friend
- 1,448
- 9
I'm wondering what the Dirac delta of a function would be in n dimensions. What is [itex]{\delta ^n}(f(x))[/itex]?
I understand that in 3 dimensional flat space, the Dirac delta function is
[tex]{\delta ^3}(x,y,z) = \delta (x)\delta (y)\delta (z)[/tex]
and
[tex]{\delta ^3}({{\vec x}_1} - {{\vec x}_0}) = \delta ({x_1} - {x_0})\delta ({y_1} - {y_0})\delta ({z_1} - {z_0})[/tex]
But I'm not sure what the expression would be when the 3D Dirac delta is composed with a scalar function. What is
[tex]{\delta ^3}(f(\vec x))[/tex]
In general [itex]f(\vec x)[/itex] is a scalar, not a vector, and I cannot break down [tex]f(\vec x) = ({f_1}(\vec x),{f_2}(\vec x),{f_3}(\vec x))[/tex]
Even if I could, would
[tex]{\delta ^3}(f(\vec x)) = \delta ({f_1}(\vec x)) \cdot \delta ({f_2}(\vec x)) \cdot \delta ({f_3}(\vec x))[/tex]
Somehow, it doesn't seem to make sense to say,
[tex]{\delta ^3}(f(\vec x)) = \delta (f(\vec x)) \cdot \delta (f(\vec x)) \cdot \delta (f(\vec x))[/tex]
So maybe that means we have to cook up a 3D version of the Dirac delta on first principles and not try to decompose it into a multiple of 3 separate deltas, even is flat space.
I understand that in 3 dimensional flat space, the Dirac delta function is
[tex]{\delta ^3}(x,y,z) = \delta (x)\delta (y)\delta (z)[/tex]
and
[tex]{\delta ^3}({{\vec x}_1} - {{\vec x}_0}) = \delta ({x_1} - {x_0})\delta ({y_1} - {y_0})\delta ({z_1} - {z_0})[/tex]
But I'm not sure what the expression would be when the 3D Dirac delta is composed with a scalar function. What is
[tex]{\delta ^3}(f(\vec x))[/tex]
In general [itex]f(\vec x)[/itex] is a scalar, not a vector, and I cannot break down [tex]f(\vec x) = ({f_1}(\vec x),{f_2}(\vec x),{f_3}(\vec x))[/tex]
Even if I could, would
[tex]{\delta ^3}(f(\vec x)) = \delta ({f_1}(\vec x)) \cdot \delta ({f_2}(\vec x)) \cdot \delta ({f_3}(\vec x))[/tex]
Somehow, it doesn't seem to make sense to say,
[tex]{\delta ^3}(f(\vec x)) = \delta (f(\vec x)) \cdot \delta (f(\vec x)) \cdot \delta (f(\vec x))[/tex]
So maybe that means we have to cook up a 3D version of the Dirac delta on first principles and not try to decompose it into a multiple of 3 separate deltas, even is flat space.