumieux, C. Carrapiço, D. Karamanis, F Belloni, P M Milazzo, M Calviani, N Colonna, P Mastinu, U Abbondanno, G Aert, H Álvarez, F Álvarez-Velarde, S Andriamonje, J Andrzejewski, P Assimakopoulo, L Audouin, G Badurek, M Barbagallo, P Baumann, F Bečvář, E Berthoumieux, F Calviño, F Cerutti, D Cano-Ott, R Capote, C Carrapiço, A Carrillo de Albornoz, P Cennini, V Chepel, E Chiaveri, G Corte, A Couture, J Cox, M Dahlfor, S David, I Dillmann, R Dolfini, C Domingo-Pardo, W Dridi, I Duran, C Eleftheriadi, M Embid-Segura, L Ferrant, A Ferrari, R Ferreira-Marque, L Fitzpatrick, H Frais-Koelbl, K Fujii, W Furman, I Goncalve, E González-Romero, A Goverdovski, F Gramegna, E Griesmayer, C Guerrero, F Gunsing, B Haa, R Haight, M Heil, A Herrera-Martinez, M Igashira, S Isaev, E Jericha, F Käppeler, Y Kadi, D Karadimo, D Karamani, V Ketlerov, M Kerveno, P Koehler, V Konovalov, E Kossionide, M Krtička, C Lampoudi, C Lederer, H Leeb, A Lindote, I Lope, M Lozano, S Lukic, J Marganiec, L Marque, S Marrone, T Martínez, C Massimi, M H Meaze, A Mengoni, C Moreau, M Mosconi, F Neve, H Oberhummer, S O'Brien, M Oshima, J Pancin, C Papachristodoulou, C Papadopoulo, C Paradela, N Patroni, A Pavlik, P Pavlopoulo, L Perrot, M T Pigni, R Plag, A Plompen, A Pluki, A Poch, J Praena, C Pretel, J Quesada, T Rauscher, R Reifarth, M Rosetti, C Rubbia, G Rudolf, P Rullhusen, J Salgado, C Santo, L Sarchiapone, I Savvidi, C Stephan, G Tagliente, J L Tain, L Tassan-Got, L Tavora, R Terlizzi, G Vannini, P Vaz, A Ventura, D Villamarin, M C Vincente, V Vlachoudi, R Vlastou, F Vo, A Wallner, S Walter, H Wendler, M Wiescher, and K Wisshak
- Subjects
Fission ,Physics::Instrumentation and Detectors ,Astrophysics::High Energy Astrophysical Phenomena ,Nuclear Theory ,01 natural sciences ,7. Clean energy ,Nuclear physics ,Cross section (physics) ,0103 physical sciences ,Neutron cross section ,Neutron ,010306 general physics ,Nuclear Experiment ,Mathematical Physics ,EMERGING NUCLEAR TECHNOLOGIES ,Physics ,Large Hadron Collider ,010308 nuclear & particles physics ,Neutron radiation ,Condensed Matter Physics ,Atomic and Molecular Physics, and Optics ,NEUTRON INDUCED FISSION ,Time of flight ,TIME-OF-FLIGHT ,Ionization chamber ,Physics::Accelerator Physics ,Atomic physics - Abstract
Neutron-induced fission cross section measurements of U-233, Am-243 and Am-241 relative to U-235 have been carried out at the neutron time-of-flight facility n_TOF at CERN. A fast ionization chamber has been employed. All samples were located in the same detector; therefore the studied elements and the reference U-235 target are subject to the same neutron beam.
- Published
- 2012
50. Direct capture in the3+resonance ofH2(α,γ)6Li
- Author
-
V. Kölle, H. Krauss, J. W. Hammer, S. Wilmes, G. Staudt, Heinz Oberhummer, U. Atzrott, and P. Mohr
- Subjects
Physics ,Nuclear reaction ,Nuclear and High Energy Physics ,Light nucleus ,Range (particle radiation) ,Particle properties ,Isotopes of lithium ,Analytical chemistry ,Resonance ,Spin (physics) - Abstract
The cross section for the capture reaction[sup 2]H([alpha],[gamma])[sup 6]Li was measured in the energy range of about [ital E][sub [alpha],lab][approx]2 MeV corresponding to the 3[sup +] resonance in [sup 6]Li at [ital E][sub [ital x]]=2186 keV. Calculations in a direct-capture model using double-folded [alpha]-[ital d] potentials reproduce strength and width of this resonance as well as the nonresonant capture cross section at lower and higher energies.
- Published
- 1994
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