Mathematical Physicsundergraduategraduate

Characteristic Polynomial

Also known as: Secular equation · Eigenvalue equation

To find a matrix's eigenvalues — the special scaling factors along which it merely stretches vectors — you ask when A−λI collapses a direction to zero, i.e. when its determinant vanishes. That determinant, as a function of λ, is the characteristic polynomial. Its roots are the eigenvalues. Physicists call it the 'secular equation' because it first arose computing slow (secular) perturbations of planetary orbits. Its coefficients encode invariants: the trace and determinant of A.

p(λ)=det(AλI)=0p(\lambda)=\det(A-\lambda I)=0
Live simulation
warming up the physics…

Eigenvalues are where det(A−λI) crosses zero; the curve slides as the sweep parameter moves.

Equivalent forms

λn(trA)λn1++(1)ndetA=0\lambda^n - (\mathrm{tr}\,A)\lambda^{n-1}+\dots+(-1)^n\det A=0
One polynomial packages every eigenvalue, and its coefficients are exactly the rotation-invariant quantities (trace, determinant) of the matrix.