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Mountains on neutron stars

Author
HASKELL, B1
[1] School of Mathematics, University of Southampton, Southampton, SO17 1BJ, United Kingdom
Conference title
18th International Conference on General Relativity and Gravitation (GRG18) and 7th Edoardo Amaldi Conference on Gravitational Waves (Amaldi7), Sydney, Australia, July 2007
Conference name
Edoardo Amaldi Conference on Gravitational Waves (Amaldi7) (Amaldi7) (7 ; Sydney 2007) = International Conference on General Relativity and Gravitation (GRG18) (GRG18) (18 ; Sydney 2007)
Author (monograph)
SCOTT, Susan M (Editor)1 ; MCCLELLAND, David (Editor)1
[1] Centre for Gravitational Physics, The Australian National University, Australia
Source

Classical and quantum gravity (Print). 2008, Vol 25, Num 11 ; 114049.1-114049.7 ; ref : 19 ref

CODEN
CQGRDG
ISSN
0264-9381
Scientific domain
Theoretical physics
Publisher
Institute of Physics, Bristol
Publication country
United Kingdom
Document type
Conference Paper
Language
English
Keyword (fr)
Accrétion stellaire Analyse donnée Champ intense Champ magnétique Chromodynamique quantique Déformation Détecteur onde gravitationnelle Emission onde Etoile faible masse Etoile neutron Etoile rotation Onde gravitationnelle
Keyword (en)
Star accretion Data analysis High field Magnetic fields Quantum chromodynamics Deformation Gravitational wave detectors Wave emission Low-mass stars Neutron stars Rotating star Gravitational waves
Keyword (es)
Emisión onda Estrella rotación
Classification
Pascal
001 Exact sciences and technology / 001B Physics / 001B00 General / 001B00D General relativity and gravitation

Discipline
Theoretical physics
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20419921

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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