Hu W, Peebles PJ
Astrophys J. 2000 Jan 10;528(2):L61-L64. doi: 10.1086/312442.
This model assumes the baryons, radiation, three families of massless neutrinos, and cold dark matter were mutually thermalized before the baryon number was fixed, primeval curvature fluctuations were subdominant, and homogeneity was broken by scale-invariant fluctuations in a new dark matter component that behaves like a relativistic ideal fluid. The fluid behavior could follow if this new component were a single scalar field that interacts only with gravity and with itself by a pure quartic potential. The initial energy distribution could follow if this component were gravitationally produced by inflation. The power spectra of the present distributions of mass and radiation in this model are not inconsistent with the measurements but are sufficiently different from the adiabatic cold dark matter model to allow a sharp test in the near future.
该模型假定,在重子数确定之前,重子、辐射、三代无质量中微子以及冷暗物质相互热化,原初曲率涨落处于次要地位,并且均匀性被一种新暗物质成分中的标度不变涨落打破,这种新暗物质成分表现得像一种相对论性理想流体。如果这种新成分是一个仅通过纯四次势与引力以及自身相互作用的单标量场,那么流体行为就能成立。如果这种成分是由暴胀引力产生的,那么初始能量分布就能成立。该模型中质量和辐射当前分布的功率谱与测量结果并不矛盾,但与绝热冷暗物质模型有足够差异,从而在不久的将来能进行严格检验。