1 Alford, M., Berges, J., and Rajagopal, K., “Magnetic Fields within Color Superconducting Neutron Star Cores”, Nucl. Phys. B, 571, 269–284, (2000). Related online version (cited on 14 December 2006):
External Linkhttp://adsabs.harvard.edu/abs/2000NuPhB.571..269A
2 Amsden, A.A., Bertsch, G.F., Harlow, F.H., and Nix, J.R., “Relativistic Hydrodynamic Theory of Heavy-Ion Collisions”, Phys. Rev. Lett., 35, 905–908, (1975). Related online version (cited on 14 December 2006):
External Linkhttp://adsabs.harvard.edu/abs/1975PhRvL..35..905A
3 Amsden, A.A., Harlow, F.H., and Nix, J.R., “Relativistic Nuclear Fluid Dynamics”, Phys. Rev. C, 15, 2059–2071, (1977). Related online version (cited on 14 December 2006):
External Linkhttp://adsabs.harvard.edu/abs/1977PhRvC..15.2059A
4 Andersson, N., “TOPICAL REVIEW: Gravitational Waves from Instabilities in Relativistic Stars”, Class. Quantum Grav., 20, 105–144, (2003). Related online version (cited on 14 December 2006):
External Linkhttp://adsabs.harvard.edu/abs/2002astro.ph.11057A
5 Andersson, N., and Comer, G.L., “On the Dynamics of Superfluid Neutron Star Cores”, Mon. Not. R. Astron. Soc., 328, 1129–1143, (2005). Related online version (cited on 14 December 2006):
External Linkhttp://arXiv.org/abs/astro-ph/0101193
6 Andersson, N., and Comer, G.L., “A Flux-Conservative Formalism for Convective and Dissipative Multi-Fluid Systems, with Application to Newtonian Superfluid Neutron Stars”, Class. Quantum Grav., 23, 5505–5529, (2006)
7 Andersson, N., Comer, G.L., and Grosart, K., “Lagrangian Perturbation Theory of Non-relativistic Rotating Superfluid Stars”, Mon. Not. R. Astron. Soc., 355, 918–928, (2004)
8 Andreev, A.F., and Bashkin, E.P., “Three-Velocity Hydrodynamics of Superfluid Solutions”, Zh. Eksp. Teor. Fiz., 69, 319–326, (1975)
9 Anile, A.M., Relativistic fluids and magneto-fluids: With applications in astrophysics and plasma physics, Cambridge Monographs on Mathematical Physics, (Cambridge University Press, Cambridge, U.K.; New York, U.S.A., 1989)
10 Arnold, V.I., Mathematical Methods of Classical Mechanics, vol. 60 of Graduate Texts in Mathematics, (Springer, Berlin, Germany; New York, U.S.A., 1995), 2nd edition
11 Bekenstein, J.D., “Helicity Conservation Laws for Fluids and Plasmas”, Astrophys. J., 319, 207–214, (1987). Related online version (cited on 14 December 2006):
External Linkhttp://adsabs.harvard.edu/abs/1987ApJ...319..207B
12 Belenkij, S.Z., and Landau, L.D., “Hydrodynamic Theory of Multiple Production of Particles”, Usp. Fiz. Nauk, 56, 309, (1955)
13 Birrell, N.D., and Davies, P.C.W., Quantum fields in curved space, Cambridge Monographs on Mathematical Physics, (Cambridge University Press, Cambridge, U.K.; New York, U.S.A., 1982)
14 Bonazzola, S., Gourgoulhon, E., Salgado, M., and Marck, J.-A., “Axisymmetric rotating relativistic bodies: a new numerical approach for ‘exact’ solutions”, Astron. Astrophys., 278, 421–443, (1993)
15 Carruthers, P., “Heretical Models of Particle Production”, Ann. N.Y. Acad. Sci., 229, 91–123, (1974)
16 Carter, B., “The Commutation Property of a Stationary, Axisymmetric System”, Commun. Math. Phys., 17, 233–238, (1970). Related online version (cited on 14 December 2006):
External Linkhttp://projecteuclid.org/getRecord?id=euclid.cmp/1103842335
