Low-Energy Nuclear Reactions Exploratory Work on 11Be
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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. -
6.2 Transition Radiation
Contents I General introduction 9 1Preamble 11 2 Relevant publications 15 3 A first look at the formation length 21 4 Formation length 23 4.1Classicalformationlength..................... 24 4.1.1 A reduced wavelength distance from the electron to the photon ........................... 25 4.1.2 Ignorance of the exact location of emission . ....... 25 4.1.3 ‘Semi-bare’ electron . ................... 26 4.1.4 Field line picture of radiation . ............... 26 4.2Quantumformationlength..................... 28 II Interactions in amorphous targets 31 5 Bremsstrahlung 33 5.1Incoherentbremsstrahlung..................... 33 5.2Genericexperimentalsetup..................... 35 5.2.1 Detectors employed . ................... 35 5.3Expandedexperimentalsetup.................... 39 6 Landau-Pomeranchuk-Migdal (LPM) effect 47 6.1 Formation length and LPM effect.................. 48 6.2 Transition radiation . ....................... 52 6.3 Dielectric suppression - the Ter-Mikaelian effect.......... 54 6.4CERNLPMExperiment...................... 55 6.5Resultsanddiscussion....................... 55 3 4 CONTENTS 6.5.1 Determination of ELPM ................... 56 6.5.2 Suppression and possible compensation . ........ 59 7 Very thin targets 61 7.1Theory................................ 62 7.1.1 Multiple scattering dominated transition radiation . .... 62 7.2MSDTRExperiment........................ 63 7.3Results................................ 64 8 Ternovskii-Shul’ga-Fomin (TSF) effect 67 8.1Theory................................ 67 8.1.1 Logarithmic thickness dependence -
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. -
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. -
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) ............................................................................... -
Generation and Modeling of Radiation for Clinical and Research Applications Bishwambhar Sengupta Clemson University, [email protected]
Clemson University TigerPrints All Dissertations Dissertations 8-2019 Generation and Modeling of Radiation for Clinical and Research Applications Bishwambhar Sengupta Clemson University, [email protected] Follow this and additional works at: https://tigerprints.clemson.edu/all_dissertations Recommended Citation Sengupta, Bishwambhar, "Generation and Modeling of Radiation for Clinical and Research Applications" (2019). All Dissertations. 2440. https://tigerprints.clemson.edu/all_dissertations/2440 This Dissertation is brought to you for free and open access by the Dissertations at TigerPrints. It has been accepted for inclusion in All Dissertations by an authorized administrator of TigerPrints. For more information, please contact [email protected]. Generation and Modeling of Radiation for Clinical and Research Applications A Dissertation Presented to the Graduate School of Clemson University In Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy Physics by Bishwambhar Sengupta August 2019 Accepted by: Dr. Endre Takacs, Committee Chair Dr. Delphine Dean Dr. Brian Dean Dr. Jian He Abstract Cancer is one of the leading causes of death in todays world and also accounts for a major share of healthcare expenses for any country. Our research goals are to help create a device which has improved accuracy and treatment times that will alleviate the resource strain currently faced by the healthcare community and to shed some light on the elementary nature of the interaction between ionizing radiation and living cells. Stereotactic radiosurgery is the treatment of cases in intracranial locations using external radiation beams. There are several devices that can perform radiosurgery, but the Rotating Gamma System is relatively new and has not been extensively studied. -
Arxiv:2103.05357V1 [Nucl-Ex] 9 Mar 2021
Experimental Study of Intruder Components in Light Neutron-rich Nuclei via Single-nucleon Transfer Reaction∗ Liu Wei,1 Lou Jianling,1, y Ye Yanlin,1 and Pang Danyang2 1School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China 2School of Physics, Beijing Key Laboratory of Advanced Nuclear Materials and Physics, Beihang University, Beijing 100191, China With the development of radioactive beam facilities, study on the shell evolution in unstable nuclei has become a hot topic. The intruder components, especially s-wave intrusion, in the low-lying states of light neutron-rich nuclei near N = 8 are of particular importance for the study of shell evolution. Single-nucleon transfer reaction in inverse kinematics has been a sensitive tool to quantitatively investigate the single-particle- orbital component in the selectively populated states. The spin-parity, the spectroscopic factor (or single-particle strength), as well as the effective single-particle energy can be extracted from this kind of reaction. These ob- servables are often useful to explain the nature of shell evolution, and to constrain, check and test parameters used in nuclear structure models. In this article, we review the experimental studies of the intruder components in neutron-rich He, Li, Be, B, C isotopes by using various single-nucleon transfer reactions. Focus will be laid on the precise determination of the intruder s-wave strength in low-lying states. Keywords: single-nucleon transfer reaction, intruder component, light neutron-rich nuclei I. INTRODUCTION components in low-lying states. Sometimes, these two or- bitals are even inverted, which means the 2s1=2 orbital can Electrons confined by Coulomb potential in atoms possess intrude into 1d5=2, and occasionally even intrude into 1p1=2 a well-known shell structure. -
