ThuliumV1, Main, Exploration, bibRecord, 000A69

Introduction to Astronomy with Radioactivity

Identifieur interne : 000A69 ( Main/Exploration ); précédent : 000A68; suivant : 000A70

Introduction to Astronomy with Radioactivity

Auteurs : R. Diehl [Allemagne]

Source :

Lecture Notes in Physics [ 0075-8450 ] ; 2011.

RBID : ISTEX:032FFD94A8A8321FFB5F0611C8927DF10946D228

Descripteurs français

Wicri :
- topic : Physique nucléaire, Radioactivité.

English descriptors

KwdEn :
- Angular momentum, Astronomical abundance scale, Astrophysical, Atomic masses, Atomic nuclei, Atomic nucleus, Atomic weight, Binding energy, Chemical elements, Chemical properties, Cosmic, Cosmic evolution, Cosmic history, Cosmic material, Cosmic nucleosynthesis, Cosmic nucleosynthesis sites, Cosmic nucleosynthesis source, Cosmic objects, Cosmic radioactivity, Cosmic sites, Cosmic sources, Daughter nucleus, Decay, Decay probability, Decay time, Diehl, Different environments, Different types, Dust grains, Electromagnetic, Electromagnetic radiation, Electromagnetic spectrum, Electromagnetic transitions, Ground state, Heavier elements, Interstellar space, Isotope, Isotopic, Isotopic abundances, Isotopic composition, Isotopic information, Kinetic energy, Lower right, Magic numbers, Meteoritic inclusions, Meteoritic material, More detail, Neutrino, Neutron, Nineteenth century, Nuclear masses, Nuclear physics, Nuclear reactions, Nuclear transitions, Nucleon, Nucleosynthesis, Nucleosynthesis sites, Nucleus, Other isotopes, Penetrating radiation, Periodic table, Phase space, Phys, Potential barrier, Proton, Radioactive, Radioactive decay, Radioactive energy, Radioactive lifetime, Radioactive nucleus, Radioactivity, Reference element, Secondary products, Small solids, Solar abundances, Solar system, Stable isotope, Stellar, Stellar explosions, Stellar interiors, Supernova, Supernova explosions, Terrestrial laboratories, Unit time, Unstable isotopes, Unstable nucleus, Weak interactions.
Teeft :
- Angular momentum, Astronomical abundance scale, Astrophysical, Atomic masses, Atomic nuclei, Atomic nucleus, Atomic weight, Binding energy, Chemical elements, Chemical properties, Cosmic, Cosmic evolution, Cosmic history, Cosmic material, Cosmic nucleosynthesis, Cosmic nucleosynthesis sites, Cosmic nucleosynthesis source, Cosmic objects, Cosmic radioactivity, Cosmic sites, Cosmic sources, Daughter nucleus, Decay, Decay probability, Decay time, Diehl, Different environments, Different types, Dust grains, Electromagnetic, Electromagnetic radiation, Electromagnetic spectrum, Electromagnetic transitions, Ground state, Heavier elements, Interstellar space, Isotope, Isotopic, Isotopic abundances, Isotopic composition, Isotopic information, Kinetic energy, Lower right, Magic numbers, Meteoritic inclusions, Meteoritic material, More detail, Neutrino, Neutron, Nineteenth century, Nuclear masses, Nuclear physics, Nuclear reactions, Nuclear transitions, Nucleon, Nucleosynthesis, Nucleosynthesis sites, Nucleus, Other isotopes, Penetrating radiation, Periodic table, Phase space, Phys, Potential barrier, Proton, Radioactive, Radioactive decay, Radioactive energy, Radioactive lifetime, Radioactive nucleus, Radioactivity, Reference element, Secondary products, Small solids, Solar abundances, Solar system, Stable isotope, Stellar, Stellar explosions, Stellar interiors, Supernova, Supernova explosions, Terrestrial laboratories, Unit time, Unstable isotopes, Unstable nucleus, Weak interactions.

