Collaborators: Prof. W. Sandhas and members of his group (Bonn),
|
|
- Carmel Lawson
- 6 years ago
- Views:
Transcription
1 Few Body Systems A1 Integral Equations (AGS) A2 Integro-differential equations (Hyperspherical Harmonics) A3 Time evolution methods A4 Supersymmetric Quantum Mechanics (SUSY) and Few-Body systems A5 Astrophysics A6 Few--quark systems A7 Eta-meson light nucleus scattering A8 Resonances A9 Molecular Systems A10 Numerical and computational methods Collaborators: Prof. W. Sandhas and members of his group (Bonn), Dr M. Fabre de la Ripelle (Orsay) Prof. I. Lagaris and members of his group (Ioannina) Prof. V.B. Belyaev and members of his group (Dubna), Dr S.A. Rakityansky (Dubna) Dr H. Leeb (Vienna) Prof. E.O. Alt (Mainz), Dr W. Schweizer (T\"ubingen) Prof. S.Y. Larsen (Temple), Mr I. Matamba (Venda). Prof S Oryu (Tokyo) [A.1] Integral Equations (AGS) Study of few-body reactions, such as n + 3He ---> n + 3He p + 3H ---> d + d n + 4He ---> n + 4He in order to obtain insight into the low-energy dynamics; Test the Nucleon-Nucleon force; study break up and clustering; phenomena of light nuclei; study inter-cluster interactions; study photo- and electro-processes; develop the necessary numerical methods to
2 handle reliably fusion and astrophysical reactions. Published work (during the last 4 years): S. A Sofianos, H. Fiedeldey, and W. Sandhas, "Photo-disintegration of $^4He$ in the Integro-differential Equation approach" Phys. Rev. C 48, 2285 (1993). 2. S. A Sofianos, H. Fiedeldey, and W. Sandhas, Photo-induced Reactions on 4He" Few-Body Systems 7, 193 (1994). 3. S.A. Sofianos, H. Fiedeldey, and G. Ellerkmann, "Inclusion of Final--State-Interaction Effects in the Photo-disintegration of the alpha-particle" Few-Body Systems 18, 173(1995). 4. G. Ellerkmann, W. Sandhas, and S. A. Sofianos "Integral Equation Calculations for the Photo-disintegration of 4He" Few-Body Systems Suppl. 8, 102(1995). 5. G. Ellerkmann, W. Sandhas, S. A. Sofianos, and H. Fiedeldey "Integral Equation Calculations for the Photo-disintegration process 4He(gamma,n)3He" Phys. Rev C 53, 2638 (1996). 6. S.A. Sofianos, H. Fiedeldey, G. Ellerkmann, and W. Sandhas "Photo-induced Reactions on 4He" Few-Body Systems 7, 193 (1994). 7. R.M. Adam, H. Fiedeldey, S. A. Sofianos, and H. Leeb, "Error propagation from the nucleon--nucleon data to three- and four-nucleon binding energies" Nucl. Phys., A559, 157 (1993). 8. L. L. Howell, S. A. Sofianos, H. Fiedeldey, and G. Pantis, "Nucleon-alpha Potential by Marchenko Inversion and Supersymmetry" Nucl. Phys., A556, 29 (1993) [A.2] Integro-differential equations (Hyperspherical Harmonics) Easy construction of wave functions Obtain Bound states GO BEYOND A = 4 1. M. Fabre de la Ripelle, M. Braun, and S. A. Sofianos, "Integro-differential Equation for a Large Number of Particles" Submitted: Prog. Theor Phys. [A.3] Time evolution methods
3 Study systems where the underlying Hamiltonian is time-dependent. Developing computational methods for handling the evolution of quantum mechanical systems in time, i.e., "photograph" the events of a certain process such as the electron-light nucleus scattering. 1. I. E. Lagaris, D. G. Papageorgiou, M. Braun, and S. A. Sofianos, "A Relaxation method for Nonlocal and non-hermitian Operators" J. of Comp. Phys. 125, 229 (1996) [A.4] Supersymmetric Quantum Mechanics (SUSY) and Few-Body systems To study: Deep NN potential and their SUSY partners. Effect of SUSY applied at two--body level on few--body systems. # Intercluster interactions (see SUSY) [A.5]Astrophysics To study Helium--like Atoms in Strong (Astrophysical) Magnetic fields Besides the astrophysical aspects white dwarf stars are ``high magnetic field laboratories'' For example: The spectrum of the magnetic white dwarf GD229, discovered two decades ago, is still a complete mystery. This is the same situation as for hydrogen rich white dwarfs a few years ago. By calculating transitions of helium in strong magnetic fields it might be possible to decipher these spectra (Step towards understanding white dwarfs) Calculate bound/bound transitions for helium in strong magnetic fields relevant for white dwarf stars. Nucleosynthesis; Primordial abundances of the light elements and their impact on the standard big--bang nucleosynthesis theory. As a staring point we studied: p + d + e- ---> 3He+e- 3He + 4He + e- ----> 3He + 4He + e- at thermonuclear energies. 1. S. A. Rakityansky, S. A. Sofianos, L. L. Howell, M. Braun, and V. B. Belyaev, "Nonradiative proton-deuteron fusion in stellar plasastrma" To appear: Nucl. Phys. A. [A.6] Few--quark systems
