L2 loss vs. mean squared loss

Question

I see some literature consider L2 loss (least squared error) and mean squared error loss are two different kinds of loss functions.

However, it seems to me these two loss functions essentially compute the same thing (with a 1/n factor difference).

So I am wondering if I have missed anything? Is there any scenario that one should use one of the two loss functions?

Answer 1

Function $L_2(x):=\left \|x \right \|_2$ is a norm, it is not a loss by itself. It is called a "loss" when it is used in a loss function to measure a distance between two vectors, $\left \| y_1 - y_2 \right \|^2_2$, or to measure the size of a vector, $\left \| \theta \right \|^2_2$. This goes with a loss minimization that tries to bring these quantities to the "least" possible value.

These are some illustrations:

1. $L_p$ norm: $L_p(x) := \left \|x \right \|_p = (\sum_{i=1}^{D} |x_i|^p)^{1/p}$,
   where $D$ is the dimension of vector $x$,

2. Squared error: $\mbox{SE}(A, \theta) =\sum_{n=1}^{N} \left \| y_n - f_{\theta}(x_n) \right \|^2_2$,
   where $A=\{(x_n, y_n)_{n=1}^{N}\}$ is a set of data points, and $f_{\theta}(x_n)$ is model's estimation of $y_n$,

3. Mean squared error: $\mbox{MSE}(A, \theta) =\mbox{SE}(A, \theta)/N$,

4. Least squares optimization: $\theta^*=\mbox{argmin}_{\theta} \mbox{MSE}(A, \theta)$$=\mbox{argmin}_{\theta} \mbox{SE}(A, \theta)$,

5. Ridge loss: $\mbox{R}(A, \theta, \lambda) = \mbox{MSE}(A, \theta) + \lambda\left \| \theta \right \|^2_2$

6. Ridge optimization (regression): $\theta^*=\mbox{argmin}_{\theta} \mbox{R}(A, \theta, \lambda)$.

In all of the above examples, $L_2$ norm can be replaced with $L_1$ norm or $L_\infty$ norm, etc.. However the names "squared error", "least squares", and "Ridge" are reserved for $L_2$ norm. For example for $L_1$, "squared error" becomes "absolute error":

1. Absolute error: $\mbox{AE}(A, \theta) =\sum_{n=1}^{N} \left \| y_n - f_{\theta}(x_n) \right \|_1$,

Answer 2

To be precise, L2 norm of the error vector is a root mean-squared error, up to a constant factor. Hence the squared L2-norm notation $\|e\|^2_2$, commonly found in loss functions.

However, $L_p$-norm losses should not be confused with regularizes. For instance, a combination of the L2 error with the L2 norm of the weights (both squared, of course) gives you a well known ridge regression loss, while a combination of L2 error + L1 norm of the weights gives rise to a Lasso regression.

Answer 3

They are different:

L2 = $\sqrt{\sum_{i=1}^{N}(y_i-y_{i}^{pred})^2}$

MSE = $\frac{\sum_{i=1}^{N}(y_i-y_{i}^{pred})^2}{N}$

There are sum and square root for L2-Norm, but sum and mean for MSE!

We can check it by following code:

import numpy as np
from sklearn.metrics import mean_squared_error

y = np.array(range(10, 20))  # array([10, 11, 12, 13, 14, 15, 16, 17, 18, 19])
y_pred = np.array(range(10))  # array([0, 1, 2, 3, 4, 5, 6, 7, 8, 9])
np.linalg.norm(y_pred - y, ord=2)  # L2-Nomr: 31.622776601683793
mean_squared_error(y_pred, y)  # MSE: 100.0

Answer 4

I think for computation purpose we are using L2 norms. Because if we use MSE we have to use "for loop" and this will take more computation. But, on the other hand, we can use N2 norms by using matrix and this saves more computation for any programing language considering if we have a huge data. Overall, I think both are doing the same thing. Please correct me if I am wrong!