Definitions and Units 263

Total Page:16

File Type:pdf, Size:1020Kb

Definitions and Units 263 Definitions and units 263 Definitions and units The following glossary is intended as a conveniently accessible source of technical terms used in context with ion tracks. It is compiled mainly on the basis of the references [1], [2], [3], [4], [5], [6]. [1] D.H. Menzel (editor): "Fundamental Formulas of Physics." Dover Publications, New York, 1960 [2] "Glossary of Terms used in Nuclear Science." British Standards Institution, B.S. 3455, 1962 [3] "The Radiochemical Manual." Amersham, the Radiochemical Centre, 1966 [4] Cohen, E., P. Giacomo: "Symbols, Units, Nomenclature and Fundamental Constants in Physics." International Union of Pure and Applied Physics (IUPAP), Revision 1987,67 pp. (1987). [5] Alan Isaacs (editor): "Concise Dictionary of Physics." Oxford University Press, pp. 1-295, 1985. [6] Hansen, J.W.: "Experimental Investigation of the Suitability of the Track Structure Theory in Describing the Relative Effectiveness of High-LET Irradiation of Physical Radiation Detectors." RiSl/l National Laboratory, DK-4000 Roskilde, Denmark; RiSl/l-R-507, (1984). absorbed dose, absorbed energy per unit mass. SI atoms of the element. The atomic number de­ unit is the Gray (Gy). I Gy = 1 J / fines the chemical properties of the element. kg = 104 erg / g = 6.25-1015 eV/g. atomic radius of hydrogen, ao = h2 / 4n2 m e2 = actuator, a device for inducing an action. 0.5292-10-8 cm. alpha particle, (a), the nucleus of a 4He atom con­ atomic weight (W), for a given specimen of an sisting of two protons and two neutrons. element, the mean weight of its atoms, ex­ pressed in either atomic mass units (physical areal density of targets, (Ps)' thickness-equivalent scale) or atomic weight units (chemical scale). of targets, Ps ;;; P d, where p is the mass density and d the target thickness, usually given in atomic weight unit (awu), one-twelfth of the mean mg / cm2. mass of the neutral atoms of naturally occurring carbon. areal dose (fluence), number of accumulated (recorded) particle tracks per unit surface area. A vogadro number, N A = 6.0220-1023 / mole, number of molecules per mole. asp~ct ratio, ratio between length and width of an ion track. bar, unit of pressure. 1 bar = lOS Pa = 750.19 torr. atom, a unit of matter consisting of a single nu­ barn, a unit of cross-section. 1 bam = 10-24 cm. cleus surrounded by one or more orbital elec­ Becquerel (Bq), unit of radioactivity, 1 Bq = trons. The number of electrons corresponds to 1 decay event / s. Official unit before 1986: the number of protons in the nucleus. 1 Curie (Ci) = 3.7-1010 decay events / s. atomic mass (A • u), mass of a nuclide measured beta particle, electron. in atomic mass units, where A = atomic mass Bohr magneton, JlB = e h / (4n me c) = number, and u = atomic mass unit. 9.2741 - 10-24 Joule pro Tesla. atomic mass number (A), mass number of a nu­ Bohr radius, ao = a / 4 n R~ = 0.529177-10-8 cm. clide, nucleon number, number of protons and a = fine structure constant, n = 3.1415, R~ = neutrons in the nuclide. A is the nearest integer Rydberg constant. to its atomic mass. Bohr velocity, Vo = 2n e 2 / h = a c = atomic mass unit (u), one-twelfth of the mass of a 2.1847-108 cm / s, where e electron charge, 27 = neutral atom of 12C, u = 1.6606-10- kg. h = Planck constant, a = fine structure con­ atomic number (2) of an element, nuclear charge stant, C = velocity of light. number, number of protons in the nucleus of the Boltzmann constant, k = R / N A = 1.3806-10-23 J 264 Defmitions and units fK = 1.3806.10-16 erg / K. R = molar gas con­ number, u = atomic mass unit, NA = Avogadro stant, N A = Avogadro constant. number, V rn = molar volume. Bragg peak: region of maximum energy loss of a density, number - (N), number of atoms per vol­ high energy ion traversing matter. ume element, N = P / (A u), where p = mass bremsstrahlung, the electromagnetic radiation re­ density, A = atomic mass number, u = atomic sulting from the retardation of charged particles. mass unit. calorie, unit of thermal energy, 1 calorie = dose, energy -, absorbed energy per unit mass. SI 4.18400 Joules. unit is the Gray (Gy). 1 Gy = 1 J / kg = 104 erg / g = 6.25.1015 eV / g. Radiation en­ capacitance, unit of capacitance is the Farad (F). 1 2 ergy deposited in a medium causes bond rupture, Farad = 1 Coulomb / Volt = 1 m- kg-I S4 N. radical formation, and physico- and chemical charge, electric -, given in units of Coulomb (C). changes, which are detectable in different ways. 9 1 C = 1 A s = 3.10 esu. dose equivalent, see Rem. A unit of biologically cross section of a nucleus, atom, or grain for a effective dose, defined as the absorbed dose in rad given radiation, that area perpendicular to the di­ multiplied by the quality factor - or relative bi­ rection of the radiation attributed geometrically ological effectiveness (RBE) -. For all x rays, for its interaction with the radiation; or, in other y rays, ~- rays and ~+ rays encountered from ra­ words, the number of interactions per unit time dioisotopes the RBE is 1. For a-particles and divided by the radiation flux and the number of heavier ions the RBE can be different from 1, scattering objects present. The cross section of a depending on the ion charge and its velocity. nucleus is roughly of the order of 10-24 cm, of an 16 Dose-response: relation between the deposited en­ atom roughly of the order of 10- cm. ergy per volume, in other words the dose, and Coulomb (C), the unit of electric charge. The the observed effect, which may for example be charge of 1 Coulomb corresponds to the charge optical absorption, survival of cells, etc .. For of an electrical current of 1 Ampere flowing dur­ many physical radiation recorders, irradiated by ing 1 second. 1 C = 1 A s. 1 Coulomb corre­ low-LET radiation, the dose-response function is sponds to the charge of 0.62414.1019 electrons. approximately linear at low doses and saturates Coulomb barrier of nuclear reactions, minimum exponentially at high doses and the response is a energy of projectile ions required for inducing single-valued function of dose within a large nuclear reactions. The coulomb barrier corre­ range of initial photon and electron energies. sponds to a specific energy in the range between dyne, unit of force, 1 dyne = 1 g cm S-2. 1 and 10 MeV/nucleon, depending on the projec­ electron, the negatively charged particle which tile/target combination. forms a constituent of all atoms. Electron charge Coulomb explosion, origin of the atomic collision e = - 1.60219.10-19 Coulomb = -4.8032.10-10 cascade.in solids, caused by the passage of a esu. Electron mass me = 9.1095.10-28 g. rapidly moving ion and leading to displaced Classical electron radius r e = e 2 / (me c2 ) = atoms and ultimately to a latent track. 2.8179.10-13 cm. Coulomb per kilogramm (C / kg), "unit" of ab­ electron volt (eV), a unit of energy equal to the ki­ sorbed dose, defined as total electron charge gen­ netic energy acquired by an electron when accel­ erated during - preferentially x or y - irradia­ erated through a potential difference of 1 volt. 1 tion. Official unit before 1986: 1 Roentgen = eV = 1.602.10-12 erg = 1.602.10-19 Joule. 