17 Carter, B., “The Canonical Treatment of Heat Conduction and Superfluidity in Relativistic Hydrodynamics”, in Dadhich, N., Rao, J.K., Narlikar, J.V., and Vishveshwara, C.V., eds., A Random Walk in General Relativity and Cosmology: Festschrift for Professors P.C. Vaidya & A.K. Raychaudhuri, 49–62, (Wiley Eastern, New Delhi, India, 1983)
18 Carter, B., “Conductivity with Causality in Relativistic Hydrodynamics: The Regular Solution to Eckart’s Problem”, in Iyer, B.R., Kembhavi, A., Narlikar, J.V., and Vishveshwara, C.V., eds., Highlights in Gravitation and Cosmology, Proceedings of the International Conference on Gravitation and Cosmology, Goa, India, 14–19 December 1987,  58, (Cambridge University Press, Cambridge, U.K.; New York, U.S.A., 1988)
19 Carter, B., “Covariant Theory of Conductivity in Ideal Fluid or Solid Media”, in Anile, A., and Choquet-Bruhat, M., eds., Relativistic Fluid Dynamics, Lectures given at the 1st 1987 session of the Centro Internazionale Matematico Estivo (C.I.M.E.) held at Noto, Italy, May 25 – June 3, 1987, vol. 1385 of Lecture Notes in Mathematics, 1–64, (Springer, Berlin, Germany; New York, U.S.A., 1989)
20 Carter, B., “Convective Variational Approach to Relativistic Thermodynamics of Dissipative Fluids”, Proc. R. Soc. London, Ser. A, 433, 45, (1991)
21 Carter, B., “Basic Brane Theory”, Class. Quantum Grav., 9, 19–33, (1992)
22 Carter, B., and Chamel, N., “Covariant Analysis of Newtonian Multi-fluid Models for Neutron Stars: I. Milne–Cartan Structure and Variational Formulation”, Int. J. Mod. Phys. D, 13, 291–326, (2004)
23 Carter, B., and Chamel, N., “Covariant Analysis of Newtonian Multi-Fluid Models for Neutron Stars: II. Stress-Energy Tensors and Virial Theorems”, Int. J. Mod. Phys. D, 14, 717–748, (2005)
24 Carter, B., and Chamel, N., “Covariant Analysis of Newtonian Multi-fluid Models for Neutron stars: III. Transvective, Viscous, and Superfluid Drag Dissipation”, Int. J. Mod. Phys. D, 14, 749–774, (2005)
25 Carter, B., and Khalatnikov, I.M., “Momentum, Vorticity and Helicity in Covariant Superfluid Dynamics”, Ann. Phys. (N.Y.), 219, 243–265, (1992)
26 Carter, B., and Khalatnikov, I.M., “Canonically Covariant Formulation of Landau’s Newtonian Superfluid Dynamics”, Rev. Math. Phys., 6, 277–304, (1994)
27 Carter, B., and Langlois, D., “The Equation of State for Cool Relativisitic Two Constituent Superfluid Dynamics”, Phys. Rev. D, 51, 5855–5864, (1995)
28 Carter, B., and Langlois, D., “Kalb–Ramond Coupled Vortex Fibration Model for Relativistic Superfluid Dynamics”, Nucl. Phys. B, 454, 402–424, (1995)
29 Carter, B., and Langlois, D., “Relativistic Models for Superconducting-Superfluid Mixtures”, Nucl. Phys. B, 531, 478–504, (1998)
30 Chandrasekhar, S., “Solutions of Two Problems in the Theory of Gravitational Radiation”, Phys. Rev. Lett., 24, 611–615, (1970)
31 Chandrasekhar, S., and Friedman, J.L., “On the Stability of Axisymmetric Systems to Axisymmetric Perturbations in General Relativity. I. The Equations Governing Nonstationary, Stationary, and Perturbed Systems”, Astrophys. J., 175, 379–405, (1972)
32 Chandrasekhar, S., and Friedman, J.L., “On the Stability of Axisymmetric Systems to Axisymmetric Perturbations in General Relativity. II. A Criterion for the Onset of Instability in Uniformly Rotating Configurations and the Frequency of the Fundamental Mode in Case of Slow Rotation”, Astrophys. J., 176, 745–768, (1972). Related online version (cited on 28 April 2006):
External Linkhttp://adsabs.harvard.edu/abs/1972ApJ...176..745C
