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Libros sobre el tema "Neutron emissions"

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Publicado: 14 de marzo de 2023

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1

Carpinteri, Alberto, Giuseppe Lacidogna y Amedeo Manuello, eds. Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2.

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2

Norbury, John W. Calculation of two-neutron multiplicity in photonuclear reactions. Hampton, Va: Langley Research Center, 1990.

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3

Inferences from Surface Thermal Emission of Young Neutron Stars. [New York, N.Y.?]: [publisher not identified], 2020.

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4

J, Hughes M., Cowell Michael, Hook Duncan R y British Museum. Dept. of Scientific Research., eds. Neutron activation and plasma emission spectrometric analysis in archaeology: Techniques and applications. London: British Museum, 1994.

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5

Howarth, P. J. A. The JET neutron emission profile diagnostic: Data exploitation and the development of an upgraded version. Birmingham: University of Birmingham, 1994.

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6

Hartmann, Dap. The Leiden/Dwingeloo survey of galactic neutral hydrogen. Leiden: Sterrewacht Leiden, 1994.

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7

Hartmann, Dap. The Leiden/Dwingeloo survey of galactic neutral hydrogen. Leiden: Sterrewacht Leiden, 1995.

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8

Civiš, Svatopluk, Ekaterina Zanozina, Adam Pastorek, Petr Kubelík, Martin Ferus y Ashok Chilukoti. Atomic Emission Spectra of Neutral Noble Gases in the Infrared Spectral Range. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-47352-5.

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9

Nanda, Rea y SpringerLink (Online service), eds. High-Energy Emission from Pulsars and their Systems: Proceedings of the First Session of the Sant Cugat Forum on Astrophysics. Berlin, Heidelberg: Springer-Verlag Berlin Heidelberg, 2011.

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10

R, Cominsky Lynn y United States. National Aeronautics and Space Administration., eds. ROSAT observations of the binary Be-star/radio pulsar PSR1259-63: Final technical report for NASA NAG 5-1684. [Washington, DC: National Aeronautics and Space Administration, 1994.

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11

McElroy, Kenneth L. The atmospheric emission method of calculating the neutral atmosphere and changed particle densities in the upper atmosphere. Monterey, Calif: Naval Postgraduate School, 1992.

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12

United States. National Aeronautics and Space Administration., ed. Diffuse emission and pathological Seyfert spectra: National Aeronuatics and Space Administration ROSAT annual status report for NAG 5-1935. [Washington, D.C.]: National Aeronautics and Space Administration, 1995.

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13

Afarideh, Hossein. A study of fission in [superior] 238 U induced by Monoenergetic neutrons and heavy ions and oflight particle emission in [superior] 252 Cf spontaneous fission. Birmingham: University of Birmingham, 1988.

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14

Smyth, William H. Studies for the loss of atomic and molecular species for Io: Final report for the period of May 7, 1993 to May 6, 1996. [Washington, DC: National Aeronautics and Space Administration, 1996.

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15

United States. National Aeronautics and Space Administration., ed. Reduction and analysis of seasons 15 and 16 (1991-1992), Pioneer Venus radio occultation data and correlative studies with observations of the near infra-red emission of Venus: Report to the National Aeronautics and Space Administration, Ames Research Center for grant NCC2-753, April 1, 1992 through May 31, 1995. [Washington, DC: National Aeronautics and Space Administration, 1995.

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16

Carpinteri, Alberto, Giuseppe Lacidogna y Amedeo Manuello. Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes. Springer, 2015.

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17

Carpinteri, Alberto, Giuseppe Lacidogna y Amedeo Manuello. Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes. Springer, 2019.

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18

Carpinteri, Alberto, Giuseppe Lacidogna y Amedeo Manuello. Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes. Springer London, Limited, 2016.

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19

Maggiore, Michele. Neutron stars. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198570899.003.0002.

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Observation of neutron stars as pulsars. Pulsar demography. Magnetars. GW emission from neutron stars. Normal modes of neuton stars. CFS instability; r-mode instability. GWs from the post-merger NS remnant. Ellipticity of deformed neutron stars.
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20

Nadel-Turonski, Pawel. Experimental Studies of Neutron Emission Induced by Heavy-Ion Scattering. Uppsala Universitet, 2003.

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21

(Editor), M. J. Hughes, Michael R. Cowell (Editor) y Duncan R. Hook (Editor), eds. Neutron Activation and Plasma Emission Spectrometric Analysis in Archaeology (Occasional Papers). British Museum Press, 1991.

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22

Tardocchi, Marco. Neutron Emission Spectroscopy Studies of Fusion Plasmas of Deuterium - Tritium in Tokamaks. Uppsala Universitet, 2000.

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23

Stuewer, Roger H. New Particles. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198827870.003.0007.

