Definition

In this collection, Minkowski vector space is R1,3=R4\mathbb R^{1,3}=\mathbb R^4 with coordinates (t,x,y,z)(t,x,y,z), symmetric

η(u,v)=u0v0+u1v1+u2v2+u3v3,\eta(u,v)=-u_0v_0+u_1v_1+u_2v_2+u_3v_3,

and associated

q(v)=η(v,v)=t2+x2+y2+z2.q(v)=\eta(v,v)=-t^2+x^2+y^2+z^2.

Thus the matrix of η\eta is diag(1,1,1,1)\operatorname{diag}(-1,1,1,1); throughout this collection, the notation (1,3)(1,3) means one negative and three positive directions.

Causal types

A nonzero vector vv is timelike, null (or lightlike), or spacelike according as q(v)<0q(v)<0, q(v)=0q(v)=0, or q(v)>0q(v)>0. The timelike cone has two . Choosing one as the future cone is a .

Sources that list positive directions first call the displayed form's signature (3,1)(3,1). Other sources reverse the overall sign and use t2x2y2z2t^2-x^2-y^2-z^2; in this collection's negative-first ordering, that opposite form has signature (3,1)(3,1). Formulas in linked knowls use the displayed (+++)(-+++) form, so the satisfies detX(v)=q(v)\det X(v)=-q(v), not detX(v)=q(v)\det X(v)=q(v).

References
  1. Barrett O'Neill, Semi-Riemannian Geometry With Applications to Relativity, Academic Press, 1983, Chapter 5. Publisher record.
  2. Gregory L. Naber, The Geometry of Minkowski Spacetime, 2nd ed., Springer, 2012, Chapter 1. Publisher record.