4 2.58.10- C / kg. One Roentgen produces eV, electron volt. 1 eV = 1.602.10-12 erg. 3.7·1010 ion pairs in air at standard pressure and temperature. element, matter consisting of atoms having the same atomic number Z. Curie (Ci), old unit of activity. One curie corre­ sponds to 3.7.1010 nuclear transformations per energy, a measure of a system's ability to do work. second. 1 Ci = 3.7·1010 Bq. Potential energy is the energy stored in a body or system as a consequence of its position, shape, De Broglie wavelength of a particle, A = h / p , or state. Kinetic energy is energy of motion and where h = Planck constant, and p is the particle is usually defined as the work that will be done momentum. The magnitude of the associated by the body when it is brought to rest. For a wave vector is k == 21t / A = 21t P / h. body of mass m having a speed v, the kinetic delta ray: secondary and higher order electrons gen­ energy is m v2/2. The rotational kinetic energy erated by a primary radiation. This term is anal­ of a body with an angular velocity 0) is I 0)2/ 2, ogous to the terms alpha-ray and beta-ray. where I is its moment of inertia. density, electron - (Ne)' number of electrons per energy units, 1 erg = I g cm2 S-2. 1 J = 107 erg = volume element, Ne = Z P / (A u), where Z = 0.239 calories. 1 erg = 6.25.1011 eV. 1 eV = nuclear charge number, p = mass density, A = 1.6.10-12 erg. 1 kJ / mole = 1.038.10-2 eV / atomic mass number, u = atomic mass unit. molecule. density, mass - (p), mass per volume element, energy, free -, corresponds to the following two p = Au NA / V rn , where A = atomic mass thermodynamic functions. Gibbs free energy, Definitions and units 265 G=H-TS, is the energy liberated or absorbed in a ture T at which the energy is absorbed, reversible process at constant pressure and con­ t1S=t1Q/T.
Recommended publications
  • Glossary Physics (I-Introduction)
    1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay.
    [Show full text]
  • Quantum Theory of the Hydrogen Atom
    Quantum Theory of the Hydrogen Atom Chemistry 35 Fall 2000 Balmer and the Hydrogen Spectrum n 1885: Johann Balmer, a Swiss schoolteacher, empirically deduced a formula which predicted the wavelengths of emission for Hydrogen: l (in Å) = 3645.6 x n2 for n = 3, 4, 5, 6 n2 -4 •Predicts the wavelengths of the 4 visible emission lines from Hydrogen (which are called the Balmer Series) •Implies that there is some underlying order in the atom that results in this deceptively simple equation. 2 1 The Bohr Atom n 1913: Niels Bohr uses quantum theory to explain the origin of the line spectrum of hydrogen 1. The electron in a hydrogen atom can exist only in discrete orbits 2. The orbits are circular paths about the nucleus at varying radii 3. Each orbit corresponds to a particular energy 4. Orbit energies increase with increasing radii 5. The lowest energy orbit is called the ground state 6. After absorbing energy, the e- jumps to a higher energy orbit (an excited state) 7. When the e- drops down to a lower energy orbit, the energy lost can be given off as a quantum of light 8. The energy of the photon emitted is equal to the difference in energies of the two orbits involved 3 Mohr Bohr n Mathematically, Bohr equated the two forces acting on the orbiting electron: coulombic attraction = centrifugal accelleration 2 2 2 -(Z/4peo)(e /r ) = m(v /r) n Rearranging and making the wild assumption: mvr = n(h/2p) n e- angular momentum can only have certain quantified values in whole multiples of h/2p 4 2 Hydrogen Energy Levels n Based on this model, Bohr arrived at a simple equation to calculate the electron energy levels in hydrogen: 2 En = -RH(1/n ) for n = 1, 2, 3, 4, .
