Atomic Spectra Atomic Structure
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Orbital Angular Momentum, R = 0, 1, 2,
Atomic Spectroscopy of Polyelectronic Atoms Atoms, Energy Levels and Spectroscopy Energy Levels in Atoms (13.2, 13.3, 13.4, 13.5) Coupling of Angular Momenta (13.7, 13.8) Term Symbols and Selection Rules (13.9) Russell-Saunders Coupling (13.9) Examples Hydrogen and Alkali Metal Atoms Helium Selection rules and other polyelectronic atoms Supplementary Notes Coupling of Angular Momenta Hyperfine Splitting Zeeman Interaction Stark Effect Atomic Spectroscopy Electronic spectroscopy is the study of absorption and emission transitions between electronic states in an atom or a molecule. Atomic spectroscopy is concerned with the electronic transitions in atoms, and is quite simple compared to electronic molecular spectroscopy. This is because atoms only have translational and electronic degrees of freedom, and sometime influenced by nuclear spin (molecules also have vibrations and rotations). Recall (Lecture 5) that for hydrogen and hydrogen-like ions (i.e., He+, Li2+, Be3+, etc.) with a single electron and a nucleus with charge +Ze, the hamiltonian is: £ 2 Ze 2 ,'& L2 & 2µ 4B,0r µ = (memp)/(me + mp) reduced mass e = 1.6021 × 10-19 C charge on an electron r = distance between +e and -e -12 2 2 -1 -3 ,0 = 8.854 × 10 C s kg m permitivity of free space For a polyelectronic atom, the hamiltonian becomes: 2 2 2 £ 2 Ze e ,'& j Li & j % j 2me i i 4B,0ri i<j 4B,0rij summed over i electrons. The new term describes coulombic repulsions between pairs of electrons which are distance rij apart (second term is coulombic attraction between nucleus and electrons) SCF Method The electron-electron repulsion term creates a many-body problem, in which the hamiltonian cannot be broken down into a sum of contributions from each electron - the result is that the Schroedinger equation cannot be solved exactly. -
Studies Absorption Or Emission Transitions Between Electronic States of Atoms Or Molecules
Chapter III: Atomic spectroscopy Electronic spectroscopy: studies absorption or emission transitions between electronic states of atoms or molecules. Atoms only electronic degrees of freedom (apart translation and nuclear spin), whereas molecules have, in addition, vibrational and rotational degrees of freedom. III.1 The periodic table For the hydrogen atom, and for the hydrogen-like ions (He+, Li++ ,…) , with a single electron in the field of a nucleus with charge +Ze, the hamiltonian is: (III.1) analogous to Equation (I.30) for the hydrogen atom, where the terms are explained. For a polyelectronic atom the hamiltonian becomes: (III.2) where the summation is over all electrons i. The first two terms are simply sums of terms like those for one electron in Equation (III.1). The third term is new and represents the Coulomb repulsions between all possible pairs of electrons distant of rij . The second term represents the Coulomb attraction between each electron and the nucleus at a distance ri . Because of the electron-electron repulsion term in Equation (III.2) the Hamiltonian cannot be broken down into a sum of contributions from each electron and the Schrödinger equation is no longer be solved exactly. Various approximate methods of solution have been devised of which the self-consistent field (SCF) method is one of the most useful. In it the Hamiltonian has the form: (III.3) He approximated the contributions to the potential energy due to electron repulsions as a sum of contributions from individual electrons. The Schrödinger equation is then soluble. Important effect of electron repulsions: removes the degeneracy of those orbitals. -
Quantum Mechanics and Merged Them Into a Coherent Theory, and Why the Mathematical Infrastructure of Quan- Tum Mechanics Has to Be As Complex As It Is
QuantumConceptsinPhysics Written for advanced undergraduates, physicists, and historians and philosophers of physics, this book tells the story of the development of our understanding of quantum phenomena through the extraordinary years of the first three decades of the twentieth century. Rather than following the standard axiomatic approach, this book adopts a histori- cal perspective, explaining clearly and authoritatively how pioneers such as Heisenberg, Schrodinger,¨ Pauli and Dirac developed the fundamentals of quantum mechanics and merged them into a coherent theory, and why the mathematical infrastructure of quan- tum mechanics has to be as complex as it is. The author creates a compelling narrative, providing a remarkable example of how physics and mathematics work in practice. The book encourages an enhanced appreciation of the interactions between mathematics, theory and experiment, helping the reader gain a deeper understanding of the development and content of quantum mechanics than with any other text at this level. Malcolm Longair is Emeritus Jacksonian Professor of Natural Philosophy and Director of Development at the Cavendish Laboratory, University of Cambridge. He has held many highly respected positions within physics and astronomy, and he has served on and chaired many international committees, boards and panels, working with both NASA and the European Space Agency. He has received much recognition for his work, including the Pilkington Prize of the University of Cambridge for Excellence in Teaching and a CBE in the millennium honours list for his services to astronomy and cosmology. His previous well- received books for Cambridge University Press include Theoretical Concepts in Physics (2003), The Cosmic Century: A History of Astrophysics and Cosmology (2005) and High Energy Astrophysics (2011).