Summary
Relativistic superfluids are of interest in extreme astrophysical or cosmological situations. Some of their properties, ultrabaricity in particular, are studied by means of exact solutions of Einstein’s equations. Those found are almost invariably characterized by equations of state of the typeP = αϱ + const with 0 ≤ α ≤ 1 and ϱ proportional to the square of the number density. They are therefore neither ultrabaric (P > ϱ nor superluminal (v S > 1). Exceptions are, however, represented by the generalized interior Schwarzschild solution, the Stephani solution and a new conformally flat solution also of the Stephani type. For these superluminality is allowed if no assumptions are introduced regarding the mechanism of propagation of sound waves. In the one with Stephani metric, transitions can occur in principle from evolutionary stages withv S > 1 to others withv S < 1, andvice versa.
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References
See, for instance, the most comprehensive treatiseExact Solutions of Einstein’s Field Equations byD. Kramer, H. Stephani, M. McCallum andE. Herlt (Berlin, 1980).
G. Bayn andC. Pethick:Ann. Rev. Astron. Astrophys.,17, 415 (1979).
V. A. Kuzmin andM. E. Shaposhnikov:Phys. Lett. A,69, 462 (1979).
D. J. Gross, M. J. Perry andL. G. Yaffe:Phys. Rev. D,25, 330 (1980);Y. Kikuchi, T. Moriya andH. Tsukahara:Phys. Rev. D,29, 2220 (1984).
G. Papini andM. Weiss:Phys. Lett. A,89, 329 (1982).
A. H. Guth:Phys. Rev. D,23, 347 (1981).
W. Pauli:Theory of Relativity (New York, N. Y., 1958).
S. A. Bludman andM. A. Ruderman:Phys. Rev.,170, 1176 (1968);M. Ruderman:Phys. Rev.,172, 1286 (1968);S. A. Bludman andM. A. Rudermann:Phys. Rev. D,1, 3243 (1970);S. A. Bludman,Equations of state of ultradense relativislic matter, inProc. S.I.F., Course LIV (New York, N. Y., 1972).
G. Caporaso andK. Brecher:Phys. Rev. D,20, 1823 (1979).
E. N. Glass:Phys. Rev. D,28, 2693 (1983);G. Caporaso andK. Brecher:Phys. Rev. D,28, 2694 (1983).
G. F. R. Ellis Relativistic Cosmology, inCargèse Lect. Phys., Vol. 6 (New York, N. Y., 1973), p. 1.
W. Israel:Quantum Grav ity, inProceedings of the Third Moscow Seminar, edited byM. A. Markov andV. P. Frolov (Singapore, 1985), in press.
F. Rothen:Helv. Phys. Acta,11, 591 (1968);W. Israel:Phys. Lett. A,86, 79 (1981).
H. Stephani:Comm. Math. Phys.,4, 137 (1967) and ref. (’).
R. Tabenskt:Some Exact Solutions in Relativistic Hydrodynamics, Ph. D. Thesis, University of California (1972).
J. A. Allnutt:Gen. Bel. Grav.,13, 1017 (1981).
P. Letelier andR. Tabensky:J. Math. Phys.,16, 8 (1975).
F. Wainwright:Commun. Math. Phys.,17, 42 (1970).
A. Barnes:J. Phys. A,5, 374 (1972).
J. Ibanez andJ. L. Sanz:J. Math. Phys.,23, 1364 (1982).
A. H. Taub:Plane symmetric similarity solutions for self-gravitating fluids, inGeneral Relativity, Papers in Honour ofJ. L. Synge andL. O’Raifeartaigh (Editor, Oxford, 1972).
A. F. da Teixeira, I. Wolk andM. M. Som:J. Phys. A,10, 1679 (1977).
H. Stephani:Commun. Math. Phys.,4, 137 (1967);D. Kramer, G. Neugebauer andH. Stephani:Fortschr. Phys.,20, 1 (1972).
E. M. Lifschitz andL. P. Pitaevskii:Statistical Physics, Part 2 (Oxford, 1980), p. 101.
E. M. Lifschitz andL. P. Pitaevskii:Statistical Physics, Part 1 (Oxford, 1980), p. 178.
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Research supported in part by the Natural Sciences and Engineering Research. Council of Canada.
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Papini, G., Weiss, M. Ultrabaric relativistic superfluids. Lett. Nuovo Cimento 44, 83–87 (1985). https://doi.org/10.1007/BF02746993
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DOI: https://doi.org/10.1007/BF02746993