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Books on the topic 'Massa del neutrino'

Author: Grafiati

Published: 9 March 2023

Last updated: 31 July 2025

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1

B, Pal P., ed. Massive neutrinos in physics and astrophysics. World Scientific, 1991.

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2

B, Pal P., ed. Massive neutrinos in physics and astrophysics. 3rd ed. World Scientific, 2004.

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3

Mohapatra, R. N. Massive neutrinos in physics and astrophysics. 3rd ed. World Scientific, 2005.

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4

Casanova, Gaston. Logique de l'identité-différence et différences de masses: Masse du troisième neutrino. International Logic Review, 1986.

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5

United States. High Energy Physics Advisory Panel. Subpanel on Accelerator-Based Neutrino Oscillation Experiments. High Energy Physics Advisory Panel, Subpanel on Accelerator-Based Neutrino Oscillation Experiments. U.S. Dept. of Energy, Office of Energy Research, Division of High Energy Physics, 1995.

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6

International Conference on the Seesaw Mechanism (2004 Paris, France). SEESAW 25: Proceedings of the International Conference on the Seesaw Mechanism : Institut Henri Poincaré, Paris, 10-11 June 2004. Edited by Orloff J, Lavignac S, and Cribier Michel. World Scientific, 2005.

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7

Fujihara Seminar on Neutrino Mass and Seesaw Mechanism (2004 Kō-enerugī Kasokuki Kenkyū Kikō). Neutrino mass and seesaw mechanism: Proceedings of Fujihara Seminar on Neutrino Mass and Seesaw Mechanism : KEK, Japan, 23-25 February 2004. Elsevier, 2004.

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8

(Fernando), Ferroni F., Vissani F. (Francesco), Brofferio C. (Chiara), and Società italiana di fisica, eds. Measurements of neutrino mass: Proceedings of the International School of Physics "Enrico Fermi", Varenna on Lake Como, Villa Monastero, 17-27 June 2008. IOS Press, 2009.

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9

H, Lee William. Merger of a neutron star with a Newtonian black hole. National Aeronautics and Space Administration, 1995.

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10

H, Lee William. Merger of a neutron star with a Newtonian black hole. National Aeronautics and Space Administration, 1995.

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11

Sciama, D. W. Modern cosmology and the dark matter problem. Cambridge University Press, 1993.

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12

Ryabov, Vladimir. Oil and Gas Chemistry. INFRA-M Academic Publishing LLC., 2021. http://dx.doi.org/10.12737/1017513.

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The textbook provides up-to-date data on the composition and properties of hydrocarbons and other oil and gas compounds, on the physical and chemical methods and methods for separating and identifying oil components (molecular spectroscopy, mass spectrometry, NMR spectroscopy, electron paramagnetic resonance, atomic adsorption spectroscopy, neutron activation analysis). The chemistry and mechanism of thermal and catalytic transformations of oil components in the main processes of oil raw materials processing, as well as the problems of the origin of oil and the transformation of oil in the env

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13

C, Joss Paul, and United States. National Aeronautics and Space Administration., eds. The nature and evolutionary history of GRO J1744-28. National Aeronautics and Space Administration, 1997.

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14

N, Zhang S., and United States. National Aeronautics and Space Administration., eds. Broadband high-energy observations of the superluminal jet source gro J1655--40 during an outburst. National Aeronautics and Space Administration, 1997.

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15

Salvatore, Esposito, ed. Ettore Majorana: Notes on theoretical physics. Kluwer Academic Publishers, 2003.

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16

Salvatore, Esposito, ed. Ettore Majorana: Unpublished research notes on theoretical physics. Springer, 2009.

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17

Majorana, Ettore. Ettore Majorana: Scientific papers : on occasion of the centenary of his birth. Springer, 2006.

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18

Massive Neutrinos in Physics and Astrophysics (World Scientific Lecture Notes in Physics). 2nd ed. World Scientific Publishing Company, 1998.

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19

Massive Neutrinos in Physics and Astrophysics. World Scientific Publishing Co Pte Ltd, 2004.

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20

'86 Massive neutrinos in astrophysics and in particle physics: Proceedings of the Sixth Moriond Workshop, Tignes, Savoie, France, January 25-February 1st, 1986. Editions Frontieres, 1986.

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21

Neutrino Mass. Springer, 2010.

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22

Stuewer, Roger H. Nuclear Physicists at the Crossroads. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198827870.003.0009.

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The Nazi Civil Service Law of April 7, 1933, prompted the establishment of refugee organizations to cope with the greatest intellectual migration in history, a difficult task in the Great Depression. It was in full swing in October when the seventh Solvay Conference was convened to address fundamental questions in nuclear physics. Foremost was the exact value of the mass of the neutron. Chadwick, Curie and Joliot, and Lawrence advanced very different values, and Lawrence soon had to admit that his very low value was mistaken. In January 1934, Fermi published his far-reaching theory of beta dec

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23

Kato, S., and Ins International Symposium on Neutrino Mass and Related Topics 1988. Neutrino Mass and Related Topics: Proceedings of XVI Ins International Symposium, Tokyo 16-18 March 1988. World Scientific Pub Co Inc, 1989.