4 Study the few quark system within the non-relativistic few--body theory 1. E.J.O Gavin, H.Fiedeldey, H. Leeb, and S. A. Sofianos, "Supersymmetric quantum mechanics applied to non-relativistic quark models" Int. J. Mod. Phys. A, 8, 1437 (1993). 2. E. J. O. Gavin, H. Fiedeldey, and S. A. Sofianos, "Three-body forces from n-body inversion" Intern. Journal of Modern Phys. E 4, 431(1995) 3. E. J. O. Gavin, R. M. Adam, H. Fiedeldey, and S. A. Sofianos, "Relationship between the proton charge form factor and the quark--quark interaction" Few-Body Systems 19, 59(1995) [A.7] Eta-meson light nucleus scattering To study the question of isotopic invariance breaking, the meson--nucleus scattering mechanism and various other particle and nuclear physics questions S. Rakityansky, S. A. Sofianos and B. V. Belyaev, "Near Threshold eta-meson interaction with light nuclei in "Effective Interactions in Quantal Systems" ed. S. A. Sofianos, Unisa, Dec S. Rakityansky, S. A. Sofianos, V. B. Belyaev, and W. Sandhas in "On the possibility of an eta-meson light nucleus bound state formation'' Few-Body Systems Suppl. 9, 227(1995). 3. S. Rakityansky, S. A. Sofianos, W. Sandhas, and V. B. Belyaev "Threshold scattering of the eta-meson off light nuclei" Physics Letter B 359, 33(1995). 4. V. B. Belyaev, S. A. Rakityansky, S. A. Sofianos, M Braun, and W. Sandhas in "Low-- energy interaction of eta-meson with light nuclei'' Chinese Journal of Physics 34,998 (1996). 5. S. A. Rakityansky, S. A. Sofianos, M Braun, V. B. Belyaev, and W. Sandhas in "Quasi-- bound states of eta-nucleus systems" Phys. Rev. C 53, R2043 (1996). [A.8] Resonances Investigate via an exact method the presence of potential resonances (two-body) and their manifestation and effects in few-body systems. Extremely important in molecular physics.
5 1. S. Rakityansky, S. A. Sofianos, and K. Amos "A method of calculating the Jost function for analytic potentials" Il Nuovo Cimento, 111 B, 353 (1996). 2. S. A. Sofianos and S. A. Rakityansky, "Exact method for locating potential resonances and Regge trajectories" Accepted: J. of Phys. G [A.9] Molecular systems Investigate Molecular systems: bound states and ultra-low energy scattering. The 4He trimer is of interest in various areas of Physics Chemistry, and Molecular physics such as the condensed-matter, nuclear, and the rare-gas atoms behaviour under First step towards understanding liquid 4He drops, superfluidity in 4He films. Work using Variational and Monte-Carlo. Exact microscopic calculations can, in principle, performed using Faddeev equations. However, the underlying van der Waal forces are of a hard-core nature which make investigations via these equations cumbersome and tedious. Use of Boundary Condition Model. 1. M. Braun, S. A. Sofianos, D. G. Papageorgiou, I. E. Lagaris, "Ground State Calculations for 4He-molecules" Submitted: Nuovo Cimento 2. E. A. Kolganova, A. K. Motovilov, and S. A. Sofianos "Ultra-low energy scattering of a He atom off a He dimer" Submitted: PRA (Rapid Comm.) 3. E. A. Kolganova, A. K. Motovilov, and S. A. Sofianos "Three--Body Configuration Space Calculations with Hard Core Potentials" Submitted: PRA [A.10] Numerical and computational methods Study various numerical analysis questions! 1. M. Braun, S. A. Sofianos, D. G. Papageorgiou, I. E. Lagaris, "An Efficient Chebyshev-- Lanzcos Method for obtaining Eigensolutions of the Schr\"odinger Equation on a Grid" J. Comput. Phys. 125, 215 (1996).
Emission of Helium Nuclei in Relativistic Proton Interactions Leading to Total Break up of Ag and Br Nuclei. Z.Physik A 279, 407 (1976).
Emission of Helium Nuclei in Relativistic Proton Interactions Leading to Total Break up of Ag and Br Nuclei. Z.Physik A 279, 407 (1976). Inelastic Interactions of 69.0 GeV/c Protons with Emulsion Nuclei.
More informationEffective Field Theory for Nuclear Physics! Akshay Vaghani! Mississippi State University!
