Relativistic thermodynamic fluid

1970 ◽  
Vol 3 (16) ◽  
pp. 521-525 ◽  
Author(s):  
G. Boillat
Keyword(s):  
Relativistic Thermodynamic

Convective variational approach to relativistic thermodynamics of dissipative fluids

1991 ◽  
Vol 433 (1887) ◽  
pp. 45-62 ◽  
Keyword(s):  
Traditional Approach ◽  
Chemical Constituents ◽  
Momentum Density ◽  
Energy Tensor ◽  
Cauchy Type ◽  
Entropy Current ◽  
Master Function ◽  
Relativistic Thermodynamic ◽  
Set Up ◽  
Generalized Variation

Using guidelines provided by Noether identities arising from a generalized variation procedure of convective type, a new (nonlinear and exactly self-consistent) category of relativistic thermodynamic models is developed for the systematic representation of viscous conducting fluid media (allowing for several independent charged or neutral chemical constituents). Apart from the provision of a set of dissipation coefficients of the usual (reactivity, resistivity, and viscosity) type, the specification of a particular model is determined just by giving the algebraic dependence a single ‘master function’, ͘ Λ say, on the relevant dynamical variables, which are supposed here to consist of an entropy current 4-vector and a set of particle current 4-vectors corresponding to the various chemical constituents, together with a set of symmetric (rank 3) viscosity tensors, which are considered as being dynamically independent of the corresponding current vectors except in the degenerate limit of linear viscosity. The master function is set up as a generalization of an ordinary lagrangian function, to which it reduces in the relevant non - dissipative limit, and, as in the conservative case, it is used for the construction of derived quantities in such a way that appropriate self-consistency conditions are satisfied as identities. In particular the relevant stress-momentum-energy tensor is obtained directly in terms of the independent variables and of their dynamical conjugates (whose role is hidden in the traditional approach as developed by Israel & Stewart), which are set of ordinary 4-momentum (not 4-momentum density) covectors associated with the independent currents, and a set of generalised Cauchy type strain (not strain - rate) tensors associated with the independent viscous stress contributions. The range of application of the category obtained in this way is intended to include that of the standard (Israel-Stewart) formalism to which it is expected to be effectively equivalent in the limit of sufficiently small deviations from thermodynamic equilibrium.

scholarly journals Relativistic polytrope from the collimation and acceleration profiles of the M87 jet at subparsec scales and thermodynamic evidence for the Blandford–Znajek mechanism

2019 ◽  
Vol 489 (1) ◽  
pp. L7-L11
Author(s):  
Denis Nikolaevich Sob’yanin (Денис Николаевич Собьянин)
Keyword(s):  
Lorentz Factor ◽  
Polytropic Index ◽  
Sharp Change ◽  
Exact Nature ◽  
Electromagnetic Structure ◽  
Long Baseline ◽  
Electron Positron ◽  
Relativistic Jet ◽  
Polytropic Equation ◽  
Relativistic Thermodynamic

ABSTRACT Recent Very Long Baseline Interferometry observations of the relativistic jet in the M87 radio galaxy at 43 GHz show gradual relativistic acceleration of the plasma and suggest a linear dependence of Lorentz factor on jet radius at scales up to 8 marcsec (0.65 pc) from the core (2.5 marcsec in projection). General analysis of integrals of motion being unaltered along the jet and reflecting fundamental conservation laws shows that the above dependence implies a polytropic equation of state with index 4/3. The inferred value of the polytropic index appears independent of the exact nature of forces sustaining the transverse balance of the jet and indicates exact conservation of the longitudinal electric current and hence the existence of a stable internal electromagnetic structure at the scales under consideration. At this index the flow is hot and corresponds to relativistic thermodynamic motion of particles. Considerable weakening of the acceleration efficiency after 8 marcsec with the jet form being unchanged can be related to the plasma cooling, when the polytropic index becomes 5/3. Such a sharp change in the index without intermediate delay at 1.44 during cooling favours the existence of an electron–positron plasma and requires at least partial participation of the Blandford–Znajek mechanism in the launching of the M87 jet.

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