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Linear Algebra Terms and Definitions

AAdjugateDeterminantsAAlgebraic MultiplicityEigenAAugmented MatrixLinear SystemsBBack-SubstitutionLinear SystemsBBasisVector SpacesCChange of Basis MatrixTransformationsCCharacteristic PolynomialEigenCCholesky FactorizationOrthogonalityCCoefficient MatrixLinear SystemsCCofactorDeterminantsCCofactor ExpansionDeterminantsCCofactor Matrix (Adjugate)DeterminantsCColumn SpaceVector SpacesCCondition NumberMatricesCConformabilityMatricesCConsistent SystemLinear SystemsCCoordinatesVector SpacesCCramer's RuleDeterminantsCCross ProductVectorsDDefective MatrixEigenDDesign MatrixLinear SystemsDDeterminantDeterminantsDDiagonal MatrixMatricesDDiagonalizable MatrixEigenDDiagonalizationEigenDDimensionVector SpacesDDirectionVectorsDDominant EigenvalueEigenDDot ProductVectorsEEigenspaceEigenEEigenvalueEigenEEigenvectorEigenEElement-wise OperationMatricesEElementary Row OperationLinear SystemsFForward SubstitutionLinear SystemsFFree VariableVector SpacesFFrobenius Inner ProductVectorsFFrobenius NormVectorsFFull RankVector SpacesGGaussian EliminationLinear SystemsGGeometric MultiplicityEigenGGram-Schmidt ProcessOrthogonalityHHadamard ProductVectorsHHomogeneous SystemLinear SystemsIIdempotent MatrixMatricesIIdentity MatrixMatricesIImage (Range)TransformationsIInner ProductOrthogonalityIInner Product SpaceVectorsIInverse MatrixMatricesIInvolutory MatrixMatricesIIsometryVectorsLLeast-Squares SolutionLinear SystemsLLeft Null SpaceVector SpacesLLinear CombinationVectorsLLinear IndependenceVector SpacesLLinear TransformationTransformationsLLU DecompositionLinear SystemsMMagnitude (Norm)VectorsMMain DiagonalMatricesMMatrixMatricesMMatrix RepresentationTransformationsMMatrix Square RootMatricesMMinorDeterminantsNNilpotent MatrixMatricesNNull Space (Kernel)Vector SpacesNNullityVector SpacesOOrientationDeterminantsOOrthogonal ComplementOrthogonalityOOrthogonal DecompositionVectorsOOrthogonal MatrixOrthogonalityOOrthogonal SetOrthogonalityOOrthogonal VectorsOrthogonalityOOrthonormal SetOrthogonalityOOuter ProductVectorsOOverdetermined SystemLinear SystemsPPartial PivotingLinear SystemsPPermutation MatrixMatricesPPivotLinear SystemsPPivot ColumnVector SpacesPPositive Definite MatrixMatricesPProjection MatrixTransformationsPPseudoinverseLinear SystemsQQR DecompositionOrthogonalityQQuadratic FormEigenRRankMatricesRRank-Nullity TheoremVector SpacesRRayleigh QuotientEigenRReduced Row Echelon FormLinear SystemsRReflectionTransformationsRResidualLinear SystemsRRight-Hand RuleVectorsRRotationTransformationsRRow Echelon FormLinear SystemsRRow SpaceVector SpacesSSarrus's RuleDeterminantsSScalarVectorsSScalar MatrixMatricesSSimilar MatricesTransformationsSSingular MatrixMatricesSSingular ValueEigenSSingular Value DecompositionEigenSSkew-Symmetric MatrixMatricesSSpanVector SpacesSSpecial SolutionsVector SpacesSSpectral DecompositionEigenSSpectral NormMatricesSSquare MatrixMatricesSSubspaceVector SpacesSSymmetric MatrixMatricesSSystem of Linear EquationsLinear SystemsTTraceMatricesTTransposeMatricesTTriangular MatrixMatricesUUnit VectorVectorsVVectorVectorsVVector ProjectionVectorsVVector SpaceVector SpacesZZero MatrixMatricesZZero VectorVectors
Determinants(9)
Eigen(15)
Linear Systems(19)
Matrices(25)
Orthogonality(9)
Transformations(8)
Vector Spaces(17)
Vectors(18)
120 of 120 terms
Determinants
DeterminantMinorCofactorCofactor Matrix (Adjugate)Cofactor ExpansionSarrus's RuleAdjugateCramer's RuleOrientation
Eigen
EigenvalueEigenvectorEigenspaceCharacteristic PolynomialAlgebraic MultiplicityGeometric MultiplicitySingular ValueDiagonalizable MatrixDiagonalizationDefective MatrixDominant EigenvalueRayleigh QuotientQuadratic FormSpectral DecompositionSingular Value Decomposition
Linear Systems
System of Linear EquationsAugmented MatrixRow Echelon FormReduced Row Echelon FormPivotHomogeneous SystemCoefficient MatrixElementary Row OperationGaussian EliminationBack-SubstitutionForward SubstitutionPartial PivotingConsistent SystemOverdetermined SystemLU DecompositionLeast-Squares SolutionResidualDesign MatrixPseudoinverse
Matrices
MatrixSquare MatrixIdentity MatrixSymmetric MatrixInverse MatrixSingular MatrixRankTraceDiagonal MatrixPositive Definite MatrixTransposeMain DiagonalZero MatrixScalar MatrixSkew-Symmetric MatrixTriangular MatrixPermutation MatrixNilpotent MatrixIdempotent MatrixInvolutory MatrixConformabilityElement-wise OperationMatrix Square RootSpectral NormCondition Number
Orthogonality
Inner ProductOrthogonal VectorsOrthogonal SetOrthonormal SetOrthogonal ComplementOrthogonal MatrixGram-Schmidt ProcessQR DecompositionCholesky Factorization
Transformations
Linear TransformationImage (Range)Matrix RepresentationChange of Basis MatrixSimilar MatricesRotationReflectionProjection Matrix
Vector Spaces
Vector SpaceSubspaceSpanLinear IndependenceBasisDimensionColumn SpaceNull Space (Kernel)Row SpaceLeft Null SpaceCoordinatesPivot ColumnFree VariableSpecial SolutionsNullityRank-Nullity TheoremFull Rank
Vectors
VectorScalarMagnitude (Norm)Unit VectorDot ProductCross ProductLinear CombinationZero VectorDirectionVector ProjectionOrthogonal DecompositionOuter ProductHadamard ProductFrobenius Inner ProductFrobenius NormInner Product SpaceRight-Hand RuleIsometry

