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Books on the topic 'Nucleu'

Author: Grafiati
Published: 9 March 2023
Last updated: 10 March 2023

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1

Wilson, John W. Nucleon-nucleus interaction data base: Total nuclear and absorption cross sections. Hampton, Va: Langley Research Center, 1988.

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2

1940-, Wilson John W., and United States. National Aeronautics and Space Administration. Scientific and Technical Information Division., eds. Nucleon-nucleus interaction data base: Total nuclear and absorption cross section. [Washington, D.C.]: National Aeronautics and Space Administration, Scientific and Technical Information Division, 1988.

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3

1940-, Wilson John W., and United States. National Aeronautics and Space Administration. Scientific and Technical Information Division., eds. Nucleon-nucleus interaction data base: Total nuclear and absorption cross section. [Washington, D.C.]: National Aeronautics and Space Administration, Scientific and Technical Information Division, 1988.

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4

1940-, Wilson John W., and United States. National Aeronautics and Space Administration. Scientific and Technical Information Division., eds. Nucleon-nucleus interaction data base: Total nuclear and absorption cross section. [Washington, D.C.]: National Aeronautics and Space Administration, Scientific and Technical Information Division, 1988.

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5

Antonov, Anton Nikolaev, Peter Edward Hodgson, and Ivan Zhelyazkov Petkov. Nucleon Correlations in Nuclei. Berlin, Heidelberg: Springer Berlin Heidelberg, 1993. http://dx.doi.org/10.1007/978-3-642-77766-0.

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6

Antonov, Anton Nikolaev. Nucleon Correlations in Nuclei. Berlin, Heidelberg: Springer Berlin Heidelberg, 1993.

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7

E, Hodgson P., and Petkov I. Zh, eds. Nucleon correlations in nuclei. Berlin: Springer-Verlag, 1993.

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8

International Conference on Antinucleon- and Nucleon-Nucleus Interactions (1985 Telluride, Colo.). Antinucleon- and nucleon-nucleus interactions. New York: Plenum Press, 1985.

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9

Sitenko, A. G. Theory of nucleus: Nuclear structure and nuclear interaction. Dordrecht: Kluwer Academic, 1997.

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10

Sitenko, A. G. Theory of Nucleus: Nuclear Structure and Nuclear Interaction. Dordrecht: Springer Netherlands, 1997.

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11

Peña, M. Teresa, Alfred Stadler, Ana M. Eiró, and Jiří Adam, eds. Nuclear Dynamics: From Quarks to Nuclei. Vienna: Springer Vienna, 2003. http://dx.doi.org/10.1007/978-3-7091-6014-5.

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12

Bradamante, F., J. M. Richard, and R. Klapisch, eds. Antiproton-Nucleon and Antiproton-Nucleus Interactions. Boston, MA: Springer US, 1990. http://dx.doi.org/10.1007/978-1-4613-0595-8.

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13

International, School of Physics with Low Energy Antiprotons on Antiproton-Nucleon and Antiproton-Nucleus Interactions (3rd 1988 Erice Italy). Antiproton-nucleon and antiproton-nucleus interactions. New York: Plenum Press, 1990.

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14

W, Townsend Lawrence, Cucinotta Francis A, and Langley Research Center, eds. Transport model of nucleon-nucleus reaction. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1986.

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15

Antonov, A. N. Nucleon momentum and density distributions in nuclei. Oxford: Clarendon Press, 1988.

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16

Tripathi, Ram K. A Simple method for nucleon-nucleon cross sections in a nucleus. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1999.

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17

A, Cucinotta Francis, Wilson John W. 1940-, and Langley Research Center, eds. A simple method for nucleon-nucleon cross sections in a nucleus. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1999.

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18

L, James Thomas, ed. Nuclear magnetic resonance and nucleic acids. San Diego: Academic Press, 1995.

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19

Nucleus: Reconnecting science and religion in the nuclear age. Santa Fe, N.M: Bear, 1987.

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20

The nucleus. Cold Spring Harbor, N.Y: Cold Spring Harbor Laboratory Press, 2011.

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21

Heyde, Kris. From Nucleons to the Atomic Nucleus: Perspectives in Nuclear Physics. Berlin, Heidelberg: Springer Berlin Heidelberg, 1998.

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22

Heyde, Kris L. G. From nucleons to the atomic nucleus: Perspectives in nuclear physics. Berlin: Springer, 1998.

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23

Magill, Joseph, Heinrich Schwoerer, and Burgard Beleites. Lasers and nuclei: Applications of ultrahigh intensity lasers in nuclear science. Berlin: Springer, 2011.

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24

Rho, Mannque. Chiral nuclear dynamics II: From quarks to nuclei to compact stars. Singapore: World Scientific, 2008.

