Serveur d'exploration H2N2

Attention, ce site est en cours de développement !
Attention, site généré par des moyens informatiques à partir de corpus bruts.
Les informations ne sont donc pas validées.

Adiabatic Invariant of Radiative Transitions in the Coulomb Field

Identifieur interne : 002126 ( Main/Exploration ); précédent : 002125; suivant : 002127

Adiabatic Invariant of Radiative Transitions in the Coulomb Field

Auteurs : S. P. Alliluev [Russie] ; S. S. Gershtein [Russie]

Source :

RBID : ISTEX:564CA0BE6E4368B1FF1908A5DD15502E54AF9A6E

Abstract

Abstract: I. The adiabatic invariants1 turn out quite useful in describing nonconservative systems with slowly changing parameters. The examples of their existence are well-known. Thus, for an oscillator such adiabatic invariant is the ratio of the oscillator energy (E) its frequency ((d), which remains constant under slow changes of the latter (as compared with the period). If we take a charged particle moving in a weakly variable magnetic field (H), its adiabatic invariant is P⊥/H (P⊥ is a particle momentum component, perpendicular to the field). In this Lecture we want to point out that such an adiabatic invariant does exist for the finite motion of a charged particle emitting electro-magnetic waves in the Coulomb field.

Url:
DOI: 10.1007/978-1-4899-3701-8_18


Affiliations:


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


Le document en format XML

<record>
<TEI wicri:istexFullTextTei="biblStruct">
<teiHeader>
<fileDesc>
<titleStmt>
<title xml:lang="en">Adiabatic Invariant of Radiative Transitions in the Coulomb Field</title>
<author>
<name sortKey="Alliluev, S P" sort="Alliluev, S P" uniqKey="Alliluev S" first="S. P." last="Alliluev">S. P. Alliluev</name>
</author>
<author>
<name sortKey="Gershtein, S S" sort="Gershtein, S S" uniqKey="Gershtein S" first="S. S." last="Gershtein">S. S. Gershtein</name>
</author>
</titleStmt>
<publicationStmt>
<idno type="wicri:source">ISTEX</idno>
<idno type="RBID">ISTEX:564CA0BE6E4368B1FF1908A5DD15502E54AF9A6E</idno>
<date when="1990" year="1990">1990</date>
<idno type="doi">10.1007/978-1-4899-3701-8_18</idno>
<idno type="url">https://api.istex.fr/ark:/67375/HCB-KLPWSPL9-K/fulltext.pdf</idno>
<idno type="wicri:Area/Istex/Corpus">000651</idno>
<idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Corpus" wicri:corpus="ISTEX">000651</idno>
<idno type="wicri:Area/Istex/Curation">000651</idno>
<idno type="wicri:Area/Istex/Checkpoint">000E57</idno>
<idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Checkpoint">000E57</idno>
<idno type="wicri:Area/Main/Merge">002228</idno>
<idno type="wicri:Area/Main/Curation">002126</idno>
<idno type="wicri:Area/Main/Exploration">002126</idno>
</publicationStmt>
<sourceDesc>
<biblStruct>
<analytic>
<title level="a" type="main" xml:lang="en">Adiabatic Invariant of Radiative Transitions in the Coulomb Field</title>
<author>
<name sortKey="Alliluev, S P" sort="Alliluev, S P" uniqKey="Alliluev S" first="S. P." last="Alliluev">S. P. Alliluev</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Russie</country>
<wicri:regionArea>Institute for High Energy Physics, 142284, Serpukhov Moscow Region</wicri:regionArea>
<wicri:noRegion>Serpukhov Moscow Region</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Gershtein, S S" sort="Gershtein, S S" uniqKey="Gershtein S" first="S. S." last="Gershtein">S. S. Gershtein</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Russie</country>
<wicri:regionArea>Institute for High Energy Physics, 142284, Serpukhov Moscow Region</wicri:regionArea>
<wicri:noRegion>Serpukhov Moscow Region</wicri:noRegion>
</affiliation>
</author>
</analytic>
<monogr></monogr>
<series>
<title level="s" type="main" xml:lang="en">Ettore Majorana International Science Series</title>
</series>
</biblStruct>
</sourceDesc>
</fileDesc>
<profileDesc>
<textClass></textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">Abstract: I. The adiabatic invariants1 turn out quite useful in describing nonconservative systems with slowly changing parameters. The examples of their existence are well-known. Thus, for an oscillator such adiabatic invariant is the ratio of the oscillator energy (E) its frequency ((d), which remains constant under slow changes of the latter (as compared with the period). If we take a charged particle moving in a weakly variable magnetic field (H), its adiabatic invariant is P⊥/H (P⊥ is a particle momentum component, perpendicular to the field). In this Lecture we want to point out that such an adiabatic invariant does exist for the finite motion of a charged particle emitting electro-magnetic waves in the Coulomb field.</div>
</front>
</TEI>
<affiliations>
<list>
<country>
<li>Russie</li>
</country>
</list>
<tree>
<country name="Russie">
<noRegion>
<name sortKey="Alliluev, S P" sort="Alliluev, S P" uniqKey="Alliluev S" first="S. P." last="Alliluev">S. P. Alliluev</name>
</noRegion>
<name sortKey="Gershtein, S S" sort="Gershtein, S S" uniqKey="Gershtein S" first="S. S." last="Gershtein">S. S. Gershtein</name>
</country>
</tree>
</affiliations>
</record>

Pour manipuler ce document sous Unix (Dilib)

EXPLOR_STEP=$WICRI_ROOT/Sante/explor/H2N2V1/Data/Main/Exploration
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 002126 | SxmlIndent | more

Ou

HfdSelect -h $EXPLOR_AREA/Data/Main/Exploration/biblio.hfd -nk 002126 | SxmlIndent | more

Pour mettre un lien sur cette page dans le réseau Wicri

{{Explor lien
   |wiki=    Sante
   |area=    H2N2V1
   |flux=    Main
   |étape=   Exploration
   |type=    RBID
   |clé=     ISTEX:564CA0BE6E4368B1FF1908A5DD15502E54AF9A6E
   |texte=   Adiabatic Invariant of Radiative Transitions in the Coulomb Field
}}

Wicri

This area was generated with Dilib version V0.6.33.
Data generation: Tue Apr 14 19:59:40 2020. Site generation: Thu Mar 25 15:38:26 2021