Collective Structure of Neutron-Rich Rare-Earth Nuclei And
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Systematical Study of Optical Potential Strengths in Reactions Involving Strongly, Weakly Bound and Exotic Nuclei on 120Sn
Systematical study of optical potential strengths in reactions involving strongly, weakly bound and exotic nuclei on 120Sn M. A. G. Alvarez, J. P. Fern´andez-Garc´ıa, J. L. Le´on-Garc´ıa Departamento FAMN, Universidad de Sevilla, Apartado 1065, 41080 Sevilla, Spain M. Rodr´ıguez-Gallardo Departamento FAMN, Universidad de Sevilla, Apartado 1065, 41080 Sevilla, Spain and Instituto Carlos I de F´ısica Te´orica y Computacional, Universidad de Sevilla, Spain L. R. Gasques, L. C. Chamon, V. A. B. Zagatto, A. L´epine-Szily, J. R. B. Oliveira Universidade de Sao Paulo, Instituto de Fisica, Rua do Matao, 1371, 05508-090, Sao Paulo, SP, Brazil V. Scarduelli Instituto de F´ısica, Universidade Federal Fluminense, 24210-340 Niter´oi,Rio de Janeiro, Brazil and Instituto de F´ısica da Universidade de S~aoPaulo, 05508-090, S~aoPaulo, SP, Brazil B. V. Carlson Departamento de F´ısica, Instituto Tecnol´ogico de Aeron´autica, S~aoJos´edos Campos, SP, Brazil J. Casal Dipartimento di Fisica e Astronomia "G. Galilei" and INFN-Sezione di Padova, Via Marzolo, 8, I-35131, Padova, Italy A. Arazi Laboratorio TANDAR, Comisi´onNacional de Energ´ıa At´omica, Av. Gral. Paz 1499, BKNA1650 San Mart´ın, Argentina D. A. Torres, F. Ramirez Departamento de F´ısica, Universidad Nacional de Colombia, Bogot´a,Colombia (Dated: December 20, 2019) We present new experimental angular distributions for the elastic scattering of 6Li + 120Sn at three bombarding energies. We include these data in a wide systematic involving the elastic scattering of 4;6He, 7Li, 9Be, 10B and 16;18O projectiles on the same target at energies around the respective Coulomb barriers. -
Two-Proton Radioactivity 2
Two-proton radioactivity Bertram Blank ‡ and Marek P loszajczak † ‡ Centre d’Etudes Nucl´eaires de Bordeaux-Gradignan - Universit´eBordeaux I - CNRS/IN2P3, Chemin du Solarium, B.P. 120, 33175 Gradignan Cedex, France † Grand Acc´el´erateur National d’Ions Lourds (GANIL), CEA/DSM-CNRS/IN2P3, BP 55027, 14076 Caen Cedex 05, France Abstract. In the first part of this review, experimental results which lead to the discovery of two-proton radioactivity are examined. Beyond two-proton emission from nuclear ground states, we also discuss experimental studies of two-proton emission from excited states populated either by nuclear β decay or by inelastic reactions. In the second part, we review the modern theory of two-proton radioactivity. An outlook to future experimental studies and theoretical developments will conclude this review. PACS numbers: 23.50.+z, 21.10.Tg, 21.60.-n, 24.10.-i Submitted to: Rep. Prog. Phys. Version: 17 December 2013 arXiv:0709.3797v2 [nucl-ex] 23 Apr 2008 Two-proton radioactivity 2 1. Introduction Atomic nuclei are made of two distinct particles, the protons and the neutrons. These nucleons constitute more than 99.95% of the mass of an atom. In order to form a stable atomic nucleus, a subtle equilibrium between the number of protons and neutrons has to be respected. This condition is fulfilled for 259 different combinations of protons and neutrons. These nuclei can be found on Earth. In addition, 26 nuclei form a quasi stable configuration, i.e. they decay with a half-life comparable or longer than the age of the Earth and are therefore still present on Earth. -
Scientific Opportunities with Fast Fragmentation Beams from RIA