120 terms

Vectors

(18 items)

Vector

An ordered list of nn real numbers: v=(v1,v2,…,vn)∈Rn\mathbf{v} = (v_1, v_2, \ldots, v_n) \in \mathbb{R}^n
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A quantity with both magnitude and direction. In R2\mathbb{R}^2 and R3\mathbb{R}^3, vectors can be visualized as arrows from the origin to a point.
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Scalar

An element of the underlying field — in standard linear algebra, a real number c∈Rc \in \mathbb{R}
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A single number used to scale vectors. Multiplying a vector by a scalar changes its length without altering its direction (unless the scalar is negative, which reverses direction).
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Magnitude (Norm)

The length of a vector, measured as its distance from the origin:
∥v∥=v12+v22+⋯+vn2\|\mathbf{v}\| = \sqrt{v_1^2 + v_2^2 + \cdots + v_n^2}
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In R2\mathbb{R}^2, this reduces to the hypotenuse given by the Pythagorean theorem. The concept generalizes to any Rn\mathbb{R}^n.
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Unit Vector

A vector u^\hat{\mathbf{u}} with ∥u^∥=1\|\hat{\mathbf{u}}\| = 1
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A vector that encodes direction only, with all length information removed. Any nonzero vector v\mathbf{v} can be normalized to a unit vector by dividing by its magnitude: v^=v∥v∥\hat{\mathbf{v}} = \frac{\mathbf{v}}{\|\mathbf{v}\|}.
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Dot Product

An operation that takes two vectors and returns a scalar, computed by summing the products of corresponding components:
u⋅v=u1v1+u2v2+⋯+unvn=∥u∥ ∥v∥cos⁡θ\mathbf{u} \cdot \mathbf{v} = u_1 v_1 + u_2 v_2 + \cdots + u_n v_n = \|\mathbf{u}\|\,\|\mathbf{v}\|\cos\theta
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A scalar measure of how much two vectors point in the same direction. Positive when the angle between them is acute, zero when perpendicular, negative when obtuse.
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Cross Product

A binary operation on two vectors in R3\mathbb{R}^3 that produces a vector perpendicular to both inputs:
u×v=(u2v3−u3v2u3v1−u1v3u1v2−u2v1)\mathbf{u} \times \mathbf{v} = \begin{pmatrix} u_2 v_3 - u_3 v_2 \\ u_3 v_1 - u_1 v_3 \\ u_1 v_2 - u_2 v_1 \end{pmatrix}
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Its magnitude equals the area of the parallelogram spanned by the two vectors. The direction follows the right-hand rule.
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Linear Combination

A sum of vectors, each multiplied by a scalar coefficient:
c1v1+c2v2+⋯+ckvkc_1\mathbf{v}_1 + c_2\mathbf{v}_2 + \cdots + c_k\mathbf{v}_k
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A new vector built by scaling given vectors and adding the results. The set of all possible linear combinations of a collection of vectors defines their span.
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Zero Vector

The vector 0=(0,0,…,0)\mathbf{0} = (0, 0, \ldots, 0) whose every component is zero
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The "nothing" vector: no length and no direction. It is the additive identity, so v+0=v\mathbf{v} + \mathbf{0} = \mathbf{v} for every v\mathbf{v}, and it is the one vector that cannot be normalized.
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Direction

The orientation of a non-zero vector, captured by its unit vector v/∥v∥\mathbf{v} / \|\mathbf{v}\|
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What is left of a vector once its length is stripped away. Two vectors share a direction exactly when one is a positive multiple of the other; a negative multiple reverses it.
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Vector Projection

The component of u\mathbf{u} lying along v\mathbf{v}:
projvu=u⋅vv⋅v v\text{proj}_{\mathbf{v}}\mathbf{u} = \frac{\mathbf{u} \cdot \mathbf{v}}{\mathbf{v} \cdot \mathbf{v}}\,\mathbf{v}
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The shadow u\mathbf{u} casts onto the line through v\mathbf{v}. It is always a multiple of v\mathbf{v}, never of u\mathbf{u} — the formula hides that asymmetry and the picture does not. The signed length of the shadow, (u⋅v)/∥v∥(\mathbf{u} \cdot \mathbf{v}) / \|\mathbf{v}\|, is the scalar projection.
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Orthogonal Decomposition

The unique splitting of a vector into a part inside a subspace WW and a part in its orthogonal complement:
u=projWu+(u−projWu)\mathbf{u} = \text{proj}_W\mathbf{u} + (\mathbf{u} - \text{proj}_W\mathbf{u})
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Every vector is "some of WW plus something perpendicular to WW", and there is only one way to do the split. The perpendicular part is the error a projection leaves behind, which is why least squares rests on this decomposition.
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Outer Product

The matrix uvT\mathbf{u}\mathbf{v}^T with entries (uvT)ij=uivj(\mathbf{u}\mathbf{v}^T)_{ij} = u_i v_j
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Where the dot product collapses two vectors into a number, the outer product spreads them into a table. Every column is a multiple of u\mathbf{u} and every row a multiple of vT\mathbf{v}^T, so the result has rank one. Also called the dyadic or tensor product.
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Hadamard Product

The entry-wise product of two same-shaped matrices: (A∘B)ij=aij bij(A \circ B)_{ij} = a_{ij}\,b_{ij}
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Multiply each entry by the entry in the same position and nothing else. Unlike ordinary matrix multiplication it is commutative, needs identical shapes, and never mixes positions. Also called the Schur product.
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Frobenius Inner Product

The inner product of two same-shaped matrices obtained by treating them as long vectors:
⟨A,B⟩F=∑i,jaij bij=tr(ATB)\langle A, B \rangle_F = \sum_{i,j} a_{ij}\,b_{ij} = \text{tr}(A^T B)
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Flatten both matrices into vectors and take the ordinary dot product. The trace form tr(ATB)\text{tr}(A^T B) is the same number written without flattening, which is what makes it useful in proofs.
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Frobenius Norm