Effective Field Theory for Nuclear Physics! Akshay Vaghani! Mississippi State University! Overview! Introduction! Basic ideas of EFT! Basic Examples of EFT! Algorithm of EFT! Review NN scattering! NN scattering
More informationNeutron-to-proton ratio
Neutron-to-proton ratio After one second, the Universe had cooled to 10 13 K. The Universe was filled with protons, neutrons, electrons, and neutrinos. The temperature was high enough that they interconverted
More informationElectromagnetic reactions from few to many-body systems Giuseppina Orlandini
Electromagnetic reactions from few to many-body systems Giuseppina Orlandini ECT* Workshop on Recent advances and challenges in the description of nuclear reactions at the limit of stability, March 5-9,
More informationCHEM 312: Lecture 9 Part 1 Nuclear Reactions
CHEM 312: Lecture 9 Part 1 Nuclear Reactions Readings: Modern Nuclear Chemistry, Chapter 10; Nuclear and Radiochemistry, Chapter 4 Notation Energetics of Nuclear Reactions Reaction Types and Mechanisms
More informationThe Neutron Structure Function from BoNuS
The Neutron Structure Function from BoNuS Stephen Bültmann 1 Physics Department, Old Dominion University, Norfolk, VA 359, USA Abstract. The BoNuS experiment at Jefferson Lab s Hall B measured the structure
More informationClusters in Dense Matter and the Equation of State
Clusters in Dense Matter and the Equation of State Excellence Cluster Universe, Technische Universität München GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt in collaboration with Gerd Röpke
More informationRecent results in lattice EFT for nuclei
Recent results in lattice EFT for nuclei Dean Lee (NC State) Nuclear Lattice EFT Collaboration Centro de Ciencias de Benasque Pedro Pascua Bound states and resonances in EFT and Lattice QCD calculations
More informationASTRONOMY 220C ADVANCED STAGES OF STELLAR EVOLUTION AND NUCLEOSYNTHESIS. Spring, This is a one quarter course dealing chiefly with:
This is a one quarter course dealing chiefly with: ASTRONOMY 220C ADVANCED STAGES OF STELLAR EVOLUTION AND NUCLEOSYNTHESIS Spring, 2015 http://www.ucolick.org/~woosley a) Nuclear astrophysics and the relevant
More informationUnitary-model-operator approach to nuclear many-body problems
Unitary-model-operator approach to nuclear many-body problems in collaboration with Structure calc. for many-nucleon systems Kenji Suzuki (Kyushu Inst. of Tech.) Ryoji kamoto (Kyushu Inst. of Tech.) V
More informationTheoretical Nuclear Physics
Theoretical Nuclear Physics (SH2011, Second cycle, 6.0cr) Comments and corrections are welcome! Chong Qi, chongq@kth.se The course contains 12 sections 1-4 Introduction Basic Quantum Mechanics concepts
More informationChiral effective field theory on the lattice: Ab initio calculations of nuclei
Chiral effective field theory on the lattice: Ab initio calculations of nuclei Nuclear Lattice EFT Collaboration Evgeny Epelbaum (Bochum) Hermann Krebs (Bochum) Timo Lähde (Jülich) Dean Lee (NC State)
More informationWeakly-Bound Systems in Atomic and Nuclear Physics March 2010
Electroweak properties of Weakly- Bound Light Nuclei Weakly-Bound Systems in Atomic and Nuclear Physics March 2010 INSTITUTE FOR NUCLEAR THEORY Collaborators Sonia Bacca Winfried Leidemann, Giuseppina
More informationNuclear Physics and Astrophysics
Nuclear Physics and Astrophysics PHY-302 Dr. E. Rizvi Lecture 1 - Course Organiser: Deputy: Dr E. Rizvi (room 401) Prof. J. Emerson My Office hours 1000 1100 Thursday 3 lecture slots per week Thursday
More informationThe Nuclear Many-Body Problem. Lecture 2
The Nuclear Many-Body Problem Lecture 2 How do we describe nuclei? Shell structure in nuclei and the phenomenological shell model approach to nuclear structure. Ab-initio approach to nuclear structure.
More informationThe origin of the light elements in the early Universe
1 HUBERT REEVES* The origin of the light elements in the early Universe Shortly after World War II, George Gamov and his collaborators (Alpher et al. 148) considered the possibility that all chemical elements
More information= : K A
Atoms and Nuclei. State two limitations of JJ Thomson s model of atom. 2. Write the SI unit for activity of a radioactive substance. 3. What observations led JJ Thomson to conclusion that all atoms have
More informationp 3 A = 12 C s A = 16 O s d E η m η (MeV)
PRODUCTION AND DECAY OF ETA-MESIC NUCLEI A. I. L'VOV P. N. Lebedev Physical Institute, Russian Academy of Sciences Leninsky Prospect 5, Moscow 79, Russia Using the Green function method, binding eects
More information:Lecture 27: Stellar Nucleosynthesis. Cassieopia A
:Lecture 27: Stellar Nucleosynthesis Cassieopia A Major nuclear burning processes Common feature is release of energy by consumption of nuclear fuel. Rates of energy release vary enormously. Nuclear processes
More informationPHY-105: Introduction to Particle and Nuclear Physics
M. Kruse, Spring 2011, Phy-105 PHY-105: Introduction to Particle and Nuclear Physics Up to 1900 indivisable atoms Early 20th century electrons, protons, neutrons Around 1945, other particles discovered.