    [Show full text]
  • Principal, Azimuthal and Magnetic Quantum Numbers and the Magnitude of Their Values
    268 A Textbook of Physical Chemistry – Volume I Principal, Azimuthal and Magnetic Quantum Numbers and the Magnitude of Their Values The Schrodinger wave equation for hydrogen and hydrogen-like species in the polar coordinates can be written as: 1 휕 휕휓 1 휕 휕휓 1 휕2휓 8휋2휇 푍푒2 (406) [ (푟2 ) + (푆푖푛휃 ) + ] + (퐸 + ) 휓 = 0 푟2 휕푟 휕푟 푆푖푛휃 휕휃 휕휃 푆푖푛2휃 휕휙2 ℎ2 푟 After separating the variables present in the equation given above, the solution of the differential equation was found to be 휓푛,푙,푚(푟, 휃, 휙) = 푅푛,푙. 훩푙,푚. 훷푚 (407) 2푍푟 푘 (408) 3 푙 푘=푛−푙−1 (−1)푘+1[(푛 + 푙)!]2 ( ) 2푍 (푛 − 푙 − 1)! 푍푟 2푍푟 푛푎 √ 0 = ( ) [ 3] . exp (− ) . ( ) . ∑ 푛푎0 2푛{(푛 + 푙)!} 푛푎0 푛푎0 (푛 − 푙 − 1 − 푘)! (2푙 + 1 + 푘)! 푘! 푘=0 (2푙 + 1)(푙 − 푚)! 1 × √ . 푃푚(퐶표푠 휃) × √ 푒푖푚휙 2(푙 + 푚)! 푙 2휋 It is obvious that the solution of equation (406) contains three discrete (n, l, m) and three continuous (r, θ, ϕ) variables. In order to be a well-behaved function, there are some conditions over the values of discrete variables that must be followed i.e. boundary conditions. Therefore, we can conclude that principal (n), azimuthal (l) and magnetic (m) quantum numbers are obtained as a solution of the Schrodinger wave equation for hydrogen atom; and these quantum numbers are used to define various quantum mechanical states. In this section, we will discuss the properties and significance of all these three quantum numbers one by one. Principal Quantum Number The principal quantum number is denoted by the symbol n; and can have value 1, 2, 3, 4, 5…..∞.
    [Show full text]
  • Further Quantum Physics
    Further Quantum Physics Concepts in quantum physics and the structure of hydrogen and helium atoms Prof Andrew Steane January 18, 2005 2 Contents 1 Introduction 7 1.1 Quantum physics and atoms . 7 1.1.1 The role of classical and quantum mechanics . 9 1.2 Atomic physics—some preliminaries . .... 9 1.2.1 Textbooks...................................... 10 2 The 1-dimensional projectile: an example for revision 11 2.1 Classicaltreatment................................. ..... 11 2.2 Quantum treatment . 13 2.2.1 Mainfeatures..................................... 13 2.2.2 Precise quantum analysis . 13 3 Hydrogen 17 3.1 Some semi-classical estimates . 17 3.2 2-body system: reduced mass . 18 3.2.1 Reduced mass in quantum 2-body problem . 19 3.3 Solution of Schr¨odinger equation for hydrogen . ..... 20 3.3.1 General features of the radial solution . 21 3.3.2 Precisesolution.................................. 21 3.3.3 Meanradius...................................... 25 3.3.4 How to remember hydrogen . 25 3.3.5 Mainpoints.................................... 25 3.3.6 Appendix on series solution of hydrogen equation, off syllabus . 26 3 4 CONTENTS 4 Hydrogen-like systems and spectra 27 4.1 Hydrogen-like systems . 27 4.2 Spectroscopy ........................................ 29 4.2.1 Main points for use of grating spectrograph . ...... 29 4.2.2 Resolution...................................... 30 4.2.3 Usefulness of both emission and absorption methods . 30 4.3 The spectrum for hydrogen . 31 5 Introduction to fine structure and spin 33 5.1 Experimental observation of fine structure . ..... 33 5.2 TheDiracresult ..................................... 34 5.3 Schr¨odinger method to account for fine structure . 35 5.4 Physical nature of orbital and spin angular momenta .
    [Show full text]
  • 1.2 Formulation of the Schrödinger Equation for the Hydrogen Atom
    2 1 Hydrogen orbitals 1.2 Formulation of the Schrodinger¨ equation for the hydrogen atom In this initial treatment, we will make some practical approximations and simplifi- cations. Since we are for the moment only trying to establish the general form of the hydrogenic wave functions, this will suffice. To start with, we will assume that the nucleus has zero extension. We place the origin at its position, and we ignore the centre-of-mass motion. This reduces the two-body problem to a single particle, the electron, moving in a central-field potential. To take the finite mass of the nu- cleus into account, we replace the electron mass with the reduced mass, m, of the two-body problem. Moreover, we will in this chapter ignore the effect on the wave function of relativistic effects, which automatically implies that we ignore the spins of the electron and of the nucleus. This makes us ready to formulate the Hamilto- nian. The potential is the classical Coulomb interaction between two particles of op- posite charges. With spherical coordinates, and with r as the radial distance of the electron from the origin, this is: Ze2 V(r) = − ; (1.1) 4pe0 r with Z being the charge state of the nucleus. The Schrodinger¨ equation is: h¯ 2 − ∇2y(r) +V(r)y = Ey(r) ; (1.2) 2m where the Laplacian in spherical coordinates is: 1 ¶ ¶ 1 ¶ ¶ 1 ¶ 2 ∇2 = r2 + sinq + : (1.3) r2 ¶r ¶r r2 sinq ¶q ¶q r2 sin2 q ¶j2 Since the potential is purely central, the solution to (1.2) can be factorised into a radial and an angular part, y(r;q;j) = R(r)Y(q;j).