Scientific Opportunities with Fast Fragmentation Beams from RIA National Superconducting Cyclotron Laboratory Michigan State University March 2000 EXECUTIVE SUMMARY................................................................................................... 1 1. INTRODUCTION............................................................................................................. 5 2. EXTENDED REACH WITH FAST BEAMS .................................................................. 9 3. SCIENTIFIC MOTIVATION......................................................................................... 12 3.1. Properties of Nuclei far from Stability ..................................................................... 12 3.2. Nuclear Astrophysics................................................................................................ 15 4. EXPERIMENTAL PROGRAM...................................................................................... 20 4.1. Limits of Nuclear Existence ..................................................................................... 20 4.2. Extended and Unusual Distributions of Neutron Matter .......................................... 33 4.3. Properties of Bulk Nuclear Matter............................................................................ 39 4.4. Collective Oscillations.............................................................................................. 51 4.5. Evolution of Nuclear Properties Towards the Drip Lines ........................................ 56 Appendix A: Rate -
Pair and Single Neutron Transfer with Borromean 8He A
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by HAL-CEA Pair and single neutron transfer with Borromean 8He A. Lemasson, A. Navin, M. Rejmund, N. Keeley, V. Zelevinsky, S. Bhattacharyya, A. Shrivastava, Dominique Bazin, D. Beaumel, Y. Blumenfeld, et al. To cite this version: A. Lemasson, A. Navin, M. Rejmund, N. Keeley, V. Zelevinsky, et al.. Pair and single neutron transfer with Borromean 8He. Physics Letters B, Elsevier, 2011, 697, pp.454-458. <10.1016/j.physletb.2011.02.038>. <in2p3-00565792> HAL Id: in2p3-00565792 http://hal.in2p3.fr/in2p3-00565792 Submitted on 14 Feb 2011 HAL is a multi-disciplinary open access L'archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destin´eeau d´ep^otet `ala diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publi´esou non, lished or not. The documents may come from ´emanant des ´etablissements d'enseignement et de teaching and research institutions in France or recherche fran¸caisou ´etrangers,des laboratoires abroad, or from public or private research centers. publics ou priv´es. Pair and single neutron transfer with Borromean 8He A. Lemassona,1, A. Navina,∗, M. Rejmunda, N. Keeleyb, V. Zelevinskyc, S. Bhattacharyyaa,d, A. Shrivastavaa,e, D. Bazinc, D. Beaumelf, Y. Blumenfeldf, A. Chatterjeee, D. Guptaf,2, G. de Francea, B. Jacquota, M. Labicheg, R. Lemmong, V. Nanalh, J. Nybergi, R. G. Pillayh, R. Raabea,3, K. Ramachandrane, J.A. Scarpacif, C. Schmitta, C. Simenelj, I. Stefana,f,4, C.N. -
Nucleosynthesis
Nucleosynthesis Nucleosynthesis is the process that creates new atomic nuclei from pre-existing nucleons, primarily protons and neutrons. The first nuclei were formed about three minutes after the Big Bang, through the process called Big Bang nucleosynthesis. Seventeen minutes later the universe had cooled to a point at which these processes ended, so only the fastest and simplest reactions occurred, leaving our universe containing about 75% hydrogen, 24% helium, and traces of other elements such aslithium and the hydrogen isotope deuterium. The universe still has approximately the same composition today. Heavier nuclei were created from these, by several processes. Stars formed, and began to fuse light elements to heavier ones in their cores, giving off energy in the process, known as stellar nucleosynthesis. Fusion processes create many of the lighter elements up to and including iron and nickel, and these elements are ejected into space (the interstellar medium) when smaller stars shed their outer envelopes and become smaller stars known as white dwarfs. The remains of their ejected mass form theplanetary nebulae observable throughout our galaxy. Supernova nucleosynthesis within exploding stars by fusing carbon and oxygen is responsible for the abundances of elements between magnesium (atomic number 12) and nickel (atomic number 28).[1] Supernova nucleosynthesis is also thought to be responsible for the creation of rarer elements heavier than iron and nickel, in the last few seconds of a type II supernova event. The synthesis of these heavier elements absorbs energy (endothermic process) as they are created, from the energy produced during the supernova explosion. Some of those elements are created from the absorption of multiple neutrons (the r-process) in the period of a few seconds during the explosion. -
