2010
DOI: 10.1088/1475-7516/2010/01/011
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Acquired scaling relations in dark matter turbulence

Abstract: Many scaling relations are observed for self-gravitating systems in the universe. We explore the consistent understanding of them from a simple principle based on the proposal that the collisionless dark matter fluid terns into a turbulent state, i.e. dark turbulence, after crossing the caustic surface in the non-linear stage. The dark turbulence will not eddy dominant reflecting the collisionless property. After deriving Kolmogorov scaling laws from Navier-Stokes equation by the method similar to the one for … Show more

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Cited by 4 publications
(3 citation statements)
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“…The scaling relation derived from this equation is applied to various observations such as the scale dependent mass density, L/M ratio, magnetic field distributions, etc. They all consistently point the value ǫ ≈ 0.3cm 2 /sec 3(Nakamichi, & Morikawa. (2010)).…”
mentioning
confidence: 53%
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“…The scaling relation derived from this equation is applied to various observations such as the scale dependent mass density, L/M ratio, magnetic field distributions, etc. They all consistently point the value ǫ ≈ 0.3cm 2 /sec 3(Nakamichi, & Morikawa. (2010)).…”
mentioning
confidence: 53%
“…The latter is the scaling velocity vout ≡ (ǫr) 1/3 , where ǫ is a constant. This is derived by the scaling property of the cosmic turbulence (Nakamichi, & Morikawa. (2010)).…”
Section: Separation Into Globular Clusters and Ellipsoidsmentioning
confidence: 99%
“…However, an appropriate amount of angular momentum may be important to get the coexistence of SMBH and DH, because the whole system would collapse into BH otherwise. In this context, from various observations, the individual angular momentum A of the cosmological objects shows the following scaling [Nakamichi 2010], In our case, if we start from the wave function…”
Section: Collapse With Angular Momentummentioning
confidence: 89%