More informationLIST OF PUBLICATIONS. Subject: "Pion absorption in the nucleus through the ; nn reaction". Carried
LIST OF PUBLICATIONS I. Ph.D. Thesis Subject: "Pion absorption in the nucleus through the ; nn reaction". Carried out under the supervision of Professor Judah M. Eisenberg, July 1981. II. Scientic Papers
More informationFROM QCD TO NUCLEI: ASPECTS OF NUCLEAR THEORY IN FRANCE
FROM QCD TO NUCLEI: ASPECTS OF NUCLEAR THEORY IN FRANCE Ubirajara van Kolck Institut de Physique Nucléaire 1 Outline Hadronic theory in France Nuclear forces from QCD Low-energy nuclear theory in France
More informationORIGIN OF THE ELEMENETS
VISUAL PHYSICS ONLINE ORIGIN OF THE ELEMENETS Watch Video: The Origin of the Elements The ordinary matter in our universe (known as baryonic matter) is made up of 94 naturally occurring elements. It is
More informationNuclear Structure for the Crust of Neutron Stars
Nuclear Structure for the Crust of Neutron Stars Peter Gögelein with Prof. H. Müther Institut for Theoretical Physics University of Tübingen, Germany September 11th, 2007 Outline Neutron Stars Pasta in
More information[1] (c) Some fruits, such as bananas, are naturally radioactive because they contain the unstable isotope of potassium-40 ( K.
(a) State, with a reason, whether or not protons and neutrons are fundamental particles....... [] (b) State two fundamental particles that can be classified as leptons.... [] (c) Some fruits, such as bananas,
More informationChapter 27 The Early Universe Pearson Education, Inc.
Chapter 27 The Early Universe Units of Chapter 27 27.1 Back to the Big Bang 27.2 The Evolution of the Universe More on Fundamental Forces 27.3 The Formation of Nuclei and Atoms 27.4 The Inflationary Universe
More informationPhysics Courses. Courses. Physics Courses 1
Physics Courses 1 Physics Courses Courses PHYS 1403. General Physics I (C). General Physics I (3-2) A non-calculus treatment of mechanics and heat. Laboratory experience is an essential component of this
More informationNew Frontiers in Nuclear Structure Theory
New Frontiers in Nuclear Structure Theory From Realistic Interactions to the Nuclear Chart Robert Roth Institut für Kernphysik Technical University Darmstadt Overview Motivation Nucleon-Nucleon Interactions
More informationNuclear Physics from Lattice Effective Field Theory
Nuclear Physics from Lattice Effective Field Theory Dean Lee (NCSU/Bonn) work done in collaboration with Evgeny Epelbaum (Bochum) Hermann Krebs (Bochum) Ulf-G. Meißner (Bonn/Jülich) Buḡra Borasoy (now
More informationThe double tetrahedron structure of the nucleus
The double tetrahedron structure of the nucleus Jozsef Garai Department of Earth Sciences Florida International University University Park, PC-344 Miami, FL 33199 Ph: 305-348-3445 Fax: 305-348-3070 E-mail:
More information1 Geant4 to simulate Photoelectric, Compton, and Pair production Events
Syed F. Naeem, hw-12, Phy 599 1 Geant4 to simulate Photoelectric, Compton, and Pair production Events 1.1 Introduction An Aluminum (Al) target of 20cm was used in this simulation to see the eect of incoming
More informationNuclear Physics and Nuclear Reactions
Slide 1 / 33 Nuclear Physics and Nuclear Reactions The Nucleus Slide 2 / 33 Proton: The charge on a proton is +1.6x10-19 C. The mass of a proton is 1.6726x10-27 kg. Neutron: The neutron is neutral. The
More informationRadioactivity, Radiation and the Structure of the atom
Radioactivity, Radiation and the Structure of the atom What do you know (or can we deduce) about radioactivity from what you have learned in the course so far? How can we learn about whether radioactive
More informationNuclear Reactions. Shape, interaction, and excitation structures of nuclei. scattered particles. detector. solid angle. target. transmitted particles
Nuclear Reactions Shape, interaction, and excitation structures of nuclei scattering expt. scattered particles detector solid angle projectile target transmitted particles http://www.th.phys.titech.ac.jp/~muto/lectures/qmii11/qmii11_chap21.pdf
More informationNuclear Structure and Reactions using Lattice Effective Field Theory
Nuclear Structure and Reactions using Lattice Effective Field Theory Dean Lee North Carolina State University Nuclear Lattice EFT Collaboration Frontiers of Nuclear Physics Kavli Institute for Theoretical
More informationNuclear Physics and Astrophysics