    [Show full text]
  • Mass Defect & Binding Energy the Nuclear Reaction Used by Stars To
    Mass Defect & Binding Energy The nuclear reaction used by stars to produce energy (for most of their lives anyway) is the proton proton cycle: 1H + 1H → 2H + e– + ν 1H + 2H → 3He + γ 1H + 3He → 4He + e– + ν or 3He + 3He → 4He + 1H + 1H In the overall reaction, 4 hydrogen-1 atoms combine to form 1 He-4 atom plus some other parti- cles and energy. But examining the atomic masses of hydrogen and helium on the periodic table, the mass of four hydrogen atoms is greater than the mass of one helium atom. Subtracting the dif- ference gives: 4 × 1.007825 – 4.002603 = 0.028697 amu This difference is called the mass defect and measures the amount of “binding energy” stored in an atom’s nucleus or the amount of energy required to break up the nucleus back into the individ- ual protons and neutrons. In general, the mass defect is calculated by summing the mass of protons, neutrons, and electrons in an atom, and subtracting the atom’s actual atomic mass. The general formula is: Md = Z mp + N mn - Ma where Z is the atomic number, N is the number of neutrons in the atom, and Ma is the actual mea- sured mass of the atom. Placing Md into Einstein's equation for relating mass and energy gives the energy release from forming the atom from its constituent particles: 2 E = Md c where c is the speed of light (≈ 3.00 × 108 m/s). For example, using the information from the reac- tion above, one can deduce that to form 1 kg of 4He from requires 1.0073 kg of 1H.
    [Show full text]
  • Fission and Fusion Can Yield Energy
    Nuclear Energy Nuclear energy can also be separated into 2 separate forms: nuclear fission and nuclear fusion. Nuclear fusion is the splitting of large atomic nuclei into smaller elements releasing energy, and nuclear fusion is the joining of two small atomic nuclei into a larger element and in the process releasing energy. The mass of a nucleus is always less than the sum of the individual masses of the protons and neutrons which constitute it. The difference is a measure of the nuclear binding energy which holds the nucleus together (Figure 1). As figures 1 and 2 below show, the energy yield from nuclear fusion is much greater than nuclear fission. Figure 1 2 Nuclear binding energy = ∆mc For the alpha particle ∆m= 0.0304 u which gives a binding energy of 28.3 MeV. (Figure from: http://hyperphysics.phy-astr.gsu.edu/hbase/nucene/nucbin.html ) Fission and fusion can yield energy Figure 2 (Figure from: http://hyperphysics.phy-astr.gsu.edu/hbase/nucene/nucbin.html) Nuclear fission When a neutron is fired at a uranium-235 nucleus, the nucleus captures the neutron. It then splits into two lighter elements and throws off two or three new neutrons (the number of ejected neutrons depends on how the U-235 atom happens to split). The two new atoms then emit gamma radiation as they settle into their new states. (John R. Huizenga, "Nuclear fission", in AccessScience@McGraw-Hill, http://proxy.library.upenn.edu:3725) There are three things about this induced fission process that make it especially interesting: 1) The probability of a U-235 atom capturing a neutron as it passes by is fairly high.
