Chaplygin gas

Chaplygin gas,[1][2] which occurs in certain theories of cosmology, is a hypothetical substance that satisfies an exotic equation of state in the form p = A / ρ α {\displaystyle p=-A/\rho ^{\alpha }} , where p {\displaystyle p} is the pressure, ρ {\displaystyle \rho } is the density, with α = 1 {\displaystyle \alpha =1} and A {\displaystyle A} a positive constant. The substance is named after Sergey Chaplygin.

In some models, generalized Chaplygin gas is considered, where α {\displaystyle \alpha } is a parameter, which can take on values 0 < α 1 {\displaystyle 0<\alpha \leq 1} .

See also

  • iconPhysics portal
  • Dark fluid

References

  1. ^ Kamenshchik, Alexander Yu.; Moschellai, Ugo; Pasquier, Vincent (2001), "An alternative to quintessence", Phys. Lett. B, 511 (2–4): 265, arXiv:gr-qc/0103004, Bibcode:2001PhLB..511..265K, doi:10.1016/S0370-2693(01)00571-8, S2CID 14097770
  2. ^ Bento, M. C.; Bertolami, O.; Sen, A. A. (2002), "Generalized Chaplygin gas, accelerated expansion and dark energy-matter unification", Phys. Rev., 66 (4): 043507, arXiv:gr-qc/0202064, Bibcode:2002PhRvD..66d3507B, doi:10.1103/PhysRevD.66.043507, S2CID 119357931


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