Lagrangian perturbation theory for a superfluid immersed in an elastic neutron star crust

Monthly Notices of the Royal Astronomical Society

Volumn 416, Issue 1, 2011, Pages 118-132

  Andersson, N ^a   Haskell, B ^a,b   Samuelsson, L ^c,d  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b UNIVERSITY OF AMSTERDAM   (Netherlands)

^c UMEÅ UNIVERSITY   (Sweden)

^d NORDITA   (Denmark)

Author keywords

Asteroseismology; Dense matter; Gravitational waves; Hydrodynamics; Stars: neutron

Indexed keywords

GRAVITY WAVES; LAGRANGE MULTIPLIERS; NEUTRONS; PERTURBATION TECHNIQUES; STARS; THERMAL CONDUCTIVITY;

ASTEROSEISMOLOGY; ASTROPHYSICAL PHENOMENA; DENSE MATTER; ELASTIC LATTICE; LAGRANGIAN; NEUTRON STARS; NEUTRON-RICH NUCLEI; PERTURBATION THEORY; STARS: NEUTRONS; SURFACE TEMPERATURES;

ASTROPHYSICS;

EID: 80051815118     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.19015.x     Document Type: Article

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