33 Clare, R.B., and Strottman, D., “Relativistic hydrodynamics and heavy ion reactions”, Phys. Rep., 141, 177–280, (1986)
34 Comer, G.L., “Do Neutron Star Gravitational Waves Carry Superfluid Imprints?”, Found. Phys., 32, 1903–1942, (2002). Related online version (cited on 29 July 2002):
External Linkhttp://arXiv.org/abs/astro-ph/0207608
35 Comer, G.L., and Joynt, R., “Relativistic mean field model for entrainment in general relativistic superfluid neutron stars”, Phys. Rev. D, 68, 12, 023002, (2003). Related online version (cited on 28 April 2006):
External Linkhttp://adsabs.harvard.edu/abs/2003PhRvD..68b3002C
36 Comer, G.L., and Langlois, D., “Hamiltonian Formulation for Multi-constituent Relativistic Perfect Fluids”, Class. Quantum Grav., 10, 2317–2327, (1993)
37 Comer, G.L., and Langlois, D., “Hamiltonian Formulation for Relativistic Superfluids”, Class. Quantum Grav., 11, 709–721, (1994)
38 Comer, G.L., Langlois, D., and Lin, L.M., “Quasinormal modes of general relativistic superfluid neutron stars”, Phys. Rev. D, 60, 1–20, 104025, (1999)
39 Eckart, C., “The Thermodynamics of Irreversible Processes. III. Relativistic Theory of the Simple Fluid”, Phys. Rev., 58, 919–924, (1940)
40 Elze, H.-T., Hama, Y., Kodama, T., Makler, M., and Rafelski, J., “Variational Principle for Relativistic Fluid Dynamics”, J. Phys. G, 25, 1935–1957, (1999)
41 Epstein, R.I., “Acoustic Properties of Neutron Stars”, Astrophys. J., 333, 880–894, (1988). Related online version (cited on 29 April 2006):
External Linkhttp://adsabs.harvard.edu/abs/1988ApJ...333..880E
42 Friedman, J.L., “Generic Instability of Rotating Relativistic Stars”, Commun. Math. Phys., 62, 247–278, (1978)
43 Friedman, J.L., and Schutz, B.F., “On the Stability of Relativistic Systems”, Astrophys. J., 200, 204–220, (1975). Related online version (cited on 28 April 2006):
External Linkhttp://adsabs.harvard.edu/abs/1975ApJ...200..204F
44 Friedman, J.L., and Schutz, B.F., “Lagrangian Perturbation Theory of Nonrelativistic Fluids”, Astrophys. J., 221, 937–957, (1978). Related online version (cited on 28 April 2006):
External Linkhttp://adsabs.harvard.edu/abs/1978ApJ...221..937F
45 Friedman, J.L., and Schutz, B.F., “Secular Instability of Rotating Newtonian Stars”, Astrophys. J., 222, 281–296, (1978). Related online version (cited on 28 April 2006):
External Linkhttp://adsabs.harvard.edu/abs/1978ApJ...222..281F
46 Gad-el Hak, M., “Fluid Mechanics from the Beginning to the Third Millennium”, Int. J. Engng. Ed., 14, 177–185, (1998)
47 Geroch, R., “Relativistic theories of dissipative fluids”, J. Math. Phys., 36, 4226–4241, (1995)
48 Glendenning, N.K., Compact Stars: Nuclear Physics, Particle Physics and General Relativity, Astronomy and Astrophysics Library, (Springer, New York, U.S.A.; Berlin, Germany, 1997)
49 Gourgoulhon, E., “An Introduction to Relativistic Hydrodynamics”, in Rieutord, M., and Dubrulle, B., eds., Stellar Fluid Dynamics and Numerical Simulations: From the Sun to Neutron Stars, Aussois and Cargèse, France, September 2004 and May 2005, EAS Publications Series, 43–79, (EDP Sciences, Les Ulis, France, 2006). Related online version (cited on 28 April 2006):
External Linkhttp://arXiv.org/abs/gr-qc/0603009
50 Grad, H., “On the Kinetic Theory of Rarefied Gases”, Commun. Pure Appl. Math., 2, 331–407, (1949)
51 Hartle, J.B., Gravity: An Introduction to Einstein’s General Relativity, (Addison Wesley, San Francisco, U.S.A., 2003)
52