Nuclear Physics and Astrophysics PHY-302 Dr. E. Rizvi Lecture 1 - Course Organiser: Deputy: Dr E. Rizvi (room 401) Dr A. Bevan My Office hours 1000 1100 Thursday 3 lecture slots per week Thursday 0900-1000
More informationLecture 3: Big Bang Nucleosynthesis The First Three Minutes
Lecture 3: Big Bang Nucleosynthesis The First Three Minutes Last time: particle anti-particle soup --> quark soup --> neutron-proton soup p / n ratio at onset of 2 D formation Today: Form 2 D and 4 He
More informationSolar Fusion Cross Sections for the pp chain and CNO cycles
Solar Fusion Cross Sections for the pp chain and CNO cycles Working Group 10: Theoretical Issues (Wick Haxton, Stefan Typel) status of theory at 1997 meeting (Rev. Mod. Phys. 70 (1998) 1265) progress during
More informationSome nuclear particles:
1 N U C L E A R R E A C T I O N S Definitions: Atomic Number or Nuclear Charge: The number of protons in the nucleus. This determines which element is present. It s the whole number of the element on the
More information26 January 2014 BLACK HOLES AND GAP
26 January 2014 BLACK HOLES AND GAP Antonino Zichichi INFN and University of Bologna, Italy CERN, Geneva, Switzerland Enrico Fermi Centre, Rome, Italy World Federation of Scientists, Beijing, Geneva, Moscow,
More informationThe Nuclear Many Body Problem Lecture 3
The Nuclear Many Body Problem Lecture 3 Shell structure in nuclei and the phenomenological shell model approach to nuclear structure Ab initio approach to nuclear structure. Green's function Monte Carlo
More informationhttp://imgs.xkcd.com/comics/cell_phones.png Announcements: Thursday: Group A to Hayes 105 for hands-on experience Group B comes here to work on worksheet Both groups: bring your calculator! Next Tuesday
More informationAFDMC Method for Nuclear Physics and Nuclear Astrophysics
AFDMC Method for Nuclear Physics and Nuclear Astrophysics Thanks to INFN and to F. Pederiva (Trento) Outline Motivations: NN scattering data few body theory. Few-body many body experiments/observations?
More informationJames Maxwell ( )
From Atoms To Stars James Maxwell (1831 1879) Finalized the work of others on electricity and magnetism. He formulated Maxwell Equations for the electromagnetic field. His equations predicted the existence
More informationNuclear Forces - Lecture 1 - R. Machleidt University of Idaho
CNS Summer School, Univ. of Tokyo, at Wako campus of RIKEN, Aug. 18-23, 2005 Nuclear Forces - Lecture 1 - R. Machleidt University of Idaho 1 Nuclear Forces - Overview of all lectures - Lecture 1: History,
More informationO WILEY- MODERN NUCLEAR CHEMISTRY. WALTER D. LOVELAND Oregon State University. DAVID J. MORRISSEY Michigan State University
MODERN NUCLEAR CHEMISTRY WALTER D. LOVELAND Oregon State University DAVID J. MORRISSEY Michigan State University GLENN T. SEABORG University of California, Berkeley O WILEY- INTERSCIENCE A JOHN WILEY &
More informationINTRODUCTION TO THE STRUCTURE OF MATTER
INTRODUCTION TO THE STRUCTURE OF MATTER A Course in Modern Physics John J. Brehm and William J. Mullin University of Massachusetts Amherst, Massachusetts Fachberelch 5?@8hnlsdie Hochschule Darmstadt! HochschulstraSa
More informationPhys102 Lecture 29, 30, 31 Nuclear Physics and Radioactivity
Phys10 Lecture 9, 30, 31 Nuclear Physics and Radioactivity Key Points Structure and Properties of the Nucleus Alpha, Beta and Gamma Decays References 30-1,,3,4,5,6,7. Atomic Structure Nitrogen (N) Atom
More informationPrimordial (Big Bang) Nucleosynthesis
Primordial (Big Bang) Nucleosynthesis H Li Be Which elements? He METALS - 1942: Gamow suggests a Big Bang origin of the elements. - 1948: Alpher, Bethe & Gamow: all elements are synthesized minutes after
More informationNuclear electric dipole moment in the Gaussian expansion method
Nuclear electric dipole moment in the Gaussian expansion method Nodoka Yamanaka (ithes Group, RIKEN) In collaboration with E. Hiyama (RIKEN), T. Yamada (Kanto-Gakuin Univ.), Y. Funaki (RIKEN) 2015/10/12
More informationLecture 36: The First Three Minutes Readings: Sections 29-1, 29-2, and 29-4 (29-3)
Lecture 36: The First Three Minutes Readings: Sections 29-1, 29-2, and 29-4 (29-3) Key Ideas Physics of the Early Universe Informed by experimental & theoretical physics Later stages confirmed by observations
More informationNuclear Landscape not fully known
Nuclear Landscape not fully known Heaviest Elements? Known Nuclei Limit of proton rich nuclei? Fission Limit? Possible Nuclei Limit of Neutron Rich Nuclei? Nuclear Radii Textbooks: R = r 00 A 1/3 1/3 I.
