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Volumn 13, Issue 2, 2004, Pages 291-325

Covariant analysis of Newtonian multi-fluid models for neutron stars: I Milne-Cartan structure and variational formulation

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EID: 10844271257     PISSN: 02182718     EISSN: None     Source Type: Journal    
DOI: 10.1142/S0218271804004542     Document Type: Article
Times cited : (49)

References (19)
  • 3
    • 0010999213 scopus 로고
    • Covariant theory of conductivity in ideal fluid or solid media
    • Relativistic Fluid Dynamics, C.I.M.E., Noto, May 1987, eds. A. M. Anile and Y. Choquet-Bruhat Springer-Verlag, Heidelberg
    • B. Carter, "Covariant theory of conductivity in ideal fluid or solid media," in Relativistic Fluid Dynamics, C.I.M.E., Noto, May 1987, Lecture Notes in Mathematics 1385, eds. A. M. Anile and Y. Choquet-Bruhat (Springer-Verlag, Heidelberg, 1989), pp. 1-64.
    • (1989) Lecture Notes in Mathematics 1385 , pp. 1-64
    • Carter, B.1
  • 7
    • 0036188007 scopus 로고    scopus 로고
    • Slowly rotating superfluid Newtonian star-model with entrainment
    • astro-ph/0107176
    • R. Prix, G. L. Comer and N. Andersson, "Slowly rotating superfluid Newtonian star-model with entrainment," Astron. & Astrophys. 381, 178 (2002) [astro-ph/0107176].
    • (2002) Astron. & Astrophys. , vol.381 , pp. 178
    • Prix, R.1    Comer, G.L.2    Andersson, N.3
  • 13
    • 23544457426 scopus 로고
    • gr-qc/9409008
    • W. Unruh, Phys. Rev. D51, 2827 (1995) [gr-qc/9409008].
    • (1995) Phys. Rev. , vol.D51 , pp. 2827
    • Unruh, W.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.