tspiral structure

En résumé (grâce à un LLM libre auto-hébergé)

  • The text deals with the spiral structure in the context of astrophysics.
  • It presents mathematical equations describing the behavior of matter distributions and velocity ellipses.
  • Concepts such as mass density, thermal velocities, and characteristic lengths are introduced.

spiral structure ghost matter astrophysics.6: Spiral structure. (p4) Returning to the first-order terms, we have: (15)

In polar coordinates: (16)

The third-order terms vanish. (17)

i.e.: (18)

The 2D distribution function is: (19)

And the axis of the velocity ellipse follows: (20)

Then, introducing the number density n(ρ), we obtain: (21)

and: (22)

In the twin fold F*, we also adopt a solution of the Eddington type. (23)

(24)

(25)

(26)

According to reference [1], we know that the Poisson equation is written as: (27)

where φ is the gravitational potential. ρ₁ is the mass density in the first fold and ρ₂ is the mass density in the second fold. The final differential equation for this axially symmetric system is: (28)

Introduce: (29)

where V₀ and V₀* are characteristic velocities. Introduce the following dimensionless quantities: (30)

Let us write the axis of the velocity ellipses as: (31)

We then obtain the Poisson differential equation, referring to a non-rotating axisymmetric system, expressed in terms of dimensionless parameters ρ, ξ, η, and ζ: (32)

  • η represents the importance of the twin structure (characteristic mass ratio).

  • ξ is the ratio of the thermal velocities in the two adjacent folds F and F*.

  • ρ and ζ refer to the characteristic lengths (equivalent to the Jeans length) in the two populations.

The mass densities, written in dimensionless form, obey: (33)

Initial conditions, for numerical computation, will be given for η = 0. Then: (34)

Strictly speaking, this is not physical, since the -motions are essentially neglected, but 2D simulations are not physical either. We construct this material in order to drive numerical 2D simulations, seeking, as a starting point, steady-state conditions.