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Livres sur le sujet « Energy distributions of desorbates »

Auteur : Grafiati
Publié le 21 décembre 2024

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1

Kay, M. J. Ion energy distributions. Manchester : UMIST, 1993.

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2

Fretwell, Tracey Ann. Monte Carlo simulation of energy intensity distributions for electron beam lithography. Manchester : University of Manchester, 1995.

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3

Hodge, Bri-Mathias. Solar ramping distributions over multiple timescales and weather patterns. Golden, Colo : National Renewable Energy Laboratory, 2011.

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4

J, Shainsky Lauri, dir. Biomass and nutrient distributions in central Oregon second-growth Ponderosa pine ecosystems. Portland, OR (333 S.W. First Avenue, P.O. Box 3890, Portland 97208-3890) : U.S. Dept. of Agriculture, Forest Service, Pacific Northwest Research Station, 1995.

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5

C, Popescu Cristina, Tuffs Richard J et SED2004 International Workshop on the Spectral Energy Distributions of Gas-Rich Galaxies (2004 : Heidelberg, Germany), dir. The spectral energy distributions of gas-rich galaxies : Confronting models with data : international workshop, Heidelberg, Germany, 4 - 8 October 2004. Melville, N.Y : American Institute of Physics, 2005.

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6

SED, 2004 (2004 Heidelberg Germany). The spectral energy distributions of gas-rich galaxies : Confronting models with data : international workshop, Heidelberg, Germany, 4-8 October 2004 : SED 2004 Heidelberg. [Melville, N.Y.] : American Institute of Physics, 2005.

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7

Andreo, P. Tables of charge and energy deposition distributions in elemental materials irradiated by plane-parallel electron beams with energies between 0.1 and 100 MeV. Osaka, Japan : Research Institute for Advanced Science and Technology, University of Osaka Prefecture (1-2 Gakuen-cho, Sakai, Osaka 593, Japan), 1992.

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8

Papanikolaou, N. Handbook of calculated electron momentum distributions, compton profiles, and x-ray form factors of elemental solids. Boca Raton : CRC Press, 1991.

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9

United States. Congress. House. Committee on Energy and Commerce. Subcommittee on Commerce, Consumer Protection, and Competitiveness. Long-term care insurance standards : Hearing before the Subcommittee on Commerce, Consumer Protection, and Competitiveness of the Committee on Energy and Commerce, House of Representatives, One Hundred Second Congress, first session, on H.R. 1205, H.R. 1916, and H.R. 2378, bills to regulate long-term care insurance policies, to allow tax-free distributions from IRA's for purchase of long-term care insurance by certain individuals, and to establish federal standards for long-term care insurance policies, October 24, 1991. Washington : U.S. G.P.O., 1992.

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10

National Aeronautics and Space Administration (NASA) Staff. Far-Infrared Spectral Energy Distributions of Quasars. Independently Published, 2018.

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11

Hao, Heng. Spectral Energy Distributions of Type 1 AGNs. 2011.

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12

Crombie, Michael Byrne. Hadronic energy distributions in deep-inelastic electron-proton scattering. 1994.

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13

National Aeronautics and Space Administration (NASA) Staff. Nuclear Fragmentation Energy and Momentum Transfer Distributions in Relativistic Heavy-Ion Collisions. Independently Published, 2018.

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14

Winterbon, K. Bruce. Ion Implantation Range and Energy Deposition Distributions : Volume 2 : Low Incident Ion Energies. Springer, 2013.

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15

Daniel, Robert George. Photoelectron angular and energy distributions from the resonant two-photon ionization of diatomic sodium. 1991.

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16

Atherton, James Vincent. A Monte Carlo study of dose distributions and energy imparted in computed tomography dosimetry phantoms. 1993.

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17

Atherton, James Vincent. A Monte Carlo study of dose distributions and energy imparted in computed tomography dosimetry phantoms. 1993.

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18

Fliszár, Sándor. Charge Distributions and Chemical Effects : A New Approach to the Electronic Structure and Energy of Molecules. Springer, 2011.