The length of a matrix measured as if its entries were one long vector:
∥A∥F=∑i,jaij2=tr(ATA)\|A\|_F = \sqrt{\sum_{i,j} a_{ij}^2} = \sqrt{\text{tr}(A^T A)}
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The most literal way to say how "big" a matrix is: square every entry, add, take the root. It equals the square root of the sum of the squared singular values, which ties it to the geometry of the matrix rather than only its entries.
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Inner Product Space

A vector space equipped with an inner product ⟨⋅,⋅⟩\langle \cdot, \cdot \rangle that is symmetric, linear in each argument, and positive definite
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A vector space in which length, distance, angle and perpendicularity all make sense, because a single pairing supplies them: ∥v∥=⟨v,v⟩\|\mathbf{v}\| = \sqrt{\langle \mathbf{v}, \mathbf{v} \rangle} and orthogonality means ⟨u,v⟩=0\langle \mathbf{u}, \mathbf{v} \rangle = 0. Rn\mathbb{R}^n with the dot product is the standard example.
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Right-Hand Rule

The convention fixing the direction of a cross product u×v\mathbf{u} \times \mathbf{v}
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Curl the fingers of your right hand from u\mathbf{u} toward v\mathbf{v}; your thumb points along u×v\mathbf{u} \times \mathbf{v}. Swapping the two vectors curls the other way, which is why the cross product changes sign when its arguments are swapped.
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Isometry

A linear transformation that preserves lengths: ∥Tv∥=∥v∥\|T\mathbf{v}\| = \|\mathbf{v}\| for every v\mathbf{v}
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A rigid motion of space about the origin: nothing is stretched, squashed or sheared, so distances and angles survive too. In Rn\mathbb{R}^n the isometries are exactly the orthogonal matrices — rotations and reflections.
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Vector Spaces

(17 items)

Vector Space

A set VV equipped with vector addition and scalar multiplication satisfying the vector space axioms
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A collection of objects (vectors) that can be added together and scaled by numbers, where these operations behave predictably. Rn\mathbb{R}^n is the most familiar example, but the concept extends to function spaces, polynomial spaces, and more.
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Subspace

A nonempty subset W⊆VW \subseteq V that is itself a vector space under the same operations
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A subset of a vector space that is closed under addition and scalar multiplication. Every subspace must contain the zero vector.
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Span

The set of all linear combinations of a given collection of vectors:
Span{v1,…,vk}={c1v1+⋯+ckvk∣ci∈R}\text{Span}\{\mathbf{v}_1, \ldots, \mathbf{v}_k\} = \{c_1\mathbf{v}_1 + \cdots + c_k\mathbf{v}_k \mid c_i \in \mathbb{R}\}
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Geometrically, spanning two non-parallel vectors in R3\mathbb{R}^3 gives a plane; spanning three linearly independent vectors fills the entire space.
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Linear Independence

Vectors v1,…,vk\mathbf{v}_1, \ldots, \mathbf{v}_k are linearly independent if the only solution to
c1v1+⋯+ckvk=0c_1\mathbf{v}_1 + \cdots + c_k\mathbf{v}_k = \mathbf{0}

is c1=c2=⋯=ck=0c_1 = c_2 = \cdots = c_k = 0
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No vector in the set can be written as a linear combination of the others. Each vector contributes a genuinely new direction. Removing any one reduces the span.
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Basis

A set {v1,…,vn}\{\mathbf{v}_1, \ldots, \mathbf{v}_n\} that is linearly independent and spans the entire vector space
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A minimal set of vectors that can produce every vector in the space through linear combinations. Every vector has a unique representation as a linear combination of basis vectors.
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Dimension

The number of vectors in any basis of a vector space VV, denoted dim⁡(V)\dim(V)
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The number of independent directions in a space. R3\mathbb{R}^3 is three-dimensional because any basis has exactly three vectors.
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Column Space

The set of all vectors expressible as AxA\mathbf{x} — equivalently, the span of the columns of AA:
Col(A)={Ax∣x∈Rn}\text{Col}(A) = \{A\mathbf{x} \mid \mathbf{x} \in \mathbb{R}^n\}
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The set of all vectors b\mathbf{b} for which Ax=bA\mathbf{x} = \mathbf{b} has a solution. It captures everything the matrix can "reach" as output.
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Null Space (Kernel)

The set of all solutions to the homogeneous system Ax=0A\mathbf{x} = \mathbf{0}:
Nul(A)={x∈Rn∣Ax=0}\text{Nul}(A) = \{\mathbf{x} \in \mathbb{R}^n \mid A\mathbf{x} = \mathbf{0}\}
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The set of all inputs that the matrix sends to the zero vector. If the null space contains only 0\mathbf{0}, the matrix is injective (one-to-one). A larger null space means the matrix "collapses" some directions.
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Row Space

The span of the rows of a matrix, equivalently the column space of its transpose:
Row(A)=Col(AT)\text{Row}(A) = \text{Col}(A^T)
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A subspace of Rn\mathbb{R}^n spanned by the rows of AA. Row operations change individual rows but preserve the row space, making echelon form useful for finding a basis.
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Left Null Space

The null space of the transpose ATA^T — the set of all vectors y\mathbf{y} satisfying ATy=0A^T\mathbf{y} = \mathbf{0}:
Nul(AT)={y∈Rm∣ATy=0}\text{Nul}(A^T) = \{\mathbf{y} \in \mathbb{R}^m \mid A^T\mathbf{y} = \mathbf{0}\}
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It completes the four fundamental subspaces: column space, null space, row space, and left null space.
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Coordinates

The unique scalars c1,…,cnc_1, \ldots, c_n expressing a vector in a chosen basis:
v=c1b1+c2b2+⋯+cnbn\mathbf{v} = c_1\mathbf{b}_1 + c_2\mathbf{b}_2 + \cdots + c_n\mathbf{b}_n
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An address for a vector, read against a particular ruler. Change the basis and the same vector gets different numbers — the coordinates belong to the basis, not to the vector. Uniqueness is what makes them an address rather than one description among many.
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Pivot Column