Primordial Nucleosynthesis: from Precision Cosmology To
DSF-20/2008, FERMILAB-PUB-08-216-A, IFIC/08-37 Primordial Nucleosynthesis: from precision cosmology to fundamental physics Fabio Iocco a1 , Gianpiero Mangano b, Gennaro Miele b,c, Ofelia Pisanti b, Pasquale D. Serpico d2 aINAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy bDip. Scienze Fisiche, Universit`adi Napoli Federico II & INFN, Sez. di Napoli, Complesso Univ. Monte S. Angelo, Via Cintia, I-80126 Napoli, Italy c Instituto de F´ısica Corpuscular (CSIC-Universitat de Val`encia), Ed. Institutos de Investigaci´on, Apartado de Correos 22085, E-46071 Val`encia, Spain dCenter for Particle Astrophysics, Fermi National Accelerator Laboratory, Batavia, IL 60510-0500, USA Abstract We present an up-to-date review of Big Bang Nucleosynthesis (BBN). We discuss the main improvements which have been achieved in the past two decades on the overall theoretical framework, summarize the impact of new experimental results on nuclear reaction rates, and critically re-examine the astrophysical determinations of light nuclei abundances. We report then on how BBN can be used as a powerful test of new physics, constraining a wide range of ideas and theoretical models of fundamental interactions beyond the standard model of strong and electroweak forces and Einstein’s general relativity. Key words: Primordial Nucleosynthesis; Early Universe; Physics Beyond the arXiv:0809.0631v2 [astro-ph] 16 Apr 2009 Standard Model PACS: 98.80.Ft; 26.35.+c; 98.62.Ai Contents 1 Introduction 3 2 Standard Cosmology 6 1 Present address: Institut -
Direct Measurement of the Neutron
Louisiana State University LSU Digital Commons LSU Doctoral Dissertations Graduate School 1-9-2020 Stellar Nucleosynthesis: Direct Measurement of the Neutron- Capture Cross Sections of Stable Germanium Isotopes and Design of a Next Generation Ion Trap for the Study of Beta- Delayed Neutron Emission Alexander Laminack Louisiana State University and Agricultural and Mechanical College Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_dissertations Part of the Instrumentation Commons, Nuclear Commons, Physical Processes Commons, and the Stars, Interstellar Medium and the Galaxy Commons Recommended Citation Laminack, Alexander, "Stellar Nucleosynthesis: Direct Measurement of the Neutron-Capture Cross Sections of Stable Germanium Isotopes and Design of a Next Generation Ion Trap for the Study of Beta- Delayed Neutron Emission" (2020). LSU Doctoral Dissertations. 5131. https://digitalcommons.lsu.edu/gradschool_dissertations/5131 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Doctoral Dissertations by an authorized graduate school editor of LSU Digital Commons. For more information, please [email protected]. STELLAR NUCLEOSYNTHESIS: DIRECT MEASUREMENT OF THE NEUTRON-CAPTURE CROSS SECTIONS OF STABLE GERMANIUM ISOTOPES AND DESIGN OF A NEXT GENERATION ION TRAP FOR THE STUDY OF β-DELAYED NEUTRON EMISSION A Dissertation Submitted to the Graduate Faculty of the Louisiana State University and Agricultural and Mechanical College in partial fulfillment of the requirements for the degree of Doctor of Philosophy in The Department of Physics and Astronomy by Alexander Laminack B. S., The Unviersity of Alabama, 2015 May 2020 To my wife and son: Kristy Allen Alexander Laminack and Daniel Allen Laminack. -
Nucleosynthetic Isotope Variations of Siderophile and Chalcophile
