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Influence of pion-delta-hole configuration on the rho meson mass spectrum in dense hadronic matter

Author
Chanfray, G; Schuck, P
IN2P3, Institut de physique nucléaire de Lyon, Villeurbanne, France
Université de Lyon 1, Institut de physique nucléaire de Lyon, Villeurbanne, France
Source

1997, 7 p. ; Figure ; ref : 14 ref

Report number
LYCEN - 9748
Scientific domain
Physics
Document type
Report
Language
English
Keyword (fr)
Donnée expérimentale Forme delta Méson rhô Pion Production hadron Propagateur Spectre masse
Keyword (en)
Experimental data Delta form Rho mesons Pions Hadron production Propagator Mass spectra
Keyword (es)
Forma delta
Classification
Pascal
001 Exact sciences and technology / 001B Physics / 001B10 The physics of elementary particles and fields / 001B10D Properties of specific particles / 001B10D40 Mesons

Pascal
001 Exact sciences and technology / 001B Physics / 001B30 Atomic and molecular physics / 001B30B Atomic properties and interactions with photons / 001B30B10 Properties of atoms and atomic ions / 001B30B10B Atomic masses, mass spectra, abundances and isotopes

Pascal
001 Exact sciences and technology / 001B Physics / 001B30 Atomic and molecular physics / 001B30C Molecular properties and interactions with photons / 001B30C15 Properties of molecules and molecular ions / 001B30C15T Mass spectra

Pacs
1440 Mesons

Pacs
3210B Atomic masses, mass spectra, abundances, and isotopes

Pacs
3315T Mass spectra

Sigle
430A20B Elementary particles; high energy physics

Discipline
Atomic and molecular physics Physics of elementary particles and fields
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
98825

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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