The 29F Nucleus As a Lighthouse on the Coast of the Island of Inversion ✉ L
PERSPECTIVE https://doi.org/10.1038/s42005-020-00402-5 OPEN The 29F nucleus as a lighthouse on the coast of the island of inversion ✉ L. Fortunato 1,2 , J. Casal 1,2, W. Horiuchi 3, Jagjit Singh 4 & A. Vitturi1,2 1234567890():,; The exotic, neutron-rich and weakly-bound isotope 29F stands out as a waymarker on the southern shore of the island of inversion, a portion of the nuclear chart where the effects of nuclear forces lead to a reshuffling of the single particle levels and to a reorganization of the nuclear structure far from stability. This nucleus has become very popular, as new measurements allow to refine theoretical models. We review the latest developments and suggest how to further assess the structure by proposing predictions on electromagnetic transitions that new experiments of Relativistic Coulomb Excitation should soon become able to measure. eakly bound nuclear systems severely test our ability to disentangle the mysteries and oddities of the nuclear interactions and how nuclear systems achieve stability. One of W fl the latest conundrums in this respect is the structure of the exotic 29- uorine isotope. With nine protons and 20 neutrons, it is located almost on the edge of the stability valley of the = nuclide chart, very close to the neutron drip-line, i.e., the dividing line (Sn 0, null separation energy) between bound and unbound neutron-rich nuclei. Pioneering researches on this isotope have recently skyrocketed, as more and more theoretical and experimental papers are being published. The main interest lies in understanding if it belongs to the so-called island of inversion, a portion of the nuclear chart where the standard list of single-particle energy levels (that are filled by nucleons, very similarly to the atomic physics counterpart, in a sort of Aufbauprinzip, a.k.a. -
Interactions of Particles and Matter, with a View to Tracking
Interactions of particles and matter, with a view to tracking 2nd EIROforum School on Instrumentation, May 15th-22nd 2011, EPN science campus, Grenoble The importance of interactions Particles can interact with matter they traverse according to their nature and energy, and according to the properties of the matter being traversed. These interactions blur the trajectory and cause energy loss, but ... they are the basis for tracking and identification. In this presentation, we review the mechanisms that are relevant to present particle physics experiments. Particles we©re interested in Common, long-lived particles that high- energy experiments track and identify: gauge bosons: leptons: e±, µ±, , e µ hadrons: p, n, , K, ... Most are subject to electro-magnetic interactions (), some interact through the strong force (gluons), a few only feel the weak force (W±, Z). No gravity ... [Drawings: Mark Alford (0- mesons, ½+ baryons), ETHZ (bottom)] Energies that concern us The physics of current experiments may play in the TeV-EeV energy range. But detection relies on processes from the particle energy down to the eV ! [Top: LHC, 3.5+3.5 TeV, Bottom: Auger Observatory, > EeV] Interactions of neutrinos Neutrino interactions with matter are exceedingly rare. Interactions coming in 2 kinds: W± exchange: ªcharged currentº Z exchange: ªneutral currentº Typical reactions: - e n p e + e p n e ( discovery: Reines and Cowan, 1956) - + ± (in the vicinity of a nucleus, W or Z) - - e e (neutral current discovery, 1973) First neutral current event First neutral current event, seen in + the Gargamelle bubble chamber: e - - + - e e e e - One candidate found in 360,000 e anti-neutrino events. -
Bethe Formula
Bethe formula The Bethe formula describes[1] the mean energy loss per distance travelled of swift charged particles (protons, alpha particles, atomic ions) traversing matter (or alternatively the stopping power of the material). For electrons the energy loss is slightly different due to their small mass (requiring relativistic corrections) and their indistinguishability, and since they suffer much larger losses by Bremsstrahlung, terms must be added to account for this. Fast charged particles moving through matter interact with the electrons of atoms in the material. The interaction excites or ionizes the atoms, leading to an energy loss of the traveling particle. The non-relativistic version was found by Hans Bethe in 1930; the relativistic version (shown below) was found by him in 1932.[2] The most probable energy loss differs from the mean energy loss and is described by the Landau-Vavilov distribution.[3] The Bethe formula is sometimes called "Bethe-Bloch formula", but this is misleading (see below). Contents The formula The mean excitation potential Corrections to the Bethe formula The problem of nomenclature See also References External links The formula For a particle with speed v, charge z (in multiples of the electron charge), and energy E, traveling a distance x into a target of electron number density n and mean excitation potential I, the relativistic version of the formula reads, in SI units:[2] (1) where c is the speed of light and ε0 the vacuum permittivity, , e and me the electron charge and rest mass respectively. Here, the electron density of the material can be calculated by where ρ is the density of the material, Z its atomic number, A its relative atomic mass, NA the Avogadro number and Mu the Molar mass constant.