A column of a matrix that contains a pivot after row reduction
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The columns that carry genuinely new directions. Their variables are the leading variables of the system, and the pivot columns of the original matrix — not of the reduced one — form a basis for the column space.
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Free Variable

A variable whose column carries no pivot after row reduction
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A variable the equations do not pin down: it may take any value, and the leading variables then follow. Each free variable adds one parameter to the solution set and one dimension to the null space.
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Special Solutions

The solutions of Ax=0A\mathbf{x} = \mathbf{0} obtained by setting one free variable to 11 and the others to 00
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One solution per free variable, each switching on a single free variable and solving for the rest. They are independent by construction and every solution of the homogeneous system is a combination of them, so together they form a basis for the null space.
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Nullity

The dimension of the null space: nullity(A)=n−rank(A)\text{nullity}(A) = n - \text{rank}(A)
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How many independent directions the matrix crushes to zero — equivalently, how many free variables the system has. Rank counts what survives, nullity counts what is lost, and the two always add up to the number of columns.
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Rank-Nullity Theorem

For an m×nm \times n matrix: rank(A)+nullity(A)=n\text{rank}(A) + \text{nullity}(A) = n
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Bookkeeping rather than a surprise: every column is either a pivot column, contributing a dimension to the column space, or a free column, contributing a dimension to the null space. No column is both and none is left out.
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Full Rank

A matrix whose rank is as large as its shape allows: rank(A)=min⁡(m,n)\text{rank}(A) = \min(m, n)
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Nothing is wasted. A square matrix of full rank is invertible; a tall one has independent columns and a wide one has independent rows. Losing full rank is the same event as the columns becoming dependent.
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Matrices

(25 items)

Matrix

A rectangular array of numbers with mm rows and nn columns: A∈Rm×nA \in \mathbb{R}^{m \times n}
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A compact way to encode a linear transformation or a system of linear equations. The entry in row ii, column jj is denoted aija_{ij}.
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Square Matrix

A matrix with equal numbers of rows and columns: A∈Rn×nA \in \mathbb{R}^{n \times n}
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Only square matrices can have determinants, eigenvalues, inverses, and a trace. They represent transformations from a space to itself.
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Identity Matrix

The square matrix with 11s on the main diagonal and 00s elsewhere, denoted InI_n:
In=(10⋯001⋯0⋮⋮⋱⋮00⋯1)I_n = \begin{pmatrix} 1 & 0 & \cdots & 0 \\ 0 & 1 & \cdots & 0 \\ \vdots & \vdots & \ddots & \vdots \\ 0 & 0 & \cdots & 1 \end{pmatrix}
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The matrix that leaves every vector unchanged: Iv=vI\mathbf{v} = \mathbf{v}. It is the multiplicative identity for matrices, analogous to the number 11.
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Symmetric Matrix

A square matrix satisfying A=ATA = A^T
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A matrix that equals its own transpose — entries are mirrored across the main diagonal. Symmetric matrices arise naturally in distance, covariance, and quadratic form problems.
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Inverse Matrix

A square matrix A−1A^{-1} such that AA−1=A−1A=IAA^{-1} = A^{-1}A = I
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The matrix that "undoes" the transformation applied by AA. If AA maps x\mathbf{x} to b\mathbf{b}, then A−1A^{-1} maps b\mathbf{b} back to x\mathbf{x}.
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Singular Matrix

A square matrix AA with det⁡(A)=0\det(A) = 0
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A matrix that collapses at least one dimension — it maps some nonzero vector to 0\mathbf{0}. A singular matrix has no inverse and the system Ax=bA\mathbf{x} = \mathbf{b} either has no solution or infinitely many.
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Rank

The number of linearly independent columns (equivalently, rows) in a matrix:
rank(A)=dim⁡(Col(A))=dim⁡(Row(A))\text{rank}(A) = \dim(\text{Col}(A)) = \dim(\text{Row}(A))
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It measures the "effective dimensionality" of the transformation — how many independent output directions the matrix produces.
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Trace

The sum of the main diagonal entries of a square matrix:
tr(A)=a11+a22+⋯+ann=∑i=1naii\text{tr}(A) = a_{11} + a_{22} + \cdots + a_{nn} = \sum_{i=1}^{n} a_{ii}
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It equals the sum of all eigenvalues (counted with multiplicity), providing a quick invariant of the matrix.
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Diagonal Matrix

A square matrix where aij=0a_{ij} = 0 for all i≠ji \neq j
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A matrix whose only nonzero entries lie on the main diagonal. Diagonal matrices scale each coordinate axis independently, making them the simplest matrices to work with.
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Positive Definite Matrix

A symmetric matrix AA satisfying xTAx>0\mathbf{x}^T A \mathbf{x} > 0 for all nonzero x\mathbf{x}
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A matrix where the associated quadratic form is always positive — it curves upward in every direction, like a bowl. Positive definite matrices generalize the idea of a positive number to matrix algebra.
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Transpose

The matrix ATA^T obtained by swapping rows and columns: (AT)ij=aji(A^T)_{ij} = a_{ji}
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A reflection of the matrix across its main diagonal. The diagonal itself does not move, which is why transposing twice returns the original and why a matrix equal to its own transpose is symmetric about that line.
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Main Diagonal

The entries a11,a22,a33,…a_{11}, a_{22}, a_{33}, \ldots whose row index equals their column index
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The line running from the top-left corner downward. Everything else is off-diagonal, either above it or below it, and a great many matrix types are defined by what sits where relative to this line: diagonal, triangular, symmetric.
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Zero Matrix

The matrix 00 with every entry equal to zero
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The additive identity for matrices of its shape: A+0=AA + 0 = A. Multiplying by it wipes everything out, so its determinant, rank and every eigenvalue are all 00.
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Scalar Matrix

A diagonal matrix whose diagonal entries are all the same number: cIcI
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A matrix that does nothing but scale: multiplying by cIcI stretches every vector by cc without turning it. The identity matrix is the case c=1c = 1.
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Skew-Symmetric Matrix

A square matrix equal to the negative of its transpose: AT=−AA^T = -A
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Mirrored entries carry opposite signs, aij=−ajia_{ij} = -a_{ji}. The diagonal is forced to be zero, since each diagonal entry must equal its own negative.
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Triangular Matrix

