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Rigid body

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In physics, a rigid body is an idealization of a solid body of finite size in which deformation is neglected. In other words, the distance between any two given points of a rigid body remains constant regardless of external forces exerted on it.

The configuration space of a rigid body with one point fixed is given by the underlying manifold of the rotation group SO(3). The configuration space of a nonfixed rigid body is E+(n), the subgroup of direct isometries of the Euclidean group (combinations of translations and rotations).

For any particle of a moving and spinning body we have

[ \mathbf(t,\mathbf_0) = \mathbf_c(t) + A(t) \mathbf_0 ]
[ \mathbf(t,\mathbf_0) = \mathbf_c(t) + \boldsymbol\omega(t) \times (\mathbf(t,\mathbf_0) - \mathbf_c(t)) = \mathbf_c(t) + \boldsymbol\omega(t) \times A(t) \mathbf_0 ]
[ A'(t)\mathbf_0 = \boldsymbol\omega(t) \times A(t)\mathbf_0 ]
where To describe the motion the reference point can be any particle of the body or imaginary point that is rigidly connected to the body (the translation vector depends on the choice). Depending on the application a convenient choice may be: When the cross product
[\boldsymbol\omega(t) \times A(t)\mathbf_0 ]
is written as a matrix multiplication, this matrix is a skew-symmetric matrix with zeros on the main diagonal and plus and minus the components of the angular velocity as the other elements.

In 2D the matrix A(t) simply represents a rotation in the xy-plane by an angle which is the integral of the scalar angular velocity over time.

Vehicles, walking people, etc. usually rotate according to changes in the direction of the velocity: they move forward with respect to their own orientation. Then, if the body follows a closed orbit in a plane, the angular velocity integrated over a time interval in which the orbit is completed once, is an integer times 360°. This integer is the winding number with respect to the origin of the velocity. Compare the amount of rotation associated with the vertices of a polygon.

The orientation can also be described in a different way, e.g. as a unit-quaternion-valued function of time. Although the latter is specific up to a factor -1, it would be reasonable to choose it continuously.

Two rigid bodies are said to be different (not copies) is that there is no proper rotation from one to the other. A rigid body is called chiral if its mirror image is different in that sense, i.e., if it has either no symmetry or its symmetry group contains only proper rotations. In the opposite case an object is called achiral: the mirror image is a copy, not a different object. Such an object may have a symmetry plane, but not necessarily: there may also be a plane of reflection with respect to which the image of the object is a rotated version. The latter applies for S2n, of which the case n = 1 is inversion symmetry.

For a (rigid) rectangular transparent sheet, inversion symmetry corresponds to having on one side an image without rotational symmetry and on the other side an image such that what shines through is the image at the top side, upside down. We can distinguish two cases:

A sheet with a through and through image is achiral. We can distinguish again two cases:

See also

 


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