Reviews in Mineralogy & Geochemistry Vol.81 pp. 107-160, 2016 3 Copyright © Mineralogical Society of America Nucleosynthetic Isotope Variations of Siderophile and Chalcophile Elements in the Solar System Tetsuya Yokoyama Department of Earth and Planetary Sciences Tokyo Institute of Technology Ookayama, Tokyo 152-885 Japan [email protected] Richard J. Walker Department of Geology University of Maryland College Park, MD 20742 USA [email protected] INTRODUCTION Numerous investigations have been devoted to understanding how the materials that contributed to the Solar System formed, were incorporated into the precursor molecular cloud and the protoplanetary disk, and ultimately evolved into the building blocks of planetesimals and planets. Chemical and isotopic analyses of extraterrestrial materials have played a central role in decoding the signatures of individual processes that led to their formation. Among the elements studied, the siderophile and chalcophile elements are crucial for considering a range of formational and evolutionary processes. Consequently, over the past 60 years, considerable effort has been focused on the development of abundance and isotopic analyses of these elements in terrestrial and extraterrestrial materials (e.g., Shirey and Walker 1995; Birck et al. 1997; Reisberg and Meisel 2002; Meisel and Horan 2016, this volume). In this review, we consider nucleosynthetic isotopic variability of siderophile and chalcophile elements in meteorites. Chapter 4 provides a review for siderophile and chalcophile elements in planetary materials in general (Day et al. 2016, this volume). In many cases, such variability is denoted as an “isotopic anomaly”; however, the term can be ambiguous because several pre- and post- Solar System formation processes can lead to variability of isotopic compositions as recorded in meteorites. -
A Doorway to Borromean Halo Nuclei: the Samba Configuration
A doorway to Borromean halo nuclei: the Samba configuration M. T. Yamashita Universidade Estadual Paulista, CEP 18409-010 Itapeva, SP, Brasil T. Frederico Departamento de F´ısica, Instituto Tecnol´ogico de Aeron´autica, Centro T´ecnico Aeroespacial, 12228-900 S˜ao Jos´edos Campos, Brasil M. S. Hussein Instituto de F´ısica, Universidade de S˜ao Paulo, C.P. 66318, CEP 05315-970 S˜ao Paulo, Brasil (Dated: October 22, 2018) We exploit the possibility of new configurations in three-body halo nuclei - Samba type - (the neutron-core form a bound system) as a doorway to Borromean systems. The nuclei 12Be, 15B, 23N and 27F are of such nature, in particular 23N with a half-life of 37.7 s and a halo radius of 6.07 fm is an excellent example of Samba-halo configuration. The fusion below the barrier of the Samba halo nuclei with heavy targets could reveal the so far elusive enhancement and a dominance of one-neutron over two-neutron transfers, in contrast to what was found recently for the Borromean halo nucleus 6He + 238U. PACS numbers: 25.70.Jj, 25.70.Mn, 24.10.Eq, 21.60.-n Borromean nuclei, be them halo or not, are quite com- isotope exists in oxygen (see, however, Ref. [1]). mon and their study has been intensive [1, 2, 3, 4]. These As an example we consider the boron isotopes: A = three-body systems have the property that any one of 8, 9, 10, 11, 12, 13, 14, 15, 17, 19. Both 17B and 19B their two-body subsystems is unbound. -
Analysing Dense Passage Retrieval for Multi-Hop Estion Answering
Combining Lexical and Dense Retrieval for Computationally Efficient Multi-hop Question Answering Georgios Sidiropoulos1, Nikos Voskarides2∗, Svitlana Vakulenko1, Evangelos Kanoulas1 1 University of Amsterdam, Amsterdam, The Netherlands 2 Amazon, Barcelona, Spain [email protected], [email protected], [email protected], [email protected] Abstract QA systems typically consist of (i) a retriever that identifies the passage/document in the underly- In simple open-domain question answering ing collection that contains the answer to the user’s (QA), dense retrieval has become one of the question, and (ii) a reader that extracts or generates standard approaches for retrieving the relevant the answer from the identified passage (Chen et al., passages to infer an answer. Recently, dense retrieval also achieved state-of-the-art results 2017). Given that often the answer cannot be found in multi-hop QA, where aggregating informa- in the top-ranked passage, inference follows a stan- tion from multiple pieces of information and dard beam-search procedure, where top-k passages reasoning over them is required. Despite their are retrieved and the reader scores are computed for success, dense retrieval methods are compu- all k passages (Lee et al., 2019). However, readers tationally intensive, requiring multiple GPUs are very sensitive to noise in the top-k passages, to train. In this work, we introduce a hy- thus making the performance of the retriever criti- brid (lexical and dense) retrieval approach that is highly competitive with the state-of-the-art cal for the performance of QA systems (Yang et al., dense retrieval models, while requiring sub- 2019). -