    [Show full text]
  • The Principal Quantum Number the Azimuthal Quantum Number The
    To completely describe an electron in an atom, four quantum numbers are needed: energy (n), angular momentum (ℓ), magnetic moment (mℓ), and spin (ms). The Principal Quantum Number This quantum number describes the electron shell or energy level of an atom. The value of n ranges from 1 to the shell containing the outermost electron of that atom. For example, in caesium (Cs), the outermost valence electron is in the shell with energy level 6, so an electron incaesium can have an n value from 1 to 6. For particles in a time-independent potential, as per the Schrödinger equation, it also labels the nth eigen value of Hamiltonian (H). This number has a dependence only on the distance between the electron and the nucleus (i.e. the radial coordinate r). The average distance increases with n, thus quantum states with different principal quantum numbers are said to belong to different shells. The Azimuthal Quantum Number The angular or orbital quantum number, describes the sub-shell and gives the magnitude of the orbital angular momentum through the relation. ℓ = 0 is called an s orbital, ℓ = 1 a p orbital, ℓ = 2 a d orbital, and ℓ = 3 an f orbital. The value of ℓ ranges from 0 to n − 1 because the first p orbital (ℓ = 1) appears in the second electron shell (n = 2), the first d orbital (ℓ = 2) appears in the third shell (n = 3), and so on. This quantum number specifies the shape of an atomic orbital and strongly influences chemical bonds and bond angles.
    [Show full text]
  • Importance of Hydrogen Atom
    Hydrogen Atom Dragica Vasileska Arizona State University Importance of Hydrogen Atom • Hydrogen is the simplest atom • The quantum numbers used to characterize the allowed states of hydrogen can also be used to describe (approximately) the allowed states of more complex atoms – This enables us to understand the periodic table • The hydrogen atom is an ideal system for performing precise comparisons of theory and experiment – Also for improving our understanding of atomic structure • Much of what we know about the hydrogen atom can be extended to other single-electron ions – For example, He+ and Li2+ Early Models of the Atom • ’ J.J. Thomson s model of the atom – A volume of positive charge – Electrons embedded throughout the volume • ’ A change from Newton s model of the atom as a tiny, hard, indestructible sphere “ ” watermelon model Experimental tests Expect: 1. Mostly small angle scattering 2. No backward scattering events Results: 1. Mostly small scattering events 2. Several backward scatterings!!! Early Models of the Atom • ’ Rutherford s model – Planetary model – Based on results of thin foil experiments – Positive charge is concentrated in the center of the atom, called the nucleus – Electrons orbit the nucleus like planets orbit the sun ’ Problem: Rutherford s model “ ” ’ × – The size of the atom in Rutherford s model is about 1.0 10 10 m. (a) Determine the attractive electrical force between an electron and a proton separated by this distance. (b) Determine (in eV) the electrical potential energy of the atom. “ ” ’ × – The size of the atom in Rutherford s model is about 1.0 10 10 m. (a) Determine the attractive electrical force between an electron and a proton separated by this distance.
    [Show full text]
  • Atomic Weights and Isotopic Abundances*
    Pure&App/. Chem., Vol. 64, No. 10, pp. 1535-1543, 1992. Printed in Great Britain. @ 1992 IUPAC INTERNATIONAL UNION OF PURE AND APPLIED CHEMISTRY INORGANIC CHEMISTRY DIVISION COMMISSION ON ATOMIC WEIGHTS AND ISOTOPIC ABUNDANCES* 'ATOMIC WEIGHT' -THE NAME, ITS HISTORY, DEFINITION, AND UNITS Prepared for publication by P. DE BIEVRE' and H. S. PEISER2 'Central Bureau for Nuclear Measurements (CBNM), Commission of the European Communities-JRC, B-2440 Geel, Belgium 2638 Blossom Drive, Rockville, MD 20850, USA *Membership of the Commission for the period 1989-1991 was as follows: J. R. De Laeter (Australia, Chairman); K. G. Heumann (FRG, Secretary); R. C. Barber (Canada, Associate); J. CCsario (France, Titular); T. B. Coplen (USA, Titular); H. J. Dietze (FRG, Associate); J. W. Gramlich (USA, Associate); H. S. Hertz (USA, Associate); H. R. Krouse (Canada, Titular); A. Lamberty (Belgium, Associate); T. J. Murphy (USA, Associate); K. J. R. Rosman (Australia, Titular); M. P. Seyfried (FRG, Associate); M. Shima (Japan, Titular); K. Wade (UK, Associate); P. De Bi&vre(Belgium, National Representative); N. N. Greenwood (UK, National Representative); H. S. Peiser (USA, National Representative); N. K. Rao (India, National Representative). Republication of this report is permitted without the need for formal IUPAC permission on condition that an acknowledgement, with full reference together with IUPAC copyright symbol (01992 IUPAC), is printed. Publication of a translation into another language is subject to the additional condition of prior approval from the relevant IUPAC National Adhering Organization. ’Atomic weight‘: The name, its history, definition, and units Abstract-The widely used term “atomic weight” and its acceptance within the international system for measurements has been the subject of debate.
