Industrial Applications of Photonuclear Resonance Excitation
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The R-Process Nucleosynthesis and Related Challenges
EPJ Web of Conferences 165, 01025 (2017) DOI: 10.1051/epjconf/201716501025 NPA8 2017 The r-process nucleosynthesis and related challenges Stephane Goriely1,, Andreas Bauswein2, Hans-Thomas Janka3, Oliver Just4, and Else Pllumbi3 1Institut d’Astronomie et d’Astrophysique, Université Libre de Bruxelles, CP 226, 1050 Brussels, Belgium 2Heidelberger Institut fr¨ Theoretische Studien, Schloss-Wolfsbrunnenweg 35, 69118 Heidelberg, Germany 3Max-Planck-Institut für Astrophysik, Postfach 1317, 85741 Garching, Germany 4Astrophysical Big Bang Laboratory, RIKEN, 2-1 Hirosawa, Wako, Saitama, 351-0198, Japan Abstract. The rapid neutron-capture process, or r-process, is known to be of fundamental importance for explaining the origin of approximately half of the A > 60 stable nuclei observed in nature. Recently, special attention has been paid to neutron star (NS) mergers following the confirmation by hydrodynamic simulations that a non-negligible amount of matter can be ejected and by nucleosynthesis calculations combined with the predicted astrophysical event rate that such a site can account for the majority of r-material in our Galaxy. We show here that the combined contribution of both the dynamical (prompt) ejecta expelled during binary NS or NS-black hole (BH) mergers and the neutrino and viscously driven outflows generated during the post-merger remnant evolution of relic BH-torus systems can lead to the production of r-process elements from mass number A > 90 up to actinides. The corresponding abundance distribution is found to reproduce the∼ solar distribution extremely well. It can also account for the elemental distributions observed in low-metallicity stars. However, major uncertainties still affect our under- standing of the composition of the ejected matter. -
Photofission Cross Sections of 238U and 235U from 5.0 Mev to 8.0 Mev Robert Andrew Anderl Iowa State University
Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 1972 Photofission cross sections of 238U and 235U from 5.0 MeV to 8.0 MeV Robert Andrew Anderl Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Part of the Nuclear Commons, and the Oil, Gas, and Energy Commons Recommended Citation Anderl, Robert Andrew, "Photofission cross sections of 238U and 235U from 5.0 MeV to 8.0 MeV " (1972). Retrospective Theses and Dissertations. 4715. https://lib.dr.iastate.edu/rtd/4715 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. INFORMATION TO USERS This dissertation was produced from a microfilm copy of the original document. While the most advanced technological means to photograph and reproduce this document have been used, the quality is heavily dependent upon the quality of the original submitted. The following explanation of techniques is provided to help you understand markings or patterns which may appear on this reproduction, 1. The sign or "target" for pages apparently lacking from the document photographed is "Missing Page(s)". If it was possible to obtain the missing page(s) or section, they are spliced into the film along with adjacent pages. This may have necessitated cutting thru an image and duplicating adjacent pages to insure you complete continuity, 2. -
Separation of Nuclear Isomers for Cancer Therapeutic Radionuclides
www.nature.com/scientificreports OPEN Separation of nuclear isomers for cancer therapeutic radionuclides based on nuclear decay after- Received: 03 November 2016 Accepted: 06 February 2017 effects Published: 13 March 2017 R. Bhardwaj1,2, A. van der Meer1, S. K. Das1, M. de Bruin1, J. Gascon2, H. T. Wolterbeek1, A. G. Denkova1 & P. Serra-Crespo1 177Lu has sprung as a promising radionuclide for targeted therapy. The low soft tissue penetration of its β− emission results in very efficient energy deposition in small-size tumours. Because of this, 177Lu is used in the treatment of neuroendocrine tumours and is also clinically approved for prostate cancer therapy. In this work, we report a separation method that achieves the challenging separation of the physically and chemically identical nuclear isomers, 