Abstract

Abstract: The nineteenth century spawned various efforts to bring order into the elements encountered in nature. Among the most important was an inventory of the elements Chemical elements Elements!chemical assembled by the Russian chemist Dimitri Mendeleyev Mendeleyev, D. in 1869, which grouped elements according to their chemical properties, their valences, as derived from the compounds they were able to form, at the same time sorting the elements by atomic weight. The genius of Mendeleyev lay in his confidence in these sorting principles, which enforced gaps in his table for expected but then unknown elements, and Mendeleyev was able to predict the physical and chemical properties of such elements-to-be-found. The tabular arrangement invented by Mendeleyev (Fig. 1.1) still is in use today, and is being populated at the high-mass end by the great experiments in heavy-ion collider laboratories to create the short-lived elements predicted to exist. The second half of the nineteenth century thus saw scientists being all-excited about chemistry and the fascinating discoveries one could make using Mendeleyev’s sorting principles. Note that this was some 30 years before sub-atomic particles and the atom were discovered. Today the existence of 112 elements is firmly established (the currently heaviest) element no. 112 was officially named Copernicium (Cn) in February 2010 by IUPAC, the international union of chemistry.

Url:

https://api.istex.fr/document/032FFD94A8A8321FFB5F0611C8927DF10946D228/fulltext/pdf

DOI: 10.1007/978-3-642-12698-7_1

Affiliations:

Allemagne

Links toward previous steps (curation, corpus...)

to stream Istex, to step Corpus: 000080
to stream Istex, to step Curation: 000080
to stream Istex, to step Checkpoint: 000205
to stream Main, to step Merge: 000A73
to stream Main, to step Curation: 000A69

Le document en format XML

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<term>Radioactive decay</term>
<term>Radioactive energy</term>
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<term>Radioactive nucleus</term>
<term>Radioactivity</term>
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<term>Secondary products</term>
<term>Small solids</term>
<term>Solar abundances</term>
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<term>Stable isotope</term>
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<term>Stellar explosions</term>
<term>Stellar interiors</term>
<term>Supernova</term>
<term>Supernova explosions</term>
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<term>Unit time</term>
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<term>Atomic nucleus</term>
<term>Atomic weight</term>
<term>Binding energy</term>
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<term>Cosmic history</term>
<term>Cosmic material</term>
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<term>Cosmic sites</term>
<term>Cosmic sources</term>
<term>Daughter nucleus</term>
<term>Decay</term>
<term>Decay probability</term>
<term>Decay time</term>
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<term>Different environments</term>
<term>Different types</term>
<term>Dust grains</term>
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<term>Electromagnetic radiation</term>
<term>Electromagnetic spectrum</term>
<term>Electromagnetic transitions</term>
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<term>Heavier elements</term>
<term>Interstellar space</term>
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<term>Isotopic</term>
<term>Isotopic abundances</term>
<term>Isotopic composition</term>
<term>Isotopic information</term>
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<term>Magic numbers</term>
<term>Meteoritic inclusions</term>
<term>Meteoritic material</term>
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<term>Neutron</term>
<term>Nineteenth century</term>
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<term>Nuclear physics</term>
<term>Nuclear reactions</term>
<term>Nuclear transitions</term>
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<term>Nucleosynthesis sites</term>
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<front><div type="abstract" xml:lang="en">Abstract: The nineteenth century spawned various efforts to bring order into the elements encountered in nature. Among the most important was an inventory of the elements Chemical elements Elements!chemical assembled by the Russian chemist Dimitri Mendeleyev Mendeleyev, D. in 1869, which grouped elements according to their chemical properties, their valences, as derived from the compounds they were able to form, at the same time sorting the elements by atomic weight. The genius of Mendeleyev lay in his confidence in these sorting principles, which enforced gaps in his table for expected but then unknown elements, and Mendeleyev was able to predict the physical and chemical properties of such elements-to-be-found. The tabular arrangement invented by Mendeleyev (Fig. 1.1) still is in use today, and is being populated at the high-mass end by the great experiments in heavy-ion collider laboratories to create the short-lived elements predicted to exist. The second half of the nineteenth century thus saw scientists being all-excited about chemistry and the fascinating discoveries one could make using Mendeleyev’s sorting principles. Note that this was some 30 years before sub-atomic particles and the atom were discovered. Today the existence of 112 elements is firmly established (the currently heaviest) element no. 112 was officially named Copernicium (Cn) in February 2010 by IUPAC, the international union of chemistry.</div>
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Introduction to Astronomy with Radioactivity

Introduction to Astronomy with Radioactivity

Source :

Descripteurs français

English descriptors

Abstract

Links toward previous steps (curation, corpus...)

Le document en format XML

Pour manipuler ce document sous Unix (Dilib)

Pour mettre un lien sur cette page dans le réseau Wicri