A square matrix with zeros on one side of the main diagonal
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Upper triangular when everything below the diagonal is zero, lower triangular when everything above is, and unit triangular when the diagonal is all ones. Elimination is the business of turning an arbitrary matrix into this shape, because a triangular system can be solved by substitution alone.
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Permutation Matrix

A square matrix with exactly one entry equal to 11 in each row and each column, and 00 everywhere else — the identity matrix with its rows rearranged:
P=(010001100)P = \begin{pmatrix} 0 & 1 & 0 \\ 0 & 0 & 1 \\ 1 & 0 & 0 \end{pmatrix}
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It moves entries without changing them. PAPA reorders the rows of AA and APAP reorders the columns, but nothing is scaled and nothing is combined. There are n!n! permutation matrices of order nn, one for each permutation of the indices. It is orthogonal, so its inverse is its transpose, and it is how the row swaps of partial pivoting get recorded in PA=LUPA = LU.
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Nilpotent Matrix

A square matrix some power of which is the zero matrix: Nk=0N^k = 0
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A matrix that destroys everything if applied often enough. A strictly upper triangular matrix is the standard example — each multiplication pushes the non-zero band one step further from the diagonal until nothing is left. Every eigenvalue of a nilpotent matrix is 00.
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Idempotent Matrix

A square matrix that equals its own square: P2=PP^2 = P
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Applying it twice changes nothing after the first time. Every projection matrix is idempotent — once a vector has been dropped onto a subspace, dropping it again leaves it where it is. The eigenvalues can only be 00 or 11.
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Involutory Matrix

A square matrix that is its own inverse: A2=IA^2 = I
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Applying it twice returns every vector to where it started, as a reflection does. Its eigenvalues can only be ±1\pm 1.
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Conformability

The shape condition under which a matrix operation is defined
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Addition and subtraction need identical shapes. The product ABAB needs the inner dimensions to agree — AA is m×nm \times n and BB is n×pn \times p — and the result takes the outer dimensions, m×pm \times p. Where the requirement fails the operation simply does not exist.
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Element-wise Operation

An operation applied independently at each position, so the entry at (i,j)(i, j) of the result depends only on the entries at (i,j)(i, j) of the inputs
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The positions never talk to each other. Addition, subtraction, scalar multiplication and the Hadamard product are all element-wise; ordinary matrix multiplication is the important operation that is not.
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Matrix Square Root

A matrix BB with B2=AB^2 = A, or more loosely BBT=ABB^T = A
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A positive definite matrix has exactly one positive definite square root, and its Cholesky factor LL, with LLT=ALL^T = A, is a lower-triangular one. Most matrices have no square root at all.
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Spectral Norm

The largest factor by which a matrix can stretch any vector:
∥A∥2=max⁡x≠0∥Ax∥∥x∥\|A\|_2 = \max_{\mathbf{x} \neq \mathbf{0}} \frac{\|A\mathbf{x}\|}{\|\mathbf{x}\|}
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Feed the matrix every possible direction and record the worst-case stretch. That maximum is the largest singular value, which is why the SVD is the natural way to compute it.
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Condition Number

The ratio of the largest to the smallest singular value: κ(A)=σmax⁡/σmin⁡\kappa(A) = \sigma_{\max} / \sigma_{\min}
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How much a small change in the data of Ax=bA\mathbf{x} = \mathbf{b} can be amplified in the answer. A condition number near 11 means a well-behaved system; a huge one means tiny rounding errors become large errors; an infinite one means the matrix is singular.
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Determinants

(9 items)

Determinant

A scalar det⁡(A)∈R\det(A) \in \mathbb{R} assigned to every square matrix, defined recursively via cofactor expansion
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The signed volume scaling factor of the linear transformation represented by the matrix. A determinant of zero means the transformation collapses space into a lower dimension.
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Minor

The determinant of the submatrix obtained by deleting row ii and column jj from a matrix:
Mij=det⁡(A^ij)M_{ij} = \det(\hat{A}_{ij})
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Minors are the building blocks for cofactors and, through them, for the full determinant computation.
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Cofactor

A signed minor, with sign determined by the position (i,j)(i,j):
Cij=(−1)i+jMijC_{ij} = (-1)^{i+j} M_{ij}
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The sign alternates in a checkerboard pattern (+,−,+,…+, -, +, \ldots). Cofactors are used in the expansion formula for determinants and in computing the adjugate.
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Cofactor Matrix (Adjugate)

The transpose of the matrix of cofactors of AA:
adj(A)=CT\text{adj}(A) = C^T
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It provides a formula for the inverse: A−1=1det⁡(A) adj(A)A^{-1} = \frac{1}{\det(A)}\,\text{adj}(A).
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Cofactor Expansion

Computing a determinant by expanding along any row or column:
det⁡A=∑jaij Cij\det A = \sum_{j} a_{ij}\,C_{ij}
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Each entry of the chosen row is multiplied by its cofactor — the signed determinant of what is left when its row and column are struck out — and the products are summed. The signs follow the checkerboard (−1)i+j(-1)^{i+j}. Any row or column gives the same answer, so pick the one with the most zeros. Also called Laplace expansion.
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Sarrus's Rule

A shortcut for 3×33 \times 3 determinants: add the three products along the down-right diagonals, subtract the three along the down-left diagonals
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Copy the first two columns to the right of the matrix and trace six diagonals. It is a mnemonic, not a method — it works for 3×33 \times 3 only and does not extend to larger matrices, where the number of terms jumps to 2424 and beyond.
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Adjugate

The transpose of the cofactor matrix: adj(A)=CT\text{adj}(A) = C^T
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The matrix that almost inverts AA: A adj(A)=(det⁡A) IA\,\text{adj}(A) = (\det A)\,I. Dividing by the determinant finishes the job, which puts the invertibility condition in plain view — the division fails precisely when det⁡A=0\det A = 0.
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Cramer's Rule

For a square system Ax=bA\mathbf{x} = \mathbf{b} with det⁡A≠0\det A \neq 0: xi=det⁡(Ai)det⁡Ax_i = \dfrac{\det(A_i)}{\det A}, where AiA_i is AA with its ii-th column replaced by b\mathbf{b}
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Each unknown is a ratio of two determinants. It is exact and elegant for two or three unknowns and hopeless beyond that, since every unknown costs a full determinant — elimination beats it for anything you would actually solve.
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Orientation