177mLu and 177Lu. The separation method combines the nuclear after-effects of the nuclear decay, the use of a very stable chemical complex and a chromatographic separation. Based on this separation concept, a new type of radionuclide generator has been devised, in which the parent and the daughter radionuclides are the same elements. The 177mLu/177Lu radionuclide generator provides a new production route for the therapeutic radionuclide 177Lu and can bring significant growth in the research and development of177 Lu based pharmaceuticals. Lutetium-177 (177Lu) has emerged as a promising radionuclide for targeted therapy. The low energy β− emissions, a half-life of 6.64 days and the emission of low energy and low abundance γ-rays has made 177Lu a solid candidate to be the most applied therapeutic radionuclide by 20201. Its low energy β − particles with a tissue penetration of less than 3 mm make it suitable for targeting small primary and metastatic tumours, like prostate, breast, mela- noma, lung and pancreatic tumours, for bone palliation therapy and other chronic diseases2–4. -
Neutron Drip Line Nuclei HUGE D I F F U S E D PA IR ED
Neutron Drip line nuclei HUGE D i f f u s e d PA IR ED 4He 5He 6He 7He 8He 9He 10He Pairing and binding The Grand Nuclear Landscape (finite nuclei + extended nucleonic matter) superheavy Z=118, A=294 nuclei known up to Z=91 82 126 terra incognita known nuclei protons proton drip line 50 82 neutron stars 28 20 50 stable nuclei neutron drip line 8 28 2 20 probably known only up to oxygen 2 8 neutrons Binding Blocks http://www.york.ac.uk/physics/public-and-schools/schools/secondary/binding-blocks/ http://www.york.ac.uk/physics/public-and-schools/schools/secondary/binding- blocks/interactive/ https://arxiv.org/abs/1610.02296 http://www.nishina.riken.jp/enjoy/kakuzu/kakuzu_web.pdf The limits: Skyrme-DFT Benchmark 2012 120 stable nuclei 288 known nuclei ~3,000 drip line two-proton drip line N=258 80 S2n = 2 MeV Z=82 SV-min two-neutron drip line N=184 Asymptotic freedom ? 110 Z=50 40 N=126 100 proton number Z=28 N=82 proton number Z=20 90 230 244 N=50 232 240 248 256 N=28 Nuclear Landscape 2012 neutron number 0 N=20 0 40 80 120 160 200 240 280 fromneutron B. Sherrill number How many protons and neutrons can be bound in a nucleus? Literature: 5,000-12,000 Erler et al. Skyrme-DFT: 6,900±500 Nature 486, 509 (2012) syst HW: a) Using http://www.nndc.bnl.gov/chart/ find one- and two-nucleon separation energies of 6He, 7He, 8He, 141Ho, and 132Sn. -
Radioactive Decay & Decay Modes
CHAPTER 1 Radioactive Decay & Decay Modes Decay Series The terms ‘radioactive transmutation” and radioactive decay” are synonymous. Many radionuclides were found after the discovery of radioactivity in 1896. Their atomic mass and mass numbers were determined later, after the concept of isotopes had been established. The great variety of radionuclides present in thorium are listed in Table 1. Whereas thorium has only one isotope with a very long half-life (Th-232, uranium has two (U-238 and U-235), giving rise to one decay series for Th and two for U. To distin- guish the two decay series of U, they were named after long lived members: the uranium-radium series and the actinium series. The uranium-radium series includes the most important radium isotope (Ra-226) and the actinium series the most important actinium isotope (Ac-227). In all decay series, only α and β− decay are observed. With emission of an α particle (He- 4) the mass number decreases by 4 units, and the atomic number by 2 units (A’ = A - 4; Z’ = Z - 2). With emission β− particle the mass number does not change, but the atomic number increases by 1 unit (A’ = A; Z’ = Z + 1). By application of the displacement laws it can easily be deduced that all members of a certain decay series may differ from each other in their mass numbers only by multiples of 4 units. The mass number of Th-232 is 323, which can be written 4n (n=58). By variation of n, all possible mass numbers of the members of decay Engineering Aspects of Food Irradiation 1 Radioactive Decay series of Th-232 (thorium family) are obtained. -
Photofission Cross Sections of 232Th and 236U from Threshold to 8
Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 1972 Photofission cross sections of 232Th nda 236U from threshold to 8 MeV Michael Vincent Yester Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Part of the Nuclear Commons Recommended Citation Yester, Michael Vincent, "Photofission cross sections of 232Th nda 236U from threshold to 8 MeV " (1972). Retrospective Theses and Dissertations. 6137. https://lib.dr.iastate.edu/rtd/6137 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. INFORMATION TO USERS This dissertation was produced from a microfilm copy of the original document. While the most advanced technological means to photograph and reproduce this document have been used, the quality is heavily dependent upon the quality of the original submitted. The following explanation of techniques is provided to help you understand markings or patterns which may appear on this reproduction. 1. The sign or "target" for pages apparently lacking from the document photographed is "Missing Page(s)". If it was possible to obtain the missing page(s) or section, they are spliced into the film along with adjacent pages. This may have necessitated cutting thru an image and duplicating adjacent pages to insure you complete continuity. 2. When an image on the film is obliterated with a large round black mark, it is an indication that the photographer suspected that the copy may have moved during exposure and thus cause a blurred image. -
Quantum Optics with Gamma Radiation
FEATURES gamma rays of 14.4 keY emitted by the excited 57mFe state (r= 141 ns,I=312), the coherencelength is about 40 m. Forthe 6.2 Quantum optics with keV gammaradiationfrom 181~a ,having alifetime of8.73 flS, the coherence length is 4 km. The appreciable coherence length of these gamma photons allows us to observe the interference gamma radiation between the transition amplitudes from two paths ofthe single , photon, passing through two different samples. In one path the Romain Coussement'·2, Rustem Shahkmoumtov ,3, Gerda Neyens' photon interacts withnuclei ofa reference sample and inthe other and Jos Odeurs1 path it interacts with the nuclei ofa sample under investigation. lInstituut voor Kern- en Stmlingsfysica, Katholieke Universiteit The distance betweenthe samples canbeas large as the coherence Leuven, Celestijnenlaan 200 D, B-3001 Leuven, Belgium length ofthe photon. Interference ofthese two transition ampli 2Optique Nonlineaire Theorique, Universite Libre de Bruxelles, tudes provides spectroscopic CP 231, Bid du Triomphe, B-lOS0 Bruxelles, Belgium information about the hyper- 3Kazan Physico- Technical Institute ofRussian Academy of fine interaction ofthe nuclei in Sciences, 10/7 Sibirsky tmkt, Kazan 420029, Russia the investigated sample, pro vided the hyperfine spectrum Since the discovery of the nuclei in the reference AN one slow down a gamma photon to a group velocity ofa sample is known. Suchinterfer of optical lasers, the Cfew m/s, or can one stop it in a piece ofmaterial only a few ence phenomena have been micron thick and release it? Can one, on command, induce trans explored using synchrotron scientific community parency ofa nuclear resonant absorber for gamma radiation and radiation [5) and are nowadays make a gate? Can one change the index ofrefraction for gamma used as a tool for solid state has been challenged rays in such a way that one could think of optical devices for physics studies. -
The R-Process Nucleosynthesis During the Decompression of Neutron Star Crust Material
Journal of Physics: Conference Series PAPER • OPEN ACCESS Related content - The Impact of Fission on R-Process The r-process nucleosynthesis during the Calculations M Eichler, A Arcones, R Käppeli et al. decompression of neutron star crust material - Variances in r-process predictions from uncertain nuclear rates Matthew Mumpower, Rebecca Surman To cite this article: S Goriely et al 2016 J. Phys.: Conf. Ser. 665 012052 and Ani Aprahamian - Discovery of a strongly r-process enhanced extremely metal-poor star LAMOST J110901.22plus075441.8 Hai-Ning Li, Wako Aoki, Satoshi Honda et View the article online for updates and enhancements. al. This content was downloaded from IP address 188.184.3.52 on 18/01/2018 at 15:57 Nuclear Physics in Astrophysics VI (NPA6) IOP Publishing Journal of Physics: Conference Series 665 (2016) 012052 doi:10.1088/1742-6596/665/1/012052 The r-process nucleosynthesis during the decompression of neutron star crust material S Goriely1,ABauswein2,H-TJanka2, S Panebianco3, J-L Sida3,J-F Lemaˆıtre3, S Hilaire4, N Dubray4 1 Institut d’Astronomie et d’Astrophysique, ULB, CP226, 1050 Bruxelles, Belgium 2 Max-Planck-Institut f¨urAstrophysik, Postfach 1317, 85741 Garching, Germany 3 CEA Saclay, Irfu/Service de Physique Nuclaire, 91191 Gif-sur-Yvette, France 4 CEA, DAM, DIF, F-91297 Arpajon, France E-mail: [email protected] Abstract. About half of the nuclei heavier than iron observed in nature are produced by the so-called rapid neutron capture process, or r-process, of nucleosynthesis. The identification of the astrophysics site and the specific conditions in which the r-process takes place remains, however, one of the still-unsolved mysteries of modern astrophysics. -
Towards a Nuclear Clock with the 229Th Isomeric Transition
Dissertation SUBMITTED TO THE Combined Faculties of the Natural Sciences and Mathematics of the Ruperto-Carola-University of Heidelberg, Germany FOR THE DEGREE OF Doctor of Natural Sciences Put forward by Pavlo V. Bilous Born in: Kherson, Ukraine Oral examination: 13.12.2018 Towards a nuclear clock with the 229Th isomeric transition The first referee: PD Dr. Adriana Pálffy-Buß The second referee: Prof. Dr. Klaus Blaum Zusammenfassung Der Kern 229Th mit seinem Isomerzustand bei 7.8 eV ist ein einzigartiger Kandidat für die erste nukleare optische Uhr mit außerordentlicher Genauigkeit von 10−19. Auf- grund der niedrigen Isomerübergangsenergie ist die Kopplung an die atomare Hülle bei den Prozessen der inneren Konversion (IK) oder Elektronenbrücke (EB) sehr stark. In dieser Arbeit untersuchen wir theoretisch die IK- und EB-Mechanismen und entwerfen neuartige lasergestützte Systeme, die auf (i) eine genauere Bestimmung der Isomerenen- ergie Em und (ii) effiziente Anregung des Isomers abzielen. Einerseits zeigen wir, wie die IK von angeregten elektronischen Zuständen von Th-Ionen zur Bestimmung der Iso- merübergangsenergie verwendet werden kann. Wir schlagen auch einen neuen Ansatz zur Messung der Isomerenergie mit Laserspektroskopie-Genauigkeit mit der laserinduzierten EB in 229Th3+ Ionen vor. Andererseits stellen wir mögliche Isomeranregungsschemata vor, die auf dem EB-Prozess in hochgeladenen Th-Ionen oder auf lasergestützter Ker- nanregung durch Elektroneneinfang des 29.19 keV-Kernzustands direkt über dem Isomer beruhen. Durch die Anwendung von hochgeladenen Ionen wird möglich, die EB optisch mit Hochleistungslasern zu treiben, was laut unserer Ergebnisse zu einer effizienten An- regung führen sollte. Ein solcher Aufbau mit Ionenfallen könnte für die zukünftige Entwicklung der Atomkernuhr relevant werden. -
Effect of Gamma-Strength on Nuclear Reaction Calculations
Effect of gamma-strength on nuclear reaction calculations Igor Kadenko1, Vladimir Plujko1,*, Borys Bondar1, Oleksandr Gorbachenko1, Borys Leshchenko2, Kateryna Solodovnyk1, Oleksandr Tkach1, and Viktor Zheltonozhskyi3. 1Nuclear Physics Department, Taras Shevchenko National University, Kyiv, Ukraine 2National Technical University of Ukraine “Kyiv Polytechnic Institute”, Kyiv, Ukraine 3Nuclear Structure Department, Institute for Nuclear Research of NAS, Kyiv, Ukraine Abstract. The results of the study of gamma-transition description in fast neutron capture and photofission are presented. Recent experimental data were used, namely, the spectrum of prompt gamma-rays in the energy range 2÷18 MeV from 14-MeV neutron capture in natural Ni and isomeric ratios in primary fragments of photofission of the isotopes of U, Np and Pu by bremsstrahlung with end-point energies Ee= 10.5, 12 and 18 MeV. The data are compared with the theoretical calculations performed within EMPIRE 3.2 and TALYS 1.6 codes. The mean value of angular momenta and their distributions were determined in the primary fragments 84Br, 97Nb, 90Rb, 131,133Te, 132Sb, 132,134I, 135Xe of photofissions. An impact of the characteristics of nuclear excited states on the calculation results is studied using different models for photon strength function and nuclear level density. determination of mean angular momenta in primary fragments is analyzed. 1 Introduction Nuclear reactions with different projectiles provide an 2 Experimental data information on properties of the excited nuclear states and nuclear reaction mechanisms. They are also Figure 1 demonstrates comparison of our recent required to different applications. Specifically, data of experimental data [4] for γ-spectrum from (n,x γ ) (n,x γ ) reactions with any outgoing particle (x) and reactions on natNi with the earlier data from EXFOR gamma-rays for atomic nuclei of the reactor materials database [5-8]. -
