Astronomy:Chaplygin gas
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Short description: Hypothetical substance used in certain cosmological theories
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 , where is the pressure, is the density, with and a positive constant. The substance is named after Sergey Chaplygin.
In some models, generalized Chaplygin gas is considered, where is a parameter, which can take on values .
A slowly rotating spherically symmetric, non-viscous, self-gravitating Chapligin gas solves the Hubble tension.[3]
See also
References
- ↑ Kamenshchik, Alexander Yu.; Moschellai, Ugo; Pasquier, Vincent (2001), "An alternative to quintessence", Phys. Lett. B 511 (2–4): 265, doi:10.1016/S0370-2693(01)00571-8, Bibcode: 2001PhLB..511..265K
- ↑ Bento, M. C.; Bertolami, O.; Sen, A. A. (2002), "Generalized Chaplygin gas, accelerated expansion and dark energy-matter unification", Phys. Rev. 66 (4), doi:10.1103/PhysRevD.66.043507, Bibcode: 2002PhRvD..66d3507B
- ↑ Szigeti, Balázs Endre; Szapudi, István; Barna, Imre Ferenc; Barnaföldi, Gergely Gábor (2025). "Can Rotation Solve the Hubble Puzzle?". Monthly Notices of the Royal Astronomical Society 538 (4): 3038–3041. doi:10.1093/mnras/staf446. https://academic.oup.com/mnras/article/538/4/3038/8090496.