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24

Orloff, J., S. Lavignac, and International Conference on the Seesaw M. Seesaw 25: Proceedings of the International Conference on the Seesaw Mechanism, Institut Henri Poincare, Paris 10-11 June, 2004. World Scientific Publishing Company, 2005.

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25

Light domain walls, massive neutrinos and the large scale structure of the universe. Fermi National Accelerator Laboratory, 1991.

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26

Seesaw25: Proceedings of the international conference on the Seesaw mechanism. World Scientific, 2004.

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27

Neutrino Mass and Gauge Structure of Weak Interactions (AIP Conference Proceedings). American Institute of Physics, 1998.

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28

Peskin, Michael E. Concepts of Elementary Particle Physics. Oxford University Press, 2019. http://dx.doi.org/10.1093/oso/9780198812180.001.0001.

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This is a textbook of elementary particle physics whose goal is to explain the Standard Model of particle interactions. Part I introduces the basic concepts governing high-energy particle physics: elements of relativity and quantum field theory, the quark model of hadrons, methods for detection and measurement of elementary particles, methods for calculating predictions for observable quantitites. Part II builds up our understanding of the strong interaction from the key experiments to the formulation of Quantum Chromodynamics and its application to the description of evetns at the CERN Large

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29

Stuewer, Roger H. Beta Decay Redux, Slow Neutrons, Bohr and his Realm. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198827870.003.0012.

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A large conference on nuclear physics was held in London and Cambridge from October 1–6, 1934. Six German refugee physicists were present, but Werner Heisenberg was not. Czech theoretical physicists Guido Beck and Kurt Sitte had proposed a theory of beta decay that challenged Fermi’s, which Beck presented but apparently gained no support for. On October 22, Fermi serendipitously discovered the efficaciousness of slow neutrons in producing nuclear reactions. Niels Bohr would be the greatest beneficiary of Fermi’s discovery. In 1935 Bohr, with the assistance of refugee Otto Robert Frisch, began

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30

Ettore Majorana: Notes on Theoretical Physics (Fundamental Theories of Physics). Springer, 2003.

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31

Wigmans, Richard. Contributions of Calorimetry to the Advancement of Science. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198786351.003.0011.

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In this last chapter, some scientific discoveries are described in which calorimeters have played a crucial role. The chosen examples were all awarded a Nobel prize in physics. The first example concerns the discovery of the intermediate vector bosons (W and Z) by the experiments UA1 and UA2 at CERN (1982). More than anything else, this discovery has been crucial for the dominant role that calorimeters have played in the design of experiments at the subsequent generation(s) of particle accelerators. The second example concerns the discovery of the fact that neutrinos have a non-zero rest mass,

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32

Ellam, Rob. 1. Identical outsides … different insides. Oxford University Press, 2016. http://dx.doi.org/10.1093/actrade/9780198723622.003.0001.

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‘Identical outsides … different insides’ describes the isotopes of hydrogen (protium, deuterium, tritium) and carbon (carbon-12, carbon-13, carbon-14). The isotopes exist due to an extra particle (neutron) or two in the element’s nucleus, which adds extra mass to the atom. Tritium and carbon-14 are both unstable and undergo radioactive decay. There are four types of radioactive decay: α, β, γ (alpha, beta, gamma), and spontaneous fission. Radioactive decay is the process whereby the nucleus of an unstable atom loses energy by emission of ionizing radiation. The rate of the radioactive decay is

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33

Croddy, Eric A., Jeffrey A. Larsen, and James J. Wirtz, eds. Weapons of Mass Destruction. ABC-CLIO, LLC, 2018. http://dx.doi.org/10.5040/9798216034247.

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Whether one is interested in learning about anthrax, sarin, the neutron bomb—or any other weapon of mass destruction—this thorough and detailed reference is the place to find answers. The threat posed by weapons of mass destruction (WMD), whether nuclear, radiological, chemical, or biological, is the number-one topic of concern for the intelligence community, first responders, policymakers, and myriad non-governmental organizations—and many members of the general public. This authoritative reference will serve all of those parties by covering the full spectrum of mass-casualty weapons. The gui

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34

(Editor), G. F. Bassani, and Società Italiana di Fisica (Editor), eds. Ettore Majorana: Scientific Papers. Springer, 2007.

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35

IL SEGRETO DEL VENTO: Viaggio nella profondità dell'essere. ONLUS S.M.V.P - 90041 Balestrate (PA), 2010.

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36

IL SEGRETO DEL VENTO: VIAGGIO PROFONDO NELLA CONOSCENZA DELL'ESSERE. ONLUS S.M.V.P - 90041 Balestrate (PA) tel +393287573178, 2009.

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IL SEGRETO DEL VENTO: Viaggio nella profondità dell'essere. ONLUS S.M.V.P - 90041 Balestrate (PA), 2007.

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