    [Show full text]
  • Electron Binding Energy for Atoms: Relativistic Corrections
    Electron binding energy for atoms : relativistic corrections I.K. Dmitrieva, G.I. Plindov To cite this version: I.K. Dmitrieva, G.I. Plindov. Electron binding energy for atoms : relativistic corrections. Journal de Physique, 1982, 43 (11), pp.1599-1605. 10.1051/jphys:0198200430110159900. jpa-00209542 HAL Id: jpa-00209542 https://hal.archives-ouvertes.fr/jpa-00209542 Submitted on 1 Jan 1982 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. J. Physique 43 (1982) 1599-1605 NOVEMBRE 1982,1 1599 Classification Physics Abstracts 31.10 - 31.20L Electron binding energy for atoms : relativistic corrections I. K. Dmitrieva (*) and G. I. Plindov (**) (*) A. V. Luikov Heat and Mass Transfer Institute, Byelorussian Academy of Sciences, Minsk, U.S.S.R. (**) Nuclear Power Engineering Institute, Byelorussian Academy of Sciences, Minsk, U.S.S.R. (Reçu le 13 avril 1982, accepti le 9 juillet 1982) Résumé. - L’énergie de liaison pour un atome de degré d’ionisation arbitraire est trouvée dans le cadre de la théorie statistique tenant compte de l’inhomogénéité de la densité électronique. La méthode de Schwinger per- met d’obtenir la dépendance analytique de la correction relativiste en fonction du nombre d’électrons N et de la charge nucléaire Z.
    [Show full text]
  • Nuclear Criticality Safety Engineer Training Module 1 1
    Nuclear Criticality Safety Engineer Training Module 1 1 Introductory Nuclear Criticality Physics LESSON OBJECTIVES 1) to introduce some background concepts to engineers and scientists who do not have an educational background in nuclear engineering, including the basic ideas of moles, atom densities, cross sections and nuclear energy release; 2) to discuss the concepts and mechanics of nuclear fission and the definitions of fissile and fissionable nuclides. NUCLEAR CRITICALITY SAFETY The American National Standard for Nuclear Criticality Safety in Operations with Fissionable Materials Outside Reactors, ANSI/ANS-8.1 includes the following definition: Nuclear Criticality Safety: Protection against the consequences of an inadvertent nuclear chain reaction, preferably by prevention of the reaction. Note the words: nuclear - related to the atomic nucleus; criticality - can it be controlled, will it run by itself; safety - protection of life and property. DEFINITIONS AND NUMBERS What is energy? Energy is the ability to do work. What is nuclear energy? Energy produced by a nuclear reaction. What is work? Work is force times distance. 1 Developed for the U. S. Department of Energy Nuclear Criticality Safety Program by T. G. Williamson, Ph.D., Westinghouse Safety Management Solutions, Inc., in conjunction with the DOE Criticality Safety Support Group. NCSET Module 1 Introductory Nuclear Criticality Physics 1 of 18 Push a car (force) along a road (distance) and the car has energy of motion, or kinetic energy. Climb (force) a flight of steps (distance) and you have energy of position relative to the first step, or potential energy. Jump down the stairs or out of a window and the potential energy is changed to kinetic energy as you fall.
    [Show full text]