Photonuclear Reactions of Actinide and Pre-Actinide Nuclei at Intermediate Energies
Photonuclear reactions of actinide and pre-actinide nuclei at intermediate energies Tapan Mukhopadhyay1 and D.N. Basu2 Variable Energy Cyclotron Centre, 1/AF Bidhan Nagar, Kolkata 700 064, India ∗ (Dated: August 9, 2021) Photonuclear reaction is described with an approach based on the quasideuteron nuclear pho- toabsorption model followed by the process of competition between light particle evaporation and fission for the excited nucleus. Thus fission process is considered as a decay mode. The evaporation- fission process of the compound nucleus is simulated in a Monte-Carlo framework. Photofission reaction cross sections are analysed in a systematic manner in the energy range ∼ 50-70 MeV for the actinides 232Th, 233U, 235U, 238U and 237Np and the pre-actinide nuclei 208Pb and 209Bi. The study reproduces satisfactorily well the available experimental data of photofission cross sections at energies ∼ 50-70 MeV and the increasing trend of nuclear fissility with the fissility parameter Z2/A for the actinides and pre-actinides at intermediate energies [∼ 20-140 MeV]. Keywords: Photonuclear reactions; Photofission; Nuclear fissility; Monte-Carlo PACS numbers: 25.20.-x, 27.90.+b, 25.85.Jg, 25.20.Dc, 24.10.Lx I. INTRODUCTION Isotopes of plutonium and other actinides tend to be long-lived with half-lives of many thousands of years, whereas radioactive fission products tend to be shorter- In recent years the study of photofission has attracted lived (most with half-lives of 30 years or less). Many of considerable interest. When a gamma (photon) above the actinides are very radiotoxic because they also have the nuclear binding energy of an element is incident on long biological half-lives and are α emitters as well. -
Photofission Analysis for Fissile Dosimeters Dedicated to Reactor
EPJ Web of Conferences 106, 02007 (2016) DOI: 10.1051/epjconf/201610602007 C Owned by the authors, published by EDP Sciences, 2016 Photofission Analysis for Fissile Dosimeters Dedicated to Reactor Pressure Vessel Surveillance Stéphane Bourganel1,a , Margaux Faucher2, and Nicolas Thiollay3 1 CEA Saclay, DEN/DANS/DM2S/SERMA/LPEC, 91191 Gif-sur-Yvette Cedex, France 2 PHELMA, 3 Parvis Louis Néel - CS 50257, 38016 Grenoble Cedex 1, France 3 CEA Cadarache, DEN/DER/SPEx/LDCI, 13108 Saint Paul Lez Durance Cedex, France Abstract. Fissile dosimeters are commonly used in reactor pressure vessel surveillance programs. In this paper, the photofission contribution is analyzed for in-vessel 237Np and 238U fissile dosimeters in French PWR. The aim is to reassess this contribution using recent tools (the TRIPOLI-4 Monte Carlo code) and latest nuclear data (JEFF3.1.1 and ENDF/B- VII nuclear libraries). To be as exhaustive as possible, this study is carried out for different configurations of fissile dosimeters, irradiated inside different kinds of PWR: 900 MWe, 1300 MWe, and 1450 MWe. Calculation of photofission rate in dosimeters does not present a major problem using the TRIPOLI-4® Monte Carlo code and the coupled neutron-photon simulation mode. However, preliminary studies were necessary to identify the origin of photons responsible of photofissions in dosimeters in relation to the photofission threshold reaction (around 5 MeV). It appears that the main contribution of high enough energy photons generating photofissions is the neutron inelastic scattering in stainless steel reactor structures. By contrast, 137Cs activity calculation is not an easy task since photofission yield data are known with high uncertainty.