The handedness of an ordered set of vectors, read off the sign of the determinant
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A positive determinant keeps the standard orientation; a negative one turns space over, as a reflection does. The absolute value says how much area or volume is scaled, the sign says whether it was flipped.
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Linear Systems

(19 items)

System of Linear Equations

A collection of equations Ax=bA\mathbf{x} = \mathbf{b} where AA is an m×nm \times n matrix and b∈Rm\mathbf{b} \in \mathbb{R}^m
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A set of linear equations sharing the same unknowns. The system has either no solution, exactly one solution, or infinitely many solutions — there is no other possibility.
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Augmented Matrix

The matrix formed by appending the right-hand side vector b\mathbf{b} as an additional column to the coefficient matrix AA, written [A∣b][A \mid \mathbf{b}]
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A compact notation that combines the coefficient matrix and the right-hand side into a single matrix, so row operations can be applied to the entire system at once.
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Row Echelon Form

A matrix where:
• all zero rows are at the bottom
• each leading entry (pivot) is to the right of the pivot in the row above
• all entries below each pivot are zero
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A staircase pattern achieved by row operations, making back-substitution possible. The number of pivots equals the rank.
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Reduced Row Echelon Form

Row echelon form with the additional requirements:
• every pivot is 11
• each pivot is the only nonzero entry in its column
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The fully simplified form of a matrix under row operations. Unlike row echelon form, the reduced form is unique — every matrix has exactly one RREF.
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Pivot

The first nonzero entry in each row of a matrix in row echelon form
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Pivots mark the "independent" columns. The number of pivots determines the rank; columns without pivots correspond to free variables in the solution.
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Homogeneous System

A system of linear equations in which every equation equals zero: Ax=0A\mathbf{x} = \mathbf{0}
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It always has at least the trivial solution x=0\mathbf{x} = \mathbf{0}. Nontrivial solutions exist if and only if rank(A)<n\text{rank}(A) < n.
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Coefficient Matrix

The matrix AA of coefficients of the unknowns when a system of linear equations is written as Ax=bA\mathbf{x} = \mathbf{b}
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The numbers multiplying the unknowns, one row per equation and one column per unknown. The vector b\mathbf{b} of constants is the right-hand side, and appending it as a final column gives the augmented matrix.
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Elementary Row Operation

One of three moves that leave a system's solution set unchanged: swap two rows, multiply a row by a non-zero constant, or add a multiple of one row to another
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Each move is reversible — the same multiple can be subtracted back, the same rows swapped again — and that reversibility is the licence for the whole of elimination: nothing about the solutions can change if every step can be undone.
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Gaussian Elimination

The algorithm that reduces a matrix to row echelon form using elementary row operations
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Work column by column, clearing every entry below each pivot by subtracting multiples of the pivot row. What remains is a staircase that can be finished by back-substitution. Continuing to clear above the pivots as well is Gauss-Jordan elimination. Also called row reduction.
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Back-Substitution

Solving an upper-triangular system from the bottom row upward
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The last equation involves one unknown, so it is solved directly. That value is substituted into the row above, which now involves one unknown, and so on up the staircase. It is the second half of Gaussian elimination.
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Forward Substitution

Solving a lower-triangular system from the top row downward
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The mirror image of back-substitution: the first equation has one unknown, its value feeds the second, and so on downward. It is the first of the two triangular solves when a system is attacked through its LU decomposition.
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Partial Pivoting

Swapping rows during elimination so that the largest available entry in the current column becomes the pivot
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Dividing by a zero pivot is impossible and dividing by a tiny one wrecks accuracy, so the row with the biggest entry is moved up first. The swaps are recorded in a permutation matrix, which is why the honest form of LU is PA=LUPA = LU.
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Consistent System

A system of linear equations that has at least one solution
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Exactly one solution when every column has a pivot, infinitely many when some column is free. An inconsistent system has none, and reduction announces it with a row reading 0=c0 = c for some c≠0c \neq 0 — inconsistency is detected, not tested for.
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Overdetermined System

A system with more equations than unknowns
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Too many constraints for the unknowns to satisfy all at once, so the system is usually inconsistent. It is then solved in the least-squares sense — the answer that misses every equation by as little as possible overall — which is exactly the situation in fitting a line to data.
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LU Decomposition

Writing a matrix as A=LUA = LU, with LL lower triangular and UU upper triangular; with row swaps, PA=LUPA = LU
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Gaussian elimination with the multipliers kept instead of thrown away: UU is the result of the elimination and LL is its record. Once factored, Ax=bA\mathbf{x} = \mathbf{b} is two cheap triangular solves — forward then back — for as many right-hand sides as you like.
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Least-Squares Solution

For an inconsistent system Ax=bA\mathbf{x} = \mathbf{b}, the x^\hat{\mathbf{x}} that minimizes ∥b−Ax^∥\|\mathbf{b} - A\hat{\mathbf{x}}\|; it satisfies the normal equations ATAx^=ATbA^TA\hat{\mathbf{x}} = A^T\mathbf{b}
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When b\mathbf{b} cannot be reached, aim for the nearest point that can: its projection onto the column space. Minimizing the error and making it perpendicular to the column space turn out to be the same requirement, and that perpendicularity is what the normal equations say.
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Residual

The error vector left by an approximate solution: r=b−Ax^\mathbf{r} = \mathbf{b} - A\hat{\mathbf{x}}
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What the fit fails to explain. At the least-squares solution the residual is not merely small — it is orthogonal to the column space, which is the geometric fact everything else follows from. Its squared length is the sum of squared errors.
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Design Matrix

The matrix AA built from the data in a fitting problem: one row per observation, one column per unknown coefficient
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Fitting a line y=c0+c1xy = c_0 + c_1 x to points (xi,yi)(x_i, y_i) gives rows (1,xi)(1, x_i); fitting a parabola adds a column of xi2x_i^2. The fit is the least-squares solution of Ac=yA\mathbf{c} = \mathbf{y}, and changing the model changes only the columns, never the method.
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Pseudoinverse