More informationThe Nuclear Many-Body Problem
The Nuclear Many-Body Problem relativistic heavy ions vacuum electron scattering quarks gluons radioactive beams heavy few nuclei body quark-gluon soup QCD nucleon QCD few body systems many body systems
More informationThree-cluster dynamics within an ab initio framework
Three-cluster dynamics within an ab initio framework Universality in Few-Body Systems: Theoretical Challenges and New Directions INT 14-1, March 26, 2014 S. Quaglioni Collaborators: C. Romero-Redondo (TRIUMF)
More informationQuantum mechanics of many-fermion systems
Quantum mechanics of many-fermion systems Kouichi Hagino Tohoku University, Sendai, Japan 1. Identical particles: Fermions and Bosons 2. Simple examples: systems with two identical particles 3. Pauli principle
More information14 Supernovae (short overview) introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1
14 Supernovae (short overview) introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1 The core-collapse of a supernova The core of a pre-supernova is made of nuclei in the iron-mass range A ~
More informationPHY357 Lecture 14. Applications of QCD. Varying coupling constant. Jets and Gluons. Quark-Gluon plasma. Colour counting
PHY357 Lecture 14 Applications of QCD Varying coupling constant Jets and Gluons Quark-Gluon plasma Colour counting The proton structure function (not all of section 5.8!) Variable Coupling Constants! At
More information13 Synthesis of heavier elements. introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1
13 Synthesis of heavier elements introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1 The triple α Reaction When hydrogen fusion ends, the core of a star collapses and the temperature can reach
More informationLecture 19 Nuclear Astrophysics. Baryons, Dark Matter, Dark Energy. Experimental Nuclear Physics PHYS 741
Lecture 19 Nuclear Astrophysics Baryons, Dark Matter, Dark Energy Experimental Nuclear Physics PHYS 741 heeger@wisc.edu References and Figures from: - Haxton, Nuclear Astrophysics - Basdevant, Fundamentals
More informationFACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON
FACULTY OF SCIENCE High Energy Physics WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON AIM: To explore nature on the smallest length scales we can achieve Current status (10-20 m)
More informationLecture 4: Nuclear Energy Generation
Lecture 4: Nuclear Energy Generation Literature: Prialnik chapter 4.1 & 4.2!" 1 a) Some properties of atomic nuclei Let: Z = atomic number = # of protons in nucleus A = atomic mass number = # of nucleons
More informationThreshold Photo-production of J/5 Mesons J. Dunne Jefferson Lab
hreshold Photo-production of J/5 Mesons J. Dunne Jefferson Lab Introduction With the advent of higher energies at Jefferson Lab, the study of charmonium becomes possible. he threshold production of J/5
More informationE. Fermi: Notes on Thermodynamics and Statistics (1953))
E. Fermi: Notes on Thermodynamics and Statistics (1953)) Neutron stars below the surface Surface is liquid. Expect primarily 56 Fe with some 4 He T» 10 7 K ' 1 KeV >> T melting ( 56 Fe) Ionization: r Thomas-Fermi
More informationThe Lorentz Integral Transform (LIT) method and its connections with other approaches
The Lorentz Integral Transform (LIT) method and its connections with other approaches First proposed in V. D. Efros, W. Leidemann and G. Orlandini, Phys. Lett. B338, 130 (1994) Recent Topical Review: V.