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25

A, Barraco I. Robin, ed. Nucleus of the solitary tract. Boca Raton: CRC Press, 1994.

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26

Redondo, Daniel Galaviz. Systematic study of [alpha]-nucleus potentials for neutron deficient nuclei and its astrophysical applications. Aachen: Shaker, 2004.

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27

Carpathian Summer School of Physics (2005 Mamaia, Romania and Constanța, Romania). Exotic nuclei and nuclear/particle astrophysics: Mamaia-Constanta, Romania, 13-24 June 2005 : proceedings of the Carpathian Summer School of Physics 2005. Edited by Trache L, Stoica S, and Tribble Robert E. Hackensack, NJ: World Scientific, 2006.

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28

Exotic nuclei and nuclear/particle astrophysics: Mamaia-Constanta, Romania, 13-24 June 2005 : proceedings of the Carpathian Summer School of Physics 2005. Singapore: World Scientific, 2007.

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29

L, Trache, and Stoica S, eds. Exotic nuclei and nuclear/particle astrophysics (II): Proceedings of the Carpathian Summer School of Physics 2007 : Sinaia, Romania, 20-31 August 2007. Melville, N.Y: American Institute of Physics, 2008.

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30

Close, Frank. 7. Exotic nuclei. Oxford University Press, 2015. http://dx.doi.org/10.1093/actrade/9780198718635.003.0007.

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‘Exotic nuclei’ discusses halo nuclei, borromean nuclei, hypernuclei, strange matter, and antimatter. Unstable isotopes with a larger excess of neutrons, or an excess of protons may form halos around a central core—halo nuclei or borromean structures, which have short half-lives, typically of the order of milliseconds. If a quark in a neutron or proton is replaced by a strange quark, the resulting particle carries the property of strangeness, and is generically known as a ‘hyperon’. A hypernucleus is formed when a hyperon replaces a nucleon within a nucleus. Antimatter exists in quantum theory, but there seems no evidence that it occurs in practice in the observable universe.
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31

Glazov, M. M. Electron Spin Relaxation Beyond the Hyperfine Interaction. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198807308.003.0008.

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Here, some prospects for future studies in the field of electron and nuclear spin dynamics are outlined. In contrast to previous chapters where the electron interaction with multitude of nuclei was discussed, in Chapter 8 particular emphasis is put on a situation where hyperfine interaction is so strong that it leads to a qualitative rear rangement of the energy spectrum resulting in coherent excitation transfer between electron and nucleus. The strong coupling between the spin of the charge carrier and of the nucleus is realized; e.g., in the case of deep impurity centers in semiconductors or in isotopically purified systems. We also discuss the effect of the nuclear spin polaron; that is, the ordered state, where the carrier spin orientation results in alignment of spins of the nucleus interacting with the electron or hole. Such problems have been briefly discussed in the literature but, in our opinion, call for in-depth investigation.
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32

Glazov, M. M. Hyperfine Interaction of Electron and Nuclear Spins. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198807308.003.0004.

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This chapter discusses the key interaction–hyperfine coupling–which underlies most of phenomena in the field of electron and nuclear spin dynamics. This interaction originates from magnetic interaction between the nuclear and electron spins. For conduction band electrons in III–V or II–VI semiconductors, it is reduced to a Fermi contact interaction whose strength is proportional to the probability of finding an electron at the nucleus. A more complex situation is realized for valence band holes where hole Bloch functions vanish at the nuclei. Here the hyperfine interaction is of the dipole–dipole type. The modification of the hyperfine coupling Hamiltonian in nanosystems is also analyzed. The chapter contains also an overview of experimental data aimed at determination of the hyperfine interaction parameters in semiconductors and semiconductor nanostructures.
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33

Hancock, Ronald. Nucleus : Volume 1: Nuclei and Subnuclear Components. Humana Press, 2010.

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34

(Editor), Catherine Olmer, ed. Antinucleon-And-Nucleon-Nucleus Interaction. Plenum Pub Corp, 1986.

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35

Sitenko, A., and V. Tartakovskii. Theory of Nucleus: Nuclear Structure and Nuclear Interaction. Springer, 2012.

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36

Stuewer, Roger H. The Quantum-Mechanical Nucleus. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198827870.003.0005.