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In December 1931, Harold Urey discovered deuterium (and its nucleus, the deuteron) by spectroscopically detecting the faint companion lines in the Balmer spectrum of atomic hydrogen that were produced by the heavy hydrogen isotope. In February 1932, James Chadwick, stimulated by the claim of the wife-and-husband team of Irène Curie and Frédéric Joliot that polonium alpha particles cause the emission of energetic gamma rays from beryllium, proved experimentally that not gamma rays but neutrons are emitted, thereby discovering the particle whose existence had been predicted a dozen years earlier by Chadwick’s mentor, Ernest Rutherford. In August 1932, Carl Anderson took a cloud-chamber photograph of a positron traversing a lead plate, unaware that Paul Dirac had predicted the existence of the anti-electron in 1931. These three new particles, the deuteron, neutron, and positron, were immediately incorporated into the experimental and theoretical foundations of nuclear physics.
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24

Siliņa, Ilze. Energy Management System in Climate-neutral District Heating. RTU Press, 2022. http://dx.doi.org/10.7250/9789934228001.

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District heating (DH) has big potential for implementing energy efficiency measures and renewable energy sources (RES) and reducing CO2 emissions, as the range of RES technologies used is wide: biomass, solar panels, heat pumps, and other technologies and their combinations. The aim of the Thesis is to assess the potential for extending the energy management system to integrate renewable energy technologies, with a particular focus on the solar system.
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25

O'Connor, Gregory. Neutron induced gamma-ray emission and transmission tomography in the analysis of human brain tissue. 1995.

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26

Civiš, Svatopluk, Martin Ferus, Ekaterina Zanozina, Adam Pastorek, Petr Kubelík y Ashok Chilukoti. Atomic Emission Spectra of Neutral Noble Gases in the Infrared Spectral Range. Springer, 2020.

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27

Maggiore, Michele. Stellar collapse. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198570899.003.0001.

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Stellar collapse and supernova explosions. Properties and classification of supernovae. Historical supernovae. Explosion mechanisms and core-collapse dynamics. The remnant of the collapse. GW production during core collapse, bar-mode instabilities, anisotropic neutrino emission.
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28

Thun, Johan. Studies of the Nuclear Processes of Proton Capture Photon Production and Spallation Neutron Emission With Advanced Experimental Techniques. Uppsala Universitet, 1999.

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29

Torres, Diego F. y Nanda Rea. High-Energy Emission from Pulsars and their Systems: Proceedings of the First Session of the Sant Cugat Forum on Astrophysics. Springer, 2013.

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30

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 measured by the ‘half-life’—the time needed for half the radioactive isotopes of a substance to decay.
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31

ROSAT observations of the binary Be-star/radio pulsar PSR1259-63: Final technical report for NASA NAG 5-1684. [Washington, DC: National Aeronautics and Space Administration, 1994.

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32

Fuss, Sabine. The 1.5°C Target, Political Implications, and the Role of BECCS. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190228620.013.585.

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The 2°C target for global warming had been under severe scrutiny in the run-up to the climate negotiations in Paris in 2015 (COP21). Clearly, with a remaining carbon budget of 470–1,020 GtCO2eq from 2015 onwards for a 66% probability of stabilizing at concentration levels consistent with remaining below 2°C warming at the end of the 21st century and yearly emissions of about 40 GtCO2 per year, not much room is left for further postponing action. Many of the low stabilization pathways actually resort to the extraction of CO2 from the atmosphere (known as negative emissions or Carbon Dioxide Removal [CDR]), mostly by means of Bioenergy with Carbon Capture and Storage (BECCS): if the biomass feedstock is produced sustainably, the emissions would be low or even carbon-neutral, as the additional planting of biomass would sequester about as much CO2 as is generated during energy generation. If additionally carbon capture and storage is applied, then the emissions balance would be negative. Large BECCS deployment thus facilitates reaching the 2°C target, also allowing for some flexibility in other sectors that are difficult to decarbonize rapidly, such as the agricultural sector. However, the large reliance on BECCS has raised uneasiness among policymakers, the public, and even scientists, with risks to sustainability being voiced as the prime concern. For example, the large-scale deployment of BECCS would require vast areas of land to be set aside for the cultivation of biomass, which is feared to conflict with conservation of ecosystem services and with ensuring food security in the face of a still growing population.While the progress that has been made in Paris leading to an agreement on stabilizing “well below 2°C above pre-industrial levels” and “pursuing efforts to limit the temperature increase to 1.5°C” was mainly motivated by the extent of the impacts, which are perceived to be unacceptably high for some regions already at lower temperature increases, it has to be taken with a grain of salt: moving to 1.5°C will further shrink the time frame to act and BECCS will play an even bigger role. In fact, aiming at 1.5°C will substantially reduce the remaining carbon budget previously indicated for reaching 2°C. Recent research on the biophysical limits to BECCS and also other negative emissions options such as Direct Air Capture indicates that they all run into their respective bottlenecks—BECCS with respect to land requirements, but on the upside producing bioenergy as a side product, while Direct Air Capture does not need much land, but is more energy-intensive. In order to provide for the negative emissions needed for achieving the 1.5°C target in a sustainable way, a portfolio of negative emissions options needs to minimize unwanted effects on non–climate policy goals.
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