@article{AIHPA_1968__9_1_17_0, author = {Droz-Vincent, Philippe and Hakim, R\'emi}, title = {Collective motions of the relativistic gravitational gas}, journal = {Annales de l'I.H.P. Physique th\'eorique}, volume = {8}, year = {1968}, pages = {17-33}, language = {en}, url = {http://dml.mathdoc.fr/item/AIHPA_1968__9_1_17_0} }
Droz-Vincent, Ph.; Hakim, Rémi. Collective motions of the relativistic gravitational gas. Annales de l'I.H.P. Physique théorique, Tome 8 (1968) pp. 17-33. http://gdmltest.u-ga.fr/item/AIHPA_1968__9_1_17_0/
[1] Einstein's Random Equations, to be published.
,[2] 122, 1961, p. 1342. | MR 122525 | Zbl 0103.22706
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, Ann. Phys., t.[3] 8, 1967, p. 1153 ; Ibid. , t. 8, 1967, p. 1379.
, J. Math. Phys., t.See also, Ann. Inst. H. Poincaré, t. 6, 1967, p. 225. | Numdam | Zbl 0155.32601
[4] Phase space is always the tangent fibre bundle of the manifold configuration space.
[5] Actually E is 6-dimensional if we bear in mind the constraint (2).
[6] Since μ is the tangent bundle of a metric manifold (i. e. U4), then on this space one can construct a canonical metric tensor GAB. See the article by Lindquist (Ref. [2]) and references quoted therein.
[7] By « effective volume » we mean a 6-dimensional volume. This conservation law, i. e. the Liouville theorem, means that if Δ1 ⊂ Σ1 is such a 6-dimensional volume, then mes (Δ1) = mes (Δ2) where Δ2 is the « volume » in Σ2 obtained from the transformation of Δ1 under the group motion (i. e. Eq. (3)).
[8] Such as those given by 128, 1962, p. 398. | Zbl 0111.42104
and , Phys. Rev., t.[9] This would be only a simple generalization of previous results where the electromagnetic radiation was dealt with (See Ref. [3] and also Relativistic kinetic equations including radiation effects I. Vlasov approximation (to appear in J. Math. Phys., 9, 116 (1968)). | Zbl 0173.30402
and ,[10] Numdam | Zbl 0098.42607
, Propagateurs et commutateurs en relativité générale (Publications. Mathématiques n° 10 de l'I. H. E. S.), p. 40. |[11] We mainsly use the notations of Ref [10].
[12] Ref. [10], p. 43.
[13] Ref. [10], p. 27.
[14] Ref. [10], p. 39.
[15] In the same way as neglecting correlations of electromagnetic field or of particles amounts to dealing with a kinetic equation valid at order ∼ e2, neglecting correlations of the gravitational field is expected to provide a kinetic equation valid at order χ. We verify this statement on the resulting equation.
[16] Ref. [10], p. 33.
[17] 9, 1960, p. 220. | Zbl 0092.45003
, Ann. Phys., t.[18] Ref. [10], p. 30.
[19] Ref. [10], p. 35.