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- Noriyasu Mori, Denys Schmitt, +4 authors Michihiro Morikawa
- Physical review. E, Statistical, nonlinear, andâ€¦
- 2013

We solve the equations of motion of a one-dimensional planar Heisenberg (or Vaks-Larkin) model consisting of a system of interacting macrospins aligned along a ring. Each spin has unit length and isâ€¦ (More)

- Hideaki Mouri
- Physical review. E, Statistical, nonlinear, andâ€¦
- 2013

The central limit theorem ensures that a sum of random variables tends to a Gaussian distribution as their total number tends to infinity. However, for a class of positive random variables, we findâ€¦ (More)

- Hideaki Mouri
- 2002

Mass segregation in a star cluster is studied in an analytical manner. We consider a two-component cluster, which consists of two types of stars with different masses. Plummerâ€™s model is used for theâ€¦ (More)

- Hideaki Mouri, Akihiro Hori, Yoshihide Kawashima
- Physical review. E, Statistical, nonlinear, andâ€¦
- 2004

The most elementary structures of turbulence, i.e., vortex tubes, are studied using velocity data obtained in a laboratory experiment for boundary layers with Reynolds numbers Re(lambda) =295-1258 .â€¦ (More)

- Hideaki Mouri, Masanori Takaoka, Akihiro Hori, Yoshihide Kawashima
- Physical review. E, Statistical, nonlinear, andâ€¦
- 2002

The probability density function (PDF) of velocity fluctuations is studied experimentally for grid turbulence in a systematical manner. At small distances from the grid, where the turbulence is stillâ€¦ (More)

- Hideaki Mouri, Akihiro Hori, Yoshihide Kawashima, Kosuke Hashimoto
- Physical review. E, Statistical, nonlinear, andâ€¦
- 2012

The mean rate of energy dissipation [Îµ] per unit mass of turbulence is often written in the form of [Îµ]=C(u)[u(2)](3/2)/L(u), where the root-mean-square velocity fluctuation [u(2)](1/2) and theâ€¦ (More)

Using the initial peculiar velocity field, we analytically study the hierarchical formation of gravitationally bound objects. The field is smoothed over a scale that corresponds to the mass of aâ€¦ (More)

The probability density function of single-point velocity fluctuations in turbulence is studied systematically using Fourier coefficients in the energy-containing range. In ideal turbulence whereâ€¦ (More)

Old starburst galaxies are deficient in O stars, and hence do not exhibit strong line emission in the optical regime. However, there remain many B stars, which are expected to heat dust grains andâ€¦ (More)

Galaxy interactions are studied in terms of the starburst-Seyfert connection. The starburst requires a high rate of gas supply. Since the efficiency for supplying the gas is high in a galaxyâ€¦ (More)