The matrix A+A^+ that plays the role of an inverse for a matrix that has none; for independent columns, A+=(ATA)−1ATA^+ = (A^TA)^{-1}A^T
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It sends b\mathbf{b} to the least-squares solution of smallest length, and reduces to the ordinary inverse when one exists. In general it is built from the SVD by inverting the non-zero singular values and leaving the zero ones alone.
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Transformations

(8 items)

Linear Transformation

A function T:V→WT: V \to W between vector spaces that preserves addition and scalar multiplication:
T(u+v)=T(u)+T(v)T(\mathbf{u} + \mathbf{v}) = T(\mathbf{u}) + T(\mathbf{v})

T(cu)=cT(u)T(c\mathbf{u}) = cT(\mathbf{u})
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Lines map to lines (or to the origin), and the origin stays fixed. Every linear transformation between finite-dimensional spaces can be represented by a matrix.
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Image (Range)

The set of all output vectors of a linear transformation:
Im(T)={T(v)∣v∈V}\text{Im}(T) = \{T(\mathbf{v}) \mid \mathbf{v} \in V\}
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For a matrix transformation T(x)=AxT(\mathbf{x}) = A\mathbf{x}, the image equals the column space of AA.
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Matrix Representation

A matrix AA such that T(v)=A[v]BT(\mathbf{v}) = A[\mathbf{v}]_{\mathcal{B}} for a chosen basis B\mathcal{B}
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Every linear transformation between finite-dimensional spaces can be encoded as a matrix once bases are chosen. Different bases produce different matrices representing the same transformation.
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Change of Basis Matrix

A matrix PP that converts coordinates from one basis to another: [v]B′=P−1[v]B[\mathbf{v}]_{\mathcal{B}'} = P^{-1}[\mathbf{v}]_{\mathcal{B}}
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The same vector can be described using different coordinate systems (bases). The change of basis matrix translates between these coordinate systems.
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Similar Matrices

Matrices AA and BB are similar if B=P−1APB = P^{-1}AP for some invertible matrix PP
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Two matrices are similar when they represent the same linear transformation under different bases. They share all basis-independent properties.
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Rotation

A linear transformation that turns every vector through the same angle about the origin; in R2\mathbb{R}^2:
Rθ=[cos⁡θ−sin⁡θsin⁡θcos⁡θ]R_\theta = \begin{bmatrix} \cos\theta & -\sin\theta \\ \sin\theta & \cos\theta \end{bmatrix}
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Lengths and angles survive, only headings change. The matrix is orthogonal with determinant +1+1, and a rotation by a non-trivial angle has no real eigenvectors — no direction is left pointing where it started.
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Reflection

A linear transformation that mirrors every vector across a line through the origin — or a plane, in three dimensions
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Points on the mirror stay put while everything else swaps to the far side at equal distance. The matrix is orthogonal with determinant −1-1 and is its own inverse: reflecting twice restores everything.
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Projection Matrix

The matrix PP sending every vector to its orthogonal projection onto a subspace; for a subspace with basis matrix AA:
P=A(ATA)−1ATP = A(A^TA)^{-1}A^T
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Drop every point perpendicularly onto the subspace. Points already there do not move, so applying PP twice changes nothing after the first time — it is idempotent, P2=PP^2 = P, and symmetric. Its determinant is 00 whenever the subspace is smaller than the whole space, because information has been lost.
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Eigen

(15 items)

Eigenvalue

A scalar λ\lambda such that Av=λvA\mathbf{v} = \lambda\mathbf{v} for some nonzero vector v\mathbf{v}
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The factor by which the linear transformation stretches or compresses an eigenvector. A negative eigenvalue means the eigenvector's direction is reversed.
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Eigenvector

A nonzero vector v\mathbf{v} such that Av=λvA\mathbf{v} = \lambda\mathbf{v} for some scalar λ\lambda
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A direction that the matrix preserves — the transformation only stretches or compresses along this direction without rotating it. Eigenvectors from distinct eigenvalues are always linearly independent.
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Eigenspace

The set of all eigenvectors for a given eigenvalue λ\lambda, together with the zero vector — equivalently, the null space of (A−λI)(A - \lambda I):
Eλ=Nul(A−λI)E_\lambda = \text{Nul}(A - \lambda I)
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It is always a subspace, and its dimension reveals how many independent eigenvector directions exist for that eigenvalue.
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Characteristic Polynomial

The polynomial whose roots are the eigenvalues of AA, obtained by computing:
p(λ)=det⁡(A−λI)p(\lambda) = \det(A - \lambda I)
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For an n×nn \times n matrix, the characteristic polynomial has degree nn, so there are at most nn eigenvalues (counted with multiplicity).
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Algebraic Multiplicity

The multiplicity of λ\lambda as a root of the characteristic polynomial
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How many times the eigenvalue appears as a root. If p(λ)=(λ−2)3(λ+1)p(\lambda) = (\lambda - 2)^3(\lambda + 1), then λ=2\lambda = 2 has algebraic multiplicity 33 and λ=−1\lambda = -1 has algebraic multiplicity 11.
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Geometric Multiplicity

The dimension of the eigenspace associated with an eigenvalue λ\lambda:
geo. mult.(λ)=dim⁡(Eλ)=dim⁡(Nul(A−λI))\text{geo. mult.}(\lambda) = \dim(E_\lambda) = \dim(\text{Nul}(A - \lambda I))
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The number of independent eigenvector directions for a given eigenvalue. A matrix is diagonalizable if and only if every eigenvalue has geometric multiplicity equal to its algebraic multiplicity.
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Singular Value

A nonnegative scalar measuring how much a matrix stretches space along each principal direction, derived from the eigenvalues of ATAA^TA:
σi=λi(ATA)\sigma_i = \sqrt{\lambda_i(A^TA)}
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Unlike eigenvalues, singular values are always nonnegative and exist for any matrix, not just square ones.
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Diagonalizable Matrix

A square matrix with a full set of nn linearly independent eigenvectors — equivalently, one that can be written as A=PDP−1A = PDP^{-1} with DD diagonal
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A matrix that is secretly just a stretch along some set of directions. Every matrix with nn distinct eigenvalues qualifies, and every symmetric matrix does; what disqualifies a matrix is never awkward eigenvalues, only running out of independent eigenvectors.
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Diagonalization

