Relativistic r modes and shear viscosity: Regularizing the continuous spectrum

Monthly Notices of the Royal Astronomical Society

Volumn 363, Issue 1, 2005, Pages 121-130

  Pons, J A ^a   Gualtieri, L ^b   Miralles, J A ^a   Ferrari, V ^b  

^a UNIVERSITY OF ALICANTE   (Spain)

^b SAPIENZA UNIVERSITY OF ROME   (Italy)

Author keywords

Gravitational waves; Stars: neutron; Stars: oscillations

Indexed keywords

DAMPING; EIGENVALUES AND EIGENFUNCTIONS; ENERGY DISSIPATION; GRAVITY WAVES; PERTURBATION TECHNIQUES; SHEAR FLOW; SHEAR VISCOSITY; STARS;

CONTINUOUS SPECTRUM; DAMPING TIME; EQUATION-OF-STATE; INVISCID LIMITS; PERTURBATION EQUATION; RELATIVISTIC STARS; RELATIVISTICS; STAR OSCILLATIONS; STARS: NEUTRONS; VISCOUS DAMPING;

EQUATIONS OF STATE;

EID: 26444591892     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09429.x     Document Type: Article

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