More informationPoS(Confinement8)147. Universality in QCD and Halo Nuclei
Helmholtz-Institut für Strahlen- und Kernphysik (Theorie) and Bethe Center for Theoretical Physics, University of Bonn, Germany E-mail: hammer@itkp.uni-bonn.de Effective Field Theory (EFT) provides a powerful
More informationCarbon-12 in Nuclear Lattice EFT
Carbon-12 in Nuclear Lattice EFT Nuclear Lattice EFT Collaboration Evgeny Epelbaum (Bochum) Hermann Krebs (Bochum) Timo A. Lähde (Jülich) Dean Lee (NC State) Thomas Luu (Jülich) Ulf-G. Meißner (Bonn/Jülich)
More informationFew Body Methods in Nuclear Physics - Lecture I
Few Body Methods in Nuclear Physics - Lecture I Nir Barnea The Hebrew University, Jerusalem, Israel Sept. 2010 Course Outline 1 Introduction - Few-Body Nuclear Physics 2 Gaussian Expansion - The Stochastic
More informationBIG BANG SUMMARY NOTES
BIG BANG SUMMARY NOTES BIG BANG THEORY Studies of red-shifts of distant galaxies show that the universe is expanding. This and other observations has led to the Big Bang Theory The Big Bang Theory claims
More informationPoS(NIC XII)250. A new equation of state with abundances of all nuclei in core collapse simulations of massive stars
A new equation of state with abundances of all nuclei in core collapse simulations of massive stars 1, Kohsuke Sumiyoshi 2, Shoichi Yamada 1,3, Hideyuki Suzuki 4 1 Department of Science and Engineering,
More informationAtoms, nuclei, particles
Atoms, nuclei, particles Nikolaos Kidonakis Physics for Georgia Academic Decathlon September 2016 Age-old questions What are the fundamental particles of matter? What are the fundamental forces of nature?
More informationL. David Roper
The Heavy Proton L. David Roper mailto:roperld@vt.edu Introduction The proton is the nucleus of the hydrogen atom, which has one orbiting electron. The proton is the least massive of the baryons. Its mass
More informationAb initio alpha-alpha scattering using adiabatic projection method
Ab initio alpha-alpha scattering using adiabatic projection method Serdar Elhatisari Advances in Diagrammatic Monte Carlo Methods for QFT Calculations in Nuclear-, Particle-, and Condensed Matter Physics
More informationLecture 24: Cosmology: The First Three Minutes. Astronomy 111 Monday November 27, 2017
Lecture 24: Cosmology: The First Three Minutes Astronomy 111 Monday November 27, 2017 Reminders Last star party of the semester tomorrow night! Online homework #11 due Monday at 3pm The first three minutes
More informationNuclear and Particle Physics
Nuclear and Particle Physics W. S. С Williams Department of Physics, University of Oxford and St Edmund Hall, Oxford CLARENDON PRESS OXFORD 1991 Contents 1 Introduction 1.1 Historical perspective 1 1.2
More informationTHE NUCLEUS: A CHEMIST S VIEW Chapter 20
THE NUCLEUS: A CHEMIST S VIEW Chapter 20 "For a long time I have considered even the craziest ideas about [the] atom[ic] nucleus... and suddenly discovered the truth." [shell model of the nucleus]. Maria
More informationLecture 3: Big Bang Nucleosynthesis
Lecture 3: Big Bang Nucleosynthesis Last time: particle anti-particle soup --> quark soup --> neutron-proton soup. Today: Form 2 D and 4 He Form heavier nuclei? Discuss primordial abundances X p, Y p,
More information13. Basic Nuclear Properties
13. Basic Nuclear Properties Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 13. Basic Nuclear Properties 1 In this section... Motivation for study The strong nuclear force Stable nuclei Binding
More informationNuclear structure Anatoli Afanasjev Mississippi State University
Nuclear structure Anatoli Afanasjev Mississippi State University 1. Nuclear theory selection of starting point 2. What can be done exactly (ab-initio calculations) and why we cannot do that systematically?
More informationRadioactivity, Radiation and the Structure of the atom
Radioactivity, Radiation and the Structure of the atom What do you know (or can we deduce) about radioactivity from what you have learned in the course so far? How can we learn about whether radioactive
More informationPoS(Baldin ISHEPP XXII)042
Multifragmentation of nuclei by photons: new approaches and results Institute for Nuclear Research RAS Prospect 60-let Octabra, 7A, 117312 Moscow, Russia E-mail: vladimir@cpc.inr.ac.ru A review on multifragmentation
More informationAn Introduction to. Nuclear Physics. Yatramohan Jana. Alpha Science International Ltd. Oxford, U.K.
