Cramer's rule in civilised form with Clifford algebra
Robin K. S. Hankin
Source:vignettes/cramer_clifford.Rmd
cramer_clifford.Rmd
To cite the clifford
package in publications please use
Hankin (2022). This short document shows a
nice application of Clifford algebras to linear algebra. Suppose we have
vectors \({\mathbf a}, {\mathbf b}, {\mathbf
c}\) spanning \(\mathbb{R}^3\)
and are given \({\mathbf
x}\in\mathbb{R}^3\). We wish to write \({\mathbf
x}=\alpha {\mathbf a}+\beta {\mathbf b}+\gamma {\mathbf c}\) for
some \(\alpha,\beta,\gamma\in\mathbb{R}\). The
traditional Cramer’s rule for finding \(\alpha,\beta,\gamma\) would be
\[ \alpha=\frac{ \det\begin{bmatrix} x_1&b_1&c_1\\ x_2&b_2&c_2\\ x_3&b_3&c_3 \end{bmatrix} }{ \det\begin{bmatrix} a_1&b_1&c_1\\ a_2&b_2&c_2\\ a_3&b_3&c_3 \end{bmatrix} } \qquad\beta=\frac{ \det\begin{bmatrix} a_1&x_1&c_1\\ a_2&x_2&c_2\\ a_3&x_3&c_3 \end{bmatrix} }{ \det\begin{bmatrix} a_1&b_1&c_1\\ a_2&b_2&c_2\\ a_3&b_3&c_3 \end{bmatrix} } \qquad \gamma=\frac{ \det\begin{bmatrix} a_1&b_1&x_1\\ a_2&b_2&x_2\\ a_3&b_3&x_3 \end{bmatrix} }{ \det\begin{bmatrix} a_1&b_1&c_1\\ a_2&b_2&c_2\\ a_3&b_3&c_3 \end{bmatrix} } \]
where \({\mathbf x}=(x_1,x_2,x_3)^T\), \({\mathbf a}=(a_1,a_2,a_3)^T\), \({\mathbf b}=(b_1,b_2,b_3)^T\) and \({\mathbf c}=(c_1,c_2,c_3)^T\). However, observe that this solution, while accurate, requires one to take a coordinate basis; and offers little in the way of intuition.
Using Clifford algebra
Considering \(\mathbb{R}^3\) as a vector space and given vectors \({\mathbf a}, {\mathbf b}, {\mathbf c}\) spanning the space we can express any vector \({\mathbf x}\in\mathbb{R}^3\) as
\[\mathbf{x}= \left(\frac{{\mathbf x}\wedge{\mathbf b}\wedge{\mathbf c}}{{\mathbf a}\wedge{\mathbf b}\wedge{\mathbf c}}\right){\mathbf a}+ \left(\frac{{\mathbf a}\wedge{\mathbf x}\wedge{\mathbf c}}{{\mathbf a}\wedge{\mathbf b}\wedge{\mathbf c}}\right){\mathbf b}+ \left(\frac{{\mathbf a}\wedge{\mathbf b}\wedge{\mathbf x}}{{\mathbf a}\wedge{\mathbf b}\wedge{\mathbf c}}\right){\mathbf c} \]
which is Cramer’s rule expressed directly in vector form (rather than components). Observe that the numerator and denominator of each bracketed term is a pseudoscalar; the ratio of two pseudoscalars is an ordinary scalar. Package idiom is straightforward:
a <- as.1vector(runif(3))
b <- as.1vector(runif(3))
c <- as.1vector(runif(3))
(x <- as.1vector(1:3))
## Element of a Clifford algebra, equal to
## + 1e_1 + 2e_2 + 3e_3
options(maxdim = 3) # needed to drop() pseudoscalars
abc <- drop(a ^ b ^ c)
alpha <- drop(x ^ b ^ c)/abc
beta <- drop(a ^ x ^ c)/abc
gamma <- drop(a ^ b ^ x)/abc
c(alpha,beta,gamma)
## [1] -3.805997 -5.328439 8.309581
alpha*a + beta*b + gamma*c
## Element of a Clifford algebra, equal to
## + 1e_1 + 2e_2 + 3e_3
Mod(alpha*a + beta*b + gamma*c-x)
## [1] 0
Thus we have expressed \({\mathbf x}\) (except for possible roundoff error) as a linear combination of \({\mathbf a},{\mathbf b},{\mathbf c}\), specifically \({\mathbf x}=\alpha{\mathbf a}+\beta{\mathbf b}+\gamma{\mathbf c}\). Conversely, we might know the coefficients and try to determine them using package idiom. Here we will use \(1,2,3\) and suppose that \({\mathbf y}=1{\mathbf a}+2{\mathbf b}+3{\mathbf c}\):
## [1] 1 2 3
Higher dimensional space
To accomplish this in arbitrary-dimensional space is straightforward. Here we consider \(\mathbb{R}^{5}\):
n <- 5 # dimensionality of space
options(maxdim=5) # safety precaution
x <- as.1vector(seq_len(n)) # target vector
x
## Element of a Clifford algebra, equal to
## + 1e_1 + 2e_2 + 3e_3 + 4e_4 + 5e_5
L <- replicate(n,as.1vector(rnorm(n)),simplify=FALSE) # spanning vectors
subst <- function(L,n,x){L[[n]] <- x; return(L)} # list substitution
coeff <- function(n,L,x){
drop(Reduce(`^`,subst(L,n,x))/Reduce(`^`,L))
}
Then the coefficients are given by:
## [1] 21.610237 27.030973 11.866383 -22.222116 3.199427
and we can reconstitute vector \(x\):
out <- as.clifford(0)
f <- function(i){alpha[i]*L[[i]]}
for(i in seq_len(n)){
out <- out + f(i)
}
Mod(out-x) # zero to numerical precision
## [1] 2.340649e-14
Or, somewhat slicker:
## Element of a Clifford algebra, equal to
## + 1e_1 + 2e_2 + 3e_3 + 4e_4 + 5e_5
Conversely, if we know the coefficients are, say, 15:11
,
then we would have
coeffs <- 15:11
x <- 0
for(i in seq_len(5)){x <- x + coeffs[i]*L[[i]]}
x
## Element of a Clifford algebra, equal to
## + 29.23618e_1 + 18.68409e_2 + 20.23065e_3 - 0.6361232e_4 - 40.82507e_5
And then to find the coefficients:
## [1] 15 14 13 12 11
Above we see that the original coefficients are recovered, up to numerical accuracy.