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Rutherford extended his satellite model to encompass an explanation of the alpha decay of radioactive nuclei, which was abruptly disproven in the summer of 1928 by Russian theoretical physicist George Gamow, while visiting Max Born’s institute in Göttingen, and simultaneously by English theoretical physicist Ronald Gurney and American theoretical physicist Edward Condon at Princeton University, who showed that alpha decay is a quantum-mechanical tunneling phenomenon. That December, Gamow, now in Bohr’s institute in Copenhagen, also conceived the liquid-drop model of the nucleus, which he presented in January 1929 at a meeting of the Royal Society in London, and which he discussed that April at the first of Bohr’s annual conferences in Copenhagen. He developed that model further in the 1929–30 academic year at the Cavendish and in the 1930–1 academic year in Copenhagen, where he also wrote the first monograph on theoretical nuclear physics in which he cleverly expressed his doubt that electrons are present in nuclei.
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37

Glazov, M. M. Dynamical Nuclear Polarization. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198807308.003.0005.

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The transfer of nonequilibrium spin polarization between the electron and nuclear subsystems is studied in detail. Usually, a thermal orientation of nuclei in magnetic field is negligible due to their small magnetic moments, but if electron spins are optically oriented, efficient nuclear spin polarization can occur. The microscopic approach to the dynamical nuclear polarization effect based on the kinetic equation method, along with a phenomenological but very powerful description of dynamical nuclear polarization in terms of the nuclear spin temperature concept is given. In this way, one can account for the interaction between neighbouring nuclei without solving a complex many-body problem. The hyperfine interaction also induces the feedback of polarized nuclei on the electron spin system giving rise to a number of nonlinear effects: bistability of nuclear spin polarization and anomalous Hanle effect, dragging and locking of optical resonances in quantum dots. Theory is illustrated by experimental data on dynamical nuclear polarization.
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38

Richard, J. M., F. Bradamante, and R. Klapisch. Antiproton-Nucleon and Antiproton-Nucleus Interactions. Springer London, Limited, 2013.

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39

(Editor), S. Stoica, L. Trache (Editor), and R. E. Tribble (Editor), eds. Exotic Nuclei and Nuclear/Particle Astrophysics. World Scientific Publishing Company, 2006.

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40

Bradamante, F., J. M. Richard, and R. Klapisch. Antiproton-Nucleon and Antiproton-Nucleus Interactions. Springer, 2013.

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41

Richard, J. M., F. Bradamante, and R. Klapisch. Antiproton-Nucleon and Antiproton-Nucleus Interactions. Springer, 2011.

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42

Hamkalo, Barbara A., and Sarah C. Elgin. Functional Organization of the Nucleus: A Laboratory Guide. Elsevier Science & Technology Books, 1992.

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43

Saha, Prasenjit, and Paul A. Taylor. Nuclear Fusion in Stars. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198816461.003.0006.

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This chapter enumerates some of the many nuclear reactions in stars. It focuses on a general principle: nuclear fusion requires overcoming the Coulomb barrier between nuclei, which is possible through the relatively infrequent process of quantum tunnelling. The tunnelling probability depends on the atomic num-bers and mass numbers of the nuclei involved, and also on their relative speed. These translate into steep and interesting temperature dependencies for nuclear reactions. Analytic approximations yield a rate that is almost vanishingly rare, yet within the incredibly large number of potential interactions within stars quantum tunnelling can still provide the underlying ignition of nuclear reactions.
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44

National Aeronautics and Space Administration (NASA) Staff. Simple Method for Nucleon-Nucleon Cross Sections in a Nucleus. Independently Published, 2018.

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45

Glazov, M. M. Strong Coupling of Electron and Nuclear Spins: Outlook and Prospects. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198807308.003.0011.

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In this chapter, some prospects in the field of electron and nuclear spin dynamics are outlined. Particular emphasis is put ona situation where the hyperfine interaction is so strong that it leads to a qualitative rearrangement of the energy spectrum resulting in the coherent excitation transfer between the electron and nucleus. The strong coupling between the spin of the charge carrier and of the nucleus is realized, for example in the case of deep impurity centers in semiconductors or in isotopically purified systems. We also discuss the effect of the nuclear spin polaron, that is ordered state, formation at low enough temperatures of nuclear spins, where the orientation of the carrier spin results in alignment of the spins of nucleus interacting with the electron or hole.
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46

Eisenberg, Judah M., and Walter Greiner. Nuclear Theory : Excitation Mechanisms of the Nucleus. North-Holland, 1988.

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47

Eisenberg, Judah M., and Walter Greiner. Nuclear Theory : Excitation Mechanisms of the Nucleus. Elsevier, 1988.

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48

Busch, Harris. Nuclear Particles: The Cell Nucleus, Vol. 9. Elsevier Science & Technology Books, 2013.

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49

Poenaru, Dorin. Particle Emission from Nuclei: Nuclear Reformation Energy. Crc Pr I Llc, 1988.

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50

Busch, Harris. Nuclear Particles: The Cell Nucleus, Vol. 8. Elsevier Science & Technology Books, 2013.

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