An Introduction to Nuclear Physics Yatramohan Jana Alpha Science International Ltd. Oxford, U.K. Contents Preface Acknowledgement Part-1 Introduction vii ix Chapter-1 General Survey of Nuclear Properties
More informationStrong Interactions and QCD
Strong Interactions and QCD Sourendu Gupta DTP: TIFR DIM 2009 TIFR, Mumbai November 4, 2009 SG (DTP: TIFR) Strong Interactions DIM 09 1 / 14 The experimental context of strong interactions 1 Thomson and
More informationFundamental Forces. David Morrissey. Key Concepts, March 15, 2013
Fundamental Forces David Morrissey Key Concepts, March 15, 2013 Not a fundamental force... Also not a fundamental force... What Do We Mean By Fundamental? Example: Electromagnetism (EM) electric forces
More informationIsospin-symmetry breaking in nuclei around the N=Z line
Isospin-symmetry breaking in nuclei around the N=Z line Yang Sun Shanghai Jiao Tong University University of Hong Kong, July. 6-9, 2015 The concept of isospin Isospin of a nucleon: Projection of isospin:
More informationExtreme QCD. Sourendu Gupta. International Colloquium on Perspectives in Fundamental Research TIFR, Mumbai March 4, 2010 TIFR
Extreme QCD Sourendu Gupta TIFR International Colloquium on Perspectives in Fundamental Research TIFR, Mumbai March 4, 2010 Extreme reductionism Building things up Particles Nuclei and stars Hot matter
More informationBasic Nuclear Theory. Lecture 1 The Atom and Nuclear Stability
Basic Nuclear Theory Lecture 1 The Atom and Nuclear Stability Introduction Nuclear power is made possible by energy emitted from either nuclear fission or nuclear fusion. Current nuclear power plants utilize
More informationChapter 22. Preview. Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem. Section 1 The Nucleus
Section 1 The Nucleus Preview Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem Section 1 The Nucleus Objectives Identify the properties of the nucleus of an atom. Explain
More informationThe Mystery of Dark Matter
The Mystery of Dark Matter Maxim Perelstein, LEPP/Cornell U. CIPT Fall Workshop, Ithaca NY, September 28 2013 Introduction Last Fall workshop focused on physics of the very small - elementary particles
More informationHypernuclei Production by K at rest
Hypernuclei Production by K at rest Germano Bonomi 1 Department of Mechanical and Industrial Engineering via Branze 38, Brescia, ITALY & INFN Pavia via Bassi 6, Pavia, ITALY The creation of a hypernucleus
More informationIntroduction to Modern Physics
SECOND EDITION Introduction to Modern Physics John D. McGervey Case Western Reserve University Academic Press A Subsidiary of Harcourt Brace Jovanovich Orlando San Diego San Francisco New York London Toronto
More informationMODERN PHYSICS Frank J. Blatt Professor of Physics, University of Vermont
MODERN PHYSICS Frank J. Blatt Professor of Physics, University of Vermont McGRAW-HILL, INC. New York St. Louis San Francisco Auckland Bogota Caracas Lisbon London Madrid Mexico Milan Montreal New Delhi
More informationRelativistic EOS for Supernova Simulations
Relativistic EOS for Supernova Simulations H. Shen Nankai University, Tianjin, China 申虹 In collaboration with H. Toki RCNP, Osaka University, Japan K. Sumiyoshi Numazu College of Technology, Japan K. Oyamatsu
More informationModels for Low-Temperature Helium Dimers and Trimers. Department of Chemistry, University of Michigan, Ann Arbor, Michigan,
Models for Low-Temperature Helium Dimers and Trimers LAWRENCE L. LOHR, S. M. BLINDER Department of Chemistry, University of Michigan, Ann Arbor, Michigan, 48109-1055 Received 10 April 001; revised 19 June
More informationThe Nuclear Many-Body problem. Lecture 3
The Nuclear Many-Body problem Lecture 3 Emergent phenomena at the drip lines. How do properties of nuclei change as we move towards the nuclear driplines? Many-body open quantum systems. Unification of
More informationPHYS 420: Astrophysics & Cosmology
PHYS 420: Astrophysics & Cosmology Dr Richard H. Cyburt Assistant Professor of Physics My office: 402c in the Science Building My phone: (304) 384-6006 My email: rcyburt@concord.edu My webpage: www.concord.edu/rcyburt
More informationHIGHER ORDER THERMAL CORRECTIONS TO PHOTON SELF ENERGY
HIGHER ORDER THERMAL CORRECTIONS TO PHOTON SELF ENERGY Mahnaz Q. Haseeb Physics Department COMSATS Institute of Information Technology Islamabad Outline Relevance Finite Temperature Effects One Loop Corrections
More informationComplex 2D Matrix Model and Internal Structure of Resonances
Complex 2D Matrix Model and Internal Structure of Resonances Kanabu Nawa (RIKEN) In collaboration with Sho Ozaki, Hideko Nagahiro, Daisuke Jido and Atsushi Hosaka [arxiv:1109.0426[hep-ph]] CONTENTS * Nature
More informationLecture 4: Nuclear Energy Generation
Lecture 4: Nuclear Energy Generation Literature: Prialnik chapter 4.1 & 4.2!" 1 a) Some properties of atomic nuclei Let: Z = atomic number = # of protons in nucleus A = atomic mass number = # of nucleons
More information1. What does this poster contain?
This poster presents the elementary constituents of matter (the particles) and their interactions, the latter having other particles as intermediaries. These elementary particles are point-like and have
More informationA Tour to the Stars. Some Compelling Questions
Some Compelling Questions A Tour to the Stars The chemical elements essential for life: How did they form? Where did they form? Stars: How are they born? How do they live? How do they die? The stellar
More information