Choose two distinct space-diagonal directions and . Their dot product is one and their norms are both . Thus the acute angle between their unoriented lines isAny two distinct space diagonals have an absolute dot product of one when represented with components , so they give the same acute angle.
Let . These three vectors are linearly independent, so write . Taking the dot product with gives . Likewise, the dot products with and giveHere the cyclic invariance and sign change under an interchange of the scalar triple product fix every sign. Substituting the three coefficients provesThis is precisely coordinate extraction using the reciprocal basis .
Now take the cross product with . The vector triple product gives , soThe original equation, now with , also gives . Substitution eliminates the remaining cross product of the unknown and yieldsIts dot product with is , and direct substitution using the vector triple product verifies the original equation. The elimination gives a unique solution without choosing components. It is also an application of the inverse of a scalar plus a cross-product operator after the scalar component has been fixed.
The vector field is radial, while the differential displacement along a centred circle is tangential. These directions are orthogonal, so the dot product vanishes at every point. Hence
By Thales's theorem, the two sides meeting on the circular arc are orthogonal, because the opposite side is a diameter. Both vectors point towards that meeting point; reversing both does not change their dot product. Consequently
For the obtained above, the characteristic polynomial isThus the eigenvalues are and . For , gives ; for , it gives . Normalizing the eigenvectors yieldsBoth are unit vectors, their dot product is zero, and either overall sign is allowed for each eigenvector.
Compute the flux directly using the outward vector area element, as required. Restrict the vector field to the surface parametric equation and take the dot product:The terms quadratic in cancel. Therefore the surface integral isThis is a direct evaluation of the flux of the position vector through a cone.
The new cone can be parametrized byThe outward vector area element is . This is ; reversing the order is needed to retain the outward orientation after the exchange of coordinates. Its dot product with is again . HenceThis equality also follows because a rigid rotation takes the first cone into the second and leaves the radial vector field invariant.
Parametrize the segment in its stated direction by , . Then , and substitution into the two vector fields givesTaking each dot product with evaluates the line integrals:
The two directed segments have vectors and . Their dot product is and both norms equal . HenceThe common starting point fixes the obtuse angle between these segments.
Both segments start at , so their direction vectors are and . Their dot product is , and their norms are and . ThusThe angle between the rays lies in , so its sine is nonnegative:The negative cosine correctly identifies an obtuse angle. One also obtains the sine from , using the cross product.
Use only the dot product to minimize the squared Euclidean distance from the origin:Completing the square givesThe square is minimized at , yieldingGeometrically this subtracts the squared length of the orthogonal projection parallel to the line. At the minimizing point, , as required for perpendicular distance.
The dot product isBoth vectors have squared Euclidean norm . Under the given condition , their dot product is and each squared Euclidean norm is . Hence
Three vectors form a basis of three-dimensional space exactly when their scalar triple product is nonzero:It is the determinant of the matrix with these columns, so this condition is equivalent to linear independence and spanning the whole space.
Take the dot product of the expansion of with . The terms containing and vanish, leaving . Cycling the same argument yieldsThe three cross-product numerators use the reciprocal basis.
If , the first and third equations give . The middle equation then gives , so . The norm constraint gives and . Thus the hottest points and their temperature areThe coldest points areFor , the equations give , , and hence the other two constrained stationary points areThey are saddle points of the restriction to the sphere: with and as local tangent coordinates there, changes sign in every neighbourhood. The surface is compact and smooth, so the listed extreme temperatures are global. Here “zero gradient on the surface” means zero surface gradient; the ambient gradient at the hottest and coldest points is normal to the sphere, rather than zero.