Factoring a matrix as A=PDP−1A = PDP^{-1}, where the columns of PP are eigenvectors and DD carries the matching eigenvalues on its diagonal
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A change to the basis in which the matrix acts as a plain stretch. The payoff is powers: Ak=PDkP−1A^k = PD^kP^{-1}, and raising a diagonal matrix to a power is entrywise, so repeated multiplication becomes a handful of scalar powers.
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Defective Matrix

A matrix with too few independent eigenvectors to be diagonalized: for some eigenvalue the geometric multiplicity is smaller than the algebraic multiplicity
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A repeated eigenvalue that failed to bring a full set of directions with it. There are not enough independent eigenvectors to fill the columns of PP, so PP cannot be inverted and the factorization never forms. The Jordan form exists to give these matrices a canonical shape instead.
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Dominant Eigenvalue

The eigenvalue of largest absolute value
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Multiply a vector by the matrix again and again and it swings toward the dominant eigenvector, because that component grows fastest. The rate is set by the ratio ∣λ2/λ1∣|\lambda_2 / \lambda_1| — close to 11 means slow convergence — and this is exactly what power iteration exploits.
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Rayleigh Quotient

The scalar
R(x)=xTA xxTxR(\mathbf{x}) = \frac{\mathbf{x}^T A\,\mathbf{x}}{\mathbf{x}^T \mathbf{x}}
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The best estimate of an eigenvalue from a vector that is only approximately an eigenvector. It equals the eigenvalue exactly when x\mathbf{x} is an eigenvector, and for a symmetric matrix it is always trapped between the smallest and largest eigenvalues.
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Quadratic Form

A function q(x)=xTA xq(\mathbf{x}) = \mathbf{x}^T A\,\mathbf{x} built from a symmetric matrix
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Every term is a product of two coordinates — x12x_1^2, x1x2x_1 x_2 and so on — with the matrix holding the coefficients. Its sign behaviour is read off the eigenvalues of AA: all positive means positive definite, all negative means negative definite, mixed means indefinite.
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Spectral Decomposition

The diagonalization of a symmetric matrix by an orthogonal matrix:
A=QΛQT=∑iλi qiqiTA = Q\Lambda Q^T = \sum_{i} \lambda_i\,\mathbf{q}_i \mathbf{q}_i^T
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Because the eigenvectors of a symmetric matrix can be chosen orthonormal, the matrix of them is orthogonal and its inverse is just its transpose — no inverse ever has to be computed. The sum form shows the matrix as rank-one pieces weighted by eigenvalues, and dropping the smallest weights is how it becomes an approximation.
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Singular Value Decomposition

The factorization A=UΣVTA = U\Sigma V^T with UU and VV orthogonal and Σ\Sigma a rectangular diagonal matrix of singular values in decreasing order
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The one factorization every matrix has — square or not, symmetric or not, with or without eigenvectors. The columns of VV are the right singular vectors, the columns of UU the left ones, and Σ\Sigma says how much each direction is stretched. Truncating it keeps the most important part first.
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Orthogonality

(9 items)

Inner Product

A function ⟨⋅,⋅⟩:V×V→R\langle \cdot, \cdot \rangle: V \times V \to \mathbb{R} satisfying symmetry, linearity, and positive-definiteness
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A generalization of the dot product to abstract vector spaces. It defines notions of length, angle, and orthogonality in spaces where the standard dot product may not apply.
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Orthogonal Vectors

Vectors u\mathbf{u} and v\mathbf{v} are orthogonal if ⟨u,v⟩=0\langle \mathbf{u}, \mathbf{v} \rangle = 0
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Perpendicular vectors. Their dot product (or inner product) is zero, meaning they share no component in each other's direction.
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Orthogonal Set

A set of vectors {v1,…,vk}\{\mathbf{v}_1, \ldots, \mathbf{v}_k\} where ⟨vi,vj⟩=0\langle \mathbf{v}_i, \mathbf{v}_j \rangle = 0 for all i≠ji \neq j
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A collection of mutually perpendicular vectors. Every orthogonal set of nonzero vectors is automatically linearly independent.
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Orthonormal Set

An orthogonal set where every vector is a unit vector: ⟨vi,vj⟩=δij\langle \mathbf{v}_i, \mathbf{v}_j \rangle = \delta_{ij}
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Mutually perpendicular vectors, each of length 11. An orthonormal basis gives the simplest coordinate system — coordinates are just inner products with the basis vectors.
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Orthogonal Complement

The set of all vectors in VV that are orthogonal to every vector in a subspace WW:
W⊥={v∈V∣⟨v,w⟩=0 for all w∈W}W^\perp = \{\mathbf{v} \in V \mid \langle \mathbf{v}, \mathbf{w} \rangle = 0 \text{ for all } \mathbf{w} \in W\}
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Together, WW and W⊥W^\perp span the entire space, with no overlap except the zero vector.
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Orthogonal Matrix

A square matrix QQ satisfying QTQ=QQT=IQ^TQ = QQ^T = I
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A matrix whose columns (and rows) form an orthonormal set. Orthogonal matrices preserve lengths and angles — they represent rotations and reflections.
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Gram-Schmidt Process

The procedure that turns any linearly independent set into an orthonormal set spanning the same space
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Take each vector in turn, subtract its projections onto the directions already fixed, and normalize what is left. The subtraction guarantees orthogonality by construction; the normalization only fixes the length, which is why the two concerns can be separated.
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QR Decomposition

Writing a matrix with independent columns as A=QRA = QR, with QQ orthogonal and RR upper triangular
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Gram-Schmidt written as a factorization: the orthonormal vectors it produces become the columns of QQ, and the coefficients it subtracted along the way become the entries of RR. The triangularity of RR is not imposed — each column was only ever corrected against the ones before it.
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Cholesky Factorization

Writing a positive definite matrix as A=LLTA = LL^T with LL lower triangular and positive diagonal
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A square root of the matrix, computed by alternating square roots on the diagonal with simple divisions below it. It exists exactly when AA is positive definite, so attempting it doubles as the standard test for that property, and it works on only half the matrix — about twice as fast as LU.
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