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DISCRETE SUBGROUPS OF VECTOR SPACES AND LATTICES
DISCRETE SUBGROUPS OF VECTOR SPACES AND LATTICES

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14. The minimal polynomial For an example of a matrix which

... that φ is nilpotent if φk = 0 for some positive integer k. The smallest such integer is called the order of φ. We say that a matrix is nilpotent if the corresponding linear function is nilpotent. Almost by definition, if A and B are similar matrices then A is nilpotent if and only if B is nilpotent ...
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What are Kepler`s Laws?

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Components of Forces - Secrets of Engineering Mechanics

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MA 3280 Lecture 12 - Bases for a Homogeneous System Monday

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... there are 20 of them that are independent. This saves some time, in D = 4 it is still a lot of them, and we will have to use tricks every time to make it manageable. But is is good to know how to identify these. Take D = 3, where we have to repeat at least one index (since there are 3 different ones ...
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Fundamental Theorems

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rotational dynamics

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Notes on fast matrix multiplcation and inversion

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Fourier analysis on finite groups and Schur orthogonality

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Linear Algebra Libraries: BLAS, LAPACK - svmoore

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Massachusetts Institute of Technology Guido Kuersteiner

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lecture3

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Four-vector

In the theory of relativity, a four-vector or 4-vector is a vector in Minkowski space, a four-dimensional real vector space. It differs from a Euclidean vector in how its magnitude is determined. The transformations that preserve this magnitude are the Lorentz transformations, which include spatial rotations, boosts (a change by a constant velocity to another inertial reference frame), and temporal and spatial inversions. Regarded as a homogeneous space, the transformation group of Minkowski space is the Poincaré group, which adds to the Lorentz group the group of translations. The Lorentz group may be represented by 4×4 matrices.The article considers four-vectors in the context of special relativity. Although the concept of four-vectors also extends to general relativity, some of the results stated in this article require modification in general relativity.
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