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19

Track structure model for radial distributions of electron spectra and event spectra from high-energy ions. Hampton, Va : National Aeronautics and Space Administration, Langley Research Center, 1998.

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20

National Aeronautics and Space Administration (NASA) Staff. Track Structure Model for Radial Distributions of Electron Spectra and Event Spectra from High-Energy Ions. Independently Published, 2018.

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21

Charge Distributions and Chemical Effects : A New Approach to the Electronic Structure and Energy of Molecules. Springer, 2011.

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22

Fairey, P. Latent and sensible load distributions in conventional and energy efficient residences, final report January 1983-Januar. Florida Solar Energy Center, 1986.

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23

Workshop on Hadron Structure Functions and Parton Distributions et Donald F. Geesaman. Proceedings of the Workshop on Hadron Structure Functions and Parton Distributions : Fermi National Accelerator Laboratory, 26-28 April, 1990. World Scientific Pub Co Inc, 1991.

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24

Proceedings of the Workshop on Hadron Structure Functions and Parton Distributions : Fermi National Accelerator Laboratory, 26-28 April 1990. World Scientific, 1990.

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25

The Spectral Energy Distributions of Gas-Rich Galaxies : Confronting Models with Data (AIP Conference Proceedings / Astronomy and Astrophysics). American Institute of Physics, 2005.

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26

Differential Equations with Applications to Vibrations and Waves (Mathematical-Physics for Science and Technology). CRC, 2009.

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27

Morawetz, Klaus. Simulations of Heavy-Ion Reactions with Nonlocal Collisions. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198797241.003.0023.

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The scenario of heavy-ion reactions around the Fermi energy is explored. The quantum BUU equation is solved numerically with and without nonlocal corrections and the effect of nonlocal corrections on experimental values is calculated. A practical recipe is presented which allows reproducing the correct asymptotes of scattering by acting on the point of closest approach. The better description of dynamical correlations by the nonlocal kinetic equation is demonstrated by an enhancement of the high-energy part of the particle spectra and the enhancement of mid-rapidity charge distributions. The time-resolved solution shows the enhancement of neck formation. It is shown that the dissipated energy increases due to the nonlocal collision scenario which is responsible for the observed effects and not due to the enhancement of collisions. As final result, a method is presented how to incorporate the effective mass and quasiparticle renormalisation with the help of the nonlocal simulation scenario.
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28

Levin, Frank S. The Hydrogen Atom and Its Colorful Photons. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780198808275.003.0010.

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The energies, kets and wave functions obtained from the Schrödinger equation for the hydrogen atom are examined in Chapter 9. Three quantum numbers are identified. The energies turn out to be the same as in the Bohr model, and an energy-level diagram appropriate to the quantum description is constructed. Graphs of the probability distributions are interpreted as the electron being in a “cloud” around the proton, rather than at a fixed position: the atom is fuzzy, not sharp-edged. The wavelengths of the five photons of the Balmer series are shown to be in the visible range. These photons are emitted when electrons transition from higher-excited states to the second lowest one, which means that electronic-type transitions underlie the presence of colors in our visible environment. The non-collapse of the atom, required by classical physics, is shown to arise from the structure of Schrödinger’s equation.
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29

Levin, Frank S. Quantum Boxes, Stringed Instruments. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780198808275.003.0008.

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Chapter 7 illustrates the results obtained by applying the Schrödinger equation to a simple pedagogical quantum system, the particle in a one-dimensional box. The wave functions are seen to be sine waves; their wavelengths are evaluated and used to calculate the quantized energies via the de Broglie relation. An energy-level diagram of some of the energies is constructed; on it are illustrations of the corresponding wave functions and probability distributions. The wave functions are seen to be either symmetric or antisymmetric about the midpoint of the line representing the box, thereby providing a lead-in to the later exploration of certain symmetry properties of multi-electron atoms. It is next pointed out that the Schrödinger equation for this system is identical to Newton’s equation describing the vibrations of a stretched musical string. The different meaning of the two solutions is discussed, as is the concept and structure of linear superpositions of them.
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