Table of Contents (Online, Part 1)
PERIODICALS Postmaster send address changes to: PHYSICALREVIEWCTM For editorial and subscription correspondence, PHYSICAL REVIEW C please see inside front cover APS Subscription Services (ISSN: 0556-2813) P.O. Box 41 Annapolis Junction, MD 20701 THIRD SERIES, VOLUME 90, NUMBER 6 CONTENTS DECEMBER 2014 RAPID COMMUNICATIONS Nuclear Structure Stretched states in 12,13B with the (d,α) reaction (5 pages) ................................................ 061301(R) A. H. Wuosmaa, J. P. Schiffer, S. Bedoor, M. Albers, M. Alcorta, S. Almaraz-Calderon, B. B. Back, P. F. Bertone, C. M. Deibel, C. R. Hoffman, J. C. Lighthall, S. T. Marley, R. C. Pardo, K. E. Rehm, and D. V. Shetty Intermediate-energy Coulomb excitation of 104Sn: Moderate E2 strength decrease approaching 100Sn (6 pages) ..................................................................................... 061302(R) P. Doornenbal, S. Takeuchi, N. Aoi, M. Matsushita, A. Obertelli, D. Steppenbeck, H. Wang, L. Audirac, H. Baba, P. Bednarczyk, S. Boissinot, M. Ciemala, A. Corsi, T. Furumoto, T. Isobe, A. Jungclaus, V. Lapoux, J. Lee, K. Matsui, T. Motobayashi, D. Nishimura, S. Ota, E. C. Pollacco, H. Sakurai, C. Santamaria, Y. Shiga, D. Sohler, and R. Taniuchi Probing shape coexistence by α decays to 0+ states (5 pages) ............................................. 061303(R) D. S. Delion, R. J. Liotta, Chong Qi, and R. Wyss Pairing-induced speedup of nuclear spontaneous fission (5 pages) .......................................... 061304(R) Jhilam Sadhukhan, J. Dobaczewski, W. Nazarewicz, J. A. Sheikh, and A. Baran Evidence of halo structure in 37Mg observed via reaction cross sections and intruder orbitals beyond the island of inversion (5 pages) ................................................................................ 061305(R) M. Takechi et al. From the lightest nuclei to the equation of state of asymmetric nuclear matter with realistic nuclear interactions (5 pages) ............................................................................... -
Refueling the Magic Furnace: Kilonova 2017 Rewrites the Story of Element Origins
Refueling the Magic Furnace: Kilonova 2017 Rewrites the Story of Element Origins Barry Wood University of Houston Abstract For more than half a century, we have understood element creation in the stars—described in Marcus Chown’s colorful image as “the magic furnace.” From 1958 until 2017, supernova explosions were thought to be the primary site of element creation above Iron, No. 26 on the Periodic Table. This assumption was radically overturned with the August 17, 2017, arrival of signals from a catastrophic collision of neutron stars. This paper traces the history of element-creation science leading to the striking discoveries attending “Kilonova 2017” that now call for a rewriting of the nucleosynthesis chapter of Big History. Correspondence | Barry Wood, [email protected] Citation | Wood, B. (2018) Refueling the Magic Furnace: Kilonova 2017 Rewrites the Story of Element Origins. Journal of Big History, II(3); 1 - 15. DOI | http://dx.doi.org/10.22339/jbh.v2i3.2300 Introduction Beginning at 24 Hertz, it gradually rose over 100 Pangea had recently broken up . North America and seconds to several hundred Hertz—indicating the Europe were slowly drifting apart inspiraling of two massive bodies about to detonate . the Himalayas had not yet appeared . tropical in a cataclysmic collision. Following 3,000 cycles, the jungles harbored enormous predatory dinosaurs that GW signal came to an abrupt end at 12:41:04.4 UTC would roam the earth for another 65 million years . (Coordinated Universal Time). Almost immediately mammals the size of housecats kept to the shadows . (1.74 seconds later) a two-second gamma-ray burst .