Tidal Forces/Fields: Analyzing N-Body Simulation Data

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In summary, the person is working on analyzing N-body simulation data and is trying to calculate the tidal forces exerted on smaller groups of particles. They have a model for the distribution of matter and can analytically calculate the gravitational potential and directional second derivatives, but are unsure of how to translate that into forces. They ask for a reference on the subject and another person provides information on how to calculate the forces using a potential and unit vector. They also mention that the partial derivatives should normally commute and reference Clairaut's theorem for more information.
  • #1
Allday
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Hey people,

Im doing some analysis of some N-body simulation data. I'm trying to calculate the tidal forces exerted on the smaller groups of particles by the other mass. I have a model for the distribution of matter causing the tidal field so I can analytically calculate the gravitational potential and the directional second derivatives, but how do I translate that into the forces. Anybody have a reference for some good reading on the subject.
 
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  • #2
Allday said:
Hey people,

Im doing some analysis of some N-body simulation data. I'm trying to calculate the tidal forces exerted on the smaller groups of particles by the other mass. I have a model for the distribution of matter causing the tidal field so I can analytically calculate the gravitational potential and the directional second derivatives, but how do I translate that into the forces. Anybody have a reference for some good reading on the subject.

Well if you have a potential V(x,y,z) then the force in cartesian coordinates (x,y,z) is given by
[tex]
F_x = \frac{\partial{V}}{\partial{x}} \hspace{.25 in} F_y = \frac{\partial{V}}{\partial{y}} \hspace{.25 in} F_z = \frac{\partial{V}}{\partial{z}}
[/tex]

and if you have a unit vector U, the tidal force T is another vector, the gradient of the force F in the direction of vector U, given by

[tex]
T_x = \frac{\partial^2{V}}{\partial x \partial x}} U_x +
\frac{\partial^2{V}}{\partial x \partial y}} U_y +
\frac{\partial^2{V}}{\partial x \partial z}} U_z
[/tex]
[tex]
T_y = \frac{\partial^2{V}}{\partial y\partial x}} U_x +
\frac{\partial^2{V}}{\partial y\partial y}} U_y +
\frac{\partial^2{V}}{\partial y\partial z}} U_z
[/tex]
[tex]
T_z = \frac{\partial^2{V}}{\partial z\partial x}} U_x +
\frac{\partial^2{V}}{\partial z\partial y}} U_y +
\frac{\partial^2{V}}{\partial z\partial z}} U_z
[/tex]

You can write this in tensor notation

[tex]
T^i = K^i{}_j U^j
[/tex]

where [tex] K^i{}_j = \frac{\partial^2{V}}{\partial x^i \partial x^j}[/tex]


It gets more complicated if you want to use general (non-cartesian) coordinates

But you can always say that the tidal forces at a point are given by a second rank tensor, one that takes in a vector (the displacement) and spits out a vector (the tidal force).

I *think* that the partial derivates should normally alll commute, so [tex]
\frac{\partial^2 V}{\partial x \partial y} = \frac{\partial^2 V}{\partial y \partial x} [/tex]

Google finds "Clairaut's theorem"

http://planetmath.org/encyclopedia/ClairautsTheorem.html
 
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  • #3


Hi there, it sounds like you are on the right track with your analysis of the N-body simulation data. To calculate the tidal forces, you will need to use the gravitational potential and the directional second derivatives. These can be calculated using mathematical equations, as you mentioned.

To translate this into forces, you will need to use the equation F = -m∇Φ, where F is the force, m is the mass of the smaller group of particles, and ∇Φ is the gradient of the gravitational potential. This will give you the magnitude and direction of the tidal force exerted on the particles.

As for references, I would recommend looking into textbooks or articles on celestial mechanics or astrophysics. You can also find some helpful resources online, such as lectures or tutorials on tidal forces and N-body simulations. Good luck with your analysis!
 

FAQ: Tidal Forces/Fields: Analyzing N-Body Simulation Data

What is the concept of tidal forces and fields?

Tidal forces and fields refer to the gravitational forces and resulting deformations on an object caused by the gravitational pull of another nearby massive object.

How are tidal forces and fields analyzed in N-body simulations?

In N-body simulations, tidal forces and fields are analyzed by tracking the position and velocity of each individual body in the system over time and calculating the resulting gravitational interactions between them.

What factors affect the strength of tidal forces and fields?

The strength of tidal forces and fields is affected by the distance between the objects, their masses, and the distribution of mass within each object.

What are some real-world applications of studying tidal forces and fields?

Studying tidal forces and fields can help us understand the dynamics of celestial bodies such as planets, moons, and stars, as well as the formation and evolution of galaxies and other large-scale structures in the universe.

How can knowledge of tidal forces and fields be used to make predictions?

By analyzing tidal forces and fields, we can make predictions about the orbits and movements of celestial bodies, as well as the effects of gravitational interactions on the structure of the universe. This information can also be used for space missions and spacecraft navigation.

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