Eigen
3.4.99 (git rev 69adf26aa3e853418002562f623c42a9c7008271)

This is a very short guide on how to get started with Eigen. It has a dual purpose. It serves as a minimal introduction to the Eigen library for people who want to start coding as soon as possible. You can also read this page as the first part of the Tutorial, which explains the library in more detail; in this case you will continue with The Matrix class.
In order to use Eigen, you just need to download and extract Eigen's source code (see the wiki for download instructions). In fact, the header files in the Eigen
subdirectory are the only files required to compile programs using Eigen. The header files are the same for all platforms. It is not necessary to use CMake or install anything.
Here is a rather simple program to get you started.
We will explain the program after telling you how to compile it.
There is no library to link to. The only thing that you need to keep in mind when compiling the above program is that the compiler must be able to find the Eigen header files. The directory in which you placed Eigen's source code must be in the include path. With GCC you use the I option to achieve this, so you can compile the program with a command like this:
On Linux or Mac OS X, another option is to symlink or copy the Eigen folder into /usr/local/include/. This way, you can compile the program with:
When you run the program, it produces the following output:
The Eigen header files define many types, but for simple applications it may be enough to use only the MatrixXd
type. This represents a matrix of arbitrary size (hence the X
in MatrixXd
), in which every entry is a double
(hence the d
in MatrixXd
). See the quick reference guide for an overview of the different types you can use to represent a matrix.
The Eigen/Dense
header file defines all member functions for the MatrixXd type and related types (see also the table of header files). All classes and functions defined in this header file (and other Eigen header files) are in the Eigen
namespace.
The first line of the main
function declares a variable of type MatrixXd
and specifies that it is a matrix with 2 rows and 2 columns (the entries are not initialized). The statement m(0,0) = 3
sets the entry in the topleft corner to 3. You need to use round parentheses to refer to entries in the matrix. As usual in computer science, the index of the first index is 0, as opposed to the convention in mathematics that the first index is 1.
The following three statements sets the other three entries. The final line outputs the matrix m
to the standard output stream.
Here is another example, which combines matrices with vectors. Concentrate on the lefthand program for now; we will talk about the righthand program later.
Size set at run time:  Size set at compile time: 

#include <iostream>
#include <Eigen/Dense>
using namespace Eigen;
using namespace std;
int main()
{
MatrixXd m = MatrixXd::Random(3,3);
m = (m + MatrixXd::Constant(3,3,1.2)) * 50;
cout << "m =" << endl << m << endl;
VectorXd v(3);
v << 1, 2, 3;
cout << "m * v =" << endl << m * v << endl;
}
static const ConstantReturnType Constant(Index rows, Index cols, const Scalar &value) Definition: CwiseNullaryOp.h:189  #include <iostream>
#include <Eigen/Dense>
using namespace Eigen;
using namespace std;
int main()
{
Matrix3d m = Matrix3d::Random();
m = (m + Matrix3d::Constant(1.2)) * 50;
cout << "m =" << endl << m << endl;
Vector3d v(1,2,3);
cout << "m * v =" << endl << m * v << endl;
}

The output is as follows:
The second example starts by declaring a 3by3 matrix m
which is initialized using the Random() method with random values between 1 and 1. The next line applies a linear mapping such that the values are between 10 and 110. The function call MatrixXd::Constant(3,3,1.2) returns a 3by3 matrix expression having all coefficients equal to 1.2. The rest is standard arithmetic.
The next line of the main
function introduces a new type: VectorXd
. This represents a (column) vector of arbitrary size. Here, the vector v
is created to contain 3
coefficients which are left uninitialized. The one but last line uses the socalled commainitializer, explained in Advanced initialization, to set all coefficients of the vector v
to be as follows:
\[ v = \begin{bmatrix} 1 \\ 2 \\ 3 \end{bmatrix}. \]
The final line of the program multiplies the matrix m
with the vector v
and outputs the result.
Now look back at the second example program. We presented two versions of it. In the version in the left column, the matrix is of type MatrixXd
which represents matrices of arbitrary size. The version in the right column is similar, except that the matrix is of type Matrix3d
, which represents matrices of a fixed size (here 3by3). Because the type already encodes the size of the matrix, it is not necessary to specify the size in the constructor; compare MatrixXd m(3,3)
with Matrix3d m
. Similarly, we have VectorXd
on the left (arbitrary size) versus Vector3d
on the right (fixed size). Note that here the coefficients of vector v
are directly set in the constructor, though the same syntax of the left example could be used too.
The use of fixedsize matrices and vectors has two advantages. The compiler emits better (faster) code because it knows the size of the matrices and vectors. Specifying the size in the type also allows for more rigorous checking at compiletime. For instance, the compiler will complain if you try to multiply a Matrix4d
(a 4by4 matrix) with a Vector3d
(a vector of size 3). However, the use of many types increases compilation time and the size of the executable. The size of the matrix may also not be known at compiletime. A rule of thumb is to use fixedsize matrices for size 4by4 and smaller.
It's worth taking the time to read the long tutorial.
However if you think you don't need it, you can directly use the classes documentation and our Quick reference guide.