Our results provide a first step to make the formal analysis rigorous in terms of 1 c2 proposed by Chandrasekhar [S. Chandrasekhar, The post-Newtonian equations of hydrodynamics in general relativity, Astrophys. J. 142 (1965) 1488-1512; S. Chandrasekhar, post-Newtonian equations of hydrodynamics and the stability of gaseous masses in general relativity, Phys. Rev. Lett. 14 (1965) 241-244], motivated by the methods of Einstein, Infeld and Hoffmann, see Thorne [K. S. Thorne, The general-relativistic theory of stellar structure and dynamics, in Proc. Int. School of Physics "Enrico Fermi," Course XXXV, at Varenna, Italy, July 12-24, 1965, ed. L. Gratton (Academic Press, 1966), pp. 166-280]. We consider the non-relativistic limit for the local smooth solutions to the free boundary value problem of the cylindrically symmetric relativistic Euler equations when the mass energy density includes the vacuum states at the free boundary. For large enough (rescaled) speed of light c and suitably small time T, we obtain uniform, with respect to c, "a priori" estimates for the local smooth solutions. Moreover, the smooth solutions of the cylindrically symmetric relativistic Euler equations converge to the solutions of the classical compressible Euler equation at the rate of order 1 c2.

Non-relativistic limit analysis of the Chandrasekhar-Thorne relativistic Euler equations with physical vacuum

Marcati, Pierangelo
2019

Abstract

Our results provide a first step to make the formal analysis rigorous in terms of 1 c2 proposed by Chandrasekhar [S. Chandrasekhar, The post-Newtonian equations of hydrodynamics in general relativity, Astrophys. J. 142 (1965) 1488-1512; S. Chandrasekhar, post-Newtonian equations of hydrodynamics and the stability of gaseous masses in general relativity, Phys. Rev. Lett. 14 (1965) 241-244], motivated by the methods of Einstein, Infeld and Hoffmann, see Thorne [K. S. Thorne, The general-relativistic theory of stellar structure and dynamics, in Proc. Int. School of Physics "Enrico Fermi," Course XXXV, at Varenna, Italy, July 12-24, 1965, ed. L. Gratton (Academic Press, 1966), pp. 166-280]. We consider the non-relativistic limit for the local smooth solutions to the free boundary value problem of the cylindrically symmetric relativistic Euler equations when the mass energy density includes the vacuum states at the free boundary. For large enough (rescaled) speed of light c and suitably small time T, we obtain uniform, with respect to c, "a priori" estimates for the local smooth solutions. Moreover, the smooth solutions of the cylindrically symmetric relativistic Euler equations converge to the solutions of the classical compressible Euler equation at the rate of order 1 c2.
local smooth solution; non-relativistic limits; physical vacuum; Relativistic Euler equations; Modeling and Simulation; Applied Mathematics
File in questo prodotto:
File Dimensione Formato  
2019_MathModelsMethodsApplSci_29_Mai.pdf

non disponibili

Descrizione: PDF
Tipologia: Versione Editoriale (PDF)
Licenza: Non pubblico
Dimensione 760.28 kB
Formato Adobe PDF
760.28 kB Adobe PDF   Visualizza/Apri   Richiedi una copia

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/20.500.12571/1864
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 5
  • ???jsp.display-item.citation.isi??? 4
social impact