Physical simulations are a crucial tool in many fields, from game development and computer graphics to robotics and
prototype modeling. One fundamental aspect of these simulations is the concept of rotation. Be it planets whirling
around a star in a space simulation, joints operating in a humanoid robot, or an animated character performing a
thrilling parkour backflip, **rotations are indeed everywhere**. This blog post seeks to unravel the complexities of
3D
rotations and acquaint you with the diverse rotation representations used in physical simulations.

## Challenges of 3D Rotations

3D rotations are crucial for modeling the orientation of objects in space. They enable us to visualize and
manipulate 3D models mathematically. However, handling rotations in 3D space can be quite tricky. Many bugs in
simulations can be traced back to mismanaged rotations. The complexities arise from the nature of the 3D rotation
itself – it isn't commutative (the sequence of rotations is crucial) and interpolation isn't straightforward (
calculating a rotation halfway between two given rotations is complex). Additionally, 3D rotations form a group
structure known as the Special Orthogonal Group, SO(3), which isn't a typical Euclidean space where we can perform
standard linear operations.

## Rotation Representations

### 1. Rotation Matrices

Rotation matrices are 3x3 matrices that signify a rotation around the origin in 3D space. They provide an intuitive
approach to understanding rotation, with each column (or row, depending on convention) of the matrix representing the
new directions of the original axes after the rotation.

However, rotation matrices come with their set of limitations. The degree of freedom for rotation in an $n$-dimensional
space is $\frac{n (n-1)}{2}$. Thus, the 3D rotation resides in a 3-dimensional space (while 2D rotation resides in a
1-dimensional space). This means that 3D rotation matrices consume more memory (9 floating point numbers) than
necessary, and maintaining the orthogonality and normalization of the rotation matrix during numerical operations can be
computationally burdensome. In practical applications, the majority of libraries, including the simulators we've
discussed, employ quaternions as their core representation for rotations.

### 2. Quaternions

Quaternions are a type of mathematical object that extend complex numbers. They consist of one real component and three
imaginary components, often denoted as $w+xi+yj+zk$. Quaternions have emerged as an extremely effective method of
representing rotations in 3D space for computation.

Different from rotation matrix, they merely require four floating point numbers, can be easily interpolated using
techniques like Spherical Linear Interpolation (SLERP), and they bypass the gimbal lock problem. However, they are not
as intuitive as the other methods, and comprehending how they work necessitates some mathematical background. Also,
quaternions have a double covering problem. This means that each 3D rotation can be represented by two different
quaternions: one and its negation. In other words, a quaternion $q$ and its negative $-q$ will represent the same 3D
rotation.

### 3. Euler Angles

Euler angles represent a rotation as three angular rotations around the axes of a coordinate system. The axes can be in
any order (XYZ, ZYX, etc.), and this order makes a difference, leading to what is known as the "gimbal lock" problem.

Gimbal lock occurs when the axes of rotation align, causing a loss of one degree of freedom. This can lead to unexpected
behavior in simulations. And same 3D rotation can be mapped into multiple Euler angles.
Euler angles also have issues with interpolation, as interpolating between two sets of Euler angles will not produce a
smooth rotation.

### 4. Axis-Angle Representation

The Axis-Angle representation is another way to understand 3D rotations. In this representation, a 3D rotation is
characterized by a single rotation about a specific axis. The amount of rotation is given by the angle, and the
direction of rotation is specified by the unit vector along this axis.

This representation is simple and intuitive, but it's not easy to concatenate multiple rotations. Also, like Euler
angles, it has a gimbal lock problem when the rotation angle reaches 180 degrees. However, it's very useful in some
scenarios such as generating a random rotation, or rotating an object around a specific axis.

## Conversion Between Representations

Now, let's discuss the conversion between a rotation matrix and other common rotation representations: Euler angles,
quaternions, and the axis-angle representation.

### 1. Rotation Matrix to Euler Angles

The process of extracting Euler angles from a rotation matrix depends on the Euler angles convention. For the XYZ
convention (roll, pitch, yaw), the extraction is:

`roll = atan2(R[2, 1], R[2, 2])`

pitch = atan2(-R[2, 0], sqrt(R[0, 0]^2 + R[1, 0]^2))

yaw = atan2(R[1, 0], R[0, 0])

where `R[i, j]`

denotes the element at the `i`

-th row and the `j`

-th column of the rotation matrix `R`

.

### 2. Rotation Matrix to Quaternions

The conversion from a rotation matrix `R`

to a quaternion `q = (w, x, y, z)`

can be computed as:

`w = sqrt(1 + R[0, 0] + R[1, 1] + R[2, 2]) / 2`

x = (R[2, 1] - R[1, 2]) / (4 * w)

y = (R[0, 2] - R[2, 0]) / (4 * w)

z = (R[1, 0] - R[0, 1]) / (4 * w)

### 3. Rotation Matrix to Axis-Angle

For converting a rotation matrix to axis-angle representation, the axis `a = (a_x, a_y, a_z)`

and the angle `θ`

can be
calculated as:

`θ = acos((trace(R) - 1) / 2)`

a_x = (R[2, 1] - R[1, 2]) / (2 * sin(θ))

a_y = (R[0, 2] - R[2, 0]) / (2 * sin(θ))

a_z = (R[1, 0] - R[0, 1]) / (2 * sin(θ))

where `trace(R)`

is the sum of the elements on the main diagonal of `R`

.

## Common Issues and Bugs

### Different Simulator, Different Convention

Both Euler Angles and Quaternions adhere to multiple conventions. Various software libraries utilize different
conventions, which can potentially lead to errors when these libraries are used in tandem, a situation that occurs quite
frequently.

For instance, some libraries represent Quaternion as `(w, x, y, z)`

, positioning the real part as the first element,
while others represent it as `(x, y, z, w)`

. The following table illustrates the convention adopted by some widely used
software and simulators.

Quaternion Convention | Simulator/Library |
---|

wxyz | MuJoCo, SAPIEN, CoppeliaSim, IsaacSim, Gazebo, Blender, Taichi, Transforms3d, Eigen, PyTorch3D, USD |

xyzw | IsaacGym, ROS 1&2, IsaacSim Dynamic Control Extension, PhysX, SciPy, Unity, PyBullet |

It's crucial to be aware of these differences when employing multiple libraries to avoid any inconsistency in
results.

## Conclusion

Understanding 3D rotation representations and their conversion plays a pivotal role in creating sophisticated and
realistic physical simulations. While this tutorial provides a comprehensive overview of the primary rotation
representations, it's up to developers to determine which representation best suits their specific use-cases and
computational constraints.